Category: Earth & Climate

New leaf fossils found in Ethiopia’s Mush Valley

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Post date February 12, 2020
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DALLAS (SMU) – Leaf fossils from Ethiopia’s Mush Valley that date back nearly 22 million years have been found by SMU’s Earth Science professors Bonnie Jacobs and Neil J. Tabor and a dozen other international scientists.

The Mush Valley is the first site in Africa to produce an assemblage of some 2,400 leaves from that time interval, and the first to be studied using multiple lines of evidence, including associated microscopic fossils and chemical constituents, that tell us details about the ancient ecosystem.

Paleobotanical remains that an international team found in Ethiopia’s Mush Valley.

Scientists can use data from the study to answer fundamental questions, like what climate change may look like in the future. Specifically, climate scientists can take information from the study, along with other data, to test models used to estimate future global climate change.

“The past helps us to understand how ecological processes operate under conditions so different from now. It is like the Earth has done experiments for us,” said Jacobs, a world-renowned paleobotanist at SMU (Southern Methodist University).

In addition, using fossils to learn more about what Africa’s prehistoric ecosystems were like can provide context for events in the past, such as when a land bridge developed between Africa and Eurasia 24 million years ago or the environment for primate precursors to the human family.

The fossils found in this study span an interval of 60,000 years during the early Miocene Epoch, which began 23 million years ago. Ellen D. Currano, a paleoecologist at the University of Wyoming, was the lead author of the study. It was published in the journal Palaeogeography, Palaeoclimatology, Palaeoecology.

You can read more about the work that Jacobs, Currano and the international colleagues have been doing in the Mush Valley here.

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Wastewater leak in West Texas revealed by satellite radar imagery and sophisticated modeling

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Post date November 25, 2019
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Leakage in Ken Regan field could have contaminated groundwater for livestock and irrigation between 2007 and 2011

DALLAS (SMU) – Geophysicists at SMU say that evidence of leak occurring in a West Texas wastewater disposal well between 2007 and 2011 should raise concerns about the current potential for contaminated groundwater and damage to surrounding infrastructure.

SMU geophysicist Zhong Lu and the rest of his team believe the leak happened at a wastewater disposal well in the Ken Regan field in northern Reeves County, which could have leaked toxic chemicals into the Rustler Aquifer. The same team of geophysicists at SMU has revealed that sinkholes are expanding and forming in West Texas at a startling rate.

a) Coverage of the ALOS PALSAR scenes used (white box). Black line shows the boundary of the Ken Regan field. Dark green line and light green line represent the boundaries of the Rustler Aquifer and Pecos Valley Aquifer in Texas, respectively. Red star represents the epicenter of the earthquake that occurred in May 2018. Blue circle represents the groundwater well for livestock drawing from the Rustler Aquifer in this area. Blue triangles are wells, which provide groundwater leveling records. (b) Vertical deformation (cm/yr) (in the red box in Fig. 1a) estimated from InSAR. Green circles with and without arrows indicate active injection/disposal wells in the Ken Regan field and oil production wells within 1.5 km from the deformation center during the research period, respectively. Purple circle represents the groundwater which provides groundwater quality records. Source: Zhong Lu

Wastewater is a byproduct of oil and gas production. Using a process called horizontal drilling, or “fracking,” companies pump vast quantities of water, sand and chemicals far down into the ground to help extract more natural gas and oil. With that gas and oil, however, come large amounts of wastewater that is injected deep into the earth through disposal wells.

Federal and state oil and gas regulations require wastewater to be disposed of at a deep depth, typically ranging from about 1,000 to 2,000 meters deep in this region, so it does not contaminate groundwater or drinking water. A small number of studies suggest that arsenic, benzene and other toxins potentially found in fracking fluids may pose serious risks to reproductive and development health.

Even though the leak is thought to have happened between 2007 and 2011, the finding is still potentially dangerous, said Weiyu Zheng, a Ph.D. student at SMU (Southern Methodist University) who led the research.

“The Rustler Aquifer, within the zone of the effective injection depth, is only used for irrigation and livestock but not drinking water due to high concentrations of dissolved solids. Wastewater leaked into this aquifer may possibly contaminate the freshwater sources,” Zheng explained.

“If I lived in this area, I would be a bit worried,” said Lu, professor of Shuler-Foscue Chair at SMU’s Roy M. Huffington Department of Earth Sciences and the corresponding researcher of the findings.

He also noted that leaking wastewater can do massive damage to surrounding infrastructure. For example, oil and gas pipelines can be fractured or damaged beneath the surface, and the resulting heaving ground can damage roads and put drivers at risk.

SMU geophysicists say satellite radar imagery indicates a leak in the nearby disposal well happened because of changes shown to be happening in the nearby Ken Regan field: a large section of ground, five football fields in diameter and about 230 feet from the well, was raised nearly 17 centimeters between 2007 and 2011. In the geology world, this is called an uplift, and it usually happens where parts of the earth have been forced upward by underground pressure.

Lu said the most likely explanation for that uplift is that leakage was happening at the nearby well.

“We suspect that the wastewater was accumulated at a very shallow depth, which is quite dramatically different from what the report data says about that well,” he said.

Only one wastewater disposal well is located in close proximity to the uplifted area of the Ken Regan field. The company that owns it reported the injection of 1,040 meters of wastewater deep into the disposal well in Ken Regan. That well is no longer active.

But a combination of satellite images and models done by SMU show that water was likely escaping at a shallower level than the well was drilled for.

And the study, which was published in the Nature publication Scientific Reports, estimates that about 57 percent of the injected wastewater went to this shallower depth. At that shallower depth, the wastewater–which typically contains salt water and chemicals–could have mixed in with groundwater from the nearby Rustler Aquifer. Drinking water doesn’t come from the Rustler Aquifer, which spans seven counties. But the aquifer does eventually flow into the Pecos River, which is a drinking source.

The scientists made the discovery of the leak after analyzing radar satellite images from January 2007 to March 2011. These images were captured by a read-out radar instrument called Phased Array type L-band Synthetic Aperture Radar (PALSAR) mounted on the Advanced Land Observing Satellite, which was run by the Japan Aerospace Exploration Agency

With this technology called interferometric synthetic aperture radar, or InSAR for short, the satellite radar images allow scientists to detect changes that aren’t visible to the naked eye and that might otherwise go undetected. The satellite technology can capture ground deformation with a precision of sub-inches or better, at a spatial resolution of a few yards or better over thousands of miles, say the researchers.

Lu and his team also used data that oil and petroleum companies are required to report to the Railroad Commission of Texas (Texas RRC), as well as sophisticated hydrogeological models that mapped out the distribution and movement of water underground as well as rocks of the Earth’s crust.

“We utilized InSAR to detect the surface uplift and applied poroelastic finite element models to simulate displacement fields. The results indicate that the effective injection depth is much shallower than reported,” Zheng said. “The most reasonable explanation is that the well was experiencing leakage due to casing failures and/or sealing problem(s).”

“One issue is that the steel pipes can degrade as they age and/or wells may be inadequately managed. As a result, wastewater from failed parts can leak out,” said Jin-Woo Kim, research scientist with Lu’s SMU Radar Laboratory and a co-author of this study.

The combination of InSAR imagery and modeling done by SMU gave the scientists a clear picture of how the uplift area in Regan field developed.

Lu, who is world-renowned for leading scientists in using InSAR applications to detect surface changes, said these types of analysis are critical for the future of oil-producing West Texas.

“Our research that exploits remote sensing data and numerical models provides a clue as to understanding the subsurface hydrogeological process responding to the oil and gas activities. This kind of research can further be regarded as an indirect leakage monitoring method to supplement current infrequent leakage detection,” Zheng said.

“It’s very important to sustain the economy of the whole nation. But these operations require some checking to guarantee the operations are environmentally-compliant as well,” Lu said.

Co-author Dr. Syed Tabrez Ali from AIR-Worldwide in Boston also contributed to this study.

This research was sponsored by the NASA Earth Surface and Interior Program and the Schuler-Foscue endowment at SMU.

Previously, Kim and Lu used satellite radar imaging to find that two giant sinkholes near Wink, Texas—two counties over from the Ken Regan uplift—were likely just the tip of the iceberg of ground movement in West Texas. Indeed, they found evidence that large swaths of West Texas oil patch were heaving and sinking at alarming rates. Decades of oil production activities in West Texas appears to have destabilized localities in an area of about 4,000 square miles populated by small towns like Wink, roadways and a vast network of oil and gas pipelines and storage tanks.

Watch the WFAA Verify news segment. You can also hear a report on the study that was broadcast on Austin’s NPR KUT 90.5 below:

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Historical data confirms recent increase in West Texas earthquakes

Post author By 46778533
Post date November 4, 2019
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A new analysis of historical seismic data conducted by The University of Texas at Austin, SMU and other academies has found that earthquake activity in West Texas around Pecos has increased dramatically since 2009.

The study, published Nov. 4, 2019, in the Journal of Geophysical Research: Solid Earth, is important because it leverages old, unmined data to track seismic activity over nearly the past two decades – much further back than other studies— to show that activity has increased during the past decade in an area of the Permian Basin that is being heavily developed for oil and gas. Although researchers have generally thought that to be true, the statewide TexNet earthquake monitoring system has been gathering data since only 2017, making it impossible to definitely determine when the cluster of seismic activity around Pecos really began.

The researchers were able to extend the seismic record of the area by turning to the older TXAR system near Lajitas about 150 miles to the south. TXAR is an array of 10 seismographs installed in the 1990s by scientists at SMU (Southern Methodist University) to help track nuclear testing across the world, said lead author Cliff Frohlich, a senior research scientist emeritus at the University of Texas Institute for Geophysics (UTIG).

“Especially for these West Texas earthquakes, we would like to get some information about when they started,” Frohlich said. “I really saw this as a way to bridge the gap before TexNet.”

The TXAR system is some distance from Pecos, but Frohlich said the equipment is highly sensitive and that the area is remote and seismically very quiet, making the system perfect for picking up vibrations from explosions across the world or from earthquakes 150 miles away. Frohlich worked with Chris Hayward, director of SMU’s Geophysics Research Program, to create a method to derive the earthquake data from the international data TXAR collects and build an earthquake catalog for the Delaware Basin near Pecos from 2000 to 2017.

By analyzing data from 2000 to 2017, scientists were able to document more than 7,000 seismic events near Pecos that were determined by the team to be earthquakes. Data on these seismic events had to be manually reviewed to ensure they were in fact earthquakes and not a false detection. This was done by Frohlich and Julia Rosenblit, who was an SMU intern at the time.

Multiple events first started occurring in 2009, when 19 earthquakes of at least magnitude 1 were documented. The rate increased over time, with more than 1,600 earthquakes of magnitude 1 or greater in 2017. Most were so small that no one felt them.

The study shows a correlation between earthquake activity in the area and an increase in oil and gas activity but doesn’t make an effort to directly tie the two together as other studies have done.

“West Texas now has the highest seismicity rates in the state,” said Heather DeShon, study co-author and associate professor at SMU’s Roy M. Huffington Department of Earth Sciences. “What remained uncertain is when the earthquakes actually started. This study addresses that.”

This study is the latest in a comprehensive effort to determine what is causing an increase in seismic activity in Texas and how oil and gas operations can be managed to minimize that human-induced element. The state approved the TexNet system in 2015, which is operated in tandem with research efforts by the Center for Integrated Seismicity Research (CISR).

Co-author Peter Hennings, who leads CISR and is a Senior Research Scientist at the UT Bureau of Economic Geology said that fundamental research like this latest study is vital when trying to unravel such a complicated problem.

“The obvious next step is exactly what the University of Texas is doing – conducting these careful studies on the relationship between earthquakes and their human and natural causes to build an integrated understanding,” Hennings said.

SMU seismologists have also been the lead or co-authors of a series of studies on Texas earthquakes. For instance, UT Austin and SMU found that earthquakes triggered by human activity have been happening in Texas since 1925, and they have been widespread throughout the state ever since. In addition, SMU research showed that many of the Dallas-Fort Worth earthquakes were triggered by increases in pore pressure–the pressure of groundwater trapped within tiny spaces inside rocks in the subsurface.

The Bureau of Economic Geology and UTIG are units of the UT Jackson School of Geosciences. Scientists from SMU, Portland State University, the University of Oklahoma and the French institute IFREMER also worked on the study.

Several outlets covered the new research, including The Weather Channel, The Dallas Morning News, Texas Tribune, Midland Reporter-Telegram, and Dallas Observer. – The University of Texas at Austin

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Researchers unveil new volcanic eruption forecasting technique

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Post date September 12, 2019
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Volcanic eruptions and their ash clouds pose a significant hazard to population centers and air travel, especially those that show few to no signs of unrest beforehand. Geologists are now using a technique traditionally used in weather and climate forecasting to develop new eruption forecasting models. By testing if the models are able to capture the likelihood of past eruptions, the researchers are making strides in the science of volcanic forecasting.

The study, published in the journal Geophysical Research Letters, examined the eruption history of the Okmok volcano in Alaska. In 2008, a large eruption produced an ash plume that extended approximately 1 mile into the sky over the Aleutian Islands – posing a significant hazard to aircraft engines along a route that transports roughly 50,000 people between Asia and North America each day, the researchers said.

“The 2008 eruption of Okmok came as a bit of surprise,” said University of Illinois graduate student and lead author Jack Albright. “After an eruption that occurred in 1997, there were periods of slight unrest, but very little seismicity or other eruption precursors. In order to develop better forecasting, it is crucial to understand volcanic eruptions that deviate from the norm.”

Geologists typically forecast eruptions by looking for established patterns of preeruption unrest such as earthquake activity, groundswell and gas release, the researchers said. Volcanoes like Okmok, however, don’t seem to follow these established patterns.

To build and test new models, the team utilized a statistical data analysis technique developed after World War II called Kalman filtering.

“The version of Kalman filtering that we used for our study was updated in 1996 and has continued to be used in weather and climate forecasting, as well as physical oceanography,” said U. of I. geology professor Patricia Gregg, a co-author of the study that included collaborators from SMU (Southern Methodist University) and Michigan State University. “We are the first group to use the updated method in volcanology, however, and it turns out that this technique works well for the unique unrest that led up to Okmok’s 2008 eruption.”

One of those unique attributes is the lack of increased seismicity before the eruption, the researchers said. In a typical preeruption sequence, it is hypothesized that the reservoir under the volcano stays the same size as it fills with magma and hot gases. That filling causes pressure in the chamber to increase and the surrounding rocks fracture and move, causing earthquakes.

“In the 2008 eruption, it appears that the magma chamber grew larger to accommodate the increasing pressure, so we did not see the precursor seismic activity we would expect,” Albright said. “By looking back in time with our models, or hindcasting, we can now observe that stress had been building up in the rocks around the chamber for weeks, and the growth of the magma system ultimately led to its failure and eruption.”

This type of backward and forward modeling allows researchers to watch a volcanic system evolve over time. “While we stopped our analysis after the 2008 eruption, we are now able to propagate this new model forward in time, bring it to present day, and forecast where Okmok volcano is heading next,” Gregg said.

The researchers posit that these models will continue to find other less-recognized eruption precursors, but acknowledge that every volcano is different and that the models must be tailored to fit each unique system.

The volcano forecasting technique used in this study was based on volcano deformation data from GPS and satellite radars. Geophysicist Zhong Lu, a professor in the Roy M. Huffington Department of Earth Sciences at SMU and a global expert in satellite radar imagery analysis, processed the satellite radar images and provided the volcano deformation maps for this research.

The U. of I. team is working in collaboration with researchers from Alaska Volcano Observatory and SMU to help build a stronger forecasting system for the Aleutian Islands area. The researchers received $541,921 in grant money from NASA for the work in early 2019.

Popular Mechanics, Sci Tech Daily and other outlets highlighted the study. — University of Illinois at Urbana-Champaign

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People transformed the world through land use by 3,000 years ago

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Post date August 29, 2019
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Study sheds light on how the way our ancestors fed themselves changed our ecosystem

DALLAS (SMU) – Humans started making an impact on the global ecosystem through intensive farming much earlier than previously estimated, according to a new study published in the journal Science.

Evidence of the earliest domesticated plants and animals dates back to around 10,000 years ago. But findings from a team of more than 250 scientists, including two from SMU (Southern Methodist University), show that by 3,000 years ago our ancestors had dramatically changed the world to grow food.

“Our study shows in detail the progression from the origins of agriculture to its spread around the world,” said SMU anthropologist Mark D. McCoy. “It turns out that earth science models are probably too conservative, and intensive reshaping of the environment for food production was common by thousands of years before the onset of the kind of industrial scale farming we see today.

“That is important because over the time periods discussed, humans became the major force shaping ecosystems around the world,” McCoy said.

The new global assessment by the ArchaeoGLOBE Project also shows that scientists have previously underestimated the impact of early human land use.

Crowdsourcing the Map

Led by archeologist Lucas Stephens, a researcher affiliated with the Max Planck Institute for the Science of Human History, ArchaeoGLOBE used a crowdsourcing approach, inviting experts in ancient land use to contribute to a questionnaire on 146 regions (covering all continents except Antarctica) at ten historical time intervals to assess and integrate archaeological knowledge at a global scale. The result was a complete, though uneven, meta-analysis of global land use over time.

Significantly, the study also reveals that hunting and gathering was more varied and complex than originally thought, helping archeologists to recognize that foragers “may have initiated dramatic and sometimes irreversible environmental change.” Intensive forms of agriculture reported around the world included activities like clearing land, creating fields that were fixed on the landscape, raising large herds of animals, and putting increasing amounts of effort into growing food.

SMU anthropologist and ArchaeoGLOBE team member K. Ann Horsburgh notes the rise in agriculture and livestock is primarily due to growing populations needing to be fed.

“Food production such as agriculture and pastoralism, when compared with foraging in the same environment, is linked to a faster population growth and can sustain higher population densities,” said Horsburgh.

Horsburgh, Assistant Professor of Anthropology, and McCoy, Associate Professor of Anthropology, provided information on land use in Africa and the remote islands of the Pacific, respectively. McCoy also brought his expertise in geospatial technology to study how people in the past inhabited and shaped the world around them, while Horsburgh brought her knowledge of ancient DNA to retrace the spread of domesticated animals.

Mapping Ancient Migrations

The map could provide new light on how the spread of farming and herding were linked to major migrations in human prehistory.

“This is first time that regional expertise on ancient land use has been synthesized on this scale,” Horsburgh said. “That matters because we know that although the shift from foraging to farming tends to be a ‘one-way’ transition, it did not progress the same way around the world. The details of how it did progress has shaped everything from our diets to the languages we speak today.”

Horsburgh went on to say, “What remains the topic of intense study is how much of the transition is food producers spreading and displacing foragers, and how much is it foragers adopting or marrying into food producing groups, or some other scenario. Most of this was done in the absence of written records, so it is up to anthropology to sort things out.”

“The natural next step for this revised model of the spread of different types, and intensities, of land use is to compare them with human genetics and linguistics and integrate these findings into the big story of humanity,” said Horsburgh.

Several media outlet covered this research including The New York Times, Science and CNN.

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New map outlines seismic faults across DFW region

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Post date July 23, 2019
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Study by SMU, UT Austin and Stanford scientists rates faults for potential earthquakes; Faults under DFW urban area viewed as lower quake hazard

DALLAS (SMU) – Scientists from SMU, The University of Texas at Austin and Stanford University found that the majority of faults underlying the Fort Worth Basin are as sensitive to forces that could cause them to slip as those that have hosted earthquakes in the past.

The new study, published July 23^rd by the journal Bulletin of the Seismological Society of America (BSSA), provides the most comprehensive fault information for the region to date.

Fault slip potential modeling explores two scenarios: a model based on subsurface stress on the faults prior to high-volume wastewater injection and a model of those forces reflecting increase in fluid pressure due to injection.

A simplified version of the fault map created by the team of researchers. The map includes faults that are visible at the surface (green) and faults that are underground (black). The solid line indicates underground faults that researchers were able to map at a high resolution. The dotted line indicates faults that were mapped at a medium resolution. According to the research, in the presence of wastewater injection activity, the majority of the faults in the area are as susceptible to slipping as those faults that have already produced earthquakes. The map also marks earthquake locations and waste-water injection well locations and amounts. Credit: UT’s Bureau of Economic Geology

None of the faults shown to have the highest potential for an earthquake are located in the most populous Dallas-Fort Worth urban area or in the areas where there are currently many wastewater disposal wells.

Yet, the study also found that the majority of faults underlying the Fort Worth Basin are as sensitive to forces that could cause them to slip and cause an earthquake as those that have hosted earthquakes in recent years.

Though the majority of the faults identified on this map have not produced an earthquake, understanding why some faults have slipped and others with similar fault slip potential have not continues to be researched, said SMU seismologist and study co-author Heather DeShon, who has been the lead investigator of a series of other studies exploring the cause of the North Texas earthquakes.

Earthquakes were virtually unheard of in North Texas until slightly more than a decade ago. But more than 200 earthquakes have occurred in the region since late 2008, ranging in magnitude from 1.6 to 4.0. A series of studies have linked these events to the disposal of wastewater from oil and gas operations by injecting it deep into the earth at high volumes, triggering “dead” faults nearby.

A total of 251 faults have been identified in the Fort Worth Basin, but the researchers suspect that more exist that haven’t been identified.

The study found that the faults remained relatively stable if they were left undisturbed. However, wastewater injection sharply increased the chances of these faults slipping, if they weren’t managed properly.

“That means the whole system of faults is sensitive,” said the lead author of the study Peter L. Hennings, a research scientist from UT Austin’s Bureau of Economic Geology and the principal investigator at the Center for Integrated Seismicity Research (CISR).

DeShon said the new study provides fundamental information regarding earthquake hazard to the Dallas-Fort Worth region.

“The SMU earthquake catalog and the Texas Seismic Network catalog provide necessary earthquake data for understanding faults active in Texas right now,” she said. “This study provides key information to allow the public, cities, state and federal governments and industry to understand potential hazard and design effective public policies, regulations and mitigation strategies.”

“Industrial activities can increase the probability of triggering earthquakes before they would happen naturally, but there are steps we can take to reduce that probability,” added co-author Jens-Erik Lund Snee, a doctoral student at Stanford University.

Earthquake rates, like wastewater injection volumes, have decreased significantly since a peak in 2012. But as long as earthquakes occur, earthquake hazard remains. Dallas-Fort Worth remains the highest risk region for earthquakes in Texas because of population density.

Even after the earthquakes died away, North Texas residents have wondered about the region’s vulnerability to future earthquakes – especially since no map was available to pinpoint the existence of all known faults in the region. The new data, while still incomplete, benefited from information gleaned from newly released reflection seismic data held by oil and gas companies, reanalysis of publicly available well logs, and geologic outcrop information.

U of T at Austin and Stanford University provided the fault data and calculated fault slip potential. SMU, meanwhile, has been tracking seismic activity — which measures when the earth shakes —since people in the Dallas-Fort Worth area felt the first tremors near DFW International Airport in 2008. A catalog of all those tremors was recently published in June in the journal BSSA.

SMU seismologists have also been the lead or co-authors of a series of studies on the North Texas earthquakes. SMU research showed that many of the Dallas-Fort Worth earthquakes were triggered by increases in pore pressure — the pressure of groundwater trapped within tiny spaces inside rocks in the subsurface. An independent study done by SMU’s seismologist Beatrice Magnani found that wastewater injection reactivated dormant faults near Dallas that had been dormant for the last 300 million years.

DeShon said any future plan to mine for oil or natural gas in Fort Worth basin should be done with an understanding that the basin contains several faults that are highly-sensitive to pore-pressure changes. The study noted that rates of injection dropped sharply in the Fort Worth basin, but the practice still continues. Most of the injection that has taken place has been concentrated in the Johnson, Tarrant, and Parker counties, near areas of continued seismic activity.

“The largest earthquake the Dallas-Fort Worth region experienced was a magnitude 4 in 2015” DeShon said. “The U.S. Geological Survey and Red Cross provide practical preparedness advice for your home and work places. Just as we prepare for tornado season in north Texas, it remains important for us to have a plan for experiencing earthquake shaking.”

Many outlets covered the news:

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SMU’s catalog of North Texas earthquakes confirms continuing effects of wastewater disposal

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Post date June 12, 2019
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A comprehensive catalog of earthquake sequences in Texas’s Fort Worth Basin, from 2008 to 2018, provides a closer look at how wastewater disposal from oil and gas exploration has changed the seismic landscape in the basin.

In their report published in the Bulletin of the Seismological Society of America, Louis Quinones and Heather DeShon of Southern Methodist University (SMU) and colleagues confirmed that seismicity rates in the basin have decreased since 2014, a trend that appears to correspond with a decrease in wastewater injection.

However, their analysis also noted that new faults have become active during this period, and that seismicity continues at a greater distance from injection wells over time, suggesting that “far-field” changes in seismic stress will be important for understanding the basin’s future earthquake hazard potential.

“One thing we have come to appreciate is how broadly injection in the basin has modified stress within entire basin,” said DeShon.

The first thing researchers noted with wastewater injection into the basin “was the reactivation of individual faults,” she added, “and what we’re now starting to see is essentially the leftover energy on all sorts of little faults being released by the cumulative volume that’s been put into the basin.”

The earthquake catalog published in BSSA reported all seismicity recorded by networks operated by SMU between 2008 and 2018. Some seismic sequences in the catalog–such as the 2008 Dallas Fort Worth Airport earthquakes–are well-known and well-studied, while others such as the 2018 west Cleburne sequence are reported in the paper for the first time.

DeShon said publishing the complete catalog was important in part to help people recognize that “there are earthquakes throughout the basin, not just on these three or four sequences that have garnered a lot of press attention.”

The researchers found that overall seismicity in the Fort Worth Basin has been strongly correlated in time and space with wastewater injection activities, with most seismicity occurring within 15 kilometers of disposal wells.

Wastewater disposal volume began to decrease from its peak in 2014, mostly as a result of lower oil and gas prices, and the study showed “tapering off of seismicity along the faults that were near high-injection wells,” said Quinones.

There are exceptions to this pattern, including the 2015 Irving-Dallas and 2017 Lake Lewisville sequences that have no wells within 15 kilometers.

Induced earthquakes occur when wastewater injected back into the ground increases the pore pressure within the rocks and affects stress along faults in surrounding rock layers. In the Fort Worth Basin, these stress changes may propagate far–more than 10 kilometers–from the injection wells, the researchers suggested.

“Injection rates peaked in 2014, but we still don’t understand how spatially extensive the modification of pore pressure is at depth, so we still don’t understand how the hazard is going to reduce with time,” said DeShon.

There are still far fewer induced earthquakes in the Fort Worth Basin compared to regions such as Oklahoma, which also has experienced a dramatic increase in seismicity in the past decade as the result of wastewater disposal from oil and gas production. The volumes of injected wastewater are much higher in Oklahoma, and the faults there tend to be much closer together, DeShon said.

By contrast, Quinones said, faults in the Fort Worth Basin are more widely spaced, and there are few instances of earthquakes jumping between faults.

However, the dense population of the Dallas-Fort Worth metropolitan area makes it critical to continue monitoring the region’s induced earthquake risk, comparing seismic data with more information on wastewater injection.

For the moment, DeShon said, researchers only have access to monthly cumulative volume and average pressure at injection wellheads, in a report that is updated once a year.

“It would be best if injection data were provided in a more timely fashion in Texas, and if more detailed daily information on injection rates and volumes and some measurements of downhole pressure were provided,” she said.–Seismological Society of America

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New Smithsonian Exhibit Reflects the Passion of SMU Professor and an Army of Student Fossil Hounds

Post author By Gary O'Berg
Post date October 16, 2018
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A fossil mosasaur skull and partial skeleton excavated from Angola’s costal cliffs for display in “Sea Monsters Unearthed.” When the South Atlantic ocean basin was still young, a new deep-water connection between the Southern and Northern Hemispheres allowed giant marine reptiles to move into Angola's coastal waters. Mosasaurs and sea turtles, drawn by the region's plentiful food, were among the first reptiles to prowl these waters. “Fossils tell us about the life that once lived on Earth, and how the environments that came before us evolve over time,” said Louis Jacobs, professor emeritus of paleontology at SMU and collaborating curator for the exhibition. “Our planet has been running natural experiments on what shapes environments, and thereby life, for millions of years. If it weren’t for the fossil record, we wouldn’t understand what drives the story of life on our planet.” (Credit: Hillsman S. Jackson, Southern Methodist University)

Sea Monsters Unearthed: Life in Angola’s Ancient Seas opens Nov. 9 at National Museum of Natural History

DALLAS (SMU October 15, 2018) – Once the exhibit opens, “Sea Monsters Unearthed: Life in Angola’s Ancient Seas” will allow visitors to visually dive into the cool waters off the coast of West Africa as they existed millions of years ago when the continents of Africa and South America were drifting apart. It’s a unique opportunity to examine fossils of ancient marine reptiles and learn about the forces that continue to mold life both in out of the ocean.

But the back story is just as fascinating: SMU Emeritus Professor of Paleontology Louis Jacobs and his SMU colleague Michael Polcyn forged a partnership with collaborators in Angola, Portugal and the Netherlands to explore and excavate Angola’s rich fossil history, while laying the groundwork for returning the fossils to the West African nation. Back in Dallas Jacobs and Polcyn, director of the University’s Digital Earth Sciences Lab, and research associate Diana Vineyard went to work over a period of 13 years with a small army of SMU students to prepare the fossils excavated by Projecto PaleoAngola.

The result is a dynamic exhibit opening Nov. 9 in the Smithsonian’s National Museum of Natural History featuring large vertebrate marine reptiles from the Cretaceous Period — mosasaurs, marine turtles and plesiosaurs. This exhibit will mark the first time Angolan fossils of colossal Cretaceous marine reptiles will be on public display.

“It turns out that Angola is the best place on the surface of the earth to see the rocks that reflect and show the opening of the South Atlantic and the split between South America and Africa,” Jacobs said. But the war of independence in Angola that began in 1961 and ended (after civil war) in 2002 effectively prevented scientists from working this rich fossil zone for nearly 40 years after continental drift and plate tectonics became accepted scientific theory.

When Jacobs and the team arrived to begin digging on the coast of Angola in 2005, they were first on the scene to record this fascinating record of sea life that existed as the South Atlantic Ocean grew between two drifting continents.

SMU students did the important, time-consuming lab work

Over the past 13 years, the fossils were shipped back to Dallas, where over 100 undergraduate students have worked in basement laboratories to painstakingly clean and preserve the fossils. Some were paleontology students, most were not – but they seem to share an appreciation for their unique role in sharing new knowledge.

“Getting fossils out of rocks is a time consuming, labor-intensive operation,” Jacobs said. “But every time a student removes a grain of sand off a fossil, they have the excitement of seeing ancient life that no one else in the world has ever seen. On top of that, these fossils are going on exhibit at the Smithsonian and then back to their own homeland. That gives our students an opportunity that they simply could not get anywhere else. And what’s not to like about that?”

The Smithsonian exhibit, made possible by the Sant Ocean Hall Endowment fund, will immerse visitors in a marine environment from the Cretaceous Period, which began about 145 million years ago and ended about 66 million years ago. It features lively animations and vivid paleoart murals of life beneath the waves courtesy of natural history artist (and longtime Jacobs collaborator) Karen Carr. The exhibit brings to life 11 authentic fossils from Angola’s ancient seas, full-size fossil reconstructions of a mosasaur and a marine turtle, as well as 3-D scanned replicas of mosasaur skulls. Photomurals and video vignettes will take visitors to field sites along Angola’s modern rugged coast, where Projecto PaleoAngola scientists unearthed the fossil remains from this lost world.

“Because of our planet’s ever-shifting geology, Angola’s coastal cliffs contain the fossil remains of marine creatures from the prehistoric South Atlantic,” said Kirk Johnson, the Sant Director of the National Museum of Natural History. “We are honored by the generosity of the Angolan people for sharing a window into this part of the Earth’s unfolding story with our visitors.”

About SMU

About the National Museum of Natural History

The National Museum of Natural History is connecting people everywhere with Earth’s unfolding story. The museum is one of the most visited natural history museums in the world with approximately 7 million annual visitors from the U.S. and around the world. Opened in 1910, the museum is dedicated to maintaining and preserving the world’s most extensive collection of natural history specimens and human artifacts. It is open daily from 10 a.m. to 5:30 p.m. (closed Dec. 25). Admission is free. For more information, visit the museum on its website and on Facebook and Twitter.

In the words of smu students and graduates who sorted, cleaned and preserved fossils for Projecto Paleoangola

Pictured (L to R): Yasmin Jackson, Tania Doblado Speck, Harrison Schumann and Evan Snyder

Evan Snyder (SMU 2019)

“This experience allowed me to work on a project far bigger than myself. Exhibits just like this one excited me as a young child and led to my study of science. I’d love to think that my work will have the same impact on kids today. Working on this project also taught me how to work on challenging and stressful tasks with the right balance of confidence and care to meet deadlines with quality work.”

Yasmin Jackson (SMU 2019)

“I was able to go to the Smithsonian for the first time through this project. I really liked being able to see all of the different exhibits that are currently in the museum and imagine what our exhibit will be like in the midst of all of it.”

Harrison Schuman (SMU 2019)

“Dr. Jacobs is an inspiring individual to be around. Despite being a world-class expert in paleontology, he made himself very approachable and was always personally invested in all of the students working on the project. This kind of attitude encourages students like me to pursue careers in science.”

Alexandra Lippas (SMU 2011)

“It is because of Dr. Jacobs that I was able to be a part of this project. He encouraged students from other branches of science to work on this study. I think it demonstrates that different perspectives can lead to great discovery.”

Connor Flynn (SMU 2014)

“My time in the lab will be a source of stories for years to come and a point of pride for a lifetime. Its lessons in patience, care and passion for the labor will never be forgotten. Dr. Jacobs’ words ‘There’s nothing so broken you can’t fix it,’ carried me through more lab accidents than i care to admit — both at SMU and beyond.”

Jennifer Welch (SMU 2019)

“Dr. Jacobs is so incredibly smart, I could point out any part of the vertebrae and he would tell me what it’s for, why it was there, how that impacted the life of the animal and the stories that told about the land where the animal lived.”

Stephen Tyler Armstrong (SMU 2012)

“As an engineering major, this project exposed me to areas of research and career paths I would otherwise not encountered. It was really interesting to work so closely with those conducting the research to learn about a subject outside of my realm.”

For more information about undergraduate students working in SMU’s earth sciences labs.

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Native Bison Hunters Amplified Climate Impacts on North American Prairie Fires

Post author By Gary O'Berg
Post date July 24, 2018
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Blackfeet Burning Crow Buffalo Range, painting by Charles Marion Russell, 1905.

Study shows hunter-gatherers used active burning to improve grazing, drive bison, long before arrival of Columbus

DALLAS (SMU) – Native American communities actively managed North American prairies for centuries before Christopher Columbus’ arrival in the New World, according to a new study led by Southern Methodist University (SMU) archaeologist Christopher I. Roos.

Fire was an important indigenous tool for shaping North American ecosystems, but the relative importance of indigenous burning versus climate on fire patterns remains controversial in scientific communities. The new study, published in Proceedings of the National Academy of Sciences (PNAS), documents the use of fire to manipulate bison herds in the northern Great Plains. Contrary to popular thinking, burning by indigenous hunters combined with climate variability to amplify the effects of climate on prairie fire patterns.

The relative importance of climate and human activities in shaping fire patterns is often debated and has implications for how we approach fire management today.

“While there is little doubt that climate plays an important top-down role in shaping fire patterns, it is far less clear whether human activities – including active burning – can override those climate influences,” said Roos. “Too often, if scientists see strong correlations between fire activity and climate, the role of humans is discounted.”

Anthropologists and historians have documented a wide variety of fire uses by Native peoples in the Americas but fire scientists have also documented strong fire-climate relationships spanning more than 10,000 years.

“People often think that hunter-gatherers lived lightly on the land,” said Kacy L. Hollenback, an anthropologist at SMU and co-author of the study. “Too often we assume that hunter-gatherers were passive in their interaction with their environment. On the Great Plains and elsewhere, foragers were active managers shaping the composition, structure, and productivity of their environments. This history of management has important implications for contemporary relationships between Native American and First Nations peoples and their home landscapes – of which they were ecosystem engineers.”

Working in partnership with the Blackfeet Tribe in northern Montana, Roos and colleagues combined landscape archaeology and geoarchaeology to document changes in prairie fire activity in close spatial relationship to stones piled in formations up to a mile long that were used to drive herds of bison off of cliffs to be harvested en masse. These features are known as drivelines.

“We surveyed the uplands for stone features that delineate drivelines within which bison herds would be funneled towards a jump,” said anthropologist María Nieves Zedeño of the University of Arizona, co-author of the study. “By radiocarbon dating prairie fire charcoal deposits from the landscape near the drivelines, we were able to reconstruct periods of unusually high fire activity that are spatially associated with the drivelines,” says Roos.

The overlap between peak periods of driveline use (ca. 900-1650 CE) and prairie fire activity (ca. 1100-1650 CE) suggests that fire was an important tool in the hunting strategy involving the drivelines. Roos and colleagues suggest that fire was used to freshen up the prairie near the mouth of the drivelines to attract herds of bison, who prefer to graze recently burned areas. Episodes of high fire activity also correspond to wet climate episodes, when climate would have produced abundant grass fuel for prairie fires.

The absence of deposits indicating high prairie fire activity before or after the period of driveline use, even though comparable wet climate episodes occurred, suggests that anthropogenic burning by Native hunters amplified the climate signal in prairie fire patterns during the period of intensive bison hunting.

“We need to consider that humans and climate have more complicated and interacting influences on historical fire patterns,” said Roos. “Moreover, we need to acknowledge that hunter-gatherers can be active influences in their environments, particularly through their use of fire as a landscape tool. We expect that future studies of human/climate/fire interactions will further document the complexity of these relationships. Understanding that complexity may prove important as we try to navigate the complex wildfire problems we face today.”

About SMU

SMU is a nationally ranked global research university in the dynamic city of Dallas. SMU’s alumni, faculty and nearly 12,000 students in seven degree-granting schools demonstrate an entrepreneurial spirit as they lead change in their professions, communities and the world.

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Ancient “Sea Monsters” Reveal How the Ever-Changing Planet Shapes Life, Past and Present

Post author By Margaret Allen
Post date June 4, 2018

Never-Before-Seen Fossils From Angola Bring a Strange Yet Familiar Ocean Into View

The Smithsonian’s National Museum of Natural History will open a new exhibition Nov. 9, 2018 revealing how millions of years ago, large-scale natural forces created the conditions for real-life sea monsters to thrive in the South Atlantic Ocean basin shortly after it formed. “Sea Monsters Unearthed: Life in Angola’s Ancient Seas” will offer visitors the opportunity to dive into Cretaceous Angola’s cool coastal waters, examine the fossils of striking marine reptiles that once lived there and learn about the forces that continue to mold life in the ocean and on land.

Over 134 million years ago, the South Atlantic Ocean basin did not yet exist. Africa and South America were one contiguous landmass on the verge of separating. As the two continents drifted apart, an entirely new marine environment — the South Atlantic — emerged in the vast space created between them. This newly formed ocean basin would soon be colonized by a dizzying array of ferocious predators and an abundance of other lifeforms seizing the opportunity presented by a new ocean habitat.

“Because of our planet’s ever-shifting geology, Angola’s coastal cliffs contain the fossil remains of marine creatures from the prehistoric South Atlantic,” said Kirk Johnson, the Sant Director of the museum. “We are honored by the generosity of the Angolan people for sharing a window into this part of the Earth’s unfolding story with our visitors.”

For the first time, Angolan fossils of colossal Cretaceous marine reptiles will be on public display. Through Projecto PaleoAngola — a collaboration between Angolan, American, Portuguese and Dutch researchers focused on Angola’s rich fossil history — paleontologists excavated and studied these fossils, which were then prepared for the exhibition by a team of scientists and students at Southern Methodist University (SMU) in Dallas. The exhibition was made possible by the Sant Ocean Hall Endowment Fund.

“Fossils tell us about the life that once lived on Earth, and how the environments that came before us evolve over time,” said Louis Jacobs, professor emeritus of paleontology at SMU and collaborating curator for the exhibition. “Our planet has been running natural experiments on what shapes environments, and thereby life, for millions of years. If it weren’t for the fossil record, we wouldn’t understand what drives the story of life on our planet.”

The exhibition will immerse visitors in this Cretaceous environment with lively animations and vivid paleoart murals of life beneath the waves — courtesy of natural history artist Karen Carr — that bring to life 11 authentic fossils from Angola’s ancient seas, full-size fossil reconstructions of a mosasaur and an ancient sea turtle, as well as 3-D scanned replicas of mosasaur skulls. Photomurals and video vignettes will transport visitors to field sites along Angola’s modern rugged coast, where Projecto PaleoAngola scientists unearth the fossil remains from this lost world.

A Strange but Familiar Ocean
“Sea Monsters Unearthed” paints the picture of a flourishing ocean environment that in some ways will look strange to modern eyes, yet still bears striking similarities to today’s marine ecosystems.

Peculiar plesiosaurs — massive reptiles with long necks, stout bodies and four large flippers — swam alongside 27-foot-long toothy marine lizards called mosasaurs and more familiar creatures like sea turtles. From surprising mosasaur stomach contents to the one of the oldest known sea turtles found in Africa, fossils and reconstructions of these species will offer visitors a fuller picture of their remarkable life histories and the ecosystems they were a part of.

The exhibition will also explore deeper similarities across the ecology and anatomy of ocean animals then and now. After the marine reptiles that dominated these waters went extinct 66 million years ago, modern marine mammals would not only later replace them as top predators in the world’s ocean, but also converge on many of the same body shapes and survival strategies.

The Forces That Shape Life, Then and Now
This unique period in Earth’s history reveals how key geologic and environmental forces contributed to the early establishment and evolution of life in the South Atlantic. As Africa and South America drifted apart and a new ocean basin formed, trade winds blowing along the new Angolan coastline created the conditions for upwelling, an ocean process that drives the circulation of nutrients from the deep ocean to its surface. These nutrients in turn jump-started the food web that attracted the ferocious marine reptile predators featured throughout the exhibition.

Just as tectonic forces helped create this Cretaceous marine environment, they also shaped the arid coastal cliffs where the fossils are found today. Starting 45,000 years ago, a geologic process called uplift caused Earth’s crust to bulge along Angola’s coast, lifting part of the seafloor out of the water — and along with it, the layers upon layers of fossil-filled rocks where Projecto PaleoAngola scientists work.

Though humans do not operate on a tectonic scale, their actions also have major impacts on ocean life. Humans are now the ocean’s top predators, with one-fifth of the world’s population relying on food from upwelling-based ecosystems. Scientists caution that with such great pressure on modern upwelling-based fisheries, overfishing could change the future of life in the ocean by threatening fish populations, marine ecosystems and even human health. — National Museum of Natural History

About the National Museum of Natural History
The National Museum of Natural History is connecting people everywhere with Earth’s unfolding story. The museum is one of the most visited natural history museums in the world with approximately 7 million annual visitors from the U.S. and around the world. Opened in 1910, the museum is dedicated to maintaining and preserving the world’s most extensive collection of natural history specimens and human artifacts. It is open daily from 10 a.m. to 5:30 p.m. (closed Dec. 25). Admission is free. For more information, visit the museum on its website and on Facebook and Twitter.

Tags Dedman College, Institute for the Study of Earth and Man, Louis L. Jacobs, Roy M. Huffington Department of Earth Sciences

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SMU physicist and her students join national laboratories, other universities in high-stakes hunt for elusive dark matter

Post author By Margaret Allen
Post date May 7, 2018

The future SuperCDMS SNOLAB experiment will hunt for weakly interacting massive particles (WIMPs), hypothetical components of dark matter. If a WIMP (white trace) strikes an atom inside the experiment's detector crystals (gray), it will cause the crystal lattice to vibrate (blue). The collision will also send electrons (red) through the crystal that enhance the vibrations. (Greg Stewart/SLAC National Accelerator Laboratory)

“One of our major concerns is background particles that can mimic the dark matter signature in our detectors.” — Jodi Cooley

SMU physicist Jodi Cooley is a member of the international scientific team that will use a powerful new tool to understand one of the biggest mysteries of modern physics.

The U.S. Department of Energy has approved funding and start of construction for SuperCDMS SNOLAB, a $34 million experiment designed to detect dark matter.

SuperCDMS will begin operations in the early 2020s to hunt for hypothetical dark matter particles called weakly interacting massive particles, or WIMPs.

“Understanding the nature of dark matter is one of the most important scientific puzzles in particle astrophysics today,” said Cooley, an associate professor of experimental particle physics. “The experiment will have unprecedented sensitivity to dark matter particles that are hypothesized to have very low mass and interact very rarely. So they are extremely challenging to detect. This challenge has required us to develop cutting edge detectors.”

Cooley is one of 111 scientists from 26 institutions in the SuperCDMS collaboration. SMU graduate students on the experiment include Matt Stein (Ph.D. ’18) and Dan Jardin; and also previously Hang Qiu (Ph.D. ’17).

Physicists are searching for dark matter because although it makes up the bulk of the universe it remains a mystery. They theorize that dark matter could be composed of dark matter particles, with WIMPs a top contender for the title.

If dark matter WIMP particles exist, they would barely interact with their environment and fly right through regular matter. However, every so often, they could collide with an atom of our visible world, and dark matter researchers are looking for these rare interactions.

The SuperCDMS experiment will be the world’s most sensitive for detecting the relatively light WIMPs.

Cooley and her students in the SMU Department of Physics have been working with Washington-based Pacific Northwest National Laboratory on the challenge of background control and material selection for the experiment’s WIMP detectors.

Understanding background signals in the experiment is a major challenge for the detection of the faint WIMP signals.

“One of our major concerns is background particles that can mimic the dark matter signature in our detectors,” Cooley said. “As such, the experiment is constructed from radiopure materials that are carefully characterized through a screening and assay before they are selected.”

The SMU research team also has performed simulations of background particles in the detectors.

“Doing this helps inform the design of the experiment shield,” Cooley said. “We want to select the right materials to use in construction of the experiment. For example, materials that are too high in radioactivity will produce background particles that might produce fake dark matter signals in our detectors. We are extremely careful to use materials that block background particles. We also take great care that the material we use to hold the detectors in place — copper — is very radiopure.”

The experiment will be assembled and operated within the existing Canadian laboratory SNOLAB – 6,800 feet underground inside a nickel mine near the city of Sudbury. That’s the deepest underground laboratory in North America.

The experiment’s detectors will be protected from high-energy particles, called cosmic radiation, which can create the unwanted background signals that Cooley’s team wants to prevent.

SuperCDMS SNOLAB will be 50 times more sensitive than predecessor
Scientists know that visible matter in the universe accounts for only 15 percent of all matter. The rest is the mysterious substance called dark matter.

Due to its gravitational pull on regular matter, dark matter is a key driver for the evolution of the universe, affecting the formation of galaxies like our Milky Way. It therefore is fundamental to our very own existence.

The SuperCDMS SNOLAB experiment will be at least 50 times more sensitive than its predecessor, exploring WIMP properties that can’t be probed by other experiments.

The search will be done using silicon and germanium crystals, in which the collisions would trigger tiny vibrations. However, to measure the atomic jiggles, the crystals need to be cooled to less than minus 459.6 degrees Fahrenheit — a fraction of a degree above absolute zero temperature.

The ultra-cold conditions give the experiment its name: Cryogenic Dark Matter Search, or CDMS. The prefix “Super” indicates an increased sensitivity compared to previous versions of the experiment.

Experiment will measure “fingerprints” left by dark matter
The collisions would also produce pairs of electrons and electron deficiencies that move through the crystals, triggering additional atomic vibrations that amplify the signal from the dark matter collision. The experiment will be able to measure these “fingerprints” left by dark matter with sophisticated superconducting electronics.

Besides Pacific Northwest National Laboratory, two other Department of Energy national labs are involved in the project.

SLAC National Accelerator Laboratory in California is managing the construction project. SLAC will provide the experiment’s centerpiece of initially four detector towers, each containing six crystals in the shape of oversized hockey pucks. SLAC built and tested a detector prototype. The first tower could be sent to SNOLAB by the end of 2018.

Fermi National Accelerator Laboratory is working on the experiment’s intricate shielding and cryogenics infrastructure.

“Our experiment will be the world’s most sensitive for relatively light WIMPs,” said Richard Partridge, head of the SuperCDMS group at the Kavli Institute for Particle Astrophysics and Cosmology, a joint institute of SLAC and Stanford University. “This unparalleled sensitivity will create exciting opportunities to explore new territory in dark matter research.”

Close-knit network of strong partners is crucial to success
Besides SMU, a number of U.S. and Canadian universities also play key roles in the experiment, working on tasks ranging from detector fabrication and testing to data analysis and simulation. The largest international contribution comes from Canada and includes the research infrastructure at SNOLAB.

“We’re fortunate to have a close-knit network of strong collaboration partners, which is crucial for our success,” said Project Director Blas Cabrera from KIPAC. “The same is true for the outstanding support we’re receiving from the funding agencies in the U.S. and Canada.”

Funding is from the DOE Office of Science, $19 million, the National Science Foundation, $12 million, and the Canada Foundation for Innovation, $3 million.

SuperCDMS to search for dark matter in entirely new region
“Together we’re now ready to build an experiment that will search for dark matter particles that interact with normal matter in an entirely new region,” said SuperCDMS spokesperson Dan Bauer, Fermilab.

SuperCDMS SNOLAB will be the latest in a series of increasingly sensitive dark matter experiments. The most recent version, located at the Soudan Mine in Minnesota, completed operations in 2015.

”The project has incorporated lessons learned from previous CDMS experiments to significantly improve the experimental infrastructure and detector designs for the experiment,” said SLAC’s Ken Fouts, project manager for SuperCDMS SNOLAB. “The combination of design improvements, the deep location and the infrastructure support provided by SNOLAB will allow the experiment to reach its full potential in the search for low-mass dark matter.” — SLAC National Laboratory; and Margaret Allen, SMU

Tags Dedman College, Jodi Cooley, SMU Department of Physics

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WFAA Verify: Is West Texas sinking?

Post author By Margaret Allen
Post date April 19, 2018
No Comments on WFAA Verify: Is West Texas sinking?

A new research report, from Southern Methodist University and funded by NASA, found a “…large swath of West Texas oil patch is heaving and sinking at alarming rates.”

WFAA-TV Channel 8’s Verify journalist David Schechter covered the phenomenon of the ground sinking at alarming rates in West Texas, according to the research of SMU geophysicists Zhong Lu, professor, Shuler-Foscue Chair, and Jin-Woo Kim research scientist, both in the Roy M. Huffington Department of Earth Sciences.

The Dedman College researchers are co-authors of a new analysis using satellite radar images that discovered decades of oil production activity in West Texas have destabilized localities in an area of about 4,000 square miles populated by small towns, roadways and a vast network of oil and gas pipelines and storage tanks.

Schechter’s WFAA ABC report, “Verify: Is West Texas sinking?” aired April 18, 2018.

Lu and Kim reported their findings in the Nature publication Scientific Reports, in the article “Association between localized geohazards in West Texas and human activities, recognized by Sentinel-1A/B satellite radar imagery.”

The researchers analyzed satellite radar images that were made public by the European Space Agency, and supplemented that with oil activity data from the Railroad Commission of Texas.

The study is among the first of its kind to identify small-scale deformation signals over a vast region by drawing from big data sets spanning a number of years and then adding supplementary information.

The research is supported by the NASA Earth Surface and Interior Program, and the Shuler-Foscue Endowment at SMU.

An earlier study by the researchers revealed significant ground movement of two giant sinkholes near Wink, Texas. The SMU geophysicists found that the movement suggests the two existing holes are expanding, and new ones are forming as nearby subsidence occurs at an alarming rate.

Watch the WFAA Verify news segment.

EXCERPT:

By David Schechter
WFAA-TV Verify
A new research report, from Southern Methodist University and funded by NASA, found a “…large swath of West Texas oil patch is heaving and sinking at alarming rates.”

To find out if West Texas is sinking, first I’m going to the guy who wrote the report, Dr. Zhong Lu. He’s a geophysicist who studies the earth using satellites.

By shooting a radar beam from space — like a measuring stick — a satellite can calculate elevation changes down to the centimeter. Lu did that over a 4000 square mile area.

“This area is sinking at half meter per year,” Dr. Lu says.

That’s more than a foot-and-a-half. Lu says, that’s alarming because that much change to the earth’s surface might normally take millions of years.

One of the images in his reports shows an area of sinking earth, near Wink, TX from 2011. Five years later, the satellite shows the sunken area had spread almost 240%.

“In this area that you are studying, is oil and gas the cause of the sinking?” I ask.

“Related to the oil and gas activities,” he says.

“Oil and gas activity is causing the sinking in West Texas?” I clarify.

“Yes,” he says.

Watch the WFAA Verify news segment.

Tags Dedman College, Jin-woo Kim, Roy M. Huffington Department of Earth Sciences, Zhong Lu

Earth & Climate Energy & Matter Researcher news SMU In The News Student researchers

The Guardian: Texas sinkholes — oil and gas drilling increases threat, scientists warn

Post author By Margaret Allen
Post date April 4, 2018

Ground rising and falling in region that has been ‘punctured like a pin cushion’ since the 1940s, new study finds.

The Guardian and other news outlets covered the West Texas sinkhole and ground movement research of SMU geophysicists Zhong Lu, professor, Shuler-Foscue Chair, and Jin-Woo Kim research scientist, both in the Roy M. Huffington Department of Earth Sciences at SMU.

The Dedman College researchers are co-authors of a new analysis using satellite radar images that shows decades of oil production activity in West Texas have destabilized localities in an area of about 4,000 square miles populated by small towns, roadways and a vast network of oil and gas pipelines and storage tanks.

The Guardian article by journalist Tom Dart was published March 27, 2018, “Texas sinkholes: oil and gas drilling increases threat, scientists warn.”

Other coverage includes articles by Forbes, Tech Times, Phys.org, Ecowatch, Fox San Antonio, The Dallas Morning News and the Texas Tribune.

Others include EarthSky.org, Live Science, KERA News, San Antonio Express, Houston Chronicle, Science Daily, The Energy Mix, Digital Journal, Homeland Security News Wire and the Science Bulletin.

Lu is world-renowned for leading scientists in InSAR applications, short for a technique called interferometric synthetic aperture radar, to detect surface changes that aren’t visible to the naked eye. Lu is a member of the Science Definition Team for the dedicated U.S. and Indian NASA-ISRO InSAR mission, set for launch in 2020 to study hazards and global environmental change.

InSAR accesses a series of images captured by a read-out radar instrument mounted on the orbiting satellite Sentinel-1A. Sentinel-1A was launched in April 2014 as part of the European Union’s Copernicus program.

Lu and Kim reported their latest findings in the Nature publication Scientific Reports, in the article “Association between localized geohazards in West Texas and human activities, recognized by Sentinel-1A/B satellite radar imagery.”

Lu and Kim reported the earlier findings in the scientific journal Remote Sensing, in the article “Ongoing deformation of sinkholes in Wink, Texas, observed by time-series Sentinel-1A SAR Interferometry.”

The research is supported by the U.S. Geological Survey Land Remote Sensing Program, the NASA Earth Surface & Interior Program, and the Shuler-Foscue Endowment at Southern Methodist University.

Read the full story.

EXCERPT:

By Tom Dart
The Guardian
Oil and gas activity is contributing to alarming land movements and a rising threat of sinkholes across a huge swath of west Texas, a new study suggests.

According to geophysicists from Southern Methodist University, the ground is rising and falling in a region that has been “punctured like a pin cushion with oil wells and injection wells since the 1940s”.

There were nearly 297,000 oil wells in Texas as of last month, according to the state regulator. Many are in the Permian Basin, described in a Bloomberg article last September as the “world’s hottest oil patch”.

But the Southern Methodist report warns of unstable land and the threat of sinkholes.

“These hazards represent a danger to residents, roads, railroads, levees, dams, and oil and gas pipelines, as well as potential pollution of ground water,” Zhong Lu, a professor, said in a statement.

Wink – a tiny town 400 miles west of Dallas best known as the childhood home of the singer Roy Orbison – attracted national headlines in 2016 when the same scientists warned that the land between two expanding sinkholes a mile apart was deteriorating, risking the formation of more sinkholes or even the creation of a colossal single hole.

Injection of wastewater and carbon dioxide increases pore pressure in rocks, a likely cause of uplift. Lu told the Guardian that cracks and corrosion from ageing wells may help explain the sinking.

A “subsidence bowl” near one of the Wink sinkholes has sunk at a rate of more than 15.5in a year, probably as a result of water leaks through abandoned wells causing salt layers to dissolve, the report found. Elsewhere, a lake formed after 2003 as a result of sinking ground and rising water.

Read the full story.

Tags Dedman College, Jin-woo Kim, Roy M. Huffington Department of Earth Sciences, Zhong Lu

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Radar images show large swath of West Texas oil patch is heaving and sinking at alarming rates

Post author By Margaret Allen
Post date March 20, 2018

Analysis indicates decades of oil production activity have destabilized localities in an area of about 4,000 square miles populated by small towns, roadways and a vast network of oil and gas pipelines and storage tanks

Two giant sinkholes near Wink, Texas, may just be the tip of the iceberg, according to a new study that found alarming rates of new ground movement extending far beyond the infamous sinkholes.

That’s the finding of a geophysical team from Southern Methodist University, Dallas that previously reported the rapid rate at which the sinkholes are expanding and new ones forming.

Now the team has discovered that various locations in large portions of four Texas counties are also sinking and uplifting.

Radar satellite images show significant movement of the ground across localities in a 4000-square-mile area — in one place as much as 40 inches over the past two-and-a-half years, say the geophysicists.

“The ground movement we’re seeing is not normal. The ground doesn’t typically do this without some cause,” said geophysicist Zhong Lu, a professor in the Roy M. Huffington Department of Earth Sciences at SMU and a global expert in satellite radar imagery analysis.

“These hazards represent a danger to residents, roads, railroads, levees, dams, and oil and gas pipelines, as well as potential pollution of ground water,” Lu said. “Proactive, continuous detailed monitoring from space is critical to secure the safety of people and property.”

The scientists made the discovery with analysis of medium-resolution (15 feet to 65 feet) radar imagery taken between November 2014 and April 2017. The images cover portions of four oil-patch counties where there’s heavy production of hydrocarbons from the oil-rich West Texas Permian Basin.

The imagery, coupled with oil-well production data from the Railroad Commission of Texas, suggests the area’s unstable ground is associated with decades of oil activity and its effect on rocks below the surface of the earth.

The SMU researchers caution that ground movement may extend beyond what radar observed in the four-county area. The entire region is highly vulnerable to human activity due to its geology — water-soluble salt and limestone formations, and shale formations.

“Our analysis looked at just this 4000-square-mile area,” said study co-author and research scientist Jin-Woo Kim, a research scientist in the SMU Department of Earth Sciences.

“We’re fairly certain that when we look further, and we are, that we’ll find there’s ground movement even beyond that,” Kim said. “This region of Texas has been punctured like a pin cushion with oil wells and injection wells since the 1940s and our findings associate that activity with ground movement.”

Lu, Shuler-Foscue Chair at SMU, and Kim reported their findings in the Nature publication Scientific Reports, in the article “Association between localized geohazards in West Texas and human activities, recognized by Sentinel-1A/B satellite radar imagery.”

The researchers analyzed satellite radar images that were made public by the European Space Agency, and supplemented that with oil activity data from the Railroad Commission of Texas.

The research is supported by the NASA Earth Surface and Interior Program, and the Shuler-Foscue Endowment at SMU.

Imagery captures changes that might otherwise go undetected
The SMU geophysicists focused their analysis on small, localized, rapidly developing hazardous ground movements in portions of Winkler, Ward, Reeves and Pecos counties, an area nearly the size of Connecticut. The study area includes the towns of Pecos, Monahans, Fort Stockton, Imperial, Wink and Kermit.

The images from the European Space Agency are the result of satellite radar interferometry from recently launched open-source orbiting satellites that make radar images freely available to the public.

With interferometric synthetic aperture radar, or InSAR for short, the satellites allow scientists to detect changes that aren’t visible to the naked eye and that might otherwise go undetected.

The satellite technology can capture ground deformation with an accuracy of sub-inches or better, at a spatial resolution of a few yards or better over thousands of miles, say the researchers.

Ground movement associated with oil activity
The SMU researchers found a significant relationship between ground movement and oil activities that include pressurized fluid injection into the region’s geologically unstable rock formations.

Fluid injection includes waste saltwater injection into nearby wells, and carbon dioxide flooding of depleting reservoirs to stimulate oil recovery.

Injected fluids increase the pore pressure in the rocks, and the release of the stress is followed by ground uplift. The researchers found that ground movement coincided with nearby sequences of wastewater injection rates and volume and CO2 injection in nearby wells.

Also related to the ground’s sinking and upheaval are dissolving salt formations due to freshwater leaking into abandoned underground oil facilities, as well as the extraction of oil.

Sinking and uplift detected from Wink to Fort Stockton
As might be expected, the most significant subsidence is about a half-mile east of the huge Wink No. 2 sinkhole, where there are two subsidence bowls, one of which has sunk more than 15.5 inches a year. The rapid sinking is most likely caused by water leaking through abandoned wells into the Salado formation and dissolving salt layers, threatening possible ground collapse.

At two wastewater injection wells 9.3 miles west of Wink and Kermit, the radar detected upheaval of about 2.1 inches that coincided with increases in injection volume. The injection wells extend about 4,921 feet to 5,577 feet deep into a sandstone formation.

In the vicinity of 11 CO2 injection wells nearly seven miles southwest of Monahans, the radar analysis detected surface uplift of more than 1 inch. The wells are about 2,460 feet to 2,657 feet deep. As with wastewater injection, CO2 injection increased pore pressure in the rocks, so when stress was relieved it was followed by uplift of about 1 inch at the surface.

The researchers also looked at an area 4.3 miles southwest of Imperial, where significant subsidence from fresh water flowing through cracked well casings, corroded steel pipes and unplugged abandoned wells has been widely reported.

Water there has leaked into the easily dissolved Salado formation, created voids, and caused the ground to sink and water to rise from the subsurface, including creating Boehmer Lake, which didn’t exist before 2003.

Radar analysis by the SMU team detected rapid subsidence ranging from three-fourths of an inch to nearly 4 inches around active wells, abandoned wells and orphaned wells.

“Movements around the roads and oil facilities to the southwest of Imperial, Texas, should be thoroughly monitored to mitigate potential catastrophes,” the researchers write in the study.

About 5.5 miles south of Pecos, their radar analysis detected more than 1 inch of subsidence near new wells drilled via hydraulic fracturing and in production since early 2015. There have also been six small earthquakes recorded there in recent years, suggesting the deformation of the ground generated accumulated stress and caused existing faults to slip.

“We have seen a surge of seismic activity around Pecos in the last five to six years. Before 2012, earthquakes had not been recorded there. At the same time, our results clearly indicate that ground deformation near Pecos is occurring,” Kim said. “Although earthquakes and surface subsidence could be coincidence, we cannot exclude the possibility that these earthquakes were induced by hydrocarbon production activities.”

Scientists: Boost the network of seismic stations to better detect activity
Kim stated the need for improved earthquake location and detection threshold through an expanded network of seismic stations, along with continuous surface monitoring with the demonstrated radar remote sensing methods.

“This is necessary to learn the cause of recent increased seismic activity,” Kim said. “Our efforts to continuously monitor West Texas with this advanced satellite technique can help sustain safe, ongoing oil production.”

Near real-time monitoring of ground deformation possible in a few years
The satellite radar datasets allowed the SMU geophysicists to detect both two-dimension east-west deformation of the ground, as well as vertical deformation.

Lu, a leading scientist in InSAR applications, is a member of the Science Team for the dedicated U.S. and Indian NASA-ISRO (called NISAR) InSAR mission, set for launch in 2021 to study hazards and global environmental change.

InSAR accesses a series of images captured by a read-out radar instrument mounted on the orbiting satellite Sentinel-1A/B. The satellites orbit 435 miles above the Earth’s surface. Sentinel-1A was launched in 2014 and Sentinel-1B in 2016 as part of the European Union’s Copernicus program.

The Sentinel-1A/B constellation bounces a radar signal off the earth, then records the signal as it bounces back, delivering measurements. The measurements allow geophysicists to determine the distance from the satellite to the ground, revealing how features on the Earth’s surface change over time.

“Near real-time monitoring of ground deformation at high spatial and temporal resolutions is possible in a few years, using multiple satellites such as Sentinel-1A/B, NISAR and others,” said Lu. “This will revolutionize our capability to characterize human-induced and natural hazards, and reduce their damage to humanity, infrastructure and the energy industry.” — Margaret Allen, SMU

Tags Dedman College, Jin-woo Kim, Roy M. Huffington Department of Earth Sciences, Zhong Lu

Earth & Climate Energy & Matter Fossils & Ruins Researcher news SMU In The News

The Dallas Morning News: Earthquakes at DFW Airport continued for years after oil and gas wastewater well was shut

Post author By Margaret Allen
Post date February 23, 2018

“Faults are not like a light switch – you don’t turn off a well and automatically stop triggering earthquakes.” — Heather DeShon, SMU seismologist.

Science journalist Anna Kuchment covered the earthquake research of a team of SMU seismologists led by SMU Associate Professor Heather DeShon and SMU Post-doctoral Researcher Paul Ogwari, who developed a unique method of data analysis that yielded the study results.

Kuchment wrote Earthquakes at DFW Airport continued for years after oil and gas wastewater well was shut for The Dallas Morning News.

The results of the analysis showed that efforts to stop human-caused earthquakes by shutting down wastewater injection wells that serve adjacent oil and gas fields may oversimplify the challenge. The seismologists analyzed a sequence of earthquakes at DFW Airport and found that even though wastewater injection was halted after a year, the earthquakes continued.

The sequence of quakes began in 2008, and wastewater injection was halted in 2009. But earthquakes continued for at least seven more years.

“This tells us that high-volume injection, even if it’s just for a short time, when it’s near a critically stressed fault, can induce long-lasting seismicity,” said Ogwari. The earthquakes may be continuing even now, he said.

The article by Kuchment, “Earthquakes at DFW Airport continued for years after oil and gas wastewater well was shut,” published Feb. 21, 2018.

Read the full story.

EXCERPT:

By Anna Kuchment
The Dallas Morning News
Earthquakes beneath DFW International Airport continued for seven years after an oil and gas company shut a nearby wastewater injection well that had been linked to the quakes, according to a new study by scientists at Southern Methodist University.

A wastewater well that continues to operate at the northern end of the airport – and which some area residents have said should be closed — was probably not involved in the events and poses little earthquake hazard, the researchers concluded.

“Faults are not like a light switch – you don’t turn off a well and automatically stop triggering earthquakes,” said Heather DeShon, a seismologist at Southern Methodist University and co-author of the paper, in an email.

The earthquakes at DFW Airport started on Halloween 2008, seven weeks after Chesapeake Energy began injecting wastewater into a well at the southern end of the airport. Scientists at SMU and the University of Texas at Austin investigated the quakes at the time and concluded they were most likely associated with the well.

Though Chesapeake shut its well in August 2009, earthquakes continued through at least the end of 2015. The largest, a 3.4-magnitude event, struck three years after the well was closed.

“It’s very surprising that one year of injection could produce earthquakes running for more than seven years,” said Paul Ogwari, the study’s lead author and a post-doctoral researcher at SMU. The paper was published in the Journal of Geophysical Research.

While earthquake magnitudes did not decline, Ogwari said, earthquake rates did: More than 80 percent of quakes in the sequence occurred during the first seven months of seismicity.

The DFW quakes are significant, because they mark the start of an unprecedented surge of earthquakes in North Texas and across the middle of the country.

Read the full story.

Tags Dedman College, Heather R. DeShon, Matthew J. Hornbach, Paul Ogwari, Roy M. Huffington Department of Earth Sciences

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Solving the dark energy mystery: A new sky survey assignment for a 45-year-old telescope

Post author By Margaret Allen
Post date February 16, 2018

SMU and other members of a scientific consortium prepare for installation of the Dark Energy Spectroscopic Instrument to survey the night sky from a mile-high mountain peak in Arizona

As part of a large scientific consortium studying dark energy, SMU physicists are on course to help create the largest 3-D map of the universe ever made.

The map will emerge from data gathered by the Dark Energy Spectroscopic Instrument (DESI) being installed on the Nicholas U. Mayall Telescope atop a mountain in Arizona.

The map could help solve the mystery of dark energy, which is driving the accelerating expansion of the universe.

DESI will capture about 10 times more data than a predecessor survey of space using an array of 5,000 swiveling robots. Each robot will be carefully choreographed to point a fiber-optic cable at a preprogrammed sequence of deep-space objects, including millions of galaxies and quasars, which are galaxies that harbor massive, actively feeding black holes.

“DESI will provide the first precise measures of the expansion history of the universe covering approximately the last 10 billion years,” said SMU physicist Robert Kehoe, a professor in the SMU Department of Physics. “This is most of the 13 billion year age of the universe, and it encompasses a critical period in which the universe went from being matter-dominated to dark-energy dominated.”

The universe was expanding, but at a slowing pace, until a few billion years ago, Kehoe said.

“Then the expansion started accelerating,” he said. “The unknown ‘dark energy’ driving that acceleration is now dominating the universe. Seeing this transition clearly will provide a critical test of ideas of what this dark energy is, and how it may tie into theories of gravitation and other fundamental forces.”

The Mayall telescope was originally commissioned 45 years ago to survey the night sky and record observations on glass photographic plates. The telescope is tucked inside a 14-story, 500-ton dome atop a mile-high peak at the National Science Foundation’s Kitt Peak National Observatory – part of the National Optical Astronomy Observatory.

SMU researchers have conducted observing with the Mayall. Decommissioning of that telescope allows for building DESI in it’s place, as well as reusing some parts of the telescope and adding major new sytems. As part of DESI, SMU is involved in development of software for operation of the experiment, as well as for data simulation to aid data anlysis.

“We are also involved in studying the ways in which observational effects impact the cosmology measurements DESI is pursuing,” Kehoe said. SMU graduate students Govinda Dhungana and Ryan Staten also work on DESI. A new addition to the SMU DESI team, post-doctoral researcher Sarah Eftekharzadeh, is working on the SMU software and has studied the same kinds of galaxies
DESI will be measuring.

Now the dome is closing on the previous science chapters of the 4-meter Mayall Telescope so that it can prepare for its new role in creating the 3-D map.

The temporary closure sets in motion the largest overhaul in the telescope’s history and sets the stage for the installation of the Dark Energy Spectroscopic Instrument, which will begin a five-year observing run next year.

“This day marks an enormous milestone for us,” said DESI Director Michael Levi of the Department of Energy’s Lawrence Berkeley National Laboratory , which leads the project’s international collaboration. “Now we remove the old equipment and start the yearlong process of putting the new stuff on.”

More than 465 researchers from about 71 institutions are participating in the DESI collaboration.

The entire top end of the telescope, which weighs as much as a school bus and houses the telescope’s secondary mirror and a large digital camera, will be removed and replaced with DESI instruments. A large crane will lift the telescope’s top end through the observing slit in its dome.

Besides providing new insights about the universe’s expansion and large-scale structure, DESI will also help to set limits on theories related to gravity and the formative stages of the universe, and could even provide new mass measurements for a variety of elusive yet abundant subatomic particles called neutrinos.

“One of the primary ways that we learn about the unseen universe is by its subtle effects on the clustering of galaxies,” said DESI collaboration co-spokesperson Daniel Eisenstein of Harvard University. “The new maps from DESI will provide an exquisite new level of sensitivity in our study of cosmology.”

Mayall’s sturdy construction is perfect platform for new 9-ton instrument
The Mayall Telescope has played an important role in many astronomical discoveries, including measurements supporting the discovery of dark energy and establishing the role of dark matter in the universe from measurements of galaxy rotation. Its observations have also been used in determining the scale and structure of the universe. Dark matter and dark energy together are believed to make up about 95 percent of all of the universe’s mass and energy.

It was one of the world’s largest optical telescopes at the time it was built, and because of its sturdy construction it is perfectly suited to carry the new 9-ton instrument.

“We started this project by surveying large telescopes to find one that had a suitable mirror and wouldn’t collapse under the weight of such a massive instrument,” said Berkeley Lab’s David Schlegel, a DESI project scientist.

Arjun Dey, the NOAO project scientist for DESI, explained, “The Mayall was precociously engineered like a battleship and designed with a wide field of view.”

The expansion of the telescope’s field-of-view will allow DESI to map out about one-third of the sky.

DESI will transform the speed of science with automated preprogrammed robots
Brenna Flaugher, a DESI project scientist who leads the astrophysics department at Fermi National Accelerator Laboratory, said DESI will transform the speed of science at the Mayall Telescope.

“The telescope was designed to carry a person at the top who aimed and steered it, but with DESI it’s all automated,” she said. “Instead of one at a time we can measure the velocities of 5,000 galaxies at a time – we will measure more than 30 million of them in our five-year survey.”

DESI will use an array of 5,000 swiveling robots, each carefully choreographed to point a fiber-optic cable at a preprogrammed sequence of deep-space objects, including millions of galaxies and quasars, which are galaxies that harbor massive, actively feeding black holes.

The fiber-optic cables will carry the light from these objects to 10 spectrographs, which are tools that will measure the properties of this light and help to pinpoint the objects’ distance and the rate at which they are moving away from us. DESI’s observations will provide a deep look into the early universe, up to about 11 billion years ago.

DESI will capture about 10 times more data than a predecessor survey
The cylindrical, fiber-toting robots, which will be embedded in a rounded metal unit called a focal plate, will reposition to capture a new exposure of the sky roughly every 20 minutes. The focal plane assembly, which is now being assembled at Berkeley Lab, is expected to be completed and delivered to Kitt Peak this year.

DESI will scan one-third of the sky and will capture about 10 times more data than a predecessor survey, the Baryon Oscillation Spectroscopic Survey (BOSS). That project relied on a manually rotated sequence of metal plates – with fibers plugged by hand into pre-drilled holes – to target objects.

All of DESI’s six lenses, each about a meter in diameter, are complete. They will be carefully stacked and aligned in a steel support structure and will ultimately ride with the focal plane atop the telescope.

Each of these lenses took shape from large blocks of glass. They have criss-crossed the globe to receive various treatments, including grinding, polishing, and coatings. It took about 3.5 years to produce each of the lenses, which now reside at University College London in the U.K. and will be shipped to the DESI site this spring.

Precise measurements of millions of galaxies will reveal effects of dark energy
The Mayall Telescope has most recently been enlisted in a DESI-supporting sky survey known as the Mayall z-Band Legacy Survey, which is one of four sky surveys that DESI will use to preselect its targeted sky objects. SMU astrophysicists carried out observing duties on that survey, which wrapped up just days ago on Feb. 11, to support the coming DESI scientific results.

Data from these surveys are analyzed at Berkeley Lab’s National Energy Research Scientific Computing Center, a DOE Office of Science User Facility. Data from these surveys have been released to the public at http://legacysurvey.org.

“We can see about a billion galaxies in the survey images, which is quite a bit of fun to explore,” Schlegel said. “The DESI instrument will precisely measure millions of those galaxies to see the effects of dark energy.” 

Levi noted that there is already a lot of computing work underway at the Berkeley computing center to prepare for the stream of data that will pour out of DESI once it starts up.

“This project is all about generating huge quantities of data,” Levi said. “The data will go directly from the telescope to the Berkeley computing center for processing. We will create hundreds of universes in these computers and see which universe best fits our data.”

Installation of DESI’s components is expected to begin soon and to wrap up in April 2019, with first science observations planned in September 2019.

“Installing DESI on the Mayall will put the telescope at the heart of the next decade of discoveries in cosmology,” said Risa Wechsler, DESI collaboration co-spokesperson and associate professor of physics and astrophysics at SLAC National Accelerator Laboratory and Stanford University. “The amazing 3-D map it will measure may solve some of the biggest outstanding questions in cosmology, or surprise us and bring up new ones.” — Berkeley Lab and SMU

Tags Dark Energy Spectroscopic Instrument, Dedman College, DESI, Govinda Dhungana, Robert Kehoe, Ryan Staten, Sarah Eftekharzadeh, SMU Department of Physics

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SMU study finds earthquakes continue for years after gas field wastewater injection stops

Post author By Margaret Allen
Post date February 13, 2018

High rates of injection and large volumes can perturb critically stressed faults, triggering earthquakes years after wastewater wells are shut in.

Efforts to stop human-caused earthquakes by shutting down wastewater injection wells that serve adjacent oil and gas fields may oversimplify the challenge, according to a new study from seismologists at Southern Methodist University, Dallas.

The seismologists analyzed a sequence of earthquakes at DFW Airport and found that even though wastewater injection was halted after a year, the earthquakes continued.

The sequence of quakes began in 2008, and wastewater injection was halted in 2009. But earthquakes continued for at least seven more years.

“This tells us that high-volume injection, even if it’s just for a short time, when it’s near a critically stressed fault, can induce long-lasting seismicity,” said SMU seismologist Paul O. Ogwari, who developed a unique method of data analysis that yielded the study results.

The earthquakes may be continuing even now, said Ogwari, whose analysis extended through 2015.

The study’s findings indicate that shutting down injection wells in reaction to earthquakes, as some states such as Oklahoma and Arkansas are doing, may not have the desired effect of immediately stopping further earthquakes, said seismologist Heather DeShon, a co-author on the study and an associate professor in the SMU Earth Sciences Department.

“The DFW earthquake sequence began on Halloween in 2008 — before Oklahoma seismicity rates had notably increased,” said DeShon. “This study revisits what was technically the very first modern induced earthquake sequence in this region and shows that even though the wastewater injector in this case had been shut off very quickly, the injection activity still perturbed the fault, so that generated earthquakes even seven years later.”

That phenomenon is not unheard of. Seismologists saw that type of earthquake response from a rash of human-induced earthquakes in Colorado after wastewater injection during the 1960s at the Rocky Mountain Arsenal near Denver. Similarly in that case, injection was started and stopped, but earthquakes continued.

Such a possibility has not been well understood outside scientific circles, said DeShon. She is a member of the SMU seismology team that has studied and published extensively on their scientific findings related to the unusual spate of human-induced earthquakes in North Texas.

“The perception is that if the oil and gas wastewater injectors are leading to this, then you should just shut the injection wells down,” DeShon said. “But Paul’s study shows that there’s a lot to be learned about the physics of the process, and by monitoring continuously for years.”

Ogwari, DeShon and fellow SMU seismologist Matthew J. Hornbach reported the findings in the peer-reviewed Journal of Geophysical Research in the article “The Dallas-Fort Worth Airport Earthquake Sequence: Seismicity Beyond Injection Period.”

Known DFW Airport quakes number more than 400
The DFW Airport’s unprecedented earthquake clusters were the first ever documented in the history of the North Texas region’s oil-rich geological system known as the Fort Worth Basin. The quakes are also the first of multiple sequences in the basin tied to large-scale subsurface disposal of waste fluids from oil and gas operations.

The DFW Airport earthquakes began in 2008, as did high-volume wastewater injection of brine. Most of the seismic activity occurred in the first two months after injection began, primarily within .62 miles, or 1 kilometer, from the well. Other clusters then migrated further to the northeast of the well over the next seven years. The quakes were triggered on a pre-existing regional fault that trends 3.7 miles, or 6 kilometers, northeast to southwest.

Ogwari, a post-doctoral researcher in the SMU Roy M. Huffington Earth Sciences Department in Dedman College, analyzed years of existing seismic data from the region to take a deeper look at the DFW Airport sequence, which totaled 412 earthquakes through 2015.

Looking at the data for those quakes, Ogwari discovered that they had continued for at least seven years into 2015 along 80% of the fault, even though injection was stopped after only 11 months in August of 2009.

Rate of quakes declined, but magnitude has never lessened
In another important finding from the study, Ogwari found that the magnitude of the DFW Airport earthquakes didn’t lessen over time, but instead held steady. Magnitude ranged from 0.5 to 3.4, with the largest one occurring three years after injection at the well was stopped.

“What we’ve seen here is that the magnitude is consistent over time within the fault,” Ogwari said. “We expect to see the bigger events during injection or immediately after injection, followed by abrupt decay. But instead we’re seeing the fault continue to produce earthquakes with similar magnitudes that we saw during injection.”

While the rate of earthquakes declined — there were 23 events a month from 2008 to 2009, but only 1 event a month after May 2010 — the magnitude stayed the same. That indicates the fault doesn’t heal completely.

“We don’t know why that is,” Ogwari said. “I think that’s a question that is out there and may need more research.”

More monitoring needed for human-induced quakes
Answering that question, and others, about the complex characteristics and behavior of faults and earthquakes, requires more extensive monitoring than is currently possible given the funding allotted to monitor quakes.

Monitoring the faults involves strategically placed stations that “listen” and record waves of intense energy echoing through the ground, DeShon said.

The Fort Worth Basin includes the Barnett shale, a major gas producing geological formation, atop the deep Ellenberger formation used for wastewater storage, which overlays a granite basement layer. The ancient Airport fault system extends through all units.

Friction prevented the fault from slipping for millions of years, but in 2008 high volumes of injected wastewater disturbed the Airport fault. That caused the fault to slip, releasing stored-up energy in waves. The most powerful waves were “felt” as the earth shaking.

“The detailed physical equations relating wastewater processes to fault processes is still a bit of a question,” DeShon said. “But generally the favored hypothesis is that the injected fluid changes the pressure enough to change the ratio of the downward stress to the horizontal stresses, which allows the fault to slip.” 
Earthquakes in North Texas were unheard of until 2008, so when they began to be felt, seismologists scrambled to install monitors. When the quakes died down, the monitoring stations were removed.

“As it stands now, we miss the beginning of the quakes. The monitors are removed when the earthquakes stop being felt,” DeShon said. “But this study tells us that there’s more to it than the ‘felt’ earthquakes. We need to know how the sequences start, and also how they end. If we’re ever going to understand what’s happening, we need the beginning, the middle — and the end. Not just the middle, after they are felt.”

Innovative method tapped for studying earthquake activity
Monitors the SMU team installed at the DFW Airport were removed when seismic activity appeared to have died down in 2009.

Ogwari hypothesized he could look at historical data from distant monitoring stations still in place to extract information and document the history of the DFW Airport earthquakes.

The distant stations are a part of the U.S. permanent network monitored and maintained by the U.S. Geological Survey. The nearest one is 152 miles, 245 kilometers, away.

Earthquake waveforms, like human fingerprints, are unique. Ogwari used the local station monitoring data to train software to identify DFW earthquakes on the distant stations. Ogwari took each earthquake’s digital fingerprint and searched through years of data, cross-correlating waveforms from both the near and regional stations and identified the 412 DFW Airport events.

“The earthquakes are small, less than magnitude three,” DeShon said. “So on the really distant stations it’s like searching for a needle in a haystack, sifting them from all the other tiny earthquakes happening all across the United States.”

Each path is unique for every earthquake, and seismologists record each wave’s movement up and down, north to south, and east to west. From that Ogwari analyzed the evolution of seismicity on the DFW airport fault over space and time. He was able to look at data from the distant monitors and find seismic activity at the airport as recent as 2015.

“Earthquakes occurring close in space usually have a higher degree of similarity,” Ogwari said. “As the separation distance increases the similarity decreases.”

To understand the stress on the fault, the researchers also modeled the location and timing of the pressure in the pores of the rock as the injected water infiltrated.

For the various earthquake clusters, the researchers found that pore pressure increased along the fault at varying rates, depending on how far the clusters were from the injection well, the rate and timing of injection, and hydraulic permeability of the fault.

The analysis showed pore-pressure changes to the fault from the injection well where the earthquakes started in 2008; at the location of the May 2010 quakes along the fault; and at the northern edge of the seismicity.

Will the DFW Airport fault continue to slip and trigger earthquakes?

“We don’t know,” Ogwari said. “We can’t tell how long it will continue. SMU and TexNet, the Texas Seismic Network, continue to monitor both the DFW Airport faults and other faults in the Basin.” — Margaret Allen, SMU

Tags Dedman College, Heather R. DeShon, Matthew J. Hornbach, Paul Ogwari, Roy M. Huffington Department of Earth Sciences

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Exploring the mysteries of the universe: Reality in the Shadows

Post author By Margaret Allen
Post date December 21, 2017

New knowledge has caused us to reconsider many previous conclusions about what the universe is and how it works.

Despite centuries of scientific advancements, there is much about the universe that remains unknown. New knowledge and discoveries in the last 20 years have challenged previously accepted ideas and theories that were once regarded as scientific truth and have subjected them to increasing scrutiny.

These additions to our knowledge have caused scientists to reconsider many previous conclusions about what the universe is and how it works.

““Reality in the Shadows”” or “What the Heck’s the Higgs?” is a new book that explores the concepts that shape our current understanding of the universe and the frontiers of our knowledge of the cosmos.

The authors — two physicists and an engineer — tell us in a manner that non-scientists can readily follow, why studies have moved to superstring theory/M-theory, ideas about extra dimensions of space, and ideas about new particles in nature to find answers. It also explores why these ideas are far from established as accurate descriptions of reality.

“Our book explains how we know what we know about the universe, what we don’t know, and what we wish we did know,” said co-author Stephen Sekula, an associate professor of Physics at SMU. A physicist, Sekula conducts research into the Higgs Boson at the energy frontier on CERN’s ATLAS Experiment.

The book was initiated by Frank Blitzer, an engineer who participated on national space programs like Apollo and Patriot, several years ago, Sekula said. He was joined by co-author S. James Gates Jr., well known for his work on supersymmetry, supergravity and superstring theory, a few years ago.

“Frank and Jim sought additional input to help complete the book, and serendipitously Frank’s grandson, Ryan, was an SMU undergraduate and Hunt Scholar who helped connect them to me,” Sekula said. “After over an additional year of work, the book was completed.”

The foundations of modern physics rest on ideas that are over 100 years old and battle-tested, Sekula said.

“But nature has offered us new puzzles that have not yet been successfully explained by those ideas,” he added. “Perhaps we don’t yet have the right idea, or perhaps we haven’t searched deep enough into the cosmos. These are exciting times, with opportunities for a new generation of physicists who might crack these puzzles. Our book will help a curious reader to see the way in which knowledge was established, and encourage them to be engaged in solving the new mysteries.”

“Reality in the Shadows,” available through YBK Publishers, describes how humanity came to learn the workings of the universe as groundwork for the science that found the Higgs particle. Now scientists are hunting for the explanations for dark matter and the accelerated expansion of the cosmos, as well as for the many new questions the Higgs Boson itself has raised.

Scientists have recently discovered colliding black holes and neutron stars, that there is more non-luminous matter (dark matter) in the universe than the ordinary stuff of everyday life, and that the universe seems to grow larger each second at a faster and faster rate. Readers will learn how scientists discern such features of the universe and begin to see how to think beyond what is known to what is not yet known.

Throughout the book are descriptions of important developments in theoretical physics that lead the reader to a step-by-step understanding.

Sekula teaches physics and conducts research at ATLAS. He contributed to the measurement of decay modes of the Higgs boson and to the measurement of its spin-parity quantum numbers. Complementary to these efforts, he has worked with colleagues on the ATLAS Experiment to search for additional Higgs bosons in nature, providing intellectual leadership and direct involvement in several searches.

Gates was named 2014 “Scientist of the Year” by the Harvard Foundation. He was elected to the prestigious National Academy of Sciences in 2013 and received the 2013 National Medal of Science, the highest recognition given to scientists by the United States.

Gates has been featured on many TV documentary programs on physics, including “The Elegant Universe,” “Einstein’s Big Idea,” “Fabric of the Cosmos” and “The Hunt for the Higgs.” His DVD series, “Superstring Theory: The DNA of Reality,” makes the complexities of unification theory comprehensible.

Blitzer has more than 50 years of experience in engineering, program management, and business development and participated on national space programs, and The Strategic Defense Initiative (SDI), holding several patents in guidance and control. He has spent more than 20 years in independent research of the subject of the book.

Tags Dedman College, sekula, SMU Department of Physics, Stephen J. Sekula

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Scientific American: Drilling Reawakens Sleeping Faults in Texas, Leads to Earthquakes

Post author By Margaret Allen
Post date December 6, 2017

For 300 million years faults showed no activity, and then wastewater injections from oil and gas wells came along. Study authors took a different approach in the new work — they hunted for deformed faults below Texas.

Science journalist Anna Kuchment covered the landmark earthquake research of a team of SMU geophysicists led by SMU Associate Professor Beatrice Magnani in the SMU Department of Earth Sciences. Kuchment wrote Drilling Reawakens Sleeping Faults in Texas, Leads to Earthquakes for Scientific American.

The SMU researchers tapped seismic data to analyze earthquakes in Texas over the past decade.

The results of the analysis showed that human activity is causing the earthquakes as a result of movement in faults that have been silent for at least 300 million years, until recent injection of oil and gas wastewater.

The article by Kuchment, “Drilling Reawakens Sleeping Faults in Texas, Leads to Earthquakes,” published Nov. 24, 2017.

Read the full story.

EXCERPT:

By Anna Kuchment
Scientific American
Since 2008, Texas, Oklahoma, Kansas and a handful of other states have experienced unprecedented surges of earthquakes. Oklahoma’s rate increased from one or two per year to more than 800. Texas has seen a sixfold spike. Most have been small, but Oklahoma has seen several damaging quakes stronger than magnitude 5. While most scientists agree that the surge has been triggered by the injection of wastewater from oil and gas production into deep wells, some have suggested these quakes are natural, arising from faults in the crust that move on their own every so often. Now researchers have traced 450 million years of fault history in the Dallas-Fort Worth area and learned these faults almost never move. “There hasn’t been activity along these faults for 300 million years,” says Beatrice Magnani, a seismologist at Southern Methodist University in Dallas and lead author of a paper describing the research, published today in Science Advances. “Geologically, we usually define these faults as dead.”

Magnani and her colleagues argue that these faults would not have produced the recent earthquakes if not for wastewater injection. Pressure from these injections propagates underground and can disturb weak faults. The work is another piece of evidence implicating drilling in the quakes, yet the Texas government has not officially accepted the link to one of its most lucrative industries.

Magnani and her colleagues studied the Texas faults using images of the subsurface similar to ultrasound scans. Known as seismic reflection data, the images are created by equipment that generates sound waves and records the speeds at which the waves bounce off faults and different rock layers deep within the ground. Faults that have produced earthquakes look like vertical cracks in a brick wall, where one side of the wall has sunk down a few inches so the rows of bricks no longer line up. Scientists know the age of each rock layer—each row of bricks–based on previous studies that have used a variety of dating techniques.

Read the full story.

Tags Beatrice Magnani, Dedman College, Heather R. DeShon, Matthew J. Hornbach, Roy M. Huffington Department of Earth Sciences

Earth & Climate Energy & Matter Fossils & Ruins Researcher news SMU In The News

The Washington Post: Oil and gas industry is causing Texas earthquakes, a ‘landmark’ study suggests

Post author By Margaret Allen
Post date December 4, 2017

The study authors took a different approach in the new work — they hunted for deformed faults below Texas.

The Washington Post covered the landmark earthquake research of a team of SMU geophysicists led by SMU Associate Professor Beatrice Magnani in the SMU Department of Earth Sciences.

The researchers tapped seismic data to analyze earthquakes in Texas over the past decade.

The article by journalist Ben Guarino, “Oil and gas industry is causing Texas earthquakes, a ‘landmark’ study suggests,” published Nov. 24, 2017.

Read the full story.

EXCERPT:

By Ben Guarino
The Washington Post
An unnatural number of earthquakes hit Texas in the past decade, and the region’s seismic activity is increasing. In 2008, two earthquakes stronger than magnitude 3 struck the state. Eight years later, 12 did.

Natural forces trigger most earthquakes. But humans are causing earthquakes, too, with mining and dam construction the most frequent suspects. There has been a recent increase in natural gas extraction — including fracking, or hydraulic fracturing, but other techniques as well — which produces a lot of wastewater. To get rid of it, the water is injected deep into the ground. When wastewater works its way into dormant faults, the thinking goes, the water’s pressure nudges the ancient cracks. Pent-up tectonic stress releases and the ground shakes.

But for any given earthquake, it is virtually impossible to tell whether humans or nature triggered the quake. There are no known characteristics of a quake, not in magnitude nor in the shape of its seismic waves, that provide hints to its origins.

“It’s been a head-scratching period for scientists,” said Maria Beatrice Magnani, who studies earthquakes at Southern Methodist University in Dallas. Along with a team of researchers at the U.S. Geological Survey, Magnani, an author of a new report published Friday in the journal Science Advances, attempted to better identify what has been causing the rash of Texas quakes.

A cluster of earthquakes around a drilling project can, at best, suggest a relationship. “The main approach has been to correlate the location to where there has been human activity,” said Michael Blanpied, a USGS geophysicist and co-author of the new study.

Read the full story.

Tags Beatrice Magnani, Dedman College, Heather R. DeShon, Huffington Departhment of Earth Sciences, Matthew J. Hornbach

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SMU seismology research shows North Texas earthquakes occurring on “dead” faults

Post author By Margaret Allen
Post date November 30, 2017

Study by Beatrice Magnani, USGS and other SMU scientists shows recent seismicity in Fort Worth Basin occurred on faults not active for 300 million years

Recent earthquakes in the Fort Worth Basin — in the rural community of Venus and the Dallas suburb of Irving – occurred on faults that had not been active for at least 300 million years, according to research led by SMU seismologist Beatrice Magnani.

The research supports the assertion that recent North Texas earthquakes were induced, rather than natural – a conclusion entirely independent of previous analyses correlating seismicity to the timing of wastewater injection practices, but that corroborates those earlier findings.

The full study, “Discriminating between natural vs induced seismicity from long-term deformation history of intraplate faults,” was published online Nov. 24, 2017 by the journal Science Advances.

“To our knowledge this is the first study to discriminate natural and induced seismicity using classical structural geology analysis techniques,” said Magnani, associate professor of geophysics in SMU’s Huffington Department of Earth Sciences. Co-authors for the study include Michael L. Blanpied, associate coordinator of the USGS Earthquake Hazard program, and SMU seismologists Heather DeShon and Matthew Hornbach.

The results were drawn from analyzing the history of fault slip (displacement) over the lifetime of the faults. The authors analyzed seismic reflection data, which allow “mapping” of the Earth’s subsurface from reflected, artificially generated seismic waves. Magnani’s team compared data from the North Texas area, where several swarms of felt earthquakes have been occurring since 2008, to data from the Midwestern U.S. region that experienced major earthquakes in 1811 and 1812 in the New Madrid seismic zone.

Frequent small earthquakes are still recorded in the New Madrid seismic zone, which is believed to hold the potential for larger earthquakes in the future.

“These North Texas faults are nothing like the ones in the New Madrid Zone – the faults in the Fort Worth Basin are dead,” Magnani said. “The most likely explanation for them to be active today is because they are being anthropogenically induced to move.”

In the New Madrid seismic zone, the team found that motion along the faults that are currently active has been occurring over many millions of years. This has resulted in fault displacements that grow with increasing age of sedimentary formations.

In the Fort Worth Basin, along faults that are currently seismically active, there is no evidence of prior motion over the past 300 million years.

“The study’s findings suggest that the recent Fort Worth Basin earthquakes, which involve swarms of activity on several faults in the region, have been induced by human activity,” said USGS scientist Blanpied.

The findings further suggest that these North Texas earthquakes are not simply happening somewhat sooner than they would have otherwise on faults continually active over long time periods. Instead, Blanpied said, the study indicates reactivation of long-dormant faults as a consequence of waste fluid injection.

Seismic reflection profiles in the Venus region used for this study were provided by the U.S. Geological Survey Earthquake Hazards Program.

Seismic reflection profiles for the Irving area are proprietary. Magnani and another team of scientists collected seismic reflection data used for this research during a 2008-2011 project in the northern Mississippi embayment, home to the New Madrid seismic zone. — Kim Cobb, SMU

Tags Beatrice Magnani, Dedman College, Heather R. DeShon, Matthew J. Hornbach, Roy M. Huffington Department of Earth Sciences

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Commerce Department selects scientific team to conduct independent abundance estimate of red snapper in Gulf of Mexico

Post author By Margaret Allen
Post date November 29, 2017

The initiative addresses one of the most pressing issues currently facing U.S. Gulf of Mexico fisheries management, as the iconic red snapper supports one of the most economically valuable finfish fisheries in the Gulf.

An expert team of university and government scientists will determine the abundance of red snapper in the U.S. waters of the Gulf of Mexico, as availability of the fish is vital to the region’s economy.

“Red snapper have great economic value to all the gulf states,” said SMU statistician Lynne Stokes, a member of the team. “Maintaining the health of the species is vitally important, so it’s necessary to ensure species are fished at the right level.”

As an expert in surveys, polls and sampling, Stokes’ role in the project is to help design ways to sample the vast expanse of the gulf efficiently so that good estimates of abundance can be produced.

“The gulf is very diverse, and different sampling methods are needed for different habitats, which makes the sample design problem interesting,” said Stokes, a professor in the SMU Department of Statistical Science. “The cheapest way to collect data about the health of a marine fish species is by asking a sample of anglers about their catch. However, if fish are present in places where anglers are not, other methods are needed. There is some uncertainty about all the places red snapper exist in the gulf, so it is not known if catch-based methods provide accurate estimates of abundance.”

The project will obtain angler-independent data about red snapper abundance by sampling their potential habitat, Stokes said. The team will collect data on red snapper numbers by direct observation of a sample of transects on the sea bottom and structures on the sea floor, using remotely controlled video cameras. Stokes will help determine how extensive the observation must be.

The team of scientists was selected by an expert review panel convened by the Mississippi-Alabama Sea Grant Consortium to conduct the independent study.

“American communities across the Gulf of Mexico depend on their access to, as well as the long term sustainability of, red snapper,” said U.S. Secretary of Commerce Wilbur Ross. “I look forward to the insights this project will provide as we study and manage this valuable resource.”

Recreational anglers and commercial fishers will play a key role
The research team, made up of 21 scientists from 12 institutions of higher learning, a state agency and a federal agency, was awarded $9.5 million in federal funds for the project through a competitive research grant process. With matching funds from the universities, the project will total $12 million.

“We’ve assembled some of the best red snapper scientists around for this study,” said Greg Stunz, the project leader and a professor at the Harte Research Institute for Gulf of Mexico Studies at Texas A&M University – Corpus Christi. “The team members assembled through this process are ready to address this challenging research question. There are lots of constituents who want an independent abundance estimate that will be anxiously awaiting our findings.”

Recreational anglers and commercial fishers will be invited to play a key role in collecting data by tagging fish, reporting tags and working directly with scientists onboard their vessels.

“The local knowledge fishermen bring to this process is very valuable and meaningfully informs our study,” Stunz said.

Some stakeholder groups have expressed concerns that there are more red snapper in the Gulf than currently accounted for in the stock assessment. The team of scientists on this project will spend two years studying the issue.

In 2016, Congress directed the National Sea Grant College Program and NOAA Fisheries to fund independent red snapper data collections, surveys and assessments, including the use of tagging and advanced sampling technologies. Sea Grant and NOAA Fisheries worked collaboratively to transfer federal funds to Mississippi-Alabama Sea Grant to administer the competitive research grant process and manage this independent abundance estimate.

“Today’s announcement is welcome news for all red snapper anglers in the Gulf of Mexico,” said Sen. Richard Shelby of Alabama. “As Chairman of the U.S. Senate Appropriations Subcommittee on Commerce, Justice, Science and Related Agencies, I was proud to author and secure federal funding to address the need for better data, which is a fundamental issue plaguing the fishery. The management of red snapper must be grounded in sound science if we want to provide fair access and more days on the water for our anglers. It is my hope that these independent scientists will be able to accurately determine the abundance of red snapper in the Gulf of Mexico once and for all.”

Project team will determine abundance and distribution of red snapper
The research will be driven largely by university-based scientists with partners from state and federal agencies, Stunz said.

The funding will allow the scientists to carry out an abundance estimate using multiple sampling methods with a focus on advanced technologies and tagging for various habitat types, he said.

“I’m pleased to see that the independent estimate is moving forward and including the expertise of recreational fishermen,” said Rep. John Culberson of Texas. “I will continue to work with Texas fishermen and NOAA to address the inadequate access to red snapper.”

The project team will determine abundance and distribution of red snapper on artificial, natural and unknown bottom habitat across the northern Gulf of Mexico.

As a statistician chosen for the team, SMU’s Stokes is also an expert in non-sampling survey errors, such as errors by interviewers and respondents. She recently conducted research on evaluating the accuracy of contest judges and on improving estimates of marine fishery yields by the National Oceanic and Atmospheric Administration.

Stokes also contributes to the National Assessment of Educational Progress, or “Nation’s Report Card,” examining the way schools and students are selected for the large study.

Besides SMU, others on the team include Texas A&M University, University of Florida, University of South Alabama, Louisiana State University, Florida International University, NOAA Fisheries, Auburn University, Mississippi State University, Louisiana Department of Wildlife and Fisheries, College of William and Mary, University of Southern Mississippi, and the University of South Florida. — Mississippi-Alabama Sea Grant and Southern Methodist University

Tags Dedman College, Lynne Stokes, SMU Department of Statistical Science

Earth & Climate Fossils & Ruins Plants & Animals Student researchers Subfeature

Prehistoric puzzle settled: carbon dioxide link to global warming 22 million years ago

Post author By Margaret Allen
Post date November 14, 2017

The modern link between high carbon dioxide levels and climate change didn’t appear to hold true for a time interval about 22 million years ago; but now a new study has found the link does indeed exist.

Fossil leaves from Africa have resolved a prehistoric climate puzzle — and also confirm the link between carbon dioxide in the atmosphere and global warming.

Research until now has produced a variety of results and conflicting data that have cast doubt on the link between high carbon dioxide levels and climate change for a time interval about 22 million years ago.

But a new study has found the link does indeed exist for that prehistoric time period, say researchers at Southern Methodist University, Dallas.

The finding will help scientists understand how recent and future increases in the concentration of atmospheric carbon dioxide may impact the future of our planet, say the SMU researchers.

The discovery comes from new biochemical analyses of fossil leaves from plants that grew on Earth 27 million years ago and 22 million years ago, said geologist Tekie Tesfamichael, lead scientist on the research.

The new analyses confirm research about modern climate — that global temperatures rise and fall with increases and decreases in carbon dioxide in our atmosphere — but in this case even in prehistoric times, according to the SMU-led international research team.

Carbon dioxide is a gas that is normally present in the Earth’s atmosphere, even millions of years ago. It’s dubbed a greenhouse gas because greater concentrations cause the overall temperature of Earth’s atmosphere to rise, as happens in a greenhouse with lots of sunlight.

Recently greenhouse gas increases have caused global warming, which is melting glaciers, sparking extreme weather variability and causing sea levels to rise.

The new SMU discovery that carbon dioxide behaved in the same manner millions of years ago that it does today has significant implications for the future. The finding suggests the pairing of carbon dioxide and global warming that is seen today also holds true for the future if carbon dioxide levels continue to rise as they have been, said Tesfamichael.

“The more we understand about the relationship between atmospheric carbon dioxide concentrations and global temperature in the past, the more we can plan for changes ahead,” said Tesfamichael, an SMU postdoctoral fellow in Earth Sciences.

“Previous work reported a variety of results and conflicting data about carbon dioxide concentrations at the two intervals of time that we studied,” he said. “But tighter control on the age of our fossils helped us to address whether or not atmospheric carbon dioxide concentration corresponded to warming — which itself is independently well-documented in geochemical studies of marine fossils in ocean sediments.”

The researchers reported their findings in Geology, the scientific journal of the Geological Society of America. The article is “Settling the issue of ‘decoupling’ between atmospheric carbon dioxide and global temperature: [CO₂]_atm reconstructions across the warming Paleogene-Neogene divide.”

Co-authors from the Roy M. Huffington Department of Earth Sciences in Dedman College are professors Bonnie Jacobs, an expert in paleobotany and paleoclimate, and Neil J. Tabor, an expert in sedimentology and sedimentary geochemistry.

Other co-authors are Lauren Michel, Tennessee Technological University; Ellen Currano, University of Wyoming; Mulugeta Feseha, Addis Ababa University; Richard Barclay, Smithsonian Institution; John Kappelman, University of Texas; and Mark Schmitz, Boise State University.

Discovery of rare, well-preserved fossil leaves enables finding
The findings were possible thanks to the rare discovery of two sites with extraordinarily well-preserved fossil leaves of flowering plants from the Ethiopian Highlands of eastern Africa.

Such well-preserved fossil leaves are a rarity, Tesfamichael said.

“Finding two sites with great preservation in the same geographic region from two important time intervals was very fortunate, as this enabled us to address the question we had about the relationship between atmospheric carbon dioxide concentration and global temperatures,” he said.

Scientists know that variations in the concentration of atmospheric carbon dioxide affect carbon fixation in leaves during photosynthesis. This causes leaves to develop anatomical and physiological changes such as the frequency and size of stomata — the pores on the surface of a leaf through which carbon passes.

Scientists can measure those attributes, among others, in fossil leaves, so that leaf fossils can be used as proxies for Earth’s atmospheric carbon dioxide history.

The sites producing the leaves for the SMU study were discovered separately in years past, but major fossil collections were produced through field work coordinated by the SMU research team and their co-authors, who have been collaborating on this project for several years.

The work has had funding from the National Science Foundation, The National Geographic Committee for Research and Exploration, the SMU Ford Fellowship Program, SMU Research Council, the Institute for the Study of Earth and Man, and the Dallas Paleontological Society Frank Crane Scholarship.

The fossils are housed permanently in the collections at the National Museum of Ethiopia in Addis Ababa. Institutional and governmental support came from the National Museum of Ethiopia, the Authority for Research and Conservation of Cultural Heritage, and Addis Ababa University.

Previous studies firmly established a temperature difference
One of the sites dates to the late Oligocene Epoch, and the other to the early Miocene.

Previous studies that measured ocean temperatures from around the world for the two intervals have firmly established a temperature difference on Earth between the two times, with one much warmer than the other. So the SMU study sought to measure the levels of carbon dioxide for the two time periods.

For the SMU analyses, fossil leaves of a single species were collected from the 27 million-year-old late Oligocene site. The leaves had been deposited during prehistoric times in the area of Chilga in northwest Ethiopia most likely at a river bank. The Earth’s climate during the late Oligocene may have been somewhat warmer than today, although glaciers were forming on Antarctica. The SMU study found carbon dioxide levels, on average, around 390 parts per million, about what it is on Earth today.

Fossil leaves of the 22 million-year-old species from the early Miocene were collected from ancient lake deposits, now a rock called shale, from the modern-day Mush Valley in central Ethiopia. The early Miocene climate at that time was warmer than the late Oligocene and likewise the SMU study found higher carbon dioxide levels. Atmospheric carbon dioxide was about 870 parts per million, double what it is on Earth today.

The SMU study confirmed a relationship between carbon dioxide and temperature during the late Oligocene and early Miocene.

Paleoclimate data can help predict our planet’s future climate
While carbon dioxide isn’t the only factor affecting Earth’s climate or global mean temperature, it is widely considered by scientists among the most significant. Much is known about climate change and global warming, but questions still remain.

“One of those is ‘What’s the sensitivity of the Earth’s temperature to carbon dioxide concentration? Is it very sensitive? Is it not so sensitive?’ Estimating temperature and carbon dioxide concentrations for times in the past can help find the answer to that question,” Jacobs said. “There’s a lot of work on paleoclimate in general, but not as much on the relationship between carbon dioxide and temperature.”

The finding is an important one.

“The amount of temperature change during this interval is approximately within the range of the temperature change that is estimated from climate models for our next century given a doubling of carbon dioxide concentration since the industrial revolution,” Jacobs said.

With the new model reaffirming the prehistoric relationship, scientists can look now at related questions, said climate change scientist Lauren Michel, who worked on the study as a post-doctoral researcher at SMU.

“Answering questions about the rate of change and which factors changed first, for example, will ultimately give a clearer picture of the Earth’s climate change patterns,” Michel said. “I think it is valuable to understand the relationship of greenhouse gases and climate factors represented in the rock record so we can have a better idea of what we can expect in the future and how we can prepare for that.”

SMU study confirms relationship that previous methods overlooked
Previous studies found little to no correlation between temperature and carbon dioxide for the late Oligocene and early Miocene. That has puzzled paleoclimate researchers for at least a decade.

“We have a good test-case scenario with these well-preserved plants from both time slices, where we know one time slice, with higher levels of carbon dioxide, was a warmer climate globally than the other,” Tesfamichael said.

“It’s been a puzzle as to why the previous methods found no relationship, or an inverse correlation,” he said. “We think it’s for lack of the well-dated proxy — such as our fossil leaves from two precise times in the same region — which deliver a reliable answer. Or, perhaps the models themselves needed improvement.”

Previous studies used methodologies that differed from the SMU study, although all methods (proxies) incorporate some aspects of what is known about living organisms and how they interact with atmospheric carbon dioxide.

Some studies rely on biochemical modeling of the relationship between single-celled marine fossils and atmospheric carbon dioxide, and others rely on the relationship between stomata and atmospheric carbon dioxide concentration observed in the living relatives of particular fossil plant species.

“Each method has its assumptions,” said Tesfamichael. “We will see if our results hold up with further studies of this time interval using the same methodology we used.” — Margaret Allen, SMU

Tags Bonnie F. Jacobs, Dedman College, Lauren Michel, Neil Tabor, Roy M. Huffington Department of Earth Sciences, Tekie Tesfamichael

Culture, Society & Family Earth & Climate Energy & Matter Events Researcher news SMU In The News Videos

The CW33: Dark Matter Day rocks SMU’s campus

Post author By Margaret Allen
Post date November 2, 2017

The CW33 TV visited SMU on Halloween to get a glimpse of International Dark Matter Day in action on the SMU campus.

The CW33 TV stopped at the SMU campus during the early morning hours of Halloween to interview SMU physics professor Jodi Cooley about the capers afoot in celebration of International Dark Matter Day.

The SMU Department of Physics in Dedman College of Humanities and Sciences hosted the Oct. 31, 2017 Dark Matter Day celebration for students, faculty, staff and Dallas-area residents.

As part of the festivities, there were speaking events by scientists in the field of dark matter, including dark matter expert Cooley, to explain the elusive particles that scientists refer to as dark matter.

Then throughout Halloween day, the public was invited to test their skills at finding dark matter — in this case, a series of 26 rocks bearing educational messages related to dark matter, which the Society of Physics Students had painted and hidden around the campus. Lucky finders traded them for prizes from the Physics Department.

“In the spirit of science being a pursuit open to all, we are excited to welcome all members of the SMU family to become dark matter hunters for a day,” said Cooley, whose research is focused on the scientific challenge of detecting dark matter. “Explore your campus in the search for dark matter rocks, just as physicists are exploring the cosmos in the hunt for the nature of dark matter itself.”

Watch the full news segment.

EXCERPT:

By Shardae Neal
The CW33
On Halloween (excuse us) “International Dark Matter Day,” SMU students hosted a public witch hunt to search for the unknown: dark matter.

“What we’re doing is hiding 26 rocks that we have with the help of our society of physic students,” explained SMU Physicist Jodi Cooley.

What exactly is dark matter?

“Think about all the stuff there is in the universe,” Cooley added. “What we can account for makes up only four to five percent of the universe. The rest of it is unknown. Turns out 26% of that unknown stuff is dark matter.”

Watch the full news segment.

Tags Dedman College, Jodi Cooley, SMU Department of Physics

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SMU Dark Matter Day celebration culminates in a dark matter rock hunt on Halloween

Post author By Margaret Allen
Post date October 23, 2017

“In the spirit of science being a pursuit open to all, we are excited to welcome all members of the SMU family to become dark matter hunters for a day.” — SMU physicist Jodi Cooley

This Halloween, people around the world will be celebrating the mysterious cosmic substance that permeates our universe: dark matter.

At SMU, the Department of Physics in Dedman College of Humanities and Sciences is hosting a Dark Matter Day celebration, and students, faculty, staff and DFW residents are invited to join in the educational fun with events open to the public.

To kick off the festivities, two speaking events by scientists in the field of dark matter will familiarize participants with the elusive particles that scientists refer to as dark matter. The first talk is oriented toward the general public, while the second is more technical and will appeal to people familiar with one of the STEM areas of science, technology, engineering or mathematics, particularly physics and astrophysics.

Then throughout Halloween day, everyone is invited to test their skills at finding dark matter — in this case, a series of rocks bearing educational messages related to dark matter, which the Society of Physics Students has painted and then hidden around the campus.

Anyone lucky enough to find one of the 26 rocks can present it at the Physics Department office to receive a prize, says SMU physics professor Jodi Cooley, whose research is focused on the scientific challenge of detecting dark matter.

“In the spirit of science being a pursuit open to all, we are excited to welcome all members of the SMU family to become dark matter hunters for a day,” Cooley said. “Explore your campus in the search for dark matter rocks, just as physicists are exploring the cosmos in the hunt for the nature of dark matter itself.”

Anyone who discovers a dark matter rock on the SMU campus is encouraged to grab their phone and snap a selfie with their rock. Tweet and tag your selfie #SMUDarkMatter so that @SMU, @SMUResearch and @SMUPhysics can retweet photos of the lucky finders.

As SMU’s resident dark matter scientist, Cooley is part of the 100-person international SuperCDMS SNOLAB experiment, which uses ultra pure materials and highly sensitive custom-built detectors to listen for the passage of dark matter.

SuperCDMS, an acronym for Super Cryogenic Dark Matter Search, resides at SNOLAB, an existing underground science laboratory in Ontario, Canada. Located deep underground, SNOLAB allows scientists to use the earth as a shield to block out particles that resemble dark matter, making it easier to see the real thing.

The SuperCDMS SNOLAB experiment, expected to be operational in 2020, has been designed to go deeper below the surface of the earth than earlier generations of the research.

“Dark matter experiments have been a smashing success — they’ve progressed farther than anyone anticipated. The SuperCDMS SNOLAB experiment is quite unique,” Cooley said. “It will allow us to probe models that predict dark matter with the tiniest masses.”

For more on Cooley’s research, go to “Hunt for dark matter takes physicists deep below earth’s surface, where WIMPS can’t hide.“ — Margaret Allen, SMU

Dark Matter Day events at SMU:

Sunday, Oct. 29, 4 p.m., McCord Auditorium — Maruša Bradač, Associate Professor at the University of California at Davis, will give a public lecture on dark matter. A reception will follow the lecture from 5 p.m. to 6 p.m. in the Dallas Hall Rotunda with beverages and light snacks. This event is free and open to the public, and is designed to be open to the widest possible audience.

Monday, Oct. 30, 4 p.m., Fondren Science Building, Room 158 — SMU Associate Professor Jodi Cooley will present a seminar on the SuperCDMS direct-detection dark matter search experiment. This event is part of the Physics Department Speaker Series. While this event is open to the public, it will be a more technical talk and may appeal more to an audience interested in the STEM areas of science, technology, engineering and mathematics, especially physics and astrophysics.
Tuesday, Oct. 31, 9 a.m. – 4 p.m., SMU Main Campus, Dark Matter Rock Hunt — The SMU Department of Physics has hidden “dark matter rocks” all across the SMU main campus. If you discover one of the dark matter rocks, bring it to the main office of the Physics Department, Fondren Science Building, Room 102, and get a special prize. All SMU students, faculty, staff and community members are welcome to join in the search.

Tags Dedman College, Jodi Cooley, SMU Department of Physics

Earth & Climate Fossils & Ruins Plants & Animals Researcher news SMU In The News

Australian Geographic: Secrets of leaf size revealed

Post author By Margaret Allen
Post date September 6, 2017

New findings reveal the real reasons behind varying leaf sizes.

Australian Geographic has covered the research of SMU paleobotanist Bonnie F. Jacobs, a professor in SMU’s Roy M. Huffington Department of Earth Sciences.

Working with a global team of researchers, Jacobs and her colleagues cracked the mystery of leaf size. The research was published Sept. 1, 2017 as a cover story in Science.

The researchers from Australia, the U.K., Canada, Argentina, the United States, Estonia, Spain and China analyzed leaves from more than 7,600 species of plants over the past 20 years, then pooled and analyzed the data with new theory to create a series of equations that can predict the maximum viable leaf size anywhere in the world based on the risk of daytime overheating and night-time freezing.

The researchers will use these findings to create more accurate vegetation models. This will be used by governments to predict how vegetation will change locally and globally under climate change, and to plan for adaptation.

Jacobs contributed an extensive leaf database — research that was funded by a National Science Foundation grant. She analyzed the leaf characteristics of 880 species of modern tropical African plants, which occurred in various combinations among 30 plant communities. Jacobs measured leaves of the plant specimens at the Missouri Botanical Garden Herbarium, one of the largest archives of pressed dried plant specimens from around the world.

Jacobs is one of a handful of the world’s experts on the fossil plants of ancient Africa. As part of a team of paleontologists working there, she hunts plant and animal fossils in Ethiopia’s prolific Mush Valley, as well as elsewhere in Africa.

Read the full story.

EXCERPT:

By Karl Gruber
Australian Geographic
You may have learnt at school that leaf size depends on water availability and that they are meant to help plants avoid overheating. But a new study that looked at leaf sizes around the world found that, rather than water availability, it all boils down to temperature, both high and low.

Leaf sizes can vary by as much as 100,000 fold, with some leaves having an area of just 1 mm2 while other can have an area of up to 1 m2. But what is driving these big differences?

“The conventional explanation was that water availability and overheating were the two major limits to leaf size. But the data didn’t fit,” says Ian. “For example the tropics are both wet and hot, and leaves in cooler parts of the world are unlikely to overheat,” explained Ian Wright, from Macquarie University, who led the new study.

A key finding from the study is that for plants all around the world the main factors limiting leaf size are the risk of frosting in cold nights, which can damage leaves, and the risk of overheating during the day.

“Latitude explains 28% of variation leaf size, globally. Warm wet regions are characterised by large-leaved species, warm dry regions and cold regions by smaller-leaved species. These patterns can all be understood in relation to the energy inputs and outputs to leaves, but only if you consider both the daytime (overheating) and night-time (freezing) risks,” Wright says.

Read the full story.

Tags Bonnie F. Jacobs, Dedman College, Roy M. Huffington Department of Earth Sciences

Earth & Climate Fossils & Ruins Plants & Animals Researcher news SMU In The News

BBC: Clues to why leaves come in many sizes

Post author By Margaret Allen
Post date September 5, 2017

The huge variety of leaves in the plant kingdom has long been a source of wonder and fascination.

BBC News has covered the research of SMU paleobotanist Bonnie F. Jacobs, a professor in SMU’s Roy M. Huffington Department of Earth Sciences.

Working with a global team of researchers, Jacobs and her colleagues cracked the mystery of leaf size. The research was published Sept. 1, 2017 as a cover story in Science.

Read the full story.

EXCERPT:

By Helen Briggs
BBC News
The leaves of a banana plant, for instance, are about a million times bigger than the leaves of heather.

The conventional wisdom is that leaf size is limited by the balance between how much water is available to a plant and the risk of overheating.

However, a study of more than 7,000 plant species around the world suggests the answer may be more complex.

“A banana leaf is able to be so huge because bananas naturally grow in places that are very hot and very wet,” said Ian Wright of Macquarie University in Sydney, Australia.
“Our work shows that in fact that if there’s enough water in the soil then there’s almost no limit to how large leaves can be.”

He says this is only part of the puzzle of leaf size.

“The other part is about the tendency for larger leaves to freeze at night,” Dr Wright explained.

“And, you put these two ingredients together — the risk of freezing and the risk of overheating — and this helps understand the pattern of leaf sizes you see across the entire world.”

There are hundreds of thousands of plant species on the planet, from tiny alpine plants to massive jungle palms.

Their leaves vary in area from less than 1 square millimetre to greater than 1 square metre.

Large-leaved plants predominate in tropical jungle — something that was noted as early as the 19th Century. Meanwhile, small-leaved plants thrive in arid deserts and at high latitudes.

Some decades ago, scientists realised that variability in leaf size was related to water and temperature. They proposed that the limit to leaf size was set by the risk of overheating.

Thus, when rainfall is high, plants can get away with having larger leaves.
The new research, published in the journal Science, suggests this idea applies only in certain regions of the globe.

“There were some pieces in this puzzle that were clearly missing,” Dr. Wright told BBC News.

Read the full story.

Tags Bonnie F. Jacobs, Dedman College, Roy M. Huffington Department of Earth Sciences

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The mystery of leaf size solved by global team of scientists

Post author By Margaret Allen
Post date September 5, 2017
No Comments on The mystery of leaf size solved by global team of scientists

A global team of researchers, including SMU paleobotanist Bonnie Jacobs, have cracked the mystery of leaf size. The research was published Sept. 1, 2017 as a cover story in Science.

SMU paleobotanist Bonnie F. Jacobs has contributed research to a major new study that provides scientists with a new tool for understanding both ancient and future climate by looking at the size of plant leaves.

Why is a banana leaf a million times bigger than a common heather leaf? Why are leaves generally much larger in tropical jungles than in temperate forests and deserts? The textbooks say it’s a balance between water availability and overheating.

But it’s not that simple, the researchers found.

The study, published in the Sept. 1, 2017 issue of Science, was led by Associate Professor Ian Wright from Macquarie University, Australia. The study’s findings reveal that in much of the world the key factor limiting the size of a plant’s leaves is the temperature at night and the risk of frost damage to leaves.

Jacobs said the implications of the study are significant for enabling scientists to either predict modern leaf size in the distant future, or to understand the climate for a locality as it may have been in the past.

“This research provides scientists with another tool for predicting future changes in vegetation, given climate change, and for describing ancient climate given fossil leaves,” said Jacobs, a professor in SMU’s Roy M. Huffington Department of Earth Sciences in the Dedman College of Humanities and Sciences.

“Now we can reliably use this as another way to look at future climate models for a specific location and predict the size of plant leaves,” she said. “Or, if we’re trying to understand what the climate was for a prehistoric site tens of millions of years ago, we can look at the plant fossils discovered in that location and describe what the climate most likely was at that time.”

Wright, Jacobs and 15 colleagues from Australia, the U.K., Canada, Argentina, the United States, Estonia, Spain and China analyzed leaves from more than 7,600 species, then pooled and analyzed the data with new theory to create a series of equations that can predict the maximum viable leaf size anywhere in the world based on the risk of daytime overheating and night-time freezing.

Big data solves century-old conundrum
The iconic paintings of Henri Rousseau illustrate that when we think of steamy tropics we expect large leaves. But for scientists it’s been a century-old conundrum: why does leaf size vary with latitude – from very small near the poles to massive leaves in the tropics?

“The conventional explanation was that water availability and overheating were the two major limits to leaf size. But the data didn’t fit,” says Wright. “For example the tropics are both wet and hot, and leaves in cooler parts of the world are unlikely to overheat.”

“Our team worked both ends of the problem – observation and theory,” he says. “We used big data – measurements made on tens of thousands of leaves. By sampling across all continents, climate zones and plant types we were able to show that simple ‘rules’ seemingly operate across the world’s plant species, rules that were not apparent from previous, more limited analyses.”

Jacobs contributed an extensive leaf database she compiled about 20 years ago, funded by a National Science Foundation grant. She analyzed the leaf characteristics of 880 species of modern tropical African plants, which occurred in various combinations among 30 plant communities. Jacobs measured leaves of the plant specimens at the Missouri Botanical Garden Herbarium, one of the largest archives of pressed dried plant specimens from around the world.

She looked at all aspects of leaf shape and climate, ranging from seasonal and annual rainfall and temperature for each locale, as well as leaf shape, size, tip, base, among others. Using statistical analyses to plot the variables, she found the most prominent relationship between leaf shape and climate was that size increases with rainfall amount. Wet sites had species with larger leaves than dry sites.

Her Africa database was added to those of many other scientists who have compiled similar data for other localities around the world.

Threat of night time frost damage determines the size of a leaf
“Using our knowledge of plant function and biophysics we developed a fresh take on ‘leaf energy balance’ theory, and compared our predictions to observed leaf sizes,” Wright says.

“The most surprising result was that over much of the world the maximum size of leaves is set not by the risk of overheating, but rather by the risk of damaging frost at night. Larger leaves have thicker, insulating ‘boundary layers’ of still air that slows their ability to draw heat from their surroundings – heat that is needed to compensate for longwave energy lost to the night-time sky,” says co-author Colin Prentice from Imperial College London, who co-ordinated the mathematical modelling effort.

“International collaborations are making ecology into a predictive science at global scale,” says Emeritus Professor Mark Westoby. “At Macquarie University we’re proud to have led this networking over the past 20 years.” — Margaret Allen, SMU, and Macquarie University

By Ian Wright
Macquarie University
As a plant ecologist, I try to understand variation in plant traits (the physical, chemical and physiological properties of their tissues) and how this variation affects plant function in different ecosystems.

For this study I worked with 16 colleagues from Australia, the UK, Canada, Argentina, the US, Estonia, Spain and China to analyse leaves from more than 7,600 species. We then teamed the data with new theory to create a model that can predict the maximum viable leaf size anywhere in the world, based on the dual risks of daytime overheating and night-time freezing.

These findings will be used to improve global vegetation models, which are used to predict how vegetation will change under climate change, and also to better understand past climates from leaf fossils.

From giants to dwarfs
The world’s plant species vary enormously in the typical size of their leaves; from 1 square millimetre in desert species such as common eutaxia (Eutaxia microphylla), or in common heather (Calluna vulgaris) in Europe, to as much as 1 square metre in tropical species like Musa textilis, the Filipino banana tree.

But what is the physiological or ecological significance of all this variation in leaf size? How does it affect the way that plants “do business”, using leaves as protein-rich factories that trade water (transpiration) for carbon (photosynthesis), powered by energy from the sun?

More than a century ago, early plant ecologists such as Eugenius Warming argued that it was the high rainfall in the tropics that allowed large-leaved species to flourish there.

In the 1960s and ‘70s physicists and physiologists tackled the problem, showing that in mid-summer large leaves are more prone to overheating, requiring higher rates of “transpirational cooling” (a process akin to sweating) to avoid damage. This explained why many desert species have small leaves, and why species growing in cool, shaded understoreys (below the tree canopy) can have large leaves.

But still there were missing pieces to this puzzle. For example, the tropics are both wet and hot, and these theories predicted disadvantages for large-leafed species in hot regions. And, in any case, overheating must surely be unlikely for leaves in many cooler parts of the world.

Our research aimed to find these missing pieces. By collecting samples from all continents, climate zones and plant types, our team found simple “rules” that appear to apply to all of the world’s plant species – rules that were not apparent from previous, more limited analyses.

We found the key factors are day and night temperatures, rainfall and solar radiation (largely determined by distance from the Equator and the amount of cloud cover). The interaction of these factors means that in hot and sunny regions that are also very dry, most species have small leaves, but in hot or sunny regions that receive high rainfall, many species have large leaves. Finally, in very cold regions (e.g. at high elevation, or at high northern latitudes), most species have small leaves.

But the most surprising results emerged from teaming the new theory for leaf size, leaf temperature and water use with the global data analyses, to investigate what sets the maximum size of leaves possible at any point on the globe.

Read the author’s full essay

Tags Bonnie F. Jacobs, Dedman College, Roy M. Huffington Department of Earth Sciences

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A Total Eclipse of the First Day of School

Post author By Margaret Allen
Post date August 23, 2017

Hundreds of students, faculty and townspeople gathered in the rotunda of Dallas Hall on Monday, Aug. 21 to view a projection of the Great American Solar Eclipse at a viewing hosted by Dedman College and the SMU Physics Department. (Jeff McWhorter/SMU)

Dedman College, SMU Physics Department host Great American Solar Eclipse 2017 viewing

Thousands of students, faculty and townspeople showed up to campus Monday, Aug. 21 to observe the Great American Solar Eclipse at a viewing hosted by Dedman College of Humanities and Sciences and the SMU Department of Physics.

The festive event coincided with the kick-off of SMU’s Fall Semester and included Solar Eclipse Cookies served while viewing the rare astronomical phenomenon.

The eclipse reached its peak at 1:09 p.m. in Dallas at more than 75% of totality.

“What a great first day of the semester and terrific event to bring everyone together with the help of Dedman College scientists,” said Dedman Dean Thomas DiPiero. “And the eclipse cookies weren’t bad, either.”

Physics faculty provided indirect methods for observing the eclipse, including a telescope with a viewing cone on the steps of historic Dallas Hall, a projection of the eclipse onto a screen into Dallas Hall, and a variety of homemade hand-held devices.

Outside on the steps of Dallas Hall, Associate Professor Stephen Sekula manned his home-built viewing tunnel attached to a telescope for people to indirectly view the eclipse.

“I was overwhelmed by the incredible response of the students, faculty and community,” Sekula said. “The people who flocked to Dallas Hall were energized and engaged. It moved me that they were so interested in — and, in some cases, had their perspective on the universe altered by — a partial eclipse of the sun by the moon.”

A team of Physics Department faculty assembled components to use a mirror to project the eclipse from a telescope on the steps of Dallas Hall into the rotunda onto a screen hanging from the second-floor balcony.

Adjunct Professor John Cotton built the mount for the mirror — with a spare, just in case — and Professor and Department Chairman Ryszard Stroynowski and Sekula arranged the tripod setup and tested the equipment.

Stroynowski also projected an illustration of the Earth, the moon and the sun onto the wall of the rotunda to help people visualize movement and location of those cosmic bodies during the solar eclipse.

Professor Fred Olness handed out cardboard projectors and showed people how to use them to indirectly view the eclipse.

“The turn-out was fantastic,” Olness said. “Many families with children participated, and we distributed cardboard with pinholes so they could project the eclipse onto the sidewalk. It was rewarding that they were enthused by the science.”

Stroynowski, Sekula and others at the viewing event were interviewed by CBS 11 TV journalist Robert Flagg.

Physics Professor Thomas Coan and Guillermo Vasquez, SMU Linux and research computing support specialist, put together a sequence of photos they took during the day from Fondren Science Building.

“The experience of bringing faculty, students and even some out-of-campus community members together by sharing goggles, cameras, and now pictures of one of the great natural events, was extremely gratifying,” Vasquez said.

Sekula said the enthusiastic response from the public is driving plans to prepare for the next event of this kind.

“I’m really excited to share with SMU and Dallas in a total eclipse of the sun on April 8, 2024,” he said.

Tags David Meltzer, Dedman College, Fredrick Olness, Guillermo Vasquez, Ryszard Stroynowski, SMU Department of Physics, Stephen J. Sekula, Thomas DiPiero, Thomas E. Coan

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Texas Tribune: The Q&A — Dr. Diego Román, Simmons School

Post author By Margaret Allen
Post date August 20, 2017

In this week’s Q&A, The Texas Tribune interviews Diego Román, assistant professor of teaching and learning at Southern Methodist University.

Texas Tribune reporter Cassandra Pollock interviewed SMU education expert Diego Román in the Annette Caldwell Simmons School of Education and Human Development for a Q&A about how middle school science textbooks frame climate change as an opinion rather than scientific fact.

Román is co-author of a 2015 study of California 6th grade science textbooks and how they present global warming.

Studies estimate that only 3 percent of scientists who are experts in climate analysis disagree about the role of humans in the causes of climate change. And the most recent report from the Intergovernmental Panel on Climate Change — the evidence of 600 climate researchers in 32 countries reporting changes to Earth’s atmosphere, ice and seas — in 2013 stated “human influence on the climate system is clear.”

Yet only 54 percent of American teens believe climate change is happening, 43 percent don’t believe it’s caused by humans, and 57 percent aren’t concerned about it.

The new study measured how four sixth-grade science textbooks adopted for use in California frame the subject of global warming. Sixth grade is the first time California state standards indicate students will encounter climate change in their formal science curriculum.

“We found that climate change is presented as a controversial debate stemming from differing opinions,” said Román, an assistant professor in the Department of Teaching and Learning. “Climate skeptics and climate deniers are given equal time and treated with equal weight as scientists and scientific facts — even though scientists who refute global warming total a miniscule number.”

The findings were reported in October 2015 at the 11th Conference of the European Science Education Research Association (ESERA), held in Helsinki, Finland.

The findings were also published in the Environmental Education Research journal in the article, “Textbooks of doubt: Using systemic functional analysis to explore the framing of climate change in middle-school science textbooks.”

The Texas Tribune article, “The Q&A: Diego Román,” published Aug. 17, 2017.

Read the full story.

EXCERPT:

By Cassandra Pollock
Texas Tribune
With each issue, Tasbo+Edu brings you an interview with experts on issues related to health care. Here is this week’s subject:

Diego Román is an assistant professor in teaching and learning at Southern Methodist University. He has recently researched how climate change is framed for middle school students in science textbooks.

Tasbo+Edu: Can you briefly explain your research findings?

Dr. Diego Román: The big picture of my research is that I look at the linguistic and social factors that impact language use in the science-education context and language development for English learners who are attending school in the U.S.

I am an applied linguist, and one of my research topics was the framing of climate change in middle school textbooks. In terms of the science textbooks and what we found in that specific study, the ones we investigated don’t reflect the way scientists discuss climate change in reports. While science reports resort to the certainty that climate change is happening, the textbooks that we looked at were very uncertain about defining that issue. We looked into seeing why that would be the case, particularly at how science is seen as very specific, objective and certain, but when we discuss climate change, we use a lot of qualifiers — “would,” “could” and “might.”

We’re arguing that this places the weight on the reader to decipher what that means. “Not all” could mean 90 percent, 55 percent or 10 percent, depending on who you’re talking to. So while textbooks are required to address certain topics — such as climate change — they’re not using specific language to help students and teachers have a better understanding and discussion around the issue.

I also look at how we use language — and I do that by using a framework called systemic functional linguistics. It argues that language is caused by the context of use, so the way we talk about science and the way we frame science topics when discussing them may be different than social studies. To explain a different type of knowledge, we connect ideas differently. For example, we emphasize the idea versus the people in science, but in social studies, we look at the people. To do that, we use language. So I look at how language is used in those purposes to convey knowledge and be effective. I try to understand the perspectives of the authors or the people. That’s a big picture description of my research.

Tasbo+Edu: What are the biggest challenges you see moving forward to try to modify the textbook system?

Román: It seems to be how research can impact, in this case, textbook development, and how to find things that applied linguists are doing when it relates to how language is used and if there’s a way to convey scientific knowledge — from a contextual perspective, but also from a linguistics perspective.

Read the full story.

Tags Annette Caldwell Simmons School of Education & Human Development, Diego Román

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Dallas Innovates: SMU, UTA Scientists To Help Unlock Mystery of Neutrinos

Post author By Margaret Allen
Post date July 31, 2017

A massive particle detector a mile underground is the key to unlocking the secrets of a beam of neutrinos that will be shot beneath the Earth from Chicago to South Dakota.

Reporter Lance Murray with Dallas Innovates reported on the research of biochemistry professors Thomas E. Coan in the SMU Department of Physics.

Coan is one of about 1,000 scientists around the world collaborating on DUNE — a massive particle detector being built a mile underground in South Dakota to unlock the mysteries of neutrino particles.

The research is funded by the by the U.S. Department of Energy’s Office of Science in conjunction with CERN and international partners from 30 countries.

SMU is one of more than 100 institutions from around the world building hardware for the massive international experiment that may change our understanding of the universe. Construction will take years and scientists expect to begin taking data in the middle of the next decade, said Coan.

The Long-Baseline Neutrino Facility (LBNF) will house the international Deep Underground Neutrino Experiment. When complete, LBNF/DUNE will be the largest experiment ever built in the United States to study the properties of the mysterious particles called neutrinos.

The Dallas Innovates article, “SMU, UTA Scientists To Help Unlock Mystery of Neutrinos,” published July 28, 2017.

Read the full story.

EXCERPT:

By Lance Murray
Dallas Innovates
Construction of a huge particle detector in South Dakota could lead to a change in how we understand the universe, and scientists from the University of Texas at Arlington and Southern Methodist University in Dallas will play roles in helping to unlock the mystery of neutrinos.

Ground was broken a mile underground recently at the Sanford Underground Research Facility at the Homestake Gold Mine in Lead, South Dakota for the Long-Baseline Neutrino Facility (LBNF) that will house the Deep Underground Neutrino Experiment (DUNE).

SMU physicist Thomas E. Coan, and UTA Physics professors Jonathan Asaadi and Jaehoon Yu will be among scientists from more than 100 institutions around the world who will be involved in the experiment.

DUNE will be constructed and operated at the mine site by a group of about 1,000 scientists and engineers from 30 nations.

The Homestake Mine was the location where neutrinos were discovered by Raymond Davis Jr. in 1962. It was the the largest and deepest gold mine in North America until its closure in 2002.

LBNF/DUNE will be the biggest experiment ever built in the U.S. to study the properties of neutrinos, one of the fundamental particles that make up the universe.

“DUNE is designed to investigate a broad swath of the properties of neutrinos, one of the universe’s most abundant but still mysterious electrically neutral particles,” Coan said in the release.

These puzzling particles are similar to electrons, but they have one huge difference — they don’t carry an electrical charge. Neutrinos come in three types: the electron neutrino, the muon, and the tau.

What is the experiment’s goal? Coan said it seeks to understand strange phenomena such as neutrinos changing identities in mid-flight — known as “oscillation” — as well as the behavioral differences between a neutrino and its anti-neutrino sibling.

“A crisp understanding of neutrinos holds promise for understanding why any matter survived annihilation with antimatter from the Big Bang to form the people, planets, and stars we see today,” Coan said in the release. “DUNE is also able to probe whether or not the humble proton, found in all atoms of the universe, is actually unstable and ultimately destined to eventually decay away. It even has sensitivity to understanding how stars explode into supernovae by studying the neutrinos that stream out from them during the explosion.”

Coan also is involved in another massive particle detector in northern Minnesota knows as NOvA, where he is a principal investigator.

Read the full story.

Tags Dedman College, SMU Department of Physics, Thomas E. Coan

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LiveScience: Newfound dino looks like creepy love child of a turkey and ostrich

Post author By Margaret Allen
Post date July 27, 2017
No Comments on LiveScience: Newfound dino looks like creepy love child of a turkey and ostrich

A new giant bird-like dinosaur discovered in China has been named for SMU paleontologist Louis L. Jacobs, Corythoraptor jacobsi, by the scientists who identified the new oviraptorid.

Live Science Senior Writer Laura Geggel covered the discovery of a new Cretaceous Period dinosaur from China that is named for paleontologist Louis L. Jacobs, an SMU professor in SMU’s Roy M. Huffington Department of Earth Sciences.

Jacobs mentored three of the authors on the article. First author on the paper was Junchang Lü, an SMU Ph.D. alum, with co-authors Yuong–Nam Lee and Yoshitsugu Kobayashi, both SMU Ph.D. alums.

The Live Science article, Newfound dino looks like creepy love child of a turkey and ostrich, published July 27, 2017. The dinosaur’s name, Corythoraptor jacobsi, translates to Jacobs’ helmeted thief.

The scientific article “High diversity of the Ganzhou Oviraptorid Fauna increased by a new “cassowary-like” crested species” was published July 27, 2017 in Nature’s online open access mega-journal of primary research Scientific Reports.

Jacobs in 2016 co-authored an analysis of the Cretaceous Period dinosaur Pawpawsaurus based on the first CT scans ever taken of the dinosaur’s skull.

He is president of SMU’s Institute for the Study of Earth and Man.

A world-renowned vertebrate paleontologist, Jacobs in 2012 was honored by the 7,200-member Science Teachers Association of Texas with their prestigious Skoog Cup for his significant contributions to advance quality science education. He joined SMU’s faculty in 1983.

Jacobs is the author of “Quest for the African Dinosaurs: Ancient Roots of the Modern World” (Villard Books and Johns Hopkins U. Press, 2000); “Lone Star Dinosaurs” (Texas A&M U. Press, 1999), which is the basis of a Texas dinosaur exhibit at the Fort Worth Museum of Science and History; “Cretaceous Airport” (ISEM, 1993); and more than 100 scientific papers and edited volumes.

Read the full story.

EXCERPT:

By Laura Geggel
Live Science
The newly identified oviraptorid dinosaur Corythoraptor jacobsi has a cassowary-like head crest, known as a casque.

A Chinese farmer has discovered the remains of a dinosaur that could have passed for the ostrich-like cassowary in its day, sporting the flightless bird’s head crest and long thunder thighs, indicating it could run quickly, just like its modern-day lookalike, a new study finds.

The newfound dinosaur’s 6-inch-tall (15 centimeters) head crest is uncannily similar to the cassowary’s headpiece, known as a casque, the researchers said. In fact, the crests have such similar shapes, the cassowary’s may provide clues about how the dinosaur used its crest more than 66 million years ago, they said.

The findings suggest that the dinosaur, which would have towered at 5.5 feet (1.6 meters), may have had a similar lifestyle to the modern cassowary bird (Casuarius unappendiculatus), which is native to Australia and New Guinea, the study’s lead researcher, Junchang Lü, a professor at the Institute of Geology, Chinese Academy of Geological Sciences, told Live Science in an email.

Researchers found the oviraptorid — a type of giant, bird-like dinosaur — in Ganzhou, a city in southern China, in 2013. The specimen was in remarkable shape: The paleontologists found an almost complete skeleton, including the skull and lower jaw, which helped them estimate that the creature was likely a young adult, or at least 8 years of age, when it died.

The long-necked and crested dinosaur lived from about 100 million to 66 million years ago during the late Cretaceous period, and likely used its clawed hands to hunt lizards and other small dinosaurs, Lü added.

The research team named the unique beast Corythoraptor jacobsi. Its genus name refers to the raptor’s cassowary-like crest, and the species name honors Louis Jacobs, a vertebrate paleontologist at Southern Methodist University who mentored three of the study’s researchers.

The researchers think the crest likely served the dinosaur in different ways, they said, including in display, communication and perhaps even as an indication of the dinosaur’s fitness during the mating season.

Read the full story.

Tags Dedman College, Junchang Lü, Louis L. Jacobs, Roy M. Huffington Department of Earth Sciences, Yoshitsugu Kobayashi, Yuong–Nam Lee

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Dallas Innovates: SMU Researchers Find West Virginia Geothermal Spots

Post author By Margaret Allen
Post date June 1, 2017
No Comments on Dallas Innovates: SMU Researchers Find West Virginia Geothermal Spots

The heated energy sources were discovered in the Mountain State by examining previously overlooked oil and gas data.

Reporter Amy Wolff Sorter with Dallas Innovates reported on the research of the SMU Geothermal Lab, which has identified in West Virginia what may be the largest geothermal hot spot in the United States.

The Dallas Innovates article, “SMU Researchers Find West Virginia Geothermal Spots,” published May 26, 2017.

Read the full story.

EXCERPT:

By Amy Wolff Sorter
Dallas Innovates
The state of West Virginia has been home to coal-driven energy for nearly two centuries. Now, there could be another energy source directly under the Mountain State’s surface discovered by researchers at Southern Methodist University in Dallas.

The researchers, examining previously overlooked oil and gas data, located several hot patches of earth, some as hot as 392 degrees Fahrenheit. These hot patches are situated roughly three miles under the state’s surface. In fact, scientists believe West Virginia could be sitting on the largest geothermal hot spot in the United States.

Geothermal patches overlooked in data
SMU’s Geothermal Lab Coordinator Maria Richards told the Exponent Telegram in Clarksburg, West Virginia that the hot patches were discovered by studying previously overlooked oil and gas data.

“We were aware that there were hot springs along the faults in West Virginia, and there was a basic understanding that there could be some sort of higher elevated areas, but we had never had the resources to be able to go back out and look at the deeper data until we had this project from Google that allowed us to bring in the oil and gas data,” she said.

The hot-water reservoirs were once considered too deep for inexpensive production.

However, “because of oil and gas drilling and some of the newer technologies in terms of drilling and pumping, some new innovative ways of developing systems, we can now go into places where we can inject water or a fluid that will then bring out that heat,” Richards said.

Geothermal’s appeal is that it is emission-free. It also has a smaller footprint, as energy is generated from underground wells.

Additionally, this particular renewable energy can overlap with other forms of energy, such as coal.

SMU’s Richards said that hot fluid can be used to dry coal, which, in turn, helps it burn more efficiently. The cleaner the coal burns, the less coal is required to produce electricity.

“Rather than having to burn a fossil fuel to generate electricity to create heat, the goal is to use the heat from the earth to create that heat automatically without having to generate electricity,” Richards said.

Read the full story.

Tags Dedman College, Maria Richards, Roy M. Huffington Department of Earth Sciences, SMU Geothermal Laboratory

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Study solves mystery of how plants use sunlight to tell time via cell protein signaling

Post author By Margaret Allen
Post date May 15, 2017

Discovery may someday allow farmers to grow crops in climates where they currently won’t grow and allows scientists to make a subtle, targeted mutation to a specific native plant protein

Findings of a new study solve a key mystery about the chemistry of how plants tell time so they can flower and metabolize nutrients.

The process — a subtle chemical event — takes place in the cells of every plant every second of every day.

The new understanding means farmers may someday grow crops under conditions or in climates where they currently can’t grow, said chemist Brian D. Zoltowski, Southern Methodist University, Dallas, who led the study.

“We now understand the chemistry allowing plants to maintain a natural 24-hour rhythm in sync with their environment. This allows us to tune the chemistry, like turning a dimmer switch up or down, to alter the organism’s ability to keep time,” Zoltowski said. “So we can either make the plant’s clock run faster, or make it run slower. By altering these subtle chemical events we might be able to rationally redesign a plant’s photochemistry to allow it to adapt to a new climate.”

Specifically, the researchers figured out the chemical nuts and bolts of how a chemical bond in the protein Zeitlupe forms and breaks in reaction to sunlight, and the rate at which it does so, to understand how proteins in a plant’s cells signal the plant when to bloom, metabolize, store energy and perform other functions.

Zoltowski’s team, with collaborators at the University of Washington and Ohio State University, have made plant strains with specific changes to the way they are able to respond to blue-light.

“With these plants we demonstrate that indeed we can tune how the organisms respond to their environment in an intelligible manner,” Zoltowski said.

Zoltowski and his colleagues made the discovery by mapping the crystal structure of a plant protein whose function is to measure the intensity of sunlight. The protein is able to translate light intensity to a bond formation event that allows the plant to track the time of day and tell the plant when to bloom or metabolize nutrients.

A plant uses visual cues to constantly read every aspect of its environment and retune its physiological functions to adapt accordingly. Some of these cues are monitored by plant proteins that absorb and transmit light signals — called photoreceptors. The research team specifically studied two key photoreceptors, Zeitlupe (Zite-LOO-puh) and FKF-1.

“Plants have a very complex array of photoreceptors absorbing all different wavelengths of light to recognize every aspect of their environment and adapt accordingly,” said Zoltowski, an assistant professor in the SMU Department of Chemistry. “All their cells and tissue types are working in concert with each other.”

The finding was reported in the article “Kinetics of the LOV domain of Zeitlupe determine its circadian function in Arabidopsis” in the journal eLIFE online in advance of print publication.

Co-author and lead author is Ashutosh Pudasaini, a doctoral graduate from the SMU Department of Chemistry who is now a postdoctoral fellow at the University of Texas Southwestern Medical School, Dallas. Other co-authors are Jae Sung Shim, Young Hun Song and Takato Imaizumi, University of Washington, Seattle; Hua Shi and David E. Somers, Ohio State University; and Takatoshi Kiba, RIKEN Center for Sustainable Resource Science, Japan.

The research is funded through a grant from the National Institute of General Medical Sciences of the National Institutes of Health awarded to Zoltowski’s lab.

Nighttime is the right time for plants to grow
“If you live in the Midwest, people say you hear the corn growing at night,” said Zoltowski, who grew up in rural Wisconsin.

“During the day, a plant is storing as much energy as it can by absorbing photons of sunlight, so that during the evening it can do all its metabolism and growth and development. So there’s this separation between day and night.”

Plants measure these day and night oscillations as well as seasonal changes. Knowledge already existed of the initial chemistry, biology and physiology of that process.

In addition, Zoltowski and colleagues published in 2013 the discovery that the amino acids in Zeitlupe — working like a dimmer switch — gradually get more active as daytime turns to evening, thereby managing the 24-hour Circadian rhythm. Additionally, they found that FKF-1 is very different from Zeitlupe. FKF-1 switches on with morning light and measures seasonal changes, otherwise called photoperiodism.

But a knowledge gap remained. It was a mystery how the information is integrated by the organism.

“Ultimately that has to be related to some kind of chemical event occurring, some kind of chemical timekeeper,” Zoltowski said. “So by following that trail we figured out how the chemistry works.”

Dark state and light state snapshots
The problem required a two-pronged approach: Solving the structure of the protein to understand how forming and breaking bonds changes how the organism perceives its environment; and solving the chemistry, specifically the crystal structures of the protein’s dark and light states.

That process yielded a snapshot of the protein in the dark state and a snapshot of the protein in the light state, so the researchers could watch changes in protein structure in response to the bond-forming event.

From there, the researchers made mathematical models 1) that explain how the chemistry of the bond breaking and bond forming event, and the rate at which it occurs, should affect the organism; and 2) that design mutations to the protein that affect how it goes from the dark state to the light state to block that process.

Standard techniques yielded the discovery
The team used a few standard techniques. To get at the chemistry, they deployed ultra-violet visible spectroscopy to measure how efficiently proteins absorb light. They followed differences in the absorption spectrum, seeing what wavelengths are absorbed, to track chemical changes between the dark and the light states.

On the structure side, they crystallized the proteins and collected data at synchrotron sources at Cornell University, then mapped out like a puzzle where all the electrons are located in the crystal. From there they could fit and build — amino acid by amino acid — the protein, yielding a three-dimensional image of where every atom in the protein is located.

“This gives us pictures and snapshots of all those discrete events, where then we can look at how the atoms are moving and changing from one to the other,” Zoltowski said. “That allows us to see the bonds forming, the bonds breaking, and how the rest of the protein changes in response to that.”

Why didn’t we think of that?
The question has been an important one in the field, but challenging technical hurdles thwarted solutions, said Zoltowski. The key for his team was persistence and years of experience.

“This is not an easy protein to work with — it’s difficult to get crystals of these proteins. It requires a protein that is stable enough and will interact in a way that it yields a perfectly ordered crystal. So it’s difficult to do the chemistry and the structures. Researchers have struggled with getting adequate amounts of protein to be able to do these types of characterizations,” he said.

Think of it like a diamond, Zoltowski said, which is a perfectly ordered crystal that is just carbon atoms arranged in a specific way.

“Zeitlupe and FKF-1 have thousands of atoms in each protein, and in order to get a crystal, each molecule of the protein needs to arrange itself with the same type of accuracy and precision as carbon atoms in a diamond. Getting that to occur, where they pack nicely together, is non trivial. And some proteins just are really challenging to work with.”

Zoltowski and his colleagues have been fortunate in having years of experience working with these families of proteins, called the Light-oxygen-voltage-sensing domains, or LOV domains, for short.

“So we’ve developed a lot of skills and techniques over the years that can get over some of the technical hurdles,” he said. “So just from gaining experience over time, we’ve gotten better with working with some very difficult proteins. It makes something that is challenging, much more tractable for our lab.”

Does this apply to all LOV proteins in every plant?
Zeitlupe is a German word that means slow motion. The protein was dubbed Zeitlupe because scientists discovered when they found mutations of this protein previously that it made the Circadian clock run slower. It naturally altered the way the organism perceived time.

“We wanted to understand the proteins well enough that we could selectively alter the chemistry, or selectively alter the structure, to create mutations that would be testable in the organism,” Zoltowski said. “We wanted a predictive model that would tell us that these mutations that affect the kinetics — the rate at which this bond breaks — should do ‘X’ in the organism.”

The team’s new discovery results in hybrid plants — something nature already does and has done for millions of years through the process of evolution so that plants adapt to survive.

“We’re not putting anything into the plant or changing its genetics,” Zoltowski said. “We’re making a very subtle, targeted mutation to a specific protein that already is a native plant protein — and one that we’ve shown in this paper has evolved considerably throughout various different agricultural crops to already do this.”

The discovery gives scientists the ability to rationally interpret environmental information affecting a plant in order to introduce mutations, instead of relying on selective breeding to achieve a targeted mutation to generate phenotypes that potentially allow the plant to grow in a different environment.

What’s next?
The research opens a lot of new doors, including new questions about how these proteins are changing their configuration and how other variables, like oxidative stress, couple with the plant’s global sensory networks to also alter proteins and send multiple signals from the environment.

“What we’ve learned is that you need to pay careful attention to specific parts of the protein because they’re modulating activity selectively in different categories of this family,” Zoltowski said. “If we look at the whole family of these proteins, there are key amino acids that are evolutionarily selected, so they evolve specific modulations of this activity for their own independent niche in the environment. One of the take-homes is there are areas in the protein we need to look at to see how the amino acids are now different.”

Besides the NIH grant, the lab operates with $250,000 from the American Chemical Society’s Herman Frasch Foundation for Chemical Research Grants in Agricultural Chemistry. — Margaret Allen

Tags Brian D. Zoltowski, Dedman College, SMU Department of Chemistry

Earth & Climate Energy & Matter Learning & Education Researcher news SMU In The News

CTNewsJunkie.com: Ignoring Science At Our Own Peril

Post author By Margaret Allen
Post date April 18, 2017
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“A scientific theory is a very well-tested explanation, built from facts, confirmed hypotheses, and inferences.” — SMU physicist Stephen Sekula

An Op-Ed in the online Connecticut news outlet CTNewsJunkie.com tapped the expertise of SMU Associate Professor of Physics Stephen Sekula.

The writer of the piece, High School English teacher Barth Keck at Haddam-Killingworth High School, quoted the comments of Sekula, who spoke to Keck’s media literacy class.

The opinion piece, “Ignoring Science At Our Own Peril,” addressed the issue of science illiteracy. The editorial published April 14, 2017.

Sekula was among the SMU physicists at Geneva-based CERN — seat of the world’s largest collaborative physics experiment — in December 2011 who found hints of the long sought after Higgs boson, dubbed the fundamental “God” particle.

Sekula conducts research at the energy frontier through CERN’s ATLAS Experiment. He co-convened the ATLAS Higgs Subgroup 6: Beyond-the-Standard Model Higgs Physics from 2012-2013. He is involved in the search for additional Higgs bosons. He also is an authority on big data and high-performance computing.

Read the full Op-Ed.

EXCERPT:

By Barth Keck
CTNewsJunkie.com
Last week was a newsworthy week — at least for this high school English teacher.

In a story out of Hartford last Wednesday, the state Board of Education officially eliminated the requirement that standardized test scores be tied to teacher evaluations. The move, while controversial, was a common-sense decision that recognizes the many problems created by evaluations based on standardized tests. A newsworthy development, indeed, for anyone interested in education.

Even so, a more newsworthy event for me occurred on Tuesday when Southern Methodist University professor Stephen Sekula visited English and science classes at his alma mater and my workplace, Haddam-Killingworth High School. Speaking to my students in Media Literacy, Sekula explained in vivid detail how scientists rigorously and deliberately employ the scientific method in their never-ending search for answers. It is with similar vigilance, he explained, that individuals must consider the multitude of messages around them to become truly “media-literate.”

“A scientific theory is a very well-tested explanation, built from facts, confirmed hypotheses, and inferences,” according to the physics professor. “It is more powerful than a fact because it explains facts.”

Unfortunately, said Sekula, the word “theory” is often likened to “opinion” in public dialogue — as in “human-caused climate change is just a theory” — but there’s an essential difference between theory and opinion. Scientists know the difference, of course, but so should all citizens. Thus, a media-literate person sees a red flag whenever someone — a “pseudoscientist” — uses “theory” and “opinion” interchangeably.

“Pseudoscience readily admits opinions and equates that with the idea of scientific theory,” explained Sekula, “requiring no high quality evidence to make explanatory claims about the world.”

And there it was: the explanation for so much happening in the public sphere right now. Fake news, conspiracy theories, science-averse officials appointed to science-dependent federal agencies. Professor Sekula’s message could not be more timely and, therefore, newsworthy.

Read the full Op-Ed.

Tags Dedman College, SMU Department of Physics, Stephen J. Sekula

Earth & Climate Energy & Matter Learning & Education Researcher news SMU In The News

KDFW Fox 4: NASA discovers seven earth-like planets relatively near

Post author By Margaret Allen
Post date February 24, 2017
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A “major step forward” toward the goal of answering the very big question: Is there life on other worlds?

DFW Fox 4 TV reporter Steve Eagar expressed “nerd-level” excitement about NASA’s announcement Feb. 22 of the discovery of seven new Earth-like planets. Eagar interviewed SMU professor Robert Kehoe, who leads the SMU astronomy team from the Department of Physics.

NASA announced that the Spitzer Space Telescope has revealed the first known system of seven Earth-size planets around a single star. Three of these planets are firmly located in an area called the habitable zone, where liquid water is most likely to exist on a rocky planet.

“This is a surprising jump in our ability to understand earth like planets,” Kehoe told Eagar.

Kehoe and the SMU astronomy team recently reported discovery of a rare star as big — or bigger — than the Earth’s sun that is expanding and contracting in a unique pattern in three different directions.

The star is one that pulsates and so is characterized by varying brightness over time. It’s situated 7,000 light years away from the Earth in the constellation Pegasus. Called a variable star, this particular star is one of only seven known stars of its kind in our Milky Way galaxy.

Watch the video interview on Fox 4.

Tags Dedman College, Robert Kehoe, SMU Department of Physics

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Astronomy: High school students identify an ultra-rare star

Post author By Margaret Allen
Post date February 20, 2017
No Comments on Astronomy: High school students identify an ultra-rare star

This newly-discovered variable is one of only seven of its kind known in our galaxy.

Science journalist Alison Klesman with the online science news magazine Astronomy covered the discovery of a variable star by SMU professor Robert Kehoe and the astronomy team in the SMU Department of Physics.

A high school student in an SMU summer astronomy program made the initial discovery upon culling through archived star observation data recorded by the small but powerful ROTSE-I telescope formerly at Los Alamos National Laboratory in New Mexico.

Other authors on the study were SMU research astronomer Farley Ferrante, a member of the team, Plano Senior High School student Derek Horning, who first discovered the object in the ROTSE-I data, and Eric Guzman, a physics graduate from the University of Texas at Dallas who is entering SMU’s graduate program and who identified the star as pulsating.

The newest delta Scuti (SKOO-tee) star in our night sky is so rare it’s only one of seven identified by astronomers in the Milky Way. Discovered at SMU, the star — like our sun — is in the throes of stellar evolution, to conclude as a dying ember in millions of years. Until then, the exceptional star pulsates brightly, expanding and contracting from heating and cooling of hydrogen burning at its core.

The Astronomy article, “High school students identify an ultra-rare star,” published Feb. 15, 2017.

Read the full story.

EXCERPT:

By Alison Klesman
Astronomy
The stars shining in the night sky might seem steady and reliable, but in truth, they are constantly changing and evolving. Out of the 100 billion or so stars that inhabit the Milky Way, a little more than 400,900 are classified as variable, meaning they change in brightness over time.

Of those hundreds of thousands of variables catalogued in our galaxy, however, only seven belong to a class called Triple Mode high amplitude delta Scuti, or HADS(B), stars — and that seventh was just recently discovered by a high school student during a summer astronomy program at Southern Methodist University in Dallas.

The star, roughly the size of our Sun or possibly larger, is about 7,000 light-years away in the constellation Pegasus. It currently has only a catalog name: ROTSE1 J232056.45+345150.9. The name comes in part from the telescope used to discover it, the ROTSE-I telescope at Los Alamos National Laboratory in New Mexico.

While examining data from the telescope taken in September of 2000, Plano Senior High School student Derek Hornung noticed the star’s strange light curve, which shows the star’s brightness over time. A non-variable star’s light curve is simply a straight line, unchanging as the hours, days, and months go by. But a variable star exhibits periodic changes in brightness over the course of hours or days, creating a recognizable repeating pattern. Variable stars are classified by the patterns their light curves make, and named after the first star of each type discovered. Delta Scuti variables are thus named after the star delta Scuti.

But there’s more to this story, still. The star is not only a delta Scuti variable, of which there are thousands known, but it is also a rare type within the delta Scuti class, a HADS(B) star. HADS(B) stars show asymmetric light curves that change brightness quickly over time. These stars are pulsating in two modes, which means the star is expanding in two directions at once. There are only 114 HADS(B) stars currently known. Rarer still are Triple Mode HADS(B) stars, of which there were only six previously identified in the Milky way. Triple Mode HADS(B) stars pulsate in not two, but three directions at once. For ROTSE1 J232056.45+345150.9, this process repeats itself every 2.5 hours.

Read the full story.

Tags Dedman College, Farley Ferrante, Robert Kehoe, SMU Department of Physics

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New delta Scuti: Rare pulsating star 7,000 light years away is 1 of only 7 in Milky Way

Post author By Margaret Allen
Post date February 13, 2017

A star — as big as or bigger than our sun — in the Pegasus constellation is expanding and contracting in three different directions simultaneously on a scale of once every 2.5 hours, the result of heating and cooling of hydrogen fuel burning 28 million degrees Fahrenheit at its core

The newest delta Scuti (SKOO-tee) star in our night sky is so rare it’s only one of seven identified by astronomers in the Milky Way. Discovered at Southern Methodist University in Dallas, the star — like our sun — is in the throes of stellar evolution, to conclude as a dying ember in millions of years. Until then, the exceptional star pulsates brightly, expanding and contracting from heating and cooling of hydrogen burning at its core.

Astronomers are reporting a rare star as big — or bigger — than the Earth’s sun that is expanding and contracting in a unique pattern in three different directions.

The star is one that pulsates and so is characterized by varying brightness over time. It’s situated 7,000 light years away from the Earth in the constellation Pegasus, said astronomer Farley Ferrante, a member of the team that made the discovery at Southern Methodist University, Dallas.

Called a variable star, this particular star is one of only seven known stars of its kind in our Milky Way galaxy.

“It was challenging to identify it,” Ferrante said. “This is the first time we’d encountered this rare type.”

The Milky Way has more than 100 billion stars. But just over 400,900 are catalogued as variable stars. Of those, a mere seven — including the one identified at SMU — are the rare intrinsic variable star called a Triple Mode ‘high amplitude delta Scuti’ (pronounced SKOO-tee) or Triple Mode HADS(B), for short.

“The discovery of this object helps to flesh out the characteristics of this unique type of variable star. These and further measurements can be used to probe the way the pulsations happen,” said SMU’s Robert Kehoe, a professor in the Department of Physics who leads the SMU astronomy team. “Pulsating stars have also been important to improving our understanding of the expansion of the universe and its origins, which is another exciting piece of this puzzle.”

The star doesn’t yet have a common name, only an official designation based on the telescope that recorded it and its celestial coordinates. The star can be observed through a telescope, but identifying it was much more complicated.

Upon verification, the star was logged into the International Variable Star Index as ROTSE1 J232056.45+345150.9 by the American Association of Variable Star Observers at this link.

How in the universe was it discovered?
SMU’s astrophysicists discovered the variable star by analyzing light curve shape, a key identifier of star type. Light curves were created from archived data procured by ROTSE-I during multiple nights in September 2000. The telescope generates images of optical light from electrical signals based on the intensity of the source. Data representing light intensity versus time is plotted on a scale to create the light curves.

Plano Senior High School student Derek Hornung first discovered the object in the ROTSE-I data and prepared the initial light curves. From the light curves, the astronomers knew they had something special.

It became even more challenging to determine the specific kind of variable star. Then Eric Guzman, a physics graduate from the University of Texas at Dallas, who is entering SMU’s graduate program, solved the puzzle, identifying the star as pulsating.

“Light curve patterns are well established, and these standard shapes correspond to different types of stars,” Ferrante said. “In a particular field of the night sky under observation there may have been hundreds or even thousands of stars. So the software we use generates a light curve for each one, for one night. Then — and here’s the human part — we use our brain’s capacity for pattern recognition to find something that looks interesting and that has a variation. This allows the initial variable star candidate to be identified. From there, you look at data from several other nights. We combine all of those into one plot, as well as add data sets from other telescopes, and that’s the evidence for discerning what kind of variable star it is.”

That was accomplished conclusively during the referee process with the Variable Star Index moderator.

The work to discover and analyze this rare variable star was carried out in conjunction with analyses by eight other high school students and two other undergraduates working on other variable candidates. The high school students were supported by SMU’s chapter of the Department of Energy/National Science Foundation QuarkNet program.

Heating and cooling, expanding and contracting
Of the stars that vary in brightness intrinsically, a large number exhibit amazingly regular oscillations in their brightness which is a sign of some pulsation phenomenon in the star, Ferrante said.

Pulsation results from expanding and contracting as the star ages and exhausts the hydrogen fuel at its core. As the hydrogen fuel burns hotter, the star expands, then cools, then gravity shrinks it back, and contraction heats it back up.

“I’m speaking very generally, because there’s a lot of nuance, but there’s this continual struggle between thermal expansion and gravitational contraction,” Ferrante said. “The star oscillates like a spring, but it always overshoots its equilibrium, doing that for many millions of years until it evolves into the next phase, where it burns helium in its core. And if it’s about the size and mass of the sun — then helium fusion and carbon is the end stage. And when helium is used up, we’re left with a dying ember called a white dwarf.”

Within the pulsating category is a class of stars called delta Scuti, of which there are thousands. They are named for a prototype star whose characteristic features — including short periods of pulsating on the scale of a few hours — are typical of the entire class.

Within delta Scuti is a subtype of which hundreds have been identified, called high amplitude delta Scuti, or HADS. Their brightness varies to a particularly large degree, registering more than 10 percent difference between their minimum and maximum brightness, indicating larger pulsations.

Common delta Scuti pulsate along the radius in a uniform contraction like blowing up a balloon. A smaller sub-category are the HADS, which show asymmetrical-like pulsating curves.

Within HADS, there’s the relatively rare subtype called HADS(B) , of which there are only 114 identified.

Star evolution — just a matter of time
A HADS(B) is distinguished by its two modes of oscillation — different parts of the star expanding at different rates in different directions but the ratio of those two periods is always the same.

For the SMU star, two modes of oscillation weren’t immediately obvious in its light curve.

“But we knew there was something going on because the light curve didn’t quite match known light curves of other delta Scuti’s and HADS’ objects we had studied. The light curves — when laid on top of each other — presented an asymmetry,” Ferrante said. “Ultimately the HADS(B) we discovered is even more unique than that though — it’s a Triple Mode HADS(B) and there were previously only six identified in the Milky Way. So it has three modes of oscillation, all three with a distinct period, overlapping, and happening simultaneously.”

So rare, in fact, there’s no name yet for this new category nor a separate registry designation for it. Guzman, the student researcher who analyzed and categorized the object, recalled how the mystery unfolded.

“When I began the analysis of the object, we had an initial idea of what type it could be,” Guzman said. “My task was to take the data and try to confirm the type by finding a second period that matched a known constant period ratio. After successfully finding the second mode, I noticed a third signal. After checking the results, I discovered the third signal coincided with what is predicted of a third pulsation mode.”

The SMU Triple Mode HADS(B) oscillates on a scale of 2.5 hours, so it will expand and contract 10 times in one Earth day. It and the other known six HADS(B)’s are in the same general region of the Milky Way galaxy, within a few thousand light years of one another.

“I’m sure there are more out there,” Ferrante said, “but they’re still rare, a small fraction.”

Red giant the final phase of star’s evolution
SMU’s Triple Mode HADS(B) is unstable and further along in its stellar evolution than our sun, which is about middle-aged and whose pulsating variations occur over a much longer period of time. SMU’s Triple Mode HADS(B) core temperature, heated from the burning of hydrogen fuel, is about 15 million Kelvin or 28 million degrees Fahrenheit.

Someday, millions of years from now, SMU’s Triple Mode HADS(B) will deplete the hydrogen fuel at its core, and expand into a red giant.

“Our sun might eventually experience this as well,” Ferrante said. “But Earth will be inhospitable long before then. We won’t be here to see it.”

Funding was through the Texas Space Grant Consortium, an affiliate of NASA; SMU Dedman College. Department of Energy/National Science Foundation QuarkNet program.

ROTSE-I began operating in late 1997, surveying the sky all night, every clear night of the year for three years. It was decommissioned in 2001 and replaced by ROTSE-III. SMU owns the ROTSE-IIIb telescope at McDonald Observatory, Fort Davis, Texas.

Tags Dedman College, Farley Ferrante, Robert Kehoe, SMU Department of Physics

Earth & Climate Fossils & Ruins Researcher news SMU In The News

Nat’l Geographic: One of Earth’s most dangerous supervolcanoes is rumbling

Post author By Margaret Allen
Post date January 13, 2017

Italy’s Campi Flegrei may be awakening from a long slumber, scientists warn.

Vulcanologist James E. Quick, SMU’s associate vice president for research and dean of Graduate Studies, is quoted for his expertise in the magazine National Geographic.

Quick, a geologist in the Huffington Department of Earth Sciences, is quoted in “One of Earth’s most dangerous supervolcanoes is rumbling.” The article was published Dec. 23, 2016.

An expert in volcano hazards, Quick is an expert in geologic science and volcano risk assessment, particularly the study of magmatic systems. He is a Fellow of the American Association for the Advancement of Science.

In 2009 Quick led the international scientific team that discovered a 280-million-year-old fossil supervolcano in the Italian Alps. The supervolcano’s magmatic plumbing system is exposed to an unprecedented depth of 25 kilometers, giving scientists new understanding into the phenomenon of explosive supervolcanos.

Italian geologists in 2010 awarded Quick the Capellini Medal to recognize the discovery. In 2013 an area encompassing the supervolcano won designation as the Sesia-Val Grande Geopark by the UNESCO Global Network of National Geoparks.

Prior to SMU, Quick served a distinguished 25-year scientific career with the USGS, including as program coordinator for the Volcano Hazards Program.

Read the full story.

EXCERPT:

By Brian Clark Howard
National Geographic
A long-quiet yet huge supervolcano that lies under 500,000 people in Italy may be waking up and approaching a “critical state,” scientists report this week in the journal Nature Communications.

Based on physical measurements and computer modeling, “we propose that magma could be approaching the CDP [critical degassing pressure] at Campi Flegrei, a volcano in the metropolitan area of Naples, one of the most densely inhabited areas in the world, and where accelerating deformation and heating are currently being observed,” wrote the scientists—who are led by Giovanni Chiodini of the Italian National Institute of Geophysics in Rome.

A sudden release of hot magmatic gasses is possible in the near future, which could trigger a large eruption, the scientists warn. Yet the timing of any possible eruption is unknown and is currently not possible to predict….

The scars of another supervolcano were recently found in the Sesia Valley in the Italian Alps. That eight-mile-wide caldera likely last erupted 280 million years ago, when it blasted out a thousand times more material than Mount St. Helens spewed during its infamous 1980 eruption. The result was the blocking out of the sun, which led to global cooling.

“There will be another supervolcano explosion,” scientist James Quick, a geologist at Southern Methodist University in Texas, said in a statement when that volcano was found.
“We don’t know where, [but] Sesia Valley could help us to predict the next event.”

Read the full story.

Tags Dedman College, James E. Quick, Roy M. Huffington Department of Earth Sciences

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Green chemistry: Au naturel catalyst mimics nature to break tenacious carbon-hydrogen bond

Post author By Margaret Allen
Post date January 4, 2017

Upon mixing the reactants (copper + ligand + hydrogen peroxide + carbon-hydrogen substrate) the starting colorless solution turns green-blue, indicating that an oxidative process is occurring. (Credit: SMU)

Chemists discover new way to crack the stubborn carbon-hydrogen bond that could allow industry to make petroleum-derived commercial products easier, cheaper and cleaner

A new catalyst for breaking the tough molecular bond between carbon and hydrogen holds the promise of a cleaner, easier and cheaper way to derive products from petroleum, says a researcher at Southern Methodist University, Dallas.

“Some of the most useful building blocks we have in the world are simple, plentiful hydrocarbons like methane, which we extract from the ground. They can be used as starting materials for complex chemical products such as plastics and pharmaceuticals,” said Isaac Garcia-Bosch, Harold A. Jeskey Endowed Chair assistant professor in the Department of Chemistry at SMU. “But the first step of the process is very, very difficult — breaking that carbon-hydrogen bond. The stronger the bond, the more difficult it is to oxidize.”

The chemical industry must break the tenacious bond between carbon and hydrogen molecules to synthesize oxidative products such as methanol and phenols. It’s called oxidizing because it causes the molecule to undergo a reaction in which it combines with oxygen, breaking C-H bonds and forming new carbon-oxygen bonds.

The conventional chemical recipe calls for inefficient and expensive oxidants to break the C-H bond. That process is costly, difficult and leaves behind dirty waste products.

Chemists at SMU, in collaboration with The Johns Hopkins University, have found a cheaper, cleaner way to crack the stubborn C-H bond.

Garcia-Bosch and chemist Maxime A. Siegler, director of the X-ray Crystallography Facility at The Johns Hopkins University, used copper catalysts that in combination with hydrogen peroxide (oxygen source) can convert C-H bonds to C-O bonds.

“This is a very important discovery because it’s the first time it’s been proven that copper can carry out this kind of oxidation outside of nature in an efficient way,” Garcia-Bosch said. “The prep is very simple, so labs anywhere can do it. Copper is relatively cheap compared to other metals such as palladium, gold or silver, and hydrogen peroxide is readily available, relatively cheap and very clean. One of the byproducts of oxidations with hydrogen peroxide (H2O2) is water (H2O), which is the cleanest waste product you could have.”

Additionally, the researchers found the right ligand — a nitrogen-based material that binds to the copper so that the oxidation process can occur with close to perfect efficiency.

It’s important to have the right ligand, the right amount of hydrogen peroxide, and the right metal in order to oxidize these challenging C-H bonds.

“We found that combination,” Garcia-Bosch said.

Chemistry is like a puzzle, where you build new molecules out of other molecules, he said.

In any one molecule there are many C-H bonds. For example in octanes, such as the ones found in gasoline, there’s a carbon chain of eight carbons with multiple C-H bonds with different chemical properties, Garcia-Bosch said, and from the oxidation of each of the C-H bonds, a different product results.

Chemists design catalysts that are capable of breaking and forming bonds in order to build complex chemical structures.

“Catalysts have to be able to select between different C-H bonds and form new carbon-oxygen, carbon-nitrogen or carbon-fluoride bonds, for example,” Garcia-Bosch said. “Biological processes use metals to do this all the time, for example in our bodies when our liver processes a pharmaceutical that we ingest using iron. Minerals such as iron, copper, manganese, calcium and potassium are critical for the natural catalytic process. For example, trees use manganese (photosynthesis) to transform water into the oxygen that we breathe”

Garcia-Bosch and Siegler reported their findings in the article “Copper-Catalyzed Oxidation of Alkanes with H2O2 under a Fenton-like Regime,” published in the international edition of the journal Angewandte Chemie.

First time for using copper for C-H oxidation
In organic chemistry, there aren’t many examples of copper as a catalyst for carbon-hydrogen oxidation. Most examples are based on iron.

“This is the first time in our field that we’ve used copper to do this C-H oxidation in a very efficient way,” Garcia-Bosch said.

“Copper is very versatile in nature,” he said. “With small changes in the environment of copper, you can do very diverse chemistry. That’s why we picked it.”

That environment is the ligand, which gives properties to the copper to spark the chemical reaction when the chemical ingredients are combined in a vial or round bottom flask.

The researchers discovered that these catalysts — copper in the form of a white salt and the ligand as an oil — can oxidize C-H bonds in a very efficient way in combination with hydrogen peroxide, a reduced form of oxygen that nature uses.

“You can find hydrogen peroxide anywhere, even at home in your medicine cabinet. So it’s a mild oxidant,” Garcia-Bosch said. “It’s convenient also, because it’s a liquid, rather than, say, a gas, which might require special storage. You mix everything together in a solvent and it reacts. It’s like making a soup, a recipe, then you analyze the result to see what you get.”

Using a gas chromatography instrument, the Garcia-Bosch and Siegler analyzed the final solution to observe the results of the reaction. That allowed them to quantify the amount of oxidation product that was formed during the reaction.

Next step — targeting a specific C-H bond
“We tested this catalytic system for different substrates and we saw that it’s not very selective,” Garcia-Bosch said. “That’s a problem. So if we have molecules that have many different C-H bonds, then it’s going to oxidize all of them in a non-selective manner. In our lab, we would like to find selective catalysts. That’s the next project.”

Garcia-Bosch holds the Harold A. Jeskey Endowed Chair in Chemistry. The research was funded through The Robert A. Welch Foundation (Grant N-1900).

Tags Dedman College, Isaac Garcia-Bosch, SMU Department of Chemistry

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LiveScience: Tough Turtle — Dino-Killing Asteroid Spared Sea Creature

Post author By Margaret Allen
Post date November 14, 2016

“If these sea turtles do, in fact, form a tightly knit group, evolutionarily speaking, the [African] specimen provides proof that members of that group survived the mass extinction at the end of the Cretaceous.” — Timothy Myers, SMU

Live Science Senior Writer Laura Geggel covered the research of paleontologist Timothy Scott Myers, a postdoctoral researcher in SMU’s Roy M. Huffington Department of Earth Sciences.

Myers analyzed an ancient sea turtle, discovered in Angola in 2012, with a triangular-shaped head that lived about 64 million years ago and that is closely related to earlier sea turtles that lived before scientists think an asteroid smashed into the earth sparking a massive mass extinction event.

The article “Tough Turtle: Dino-Killing Asteroid Spared Sea Creature,” cites new findings from Myers’ research, which studied the specimen. It was found along sea cliffs near the town of Landana, in the Angolan province of Cabinda in June 2012.

Read the full story.

EXCERPT:

By Laura Geggel
Live Science
Shortly after an asteroid smashed into Earth about 65.5 million years ago, obliterating much of life on Earth,an ancient sea turtle with a triangular-shaped head swam along the relatively arid shores of southern Africa, a new study finds.

The creature, a newly identified species, lived about 64 million years ago during the Paleocene, an epoch within the Paleogene period, the researchers said. The animal is closely related to earlier sea turtles that lived before the asteroid struck, an event known as the Cretaceous–Paleogene (K-Pg) boundary, which marks the mass extinction that killed about 75 percent of all species on Earth, including the nonavian dinosaurs.

“If these sea turtles do, in fact, form a tightly knit group, evolutionarily speaking, then the [African] specimen provides proof that members of that group survived the mass extinction at the end of the Cretaceous,” study lead researcher Timothy Myers, a research assistant professor in the Department of Earth Sciences at Southern Methodist University in Texas, told Live Science in an email.

Paleontologists found the specimen along the sea cliffs near the town of Landana, in the Angolan province of Cabinda in June 2012. Study senior researcher Louis Jacobs, a vertebrate paleontologist at Southern Methodist University, noticed part of the bone protruding from the rock. He and his team soon realized it was a nearly complete turtle skull and most of a hyoid, a U-shaped neck bone that supports the tongue.

Read the full story.

Tags Dedman College, Louis L. Jacobs, Roy M. Huffington Department of Earth Sciences, Timothy S. Myers

Culture, Society & Family Earth & Climate Fossils & Ruins Plants & Animals Researcher news

Textbook theory of how humans populated America is “biologically unviable,” study finds

Post author By Margaret Allen
Post date August 10, 2016

Using ancient DNA, researchers have created a unique picture of how a prehistoric migration route evolved over thousands of years – revealing that it could not have been used by the first people to enter the Americas, as traditionally thought.

The established theory about how Ice Age peoples first reached the present-day United States has been challenged by an unprecedented study that concludes that their supposed entry route was “biologically unviable.”

The first people to reach the Americas crossed via an ancient land bridge between Siberia and Alaska but then, according to conventional wisdom, had to wait until two huge ice sheets that covered what is now Canada started to recede, creating the so-called “ice-free corridor” that enabled them to move south.

In a new study published in the journal Nature, however, an international team of researchers used ancient DNA extracted from a crucial pinch-point within this corridor to investigate how its ecosystem evolved as the glaciers began to retreat.

They created a comprehensive picture showing how and when different flora and fauna emerged so the once ice-covered landscape became a viable passageway. No prehistoric reconstruction project like this has ever been attempted before.

Present day view south in Canada's Peace River drainage basin where retreating ice sheets created an ice-free corridor more than 13,000 years ago. (Mikkel Winther Pedersen, University of Copenhagen) — Present day view south in Canada’s Peace River drainage basin where retreating ice sheets created an ice-free corridor more than 13,000 years ago. (Mikkel Winther Pedersen, University of Copenhagen)

The researchers conclude that while people may well have travelled this corridor after about 12,600 years ago, it would have been impassable earlier than that, as the corridor lacked crucial resources, such as wood for fuel and tools, as well as game animals essential to the hunter-gatherer lifestyle.

If this is true, then it means that the first Americans, who were present south of the ice sheets long before 12,600 years ago, must have made the journey south by another route. The study’s authors suggest that they probably migrated along the Pacific coast.

Who these people were is still widely disputed. Archaeologists agree, however, that early inhabitants of the modern-day contiguous United States included the so-called “Clovis” culture, which first appear in the archaeological record over 13,000 years ago. And the new study argues that the ice-free corridor would have been completely impassable at that time.

“There is compelling evidence that Clovis was preceded by an earlier and possibly separate population,” said archaeologist and co-author on the study David J. Meltzer, Henderson-Morrison Professor of Prehistory in the Department of Anthropology at Southern Methodist University, Dallas. “But either way, the first people to reach the Americas in Ice Age times would have found the corridor itself impassable.”

The ice-free corridor simply opened up too late to be the principal entry route
The research was led by evolutionary geneticist Eske Willerslev, a Fellow of St John’s College, University of Cambridge, who also holds posts at the Centre for GeoGenetics, University of Copenhagen, and the Wellcome Sanger Institute in Cambridge.

“The bottom line is that even though the physical corridor was open by 13,000 years ago, it was several hundred years before it was possible to use it,” Willerslev said. “That means that the first people entering what is now the U.S., Central and South America must have taken a different route. Whether you believe these people were Clovis, or someone else, they simply could not have come through the corridor, as long claimed.”

Mikkel Winther Pedersen, a doctoral student at the Centre for GeoGenetics, University of Copenhagen, who conducted the molecular analysis, added: “The ice-free corridor was long considered the principal entry route for the first Americans. Our results reveal that it simply opened up too late for that to have been possible.”

The corridor is thought to have been about 1,500 kilometers long, and emerged east of the Rocky Mountains 13,000 years ago in present-day western Canada, as two great ice sheets – the Cordilleran and Laurentide, retreated.

On paper, this fits well with the argument that Clovis people were the first to disperse across the Americas. The first evidence for this culture, which is named after distinctive stone tools found near Clovis, New Mexico, also dates from roughly the same time, although many archaeologists now believe that other people arrived earlier.

“What nobody has looked at is when the corridor became biologically viable,” Willerslev said. “When could they actually have survived the long and difficult journey through it?”

Radiocarbon dates, pollen, macrofossils and DNA revealed how ecosystem developed
The conclusion reached by Willerslev and his colleagues is that the journey would have been impossible until about 12,600 years ago. Their research focused on a “bottleneck,” one of the last parts of the corridor to become ice-free, and now partly covered by Charlie Lake in British Columbia, and Spring Lake, Alberta — both part of Canada’s Peace River drainage basin.

The team gathered evidence — including radiocarbon dates, pollen, macrofossils and DNA taken from lake sediment cores — which they obtained standing on the frozen lake surface during the winter season. Willerslev’s own PhD, 13 years ago, demonstrated that it is possible to extract ancient plant and mammalian DNA from sediments, as it contains preserved molecular fossils from substances such as tissue, urine and feces.

Having acquired the DNA, the group then applied a technique termed “shotgun sequencing.”

“Instead of looking for specific pieces of DNA from individual species, we basically sequenced everything in there, from bacteria to animals,” Willerslev said. “It’s amazing what you can get out of this. We found evidence of fish, eagles, mammals and plants. It shows how effective this approach can be to reconstruct past environments.”

This approach allowed the team to see, with remarkable precision, how the bottleneck’s ecosystem developed. Crucially, it showed that before about 12,600 years ago, there were no plants, nor animals, in the corridor, meaning that humans passing through it would not have had resources vital to survive.

Clovis could not have travelled through ice-free corridor as previously believed
Around 12,600 years ago, steppe vegetation started to appear, followed quickly by animals such as bison, woolly mammoth, jackrabbits and voles. Importantly 11,500 years ago, the researchers identified a transition to a “parkland ecosystem” – a landscape densely populated by trees, as well as moose, elk and bald-headed eagles, which would have offered crucial resources for migrating humans.

Somewhere in between, the lakes in the area were populated by fish, including several identifiable species such as pike and perch. Finally, about 10,000 years ago, the area transitioned again, this time into boreal forest, characterized by spruce and pine.

The fact that Clovis was clearly present south of the corridor before 12,600 years ago means that they could not have travelled through it.

“Most likely, you would say that the evidence points to their having travelled down the Pacific Coast,” Willerslev added. “That now seems the most likely scenario.”

The paper, “Postglacial viability and colonization in North America’s ice-free corridor,” is published online ahead of print in Nature on Aug. 10, 2016.

Tags David Meltzer, Dedman College, Featurette, SMU Department of Anthropology

Earth & Climate Fossils & Ruins Researcher news SMU In The News

Laser Beats Rock: Armored Dinosaur May Have Relied Most on Sense of Smell

Post author By Margaret Allen
Post date July 26, 2016

CT scans offer new insight into the little-understood Pawpawsaurus: One clue that led the researchers to determine that the sense of smell was Pawpawsaurus’s strongest sense was the large olfactory ratio.

Independent science journalist Sarah Puschmann covered the research of SMU Earth Sciences Professor Louis L. Jacobs in a post on her blog “Armored Dinosaur May Have Relied Most on Sense of Smell.”

A professor in Dedman College‘s Roy M. Huffington Department of Earth Sciences, Jacobs is co-author of a new analysis of the Cretaceous Period dinosaur Pawpawsaurus based on the first CT scans ever taken of the dinosaur’s skull.

A Texas native from what is now Tarrant County, Pawpawsaurus lived 100 million years ago, making its home along the shores of an inland sea that split North America from Texas northward to the Arctic Sea.

The Laser Beats Rock article published July 25, 2016.

Pawpawsaurus campbelli is the prehistoric cousin of the well-known armored dinosaur Ankylosaurus, famous for a hard knobby layer of bone across its back and a football-sized club on its tail.

Jacobs, a world-renowned vertebrate paleontologist, joined SMU’s faculty in 1983 and in 2012 was honored by the 7,200-member Science Teachers Association of Texas with their prestigious Skoog Cup for his significant contributions to advance quality science education.

Jacobs is president of SMU’s Institute for the Study of Earth and Man.

Read the full story.

EXCERPT:

By Sarah Puschmann
Laser Beats Rock
In 1819, the German naturalist Lorenz Oken found something astonishing inside a pterodactyl’s broken skull: petrified mud in the form of the long deceased dinosaur’s brain, so well molded into the crevices as to reveal the brain’s two distinct halves.

This so-called “fossil brain” is one of the first known instances of a cranial endocast, an internal cast of the skull that makes the impressions of the decayed soft tissue visible. For paleoneurologists not lucky enough to uncover a natural endocast, some have opted to slice open skulls and made molds using liquid latex rubber or plaster of Paris.

But cutting open a skull for study isn’t always an option, particularly if it is a holotype, the singular specimen used to define a species for the first time. This is the case for the 100 million year old skull from a dinosaur called Pawpawsaurus campbelli studied by Ariana Paulina-Carabajal of the National Research Council of Argentina (CONICET) and the Institute of Investigations in Biodiversity and the Environment (INIBIOMA) and her team, led by Louis Jacobs.

By CT scanning the skull, it was possible to make important insights about the dinosaur’s olfaction and hearing while leaving the precious holotype intact. Their analysis led the researchers to conclude that smell was the sense Pawpawsaurus most likely relied on most, as reported in the journal PLOS ONE.

This is valuable information, especially because so little is known about this dinosaur. What is known is that the four-legged herbivore most likely had long spines on its shoulders and neck, as was the case for other members of the same family of nodosaurids. It also probable that Pawpawsaurus wasn’t endowed with the knob of bone in its tail characteristic of ankylosaurids, a related dinosaur family, nor did it experience the satisfaction of slamming a club tail against, well, anything. (Was there such a thing as tail envy?)

Read the full story.

Tags Dedman College, Louis L. Jacobs, Roy M. Huffington Department of Earth Sciences

Earth & Climate Energy & Matter Researcher news SMU In The News

The Dallas Morning News: Scientists offer explanation on how oil and gas activity triggers North Texas earthquakes

Post author By Margaret Allen
Post date July 25, 2016

Long-awaited study puts forth explanation for exponential increase in North Texas earthquakes, citing unprecedented wastewater injection into a geological formation above seismically active zones.

In an article contributed to The Dallas Morning News, science journalist Anna Kuchment covered the research of SMU seismologists on a possible explanation for the spate of earthquakes in North Texas in recent years.

The study, “Ellenburger wastewater injection and seismicity in North Texas,” posted online July 17 in the peer-reviewed journal Physics of the Earth and Planetary Interiors.

It is the first scientific work to offer an explanation for the Dallas and Irving quakes, Kuchment notes in her article, “Scientists offer possible explanation for how oil and gas activity may have triggered Dallas earthquakes.”

Lead author of the study is SMU seismologist Matthew Hornbach.

Co-authors are SMU students and faculty Madeline Jones, Monique Scales, Heather DeShon, Beatrice Magnani, Brian Stump, Chris Hayward and Mary Layton, and University of Texas at Austin seismologist Cliff Frohlich.

Read the full story.

EXCERPT:

By Anna Kuchment
Dallas Morning News
In a long-awaited study, researchers have offered a possible explanation for how oil and gas activity may have triggered earthquakes in Dallas and Irving last year.

The disposal of wastewater from oil and gas production and hydraulic fracturing “plausibly” set off the tremors, which shook Dallas, Irving, Highland Park and other cities from April 2014 through January 2016, said Matthew Hornbach, the study’s lead author and professor of geophysics at Southern Methodist University.

While the quakes were too small to cause much damage to buildings, they spread alarm through a metro area unaccustomed to feeling the ground shift.

The quakes contributed to a tenfold increase in North Texas’ earthquake hazard level, prompted the Federal Emergency Management Agency to warn of stronger quakes that could cause billions of dollars of damage, and moved local emergency managers to begin preparing for worst-case scenarios.

The study, posted online this week in the peer-reviewed journal Physics of the Earth and Planetary Interiors, is the first scientific work to offer an explanation for the Dallas and Irving quakes. It also provides new evidence that other recent quakes in North Texas’ were likely induced by humans.

Such findings in recent years have prompted pushback from oil and gas companies. This week, through a trade group, they again came out swinging. Steve Everley, a spokesman for an arm of the Independent Petroleum Association of America, questioned the scientists’ work. “Were they looking for media attention?” Everley said in an email. “The authors’ willingness to shift assumptions to fit a particular narrative is concerning, to say the least.”

The state agency that regulates oil and gas, the Railroad Commission, said in a statement that it was reviewing the report “to fully understand its methodology and conclusions.”

Independent experts contacted by The Dallas Morning News praised the study, while cautioning that more work remains before the cause of the Dallas and Irving earthquakes can be firmly established.

“It’s the single best explanation for the increase in earthquakes within the Dallas-Fort Worth basin,” said Rall Walsh, a Ph.D. candidate in geophysics at Stanford University who studies human-triggered earthquakes.

Read the full story.

Tags Beatrice Magnani, Brian W. Stump, Chris Hayward, Heather R. DeShon, Madeline Jones, Matthew J. Hornbach, Monique Scales

Earth & Climate Researcher news SMU In The News Technology

KERA News: Near Wink, Texas, The Sink Holes Are Getting Bigger And Bigger

Post author By Margaret Allen
Post date June 30, 2016

“’We could have another sink hole or two or 10 someday show up,’” (Winkler County Sheriff George) Keely says. In fact, the SMU researchers used satellite imaging to show the problem is getting worse.”

KERA public radio news covered the research of SMU geophysicists Zhong Lu, professor, Shuler-Foscue Chair, and Jin-Woo Kim research scientist, both in the Roy M. Huffington Department of Earth Sciences at SMU.

KERA’s article, “Near Wink, Texas, The Sink Holes Are Getting Bigger And Bigger,” aired June 28, 2016.

The Dedman College faculty are co-authors of a new analysis using satellite radar images to reveal ground movement of two giant sinkholes near Wink, Texas. They found that the movement suggests the two existing holes are expanding, and new ones are forming as nearby subsidence occurs at an alarming rate.

Lu is a member of the Science Definition Team for the dedicated U.S. and Indian NASA-ISRO InSAR mission, set for launch in 2020 to study hazards and global environmental change.

Lu and Kim reported the findings in the scientific journal Remote Sensing, in the article “Ongoing deformation of sinkholes in Wink, Texas, observed by time-series Sentinel-1A SAR Interferometry.”

The research was supported by the U.S. Geological Survey Land Remote Sensing Program, the NASA Earth Surface & Interior Program, and the Shuler-Foscue Endowment at Southern Methodist University.

Read the full story.

EXCERPT:

KERA Public Radio News
The earth is crumbling in West Texas. Scientists from Southern Methodist University have new research that shows two massive sinkholes between the towns of Wink and Kermit are expanding.

Years of drilling for oil and gas have helped wash away salt beds underneath the ground. A shifting water table has made the problem worse and in some places the ground is sinking five inches a year, according to the satellite readings.

Now there’s concern the pits could converge into one giant hole. “A collapse could be catastrophic,” SMU research scientist Jin-Woo Kim said.

These wounds in the West Texas desert have been around for years. The first hole opened up near an abandoned oil well on June 3, 1980. Twenty-two years later, about a mile away, the second one appeared. From the sky, they look like high-caliber bullet holes

“It’s pretty scary. It’s just a big huge pit,” said Winkler County Sheriff George Keely, who has peered over the edge many times in his career. “It’s like standing on the moon looking into a crater. And you can see where it’s just caved off. It’s broken off over the years more and more. When you look down there, you’re looking at water.”

Water is the problem. West Texas, not far from Odessa, is oil country. Drillers started working near

Wink in the mid-1920s. For decades, they injected water into the ground and destabilized the earth, according to the researchers. Meanwhile, as the water table shrinks, thick layers of salt are dissolved far below the surface.

It’s like kicking the legs out from underneath a chair.

Read the full story.

Tags Dedman College, Jin-woo Kim, Roy M. Huffington Department of Earth Sciences, Zhong Lu

Earth & Climate Fossils & Ruins Plants & Animals Researcher news SMU In The News

KERA: Thanks To CT Scans, Scientists Know A Lot About Texas’ Pawpawsaurus Dinosaur

Post author By Margaret Allen
Post date June 30, 2016

“There’s no relationship between dinosaurs and armadillos, which are mammals, but it is interesting that something that looked like an armadillo was here in Texas 100 million years before highways.” — Jacobs

KERA public radio journalist Justin Martin covered the research of SMU Earth Sciences Professor Louis L. Jacobs in a KERA interview “Thanks To CT Scans, Scientists Know A Lot About Texas’ Pawpawsaurus Dinosaur.”

The KERA interview was aired June 29, 2016.

Pawpawsaurus campbelli is the prehistoric cousin of the well-known armored dinosaur Ankylosaurus, famous for a hard knobby layer of bone across its back and a football-sized club on its tail.

Jacobs is president of SMU’s Institute for the Study of Earth and Man.

Hear the KERA segment.

EXCERPT:

By Justin Martin
KERA
CT scans aren’t just for people — they can also be used on dinosaurs.

A skull from the Pawpawsaurus was discovered in North Texas in the early ’90s. It was recently scanned, allowing scientists to digitally rebuild the dinosaur’s brain. Louis Jacobs is a professor of paleontology at SMU and he talks about his research.

Interview Highlights: Louis Jacobs …

… on the reason behind the name Pawpawsaurus: “It was named Pawpawsaurus because the rock unit that it was found in is called the Pawpaw formation and that’s in Fort Worth.”

… on what the CT scan uncovered: “Basically, a CT scan, you are X-raying through the body and then you can make 3D digital models of what’s recorded. We do it with humans and medicine all the time, but dinosaurs and fossils require more energy. So, the X-rays are put through with more energy and you can get a good model.”

… on how you go from scanning to rebuilding a brain: “Visualization through software is … you can see inside the Earth, you can see inside the clouds, you can see inside people, you can see inside everything. The advances in the software make digital visualization accessible. We had the data from scanning the skull of Pawpawsaurus and then from that we rendered 3D models of the brain and also the nasal passages to figure out how the air went through.

Hear the KERA segment.

Tags Dedman College, Louis L. Jacobs, Roy M. Huffington Department of Earth Sciences

Earth & Climate Fossils & Ruins Researcher news SMU In The News Technology

Seeker.com: Giant Sinkholes Near Texas Oil Fields Are Growing

Post author By Margaret Allen
Post date June 17, 2016

New holes are also developing to join them, a satellite study shows.

Online news site Seeker.com covered the research of SMU geophysicists Zhong Lu, professor, Shuler-Foscue Chair, and Jin-Woo Kim research scientist, both in the Roy M. Huffington Department of Earth Sciences at SMU. Seeker.com’s article, “Giant Sinkholes Near Texas Oil Fields Are Growing,” published June 16, 2016.

The Dedman College geophysicists are co-authors of a new analysis using satellite radar images to reveal ground movement of two giant sinkholes near Wink, Texas. They found that the movement suggests the two existing holes are expanding, and new ones are forming as nearby subsidence occurs at an alarming rate.

The research was supported by the U.S. Geological Survey Land Remote Sensing Program, the NASA Earth Surface & Interior Program, and the Shuler-Foscue Endowment at Southern Methodist University.

Read the full story.

EXCERPT:

Seeker.com
In west Texas, they call them the “Wink Sinks.” They’re two giant sinkholes between the towns of Wink and Kermit, the after-affect of a lot of oil being pumped out of the ground in the area more than 60 years ago. And now researchers have discovered that the oddball landmarks — already the size of multiple football fields — are unstable and likely to grow even bigger.

Southern Methodist University geophysicists utilized a time series of radar images captured by an orbiting satellite 435 miles overhead to study the sinkholes. They used a technique called interferometric synthetic aperture radar, or InSAR, to detect changes that aren’t visible to a person at ground level.

Their study, published in the journal Remote Sensing, found that the extent of subsidence in the area has increased significantly over the past seven years, and that the instability originally caused by oil drilling now is being driven by changing groundwater levels.

As the groundwater increases, it dissolves a massive underground salt formation in the area, which then causes the ground to sink.

That’s a problem, because the Wink Sinks already are pretty big. Wink Sink No. 1, which is closer to the town of Kermit, has grown since 1980 to 361 feet across. Wink Sink No. 2, which is nine-tenths of a mile to the south, is about 900 feet across at its widest point.

But to make matters worse, other parts of the area around the sinkholes is sinking as well. The highest rate of ground subsidence is in an area about seven-tenths of a mile northeast of No. 2, which is collapsing at a rate of more than 5 inches per year.

“This area is heavily populated with oil and gas production equipment and installations, hazardous liquid pipelines, as well as two communities,” research scientist Jin-Woo Kim, who co-authored the study with SMU professor Zhong Lu, explained in a press release. He explained that a more massive collapse “could be catastrophic.”

Read the full story.

Follow SMU Research on Twitter, @smuresearch.

For more SMU research see www.smuresearch.com.

SMU is a nationally ranked private university in Dallas founded 100 years ago. Today, SMU enrolls nearly 11,000 students who benefit from the academic opportunities and international reach of seven degree-granting schools. For more information, www.smu.edu.

SMU has an uplink facility located on campus for live TV, radio, or online interviews. To speak with an SMU expert or book an SMU guest in the studio, call SMU News & Communications at 214-768-7650.

Tags Dedman College, Jin-woo Kim, Roy M. Huffington Department of Earth Sciences, Zhong Lu

Earth & Climate Fossils & Ruins Researcher news SMU In The News Technology

Star-Telegram: Two giant sinkholes in West Texas expanding, researchers say

Post author By Margaret Allen
Post date June 17, 2016

“They’re a ways off from the highway; if nobody mentions it, then nobody is interested in it,” Kermit City Manager Gloria Saenz told the New York Daily News.

Fort Worth Star-Telegram journalist Tom Uhler covered the research of SMU geophysicists Zhong Lu, professor, Shuler-Foscue Chair, and Jin-Woo Kim research scientist, both in the Roy M. Huffington Department of Earth Sciences at SMU. Uhler’s article, “Two giant sinkholes in West Texas expanding, researchers say,” published June 16, 2016.

The research was supported by the U.S. Geological Survey Land Remote Sensing Program, the NASA Earth Surface & Interior Program, and the Shuler-Foscue Endowment at Southern Methodist University.

Read the full story.

EXCERPT:

By Tom Uhler
Star-Telegram
A couple of giant sinkholes in the West Texas oil patch are apparently expanding, and might eventually converge into one gigantic hole.

The sinkholes are about a mile apart and sit between Wink and Kermit off I-20 west of Midland-Odessa. They were caused by lots of oil and gas extraction, which peaked from the mid-1920s to the mid-1960s, according to researchers at Southern Methodist University.

Satellite radar images indicate that the giant sinkholes are expanding and that new ones are forming “at an alarming rate” as nearby subsidence occurs, they report in the scientific journal Remote Sensing. One is 361 feet across, about the size of a football field; the other is larger, 670 to 900 feet across.

“A collapse could be catastrophic,” said geophysicist Jin-Woo Kim, who leads the SMU geophysical team reporting the findings.

In addition to Wink and Kermit (combined pop. about 7,000), there’s lots of oil and gas production equipment and installations and hazardous liquid pipelines in the area, Kim said in the report. The fresh water injected underground in the extraction process “can dissolve the interbedded salt layers and accelerate the sinkhole collapse.”

There’s something not too dissimilar happening in Daisetta, east of Houston.

Officials have fenced off the area around the sinkholes between Wink and Kermit and they’ll be monitored, but residents don’t appear to be worried about them.

“They’re a ways off from the highway; if nobody mentions it, then nobody is interested in it,” Kermit City Manager Gloria Saenz told the New York Daily News.

A preacher of the Apocalypse from Indiana had a decidedly different take, exclaiming on YouTube: “Here’s my concern. It’s like hell is being enlarged, and that without measure.”

Well, maybe not quite.

Read the full story.

Follow SMU Research on Twitter, @smuresearch.

Tags Dedman College, Jin-woo Kim, Roy M. Huffington Department of Earth Sciences, Zhong Lu

Earth & Climate Fossils & Ruins Researcher news SMU In The News Technology

New York Daily News: Giant sinkholes in Texas are growing, may collide: study

Post author By Margaret Allen
Post date June 17, 2016

The sinkholes are a little less than a mile apart, but that distance is closing as the land directly around both holes subsides about 2 inches each year.

New York Daily News journalist Anthony Izaguirre covered the research of SMU geophysicists Zhong Lu, professor, Shuler-Foscue Chair, and Jin-Woo Kim research scientist, both in the Roy M. Huffington Department of Earth Sciences at SMU. Izaguirre’s article, “Giant sinkholes in Texas are growing, may collide: study,” published June 16, 2016.

The research was supported by the U.S. Geological Survey Land Remote Sensing Program, the NASA Earth Surface & Interior Program, and the Shuler-Foscue Endowment at Southern Methodist University.

Read the full story.

EXCERPT:

By Anthony Izaguirre
New York Daily News
Two massive, rapidly expanding sinkholes in Texas are at risk of collapsing into each other and causing a “catastrophic” natural disaster, scientists warned.

Geophysicists at Southern Methodist University found that the land around the gaping sinkholes between the west Texas towns of Wink and Kermit is deteriorating — which could end up either forming more holes or creating one giant sinkhole.

These sinkholes, which were caused by the area’s oil and gas extraction industries, are nothing new to Texas residents.

The first hole, Wink Sink #1, opened up in 1980 and is currently about as wide as a football field.

Wink Sink #2, the larger of the two holes, opened in 2002 and stretches for 900 feet at its widest point.

The sinkholes are a little less than a mile apart, but that distance is closing as the land directly around both holes subsides about 2 inches each year.

“This area is heavily populated with oil and gas production equipment and installations, hazardous liquid pipelines, as well as two communities,” Jin-Woo Kim, a coauthor of the report, said in a statement. “A collapse could be catastrophic.”

Read the full story.

Follow SMU Research on Twitter, @smuresearch.

Tags Dedman College, Jin-woo Kim, Roy M. Huffington Department of Earth Sciences, Zhong Lu

Earth & Climate Fossils & Ruins Researcher news SMU In The News Technology

Daily Mail: The two massive and mysterious Texas sinkholes on the verge of creating one colossal lake

Post author By Margaret Allen
Post date June 17, 2016

‘A collapse could be catastrophic. Following our study, we are collecting more high-resolution satellite data over the sinkholes and neighboring regions to monitor further development and collapse.’

London Daily Mail online journalist Ashley Collman covered the research of SMU geophysicists Zhong Lu, professor, Shuler-Foscue Chair, and Jin-Woo Kim research scientist, both in the Roy M. Huffington Department of Earth Sciences at SMU. Collman’s article, “The two massive and mysterious Texas sinkholes on the verge of creating one colossal lake,” published June 16, 2016.

The Dedman College researchers are co-authors of a new analysis using satellite radar images to reveal ground movement of two giant sinkholes near Wink, Texas. They found that the movement suggests the two existing holes are expanding, and new ones are forming as nearby subsidence occurs at an alarming rate.

The research was supported by the U.S. Geological Survey Land Remote Sensing Program, the NASA Earth Surface & Interior Program, and the Shuler-Foscue Endowment at Southern Methodist University.

Read the full story.

EXCERPT:

By Ashley Collman
London Daily Mail
Scientists have issued a grave warning to a small Texas community home to two growing sinkholes.

Geologists at Southern Methodist University say the two sinkholes in Wink and neighboring Kermit, Texas are growing more unstable, and could spark more sinkholes or join to create one massive hole.

This will prove devastating to the local community, which has a combined population of almost 7,000.

SMU researchers Zhong Lu and Jin-Woo Kim recently published their sober warning in a recent article in the journal Remote Sensing.

‘This area is heavily populated with oil and gas production equipment and installations, hazardous liquid pipelines, as well as two communities. The intrusion of freshwater to underground can dissolve the interbedded salt layers and accelerate the sinkhole collapse,’ co-author Kim said in a press release.

‘A collapse could be catastrophic. Following our study, we are collecting more high-resolution satellite data over the sinkholes and neighboring regions to monitor further development and collapse.’

Lu and Kim discovered that the two holes were growing more unstable by using satellite images that measures depressions in the earth’s crust.

The satellite data found that the two holes – which are located about a mile apart – are rapidly growing and causing the ground around them to become more and more unstable – opening up the possibility of more sinkholes or the creation of one giant sinkhole.

The sinkhole in Wink is the oldest and smallest of the two sinkholes, but it is growing the fastest.

Right now it is about 361 feet across – or the length of a football field.

‘Even though Wink No. 1 collapsed in 1980, its neighboring areas are still subsiding,’ say the authors, ‘and the sinkhole continues to expand.’

Read the full story.

Tags Dedman College, Jin-woo Kim, Roy M. Huffington Department of Earth Sciences, Zhong Lu

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Grist: Massive sinkholes in Texas could combine to form even massiver sinkhole

Post author By Margaret Allen
Post date June 17, 2016

“This area is heavily populated with oil and gas production equipment and installations, hazardous liquid pipelines, as well as two communities,” said study author Jin-Woo Kim in a press release. “A collapse could be catastrophic.”

Grist.org journalist Katie Herzog covered the research of SMU geophysicists Zhong Lu, professor, Shuler-Foscue Chair, and Jin-Woo Kim research scientist, both in the Roy M. Huffington Department of Earth Sciences at SMU. Herzog’s article, “Massive sinkholes in Texas could combine to form even massiver sinkhole,” published June 15, 2016.

The research was supported by the U.S. Geological Survey Land Remote Sensing Program, the NASA Earth Surface & Interior Program, and the Shuler-Foscue Endowment at Southern Methodist University.

Read the full story.

EXCERPT:

By Katie Herzog
Grist.org
Welcome to West Texas, where sometimes the ground just opens up under your feet.

Two existing sinkholes — one in the adorably named town of Wink, the other in the absurdly named town of Kermit — are about a mile away from each other, but data suggests they might be expanding. Researchers from Southern Methodist University analyzed radar images of the area and found some hints of movement in the surrounding ground. If the sinkholes keep growing, it’s possible they will merge into one supermassive sinkhole.

And that would be a big problem indeed.

“This area is heavily populated with oil and gas production equipment and installations, hazardous liquid pipelines, as well as two communities,” said study author Jin-Woo Kim in a press release. “A collapse could be catastrophic.”

Sinkholes are not uncommon in this part of West Texas, thanks to the area’s prolific oil and gas industries. These particular sinkholes, however, are large even by Texas standards: The hole in Wink, which formed in 1980, is 361 feet across — or the length of a football field — and its neighbor in Kermit varies between 600 and 900 feet across. Both are over 100 feet deep.

Sinkholes occur when water dissolves bedrock over time, and then — sometimes suddenly — the ground collapses. They can be just a few feet across, or, like these ones, big enough to hold buildings. (A 2013 sinkhole opened up under the National Corvette Museum in Bowling Green, Ky., and swallowed eight classic cars.) And while sinkholes can form naturally, they are also created by human activity like oil and gas extraction.

Read the full story.

Follow SMU Research on Twitter, @smuresearch.

Tags Dedman College, Jin-woo Kim, Roy M. Huffington Department of Earth Sciences, Zhong Lu

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Geohazard: Giant sinkholes near West Texas oil patch towns are growing — as new ones lurk

Post author By Margaret Allen
Post date June 13, 2016

Satellite radar images reveal ground movement of infamous sinkholes near Wink, Texas; suggest the two existing holes are expanding, and new ones are forming as nearby subsidence occurs at an alarming rate.

Residents of Wink and neighboring Kermit have grown accustomed to the two giant sinkholes that sit between their small West Texas towns.

But now radar images taken of the sinkholes by an orbiting space satellite reveal big changes may be on the horizon.

A new study by geophysicists at Southern Methodist University, Dallas, finds the massive sinkholes are unstable, with the ground around them subsiding, suggesting the holes could pose a bigger hazard sometime in the future.

The two sinkholes — about a mile apart — appear to be expanding. Additionally, areas around the existing sinkholes are unstable, with large areas of subsidence detected via satellite radar remote sensing.

That leaves the possibility that new sinkholes, or one giant sinkhole, may form, said geophysicists and study co-authors Zhong Lu, professor, Shuler-Foscue Chair, and Jin-Woo Kim research scientist, in the Roy M. Huffington Department of Earth Sciences at SMU.

“This area is heavily populated with oil and gas production equipment and installations, hazardous liquid pipelines, as well as two communities. The intrusion of freshwater to underground can dissolve the interbedded salt layers and accelerate the sinkhole collapse,” said Kim, who leads the SMU geophysical team reporting the findings. “A collapse could be catastrophic. Following our study, we are collecting more high-resolution satellite data over the sinkholes and neighboring regions to monitor further development and collapse.”

The research was supported by the U.S. Geological Survey Land Remote Sensing Program, the NASA Earth Surface & Interior Program, and the Shuler-Foscue Endowment at Southern Methodist University.

Unstable ground linked to rising, falling groundwater
The sinkholes were originally caused by the area’s prolific oil and gas extraction, which peaked from 1926 to 1964. Wink Sink No. 1, near the Hendricks oil well 10-A, opened in 1980. Wink Sink No. 2, near Gulf WS-8 supply well, opened 22 years later in 2002.

It appears the area’s unstable ground now is linked to changing groundwater levels and dissolving minerals, say the scientists. A deep-seated salt bed underlies the area, part of the massive oil-rich Permian Basin of West Texas and southeastern New Mexico.

With the new data, the SMU geophysicists found a high correlation between groundwater level in the underlying aquifer and further sinking of the surface area during the summer months, influenced by successive roof failures in underlying cavities.

Satellite images and groundwater records indicate that when groundwater levels rise, the ground lifts. But the presence of that same groundwater then speeds the dissolving of the underground salt, which then causes the ground surface to subside.

Everything’s bigger in Texas, and the Wink sinkholes are no exception
Officials have fenced off the two sinkholes near Wink, a town of about 940 people, and Kermit, a town of about 6,000 people. The giant holes are notable features on the area’s vast plains, which are dotted mostly with oil pump jacks, storage facilities, occasional brush and mesquite trees.

Based on modeling of satellite image datasets, SMU’s researchers report that Wink Sink No. 1, which is closer to the town of Kermit, appears to be the most unstable. The smaller hole of the two, it has grown to 361 feet (110 meters) across — the length of a football field.

“Even though Wink No. 1 collapsed in 1980, its neighboring areas are still subsiding,” say the authors, “and the sinkhole continues to expand.” An oval-shaped deformation circling the sinkhole measures three-tenths of a mile (500 meters) wide and is subsiding up to 1.6 inches (4 centimeters) a year.

Wink Sink No. 2, which is nine-tenths of a mile south of No. 1 and which sits closer to the town of Wink, is the larger of the sinkholes. It varies from 670 feet to 900 feet across.

Wink No. 2 is not experiencing as much subsidence as Wink No. 1. However, its eastern side is collapsing and eroding westward at a rate of up to 1.2 inches (3 centimeters) a year.

“Wink No. 2 exhibits depression associated with the ongoing expansion of the underground cavity,” the authors report.

Some ground that doesn’t even border the edges of the two sinkholes is also subsiding, the scientists observed. An area more than half a mile (1 kilometer) northeast of No. 2 sank at a rate of 1.6 inches (4 centimeters) in just four months.

Ground northeast of sinkholes is subsiding, suggesting new ones forming
The largest rate of ground subsidence is not at either sinkhole, but at an area about seven-tenths of a mile (1.2 kilometers) northeast of No. 2. Ground there is subsiding at a rate of more than 5 inches (13 centimeters) a year.

It’s aerial extent, the researchers report, has also enlarged over the past eight years when a previous survey was done.

“The enlarged deformation could be an alarming precursor to the potential future development of hazards in the vicinity,” said the authors.

Additionally, ground along a road traveled by oil field vehicles, about a quarter mile (400 meters) directly north of No. 2, is subsiding about 1.2 inches (3 centimeters) a year.

Ground’s movement detected with radar technique
The satellite radar datasets were collected over five months between April 2015 and August 2015. With them, the geophysicists observed both two-dimension east-west deformation of the sinkholes, as well as vertical deformation.

The SMU scientists used a technique called interferometric synthetic aperture radar, or InSAR for short, to detect changes that aren’t visible to the naked eye.

“From 435 miles above the Earth’s surface, this InSAR technique allows us to measure inch-level subsidence on the ground. This is a monumental human achievement, and scientists will not stop endeavoring to improve this technique for more precise measurements,” said Lu, who is world-renowned for leading scientists in InSAR applications. Lu is a member of the Science Definition Team for the dedicated U.S. and Indian NASA-ISRO InSAR mission, set for launch in 2020 to study hazards and global environmental change.

Simply put, Sentinel-1A bounces a radar signal off the earth, then records the signal as it bounces back, delivering measurements. The measurements allow geophysicists to determine the distance from the satellite to the ground, revealing how features on the Earth’s surface change over time.

“Sinkhole formation has previously been unpredictable, but satellite remote sensing provides a great means to detect the expansion of the current sinkholes and possible development of new sinkholes,” said Kim. “Monitoring the sinkholes and modeling the rate of change can help predict potential sinkhole development.”

Sentinel-1A data were obtained from Sentinels Scientific Data Hub – Copernicus. Groundwater well data came from the Texas Water Development Board. — Margaret Allen, SMU

Tags Jin-woo Kim, Roy M. Huffington Department of Earth Sciences, Zhong Lu

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Wildfire on warming planet requires adaptive capacity at local, national, int’l scales

Post author By Margaret Allen
Post date June 1, 2016

In some parts of the world, “fire adaptive communities” have learned to live compatibly with wildfire — in some cases for centuries or millennia.

Industrialized nations that view wildfire as the enemy have much to learn from people in some parts of the world who have learned to live compatibly with wildfire, says a team of fire research scientists.

The interdisciplinary team say there is much to be learned from these “fire-adaptive communities” and they are calling on policy makers to tap that knowledge, particularly in the wake of global warming.

Such a move is critical as climate change makes some landscapes where fire isn’t the norm even more prone to fire, say the scientists in a new report published in a special issue of the Philosophical Transactions of the Royal Society B.

“We tend to treat modern fire problems as unique, and new to our planet,” said fire anthropologist Christopher Roos, Southern Methodist University, Dallas, lead author of the report. “As a result, we have missed the opportunity to recognize the successful properties of communities that have a high capacity to adapt to living in flammable landscapes — in some cases for centuries or millennia.“

One such society is the ethnically Basque communities in the French Western Pyrenees, who practice fire management to maintain seasonally flammable grassland, shrub and woodland patches for forage and grazing animals. But the practice is slowly being lost as young people leave farming.

Additionally, Aboriginal people in the grasslands of Western Australia use fire as part of their traditional hunting practices. Children begin burning at a very young age, and the everyday practice is passed down. These fires improve hunting successes but also reduce the impact of drought on the size and ecological severity of lightning fires.

Social institutions support individual benefits, preserve common good
Fire-adaptive communities have social institutions in place that support individual benefits from fire-maintained landscapes while preserving the common good, said Roos, whose fire research includes long-term archaeological and ecological partnerships with the Pueblo of Jemez in New Mexico.

“These institutions have been shaped by long-histories with wildfire, appropriate fire-use, and the development of social mechanisms to adjudicate conflicts of interest,” said Roos, an associate professor in the SMU Department of Anthropology. “There is a wealth of tried and tested information that should be considered in designing local fire management.”

The authors note that globally, a large number of people use fire as a tool to sustain livelihoods in ways that have been handed down across many generations. These include indigenous Australians and North Americans, South Asian forest dwellers, European farmers, and also hunters, farmers and herders in tropical savannahs.

Global Warming will likely bring new fire problems, more flammable landscapes
Global Warming will likely bring new fire problems, such as making some landscapes more flammable, Roos said. More effort will be required to balance conflicting fire management practices between adjacent cultures. Currently most fire-related research tends to be undertaken by physical or biological scientists from Europe, the United States and Australia. Often the research treats fire challenges as exclusively contemporary phenomena for which history is either absent or irrelevant.

“We need national policy that recognizes these dynamic challenges and that will support local solutions and traditional fire knowledge, while providing ways to disseminate scientific information about fire,” Roos said.

The authors point out that one of the greatest policy challenges of fire on a warming planet are the international consequences of smoke plumes and potential positive feedbacks on climate through carbon emissions. Most infamously, wildfire smoke plumes have had extraordinary health impacts during Southeast Asian “haze” events, which result in increased hospitalization and mortality in the region.

Not all fire is a disaster; we must learn to live with and manage fire
Carbon emissions from wildfires can be as much as 40 percent of fossil fuel emissions in any given year over the last decade. Although only deforestation fires and land conversion are a net carbon source to the atmosphere, the contribution of wildfires to global carbon emissions is non-trivial and should be a formal component of international climate dialogs.

“It is important to emphasize that not all fire is a disaster and we must learn how to both live with as well as manage fire,” said co-author Andrew Scott, earth sciences professor at Royal Holloway University of London.

The report, “Living on a flammable planet: interdisciplinary, cross-scalar and varied cultural lessons, prospects and challenges,” was published May 23, 2016 by The Royal Society, the U.K.’s independent scientific academy.

Authors call for holistic study of fire on Earth
The authors are from the United States, Great Britain, Canada, Australia, South Africa and Spain. The synthesis emerged from four days of international meetings sponsored by the Royal Society – the first of its kind for fire sciences.

The authors advocate for greater collaboration among researchers studying all aspects of fire.

Pyrogeography — the holistic study of fire on Earth , “may be one way to provide unity to the varied fire research programs across the globe,” the authors write.

“Fire researchers across disciplines from engineering, the natural sciences, social sciences and the humanities need to develop a common language to create a holistic wildfire science,” said Roos. “The magnitude of the wildfire challenges we face on a warming planet will demand greater collaboration and integration across disciplines, but our job won’t be done unless we are also able to translate our research for policymakers, land managers, and the general public.”

Other co-authors on the scientific paper include Andrew C. Scott, Claire M. Belcher, William G. Chaloner, Jonathan Aylen, Rebecca Bliege Bird, Michael R. Coughlan, Bart R. Johnson, Fay H. Johnston, Julia McMorrow, Toddi Steelman, and the Fire and Mankind Discussion Group. — Southern Methodist University

Tags Christopher I. Roos, Dedman College, SMU Department of Anthropology

Earth & Climate Fossils & Ruins Plants & Animals Researcher news SMU In The News

Dallas Morning News: North Texas dino had tough armor, keen sense of smell

Post author By Margaret Allen
Post date May 31, 2016

Jacobs said large nostrils that look “like a trumpet bell” and wide air passages helped Pawpawsaurus smell predators, look for food or find mates.

Dallas Morning News journalist Charles Scudder covered the research of SMU Earth Sciences Professor Louis L. Jacobs in a Guide Live article “North Texas dino had tough armor, keen sense of smell.”

The Dallas Morning News article published May 27, 2016.

Pawpawsaurus campbelli is the prehistoric cousin of the well-known armored dinosaur Ankylosaurus, famous for a hard knobby layer of bone across its back and a football-sized club on its tail.

Jacobs is president of SMU’s Institute for the Study of Earth and Man.

Read the full story.

EXCERPT:

By Charles Scudder
Dallas Morning News
A prehistoric skull found 24 years ago by a teenager in Fort Worth is now helping scientists understand the brain functions of a North Texas native. Pawpawsaurus campbelli lived 100 million years ago and was identified in 1996 by Yuong-Nam Lee, then a doctoral student at Southern Methodist University.

Lee and Louis Jacobs, a paleontologist at SMU, have co-authored a new paper that used CT imaging to study the brain of Pawpawsaurus. It’s the first time we’ve seen inside the Pawpawsaurus skull, as few studies have been done on the endocranial anatomy — scientist-speak for brain and skull — of its biological family.

This North Texas dino is named for the Paw Paw Formation, a geological feature where fossils are found in Texas. It lived on the shores of an inland sea that stretched from the Gulf coast to the Arctic. Think the Narrow Sea from Game of Thrones. Dallas is somewhere around Valyria. Arizona is Dorne.

Pawpawsaurus was a herbivore with armored plates on its back and eyelids, but without the clubbed tail characteristic of its younger cousin, Ankylosaurus. It didn’t have the stable vision of Ankylosaurus that helped it wield the clubbed tail. And although Pawpawsaurus had impressive sensory ability compared to its contemporaries, it was still less-evolved than Ankylosaurus.

Read the full story.

Tags Dedman College, Louis L. Jacobs, Roy M. Huffington Department of Earth Sciences

Earth & Climate Fossils & Ruins Plants & Animals Researcher news SMU In The News

Live Science: Dino Senses: Ankylosaurus Cousin Had a Super Sniffer

Post author By Margaret Allen
Post date May 26, 2016

Louis Jacobs is co-author of a new analysis of the Cretaceous dinosaur Pawpawsaurus based on the first CT scans ever taken of the dinosaur’s skull.

Science journalist Laura Geggel covered the research of SMU Earth Sciences Professor Louis L. Jacobs in her article “Dino Senses: Ankylosaurus Cousin Had a Super Sniffer.”

Pawpawsaurus campbelli is the prehistoric cousin of the well-known armored dinosaur Ankylosaurus, famous for a hard knobby layer of bone across its back and a football-sized club on its tail.

Jacobs is president of SMU’s Institute for the Study of Earth and Man.

Read the full story.

EXCERPT:

By Laura Geggel
Live Science
The armored cousin of the Ankylosaurus dinosaur didn’t have a football-size club on its tail, but it did have a super sense of smell, said scientists who examined its skull.

The Cretaceous-age Pawpawsaurus campbelli walked on all fours and lived in ancient Texas about 100 million years ago, the researchers said. It was an earlier version, so to speak, of the heavily armored Ankylosaurus, which lived about 35 million years later, they said.

But even without an impressive tail club, P. campbelli wasn’t totally defenseless. It sported armored plates on its back and eyelids. A computerized tomography (CT) scan of its braincase also suggests that the dinosaur had an excellent sense of smell for finding prey and avoiding predators.

“CT imaging has allowed us to delve into the intricacies of the brains of extinct animals, especially dinosaurs, to unlock secrets of their ways of life,” study co-author Louis Jacobs, a vertebrate paleontologist at Southern Methodist University in Dallas, Texas, said in a statement.

P. campbelli could have outsniffed other primitive dinosaur predators, including Ceratosaurus, a bipedal, meat-eating dinosaur with blade-like teeth and a horn on its snoutthat lived during the Jurassic period, the researchers said.

CT scans suggest that P. campbelli’s sense of smell — calculated by comparing the size of the brain’s olfactory bulb to the cerebral hemisphere — is somewhat less powerful than that of Ankylosaurus, said study lead researcher Ariana Paulina-Carabajal, a vertebrate paleontologist at the Biodiversity and Environment Research Institute (CONICET-INIBIOMA) in San Carlos de Bariloche, Argentina.

“Although both [P. campbelli and Ankylosaurus] have high ratios when compared with most carnivorous dinosaurs,” she said, “they are exceeded only by carcharodontosaurids and tyrannosaurids.”

Read the full story.

Tags Dedman College, Louis L. Jacobs, Roy M. Huffington Department of Earth Sciences

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Early armored dino from Texas lacked cousin’s club-tail weapon, but had a nose for danger

Post author By Margaret Allen
Post date May 23, 2016

Pawpawsaurus’s hearing wasn’t keen, and it lacked the infamous tail club of Ankylosaurus. But first-ever CT scans of Pawpawsaurus’s skull indicate the dino’s saving grace from predators may have been an acute sense of smell.

Well-known armored dinosaur Ankylosaurus is famous for a hard knobby layer of bone across its back and a football-sized club on its tail for wielding against meat-eating enemies.

It’s prehistoric cousin, Pawpawsaurus campbelli, was not so lucky. Pawpawsaurus was an earlier version of armored dinosaurs but not as well equipped to fight off meat-eaters, according to a new study, said vertebrate paleontologist Louis Jacobs, Southern Methodist University, Dallas. Jacobs is co-author of a new analysis of Pawpawsaurus based on the first CT scans ever taken of the dinosaur’s skull.

A Texas native, Pawpawsaurus lived 100 million years ago during the Cretaceous Period, making its home along the shores of an inland sea that split North America from Texas northward to the Arctic Sea.

Like Ankylosaurus, Pawpawsaurus had armored plate across its back and on its eyelids. But unlike Ankylosaurus, Pawpawsaurus didn’t have the signature club tail that was capable of knocking the knees out from under a large predator.

Ankylosaurus lived about 35 million years after Pawpawsaurus, around 66 million years ago toward the end of the Cretaceous. During the course of its evolution, ankylosaurids developed the club tail, and bone structure in its skull that improved its sense of smell and allowed it to hear a broader range of sounds. “Stable gaze” also emerged, which helped Ankylosaurus balance while wielding its clubbed tail.

“CT imaging has allowed us to delve into the intricacies of the brains of extinct animals, especially dinosaurs, to unlock secrets of their ways of life,” said Jacobs, a professor in the SMU Roy M. Huffington Department of Earth Sciences.

While Pawpawsaurus’s sense of smell was inferior to Ankylosaurus, it was still sharper than some primitive dinosaur predators such as Ceratosaurus, said vertebrate paleontologist Ariana Paulina-Carabajal, first author on the study.

“Pawpawsaurus in particular, and the group it belonged to — Nodosauridae — had no flocculus, a structure of the brain involved with motor skills, no club tail, and a reduced nasal cavity and portion of the inner ear when compared with the other family of ankylosaurs,” said Paulina-Carabajal, researcher for the Biodiversity and Environment Research Institute (CONICET-INIBIOMA), San Carlos de Bariloche, Argentina. “But its sense of smell was very important, as it probably relied on that to look for food, find mates and avoid or flee predators.”

Most dinosaurs don’t have bony ridges in their nasal cavities to guide airflow, but ankylosaurs are unique in that they do.

“We can observe the complete nasal cavity morphology with the CT scans,” Paulina-Carabajal said. “The CT scans revealed an enlarged nasal cavity compared to dinosaurs other than ankylosaurians. That may have helped Pawpawsaurus bellow out a lower range of vocalizations, improved its sense of smell, and cooled the inflow of air to regulate the temperature of blood flowing into the brain.”

First CT scans shed light on Pawpawsaurus’s sensory tools
Pawpawsaurus is more primitive than the younger derived versions of the dinosaur that evolved later, Jacobs said, although both walked on all fours and held their heads low to the ground.

“So we don’t know if their sense of smell also evolved and improved even more,” Jacobs said. “But we do suspect that scenting the environment was useful for a creature’s survival, and the sense of smell is fairly widely distributed among plant eaters and meat eaters alike.”

The team’s measurements and conclusions are reported in the journal PLosONE in the article “Endocranial Morphology of the Primitive Nodosaurid Dinosaur Pawpawsaurus campbelli from the Early Cretaceous of North America.” It is published online at PLosONE.

The skull was identified in 1996 by Yuong-Nam Lee, Seoul National University, Korea, a co-author on the paper, who was then a doctoral student under Jacobs.

The team’s discoveries emerged from Computed Tomography (CT) scans of the braincase of Pawpawsaurus campbelli’s skull. Pawpawsaurus belongs to one of the least explored clades of dinosaurs when it comes to endocranial anatomy — the spaces in the skull housing the brain.

The Pawpawsaurus skull was discovered 24 years ago by 19-year-old Cameron Campbell in the PawPaw Formation of Tarrant County near Dallas. Conventional analysis of the skull was carried out years ago to identify it as a never-before-seen nodosaurid ankylosaur. However, these are the first CT scans of Pawpawsaurus’s skull because it’s only been in recent years that fossils have been widely explored with X-rays.

In humans, a medical CT will scan the body to “see inside” with X-rays and capture a 3-D picture of the bones, blood vessels and soft tissue. In fossils, a much stronger dose of radiation than can be tolerated by humans is applied to fossils to capture 3-D images of the interior structure.

From the scans, paleontologists can then digitally reconstruct the brain and inner ear using special software.

“Once we have the 3D model, we can describe and measure all its different regions,” Paulina-Carabajal said. “We can then compare that to existing reptile brains and their senses of hearing and smell. Hearing, for example, can be determined from the size of the lagena, the region of the inner ear that perceives sounds.”

The size of the lagena in Pawpawsaurus suggests a sense of hearing similar to that of living crocodiles, she said.

Olfactory acuity, the sense of smell, is calculated from the size ratio of the olfactory bulb of the brain and the cerebral hemisphere.

“In Pawpawsaurus, the olfactory ratio is somewhat lower than it is in Ankyloxaurus, although both have high ratios when compared with most carnivorous dinosarus,” Paulina-Carabajal said. “They are exceeded only by carcharodontosaurids and tyrannosaurids. The olfactory ratios of ankylosaurs in general are more or less similar to those calculated by other authors for the living crocodile.”

The research was funded by the Agencia Nacional de Promoción Científica y Tecnológica (Argentina), Seoul National University, and SMU’s Institute for the Study of Earth and Man. — Margaret Allen, SMU

Tags Dedman College, Institute for the Study of Earth and Man, Louis L. Jacobs, Roy M. Huffington Department of Earth Sciences

Earth & Climate Energy & Matter Researcher news SMU In The News Technology

Dallas Morning News: Fracking-related activities have caused majority of recent Texas earthquakes

Post author By Margaret Allen
Post date May 17, 2016

A new study Texas seismology researchers finds that humans have been causing earthquakes not just in North Texas but throughout the state for nearly 100 years.

$earthquake, causes, SMU, oil, fracking, seismology$

Science journalist Anna Kuchment with The Dallas Morning News covered the research of SMU seismologists on the historical record of North Texas earthquakes and their causes.

The SMU seismology team on May 18 published online new evidence of human involvement in earthquakes since the 1920s in the journal Seismological Research Letters. The study found that human-caused earthquakes have been present since at least 1925, and widespread throughout the state. While they are tied to oil and gas operations, the specific production techniques behind these quakes have differed over the decades, according to Cliff Frohlich, Heather DeShon, Brian Stump, Chris Hayward, Mathew J. Hornbach and Jacob I. Walter.

Read the full story.

EXCERPT:

By Anna Kuchment
Dallas Morning News
Despite mounting evidence that oil and gas activity has triggered all of the recent earthquakes in Dallas and Fort Worth, Texas regulators have consistently questioned the link. Now a new study by University of Texas researchers argues that humans have been causing earthquakes not just in North Texas but throughout the state for nearly 100 years.

“The public thinks these started in 2008, but nothing could be further from the truth,” said Cliff Frohlich, a senior research scientist at UT-Austin and lead author of the new study.

The paper, to be published Wednesday in the journal Seismological Research Letters, concludes that activities associated with petroleum production “almost certainly” or “probably” set off 59 percent of earthquakes across the state between 1975 and 2015, including the recent earthquakes in Irving and Dallas. Another 28 percent were “possibly” triggered by oil and gas activities. Scientists deemed only 13 percent of the quakes to be natural.

A spokesperson for the Railroad Commission of Texas, which regulates the oil and gas industry, dismissed the study’s methods as “arbitrary,” but an expert at the U.S. Geological Survey said the study offers important new information that could affect the agency’s future threat assessments for Texas.

“The Commission will continue to use objective, credible scientific study as the basis for our regulatory and rulemaking functions,” Ramona Nye, a spokeswoman for the Railroad Commission, wrote in an email after she and her colleagues reviewed an embargoed copy of the paper. “However this new study acknowledges the basis for its conclusions are purely subjective in nature and in fact, admits its categorization of seismic events to be arbitrary.”

Frohlich and colleagues at UT and at Southern Methodist University argue in the paper that state regulators have been slow to acknowledge the link between industrial practices and ground shaking. Oklahoma, which experienced 890 earthquakes of magnitude 3 and above last year compared with Texas’ 21, has recognized the connection and ordered operators to slash the volume of wastewater from oil and gas production that they pump into wells. Studies by academic scientists and those at the USGS have shown that pressure from high-volume wastewater injections has disturbed faults in Oklahoma, Texas, Kansas, Arkansas and a handful of other states, creating earthquakes.

The Railroad Commission has taken some similar steps, Nye wrote. In November 2014 the commission tightened its rules for disposal wells. Since then, it has received 51 disposal well applications. Of these, 22 permits were issued with special conditions, such as requirements to reduce daily maximum injection volumes and pressure and to record volumes and pressures daily as opposed to monthly.

Following a 4-magnitude earthquake near Venus and Mansfield last year, the commission asked one operator to plug its well to a shallower depth, Nye added, presumably to lower the risk that it would disturb a deep fault. Texas’ man-made earthquakes date to the early days of the oil and gas industry, the new study reports.

The first man-made quake struck in 1925 in the Goose Creek oil field along the Gulf Coast east of Houston. Humble Oil, a precursor of Exxon, had extracted so much oil that the ground sank and caused houses to shake and dishes to crash to the floor.

Read the full story.

Follow SMU Research on Twitter, @smuresearch.

Tags Brian W. Stump, Chris Hayward, Heather R. DeShon, Matthew J. Hornbach

Earth & Climate Energy & Matter Researcher news Technology

Study: Humans have been causing earthquakes in Texas since the 1920s

Post author By Margaret Allen
Post date May 17, 2016

Since 2008 the rate of Texas earthquakes greater than magnitude 3 has increased from about two per year to 12 per year, say the authors.

Earthquakes triggered by human activity have been happening in Texas since at least 1925, and they have been widespread throughout the state ever since, according to a new historical review of the evidence publishing online May 18 in Seismological Research Letters.

The earthquakes are caused by oil and gas operations, but the specific production techniques behind these quakes have differed over the decades, according to Cliff Frohlich, the study’s lead author, and co-authors Heather DeShon, Brian Stump, Chris Hayward, Mathew J. Hornbach and Jacob I. Walter.

Frohlich is senior research scientist and associate director at the Institute for Geophysics at the University of Texas at Austin. DeShon, Stump, Hayward and Hornbach are seismologists in the Roy M. Huffington Department of Earth Sciences, Southern Methodist University, Dallas. Walter is at the University of Texas at Austin.

Frohlich said the evidence presented in the SRL paper should lay to rest the idea that there is no substantial proof for human-caused earthquakes in Texas, as some state officials have claimed as recently as 2015.

At the same time, he said, the study doesn’t single out any one or two industry practices that could be managed or avoided to stop these kinds of earthquakes from occurring. “I think we were all looking for what I call the silver bullet, supposing we can find out what kinds of practices were causing the induced earthquakes, to advise companies or regulators,” he notes. “But that silver bullet isn’t here.”

The researchers write in the article “A Historical Overview of Induced Earthquakes in Texas” that since 2008, the rate of Texas earthquakes greater than magnitude 3 has increased from about two per year to 12 per year. This change appears to stem from an increase in earthquakes occurring within 1-3 kilometers of petroleum production wastewater disposal wells where water is injected at a high monthly rate, they note.

Some of these more recent earthquakes include the Dallas-Fort Worth International Airport sequence between 2008 and 2013; the May 2012 Timpson earthquake; and the earthquake sequence near Azle that began in 2013.

The researchers suspected that induced seismicity might have a lengthy and geographically widespread history in Texas.

“For me, the surprise was that oil field practices have changed so much over the years, and that probably affects the kinds of earthquakes that were happening at each time,” Frohlich said.

In the 1920s and 1930s, for instance, “they’d find an oilfield, and hundreds of wells would be drilled, and they’d suck oil out of the ground as fast as they could, and there would be slumps” that shook the earth as the volume of oil underground was rapidly extracted, he said.

When those fields were mostly depleted, in the 1940s through the 1970s, petroleum operations “started being more aggressive about trying to drive oil by water flooding” and the huge amounts of water pumped into the ground contributed to seismic activity, said Frohlich.

In the past decade, enhanced oil and gas recovery methods have produced considerable amounts of wastewater that is disposed by injection back into the ground through special wells, triggering nearby earthquakes. Most earthquakes linked to this type of wastewater disposal in Texas are smaller (less than magnitude 3) than those in Oklahoma, the study concludes.

The difference may lie in the types of oil operations in each state, Frohlich said. The northeast Texas injection earthquakes occur near high-injection rate wells that dispose of water produced in hydrofracturing operations, while much of the Oklahoma wastewater is produced during conventional oil production and injected deep into the underlying sedimentary rock.

For the moment, there have been no magnitude 3 or larger Texas earthquakes that can be linked directly to the specific process of hydrofracturing or fracking itself, such as have been felt in Canada, the scientists concluded.

The researchers used a five-question test to identify induced earthquakes in the Texas historical records. The questions cover how close in time and space earthquakes and petroleum operations are, whether the earthquake center is at a relatively shallow depth (indicating a human rather than natural trigger); whether there are known or suspected faults nearby that might support an earthquake or ease the way for fluid movement, and whether published scientific reports support a human cause for the earthquake.

In 2015, the Texas legislature funded a program that would install 22 additional seismic monitoring stations to add to the state’s existing 17 permanent stations, with the hopes of building out a statewide monitoring network that could provide more consistent and objective data on induced earthquakes.

Seismological Research Letters is a publication of the Seismological Society of America. — Seismological Research Letters

Tags Brian W. Stump, Chris Hayward, Heather R. DeShon, Matthew J. Hornbach

Earth & Climate Fossils & Ruins Plants & Animals Researcher news SMU In The News

Live Science: Fearsome Dinosaur-Age ‘Hammerhead’ Reptile Ate … Plants?

Post author By Margaret Allen
Post date May 10, 2016

SMU paleontologist Louis Jacobs quoted by Live Science for article on prehistoric plant-eating reptile

Science journalist Laura Geggel tapped the expertise of SMU Earth Sciences Professor Louis L. Jacobs for a recent article about a prehistoric plant-eating reptile.

A professor in Dedman College‘s Roy M. Huffington Department of Earth Sciences, Jacobs is a world-renowned vertebrate paleontologist.

He joined SMU’s faculty in 1983 and in 2012 was honored by the 7,200-member Science Teachers Association of Texas with their prestigious Skoog Cup for his significant contributions to advance quality science education.

Jacobs is president of SMU’s Institute for the Study of Earth and Man.

Read the full story.

EXCERPT:

By Laura Geggel
Live Science
Despite its rows and rows of chisel- and needle-like teeth, a newly described prehistoric marine reptile wasn’t a fearsome predator but rather an herbivorous giant that acted like a lawnmower for the sea, a new study finds.

The crocodile-size reptile lived about 242 million years ago, during the Middle Triassic period. Researchers discovered the first specimen in 2014 in southern China, but because it was poorly preserved, they reported that it had a beak like a flamingo’s.

Now, two newly discovered specimens show that the beast was far more bizarre: It sported a hammerhead-shaped snout that it likely used to graze on plants lining the ocean floor, the researchers said. It’s also the earliest herbivorous marine reptile on record by about 8 million years, they said. [The 12 Weirdest Animal Discoveries]

“I haven’t seen anything like it before,” said study co-researcher Olivier Rieppel, the Rowe family curator of evolutionary biology at The Field Museum of Natural History in Chicago.

Weird reptile
The reptile’s name — Atopodentatus unicus — hints at its weird anatomy. In Latin, the genus and species names translate to “unique strangely toothed,” the researchers said. The newly analyzed specimens show that the creature had a mouthful of chisel-shaped teeth — one row on the upper jaw and two rows on the lower jaw.

“The remaining parts of the jaw [are filled with] densely packed needle-shaped teeth forming a mesh,” the researchers wrote in the study, published online today (May 6) in the journal Science Advances. This mesh likely helped A. unicus collect plant material, much like a baleen whale catches krill, said Louis Jacobs, a vertebrate paleontologist at Southern Methodist University in Texas who was not involved in the study.

The chisel-like teeth probably acted as a rake and trimmer, helping A. unicus scrape and dislodge plants from the seafloor, Jacobs said. Next, the reptile likely sucked in a mouthful of water, letting bits of plants get stuck in the mesh formed by its thin, needle-like teeth, he said.

“Then, they squish the water out of their mouth, and those little teeth along the sides of the jaw and on the roof of the mouth strain out all of the plant bits,” Jacobs told Live Science. “That’s an amazing way to feed. I’d like to do that myself.”

Read the full story.

Follow SMU Research on Twitter, @smuresearch.

For more SMU research see www.smuresearch.com.

Tags Dedman College, Louis L. Jacobs, Roy M. Huffington Department of Earth Sciences

Earth & Climate Energy & Matter Researcher news SMU In The News Technology

Dallas Morning News: Could Texas’ dirty coal power plants be replaced by geothermal systems?

Post author By Margaret Allen
Post date April 28, 2016

“We all care about the earth,” said Maria Richards, SMU geothermal lab coordinator, in welcoming the attendees. “We are applying knowledge that is applying hope.”

Biz Beat Blog reporter Jeffrey Weiss at The Dallas Morning News covered the 2016 SMU Geothermal Conference, “Power Plays: Geothermal Energy in Oil and Gas Fields.”

The conference was April 25-26 on the SMU campus in Dallas. The eighth international conference focused on using the oilfield as a base for alternative energy production through the capture of waste heat and fluids.

The geothermal technology that is the primary focus of the conference takes advantage of an existing resource frequently considered a nuisance – wastewater produced by oil and gas wells during extraction.

As a well ages it will typically produce more water and less oil or gas over time, which raises the cost of production. Where the produced wastewater is hot enough, and the water flow rate is sufficient, specially designed turbines can draw geothermal energy from the wastewater.

The SMU Geothermal Lab team members are leaders of academic data sources for exploration and assessment of existing and potential geothermal resources.

SMU scientists developed the Geothermal Map of North America and built one of the primary nodes of the National Geothermal Data System (NGDS) for temperature and oil/gas data. Their research efforts include over 50 years of continuous thermal data collection and is viewed by the community as an important first-stage resource used in determining the potential for geothermal energy production in the United States.

The SMU Geothermal Lab has been the recipient of approximately $10 million in research grants from a variety of sources, including the Department of Energy, the National Science Foundation, the Texas State Energy Conservation Office, Google.org and private industry.

Read the full story.

EXCERPT:

By Jeffrey Weiss
Dallas Morning News
For Texas electricity customers, geothermal energy is pretty much an afterthought. But some scientists — and even some people in the oil and gas business — say that heat from deep underground may become a significant source of power.

At least, that’s the message at a conference held today at Southern Methodist University, hosted by the school’s geothermal laboratory. The event pulled together an unusual mix: Academics, oil company bosses, people hawking heat-transfer equipment, geothermal experts and a few environmentalists.

This was the eighth such conference held at SMU since 2006. Those who have been to several agreed that the biggest difference over time is that the presentations have shifted from blue-sky theory to some data from working projects.

Perhaps the loudest applause for the day was when Will Gosnold of the University of North Dakota ended his talk about a demonstration project with a slide of an email saying it had started generating electricity today.

Another presenter suggested that geothermal power could be an economically sensible replacement for existing coal-fired power plants, particularly if the existing power plants and their transmission lines are near coal mines. That’s the case in Texas.

Susan Petty, president of Seattle-based AltaRock Energy, told the group that many older coal plants will be unable to meet clean-air requirements and will need replacing in the next few years. Waste water used in coal mines could be injected into wells where natural heat would make the water hot enough to drive geothermal power generators, she said.

Read the full story.

Tags Dedman College, Maria Richards, Roy M. Huffington Department of Earth Sciences, SMU Geothermal Laboratory

Earth & Climate Energy & Matter Slideshows Student researchers Videos

Nearby massive star explosion 30 million years ago equaled brightness of 100 million suns

Post author By Margaret Allen
Post date April 26, 2016

Analysis of exploding star’s light curve and color spectrum reveal spectacular demise of one of the closest supernova to Earth in recent years; its parent star was so big it’s radius was 200 times larger than our sun

A giant star that exploded 30 million years ago in a galaxy near Earth had a radius prior to going supernova that was 200 times larger than our sun, according to astrophysicists at Southern Methodist University, Dallas.

The sudden blast hurled material outward from the star at a speed of 10,000 kilometers a second. That’s equivalent to 36 million kilometers an hour or 22.4 million miles an hour, said SMU physicist Govinda Dhungana, lead author on the new analysis.

The comprehensive analysis of the exploding star’s light curve and color spectrum have revealed new information about the existence and sudden death of supernovae in general, many aspects of which have long baffled scientists.

“There are so many characteristics we can derive from the early data,” Dhungana said. “This was a big massive star, burning tremendous fuel. When it finally reached a point its core couldn’t support the gravitational pull inward, suddenly it collapsed and then exploded.”

The massive explosion was one of the closest to Earth in recent years, visible as a point of light in the night sky starting July 24, 2013, said Robert Kehoe, SMU physics professor, who leads SMU’s astrophysics team.

The explosion, termed by astronomers Supernova 2013ej, in a galaxy near our Milky Way was equal in energy output to the simultaneous brightness of 100 million of the Earth’s suns.

The star was one of billions in the spiral galaxy M74 in the constellation Pisces.

Considered close by supernova standards, SN 2013ej was in fact so far away that light from the explosion took 30 million years to reach Earth. At that distance, even such a large explosion was only visible by telescopes.

Dhungana and colleagues were able to explore SN 2013ej via a rare collection of extensive data from seven ground-based telescopes and NASA’s Swift satellite.

The data span a time period prior to appearance of the supernova in July 2013 until more than 450 days after.

The team measured the supernova’s evolving temperature, its mass, its radius, the abundance of a variety of chemical elements in its explosion and debris and its distance from Earth. They also estimated the time of the shock breakout, the bright flash from the shockwave of the explosion.

The star’s original mass was about 15 times that of our sun, Dhungana said. Its temperature was a hot 12,000 Kelvin (approximately 22,000 degrees Fahrenheit) on the tenth day after the explosion, steadily cooling until it reached 4,500 Kelvin after 50 days. The sun’s surface is 5,800 Kelvin, while the Earth’s core is estimated to be about 6,000 Kelvin.

The new measurements are published online here in the May 2016 issue of The Astrophysical Journal, “Extensive spectroscopy and photometry of the Type IIP Supernova 2013j.”

Shedding new light on supernovae, mysterious objects of our universe
Supernovae occur throughout the universe, but they are not fully understood. Scientists don’t directly observe the explosions but instead detect changes in emerging light as material is hurled from the exploding star in the seconds and days after the blast.

Telescopes such as SMU’s robotic ROTSE-IIIb telescope at McDonald Observatory in Texas, watch our sky and pick up the light as a point of brightening light. Others, such as the Hobby Eberly telescope, also at McDonald, observe a spectrum.

SN 2013ej is M74’s third supernova in just 10 years. That is quite frequent compared to our Milky Way, which has had a scant one supernova observed over the past 400 years. NASA estimates that the M74 galaxy consists of 100 billion stars.

M74 is one of only a few dozen galaxies first cataloged by the astronomer Charles Messier in the late 1700s. It has a spiral structure — also the Milky Way’s apparent shape — indicating it is still undergoing star formation, as opposed to being an elliptical galaxy in which new stars no longer form.

It’s possible that planets were orbiting SN 2013ej’s progenitor star prior to it going supernova, in which case those objects would have been obliterated by the blast, Kehoe said.

“If you were nearby, you wouldn’t know there was a problem beforehand, because at the surface you can’t see the core heating up and collapsing,” Kehoe said. “Then suddenly it explodes — and you’re toast.”

Distances to nearby galaxies help determine cosmic distance ladder
Scientists remain unsure whether supernovae leave behind a black hole or a neutron star like a giant atomic nucleus the size of a city.

“The core collapse and how it produces the explosion is particularly tricky,” Kehoe said. “Part of what makes SN 2013ej so interesting is that astronomers are able to compare a variety of models to better understand what is happening. Using some of this information, we are also able to calculate the distance to this object. This allows us a new type of object with which to study the larger universe, and maybe someday dark energy.”

Being 30 million light years away, SN 2013ej was a relatively nearby extragalactic event, according to Jozsef Vinko, astrophysicist at Konkoly Observatory and University of Szeged in Hungary.

“Distances to nearby galaxies play a significant role in establishing the so-called cosmic distance ladder, where each rung is a galaxy at a known distance.”

Vinko provided important data from telescopes at Konkoly Observatory and Hungary’s Baja Observatory and carried out distance measurement analysis on SN 2013ej.

“Nearby supernovae are especially important,” Vinko said. “Paradoxically, we know the distances to the nearest galaxies less certainly than to the more distant ones. In this particular case we were able to combine the extensive datasets of SN 2013ej with those of another supernova, SN 2002ap, both of which occurred in M74, to suppress the uncertainty of their common distance derived from those data.”

Supernova spectrum analysis is like taking a core sample
While stars appear to be static objects that exist indefinitely, in reality they are primarily a burning ball, fueled by the fusion of elements, including hydrogen and helium into heavier elements. As they exhaust lighter elements, they must contract in the core and heat up to burn heavier elements. Over time, they fuse the various chemical elements of the periodic table, proceeding from lightest to heaviest. Initially they fuse helium into carbon, nitrogen and oxygen. Those elements then fuel the fusion of progressively heavier elements such as sulfur, argon, chlorine and potassium.

“Studying the spectrum of a supernova over time is like taking a core sample,” Kehoe said. “The calcium in our bones, for example, was cooked in a star. A star’s nuclear fusion is always forging heavier and heavier elements. At the beginning of the universe there was only hydrogen and helium. The other elements were made in stars and in supernovae. The last product to get created is iron, which is an element that is so heavy it can’t be burned as fuel.”

Dhungana’s spectrum analysis of SN 2013ej revealed many elements, including hydrogen, helium, calcium, titanium, barium, sodium and iron.

“When we have as many spectra as we have for this supernova at different times,” Kehoe added, “we are able to look deeper and deeper into the original star, sort of like an X-ray or a CAT scan.”

SN 2013ej’s short-lived existence was just tens of millions of years
Analysis of SN 2013ej’s spectrum from ultraviolet through infrared indicates light from the explosion reached Earth July 23, 2013. It was discovered July 25, 2013 by the Katzman Automatic Imaging Telescope at California’s Lick Observatory. A look back at images captured by SMU’s ROTSE-IIIb showed that SMU’s robotic telescope detected the supernova several hours earlier, Dhungana said.

“These observations were able to show a rapidly brightening supernova that started just 20 hours beforehand,” he said. “The start of the supernova, termed ‘shock breakout,’ corresponds to the moment when the internal explosion crashes through the star’s outer layers.”

Like many others, SN 2013ej was a Type II supernova. That is a massive star still undergoing nuclear fusion. Once iron is fused, the fuel runs out, causing the core to collapse. Within a quarter second the star explodes.

Supernovae have death and birth written all over them
Massive stars typically have a shorter life span than smaller ones.

“SN 2013ej probably lived tens of millions of years,” Kehoe said. “In universe time, that’s the blink of an eye. It’s not very long-lived at all compared to our sun, which will live billions of years. Even though these stars are bigger and have a lot more fuel, they burn it really fast, so they just get hotter and hotter until they just gobble up the matter and burn it.”

For most of its brief life, SN 2013ej would probably have burned hydrogen, which then fused to helium, burning for a few hundred thousand years, then perhaps carbon and oxygen for a few hundred days, calcium for a few months and silicon for several days.

“Supernovae have death and birth written all over them,” Kehoe said. “Not only do they create the elements we are made of, but the shockwave that goes out from the explosion — that’s where our solar system comes from.”

Outflowing material slams into clouds of material in interstellar space, causing it to collapse and form a solar system.

“The heavy elements made in the supernova and its parent star are those which comprise the bulk of terrestrial planets, like Earth, and are necessary for life,” Kehoe said.

Besides physicists in the SMU Department of Physics, researchers on the project also included scientists from the University of Szeged, Szeged, Hungary; the University of Texas, Austin, Texas; Konkoly Observatory, Budapest, Hungary; and the University of California, Berkeley, Calif. — Margaret Allen

Tags Dedman College, Govinda Dhungana, Robert Kehoe, SMU Department of Physics

Earth & Climate Energy & Matter Learning & Education Technology

SMU “Power Plays” conference to promote development of oil and gas fields for geothermal energy production

Post author By Margaret Allen
Post date April 22, 2016

“Power Plays,” on Dallas campus April 25-26, is SMU Geothermal Laboratory’s eighth international energy conference and workshop

SMU’s renowned SMU Geothermal Laboratory will host its eighth international energy conference April 25-26 on the Dallas campus, focused on using the oilfield as a base for alternative energy production through the capture of waste heat and fluids.

In addition to oil and gas field geothermal projects, experts will discuss coal plant conversion for geothermal production, the intersection of geothermal energy and desalination, and large-scale direct use of the energy source produced by the internal heat of the earth.

“Power Plays” begins with an opening reception and poster session from 5:30 p.m. – 8 p.m. Monday, April 25, followed by a daylong program of speakers and presentations Tuesday, April 26. Conference details are available here. Walk-up registration is available at the conference site, the Collins Center at 3150 Binkley Avenue, Dallas, 75205.

The technology that is the primary focus of the conference takes advantage of an existing resource frequently considered a nuisance – wastewater produced by oil and gas wells during extraction. As a well ages it will typically produce more water and less oil or gas over time, which raises the cost of production. Where the produced wastewater is hot enough, and the water flow rate is sufficient, specially designed turbines can draw geothermal energy from the wastewater.

That “bonus” geothermal energy can be used to either generate electricity to operate the oil field equipment and lower the cost of production, sell the electricity directly to the power grid or — more likely — to nearby industry users seeking a highly secure electrical source.

“Initial demonstration projects have taught us a great deal about the complexities of transitioning an oil or gas well to geothermal energy production,” said Maria Richards, director of the SMU Geothermal Lab. “Collaboration continues between the oil and gas industry and the geothermal community, and this conference is the place to hear about the technology, business models and legislation that all play a role in developing geothermal resources. We are confident that geothermal energy production will one day be the norm for an aging oil and gas field.”

The appearance of AltaRock Energy’s Susan Petty to discuss “Transitioning Coal to Geothermal: Baseload Renewable Power With No CO2” will be the first examination of this type of geothermal production at the SMU conference, Richards said, adding that she is pleased to see geothermal technology being combined with other energy systems, from large scale solar operations to electricity generated by on-site flare gas.

“The small surface footprint of geothermal energy makes it a desirable player for developers looking to maximize all possible resources on their site,” Richards said.

SMU’s Geothermal Lab team members are leaders of academic data sources for exploration and assessment of existing and potential geothermal resources. SMU scientists developed the Geothermal Map of North America and built one of the primary nodes of the National Geothermal Data System (NGDS) for temperature and oil/gas data. Their research efforts include over 50 years of continuous thermal data collection and is viewed by the community as an important first-stage resource used in determining the potential for geothermal energy production in the United States.

Tags Dedman College, Geothermal Map of North America, Maria Richards, Roy M. Huffington Department of Earth Sciences, SMU Geothermal Laboratory

Earth & Climate Fossils & Ruins Researcher news

SMU seismology team response to March 28, 2016 U.S. Geological Survey hazard forecasts

Post author By Margaret Allen
Post date March 28, 2016

Southern Methodist University preliminary earthquake catalog for the Irving-Dallas earthquake swarm. The SMU North Texas seismic network has recorded over 600 earthquakes ranging from magnitude 0.0-3.6 in the Dallas-Irving region. Earthquakes recorded prior to Jan. 17, 2015 have a higher location uncertainty than events recorded after the complete seismic network was installed. Current seismic sensors recording the sequence are shown as gray symbols; note that some sensors are outside of the map boundaries. US Geological Survey NetQuakes data (squares) can be viewed online. Earthquake symbol size is scaled by magnitude and color coded by date of occurrence. The map is provided as part of the ongoing collaboration between SMU, the USGS, Irving, Dallas, and neighboring cities. The SMU preliminary earthquake locations and magnitudes have not been published in the peer-reviewed scientific literature and are subject to change. Prepared March 22, 2016.

The United States Geological Survey (USGS) today released maps showing potential ground shaking from induced and natural earthquakes, including forecasts for the DFW metropolitan area. The North Texas Earthquake Study at Southern Methodist University provided data, and SMU scientists co-authored peer-reviewed publications cited in the report. The new earthquake ground shaking forecasts are a reminder to the cities and residents in the region that the occurrence of earthquakes increases the earthquake hazard in the area, regardless of cause. Residents should be prepared to experience ground shaking, just as we are prepared to experience tornadoes, hail storms and other events.

FAQs
1. How did SMU research contribute to the USGS report?
SMU and partners currently operate a 30-station seismic network across North Texas, and stations are denser around the ongoing earthquake sequences (Azle-Reno, Irving-Dallas, and Venus-Johnson County). We focus on cataloging the ongoing seismicity over a wider range of magnitudes than the national USGS catalog documents, conducting detailed source studies to understand the physics of faulting, and identifying and mapping faults currently or potentially generating seismicity. We also study cause with the aim of potentially mitigating the increased seismicity rates experienced in North Texas since 2008. Finally, in order to provide improved local estimates of both the size of the earthquakes as well as their source characteristics, we are analyzing the locally recorded waveforms to produce empirical estimates of how ground shaking decays with range for each of the instrumented source regions. These empirical decay rates may provide data for refining the ground shaking forecasts.

The SMU research in its entirety helps inform appropriate parameter ranges for earthquake hazard mapping, and we therefore collaborate and cooperate with the USGS, as was done in preparation for the 2016 report being released Monday, and with city, state and federal agencies.

Peer-reviewed publications by SMU scientists and collaborators were used to classify most North Texas earthquakes as induced. These publications include those on the 2008-2009 DFW sequence (Frohlich et al., 2011), the 2009 Cleburne earthquakes (Justinic et al., 2012), and the 2013-2014 Azle-Reno earthquakes (Hornbach et al., 2015). Dr. Cliff Frohlich (UT-Austin) has published on induced earthquakes in Johnson County near the eventual 2015 Venus earthquake (Frohlich, 2012). Peer-reviewed publications regarding cause for the Irving-Dallas sequence had not been accepted for publication and the earthquakes were left classified as “undetermined cause” in the 2016 Induced Earthquake Hazard Mapping Project and treated as natural earthquakes in the probabilistic calculations for ground motion.

2. What can and should DFW Metroplex residents do with this information?
The new earthquake ground shaking forecasts are a reminder to the cities and residents in the region that the occurrence of earthquakes increases the earthquake hazard in the area, regardless of cause. Residents should be prepared to experience ground shaking, just as we are prepared to experience tornadoes, hail storms and other events. People should remember to Drop, Cover and Hold On during an earthquake and not to evacuate a building until after shaking has stopped. Brick façade damage is possible under low to mid-intensity shaking, and you are most likely to be injured by falling objects and broken windows than by building collapse at the levels of ground shaking outlined in the USGS report.

We encourage residents to explore online resources on preparedness, such as the resources made available through FEMA and the USGS. Following the seven steps to earthquake safety is always a good idea: http://earthquakecountry.org/sevensteps/.

3. Have you been recording earthquakes in the Dallas-Irving area or has that sequence stopped?
The Irving-Dallas earthquakes began in April 2014 with the largest events occurring in January 2015. Earthquake rates in the Dallas-Irving area have been highly variable. While the rate has decreased over the last few months, we have seen similar short-term decreases in the past, and therefore the rate change should not be over-interpreted.

4. What is the earthquake magnitude equivalent of the USGS ground shaking forecast?
Earthquake magnitude is not the same as ground shaking intensity. Hazard maps are used to forecast ground shaking intensities, regardless of the magnitude of the earthquake that creates the motion. Ground motion, and hence hazard, depends on the earthquake size, distance from the epicenter, local geology, etc. Online resources equating intensity to magnitude are “rule of thumb” and should not be interpreted as directly relating the ground shaking forecasts to earthquake magnitude in the DFW area. Risk calculations use the known properties of building and infrastructure to estimate the probability of damage based on the underlying hazard assessment from ground shaking intensities.

Magnitude tells you the overall size of the earthquake. A single earthquake has one magnitude.

Intensity tells you what the earthquake shaking was like at a particular location. A single earthquake produces a range of intensities that depend on the location. The USGS “Did you feel it?” for the 2015 Irving-Dallas M3.6 illustrates this point. The Modified Mercalli Scale is described further here: http://earthquake.usgs.gov/learn/topics/mercalli.php. — Kim Cobb

Follow SMUResearch.com on twitter at @smuresearch.

SMU has an uplink facility located on campus for live TV, radio, or online interviews. To speak with an SMU expert or book an SMU guest in the studio, call SMU News & Communications at 214-768-7650.

Tags Beatrice Magnani, Brian W. Stump, Chris Hayward, Dedman College, Heather R. DeShon, Matthew J. Hornbach, Roy M. Huffington Department of Earth Sciences

Earth & Climate Energy & Matter Researcher news SMU In The News

Daily Mail: Earth’s moon threw a ‘wobbly’ after it formed: Lunar poles wandered 125 MILES as volcanic bubbles threw them off balance

Post author By Margaret Allen
Post date March 25, 2016

Science reporter Richard Gray with The Daily Mail covered the research of SMU planetary scientist and research assistant professor Matthew Siegler and a team of scientists who discovered the moon wandered off its axis billions of years ago due to a shift in its mass most likely caused by volcanic activity.

The article, “Earth’s moon threw a ‘wobbly’ after it formed: Lunar poles wandered 125 MILES as volcanic bubbles threw them off balance,” published March 23. A report on the discovery of the rare event was published today in Nature: that Earth’s moon slowly moved from its original axis roughly 3 billion years ago.

Read the full story.

EXCERPT:

By Richard Gray
The Daily Mail
They are among the coldest places in the solar system, covered in deposits of ice that are thought to be billions of years old.

But the moon’s north and south poles may have shifted during its 4.53 billion-year history, according to evidence uncovered in a new study.

A team of astrophysicists claims to have found distinct matching patches of ice at either pole that indicate the tilt of the Earth’s satellite has changed as it has aged.

They said this may have occurred as the interior of the moon cooled and solidified, while other areas bubbled upwards, altering the spin of the rocky world.

The authors explained that volcanic activity in an area known as the Procellarum region around three billion years ago threw the entire moon off balance, causing it to shift its axis by around six degrees.

This caused the moon’s poles to move by around 125 miles (201km) over the course of a billion years.

Dr Matt Siegler, a planetary scientist at the Southern Methodist University in Dallas, who was part of the team to make the discovery, said: ‘Billions of years ago, heating within the Moon’s interior caused the face we see to shift upward as the pole physically changed positions.

‘It would be as if Earth’s axis relocated from Antarctica to Australia. As the pole moved, the Man on the Moon turned his nose up at the Earth,’ Siegler said.

Dr Siegler and his colleagues used data gathered by Nasa’s Lunar Reconnaissance Orbitor which has mapped the hydrogen deposits around the moon’s poles.

They found the polar hydrogen reserves, which are thought to be in the form of water ice in craters, are spread over distinct but matching patterns on either side of the moon.

The researchers said this suggests the lunar spin axis must have shifted, causing the polar regions to become displaced.
This left a permanent record painted out on the surface in ice.

Relatively few planetary bodies are thought to have shifted their axis after forming.

The Earth, Mars, Saturn’s moon Enceladus and Jupiter’s moon Europa are the only others known to have done so.

On Earth, polar wander is thought to have happened as the continental plates have shifted the mass of the planet while on Mars it occurred due to heavy volcanic region.

Read the full story.

Follow SMUResearch.com on twitter at @smuresearch.

SMU is a nationally ranked private university in Dallas founded 100 years ago. Today, SMU enrolls nearly 11,000 students who benefit from the academic opportunities and international reach of seven degree-granting schools. For more information see www.smu.edu.

SMU has an uplink facility located on campus for live TV, radio, or online interviews. To speak with an SMU expert or book an SMU guest in the studio, call SMU News & Communications at 214-768-7650.

Tags Dedman College, Matthew Siegler, Roy M. Huffington Department of Earth Sciences

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Earth & Climate Energy & Matter Researcher news SMU In The News

Wired: The Moon used to spin on a different axis

Post author By Margaret Allen

Post date March 25, 2016

Wired reporter Emily Reynolds covered the research of SMU planetary scientist and research assistant professor Matthew Siegler and a team of scientists who discovered the moon wandered off its axis billions of years ago due to a shift in its mass most likely caused by volcanic activity.

The article, “The Moon used to spin on a different axis,” published March 24. A report on the discovery of the rare event was published today in Nature: that Earth’s moon slowly moved from its original axis roughly 3 billion years ago.

Read the full story.

For more information

To book a live or taped interview with Matthew Siegler in the SMU News Broadcast Studio call SMU News, 214-768-7654, or email news@smu.edu.

Related links

SMU: Matthew Siegler

Planetary Science Institute: Matthew Siegler

Web site: Matthew Siegler

Nature: “Lunar true polar wander inferred from polar hydrogen“

Roy M. Huffington Department of Earth Sciences

Dedman College of Humanities and Sciences

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NASA data leads to rare discovery: Earth’s moon wandered off axis billions of years ago

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New look at Pizarro’s conquest of Inca reveals foot soldiers were awed by empire’s grandeur

EXCERPT:

By Emily Reynolds
Wired
The Moon used to “spin on a different axis” that was subject to “polar wander,” a new study into the satellite’s early history has said.

The Planetary Science Institute study, published in Nature, highlights two regions full of hydrogen deposits near the Moon’s two poles. This, it says, suggests the presence of ice — ice that only would have survived if it had remained in permanent shadow.

“If the orientation of the Moon has changed, then the locations of the shadowed regions will also have changed,” the researchers write.

The poles “wandered”, according to the team, because of volcanic activity in the area, which would have warmed. It also would have made them less dense, causing the “wandering” of the axes.

“The Moon has a single region of the crust where radioactive elements ended up as the Moon was forming,” said Matthew Siegler, lead author of the study. “This radioactive crust acted like an oven broiler heating the mantle below.”

“This giant blob of hot mantle was lighter than cold mantle elsewhere, causing the whole Moon to move.”

The shift probably happened over three billion years ago, the team say, and would have meant the Moon showed a completely different face. Overall, the Moon shifted around six degrees over one billion years. Only a few other planetary bodies have been said to shift their axes — Earth and Mars, as well as two moons of Saturn and Jupiter.

“The same face of the Moon has not always pointed towards Earth,” said Siegler. “As the axis moved, so did the face of the Man in the Moon. He sort of turned his nose up at the Earth.”

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SMU is a nationally ranked private university in Dallas founded 100 years ago. Today, SMU enrolls nearly 11,000 students who benefit from the academic opportunities and international reach of seven degree-granting schools. For more information see www.smu.edu.

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Earth & Climate Energy & Matter Researcher news SMU In The News

Agence France-Presse in The Japan Times, Raw Story: Moon’s ‘wandering poles’ shifted long ago: study

Post author By Margaret Allen

Post date March 25, 2016

Agence France-Presse covered the research of SMU planetary scientist and research assistant professor Matthew Siegler and a team of scientists who discovered the moon wandered off its axis billions of years ago due to a shift in its mass most likely caused by volcanic activity.

The article, “Moon’s ‘wandering poles’ shifted long ago: study,” published March 24 at The Japan Times and Raw Story, among other news sites. A report on the discovery of the rare event was published today in Nature: that Earth’s moon slowly moved from its original axis roughly 3 billion years ago.

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To book a live or taped interview with Matthew Siegler in the SMU News Broadcast Studio call SMU News, 214-768-7654, or email news@smu.edu.

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SMU: Matthew Siegler

Planetary Science Institute: Matthew Siegler

Web site: Matthew Siegler

Nature: “Lunar true polar wander inferred from polar hydrogen“

Roy M. Huffington Department of Earth Sciences

Dedman College of Humanities and Sciences

More SMU Research news

NASA data leads to rare discovery: Earth’s moon wandered off axis billions of years ago

Good news! You’re likely burning more calories than you thought

New look at Pizarro’s conquest of Inca reveals foot soldiers were awed by empire’s grandeur

EXCERPT:

By Agence France Presse
Telltale patches of water ice on opposite ends of the Moon reveal that Earth’s orbiting companion once spun on a different axis, according to a study released Wednesday.

The six-degree tilt, which happened several billion years ago, was likely caused by an ancient volcanic formation on the near side of the Moon, said the study, published in Nature.

The data underlying this startling discovery has been in plain view for nearly two decades, but scientists had failed to connect the dots, one of the researchers told AFP.

“It was kind of hidden because of the way we plotted polar maps,” explained co-author James Keane, a researcher at the University of Arizona.

Two-dimensional representations create a subtle distortion, obscuring the fact that observed concentrations of ice near each pole were exactly 180 degrees apart — and thus on an axis running through the dead centre of the Moon.

“That is my pet hypothesis about why nobody thought about this before,” Keane said.

The man who finally put the top-and-bottom pieces of the lunar puzzle together was co-author Rich Miller of the University of Alabama.

Having located the largest concentrations of water ice near the current north and south poles by detecting hydrogen molecules — the “H” in “H2O” — he rotated a 3-D model to see how they would line up.

“He found a Sigma-8 correlation,” which means that the odds of it being a coincidence were about one-in-a-million, said Keane.

Read the full story.

Follow SMUResearch.com on twitter at @smuresearch.

SMU is a nationally ranked private university in Dallas founded 100 years ago. Today, SMU enrolls nearly 11,000 students who benefit from the academic opportunities and international reach of seven degree-granting schools. For more information see www.smu.edu.

SMU has an uplink facility located on campus for live TV, radio, or online interviews. To speak with an SMU expert or book an SMU guest in the studio, call SMU News & Communications at 214-768-7650.

Tags Dedman College, Matthew Siegler, Roy M. Huffington Department of Earth Sciences

Leakage in Ken Regan field could have contaminated groundwater for livestock and irrigation between 2007 and 2011

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SMU students did the important, time-consuming lab work

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Study shows hunter-gatherers used active burning to improve grazing, drive bison, long before arrival of Columbus

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Never-Before-Seen Fossils From Angola Bring a Strange Yet Familiar Ocean Into View

“One of our major concerns is background particles that can mimic the dark matter signature in our detectors.” — Jodi Cooley

A new research report, from Southern Methodist University and funded by NASA, found a “…large swath of West Texas oil patch is heaving and sinking at alarming rates.”

Ground rising and falling in region that has been ‘punctured like a pin cushion’ since the 1940s, new study finds.

Analysis indicates decades of oil production activity have destabilized localities in an area of about 4,000 square miles populated by small towns, roadways and a vast network of oil and gas pipelines and storage tanks

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SMU and other members of a scientific consortium prepare for installation of the Dark Energy Spectroscopic Instrument to survey the night sky from a mile-high mountain peak in Arizona

High rates of injection and large volumes can perturb critically stressed faults, triggering earthquakes years after wastewater wells are shut in.

New knowledge has caused us to reconsider many previous conclusions about what the universe is and how it works.

For 300 million years faults showed no activity, and then wastewater injections from oil and gas wells came along. Study authors took a different approach in the new work — they hunted for deformed faults below Texas.

The study authors took a different approach in the new work — they hunted for deformed faults below Texas.

Study by Beatrice Magnani, USGS and other SMU scientists shows recent seismicity in Fort Worth Basin occurred on faults not active for 300 million years

The initiative addresses one of the most pressing issues currently facing U.S. Gulf of Mexico fisheries management, as the iconic red snapper supports one of the most economically valuable finfish fisheries in the Gulf.

The modern link between high carbon dioxide levels and climate change didn’t appear to hold true for a time interval about 22 million years ago; but now a new study has found the link does indeed exist.

The CW33 TV visited SMU on Halloween to get a glimpse of International Dark Matter Day in action on the SMU campus.

“In the spirit of science being a pursuit open to all, we are excited to welcome all members of the SMU family to become dark matter hunters for a day.” — SMU physicist Jodi Cooley

New findings reveal the real reasons behind varying leaf sizes.

The huge variety of leaves in the plant kingdom has long been a source of wonder and fascination.

A global team of researchers, including SMU paleobotanist Bonnie Jacobs, have cracked the mystery of leaf size. The research was published Sept. 1, 2017 as a cover story in Science.

Dedman College, SMU Physics Department host Great American Solar Eclipse 2017 viewing

In this week’s Q&A, The Texas Tribune interviews Diego Román, assistant professor of teaching and learning at Southern Methodist University.

A massive particle detector a mile underground is the key to unlocking the secrets of a beam of neutrinos that will be shot beneath the Earth from Chicago to South Dakota.

A new giant bird-like dinosaur discovered in China has been named for SMU paleontologist Louis L. Jacobs, Corythoraptor jacobsi, by the scientists who identified the new oviraptorid.

The heated energy sources were discovered in the Mountain State by examining previously overlooked oil and gas data.

Discovery may someday allow farmers to grow crops in climates where they currently won’t grow and allows scientists to make a subtle, targeted mutation to a specific native plant protein

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A “major step forward” toward the goal of answering the very big question: Is there life on other worlds?

This newly-discovered variable is one of only seven of its kind known in our galaxy.

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“If these sea turtles do, in fact, form a tightly knit group, evolutionarily speaking, the [African] specimen provides proof that members of that group survived the mass extinction at the end of the Cretaceous.” — Timothy Myers, SMU

Using ancient DNA, researchers have created a unique picture of how a prehistoric migration route evolved over thousands of years – revealing that it could not have been used by the first people to enter the Americas, as traditionally thought.

CT scans offer new insight into the little-understood Pawpawsaurus: One clue that led the researchers to determine that the sense of smell was Pawpawsaurus’s strongest sense was the large olfactory ratio.

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“’We could have another sink hole or two or 10 someday show up,’” (Winkler County Sheriff George) Keely says. In fact, the SMU researchers used satellite imaging to show the problem is getting worse.”

“There’s no relationship between dinosaurs and armadillos, which are mammals, but it is interesting that something that looked like an armadillo was here in Texas 100 million years before highways.” — Jacobs

New holes are also developing to join them, a satellite study shows.

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“They’re a ways off from the highway; if nobody mentions it, then nobody is interested in it,” Kermit City Manager Gloria Saenz told the New York Daily News.

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The sinkholes are a little less than a mile apart, but that distance is closing as the land directly around both holes subsides about 2 inches each year.

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‘A collapse could be catastrophic. Following our study, we are collecting more high-resolution satellite data over the sinkholes and neighboring regions to monitor further development and collapse.’

“This area is heavily populated with oil and gas production equipment and installations, hazardous liquid pipelines, as well as two communities,” said study author Jin-Woo Kim in a press release. “A collapse could be catastrophic.”

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Satellite radar images reveal ground movement of infamous sinkholes near Wink, Texas; suggest the two existing holes are expanding, and new ones are forming as nearby subsidence occurs at an alarming rate.

In some parts of the world, “fire adaptive communities” have learned to live compatibly with wildfire — in some cases for centuries or millennia.

Jacobs said large nostrils that look “like a trumpet bell” and wide air passages helped Pawpawsaurus smell predators, look for food or find mates.

Louis Jacobs is co-author of a new analysis of the Cretaceous dinosaur Pawpawsaurus based on the first CT scans ever taken of the dinosaur’s skull.

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A new study Texas seismology researchers finds that humans have been causing earthquakes not just in North Texas but throughout the state for nearly 100 years.

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