Category: Slideshows

Categories
Culture, Society & Family Fossils & Ruins Learning & Education Researcher news Slideshows SMU In The News Student researchers

One of the most significant Etruscan discoveries in decades names female goddess Uni

One of the longest Etruscan texts ever found, the inscription’s mention of Uni may indicate she was patroness of the Poggio Colla cult, with stone’s language spelling out ceremonial religious rituals

Archaeologists translating a very rare inscription on an ancient Etruscan temple stone have discovered the name Uni — an important female goddess.

The discovery indicates that Uni — a divinity of fertility and possibly a mother goddess at this particular place — may have been the titular deity worshipped at the sanctuary of Poggio Colla, a key settlement in Italy for the ancient Etruscan civilization.

The mention is part of a sacred text that is possibly the longest such Etruscan inscription ever discovered on stone, said archaeologist Gregory Warden, professor emeritus at Southern Methodist University, Dallas, main sponsor of the archaeological dig.

Scientists on the research discovered the ancient stone slab embedded as part of a temple wall at Poggio Colla, a dig where many other Etruscan objects have been found, including a ceramic fragment with the earliest birth scene in European art. That object reinforces the interpretation of a fertility cult at Poggio Colla, Warden said.

Now Etruscan language experts are studying the 500-pound slab — called a stele (STEE-lee) — to translate the text. It’s very rare to identify the god or goddess worshipped at an Etruscan sanctuary.

“The location of its discovery — a place where prestigious offerings were made — and the possible presence in the inscription of the name of Uni, as well as the care of the drafting of the text, which brings to mind the work of a stone carver who faithfully followed a model transmitted by a careful and educated scribe, suggest that the document had a dedicatory character,” said Adriano Maggiani, formerly Professor at the University of Venice and one of the scholars working to decipher the inscription.

“It is also possible that it expresses the laws of the sanctuary — a series of prescriptions related to ceremonies that would have taken place there, perhaps in connection with an altar or some other sacred space,” said Warden, co-director and principal investigator of the Mugello Valley Archaeological Project that made the discovery.

Warden said it will be easier to speak with more certainty once the archaeologists are able to completely reconstruct the text, which consists of as many as 120 characters or more. While archaeologists understand how Etruscan grammar works, and know some of its words and alphabet, they expect to discover new words never seen before, particularly since this discovery veers from others in that it’s not a funerary text.

The Mugello Valley archaeologists had planned to announce discovery of the goddess Uni at an exhibit in Florence on Aug. 27, “Scrittura e culto a Poggio Colla, un santuario etrusco nel Mugello,” and in a forthcoming article in the scholarly journal Etruscan Studies. The exhibit opening has been delayed to Sept. 2 due to the recent devastating earthquake in areas of Italy unrelated to the Poggio Colla research.

Text may specify the religious ritual for temple ceremonies dedicated to the goddess
It’s possible the text contains the dedication of the sanctuary, or some part of it, such as the temple proper, so the expectation is that it will reveal the early beliefs of a lost culture fundamental to western traditions.

The sandstone slab, which dates to the 6th century BCE and is nearly four feet tall by more than two feet wide, was discovered in the final stages of two decades of digging at Mugello Valley, which is northeast of Florence in north central Italy.

Etruscans once ruled Rome, influencing that civilization in everything from religion and government to art and architecture. A highly cultured people, Etruscans were also very religious and their belief system permeated all aspects of their culture and life.

Inscription may reveal data to understand concepts and rituals, writing and language
Permanent Etruscan inscriptions are rare, as Etruscans typically used linen cloth books or wax tablets. The texts that have been preserved are quite short and are from graves, thus funerary in nature.

“We can at this point affirm that this discovery is one of the most important Etruscan discoveries of the last few decades,” Warden said. “It’s a discovery that will provide not only valuable information about the nature of sacred practices at Poggio Colla, but also fundamental data for understanding the concepts and rituals of the Etruscans, as well as their writing and perhaps their language.”

Besides being possibly the longest Etruscan inscription on stone, it is also one of the three longest sacred texts to date.

One section of the text refers to “tinaś,” a reference to Tina, the name of the supreme deity of the Etruscans. Tina was equivalent to ancient Greece’s Zeus or Rome’s Jupiter.

Slab was once an imposing and monumental symbol of authority
The slab was discovered embedded in the foundations of a monumental temple where it had been buried for more than 2,500 years. At one time it would have been displayed as an imposing and monumental symbol of authority, said Warden, president and professor of archaeology at Franklin University Switzerland.

The text is being studied by two noted experts on the Etruscan language, including Maggiani, who is an epigrapher, and Rex Wallace, professor of classics at the University of Massachusetts Amherst, who is a comparative linguist.

A hologram of the stele will be shown at the Florence exhibit, as conservation of the stele is ongoing at the conservation laboratories of the Archaeological Superintendency in Florence. Digital documentation is being done by experts from the architecture department of the University of Florence. The sandstone is heavily abraded and chipped, so cleaning should allow scholars to read the inscription.

Other objects unearthed in the past 20 years have shed light on Etruscan worship, beliefs, gifts to divinities, and discoveries related to the daily lives of elites and non-elites, including workshops, kilns, pottery and homes. The material helps document ritual activity from the 7th century to the 2nd century BCE.

Besides SMU, other collaborating institutions at Mugello Valley Archaeological Project include Franklin and Marshall College, the University of Pennsylvania Museum of Archaeology, the Center for the Study of Ancient Italy at The University of Texas at Austin, The Open University (UK), and Franklin University Switzerland. — Margaret Allen, SMU

Categories
Earth & Climate Fossils & Ruins Slideshows Subfeature Technology

Geohazard: Giant sinkholes near West Texas oil patch towns are growing — as new ones lurk

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.”

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.

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.

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.

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

Categories
Earth & Climate Fossils & Ruins Researcher news Slideshows

Early armored dino from Texas lacked cousin’s club-tail weapon, but had a nose for danger

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

Categories
Earth & Climate Energy & Matter Slideshows Student researchers Videos

Nearby massive star explosion 30 million years ago equaled brightness of 100 million suns

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

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.

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

KERA: Thousands Of Vertebrate Paleontologists Descend On Dallas

SMU faculty and students presented research and led field trips for various sessions of the 2015 annual meeting in Dallas of the international Society of Vertebrate Paleontology.

Reporting for KERA News, North Texas’ public media news source, journalist Kat Chow covered the 2015 annual meeting in Dallas in October of the international Society of Vertebrate Paleontology.

The meeting was hosted locally by the Roy M. Huffington Department of Earth Sciences at SMU and the Perot Museum of Nature and Science in Dallas. SMU faculty and students presented research and led field trips for various SVP sessions.

Chow’s coverage also covered the research of SMU paleontologist Louis L. Jacobs, a professor in the Roy M. Huffington Department of Earth Sciences, Dedman College of Humanities and Sciences.

He carried out the study with paleontologist Anthony Fiorillo, vice president of research and collections and chief curator at the Perot Museum of Nature and Science, Dallas, and an adjunct research professor at SMU.

Jacobs and Fiorillo are co-authors of a study about the identification of new fossils from the oddball creature Desmostylia, discovered in the same waters where the popular “Deadliest Catch” TV show is filmed. The hippo-like creature ate like a vacuum cleaner and is a new genus and species of the only order of marine mammals ever to go extinct — surviving a mere 23 million years.

Desmostylians, every single species combined, lived in an interval between 33 million and 10 million years ago. Its strange columnar teeth and odd style of eating don’t occur in any other animal, Jacobs said. The new specimens — from at least four individuals — were recovered from Unalaska, an Aleutian island in the North Pacific.

The authors reported their discovery in a special volume of the international paleobiology journal, Historical Biology. The article published online Oct.1 at http://bit.ly/1PQAHZJ.

The KERA article aired and published Oct. 14, 2015.

Read the full story.

EXCERPT:

By Kat Chow
KERA News
Everything I knew about paleontology conferences, I learned from TV and “Friends.” There was that time Ross and his girlfriend were prepping for a conference in Barbados.

“By using CT scans and computer imaging, we can in a very real way bring the Mesozoic era into the 21st century,” Ross says.

In the real world, at the conference put on by the Society of Vertebrate Paleontology, the lingo isn’t so simple. Here are some of the session titles:

“A new large non-pterodactyloid pterosaur from a late-Jurassic interdunal desert environment with a neo-eolian nugget sandstone of Northeastern Utah.”

“The hemodynamics of vascular retia: Testing a hypothesis of blood pressure regulation through the artiodactyl carotid rete.”

“The effects of substrate, body position, and plasticity on the morphology of ruminant unguals.”

Louis Jacobs, a vertebrate paleontologist at Southern Methodist University, and Anthony Fiorillo, a paleontologist at Dallas’ Perot Museum, are helping organize the conference. Walking with them is like trailing a rock star — they’re inundated with fans and well-wishers.

”We specialize in animals with backbones, and how they’re preserved in the rocks, and what they mean, and what they tell us about the earth got to be the way it is,” Jacobs explains.

Read the full story.