back to top
27.8 C
New York
Friday, November 29, 2024
Home Blog Page 21

A first in fossil research: Seeds sprouting from an amber-encased pine cone

germinating fossil pine cone
germinating fossil pine cone

Oregon State University research has uncovered the first fossil evidence of a rare botanical condition known as precocious germination in which seeds sprout before leaving the fruit.

In a paper published in Historical Biology, George Poinar Jr. of the Oregon State College of Science describes a pine cone, approximately 40 million years old, encased in Baltic amber from which several embryonic stems are emerging.

“Crucial to the development of all plants, seed germination typically occurs in the ground after a seed has fallen,” said Poinar, an international expert in using plant and animal life forms preserved in amber to learn about the biology and ecology of the distant past. “We tend to associate viviparity — embryonic development while still inside the parent — with animals and forget that it does sometimes occur in plants.”

Most typically, by far, those occurrences involve angiosperms, Poinar said. Angiosperms, which directly or indirectly provide most of the food people eat, have flowers and produce seeds enclosed in fruit.

“Seed germination in fruits is fairly common in plants that lack seed dormancy, like tomatoes, peppers and grapefruit, and it happens for a variety of reasons,” he said. “But it’s rare in gymnosperms.”

Gymnosperms such as conifers produce “naked,” or non-enclosed, seeds. Precocious germination in pine cones is so rare that only one naturally occurring example of this condition, from 1965, has been described in the scientific literature, Poinar said.

“That’s part of what makes this discovery so intriguing, even beyond that it’s the first fossil record of plant viviparity involving seed germination,” he said. “I find it fascinating that the seeds in this small pine cone could start to germinate inside the cone and the sprouts could grow out so far before they perished in the resin.”

At the sprouts’ tips are needle clusters, some in bundles of five, associating the fossil with the extinct pine species Pinus cembrifolia, which was previously described from Baltic amber, Poinar said.

Pine cones in Baltic amber are not commonly found, he added. The ones that do appear are prized by collectors and because the cones’ scales are hard, they’re usually very well preserved and appear lifelike.

Viviparity in plants typically shows up in one of two ways, Poinar said. Precocious germination is the more common of the two, the other being vegetative viviparity, such as when a bulbil emerges directly from the flower head of a parent plant.

“In the case of seed viviparity in this fossil, the seeds produced embryonic stems that are quite evident in the amber,” he said. “Whether those stems, known as hypocotyls, appeared before the cone became encased in amber is unclear. However, based on their position, it appears that some growth, if not most, occurred after the pine cone fell into the resin.

“Often some activity occurs after creatures are entombed in resin, such as entrapped insects depositing eggs,” Poinar said. “Also, insect parasites sometimes flee their hosts into the resin after the latter become trapped. In the case of the pine cone, the cuticle covering the exposed portions of the shoots could have protected them from rapid entrance of the resin’s natural fixatives.”

Research on viviparity in extant gymnosperms suggests the condition could be linked to winter frosts. Light frosts would have been possible if the Baltic amber forest had a humid, warm-temperate environment as has been posited, Poinar said.

“This is the first fossil record of seed viviparity in plants but this condition probably occurred quite a bit earlier than this Eocene record,” he said. “There’s no reason why vegetative viviparity couldn’t have occurred hundreds of millions of years ago in ancient spore-bearing plants like ferns and lycopods.”

Reference:
George Poinar. Precocious germination of a pine cone in Eocene Baltic amber. Historical Biology, 2021; 1 DOI: 10.1080/08912963.2021.2001808

Note: The above post is reprinted from materials provided by Oregon State University. Original written by Steve Lundeberg.

Paleontologists debunk fossil thought to be missing link between lizards and first snakes

“In the shallows near shore, Tetrapodophis amplectus glides through a tangle of branches from the conifer Duartenia araripensis that have fallen into the water, sharing this habitat with a water bug in the family Belostomatidae and small fish (Dastilbe sp.).” Image credit: Julius Csotonyi
“In the shallows near shore, Tetrapodophis amplectus glides through a tangle of branches from the conifer Duartenia araripensis that have fallen into the water, sharing this habitat with a water bug in the family Belostomatidae and small fish (Dastilbe sp.).” Image credit: Julius Csotonyi

Filling in the links of the evolutionary chain with a fossil record of a ”snake with four legs” connecting lizards and early snakes would be a dream come true for paleontologists. But a specimen formerly thought to fit the bill is not the missing piece of the puzzle, according to a new Journal of Systematic Palaeontology study led by University of Alberta paleontologist Michael Caldwell.

“It has long been understood that snakes are members of a lineage of four-legged vertebrates that, as a result of evolutionary specializations, lost their limbs,” said Caldwell, lead author of the study and professor in the departments of biological sciences and earth and atmospheric sciences.

“Somewhere in the fossil record of ancient snakes is an ancestral form that still had four legs. It has thus long been predicted that a snake with four legs would be found as a fossil.”

Missing link discovered?

In a paper published in the journal Sciencein 2015, a team of researchers reported the discovery of what was believed to be an example of the first known four-legged snake fossil, an animal they named Tetrapodophis amplectus.

“If correctly interpreted based on the preserved anatomy, this would be a very important discovery,” said Caldwell.

Caldwell explained that the new study of Tetrapodophis revealed a number of mischaracterizations of the anatomy and morphology of the specimen — traits that initially seemed to be shared most closely with snakes, suggesting this might be the long-sought-after snake with four legs.

“There are many evolutionary questions that could be answered by finding a four-legged snake fossil, but only if it is the real deal. The major conclusion of our team is that Tetrapodophis amplectus is not in fact a snake and was misclassified,” said Caldwell. “Rather, all aspects of its anatomy are consistent with the anatomy observed in a group of extinct marine lizards from the Cretaceous period known as dolichosaurs.”

The clues to this conclusion, Caldwell noted, were hiding in the rock the fossil was extracted from.

“When the rock containing the specimen was split and it was discovered, the skeleton and skull ended up on opposite sides of the slab, with a natural mould preserving the shape of each on the opposite side,” said Caldwell. “The original study only described the skull and overlooked the natural mould, which preserved several features that make it clear that Tetrapodophis did not have the skull of a snake — not even of a primitive one.”

A controversial specimen

Although Tetrapodophis may not be the snake with four legs that paleontologists prize, it still has much to teach us, said study coauthor Tiago Simões, a former U of A PhD student, Harvard post- doctoral fellow and Brazilian paleontologist, who pointed out some of the features that make it unique.

“One of the greatest challenges of studying Tetrapodophis is that it is one of the smallest fossil squamates ever found,” said Simões. “It is comparable to the smallest squamates alive today that also have reduced limbs.”

An additional challenge to studying the Tetrapodophis is access to the specimen itself.

“There were no appropriate permits for the specimen’s original removal from Brazil and, since its original publication, it has been housed in a private collection with limited access to researchers. The situation was met with a large backlash from the scientific community,” said Simões.

“In our redescription of Tetrapodophis, we lay out the important legal status of the specimen and emphasize the necessity of its repatriation to Brazil, in accordance not only with Brazilian legislation but also international treaties and the increasing international effort to reduce the impact of colonialist practices in science.”

Reference:
Michael W. Caldwell, Tiago R. Simões, Alessandro Palci, Fernando F. Garberoglio, Robert R. Reisz, Michael S. Y. Lee, Randall L. Nydam. Tetrapodophis amplectus is not a snake: re-assessment of the osteology, phylogeny and functional morphology of an Early Cretaceous dolichosaurid lizard. Journal of Systematic Palaeontology, 2021; 1 DOI: 10.1080/14772019.2021.1983044

Note: The above post is reprinted from materials provided by Taylor & Francis Group.

Sierra Nevada range should celebrate two birthdays

Map showing the Great Basin drainage basin as defined hydrologically. (Image credit: Kmusser/Wikimedia Commons)
Map showing the Great Basin drainage basin as defined hydrologically. (Image credit: Kmusser/Wikimedia Commons)

When geologist Elizabeth Miller started mapping a fault system in Death Valley, she questioned the origin of some sedimentary rocks previously assumed to be locally derived. Now, analysis has revealed where they really came from: central Nevada, indicating that part of today’s Great Basin was the highest land in North America some 40 million to 20 million years ago.

The journey of these sediments southward in river systems draining into the ancient Pacific Ocean tells a story about the history of the Earth and the much-debated formation of the Sierra Nevada mountain range, the awe-inspiring backbone of eastern California that encompasses three national parks: Sequoia, Kings Canyon and Yosemite.

The ancestral Sierra Nevada began as a volcanic chain more than 100 million years ago, a time when dinosaurs still roamed the Earth. New work published Nov. 15 as chapters in a Geological Society of America Special Paper on the paleogeography and topography of the western U.S. suggests that the mountains later “died” — meaning they were dwarfed by a vast plateau — during a region-wide volcanic flare-up about 40 million to 20 million years ago. Then, they were “reborn” about 10 million years ago, lifting to the scenic heights we know today.

“The highest points 40 to 20 million years ago were in central Nevada. Then, basin and range faulting came along and broke it all up, and now the Sierra Nevada is the westernmost or last of those major fault blocks,” Miller said. “As a mountain range, it’s had three completely different histories.”

The findings from Miller and Jens-Erik Lund Snee, who conducted the research while a PhD student at Stanford, propose that the Continental Divide — which is typically considered to be static — went through a progressive shift eastward. The divide, which separates the watersheds that drain into the Pacific Ocean from those draining eastward, remained in the ancestral Sierra Nevada in eastern California for tens of millions of years before moving into central Nevada when the volcanism that started 40 million years ago lifted the Earth’s surface in a south-migrating wave.

The papers describe how the region-wide flare-up of volcanic activity in southern Idaho, Nevada and Utah caused the inland plateau to rise above the ancestral Sierra. That upheaval in the Earth’s mantle and crust created whole new systems of rivers, some of which carried sediment southward, forming the layers that Miller studied near Death Valley with co-author Mark Raftrey, a former graduate student.

“The material from those volcanoes made it all the way out to the Pacific side of the Sierra Nevada — that’s how we know the region in central Nevada where the eruptions occurred was higher than everything else,” said Miller, noting that previous papers charted the ancient rivers that carried the volcanic material. “Our work adds to this previous work in that we argue that the volcanism itself actually caused a big increase in the topography because there was so much hot material coming up from below the continent.”

For tens of million years after the plateau rose, the ancestral Sierra range was “merely the ramp from the high country in Nevada down to the paleo-ocean in what’s now the Central Valley,” Lund Snee said. That was also when much of the famous California gold was deposited in ancient rivers that flowed west from central Nevada out to the Central Valley. Then, beginning around 10 million years ago, the new Sierra Nevada emerged when the western U.S. was chiseled apart by basin and range faulting, which involved uplift and extension — a process that had very little to do with its earlier history, according to Miller.

“There’s been a lot of recent debate about when the Sierra Nevada came up as a mountain range, and our work is suggesting that both prevailing views are right — it’s old and also young for completely different tectonic reasons,” said Lund Snee, who is now a Mendenhall Research Fellow at the U.S. Geological Survey.

When the ancestral Sierra Nevada first arose over 100 million years ago, the mountains marked the edge of the North American continent, bordered by the Pacific Ocean to the west. East of that area, geologists have long thought the Earth’s crust thickened and became unstable, eventually causing the continent to spread apart and form today’s basin and range topography.

But Miller and Lund Snee found that the region east of the ancestral Sierra was relatively low, supported by thinner, more stable crust until the wave of volcanic eruptions 40 million to 20 million years ago lifted the plateau higher than the ancestral range. The eruptions came from dozens of Yellowstone-like supervolcano calderas in addition to hundreds of smaller volcanoes — an event that blanketed some areas with thousands of feet of lava.

The research paints a picture of the topographic evolution of the western U.S., which has been debated since the area was first explored by geologists in the 1800s and flooded by gold miners seeking fortunes in the Sierra Nevada’s western foothills. It also impacts our understanding of how plants and animals evolved and dispersed across the West; in order to understand migration, biologists need a clear grasp of landscape evolution.

The authors refined geologic maps and used radiometric dating of the minerals zircon and feldspar to gauge the timing of eruptions and changes in topography. They also revised the ages of previous estimates of elevation and climate from stable isotope analyses of calcite in sediments deposited before and after the volcanic rock.

“You need to know when things happened and how long it took things to happen to truly understand them in the geologic context,” Miller said. “It’s an evolving story, and as we pick up more pieces, the story begins to get tighter and tighter.”

The research was supported by the National Science Foundation and a Gerald J. Lieberman Fellowship.

Note: The above post is reprinted from materials provided by Stanford University. Original written by Danielle Torrent Tucker.

Seismic shockwave pattern may be redirecting earthquake damage

A ruptured fault in Searles Valley, California, after the 2019 Ridgecrest earthquakes. A study of earthquakes led by The University of Texas at Austin found that seismic shockwaves are shaped by jagged faults and the debris wedged between them. Credit: Ben Brooks/USGS
A ruptured fault in Searles Valley, California, after the 2019 Ridgecrest earthquakes. A study of earthquakes led by The University of Texas at Austin found that seismic shockwaves are shaped by jagged faults and the debris wedged between them. Credit: Ben Brooks/USGS

New research from The University of Texas at Austin could change the way scientists think about potential damage from earthquakes.

The study examined data from one of the densest seismic arrays ever deployed and found that earthquakes emit their strongest seismic shockwaves in four opposing directions. The effect, which leaves a pattern resembling a four-leaf clover, has been known for decades but never measured in such vivid detail.

Daniel Trugman, an earthquake geophysicist at the Department for Geological Sciences in the UT Jackson School of Geosciences, said that the study looked at only one type of seismic shaking caused by very small earthquakes in northern Oklahoma.

“What’s important in these results is that close to the source we’re seeing a variation in ground motion, and that’s not accounted for in any sort of hazard model,” Trugman said. He added that efforts were already underway to see how the phenomena plays out in California’s big fault systems.

The analysis was published in the September issue of Geophysical Research Letters and is based on measurements of two-dozen small earthquakes recorded by the LArge-n Seismic Survey in Oklahoma (LASSO), an array of 1,829 seismic sensors deployed for 28 days in 2016 to monitor a remote corner of the state measuring 15 by 20 miles.

When earthquakes strike, they release a thunderclap of seismic energy at many frequencies, but the actual ground shaking people feel ranges from about 1 hertz to 20 hertz. The study found that low frequency energy — about 1 to 10 hertz — shot from the fault in four directions, but barely registered outside of the four-leaf clover pattern. This is important because buildings are more vulnerable to low frequency waves. The four-leaf clover pattern wasn’t found for higher frequency waves, which travelled at equal strength in all directions, like ripples in a pond.

Co-author Victor Tsai, a geophysicist at Brown University, said that the reason the Earth shook unevenly at different frequencies might have something to do with the complex geometry of earthquake faults and the broken-up material packed between them.

“What happens when you have an earthquake is that pieces of broken rock inside the fault zone start to move around like pinballs,” he said. The jostling pieces redirect the energy randomly but at lower frequencies, seismic waves simply bypass the rough geologic mess near the fault, travelling in a nice four-leaf clover pattern just as physics predicts.

This means that on the surface, a person might feel the same shaking regardless of where they stood, but buildings — which are sensitive to low frequency waves — would feel the earthquake much more intensely within the lines of the four-leaf clover pattern.

Geophysicists have long known about this pattern; it’s taught in seismology 101. But, until now, evidence of its effect has been sparse. That’s because over large distances seismic waves are refracted regardless of frequency, smoothing out their differences and making earthquakes seem the same in all directions.

Near an earthquake’s source, however, the pattern should be distinct. That’s where the LASSO array came in. Its closely packed sensors recorded earthquakes while they were unfolding, gathering measurements from hundreds of locations in northern Oklahoma that the U.S. Geological Survey, which funded and deployed the array, made freely available online.

To test their idea about uneven shaking near faults, Trugman developed algorithms to filter the LASSO data. At low frequencies, each earthquake showed a four-leaf clover pattern of shaking; at higher frequencies there was no clear pattern, just as Tsai had predicted.

Although the tremors recorded by the LASSO array were barely perceptible, the physics that drive them should be the same for stronger quakes. The scientists have already begun examining larger faults to see whether their age or shape can change the intensity of ground motion. Their goal is to build a catalogue of earthquake zones, showing which faults can generate the strongest and most dangerous types of seismic waves.

The research was funded by the U.S. Geological Survey and the National Science Foundation. Trugman is also a researcher at the University of Texas Institute for Geophysics, a unit of the Jackson School of Geosciences.

Reference:
Daniel T. Trugman, Shanna X. Chu, Victor C. Tsai. Earthquake Source Complexity Controls the Frequency Dependence of Near‐Source Radiation Patterns. Geophysical Research Letters, 2021; 48 (17) DOI: 10.1029/2021GL095022

Note: The above post is reprinted from materials provided by University of Texas at Austin.

Bacteria may be key to sustainably extracting earth elements for tech

A lab-grown crystal of a synthetic form of the rare earth mineral, monazite, shows extensive damage to one face after exposure to bio-leaching compound generated by Gluconobacter oxydans. Credit: Credit: Brian Balta/Provided
A lab-grown crystal of a synthetic form of the rare earth mineral, monazite, shows extensive damage to one face after exposure to bio-leaching compound generated by Gluconobacter oxydans.
Credit: Credit: Brian Balta/Provided

Rare earth elements from ore are vital for modern life but refining them after mining is costly, harms the environment and mostly occurs abroad.

A new study describes a proof of principle for engineering a bacterium, Gluconobacter oxydans, that takes a big first step towards meeting skyrocketing rare earth element demand in a way that matches the cost and efficiency of traditional thermochemical extraction and refinement methods and is clean enough to meet U.S. environmental standards.

“We’re trying to come up with an environmentally friendly, low-temperature, low-pressure method for getting rare earth elements out of a rock,” said Buz Barstow, the paper’s senior author and an assistant professor of biological and environmental engineering at Cornell University.

The elements — of which there are 15 in the periodic table — are necessary for everything from computers, cell phones, screens, microphones, wind turbines, electric vehicles and conductors to radars, sonars, LED lights and rechargeable batteries.

While the U.S. once refined its own rare earth elements, that production stopped more than five decades ago. Now, refinement of these elements takes place almost entirely in other countries, particularly China.

“The majority of rare earth element production and extraction is in the hands of foreign nations,” said co-author Esteban Gazel, associate professor of earth and atmospheric sciences at Cornell. “So for the security of our country and way of life, we need to get back on track to controlling that resource.”

To meet U.S. annual needs for rare earth elements, roughly 71.5 million tonnes (~78.8 million tons) of raw ore would be required to extract 10,000 kilograms (~22,000 pounds) of elements.

Current methods rely on dissolving rock with hot sulphuric acid, followed by using organic solvents to separate very similar individual elements from each other in a solution.

“We want to figure out a way to make a bug that does that job better,” Barstow said.

G. oxydans is known for making an acid called biolixiviant that dissolves rock; the bacteria uses the acid to pull phosphates from rare earth elements. The researchers have begun to manipulate G. oxydans’ genes so it extracts the elements more efficiently.

To do so, the researchers used a technology that Barstow helped develop, called Knockout Sudoku, that allowed them to disable the 2,733 genes in G. oxydans’ genome one by one. The team curated mutants, each with a specific gene knocked out, so they could identify which genes play roles in getting elements out of rock.

“I am incredibly optimistic,” Gazel said. “We have a process here that is going to be more efficient than anything that was done before.”

Alexa Schmitz, a postdoctoral researcher in Barstow’s lab, is first author of the study, “Gluconobacter oxydans Knockout Collection Finds Improved Rare Earth Element Extraction,” published in Nature Communications.

The study was funded by the Cornell Atkinson Center for Sustainability, the Cornell Energy Systems Institute, the Burroughs Welcome Fund and the Advanced Research Projects Agency-Energy.

Reference:
Alexa M. Schmitz, Brooke Pian, Sean Medin, Matthew C. Reid, Mingming Wu, Esteban Gazel, Buz Barstow. Generation of a Gluconobacter oxydans knockout collection for improved extraction of rare earth elements. Nature Communications, 2021; 12 (1) DOI: 10.1038/s41467-021-27047-4

Note: The above post is reprinted from materials provided by Cornell University. Original written by Krishna Ramanujan, courtesy of the Cornell Chronicle.

Scientist reveals cause of lost magnetism at meteorite site

Photo courtesy Gunther Kletetschka Geologists inspect an outcrop near the sample collection site in New Mexico.
Photo courtesy Gunther Kletetschka
Geologists inspect an outcrop near the sample collection site in New Mexico.

A University of Alaska Fairbanks scientist has discovered a method for detecting and better defining meteorite impact sites that have long lost their tell-tale craters. The discovery could further the study of not only Earth’s geology but also that of other bodies in our solar system.

The key, according to work by associate research professor Gunther Kletetschka at the UAF Geophysical Institute, is in the greatly reduced level of natural remanent magnetization of rock that has been subjected to the intense forces from a meteor as it nears and then strikes the surface.

Rocks unaltered by humanmade or non-Earth forces have 2% to 3% natural remanent magnetization, meaning they consist of that quantity of magnetic mineral grains — usually magnetite or hematite or both. Kletetschka found that samples collected at the Santa Fe Impact Structure in New Mexico contained less than 0.1% magnetism.

Kletetschka determined that plasma created at the moment of impact and a change in the behavior of electrons in the rocks’ atoms are the reasons for the minimal magnetism.

Kletetschka reported his findings in a paper published Wednesday in the journal Scientific Reports.

The Santa Fe Impact Structure was discovered in 2005 and is estimated to be about 1.2 billion years old. The site consists of easily recognized shatter cones, which are rocks with fantail features and radiating fracture lines. Shatter cones are believed to only form when a rock is subjected to a high-pressure, high-velocity shock wave such as from a meteor or nuclear explosion.

Kletetschka’s work will now allow researchers to determine an impact site before shatter cones are discovered and to better define the extent of known impact sites that have lost their craters due to erosion.

“When you have an impact, it’s at a tremendous velocity,” Kletetschka said. “And as soon as there is a contact with that velocity, there is a change of the kinetic energy into heat and vapor and plasma. A lot of people understand that there is heat, maybe some melting and evaporation, but people don’t think about plasma.”

Plasma is a gas in which atoms have been broken into free-floating negative electrons and positive ions.

“We were able to detect in the rocks that a plasma was created during the impact,” he said.

Earth’s magnetic field lines penetrate everything on the planet. Magnetic stability in rocks can be knocked out temporarily by a shock wave, as they are when hitting an object with a hammer, for example. The magnetic stability in rocks returns immediately after the shock wave passes.

At Santa Fe, the meteorite’s impact sent a massive shock wave through the rocks, as expected. Kletetschka found that the shock wave altered the characteristics of atoms in the rocks by modifying the orbits of certain electrons, leading to their loss of magnetism.

The modification of the atoms would allow for a quick remagnetization of the rocks, but Kletetschka also found that the meteorite impact had weakened the magnetic field in the area. There was no way for the rocks to regain their 2% to 3% magnetism even though they had the capability to do so.

That’s because of the presence of plasma in the rocks at the impact surface and below. Presence of the plasma increased the rocks’ electrical conductivity as they converted to vapor and molten rock at the leading edge of the shock wave, temporarily weakening the ambient magnetic field.

“This plasma will shield the magnetic field away, and therefore the rock finds only a very small field, a residue,” Kletetschka said.

Kletetschka is also affiliated with Charles University in Prague, Czech Republic. Charles University students Radana Kavkova and Hakan Ucar assisted in the research.

Reference:
Gunther Kletetschka, Radana Kavkova, Hakan Ucar. Plasma shielding removes prior magnetization record from impacted rocks near Santa Fe, New Mexico. Scientific Reports, 2021; 11 (1) DOI: 10.1038/s41598-021-01451-8

Note: The above post is reprinted from materials provided by University of Alaska Fairbanks.

‘Volcanic winter’ likely contributed to ecological catastrophe 250 million years ago

Copper-rich minerals indicating widespread volcanic activity at the end-Permian mass extinction in different regions in southern China (A: Taoshujing locality; B: Lubei locality; C: Guanbachong; D: Taoshujing locality; E: Longmendong locality). The minerals are all copper sulfides, mostly Malachite--the minerals' green patches. Photo credit: H. Zhang, Nanjing Institute of Geology and Palaeontology.
Copper-rich minerals indicating widespread volcanic activity at the end-Permian mass extinction in different regions in southern China (A: Taoshujing locality; B: Lubei locality; C: Guanbachong; D: Taoshujing locality; E: Longmendong locality). The minerals are all copper sulfides, mostly Malachite–the minerals’ green patches. Photo credit: H. Zhang, Nanjing Institute of Geology and Palaeontology.

A team of scientists has identified an additional force that likely contributed to a mass extinction event 250 million years ago. Its analysis of minerals in southern China indicate that volcano eruptions produced a “volcanic winter” that drastically lowered earth’s temperatures — a change that added to the environmental effects resulting from other phenomena at the time.

The research, which appears in the journal Science Advances, examined the end-Permian mass extinction (EPME), which was the most severe extinction event in the past 500 million years, wiping out 80 to 90 percent of species on land and in the sea.

“As we look closer at the geologic record at the time of the great extinction, we are finding that the end-Permian global environmental disaster may have had multiple causes among marine and non-marine species,” says Michael Rampino, a professor in New York University’s Department of Biology and one of the authors of the paper.

For decades, scientists have investigated what could have caused this global ecological catastrophe, with many pointing to the spread of vast floods of lava across what is known as the Siberian Traps — a large region of volcanic rock in the Russian province of Siberia. These eruptions caused environmental stresses, including severe global warming from volcanic releases of carbon dioxide and related reduction in oxygenation of ocean waters — the latter causing the suffocation of marine life.

The team for the Science Advances work, composed of more than two dozen researchers, including scientists from China’s Nanjing University and Guangzhou Institute of Geochemistry as well as Smithsonian Institution’s National Museum of Natural History and Montclair State University, considered other factors that may have contributed to the end of the Permian Period, which stretched from 300 million to 250 million years ago.

Specifically, they found mineral and related deposits on land in the south China region — notably copper and mercury — whose age coincided with the end-Permian mass extinction in non-marine localities. Specifically, these deposits were marked by anomalies in their composition likely due to sulfur-rich emissions from nearby volcanic eruptions — they were covered by layers of volcanic ash.

“Sulfuric acid atmospheric aerosols produced by the eruptions may have been the cause of rapid global cooling of several degrees, prior to the severe warming seen across the end-Permian mass-extinction interval,” explains Rampino.

The team’s findings suggested that the Siberian Traps eruptions were not the sole cause of the end-Permian mass extinction, and that the environmental effects of the eruptions in South China, and elsewhere, may have played a vital role in the disappearance of dozens of species.

Reference:
Hua Zhang, Feifei Zhang, Jiu-bin Chen, Douglas H. Erwin, Drew D. Syverson, Pei Ni, Michael Rampino, Zhe Chi, Yao-feng Cai, Lei Xiang, Wei-qiang Li, Sheng-Ao Liu, Ru-cheng Wang, Xiang-dong Wang, Zhuo Feng, Hou-min Li, Ting Zhang, Hong-ming Cai, Wang Zheng, Ying Cui, Xiang-kun Zhu, Zeng-qian Hou, Fu-yuan Wu, Yi-gang Xu, Noah Planavsky, Shu-zhong Shen. Felsic volcanism as a factor driving the end-Permian mass extinction. Science Advances, 2021; 7 (47) DOI: 10.1126/sciadv.abh1390

Note: The above post is reprinted from materials provided by New York University.

‘Cold bone’: Researchers discover first dinosaur species that lived on Greenland 214 million years ago

Living reconstruction of Issi saaneq / Photo: Victor Beccari
Living reconstruction of Issi saaneq / Photo: Victor Beccari

The two-legged dinosaur Issi saaneq lived about 214 million years ago in what is now Greenland. It was a medium-sized, long-necked herbivore and a predecessor of the sauropods, the largest land animals ever to live. It was discovered by an international team of researchers from Portugal, Denmark and Germany, including the Martin Luther University Halle-Wittenberg (MLU). The name of the new dinosaur pays tribute to Greenland’s Inuit language and means “cold bone.” The team reports on its discovery in the journal Diversity.

The initial remains of the dinosaur — two well-preserved skulls — were first unearthed in 1994 during an excavation in East Greenland by palaeontologists from Harvard University. One of the specimens was originally thought to be from a Plateosaurus, a well-known long-necked dinosaur that lived in Germany, France and Switzerland during the Triassic Period. Only a few finds from East Greenland have been prepared and thoroughly documented. “It is exciting to discover a close relative of the well-known Plateosaurus, hundreds of which have already been found here in Germany,” says co-author Dr Oliver Wings from MLU.

The team performed a micro-CT scan of the bones, which enabled them to create digital 3D models of the internal structures and the bones still covered by sediment. “The anatomy of the two skulls is unique in many respects, for example in the shape and proportions of the bones. These specimens certainly belong to a new species,” says lead author Victor Beccari, who carried out the analyses at NOVA University Lisbon.

The plant-eating dinosaur Issi saaneq lived around 214 million years ago during the Late Triassic Period. It was at this time that the supercontinent Pangaea broke apart and the Atlantic Ocean began forming. “At the time, the Earth was experiencing climate changes that enabled the first plant-eating dinosaurs to reach Europe and beyond,” explains Professor Lars Clemmensen from the University of Copenhagen.

The two skulls of the new species come from a juvenile and an almost adult individual. Apart from the size, the differences in bone structure are minor and only relate to proportions. The new Greenlandic dinosaur differs from all other sauropodomorphs discovered so far, however it does have similarities with dinosaurs found in Brazil, such as the Macrocollum and Unaysaurus, which are almost 15 million years older. Together with the Plateosaurus from Germany, they form the group of plateosaurids: relatively graceful bipeds that reached lengths of 3 to 10 metres.

The new findings are the first evidence of a distinct Greenlandic dinosaur species, which not only adds to the diverse range of dinosaurs from the Late Triassic (235-201 million years ago) but also allows us to better understand the evolutionary pathways and timeline of the iconic group of sauropods that inhabited the Earth for nearly 150 million years.

Once the scientific work is completed, the fossils will be transferred to the Natural History Museum of Denmark.

Reference:
Victor Beccari, Octávio Mateus, Oliver Wings, Jesper Milàn, Lars B. Clemmensen. Issi saaneq gen. et sp. nov.—A New Sauropodomorph Dinosaur from the Late Triassic (Norian) of Jameson Land, Central East Greenland. Diversity, 2021; 13 (11): 561 DOI: 10.3390/d13110561

Note: The above post is reprinted from materials provided by Martin-Luther-Universität Halle-Wittenberg.

Humans hastened the extinction of the woolly mammoth

Woolly mammoth illustration Mauricio Antón © 2008 Public Library of Science
Woolly mammoth illustration Mauricio Antón © 2008 Public Library of Science

New research shows that humans had a significant role in the extinction of woolly mammoths in Eurasia, occurring thousands of years later than previously thought.

An international team of scientists led by researchers from the University of Adelaide and University of Copenhagen, has revealed a 20,000-year pathway to extinction for the woolly mammoth.

“Our research shows that humans were a crucial and chronic driver of population declines of woolly mammoths, having an essential role in the timing and location of their extinction,” said lead author Associate Professor Damien Fordham from the University of Adelaide’s Environment Institute.

“Using computer models, fossils and ancient DNA we have identified the very mechanisms and threats that were integral in the initial decline and later extinction of the woolly mammoth.”

Signatures of past changes in the distribution and demography of woolly mammoths identified from fossils and ancient DNA show that people hastened the extinction of woolly mammoths by up to 4,000 years in some regions.

“We know that humans exploited woolly mammoths for meat, skins, bones and ivory. However, until now it has been difficult to disentangle the exact roles that climate warming and human hunting had on its extinction,” said Associate Professor Fordham.

The study also shows that woolly mammoths are likely to have survived in the Arctic for thousands of years longer than previously thought, existing in small areas of habitat with suitable climatic conditions and low densities of humans.

“Our finding of long-term persistence in Eurasia independently confirms recently published environmental DNA evidence that shows that woolly mammoths were roaming around Siberia 5,000 years ago,” said Associate Professor Jeremey Austin from the University of Adelaide’s Australian Centre for Ancient DNA.

Associate Professor David Nogues-Bravo from the University of Copenhagen was a co-author of the study which is published in the journal Ecology Letters.

“Our analyses strengthens and better resolves the case for human impacts as a driver of population declines and range collapses of megafauna in Eurasia during the late Pleistocene,” he said.

“It also refutes a prevalent theory that climate change alone decimated woolly mammoth populations and that the role of humans was limited to hunters delivering the coup de grâce”.

“And shows that species extinctions are usually the result of complex interactions between threatening processes.”

The researchers emphasise that the pathway to extinction for the woolly mammoth was long and lasting, starting many millennia before the final extinction event.

Reference:
Damien A. Fordham, Stuart C. Brown, H. Reşit Akçakaya, Barry W. Brook, Sean Haythorne, Andrea Manica, Kevin T. Shoemaker, Jeremy J. Austin, Benjamin Blonder, Julia Pilowsky, Carsten Rahbek, David Nogues‐Bravo. Process‐explicit models reveal pathway to extinction for woolly mammoth using pattern‐oriented validation. Ecology Letters, 2021; DOI: 10.1111/ele.13911

Note: The above post is reprinted from materials provided by University of Adelaide. Original written by Crispin Savage.

Tooth Fast, Tooth Curious?

 Long neck, long tail, tiny head, tiny teeth. These iconic, gargantuan dinosaurs developed a wholly unique dining strategy to support their massive size. Image by Stephanie Abramowicz, courtesy of the Natural History Museum of Los Angeles County (NHM).
Long neck, long tail, tiny head, tiny teeth. These iconic, gargantuan dinosaurs developed a wholly unique dining strategy to support their massive size. Image by Stephanie Abramowicz, courtesy of the Natural History Museum of Los Angeles County (NHM).

How did the largest animals to ever walk the Earth dominate their environments? By doing something totally revolutionary: keeping it simple. Published in BMC Ecology and Evolution, a new study led by Postdoctoral Research Scientist and periodic dinosaur dentist Dr. Keegan Melstrom at the Natural History Museum of Los Angeles County’s Dinosaur Institute ??reveals that colossal sauropod dinosaurs, the largest animals to ever walk the Earth, had a strategy for dining on plants unique to long-necked dinosaurs: linking tooth complexity to how fast teeth were replaced.

“In nearly every other animal we look at, the complexity of a tooth relates to the animal’s diet,” says Dr. Melstrom. “Carnivores have simple teeth, herbivores have complex teeth, often with distinct ridges, crests, and cusps for processing plant material. But sauropods break this incredibly consistent pattern. Instead, these dinosaurs link complexity to tooth replacement rate, with simple teeth being replaced every few weeks!”

The shapes of an animal’s teeth are thought to reveal a lot about its diet and by extension its lifestyle. The banana-sized knives ringing the mouths of T. Rex are perfect for ripping flesh, and deadly simple sharp teeth abound in living and extinct carnivores. Typically, herbivores have extremely complex teeth: perfect for grinding down fibrous leaves or grasses. When it comes to the largest animals to ever walk the Earth, sauropods chewed their own path. Unlike any other plant-eating animals living or extinct, sauropods rely on quickly replacing their teeth to keep the salad flowing.

Keep It Simple, Sauropods

“The diet of extinct dinosaurs was incredibly varied, spanning tiny meat-eaters to massive plant-eaters,” says Dr. Melstrom. “Our research sheds light on the range of adaptations that allowed so many plant-eaters to live alongside one another.”

Using computerized tomography (CT) and microCT scanning, Dr. Melstrom and his colleagues made 3D models of specimens from around the globe, capturing the great diversity of tooth complexity in Late Jurassic dinosaurs.

“This whole project was conducted during the pandemic. Instead of traveling the world to gather data, we relied on researchers who had made their data available to other scientists, as well as the incredible collections here at NHM. I think this project really demonstrates the importance of sharing information, it can lead to new discoveries even during a pandemic,” says Dr. Melstrom.

They converted the toothy hills and valleys of dinosaur teeth into numbers, quantifying tooth complexity between the three groups of dinosaurs: meat-eating theropods, plant-eating ornithischians, and similarly herbivorous sauropods.

What they found was an entirely new evolutionary strategy to handle a plant-based diet 150 million years ago. While meat-eating dinosaurs had sharp simple teeth expected for carnivores, and ornithischians had the more complex teeth similar to herbivores living today, sauropods had very simple teeth, unlike any other known herbivores extinct or living.

In sauropods, they found that the more complex the tooth, the more slowly teeth were replaced, a correlation that demonstrates that tooth replacement rate is related to tooth complexity, unlike any other known animals. More specifically, diplodocoids like Apatosaurus and Diplodocus exhibited incredibly fast replacement rates and simple teeth, possibly allowing them to eat different foods from the other group of sauropods, macronarians like ??Brachiosaurus, which had more complex teeth.

Simple teeth would have made sense for sauropods’ long necks. Smaller teeth built to be lost weigh less than the tougher teeth of all other herbivores, which helps lighten the skull at the end of those long necks. The peculiar tooth replacement pattern meant these sauropods could focus on plant food other dinosaurs and non-dinosaur plant-eaters passed by.

“Time and time again, the fossil record shows us that there isn’t one solution to evolutionary problems. For sauropods, when it comes to eating tough plants, the simplest solution was the best,” says Dr. Melstrom.

Reference:
Keegan M. Melstrom, Luis M. Chiappe, Nathan D. Smith. Exceptionally simple, rapidly replaced teeth in sauropod dinosaurs demonstrate a novel evolutionary strategy for herbivory in Late Jurassic ecosystems. BMC Ecology and Evolution, 2021; 21 (1) DOI: 10.1186/s12862-021-01932-4

Note: The above post is reprinted from materials provided by Natural History Museum of Los Angeles County.

New species of iguanodontian dinosaur discovered from Isle of Wight

Brighstoneus simmondsi reconstruction. Credit: John Sibbick
Brighstoneus simmondsi reconstruction. Credit: John Sibbick

Scientists from the Natural History Museum and University of Portsmouth have described a new genus and species of dinosaur from a specimen found on the Isle of Wight.

Following on from a new species of ankylosaur, new species of therapodand two new speciesof spinosaur dinosaurs, Brighstoneus simmondsi is the latest in a host of new dinosaur species described by Museum scientists in recent weeks.

The new dinosaur is an iguanodontian, a group that also includes the iconic Iguanodon and Mantellisaurus. Until now, iguanodontian material found from the Wealden Group (representing part of the Early Cretaceous period) on the Isle of Wight has usually been referred to as one of these two dinosaurs — with more gracile fossil bones assigned to Mantellisaurus and the larger and more robust material assigned to Iguanodon.

However, when Dr Jeremy Lockwood — a PhD student at the Museum and University of Portsmouth — was examining the specimen, he came across several unique traits that distinguished it from either of these other dinosaurs.

‘For me, the number of teeth was a sign’ Dr Lockwood says. ‘Mantellisaurus has 23 or 24, but this has 28. It also had a bulbous nose, whereas the other species have very straight noses. Altogether, these and other small differences made it very obviously a new species.’

The herbivorous dinosaur was about eight metres in length and weighed about 900kg. Published in the peer-reviewed Journal of Systematic Palaeontology, Dr Lockwood describes the species and names it Brighstoneus simmondsi: Brighstoneus after the village of Brighstone, near to the excavation site, and simmondsi honouring Mr Keith Simmonds, who made the discovery of the specimen in 1978.

The discovery of this new species suggests that there were far more iguanodontian dinosaurs in the Early Cretaceous of the UK than previously thought, and that simply assigning specimens from this period to either Iguanodon or Mantellisaurus must change.

‘We’re looking at six, maybe seven million years of deposits, and I think the genus lengths have been overestimated in the past, ‘says Dr Lockwood. ‘If that’s the case on the island, we could be seeing many more new species. It seems so unlikely to just have two animals being exactly the same for millions of years without change.’

Museum scientist Dr Susannah Maidment, a co-author of the paper, says: ‘The describing of this new species shows that there is clearly a greater diversity of iguanodontian dinosaurs in the Early Cretaceous of the UK than previously realised. It’s also showing that the century-old paradigm that gracile iguanodontian bones found on the island belong to Mantellisaurus and large elements belong to Iguanodon can no longer be substantiated’.

The Isle of Wight has long been associated with dinosaur discovery, and even yielded the crucial specimens that led to Sir Richard Owen to coin the term Dinosauria. The authors conclude that the describing of Brighstoneus simmondsi as a new species calls for a reassessment of Isle of Wight material:

‘British dinosaurs are certainly not something that’s done and dusted at all,’ says Dr Lockwood. ‘I think we could be on to a bit of a renaissance.’

Reference:
Jeremy A. F. Lockwood, David M. Martill, Susannah C. R. Maidment. A new hadrosauriform dinosaur from the Wessex Formation, Wealden Group (Early Cretaceous), of the Isle of Wight, southern England. Journal of Systematic Palaeontology, 2021; 1 DOI: 10.1080/14772019.2021.1978005

Note: The above post is reprinted from materials provided by Taylor & Francis Group.

Rapidly evolving species more likely to go extinct, study suggests

Pleurosaurus from the Late Jurassic, some 150 million years ago, of southern Germany, a remarkable, long-bodied swimming rhynchocephalian.
Pleurosaurus from the Late Jurassic, some 150 million years ago, of southern Germany, a remarkable, long-bodied swimming rhynchocephalian.

In a new study of lizards and their relatives, Dr Jorge Herrera-Flores of Bristol’s School of Earth Sciences and colleagues have discovered that ‘slow and steady wins the race’.

The team studied lizards, snakes and their relatives, a group called the Lepidosauria. Today there are more than 10,000 species of lepidosaurs, and much of their recent success is a result of fast evolution in favourable circumstances. But this was not always the case.

Mr Herrera-Flores explained: “Lepidosaurs originated 250 million years ago in the early Mesozoic Era, and they split into two major groups, the squamates on the one hand, leading to modern lizards and snakes, and the rhynchocephalians on the other, represented today by a single species, the tuatara of New Zealand. We expected to find slow evolution in rhynchocephalians, and fast evolution in squamates. But we found the opposite.”

“We looked at the rate of change in body size among these early reptiles,” said Dr Tom Stubbs, a collaborator. “We found that some groups of squamates evolved fast in the Mesozoic, especially those with specialised lifestyles like the marine mosasaurs. But rhynchocephalians were much more consistently fast-evolving.”

“In fact, their average rates of evolution were significantly faster than those for squamates, about twice the background rate of evolution, and we really did not expect this,” said Dr Armin Elsler, another collaborator. “In the later part of the Mesozoic all the modern groups of lizards and snakes originated and began to diversify, living side-by-side with the dinosaurs, but probably not engaging with them ecologically. These early lizards were feeding on bugs, worms, and plants, but they were mainly quite small.”

Prof Mike Benton added: “‘After the extinction of the dinosaurs, 66 million years ago, at the end of the Mesozoic, the rhynchocephalians and squamates suffered a lot, but the squamates bounced back. But for most of the Mesozoic, the rhynchocephalians were the innovators and the fast evolvers. They tailed off quite severely well before the end of the Mesozoic, and the whole dynamic changed after that.”

This work confirms a challenging proposal made by the famous palaeontologist George Gaylord Simpson in his 1944 book Tempo and Mode in Evolution. He looked at the fundamental patterns of evolution in a framework of Darwinian evolution and observed that many fast-evolving species belonged to unstable groups, which were potentially adapting to rapidly changing environments.

Prof Benton continued: “Slow and steady wins the race. In the classic Aesop’s fable, the speedy hare loses the race, whereas the slow-moving tortoise crosses the finishing line first. Since the days of Darwin, biologists have debated whether evolution is more like the hare or the tortoise. Is it the case that big groups of many species are the result of fast evolution over a short time or slow evolution over a long time?

“In some cases, they can stabilise and survive well, but in many cases the species go extinct as fast as new ones emerge, and they can go extinct, just like the napping hare. On the other hand, Simpson predicted that slowly evolving species might also be slow to go extinct, and could in the end be successful in the longer term, just like the slow-moving but persistent tortoise in the fable.”

Reference:
Jorge A. Herrera-Flores, Armin Elsler, Thomas L. Stubbs, Michael J. Benton. Slow and fast evolutionary rates in the history of lepidosaurs. Paleontology, 10 November 2021 DOI: 10.1111/pala.12579

Note: The above post is reprinted from materials provided by University of Bristol.

Muscular wing-body junction improved Pterosaur flight performance

Laser-stimulated fluorescence imaging of a pterosaur fossil reveals flight-related soft tissues. The imaging revealed a muscular wing root fairing that smooths airflow around the wing-body junction and reduces drag, as in the wing root fairings of modern aeroplanes. (Image credit: Michael Pittman)
Laser-stimulated fluorescence imaging of a pterosaur fossil reveals flight-related soft tissues. The imaging revealed a muscular wing root fairing that smooths airflow around the wing-body junction and reduces drag, as in the wing root fairings of modern aeroplanes. (Image credit: Michael Pittman)

The flying reptiles known as pterosaurs are the closest relatives of dinosaurs and were the first vertebrates to evolve powered flight. However, many details of pterosaur flight anatomy and performance are still unclear. According to a new study led by Dr Michael Pittman — Research Assistant Professor of the Department of Earth Sciences & Vertebrate Palaeontology Laboratory, The University of Hong Kong (HKU); Assistant Dean (e-learning) of HKU Faculty of Science — pterosaurs evolved a muscular wing-body junction to reduce drag and improve flight performance. The findings were recently published in the Proceedings of the National Academy of Sciences (PNAS).

Dr Pittman and colleagues used laser-stimulated fluorescence to image the bones and reveal soft tissues of a Late Jurassic pterodactyloid pterosaur fossil to analyse its flight performance. This involved scanning the fossil with a violet laser and taking long-exposure photographs of the fluorescence produced by the pterosaur’s bones and revealed soft tissues. Their results suggest that the pterosaur possessed a wing root fairing, a feature that smooths the airflow around the wing-body junction and reduces drag, as in the wing root fairings of most modern aeroplanes. “In birds, the wing root fairing is made of feathers. In bats, the wing root fairing is made of fur. In contrast, pterosaurs had a wing root fairing primarily made of skeletal muscle,” notes Mr Luke A. Barlow, a Research Assistant in Dr Pittman’s lab that studied the specimen.

Dr Pittman said, “This muscular wing root fairing appears to have provided pterosaurs with additional flight benefits, such as improved force generation during the flight stroke and sophisticated control of the wing’s shape, including minimising unwanted vibrations or ‘flutter’.” Speaking of the significance of the study, Mr Thomas G Kaye, a study co-author and Director of the Foundation of Scientific Advancement in the United States added, “Our work shows that pterosaurs were more advanced flyers than we thought, even in the Late Jurassic when birds had just evolved flight. Our study also highlights the potential contributions of new technologies to our understanding of pterosaur flight anatomy and evolution. We are excited to see where our work takes us next.”

Reference:
Michael Pittman, Luke A. Barlow, Thomas G. Kaye, Michael B. Habib. Pterosaurs evolved a muscular wing–body junction providing multifaceted flight performance benefits: Advanced aerodynamic smoothing, sophisticated wing root control, and wing force generation. Proceedings of the National Academy of Sciences, 2021; 118 (44): e2107631118 DOI: 10.1073/pnas.2107631118

Note: The above post is reprinted from materials provided by The University of Hong Kong.

Crushed resistance: Tectonic plate sinking into a subduction zone

The model offers new insights into how the plate subducted under Japan breaks into segments by bending and thereby crushing olivine grains on its underside. (Graphic: Taras Gerya / ETH Zurich)
The model offers new insights into how the plate subducted under Japan breaks into segments by bending and thereby crushing olivine grains on its underside. (Graphic: Taras Gerya / ETH Zurich)

The Earth’s surface consists of a few large plates and numerous smaller ones that are continuously moving either away from or towards each other at an extremely slow pace. At the boundaries of two plates, the heavier oceanic plate sinks below the lighter continental plate in a process that experts call subduction. For a long time, though, those experts have been puzzling over what happens to the plate margin that dives into the Earth’s mantle, known as the subducting slab. Some scientists assumed that the slab remains as rigid and strong as the plate itself and simply bends due to the gravity force and mechanical interaction with the Earth’s mantle.

Heavily deformed plate margin

However, models of the Earth’s interior constructed by scientists using seismic tomography revealed contradictory results: in the western United States, for example, the researchers observed anomalies at different depths on their tomographic images. These indicated that the slabs submerged beneath the Americas may be segmented. The scientists therefore concluded that the slabs in the mantle must be strongly deformed and are by no means rigid and immobile.

With the aid of computer models, other researchers, including ETH Professor Paul Tackley, confirmed that subducted slabs are indeed weak and deformable. And they formulated the subduction dichotomy hypothesis that can be expressed in simple terms: plates on the surface are rigid and strong (read: non-deformable), while the slabs in the mantle are soft and weak.

Seeking a plausible mechanism

“Until now, however, research has lacked a plausible mechanism to explain how this bending occurs and why sinking plate margins (slabs) become soft and weak,” says Taras Gerya, Professor of Geophysics at ETH Zurich.

Observations revealed that numerous faults are found on the upper surface of a sinking plate where it meets the other plate. Seawater penetrates the plate through these faults and is in fact literally sucked in by suction forces. This weakens the plate on its upper side.

Yet this alone is not sufficient to explain the segmentation of the slab — the anomalies observed on tomographic images. Another mechanism must also be at work to weaken the underside of the margin enough for segmentation to occur.

Gerya and his American colleagues David Bercovici and Thorsten Becker therefore suspected that compression of the underside of the plate at the point where it bends downward was “crushing” large and strong, millimetres size olivine crystals in the plate by forcing them to recrystallise into much weaker, micrometres size granular aggregate — thereby reducing the plate’s resistance and allowing it to bend.

Sinking plate margin divided into segments

Using a new two-dimensional computer model that integrated this grain reduction as a central mechanism, the three researchers then studied the process in silico. Their study was recently published in the journal Nature.

And indeed, the simulations revealed that sinking plates deform due to the massive reduction of olivine grains on their undersides, splitting into individual segments over time. These segments are rigid and stiff, but remain connected to each other by weak hinges made of ground grains.

In the simulations, parallel cracks appear at the segment boundaries on the plate’s upper surface. Below these cracks are the zones with “crushed” mineral grains.

“Just imagine you’re breaking a bar of chocolate,” Gerya says with a grin. A bar of chocolate, too, can be divided into segments only along the specified weak points. The squares of chocolate are rigid, but the connecting pieces between them are weak. “That’s why a sinking plate isn’t uniformly bent or deformed, but segmented.”

And here’s how it might play out in reality: The heavier plate sinks under the lighter one. A weak spot with smaller mineral grains within the sinking plate allows it to bend. The bending stress causes the minerals to crumble in more places on the underside. The resulting weakness leads to a fracture, and a segment forms. As the plate margin sinks deeper and deeper into the mantle, it causes further segments to form at the bend. As a result, the slab eventually resembles a chain with rigid links and bendable connectors. At a depth of about 600 kilometres, the segmented plate margin slides onto what is known as the 670 km discontinuity in the Earth’s mantle, from which point it moves horizontally.

Clues from nature support simulation

“The results of our simulations are consistent with observations in nature,” Gerya explains. A great deal of research has been done on the natural situation along the Japan Trench, where the Pacific plate sinks below the Okhotsk plate. The pattern of faults found here is an exact match for the pattern produced in the simulations.

Researchers have also studied the seismic velocity structure of subducting Japan slab thoroughly using its recently produced high-resolution seismic tomography model. They found that the velocity of the seismic waves sent out by earthquakes was reduced at some nodes inside the slab. The pattern with which these nodes occur in reality coincides with that of the segment boundaries from the simulations. And both in nature and in the computer model, it is zones with very small crystals only micrometres across that are responsible for reducing the velocity of the seismic waves.

These tiny crystal grains also make the underside plate material less viscous; in other words, it becomes runnier. Researchers at the Japan Trench were able to demonstrate this, too.

“That means our model is very plausible and provides solid physical background for the hypothesis of rigid plates with weak slabs,” Gerya says. But the research is far from over: one of his Bachelor’s students, Simon Niggli, has modelled and described plate fractures in three dimensions for the first time. Next the researchers want to investigate whether the segmentation of plate margins can also be responsible for strong earthquakes.

Reference:
T. V. Gerya, D. Bercovici, T. W. Becker. Dynamic slab segmentation due to brittle–ductile damage in the outer rise. Nature, 2021; 599 (7884): 245 DOI: 10.1038/s41586-021-03937-x

Note: The above post is reprinted from materials provided by ETH Zurich. Original written by Peter Rueegg.

Researchers recreate deep-Earth conditions to see how iron copes with extreme stress

Despite ESA’s GOCE mission ending over seven years ago, scientists continue to use this remarkable satellite’s gravity data to delve deep and unearth secrets about our planet. Recent research shows how scientists have combined GOCE data with measurements taken at the surface to generate a new model of Earth’s crust and upper mantle. This is the first time such a model has been created this way – and it is shedding new light on the processes of plate tectonics. The new model produced in ESA’s 3D Earth study shows for the first time how dissimilar the sub-lithospheric mantle is beneath different oceans, and provides insight as to how the morphology and spreading rates of mid-oceanic ridges may be connected with the deep chemical and thermal structure. Credit: ESA/Planetary Visions)
Representative image:  Credit: ESA/Planetary Visions)

Far below you lies a sphere of solid iron and nickel about as wide as the broadest part of Texas: the Earth’s inner core. The metal at the inner core is under pressure about 360 million times higher than we experience in our everyday lives and temperatures approximately as hot as the Sun’s surface.

Earth’s planetary core is thankfully intact. But in space, similar cores can collide with other objects, causing the crystalline materials of the core to deform rapidly. Some asteroids in our solar system are massive iron objects that scientists suspect are the remnants of planetary cores after catastrophic impacts.

Measuring what happens during the collision of celestial bodies or at the Earth’s core is obviously not very practical. As such, much of our understanding of planetary cores is based on experimental studies of metals at less extreme temperatures and pressures. But researchers at the Department of Energy’s SLAC National Accelerator Laboratory have now observed for the first time how iron’s atomic structure deforms to accommodate the stress from the pressures and temperatures that occur just outside of the inner core.

The results appear in Physical Review Letters, where they have been highlighted as an Editor’s Suggestion.

Coping with stress

Most of the iron you encounter in your everyday life has its atoms arranged in nanoscopic cubes, with an iron atom at each corner and one in the center. If you squeeze these cubes by applying extremely high pressures, they rearrange into hexagonal prisms, which allow the atoms to pack in more tightly.

The group at SLAC wanted to see what would happen if you kept applying pressure to that hexagonal arrangement to mimic what happens to iron at the Earth’s core or during atmospheric reentry from space. “We didn’t quite make inner core conditions,” says co-author Arianna Gleason, a scientist in the High-Energy Density Science (HEDS) Division at SLAC. “But we achieved the conditions of the outer core of the planet, which is really remarkable.”

No one had ever directly observed iron’s response to stress under such high temperatures and pressures before, so the researchers didn’t know how it would respond. “As we continue to push it, the iron doesn’t know what to do with this extra stress,” says Gleason. “And it needs to relieve that stress, so it tries to find the most efficient mechanism to do that.”

The coping mechanism iron uses to deal with that extra stress is called “twinning.” The arrangement of atoms shunts to the side, rotating all the hexagonal prisms by nearly 90 degrees. Twinning is a common pressure response in metals and minerals — quartz, calcite, titanium and zirconium all undergo twinning.

“Twinning allows iron to be incredibly strong — stronger than we first thought — before it starts to flow plastically on much longer time scales,” Gleason said.

A tale of two lasers

Reaching these extreme conditions required two types of lasers. The first was an optical laser, which generated a shock wave that subjected the iron sample to extremely high temperatures and pressures. The second was SLAC’s Linac Coherent Light Source (LCLS) X-ray free-electron laser, which allowed the researchers to observe the iron on an atomic level. “At the time, LCLS was the only facility in the world where you could do that,” says lead author Sébastien Merkel of the University of Lille in France. “It’s been a door opener for other similar facilities in the world.”

The team fired both lasers at a tiny sample of iron about the width of a human hair, hitting the iron with a shock wave of heat and pressure. “The control room is just above the experimental room,” Merkel says. “When you trigger the discharge, you hear a loud pop.”

As the shock wave hit the iron, researchers used the X-ray laser to observe how the shock changed the arrangement of the iron atoms. “We were able to make a measurement in a billionth of a second,” Gleason says. “Freezing the atoms where they are in that nanosecond is really exciting.”

The researchers collected these images and assembled them into a flipbook that showed iron deforming. Before the experiment was complete, they didn’t know if iron would respond too fast for them to measure or too slow for them to ever see. “The fact that the twinning happens on the time scale that we can measure it as an important result in itself,” Merkel says.

The future is bright

This experiment serves as a bookend for understanding the behavior of iron. Scientists had gathered experimental data on the structure of iron at lower temperatures and pressures and used it to model how iron would behave at extremely high temperatures and pressures, but no one had ever experimentally tested those models.

“Now we can give a thumbs up, thumbs down on some of the physics models for really fundamental deformation mechanisms,” Gleason says. “That helps to build up some of the predictive capability we’re lacking for modeling how materials respond at extreme conditions.”

The study provides exciting insights into the structural properties of iron at extremely high temperatures and pressures. But the results are also a promising indicator that these methods could help scientists understand how other materials behave at extreme conditions, too.

“The future is bright now that we’ve developed a way to make these measurements,” Gleason says. “The recent X-ray undulator upgrade as part of the LCLS-II project allows higher X-ray energies — enabling studies on thicker alloys and materials that have lower symmetry and more complex X-ray fingerprints.”

The upgrade will also enable researchers to observe larger samples, which will give them a more comprehensive view of iron’s atomic behavior and improve their statistics. Plus, “we’re going to get more powerful optical lasers with the approval to proceed with a new flagship petawatt laser facility, known as MEC-U,” says Gleason. “That’ll make future work even more exciting because we’ll be able to get to the Earth’s inner core conditions without any problem.”

Researchers at Los Alamos National Laboratory (LANL) contributed to this study. Funding was provided by the University of Lille, an LANL Reines Laboratory Directed Research and Development grant, and the DOE Office of Science, including Gleason’s DOE Early Career Award in Fusion Energy Sciences. LCLS is a DOE Office of Science user facility.

Reference:
Sébastien Merkel, Sovanndara Hok, Cynthia Bolme, Dylan Rittman, Kyle James Ramos, Benjamin Morrow, Hae Ja Lee, Bob Nagler, Eric Galtier, Eduardo Granados, Akel Hashim, Wendy L Mao, Arianna E Gleason. Femtosecond Visualization of hcp-Iron Strength and Plasticity under Shock Compression. Physical Review Letters, 2021; 127 (20) DOI: 10.1103/PhysRevLett.127.205501

Note: The above post is reprinted from materials provided by DOE/SLAC National Accelerator Laboratory. Original written by Graycen Wheeler.

Fate of sinking tectonic plates is revealed

Boudins of amphibolite layers (metamorphosed basalts) that were stretched within quartz schists (Norway). Photo credits © Haakon Fossen.
Boudins of amphibolite layers (metamorphosed basalts) that were stretched within quartz schists (Norway). Photo credits © Haakon Fossen.

Our world’s surface is a jumble of jostling tectonic plates, with new ones emerging as others are pulled under. The ongoing cycle keeps our continents in motion and drives life on Earth. But what happens when a plate disappears into the planet’s interior?

The question has long puzzled scientists because conventional wisdom said that sinking tectonic plates must remain intact to keep pulling on the portion behind it, but according to geophysical evidence, they are destroyed.

Now, in a study published Nov. 11 in Nature, scientists say they’ve found an answer that reconciles the two stories: Plates are significantly weakened as they sink but not so much that they break apart entirely.

The finding came after scientists put tectonic plates through a computer-generated gauntlet of destructive geologic forces. The model showed that as the plate enters the mantle, it bends abruptly downward, cracking its cold, brittle back. At the same time, the bending changes the fine grain structure of the rock along its underbelly, leaving it weakened. Combined, the stresses pinch the plate along its weak points, leaving it mostly intact but segmented like a slinky snake.

This means the plate continues to be pulled under despite becoming folded and distorted.

According to the researchers, the model predicted a scenario that matches observations from Japan. Studies of the region where the Pacific tectonic plate dives — or subducts — under Japan have turned up large cracks where the plate bends downward, and they have shown signs of weaker material underneath. Deep seismic imaging conducted by The University of Texas at Austin’s Steve Grand has also revealed tectonic shapes in the Earth’s mantle under Japan that appear a close match for the slinky snake in the model.

Co-author Thorsten Becker, a professor in UT’s Jackson School of Geosciences, said that the study does not necessarily close the book on what happens to subducting plates, but it certainly gives a compelling case to explain several important geologic processes.

“It’s an example of the power of computational geosciences,” said Becker who assisted in developing the model and is a faculty associate at UT’s Oden Institute for Computational Engineering & Sciences. “We combined these two processes that geology and rock mechanics are telling us are happening, and we learned something about the general physics of how the Earth works that we wouldn’t have expected. As a physicist, I find that exciting.”

The study’s lead author, Taras Gerya, a professor of geophysics at ETH Zurich, added that until now, geophysicists had lacked a comprehensive explanation for how tectonic plates bend without breaking.

Things got interesting when the researchers ran their simulations with a hotter interior, similar to the early Earth. In these simulations, the tectonic snake segments made it only a few miles into the mantle before breaking off. That means that subduction would have occurred intermittently, raising the possibility that modern plate tectonics began only within the past billion years.

“Personally, I think there are a lot of good arguments for plate tectonics being much older,” Becker said, “but the mechanism revealed by our model suggests things might be more sensitive to the temperature of the mantle than we thought, and that, I think, could lead to interesting new avenues of discussion.”

Becker and Gerya were joined by David Bercovici, a geophysicist at Yale University whose investigation into how rock grains are altered in the deep mantle helped motivate the research. The study is based on a two-dimensional computer model of plate tectonics incorporating Bercovici’s rock deformation research and other plate-weakening mechanics. The researchers are now studying the phenomena using 3D models and plan to investigate what those models can tell them about the occurrence of earthquakes.

The research was supported by grants from the Swiss National Science Foundation, ETH Zurich, and the U.S. National Science Foundation. The simulations were run on high-performance computing clusters at ETH Zurich.

Reference:
T. V. Gerya, D. Bercovici, T. W. Becker. Dynamic slab segmentation due to brittle–ductile damage in the outer rise. Nature, 2021; 599 (7884): 245 DOI: 10.1038/s41586-021-03937-x

Note: The above post is reprinted from materials provided by University of Texas at Austin.

Radiocarbon is key to understanding Earth’s past

The rising Earth from the perspective of the moon.
The rising Earth from the perspective of the moon. Credit: NASA Goddard

Radiocarbon records are critical to understanding the history of Earth’s climate, magnetic field, and the Sun’s activity, say researchers.

In an article published today (November 5 2021) in the journal Science, scientists have highlighted how recent advances in our knowledge of past radiocarbon levels are improving our understanding of climate processes, solar activity, geophysics and the carbon cycle.

Understanding the past is essential to understanding our present and to projecting Earth’s potential changes in the future. Developing an accurate record of atmospheric radiocarbon extending back 55,000 years helps researchers understand Earth’s processes and consequently improve projections of climate change.

Radiocarbon also tells us about the possibility of past extreme solar storms, orders of magnitude greater than any instrumentally observed. Similar storms today would have the potential to catastrophically damage our communications networks and electricity grids.

Dr Tim Heaton, Lead Author and Senior Lecturer from the University of Sheffield’s School of Mathematics and Statistics, said: “Radiocarbon is best known as the tool by which we date and synchronise many of the various archaeological and climate records from the last 55,000 years. However, past levels of radiocarbon are also critical to understand the Sun, the geodynamo, past climate, and changes in the carbon cycle.

“Recent years have seen a revolution in our ability to construct detailed records of past radiocarbon levels, leading to new insights in the chronology of past climate events, changes in the Sun’s activity, carbon cycle and fluxes in Carbon Dioxide (CO2) levels.”

Developments in radiocarbon dating have allowed the IntCal Working Group to estimate radiocarbon levels with unprecedented accuracy back to the limits of the technique ~55,000 years ago.

Last year the IntCal Working Group recalculated the internationally-agreed radiocarbon calibration curves for the first time in seven years, making them more detailed than ever before.

They used measurements from almost 15,000 samples from objects dating back as far as 60,000 years ago to create the new radiocarbon calibration curves, which are fundamental across the scientific spectrum for accurately dating artefacts, and understanding the Earth and climate systems.

Radiocarbon is vital to geoscience and archaeology. Scientists on the Intergovernmental Panel on Climate Change (IPCC) rely upon radiocarbon to improve their models — as a proxy for the Sun, and as a target to improve their understanding of the Earth system — and as a clock to date most paleoclimatic records over the past 55,000 years. This is essential to better understand and prepare for future changes in climate. Archaeologists use radiocarbon dating to understand pivotal changes in our societal systems that help to explain our present and answer the grand challenges we face today.

Reference:
T. J. Heaton, E. Bard, C. Bronk Ramsey, M. Butzin, P. Köhler, R. Muscheler, P. J. Reimer, L. Wacker. Radiocarbon: A key tracer for studying Earth’s dynamo, climate system, carbon cycle, and Sun. Science, 2021; 374 (6568) DOI: 10.1126/science.abd7096

Note: The above post is reprinted from materials provided by University of Sheffield.

Let’s talk about the 1,800-plus ‘young’ volcanoes in the US Southwest

A view of the crater of Dotsero volcano, a monogenetic volcano that erupted in Colorado about 4,000 years ago. Credit: Greg Valentine
A view of the crater of Dotsero volcano, a monogenetic volcano that erupted in Colorado about 4,000 years ago. Credit: Greg Valentine

They’re born. They live once, erupting for a period that might last for days, years or decades. Then, they go dark and die.

This narrative describes the life of a monogenetic volcano, a type of volcanic hazard that can pose important dangers despite an ephemeral existence.

The landscape of the southwestern U.S. is heavily scarred by past eruptions of such volcanoes, and a new study marks a step toward understanding future risks for the region.

The research, which will be published on Nov. 2 in the journal Geosphere, provides a broad overview of what we know — and don’t know — about this type of volcanism in the U.S. Southwest over the past 2.58 million years, a geologic period known as the Quaternary.

During this time, more than 1,800 monogenetic volcanoes erupted in the region, according to a count covering Nevada, Utah, Arizona, Colorado, New Mexico and parts of California’s eastern edge. Add in the Pinacate volcanic field, located mostly in the Mexican state of Sonora, bordering Arizona, and the number goes up to over 2,200, scientists say. (The volcanoes included are ones whose ages are estimated to be in the range of the Quaternary, but many have not been precisely dated.)

“Monogenetic means ‘one life,'” says lead author Greg Valentine, a University at Buffalo volcanologist. “So a monogenetic volcano will erupt once, and that eruption may last for several days to several decades, but after that, the volcano is basically dead.

“In the United States, most volcanic hazards-related attention has rightly gone to places like Hawaii, and to the Pacific Northwest and Alaska, where we have big stratovolcanoes like Mount Rainier and Mount St. Helens, which will have many eruptive episodes over a long life, with widespread hazardous effects. In the past, these smaller monogenetic volcanoes really haven’t been looked at from a focus on hazards; they have been instead studied mainly for what they tell us about the deep earth. Recently, however, there has been more buzz in the research community about how we need to take a look at the kinds of hazards these volcanoes might pose.

“My experience with the general public is that most people are surprised to know that there are so many young volcanoes in the Southwest.”

The paper’s authors are Valentine, PhD, professor of geology in the UB College of Arts and Sciences; Michael H. Ort, PhD, professor emeritus of geology at Northern Arizona University; and Joaquín A. Cortés, PhD, senior lecturer of geology at Edge Hill University in England.

These volcanoes won’t erupt again. So why study them?

The 2,000-plus volcanoes noted in the paper are done erupting, so they no longer pose a threat. But studying them is important because of the potential for new ones to bloom.

“Monogenetic volcanoes tend to occur in areas that we call volcanic fields, and the American Southwest is just dotted with these,” says Valentine, who grew up in New Mexico. “These are areas of high volcanic activity where future eruptions could happen, but we don’t know when, and we don’t know exactly where.”

The city of Flagstaff, Arizona, is located in a volcanic field where multiple monogenetic volcanoes have erupted in the past, so a better understanding of possible hazards is important for people who live there.

“Two of the most recent eruptions in the Southwest occurred near Flagstaff about 1,000 years ago, one just outside of town and the other on the north rim of the Grand Canyon,” Ort says. Northern Arizona University is in Flagstaff. “People living there at the time adapted to the effects of the eruptions, changing agricultural and cultural practices as well as where they lived. We will need to do the same when the next one erupts. Albuquerque also has young volcanoes along its western margin.”

Mercifully, most volcanoes in the southwestern U.S. are in remote locations, away from large population centers. In isolated areas, threats from eruptions could include ash plumes that disrupt travel (including air) or power distribution infrastructure, researchers say.

“One of the younger eruptions in the Southwest occurred south of Grants, New Mexico a few thousand years ago, and flowed for many miles parallel to what is now Interstate 40 and part of the Burlington Northern Santa Fe railroad,” Ort says. “A similar eruption today would take out one of the most important east-west transportation routes in the country. Several volcanic fields lie along these routes, from the Mojave Desert of California to eastern New Mexico, including the one around Flagstaff.”

“The fundamental pieces of information that you need to have in order to start understanding the hazards and the chances of a future eruption are the number of volcanoes, their ages and the types of eruptions they have,” Valentine says. “What we set out to do in the study is find every bit of information that we could about these monogenetic volcanoes in the southwestern U.S. and compile it all in one place. How many of these are there? What are their characteristics? We got information from state geological surveys, published papers and other sources.”

What are the chances of a new eruption within a century?

Based solely on the total count of volcanoes that have erupted in the study region during the Quaternary Period, the chances of a new volcano emerging in the area within 100 years would be about 8%, Valentine says.

But he notes that this figure embodies lots of uncertainty. It doesn’t account for buried volcanoes, or the fact that a single eruption can create multiple vents. More research will be needed to refine this estimate and to forecast likely locations for a new eruption.

“There’s so much uncertainty here, and this is part of the problem,” he says. “It’s kind of a wide-open research field. When you look at the region from the perspective of volcanic hazards, we really have very little information. Most of the volcanoes have not been dated, so we don’t know how old they are, except that they likely formed sometime within the Quaternary Period. Very few have been studied in detail.”

That said, the study’s findings indicate that the frequency of eruptions across the study region may approach that of individual volcanoes in the Pacific Northwest, Valentine and Ort say. The new paper highlights gaps in knowledge, and the scientists hope that it can act as a launchpad for future, more detailed research. As Ort and Valentine point out, a new Southwest volcano could appear anywhere in any active volcanic field.

“We don’t have infinite resources, so we have to prioritize the efforts we put into forecasting and planning for hazards,” Valentine says. “But how do you set priorities? If you’re monitoring volcanic fields in the Southwest, where do you put the instruments? Being able to better answer questions like these is what we’re moving toward.”

Reference:
Greg A. Valentine, Michael H. Ort, Joaquín A. Cortés. Quaternary basaltic volcanic fields of the American Southwest. Geosphere, 2021; DOI: 10.1130/GES02405.1

Note: The above post is reprinted from materials provided by University at Buffalo. Original written by Charlotte Hsu.

Uncovering the secrets behind Earth’s first major mass extinction

Brachiopod fossils from the Ordovician Period outcrop on Anticosti Island, Quebec, Canada. (Credit: André Desrochers, University of Ottawa)
Brachiopod fossils from the Ordovician Period outcrop on Anticosti Island, Quebec, Canada. (Credit: André Desrochers, University of Ottawa)

We all know that the dinosaurs died in a mass extinction. But did you know that there were other mass extinctions? There are five most significant mass extinctions, known as the “big five,” where at least three-quarters of all species in existence across the entire Earth faced extinction during a particular geological period of time. With current trends of global warming and climate change, many researchers now believe we may be in a sixth.

Discovering the root cause of Earth’s mass extinctions has long been a hot topic for scientists, as understanding the environmental conditions that led to the elimination of the majority of species in the past could potentially help prevent a similar event from occurring in the future.

A team of scientists from Syracuse University’s Department of Earth and Environmental Sciences, the University of California, Berkeley and the University of California, Riverside, Université Bourgogne Franche-Comté, the University of New Mexico, the University of Ottawa, the University of Science and Technology of China and Stanford University recently co-authored a paper exploring the Late Ordovician mass extinction (LOME), which is the first, or oldest of the “big five (~445 million years ago).” Around 85% of marine species, most of which lived in shallow oceans near continents, disappeared during that time.

Lead author Alexandre Pohl, from UC Riverside (now a postdoctoral research fellow at Université Bourgogne Franche-Comté in Dijon, France) and his co-authors investigated the ocean environment before, during, and after the extinction in order to determine how the event was brewed and triggered. The results from their study will be published in the journal Nature Geoscience on Nov. 1.

To paint a picture of the oceanic ecosystem during the Ordovician Period, mass extinction expert Seth Finnegan, associate professor at UC Berkeley, says that seas were full of biodiversity. Oceans contained some of the first reefs made by animals, but lacked an abundance of vertebrates.

“If you had gone snorkeling in an Ordovician sea you would have seen some familiar groups like clams and snails and sponges, but also many other groups that are now very reduced in diversity or entirely extinct like trilobites, brachiopods and crinoids” says Finnegan.

Unlike with rapid mass extinctions, like the Cretaceous-Tertiary extinction event where dinosaurs and other species died off suddenly some 65.5 million years ago, Finnegan says LOME played out over a substantial period of time, with estimates between less than half a million to almost two million years.

One of the major debates surrounding LOME is whether lack of oxygen in seawater caused that period’s mass extinction. To investigate this question, the team integrated geochemical testing with numerical simulations and computer modeling.

Zunli Lu, professor of Earth and environmental sciences at Syracuse University, and his students took measurements of iodine concentration in carbonate rocks from that period, contributing important findings about oxygen levels at various ocean depths. The concentration of the element iodine in carbonate rocks serves as an indicator for changes in oceanic oxygen level in Earth’s history.

Their data, combined with computer modeling simulations, suggested that there was no evidence of anoxia – or lack of oxygen – strengthening during the extinction event in the shallow ocean animal habitat where most organisms lived, meaning that climate cooling that occurred during the Late Ordovician period combined with additional factors likely was responsible for LOME.

On the other hand, there is evidence that anoxia in deep oceans expanded during that same time, a mystery that cannot be explained by the classic model of ocean oxygen, climate modeling expert Alexandre Pohl says.

“Upper-ocean oxygenation in response to cooling was anticipated, because atmospheric oxygen preferentially dissolves in cold waters,” Pohl says. “However, we were surprised to see expanded anoxia in the lower ocean since anoxia in Earth’s history is generally associated with volcanism-induced global warming.”

They attribute the deep-sea anoxia to the circulation of seawater through global oceans. Pohl says that a key point to keep in mind is that ocean circulation is a very important component of the climatic system.

He was part of a team led by senior modeler Andy Ridgwell, professor at UC Riverside, whose computer modeling results show that climate cooling likely altered ocean circulation pattern, halting the flow of oxygen-rich water in shallow seas to the deeper ocean.

According to Lu, recognizing that climate cooling can also lead to lower oxygen levels in some parts of the ocean is a key takeaway from their study.

“For decades, the prevailing school of thoughts in our field is that global warming causes the oceans to lose oxygen and thus impact marine habitability, potentially destabilizing the entire ecosystem,” Lu says. “In recent years, mounting evidence point to several episodes in Earth’s history when oxygen levels also dropped in cooling climates.”

While the causes of Late Ordovician extinction have not been fully agreed upon, nor will they for some time, the team’s study rules out changes in oxygenation as a single explanation for this extinction and adds new data favoring temperature change being the killing mechanism for LOME.

Pohl is hopeful that as better climate data and more sophisticated numerical models become available, they will be able to offer a more robust representation of the factors that may have led to the Late Ordovician mass extinction.

Reference:
Alexandre Pohl, Zunli Lu, Wanyi Lu, Richard G. Stockey, Maya Elrick, Menghan Li, André Desrochers, Yanan Shen, Ruliang He, Seth Finnegan, Andy Ridgwell. Vertical decoupling in Late Ordovician anoxia due to reorganization of ocean circulation. Nature Geoscience, 2021; DOI: 10.1038/s41561-021-00843-9

Note: The above post is reprinted from materials provided by Syracuse University. Original written by Dan Bernardi.

Some of the world’s oldest rubies linked to early life

Photo of the ruby that this study looks at. Credit: University of Waterloo
Photo of the ruby that this study looks at. Credit: University of Waterloo

While analyzing some of the world’s oldest coloured gemstones, researchers from the University of Waterloo discovered carbon residue that was once ancient life, encased in a 2.5 billion-year-old ruby.

The research team, led by Chris Yakymchuk, professor of Earth and Environmental Sciences at Waterloo, set out to study the geology of rubies to better understand the conditions necessary for ruby formation. During this research in Greenland, which contains the oldest known deposits of rubies in the world, the team found a ruby sample that contained graphite, a mineral made of pure carbon. Analysis of this carbon indicates that it is a remnant of early life.

“The graphite inside this ruby is really unique. It’s the first time we’ve seen evidence of ancient life in ruby-bearing rocks,” says Yakymchuk. “The presence of graphite also gives us more clues to determine how rubies formed at this location, something that is impossible to do directly based on a ruby’s colour and chemical composition.”

The presence of the graphite allowed the researchers to analyze a property called isotopic composition of the carbon atoms, which measures the relative amounts of different carbon atoms. More than 98 per cent of all carbon atoms have a mass of 12 atomic mass units, but a few carbon atoms are heavier, with a mass of 13 or 14 atomic mass units.

“Living matter preferentially consists of the lighter carbon atoms because they take less energy to incorporate into cells,” said Yakymchuk. “Based on the increased amount of carbon-12 in this graphite, we concluded that the carbon atoms were once ancient life, most likely dead microorganisms such as cyanobacteria.”

The graphite is found in rocks older than 2.5 billion years ago, a time on the planet when oxygen was not abundant in the atmosphere, and life existed only in microorganisms and algae films.

During this study, Yakymchuk’s team discovered that this graphite not only links the gemstone to ancient life but was also likely necessary for this ruby to exist at all. The graphite changed the chemistry of the surrounding rocks to create favourable conditions for ruby growth. Without it, the team’s models showed that it would not have been possible to form rubies in this location.

References:

  • Chris Yakymchuk, Vincent van Hinsberg, Christopher L. Kirkland, Kristoffer Szilas, Carson Kinney, Jillian Kendrick, Julie A. Hollis. Corundum (ruby) growth during the final assembly of the Archean North Atlantic Craton, southern West Greenland. Ore Geology Reviews, 2021; 138: 104417 DOI: 10.1016/j.oregeorev.2021.104417
  • Vincent van Hinsberg, Chris Yakymchuk, Angunguak Thomas Kleist Jepsen, Christopher L. Kirkland, Kristoffer Szilas. The corundum conundrum: Constraining the compositions of fluids involved in ruby formation in metamorphic melanges of ultramafic and aluminous rocks. Chemical Geology, 2021; 571: 120180 DOI: 10.1016/j.chemgeo.2021.120180

Note: The above post is reprinted from materials provided by University of Waterloo.

Related Articles