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Discovery of extinct prehistoric reptile that lived among dinosaurs

Fossil of Opisthiamimus gregori  Fossil skeleton of the new lizard-like reptile Opisthiamimus gregori. The fossil was discovered in the Morrison Formation of the Bighorn Basin, north-central Wyoming, and dates to the Late Jurassic Period, approximately 150 million years ago. Credit: David DeMar for the Smithsonian Institution.
Fossil of Opisthiamimus gregori
Fossil skeleton of the new lizard-like reptile Opisthiamimus gregori. The fossil was discovered in the Morrison Formation of the Bighorn Basin, north-central Wyoming, and dates to the Late Jurassic Period, approximately 150 million years ago.
Credit: David DeMar for the Smithsonian Institution.

Smithsonian researchers have discovered a new extinct species of lizard-like reptile that belongs to the same ancient lineage as New Zealand’s living tuatara. A team of scientists, including the National Museum of Natural History’s curator of Dinosauria Matthew Carrano and research associate David DeMar Jr. as well as University College London and Natural History Museum, London scientific associate Marc Jones, describe the new species Opisthiamimus gregori, which once inhabited Jurassic North America about 150 million years ago alongside dinosaurs like Stegosaurus and Allosaurus, in a paper published today in the Journal of Systematic Palaeontology. In life, this prehistoric reptile would have been about 16 centimeters (about 6 inches) from nose to tail — and would fit curled up in the palm of an adult human hand — and likely survived on a diet of insects and other invertebrates.

“What’s important about the tuatara is that it represents this enormous evolutionary story that we are lucky enough to catch in what is likely its closing act,” Carrano said. “Even though it looks like a relatively simple lizard, it embodies an entire evolutionary epic going back more than 200 million years.”

The discovery comes from a handful of specimens including an extraordinarily complete and well-preserved fossil skeleton excavated from a site centered around an Allosaurus nest in northern Wyoming’s Morrison Formation. Further study of the find could help reveal why this animal’s ancient order of reptiles were winnowed down from being diverse and numerous in the Jurassic to just New Zealand’s tuatara surviving today.

The tuatara looks a bit like a particularly stout iguana, but the tuatara and its newly discovered relative are in fact not lizards at all. They are actually rhynchocephalians, an order that diverged from lizards at least 230 million years ago, Carrano said.

In their Jurassic heyday, rhynchocephalians were found nearly worldwide, came in sizes large and small, and filled ecological roles ranging from aquatic fish hunters to bulky plant munchers. But for reasons that still are not fully understood, rhynchocephalians all but disappeared as lizards and snakes grew to be the more common and more diverse reptiles across the globe.

This evolutionary chasm between lizards and rhynchocephalians helps explain the tuatara’s odd features such as teeth fused to the jaw bone, a unique chewing motion that slides the lower jaw back and forth like a saw blade, a 100-year-plus lifespan and a tolerance for colder climates.

Following O. gregori’s formal description, Carrano said the fossil has been added to the museum’s collections where it will remain available for future study, perhaps one day helping researchers figure out why the tuatara is all that remains of the rhynchocephalians, while lizards are now found across the globe.

“These animals may have disappeared partly because of competition from lizards but perhaps also due to global shifts in climate and changing habitats,” Carrano said. “It’s fascinating when you have the dominance of one group giving way to another group over evolutionary time, and we still need more evidence to explain exactly what happened, but fossils like this one are how we will put it together.”

The researchers named the new species after museum volunteer Joseph Gregor who spent hundreds of hours meticulously scraping and chiseling the bones from a block of stone that first caught museum fossil preparator Pete Kroehler’s eye back in 2010.

“Pete is one of those people who has a kind of X-ray vision for this sort of thing,” Carrano said. “He noticed two tiny specks of bone on the side of this block and marked it to be brought back with no real idea what was in it. As it turns out, he hit the jackpot.”

The fossil is almost entirely complete, with the exception of the tail and parts of the hind legs. Carrano said that such a complete skeleton is rare for small prehistoric creatures like this because their frail bones were often destroyed either before they fossilized or as they emerge from an eroding rock formation in the present day. As a result, rhynchocephalians are mostly known to paleontologists from small fragments of their jaws and teeth.

After Kroehler, Gregor and others had freed as much of the tiny fossil from the rock as was practical given its fragility, the team, led by DeMar, set about scanning the fossil with high-resolution computerized tomography (CT), a method that uses multiple X-ray images from different angles to create a 3D representation of the specimen. The team used three separate CT scanning facilities, including one housed at the National Museum of Natural History, to capture everything they possibly could about the fossil.

Once the fossil’s bones had been digitally rendered with accuracy smaller than a millimeter, DeMar set about reassembling the digitized bones of the skull, some of which were crushed, out of place or missing on one side, using software to eventually create a nearly complete 3D reconstruction. The reconstructed 3D skull now provides researchers an unprecedented look at this Jurassic-age reptile’s head.

Given Opisthiamimus’s diminutive size, tooth shape and rigid skull, it likely ate insects, said DeMar, adding that prey with harder shells such as beetles or water bugs might have also been on the menu. Broadly speaking, the new species looks quite a bit like a miniaturized version of its only surviving relative (tuataras are about five times longer).

“Such a complete specimen has huge potential for making comparisons with fossils collected in the future and for identifying or reclassifying specimens already sitting in a museum drawer somewhere,” DeMar said. “With the 3D models we have, at some point we could also do studies that use software to look at this critter’s jaw mechanics.”

Funding and support for this research were provided by the Smithsonian and the Australian Research Council.

Reference:
David G. DeMar, Marc E. H. Jones, Matthew T. Carrano. A nearly complete skeleton of a new eusphenodontian from the Upper Jurassic Morrison Formation, Wyoming, USA, provides insight into the evolution and diversity of Rhynchocephalia (Reptilia: Lepidosauria). Journal of Systematic Palaeontology, 2022; 20 (1) DOI: 10.1080/14772019.2022.2093139

Note: The above post is reprinted from materials provided by Smithsonian.

Diamonds and rust at Earth’s core-mantle boundary

The iron-carbon alloy reacted with water at high pressure and high temperature conditions related to the Earth’s deep mantle in a diamond-anvil cell.
The iron-carbon alloy reacted with water at high pressure and high temperature conditions related to the Earth’s deep mantle in a diamond-anvil cell.

Steel rusts by water and air on the Earth’s surface. But what about deep inside the Earth’s interior?

The Earth’s core is the largest carbon storage on Earth — roughly 90% is buried there. Scientists have shown that the oceanic crust that sits on top of tectonic plates and falls into the interior, through subduction, contains hydrous minerals and can sometimes descend all the way to the core-mantle boundary. The temperature at the core-mantle boundary is at least twice as hot as lava, and high enough that water can be released from the hydrous minerals. Therefore, a chemical reaction similar to rusting steel could occur at Earth’s core-mantle boundary.

Byeongkwan Ko, a recent Arizona State University PhD graduate, and his collaborators published their findings on the core-mantle boundary in Geophysical Research Letters. They conducted experiments at the Advanced Photon Source at Argonne National Laboratory, where they compressed iron-carbon alloy and water together to the pressure and temperature expected at the Earth’s core-mantle boundary, melting the iron-carbon alloy.

The researchers found that water and metal react and make iron oxides and iron hydroxides, just like what happens with rusting at Earth’s surface. However, they found that for the conditions of the core-mantle boundary carbon comes out of the liquid iron-metal alloy and forms diamond.

“Temperature at the boundary between the silicate mantle and the metallic core at 3,000 km depth reaches to roughly 7,000 F, which is sufficiently high for most minerals to lose H2O captured in their atomic scale structures,” said Dan Shim, professor at ASU’s School of Earth and Space Exploration. “In fact, the temperature is high enough that some minerals should melt at such conditions.”

Because carbon is an iron loving element, significant carbon is expected to exist in the core, while the mantle is thought to have relatively low carbon. However, scientists have found that much more carbon exists in the mantle than expected.

“At the pressures expected for the Earth’s core-mantle boundary, hydrogen alloying with iron metal liquid appears to reduce solubility of other light elements in the core,” said Shim. “Therefore, solubility of carbon, which likely exists in the Earth’s core, decreases locally where hydrogen enters into the core from the mantle (through dehydration). The stable form of carbon at the pressure-temperature conditions of Earth’s core-mantle boundary is diamond. So the carbon escaping from the liquid outer core would become diamond when it enters into the mantle.”

“Carbon is an essential element for life and plays an important role in many geological processes,” said Ko. “The new discovery of a carbon transfer mechanism from the core to the mantle will shed light on the understanding of the carbon cycle in the Earth’s deep interior. This is even more exciting given that the diamond formation at the core-mantle boundary might have been going on for billions of years since the initiation of subduction on the planet.”

Ko’s new study shows that carbon leaking from the core into the mantle by this diamond formation process may supply enough carbon to explain the elevated carbon amounts in the mantle. Ko and his collaborators also predicted that diamond rich structures can exist at the core-mantle boundary and that seismic studies might detect the structures because seismic waves should travel unusually fast for the structures.

“The reason that seismic waves should propagate exceptionally fast through diamond-rich structures at the core-mantle boundary is because diamond is extremely incompressible and less dense than other materials at the core-mantle boundary,” said Shim.

Ko and team will continue investigating how the reaction can also change the concentration of other light elements in the core, such as silicon, sulfur and oxygen, and how such changes can impact the mineralogy of the deep mantle.

Reference:
Byeongkwan Ko, Stella Chariton, Vitali Prakapenka, Bin Chen, Edward J. Garnero, Mingming Li, Sang‐Heon Shim. Water‐Induced Diamond Formation at Earth’s Core‐Mantle Boundary. Geophysical Research Letters, 2022; 49 (16) DOI: 10.1029/2022GL098271

Note: The above post is reprinted from materials provided by Arizona State University. Original written by Andrea Chatwood.

Early gibbon fossil found in southwest China: Discovery fills evolutionary history gap of apes

The upper jaw of the infant of Yuanmoupithecus. Image courtesy of Terry Harrison, NYU's Department of Anthropology.
The upper jaw of the infant of Yuanmoupithecus. Image courtesy of Terry Harrison, NYU’s Department of Anthropology.

A team of scientists has discovered the earliest gibbon fossil, a find that helps fill a long-elusive evolutionary gap in the history of apes.

The work, reported in the Journal of Human Evolution, centers on hylobatids, a family of apes that includes 20 species of living gibbons, which are found throughout tropical Asia from northeastern India to Indonesia.

“Hylobatids fossil remains are very rare, and most specimens are isolated teeth and fragmentary jaw bones found in cave sites in southern China and southeast Asia dating back no more than 2 million years ago,” explains Terry Harrison, a professor of anthropology at New York University and one of the paper’s authors. “This new find extends the fossil record of hylobatids back to 7 to 8 million years ago and, more specifically, enhances our understanding of the evolution of this family of apes.”

The fossil, discovered in the Yuanmou area of Yunnan Province in southwestern China, is of a small ape called Yuanmoupithecus xiaoyuan. The analysis, which included Xueping Ji of the Kunming Institute of Zoology and the lead author of the study, focused on the teeth and cranial specimens of Yuanmoupithecus, including an upper jaw of an infant that was less than 2 years old when it died.

Using the size of the molar teeth as a guide, the scientists estimate that Yuanmoupithecus was similar in size to today’s gibbons, with a body weight of about 6 kilograms — or about 13 pounds.

“The teeth and the lower face of Yuanmoupithecus are very similar to those of modern-day gibbons, but in a few features the fossil species was more primitive and points to it being the ancestor of all the living species,” observes Harrison, part of NYU’s Center for the Study of Human Origins.

Ji found the infant upper jaw during his field survey and identified it as a hylobatid by comparing it with modern gibbon skulls in the Kunming Institute of Zoology. In 2018, he invited Harrison and other colleagues to work on the specimens stored in the Yunnan Institute of Cultural Relics and Archaeology and the Yuanmou Man Museum that had been collected over the past 30 years.

“The remains of Yuanmoupithecus are extremely rare, but with diligence it has been possible to recover enough specimens to establish that the Yuanmou fossil ape is indeed a close relative of the living hylobatids,” notes Harrison.

The Journal of Human Evolution study also found that Kapi ramnagarensis, which has been claimed to be an earlier species of hylobatid, based on a single isolated fossil molar from India, is not a hylobatid after all, but a member of a more primitive group of primates that are not closely related to modern-day apes.

“Genetic studies indicate that the hylobatids diverged from the lineage leading to the great apes and humans about 17 to 22 million years ago, so there is still a 10-million-year gap in the fossil record that needs to be filled,” Harrison cautions. “With continued exploration of promising fossil sites in China and elsewhere in Asia, it is hoped that additional discoveries will help fill these critical gaps in the evolutionary history of hylobatids.”

The researchers also received access to skeletal and paleontological collections at the American Museum of Natural History in New York and the Smithsonian Institution’s National Museum of Natural History in Washington D.C., among others, in conducting their study.

Reference:
Xueping Ji, Terry Harrison, Yingqi Zhang, Yun Wu, Chunxia Zhang, Jinming Hu, Dongdong Wu, Yemao Hou, Song Li, Guofu Wang, Zhenzhen Wang. The earliest hylobatid from the Late Miocene of China. Journal of Human Evolution, 2022; 171: 103251 DOI: 10.1016/j.jhevol.2022.103251

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

Wave created by Tonga volcano eruption reached 90 meters — nine times taller than 2011 Japan tsunami

The eruption created an initial wave 90 metres high – almost the height of the Statue of Liberty
The eruption created an initial wave 90 metres high – almost the height of the Statue of Liberty

The initial tsunami wave created by the eruption of the underwater Hunga Tonga Ha’apai volcano in Tonga in January 2022 reached 90 metres in height, around nine times taller than that from the highly destructive 2011 Japan tsunami, new research has found.

An international research team says the eruption should serve as a wake-up call for international groups looking to protect people from similar events in future, claiming that detection and monitoring systems for volcano-based tsunamis are ’30 years behind’ comparable tools used to detect earthquake-based events.

Dr Mohammad Heidarzadeh, Secretary-General of the International Tsunami Commission and a senior lecturer in the University of Bath’s Department of Architecture & Civil Engineering, authored the research alongside colleagues based in Japan, New Zealand, the UK and Croatia.

By comparison, the largest tsunami waves due to earthquakes before the Tonga event were recorded following the Tōhoku earthquake near Japan in 2011 and the 1960 Chilean earthquake, reached 10 metres in initial height. Those were more destructive as they happened closer to land, with waves that were wider.

Dr Heidarzadeh says the Tonga tsunami should serve as a wake-up call for more preparedness and understanding of the causes and signs of tsunamis cause by volcanic eruptions. He says: “The Tongan tsunami tragically killed five people and caused large scale destruction, but its effects could have been even greater had the volcano been located closer to human communities. The volcano is located approximately 70 km from the Tongan capital Nuku’alofa — this distance significantly minimized its destructive power.

“This was a gigantic, unique event and one that highlights that internationally we must invest in improving systems to detect volcanic tsunamis as these are currently around 30 years behind the systems we used to monitor for earthquakes. We are under-prepared for volcanic tsunamis.”

The research was carried out by analysing ocean observation data recordings of atmospheric pressure changes and sea level oscillations, in combination with computer simulations validated with real-world data.

The research team found that the tsunami was unique as the waves were created not only by the water displaced by the volcano’s eruption, but also by huge atmospheric pressure waves, which circled around the globe multiple times. This ‘dual mechanism’ created a two-part tsunami — where initial ocean waves created by the atmospheric pressure waves were followed more than one hour later by a second surge created by the eruption’s water displacement.

This combination meant tsunami warning centres did not detect the initial wave as they are programmed to detect tsunamis based on water displacements rather than atmospheric pressure waves.

The research team also found that the January event was among very few tsunamis powerful enough to travel around the globe — it was recorded in all world’s oceans and large seas from Japan and the United States’ western seaboard in the North Pacific Ocean to the coasts within the Mediterranean Sea.

The paper, co-authored by colleagues from New Zealand’s GNS Science, the Association for the Development of Earthquake Prediction in Japan, the University of Split in Croatia and at London’s Brunel University, was published this week in Ocean Engineering.

Dr Aditya Gusman, Tsunami Modeller at the New Zealand-based geoscience service, says: “The 2018 Anak Krakatau volcano and 2022 Hunga Tonga-Hunga Ha’apai volcano eruptions clearly showed us that coastal areas surrounding volcano islands are at risk of being hit by destructive tsunamis. Although it may be preferable to have low-lying coastal areas completely clear from residential buildings, such a policy may not be practical for some places as volcanic tsunamis can be considered infrequent events.”

Co-author Dr Jadranka Šepić, from the University of Split, Croatia, adds: “What is important is to have efficient warning systems, which include both real-time warnings and education on what to do in a case of a tsunami or warning — such systems save lives. In addition, at volcanic areas, monitoring of volcanic activity should be organized, and more high-quality research into volcanic eruptions and areas at hazard is always a good idea.”

Separate research led by the University of Bath atmospheric physicist Dr Corwin Wright published in June found that the Tonga eruption triggered atmospheric gravity waves that reached the edge of space.

Reference:
Mohammad Heidarzadeh, Aditya Riadi Gusman, Takeo Ishibe, Ramtin Sabeti, Jadranka Šepić. Estimating the eruption-induced water displacement source of the 15 January 2022 Tonga volcanic tsunami from tsunami spectra and numerical modelling. Ocean Engineering, 2022; 261: 112165 DOI: 10.1016/j.oceaneng.2022.112165

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

Geological carbon sequestration in mantle rocks prevents large earthquakes in parts of the San Andreas Fault

Outcrop of carbonate-altered mantle rock in the San Andreas Fault area. A recent study shows that carbon sequestration in mantle rocks may prevent large earthquakes in parts of the San Andreas Fault. (Photo by Frieder Klein, © Woods Hole Oceanographic Institution)
Outcrop of carbonate-altered mantle rock in the San Andreas Fault area. A recent study shows that carbon sequestration in mantle rocks may prevent large earthquakes in parts of the San Andreas Fault. (Photo by Frieder Klein, © Woods Hole Oceanographic Institution)

The San Andreas Fault in California is renowned for its large and infrequent earthquakes. However, some segments of the San Andreas Fault (SAF) instead are characterized by frequent quakes of small to moderate magnitude and high rates of continuous or episodic aseismic creep. With tectonic strain released in a quasi-steady motion, that reduces the potential for large earthquakes along those segments.

Now, researchers say ubiquitous evidence for ongoing geological carbon sequestration in mantle rocks in the creeping sections of the SAF is one underlying cause of aseismic creep along a roughly 150 kilometer-long SAF segment between San Juan Bautista and Parkfield, California, and along several other fault segments.

“Although there is no consensus regarding the underlying cause of aseismic creep, aqueous fluids and mechanically weak minerals appear to play a central role,” researchers say in a new paper, “Carbonation of serpentinite in creeping faults of California,” published in Geophysical Research Letters.

The new study integrates field observations and thermodynamic modeling “to examine possible relationships between the occurrence of serpentinite, silica-carbonate rock, and CO2-rich aqueous fluids in creeping faults of California,” the paper states. “Our models predict that carbonation of serpentinite leads to the formation of talc and magnesite, followed by silica-carbonate rock. While abundant exposures of silica-carbonate rock indicate complete carbonation, serpentinite hosted CO2-rich spring fluids are strongly supersaturated with talc at elevated temperatures. Hence, carbonation of serpentinite is likely ongoing in parts of the San Andres Fault system and operates in conjunction with other modes of talc formation that may further enhance the potential for aseismic creep, thereby limiting the potential for large earthquakes.”

The paper indicates that because wet talc is a mechanically weak mineral, “its formation through carbonation promotes tectonic movements without large earthquakes.”

The researchers recognized several possible underlying mechanisms causing aseismic creep in the SAF, and they also noted that because the rates of aseismic creep are significantly higher in some parts of the SAF system, an additional or different mechanism — the carbonation of serpentinite — is needed to account for the full extent of the creep.

With fluids basically everywhere along the SAF, but with only certain portions of the fault being lubricated, researchers considered that a rock could be responsible for the lubrication. Some earlier studies had suggested that the lubricant could be talc, a soft and slippery component that is commonly used in baby powder. A well-established mechanism for forming talc is by adding silica to mantle rocks. However, the researchers here focused on another talc-forming mechanism: adding CO2 to mantle rocks to form soapstone.

“The addition of CO2 to mantle rocks — which is the mineral carbonation or carbon sequestration process — had not previously been investigated in the context of earthquake formation or the natural prevention of earthquakes. Using basic geological constraints, our study showed where these carbonate-altered mantle rocks are and where there are springs along the fault line in California that are enriched in CO2. It turned out that when you plot the occurrence and distribution of these rock types and the occurrence of CO2-rich springs in California, they all line up along the San Andreas Fault in creeping sections of the fault where you don’t have major earthquakes,” said Frieder Klein, lead author of the journal article.

Klein, an associate scientist in the Marine Chemistry and Geochemistry Department at the Woods Hole Oceanographic Institution, explained that carbonation is basically the uptake of CO2 by a rock. Klein noted that he had used existing U.S. Geological Survey databases and Google Earth to plot the locations of carbonate-altered rocks and CO2-rich springs.

“The geological evidence suggests that this mineral carbonation process is taking place and that talc is an intermediary reaction product of that process,” Klein said. Although researchers did not find soapstone on mantle rock outcrops, results from theoretical models “strongly suggest that carbonation is an ongoing process and that soapstone indeed could form in the SAF at depth,” the paper notes.

These theoretical models “suggest that carbon sequestration with the SAF is taking place today and that the process is actively helping to lubricate the fault and minimize strong earthquakes in the creeping portions of the SAF,” Klein said.

The paper also notes that this mechanism may also be present in other fault systems. “Because CO2-rich aqueous fluids and ultramafic rocks are particularly common in young orogenic belts and subduction zones, the formation of talc via mineral carbonation may play a critical role in controlling the seismic behavior of major tectonic faults around the world.”

“Our study allows us to better understand the fundamental processes that are taking place within fault zones where these ingredients are present, and allows us to better understand the seismic behavior of these faults, some of which are in densely populated areas and some of which are in lightly populated or oceanic settings,” Klein said.

This work was supported by grants from the National Science Foundation.

Reference:
Frieder Klein, David L. Goldsby, Jian Lin, Muriel Andreani. Carbonation of Serpentinite in Creeping Faults of California. Geophysical Research Letters, 2022; 49 (15) DOI: 10.1029/2022GL099185

Note: The above post is reprinted from materials provided by Woods Hole Oceanographic Institution.

More than one asteroid could have spelled doom for the dinosaurs

Earth is bombarded at random-GeologyPage
A thankfully rare event: an asteroid hits the Earth. (Visualisations: iStock / Solarseven)

A newly discovered impact crater below the seafloor hints at the possibility that more than one asteroid hit Earth during the time when dinosaurs went extinct.

Scientists have found evidence of an asteroid impact crater beneath the North Atlantic Ocean that could force researchers to rethink how the dinosaurs reached the end of their reign.

The team believes the crater was caused by an asteroid colliding with Earth around 66 million years ago—around the same time that the Chicxulub asteroid hit Earth off the coast of today’s Yucatan, Mexico, and wiped out the dinosaurs.

Spanning more than 5 miles in diameter, the crater was discovered using seismic measurements, which allow scientists to probe what lies deep below Earth’s surface.

Veronica Bray, a research scientist in the University of Arizona Lunar and Planetary Laboratory, who specializes in craters found throughout the solar system, is a co-author of a study in Science Advances detailing the discovery.

Named after a nearby seamount, the Nadir crater is buried up to 1,300 feet below the seabed about 250 miles off the coast of Guinea, West Africa. The team believes the asteroid that created the newly discovered Nadir crater could have formed by breakup of a parent asteroid or by a swarm of asteroids in that time period. If confirmed, the crater will be one of less than 20 confirmed marine impact craters found on Earth.

What impact would the asteroid have had?

Bray used computer simulations to determine what kind of collision took place and what the effects might have been. The simulations suggest the crater was caused by the collision of a 1,300 foot-wide asteroid in 1,600 to 2,600 feet of water.

“This would have generated a tsunami over 3,000 feet high, as well as an earthquake of more than magnitude 6.5,” Bray said. “Although it is a lot smaller than the global cataclysm of the Chicxulub impact, Nadir will have contributed significantly to the local devastation. And if we have found one ‘sibling’ to Chicxulub, it opens the question: Are there others?”

The estimated size of the asteroid would put it roughly on par with asteroid Bennu, the target of the UArizona-led NASA asteroid sample return mission OSIRIS-REx. According to Bray’s calculations, the energy released from the impact that caused the Nadir crater would have been around 1,000 times greater than the tsunami caused by the underwater eruption of the Hunga Tonga-Hunga Ha’apai volcano in the Polynesian country of Tonga on January 15.

“These are preliminary simulations and need to be refined when we get more data,” Bray said, “but they provide important new insights into the possible ocean depths in this area at the time of impact.”

What does the crater look like?

Uisdean Nicholson, a geologist at Heriot-Watt University in Edinburgh, discovered the crater somewhat by accident, while examining seismic reflection data from the seabed during a research project dedicated to seafloor spreading, the geologic process that caused the African and American continents to drift apart, thereby opening the Atlantic Ocean.

“I’ve interpreted lots of seismic data in my time, but had never seen anything like this. Instead of the flat sedimentary sequences I was expecting on the plateau, I found an 8.5-kilometer depression under the seabed, with very unusual characteristics,” Nicholson said. “It has particular features that point to a meteor impact crater. It has a raised rim and a very prominent central uplift, which is consistent for large impact craters.

“It also has what looks like ejecta outside the crater, with very chaotic sedimentary deposits extending for tens of kilometers outside of the crater,” he added. “The characteristics are just not consistent with other crater-forming processes like salt withdrawal or the collapse of a volcano.”

The asteroid crashed around same time as the dinosaur killer

“The Nadir Crater is an incredibly exciting discovery of a second impact close in time to the Cretaceous–Paleogene extinction,” said study co-author Sean Gulick, an impact expert at the University of Texas at Austin. “While much smaller than the extinction causing Chicxulub impactor, its very existence requires us to investigate the possibility of an impact cluster in the latest Cretaceous.”

While the seismic data indicate that the sediments impacted by the asteroid correspond with the Cretaceous-Paleogene boundary—a sedimentary layer demarcating the end of the Cretaceous period and last known occurrence of dinosaurs—there is some uncertainty about the precise time of impact, limited by the resolution of the data.

“Despite 4 billion years of impactors hitting Earth, only 200 have been discovered,” Gulick said. “It is thus exciting news whenever a new potential impact is discovered, especially in the hard-to-explore marine environment.”

Nicholson has applied for funding to drill into the seabed to confirm that it’s an asteroid impact crater and test its precise age.

Reference:
Uisdean Nicholson et al, The Nadir Crater offshore West Africa: A candidate Cretaceous-Paleogene impact structure, Science Advances (2022). DOI: 10.1126/sciadv.abn3096

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

Fossils of giant sea lizard that ruled the oceans 66 million years ago discovered

Thalassotitan atrox grew up to 12 metres (40 feet) and was at the top of the food chain.
Thalassotitan atrox grew up to 12 metres (40 feet) and was at the top of the food chain.

Researchers have discovered a huge new mosasaur from Morocco, named Thalassotitan atrox, which filled the apex predator niche. With massive jaws and teeth like those of killer whales, Thalassotitan hunted other marine reptiles — plesiosaurs, sea turtles, and other mosasaurs.

At the end of the Cretaceous period, 66 million years ago, sea monsters really existed. While dinosaurs flourished on land, the seas were ruled by the mosasaurs, giant marine reptiles.

Mosasaurs weren’t dinosaurs, but enormous marine lizards growing up to 12 metres (40 feet) in length. They were distant relatives of modern iguanas and monitor lizards.

Mosasaurs looked like a Komodo dragon with flippers instead of legs, and a shark-like tail fin. Mosasaurs became larger and more specialised in the last 25 million years of the Cretaceous, taking niches once filled by marine reptiles like plesiosaurs and ichthyosaurs. Some evolved to eat small prey like fish and squid. Others crushed ammonites and clams. The new mosasaur, named Thalassotitan atrox, evolved to prey on all the other marine reptiles.

The remains of the new species were dug up in Morocco, about an hour outside Casablanca. Here, near the end of the Cretaceous, the Atlantic flooded northern Africa. Nutrient rich waters upwelling from the depths fed blooms of plankton. Those fed small fish, feeding larger fish, which fed mosasaurs and plesiosaurs — and so on, with these marine reptiles becoming food for the giant, carnivorous Thalassotitan.

Thalassotitan, had an enormous skull measuring 1.4 metres (5 feet long), and grew to nearly 30 feet (9 metres) long, the size of a killer whale. While most mosasaurs had long jaws and slender teeth for catching fish, Thalassotitan had a short, wide muzzle and massive, conical teeth like those of an orca. These let it seize and rip apart huge prey. These adaptations suggest Thalassotitan was an apex predator, sitting at the top of the food chain. The giant mosasaur occupied the same ecological niche as today’s killer whales and great white sharks.

Thalassotitan’s teeth are often broken and worn, however eating fish wouldn’t have produced this sort of tooth wear. Instead, this suggests that the giant mosasaur attacked other marine reptiles, chipping, breaking, and grinding its teeth as it bit into their bones and tore them apart. Some teeth are so heavily damaged they have been almost ground down to the root.

Fossilised remains of prey

Remarkably, possible remains of Thalassotitan’s victims have been discovered. Fossils from the same beds show damage from acids, with teeth and bone eaten away. Fossils with this peculiar damage include large predatory fish, a sea turtle, a half-meter long plesiosaur head, and jaws and skulls of at least three different mosasaur species. They would have been digested in Thalassotitan’s stomach before it spat out their bones.

“It’s circumstantial evidence,” said Dr Nick Longrich, Senior Lecturer from the Milner Centre for Evolution at the University of Bath and lead author on the study, published in Cretaceous Research.

“We can’t say for certain which species of animal ate all these other mosasaurs. But we have the bones of marine reptiles killed and eaten by a large predator.

“And in the same location, we find Thalassotitan, a species that fits the profile of the killer — it’s a mosasaur specialised to prey on other marine reptiles. That’s probably not a coincidence.”

Thalassotitan was a threat to everything in the oceans — including other Thalassotitan. The huge mosasaurs bear injuries sustained in violent combat with other mosasaurs, with injuries to their face and jaws sustained in fights. Other mosasaurs show similar injuries, but in Thalassotitan these wounds were exceptionally common, suggesting frequent, intense fights over feeding grounds or mates.

“Thalassotitan was an amazing, terrifying animal,” said Dr Nick Longrich, who led the study. “Imagine a Komodo Dragon crossed with a great white shark crossed with a T. rex crossed with a killer whale.”

The new mosasaur lived in the final million years of the Age of Dinosaurs, a contemporary of animals like T. rex and Triceratops. Along with recent discoveries of mosasaurs from Morocco, it suggests that mosasaurs weren’t in decline before the asteroid impact that drove the Cretaceous mass extinction. Instead, they flourished.

Professor Nour-Eddine Jalil, a co-author on the paper from the Museum of Natural History in Paris, said: “The phosphate fossils of Morocco offer an unparalleled window on the paleobiodiversity at the end of Cretaceous.

“They tell us how life was rich and diversified just before the end of the ‘dinosaur era’, where animals had to specialise to have a place in their ecosystems. Thalassotitan completes the picture by taking on the role of the megapredator at the top of the food chain.”

“There’s so much more to be done,” said Longrich. “Morocco has one of the richest and most diverse marine faunas known from the Cretaceous. We’re just getting started understanding the diversity and the biology of the mosasaurs.”

Reference:
Nicholas R. Longrich, Nour-Eddine Jalil, Fatima Khaldoune, Oussama Khadiri Yazami, Xabier Pereda-Suberbiola, Nathalie Bardet. Thalassotitan atrox, a giant predatory mosasaurid (Squamata) from the Upper Maastrichtian Phosphates of Morocco. Cretaceous Research, 2022; 105315 DOI: 10.1016/j.cretres.2022.105315

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

Mineral-microbe interactions play important roles in geological and environmental processes

An anaerobic, motile, gram-positive bacterium adheres to the molybdenite (MoS2) surface to uptake the trace elements from the mineral structure for cell synthesis. Credit: Science China Press
An anaerobic, motile, gram-positive bacterium adheres to the molybdenite (MoS2) surface to uptake the trace elements from the mineral structure for cell synthesis. Credit: Science China Press

In a paper published in National Science Review, a team of scientists critically summarize major advances in mineral-microbe interactions, including molecular mechanisms of interactions and macroscopic manifestations of such interactions through time. Major challenges and future research opportunities are identified.

Minerals are the fundamental components of Earth. Microbes occupy the majority of the tree of life. In near surficial environments, minerals and microbes co-exist and interact. The studies of mineral-microbe interactions have blossomed in the last two decades, because such interactions drive major geological events and substantially determine the habitability of the Earth. A research team led by Dr. Hailiang Dong from China University of Geosciences (Beijing) has critically reviewed the mineral-microbe interactions and their coevolution, and proposed major research opportunities and challenges in the future.

Minerals and microbes mutually interact across all spatial and temporal scales. While many minerals offer protection and supply nutrients/energy to support microbial growth and metabolism, other minerals may release bio-toxic substances and produce reactive oxygen species (ROS) to limit and even to kill microorganisms. In return, microbes actively dissolve, precipitate, and transform minerals through metabolism, which may produce special biosignatures in geological record.

Throughout Earth history, both minerals and microbes increase their species diversity and functional complexity. In a prebiotic world, minerals catalyze synthesis of biological molecules and play an essential role in life emergence. Subsequently, mineral evolution drives microbial innovation through their changes of physiochemical properties through time. Microbial evolution in turn drives mineral diversification through their unique metabolism. Therefore, the evolving mineral-microbe interactions over geological time play critical roles in driving geological events such as occurrence of the Great Oxidation Event and the formation of large ore deposits.

Mineral-microbe interactions have many biotechnological applications including bioleaching of precious metals and manufacturing of mineral fertilizers, remediation of heavy metal and organic pollutants, biosynthesis of novel materials and CO2 sequestration. Despite recent advances, the authors identify major research questions for future research.

First, the roles of minerals in supporting microbial ecology are only qualitatively recognized at present. Traditional culture media do not consider minerals as important nutrients and energy, which may be one of the reasons for a low success rate of obtaining pure cultures. Mineral-based culture media should recover more microbial resources.

Second, it is challenging to distinguish biogenic minerals from abiogenic ones. A syngenetic assemblage of minerals that combine morphological, structural/textural, and geochemical evidence is more meaningful to search for the biological footprints in geological record and on other planets.

Third, it is imperative to link laboratory mechanistic investigations to field observations. Through an iterative approach mineral-microbe interactions may be inferred through time.

Fourth, manipulation of mineral-microbe interactions can benefit the humankind, such as CO2 sequestration and mitigation of the global warming effect, resource recovery, environmental protection, and manufacturing of novel materials.

Reference:
Hailiang Dong et al, A critical review of mineral-microbe interaction and coevolution: mechanisms and applications, National Science Review (2022). DOI: 10.1093/nsr/nwac128

Note: The above post is reprinted from materials provided by Science China Press.

Dinosaurs evolved different eye socket shapes to allow stronger bites

Skull and life reconstruction of Tyrannosaurus rex with original eye socket and eye (left) and hypothetical reconstruction with circular eye socket and enlarged eye (right). (Image credit: Dr Stephan Lautenschlager, University of Birmingham).
Skull and life reconstruction of Tyrannosaurus rex with original eye socket and eye (left) and hypothetical reconstruction with circular eye socket and enlarged eye (right). (Image credit: Dr Stephan Lautenschlager, University of Birmingham).

Large dinosaur predators, such as Tyrannosaurus rex, evolved different shapes of eye sockets to better deal with high bite forces, new research has shown.

While in many animals — and most dinosaurs — the eye socket is just a circular hole in the skull housing the eyeball, this is very different in large carnivores.

In a new study, published today in Communications Biology, researchers at the University of Birmingham reveal how the unusual elliptical, or oval eye sockets found in the skulls of these predators, could have evolved to help the skull absorb impact as they pounced on prey.

Dr Stephan Lautenschlager, Senior Lecturer for Palaeobiology at the University of Birmingham and author of the new study, analysed the shape of the eye sockets of ca. 500 different dinosaurs and related species.

“The results show that only some dinosaurs had eye sockets that were elliptical or keyhole-shaped,” said Dr Stephan Lautenschlager. “However, all of those were large, carnivorous dinosaurs with skull lengths of 1 m or more.”

Using computer simulations and stress analysis, Dr Lautenschlager tested what purpose these unusual eye socket shapes could have.

The results demonstrated that a skull with a circular eye socket was more prone to high stresses during biting. However, if these were replaced with other eye socket shapes stresses were considerably reduced allowing top predators, including Tyrannosaurus rex, to evolve high bite forces without compromising skull stability.

The study also showed that most plant-eating species and juvenile individuals retained a circular eye socket. Only large carnivores adopted other morphologies, such as elliptical, keyhole-shaped or figure-of-eight-shaped eye sockets.

Dr Lautenschlager added: “In these species, just the upper part of the eye socket was actually occupied by the eyeball. This also led to a relative reduction of eye size compared with skull size.”

The researchers also investigated what would have happened if eye size had increased at the same rate as skull length. In such a case, the eyes of Tyrannosaurus rex would have been up to 30 cm in diameter and weighing nearly 20 kg (instead of estimated 13 cm and 2 kg).

Reference:
Stephan Lautenschlager. Functional and ecomorphological evolution of orbit shape in mesozoic archosaurs is driven by body size and diet. Communications Biology, 2022; 5 (1) DOI: 10.1038/s42003-022-03706-0

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

Crucial evidence explains anomalously fast convergence between India and Asia in Mesozoic

The southern-central edge of the Tibetan Plateau near the border with western Nepal and the Indian state of Sikkim is pictured in this Sentinel-2A image from 1 February 2016. Credit: European Space Agency. Contains modified Copernicus Sentinel data [2016]/ processed by ESA ,CC BY-SA 3.0 IGO/Wikimedia Commons
The southern-central edge of the Tibetan Plateau near the border with western Nepal and the Indian state of Sikkim is pictured in this Sentinel-2A image from 1 February 2016. Credit: European Space Agency. Contains modified Copernicus Sentinel data [2016]/ processed by ESA ,CC BY-SA 3.0 IGO/Wikimedia Commons
Closure of the Neo-Tethys Ocean and the subsequent formation of the Tibetan Plateau is one of the most significant tectonic events on Earth. How the Indian subcontinent drifted northward anomalously fast and collided with Asia is an essential question in describing global changes in tectonics, climate and ecosystems.

Double subduction of the Neo-Tethys Ocean is a leading model in interpreting this anomalous convergence speed. But no compelling evidence from the entire Himalaya and adjacent regions has been reported before.

Recently, Yang Shun, a Ph.D. student at the Institute of Geology and Geophysics (IGG) of the Chinese Academy of Sciences (CAS), under the supervision of Profs. He Yumei and Jiang Mingming, along with their team of collaborators, reported crucial seismic evidence of slab remnants in the present upper mantle to strongly support the double subduction model.

This work was published in Science Advances on August 26.

The Myanmar region occupies the eastern end of the Indian-Asian collisional system. Due to less reworking from continental collision, it is an ideal place to probe possible slab remnants of double subduction. However, until recently, it was a blank area for seismic observation and structural imaging of the Earth’s interior.

The research group on the structure of Earth’s deep interior at IGG/CAS has deployed pioneering seismic arrays in association with the China-Myanmar Geophysical Survey in the Myanmar Orogen (CMGSMO) in Myanmar since 2016. Using data from the novel seismic arrays, the researchers investigated upper mantle structures beneath Myanmar with high resolution.

By compiling seismic tomography and waveform modeling, the researchers revealed for the first time two subparallel subducted slabs preserved in the present upper mantle beneath the Neo-Tethyan tectonic regime.

After comparing the new slab image with data on the time-space distribution of subduction-related magmatism and ophiolites in Myanmar, the researchers concluded that the new evidence supports double subduction of the Neo-Tethys Ocean. Further geodynamic numerical modeling subsequently explained why the slab remnants were preserved intact in the upper mantle without breaking off and sinking into the deep.

The study provides convincing, multidisciplinary, geoscientific evidence to consolidate the double subduction model of the Neo-Tethys Ocean.

Reference:
Shun Yang et al, Slab remnants beneath the Myanmar terrane evidencing double subduction of the Neo-Tethyan Ocean, Science Advances (2022). DOI: 10.1126/sciadv.abo1027.

Note: The above post is reprinted from materials provided by Chinese Academy of Sciences.

New model developed to predict landslides along wildfire burn scars

Steps leading to a debris flow: drought, followed by wildfires, followed by intense precipitation. Credit: Tierney Acott/Institute of Sustainability and Energy at Northwestern
Steps leading to a debris flow: drought, followed by wildfires, followed by intense precipitation. Credit: Tierney Acott/Institute of Sustainability and Energy at Northwestern

A wildfire followed by an intense rainstorm is often a recipe for disaster. Without vegetation to cushion rainfall, water runoff can turn into a fast-moving, highly destructive landslide, called a “debris flow,” which often has the power to wipe out cars, homes and highways—sometimes resulting in casualties.

Northwestern University researchers supported by the U.S. National Science Foundation have augmented a physics-based numerical model to investigate and predict areas susceptible to debris flows.

“Wildfires and their consequences, such as landslides, are exacerbated by the effects of climate change and are resulting in devastation in many regions of the nation,” said Bruce Hamilton, a program director in NSF’s Directorate for Engineering. “This research can help us anticipate and mitigate those impacts.”

This augmented model eventually could be used in an early warning system for people living in high-risk areas, enabling them to evacuate before it’s too late. Information from model simulations could also be used to design new infrastructure—such as diversion bars that deflect fast-moving water away from homes and roads—for high hazard zones.

The research is published in the journal Natural Hazards and Earth System Sciences.

“People want to know about their immediate and future risk,” said Northwestern’s Daniel Horton, the study’s senior author. “Although it’s not yet to operational standards, this modeling framework could one day be instrumental in forecasting where debris flows are likely to occur and deciding who needs to be evacuated.”

As climate change increases the likelihood of wildfires and heavy rains, debris flows also might become more common. Just last year, a debris flow tore out a 150-foot section of roadway along Highway 1 near Big Sur, California. The picturesque two-lane highway was closed for three months, cutting off tourism to the region.

The disaster resulted from a one-two punch: a wildfire that burned from August through December 2020, followed by an atmospheric river—a long, thin string of concentrated moisture in the sky—that dumped nearly a foot of rain the following January.

Following intense rainfall, areas with wildfire burn scars are more susceptible to flash flooding. In a typical situation, vegetation interacts with rain, which then soaks into the ground. But if an area is burned, vegetation is gone, so it can no longer intercept the sudden influx of moisture. Even worse, in some regions, waxes from burned vegetation melts, enters the soil and then solidifies. These waxes create a barrier for rain, blocking it from penetrating the soil. Instead, rain runs over the top of the soil, picking up rocks, mud, trees and even cars to become a debris flow.

“Because of human-caused climate change, the ingredients that lead to debris flows are certainly becoming more common,” Horton said.

Reference:
Chuxuan Li et al, Augmentation and Use of WRF-Hydro to Simulate Overland Flow- and Streamflow-Generated Debris Flow Hazards in Burn Scars (2021). DOI: 10.1002/essoar.10508144.2

Note: The above post is reprinted from materials provided by National Science Foundation.

Prehistoric podiatry: How dinos carried their enormous weight

Computer modelling showed sauropod feet had a soft tissue pad. Image: Dr Andreas Jannel
Computer modelling showed sauropod feet had a soft tissue pad. Image: Dr Andreas Jannel

Scientists have cracked an enduring mystery, discovering how sauropod dinosaurs — like Brontosaurus and Diplodocus — supported their gigantic bodies on land.

A University of Queensland and Monash University-led team used 3D modelling and engineering methods to digitally reconstruct and test the function of foot bones of different sauropods.

Dr Andréas Jannel conducted the research during his PhD studies at UQ’s Dinosaur Lab and said the team found that the hind feet of sauropod had a soft tissue pad beneath the ‘heel’, cushioning the foot to absorb their immense weight.

“We’ve finally confirmed a long-suspected idea and we provide, for the first time, biomechanical evidence that a soft tissue pad — particularly in their back feet — would have played a crucial role in reducing locomotor pressures and bone stresses,” Dr Jannel said.

“It is mind-blowing to imagine that these giant creatures could have been able to support their own weight on land.”

Sauropods were the largest terrestrial animals that roamed the Earth for more than 100 million years.

They were first thought to have been semi-aquatic with water buoyancy supporting their massive weight, a theory disproved by the discovery of sauropod tracks in terrestrial deposits in the mid-twentieth century.

Monash University’s Dr Olga Panagiotopoulou said it had also been thought sauropods had feet similar to a modern-day elephant.

“Popular culture — think Jurassic Park or Walking with Dinosaurs — often depicts these behemoths with almost-cylindrical, thick, elephant-like feet,” Dr Panagiotopoulou said.

“But when it comes to their skeletal structure, elephants are actually ‘tip-toed’ on all four feet, whereas sauropods have different foot configurations in their front and back feet.

“Sauropod’s front feet are more columnar-like, while they present more ‘wedge high heels’ at the back supported by a large soft tissue pad.”

UQ’s Associate Professor Steve Salisbury said this was because sauropods and elephants had different evolutionary origins.

“Elephants belong to an ancient order of mammals called proboscideans, which first appeared in Africa roughly 60 million years ago as small, nondescript herbivores, ” Associate Professor Salisbury said.

“In contrast, sauropods — whose ancestors first appeared 230 million years ago — are more closely related to birds.

“They were agile, two-legged herbivores and it was only later in their evolution that they walked on all fours.

“Crucially, the transition to becoming the largest land animals to walk the earth seems to have involved the adaptation of a heel pad.”

The researchers now plan to use the 3D modelling and engineering methods to make further discoveries.

“I’m keen to apply a similar method to an entire limb and to include additional soft tissue such as muscles, which are rarely preserved in fossils,” Dr Jannel said.

“We’re also excited to study the limbs and feet of other prehistoric animals.

“This should allow us to answer different questions about the biomechanics of extinct animals and better understand their environmental adaptations, movement and lifestyle.”

Reference:
Andréas Jannel, Steven W. Salisbury, Olga Panagiotopoulou. Softening the steps to gigantism in sauropod dinosaurs through the evolution of a pedal pad. Science Advances, 2022; 8 (32) DOI: 10.1126/sciadv.abm8280

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

Evidence that giant meteorite impacts created the continents

Meteorites
Meteorites

New Curtin research has provided the strongest evidence yet that Earth’s continents were formed by giant meteorite impacts that were particularly prevalent during the first billion years or so of our planet’s four-and-a-half-billion year history.

Dr Tim Johnson, from Curtin’s School of Earth and Planetary Sciences, said the idea that the continents originally formed at sites of giant meteorite impacts had been around for decades, but until now there was little solid evidence to support the theory.

“By examining tiny crystals of the mineral zircon in rocks from the Pilbara Craton in Western Australia, which represents Earth’s best-preserved remnant of ancient crust, we found evidence of these giant meteorite impacts,” Dr Johnson said.

“Studying the composition of oxygen isotopes in these zircon crystals revealed a ‘top-down’ process starting with the melting of rocks near the surface and progressing deeper, consistent with the geological effect of giant meteorite impacts.

“Our research provides the first solid evidence that the processes that ultimately formed the continents began with giant meteorite impacts, similar to those responsible for the extinction of the dinosaurs, but which occurred billions of years earlier.”

Dr Johnson said understanding the formation and ongoing evolution of the Earth’s continents was crucial given that these landmasses host the majority of Earth’s biomass, all humans and almost all of the planet’s important mineral deposits.

“Not least, the continents host critical metals such as lithium, tin and nickel, commodities that are essential to the emerging green technologies needed to fulfil our obligation to mitigate climate change,” Dr Johnson said.

“These mineral deposits are the end result of a process known as crustal differentiation, which began with the formation of the earliest landmasses, of which the Pilbara Craton is just one of many.

“Data related to other areas of ancient continental crust on Earth appears to show patterns similar to those recognised in Western Australia. We would like to test our findings on these ancient rocks to see if, as we suspect, our model is more widely applicable.”

Dr Johnson is affiliated with The Institute for Geoscience Research (TIGeR), Curtin’s flagship earth sciences research institute.

The paper, ‘Giant impacts and the origin and evolution of continents’, was published in Nature.

Reference:
Tim E. Johnson, Christopher L. Kirkland, Yongjun Lu, R. Hugh Smithies, Michael Brown, Michael I. H. Hartnady. Giant impacts and the origin and evolution of continents. Nature, 2022; 608 (7922): 330 DOI: 10.1038/s41586-022-04956-y

Note: The above post is reprinted from materials provided by Curtin University. Original written by Lucien Wilkinson.

The speed at which spinosaurid dinosaur teeth were replaced accounts for their overabundance in Cretaceous sites

Spinosaurid dinosaurs teeth
Spinosaurid dinosaurs teeth

This has been confirmed in the article ‘New contributions to the skull anatomy of spinosaurid theropods: Baryonychinae maxilla from the Early Cretaceous of Igea (La Rioja, Spain)’ published in the journal Historical Biology by Iker Isasmendi (lead author) and Xavier Pereda of the UPV/EHU-University of the Basque Country, Pablo Navarro of the UR-University of La Rioja, Angélica Torices, director of the Chair of Palaeontology at the UR, plus other experts of the Complutense University of Madrid and the Palaeontological Visitors’ Centre of La Rioja.

Scientists have reassessed fossil jaw remains published by Viera and Torres in 1995 and found in 1983 in a Lower Cretaceous site at Igea (La Rioja, Spain). The remains constitute a fragment of a left maxilla belonging to a carnivorous dinosaur and in which 8 alveoli have been preserved. Using microCT techniques, they discovered the remains of several teeth developing simultaneously in one of these dental sockets.

“We recognised up to three generations of teeth in the same alveolus: the functional tooth of the animal, another tooth being formed and which would replace the first, and the germ of the one that would end up replacing the second,” explained Pablo Navarro of the UR.

“This suggests very rapid tooth replacement and is probably one of the reasons why so many spinosaurid teeth can be found on the Iberian Peninsula during the Lower Cretaceous,” added the co-author of the paper.

To date, some species of spinosaurids -medium/large carnivorous dinosaurs with elongated skulls and crocodile-like conical teeth- were known to replace their teeth faster than other theropods, in just two months (replacement rate estimated to be 60-68 days); the research confirms that this is a trait shared by the whole group and provides evidence of how this change occurred, i.e. it was made possible by the development of several replacement teeth at the same time.

“Throughout their lives these animals grew new teeth that gradually replaced the original ones and caused them to fall out. This means that the same animal could generate multiple teeth,” said Pablo Navarro.

“These teeth, more or less conical in shape and a centimetre in size, were transported by rivers, accumulated in lake areas and, over time, became fossilised,” said the researcher. They are one of the most common vertebrate remains in Iberian sites of the Lower Cretaceous (between 145 and 113 million years ago).”

Although it is not known precisely why their teeth were replaced so often, it is believed that this allowed them to possess a greater number of functional teeth at all times. This was a decisive advantage when withstanding the considerable effort required to hold their prey by trapping them between their jaws.

In addition to these findings, the research has enabled the classification of the jaw studied to be clarified: the experts do not attribute it, as previously thought, to the genus Baryonix, but to another type of spinosaurid very close to it, an indeterminate baryonychid.

The palaeontological studies carried out to date at Igea are significant because of the presence of numerous spinosaur skeletal remains, including partial skeletons belonging to several individuals. “The current research will allow our knowledge about the diversity of this unique group of carnivorous dinosaurs to be improved. It is likely that at least two different species are represented at the Igea sites,” said Erik Isasmendi and Xabier Pereda-Suberbiola, palaeontologists in the UPV/EHU’s Department of Geology; consequently, this Riojan locality is one of the world’s leading locations in the study of spinosaurs.

Reference:
Erik Isasmendi, Pablo Navarro-Lorbés, Patxi Sáez-Benito, Luis I. Viera, Angelica Torices, Xabier Pereda-Suberbiola. New contributions to the skull anatomy of spinosaurid theropods: Baryonychinae maxilla from the Early Cretaceous of Igea (La Rioja, Spain). Historical Biology, 2022; 1 DOI: 10.1080/08912963.2022.2069019

Note: The above post is reprinted from materials provided by University of the Basque Country.

Volcanic super eruptions are millions of years in the making — followed by swift surge

Molten lava from a Hawaiian volcano. Image: Willyam/Adobe
Molten lava from a Hawaiian volcano. Image: Willyam/Adobe

Researchers at the University of Bristol and Scottish Universities Environmental Research Centre have discovered that super-eruptions occur when huge accumulations of magma deep in the Earth’s crust, formed over millions of years, move rapidly to the surface disrupting pre-existing rock.

Using a model for crustal flow, an international team of scientists were able to show that pre-existing plutons — a body of intrusive rock made from solidified magna or lava — were formed over a few million years prior to four known gigantic super eruptions and that the disruption of these plutons by newly emplaced magmas took place extraordinarily rapidly. While the magma supplying super eruptions takes place over a prolonged period of time, the magma disrupts the crust and then erupts in just a few decades.

The findings, published today in Nature, explain these extreme differences in time ranges for magma generation and eruption by flow of hot but solid crust in response to ascent of the magma, accounting for the infrequency of these eruptions and their huge volumes.

Professor Steve Sparks of Bristol’s School of Earth Sciences explained: “The longevity of plutonic and related volcanic systems contrasts with short timescales to assemble shallow magma chambers prior to large-magnitude eruptions of molten rock. Crystals formed from earlier magma pulses, entrained within erupting magmas are stored at temperatures near or below the solidus for long periods prior to eruption and commonly have very short residence in host magmas for just decades or less.”

This study casts doubt on the interpretation of prolonged storage of old crystals at temperatures high enough for some molten rocks to be present and indicates the crystals derived from previously emplaced and completely solidified plutons (granites).

Scientists have known that volcanic super-eruptions eject crystals derived from older rocks. However, before this, they were widely thought to have originated in hot environments above the melting points of rock. Previous studies that show the magma chambers for super-eruptions form very rapidly but there was no convincing explanation for this rapid process. While modelling suggested that super-volcanic eruptions would need to be preceded by very long periods of granite pluton emplacement in the upper crust, evidence for this inference was largely lacking.

Prof Sparks added: “By studying of the age and character of the tiny crystals erupted with molten rock, we can help understand how such eruptions happen.

“The research provides an advance in understanding the geological circumstances that enable super eruptions to take place. This will help identify volcanoes that have potential for future super-eruptions.”

Such eruptions are very rare and Bristol scientists estimate only one of these types of eruptions occur on earth every 20,000 years. However such eruptions are highly destructive locally and can create global scale severe climate change that would have catastrophic consequences.

This project was supported by the Mining company BHP and by NERC.

Reference:
van Zalinge, M.E., Mark, D.F., Sparks, R.S.J. et al. Timescales for pluton growth, magma-chamber formation and super-eruptions. Nature, 2022 DOI: 10.1038/s41586-022-04921-9

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

Ancient source of oxygen for life hidden deep in the Earth’s crust

Earth
Earth

Scientists at Newcastle University have uncovered a source of oxygen that may have influenced the evolution of life before the advent of photosynthesis.

The pioneering research project, led by Newcastle University’s School of Natural and Environmental Sciences and published today in Nature Communications, uncovered a mechanism that can generate hydrogen peroxide from rocks during the movement of geological faults.

While in high concentrations hydrogen peroxide can be harmful to life, it can also provide a useful source of oxygen to microbes. This additional source of oxygen may have influenced the early evolution, and feasibly even origin, of life in hot environments on the early Earth prior to the evolution of photosynthesis.

In tectonically active regions, the movement of the Earth’s crust not only generates earthquakes but riddles the subsurface with cracks and fractures lined with highly reactive rock surfaces containing many imperfections, or defects. Water can then filter down and react with these defects on the newly fractured rock.

In the laboratory, Masters student Jordan Stone simulated tScientists have shown the importance of hot temperatures in maximizing hydrogen peroxide generation from rocks during the movement of geological faultshese conditions by crushing granite, basalt and peridotite — rock types that would have been present in the early Earth’s crust. These were then added to water under well controlled oxygen-free conditions at varying temperatures.

The experiments demonstrated that substantial amounts of hydrogen peroxide — and as a result, potentially oxygen — was only generated at temperatures close to the boiling point of water. Importantly, the temperature of hydrogen peroxide formation overlaps the growth ranges of some of the most heat-loving microbes on Earth called hyperthermophiles, including evolutionary ancient oxygen-using microbes near the root of the Universal Tree of Life.

Lead author Jordan Stone, who conducted this research as part of his MRes in Environmental Geoscience, said: “While previous research has suggested that small amounts of hydrogen peroxide and other oxidants can be formed by stressing or crushing of rocks in the absence of oxygen, this is the first study to show the vital importance of hot temperatures in maximising hydrogen peroxide generation.”

Principal Investigator Dr Jon Telling, Senior Lecturer, added: “This research shows that defects on crushed rock and minerals can behave very differently to how you would expect more ‘perfect’ mineral surfaces to react. All these mechanochemical reactions need to generate hydrogen peroxide, and therefore oxygen, is water, crushed rocks, and high temperatures, which were all present on the early Earth before the evolution of photosynthesis and which could have influenced the chemistry and microbiology in hot, seismically active regions where life may have first evolved.”

The work was supported through grants from the Natural Environmental Research Council (NERC) and the UK Space Agency. A major new follow-up project led by Dr Jon Telling, funded by NERC, is underway to determine the significance of this mechanism for supporting life in the Earth’s subsurface.

Reference:
Jordan Stone, John O. Edgar, Jamie A. Gould, Jon Telling. Tectonically-driven oxidant production in the hot biosphere. Nature Communications, 2022; 13 (1) DOI: 10.1038/s41467-022-32129-y

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

One more clue to the Moon’s origin

Thin section of NASA sample, LAP 02436, Lunar Mare Basalt containing indigenous noble gases. Image type: optical microscopy, cross-​polarized light. (Image: ETH Zurich / Patrizia Will)
Thin section of NASA sample, LAP 02436, Lunar Mare Basalt containing indigenous noble gases. Image type: optical microscopy, cross-​polarized light. (Image: ETH Zurich / Patrizia Will)

Humankind has maintained an enduring fascination with the Moon. It was not until Galileo’s time, however, that scientists really began study it. Over the course of nearly five centuries, researchers put forward numerous, much debated theories as to how the Moon was formed. Now, geochemists, cosmochemists, and petrologists at ETH Zurich shed new light on the Moon’s origin story. In a study just published in the journal, Science Advances, the research team reports findings that show that the Moon inherited the indigenous noble gases of helium and neon from Earth’s mantle. The discovery adds to the already strong constraints on the currently favoured “Giant Impact” theory that hypothesizes the Moon was formed by a massive collision between Earth and another celestial body.

Meteorites from the Moon to Antarctica

During her doctoral research at ETH Zurich, Patrizia Will analysed six samples of lunar meteorites from an Antarctic collection, obtained from NASA. The meteorites consist of basalt rock that formed when magma welled up from the interior of the Moon and cooled quickly. They remained covered by additional basalt layers after their formation, which protected the rock from cosmic rays and, particularly, the solar wind. The cooling process resulted in the formation of lunar glass particles amongst the other minerals found in magma. Will and the team discovered that the glass particles retain the chemical fingerprints (isotopic signatures) of the solar gases: helium and neon from the Moon’s interior. Their findings strongly support that the Moon inherited noble gases indigenous to the Earth. “Finding solar gases, for the first time, in basaltic materials from the Moon that are unrelated to any exposure on the lunar surface was such an exciting result,” says Will.

Without the protection of an atmosphere, asteroids continually pelt the Moon’s surface. It likely took a high-energy impact to eject the meteorites from the middle layers of the lava flow similar to the vast plains known as the Lunar Mare. Eventually the rock fragments made their way to Earth in the form of meteorites. Many of these meteorite samples are picked up in the deserts of North Africa or in, in this case, the “cold desert” of Antarctica where they are easier to spot in the landscape.

Grateful Dead lyrics inspire lab instrument

In the Noble Gas Laboratory at ETH Zurich resides a state-of-the-art noble gas mass spectrometer named, “Tom Dooley” — sung about in the Grateful Dead tune by the same name. The instrument got its name, when earlier researchers, at one point, suspended the highly sensitive equipment from the ceiling of the lab to avoid interference from the vibrations of everyday life. Using the Tom Dooley instrument, the research team was able to measure sub-millimetre glass particles from the meteorites and rule out solar wind as the source of the detected gases. The helium and neon that they detected were in a much higher abundance than expected.

The Tom Dooley is so sensitive that it is, in fact, the only instrument in the world capable of detecting such minimal concentrations of helium and neon. It was used to detect these noble gases in the 7 billion years old grains in the Murchison meteorite — the oldest known solid matter to-date.

Searching for the origins of life

Knowing where to look inside NASA’s vast collection of some 70,000 approved meteorites represents a major step forward. “I am strongly convinced that there will be a race to study heavy noble gases and isotopes in meteoritic materials,” says ETH Zurich Professor Henner Busemann, one of the world’s leading scientists in the field of extra-terrestrial noble gas geochemistry. He anticipates that soon researchers will be looking for noble gases such as xenon and krypton which are more challenging to identify. They will also be searching for other volatile elements such as hydrogen or halogens in the lunar meteorites.

Busemann comments, “While such gases are not necessary for life, it would be interesting to know how some of these noble gases survived the brutal and violent formation of the moon. Such knowledge might help scientists in geochemistry and geophysics to create new models that show more generally how such most volatile elements can survive planet formation, in our solar system and beyond.”

Reference:
Patrizia Will, Henner Busemann, My E. I. Riebe, Colin Maden. Indigenous noble gases in the Moon’s interior. Science Advances, 2022; 8 (32) DOI: 10.1126/sciadv.abl4920

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

Plesiosaur fossils found in the Sahara suggest they weren’t just marine animals

Plesiosaurus and spinosaurus may have both inhabited freshwater rivers
Plesiosaurus and spinosaurus may have both inhabited freshwater rivers

Fossils of small plesiosaurs, long-necked marine reptiles from the age of dinosaurs, have been found in a 100-million year old river system that is now Morocco’s Sahara Desert. This discovery suggests some species of plesiosaur, traditionally thought to be sea creatures, may have lived in freshwater.

Plesiosaurs, first found in 1823 by fossil hunter Mary Anning, were prehistoric reptiles with small heads, long necks, and four long flippers. They inspired reconstructions of the Loch Ness Monster, but unlike the monster of Lake Loch Ness, plesiosaurs were marine animals — or were widely thought to be.

Now, scientists from the University of Bath and University of Portsmouth in the UK, and Université Hassan II in Morocco, have reported small plesiosaurs from a Cretaceous-aged river in Africa.

The fossils include bones and teeth from three-metre long adults and an arm bone from a 1.5 metre long baby. They hint that these creatures routinely lived and fed in freshwater, alongside frogs, crocodiles, turtles, fish, and the huge aquatic dinosaur Spinosaurus.

These fossils suggest the plesiosaurs were adapted to tolerate freshwater, possibly even spending their lives there, like today’s river dolphins.

The new paper was headed by University of Bath Student Georgina Bunker, along with Nick Longrich from the University of Bath’s Milner Centre for Evolution, David Martill and Roy Smith from the University of Portsmouth, and Samir Zouhri from the Universite Hassan II.

The fossils include vertebrae from the neck, back, and tail, shed teeth, and an arm bone from a young juvenile.

“It’s scrappy stuff, but isolated bones actually tell us a lot about ancient ecosystems and animals in them. They’re so much more common than skeletons, they give you more information to work with” said Dr. Nick Longrich, corresponding author on the paper.

“The bones and teeth were found scattered and in different localities, not as a skeleton. So each bone and each tooth is a different animal. We have over a dozen animals in this collection.”

Whilst bones provide information on where animals died, the teeth are interesting because they were lost while the animal was alive — so they show where the animals lived.

What’s more, the teeth show heavy wear, like those fish-eating dinosaur Spinosaurus found in the same beds.

The scientists say that implies the plesiosaurs were eating the same food- chipping their teeth on the armored fish that lived in the river. This hints they spent a lot of time in the river, rather than being occasional visitors.

While marine animals like whales and dolphins wander up rivers, either to feed or because they’re lost, the number of plesiosaur fossils in the river suggest that’s unlikely.

A more likely possibility is that the plesiosaurs were able to tolerate fresh and salt water, like some whales, such as the beluga whale.

It’s even possible that the plesiosaurs were permanent residents of the river, like modern river dolphins. The plesiosaurs’ small size would have let them hunt in shallow rivers, and the fossils show an incredibly rich fish fauna.

Dr Longrich said: “We don’t really know why the plesiosaurs are in freshwater.

“It’s a bit controversial, but who’s to say that because we paleontologists have always called them ‘marine reptiles’, they had to live in the sea? Lots of marine lineages invaded freshwater.”

Freshwater dolphins evolved at least four times — in the Ganges River, the Yangtze River, and twice in the Amazon. A species of freshwater seal inhabits Lake Baikal, in Siberia, so it’s possible plesiosaurs adapted to freshwater as well.

The plesiosaurs belong to the family Leptocleididae- a family of small plesiosaurs often found in brackish or freshwater elsewhere in England, Africa, and Australia. And other plesiosaurs, including the long-necked elasmosaurs, turn up in brackish or fresh waters in North America and China.

Plesiosaurs were a diverse and adaptable group, and were around for more than 100 million years. Based on what they’ve found in Africa — and what other scientists have found elsewhere — the authors suggest they might have repeatedly invaded freshwater to different degrees.

“We don’t really know, honestly. That’s how paleontology works. People ask, how can paleontologists know anything for certain about the lives of animals that went extinct millions of years ago? The reality is, we can’t always. All we can do is make educated guesses based on the information we have. We’ll find more fossils. Maybe they’ll confirm those guesses. Maybe not.”

“It’s been really interesting to see the direction this project has gone in,” said lead author Georgina Bunker. The study initially began as an undergraduate project involving a single bone, but over time, more plesiosaur fossils started turning up, slowly providing a clearer picture of the animal.

The new discovery also expands the diversity of Morocco’s Cretaceous. Said Dr. Samir Zouhri, “This is another sensational discovery that adds to the many discoveries we have made in the Kem Kem over the past fifteen years of work in this region of Morocco. Kem Kem was truly an incredible biodiversity hotspot in the Cretaceous.”

“What amazes me” said coauthor Dave Martill, “is that the ancient Moroccan river contained so many carnivores all living alongside each other. This was no place to go for a swim.”

But what does this all mean for the plausibility of something like a Loch Ness Monster? On one level, it’s plausible. Plesiosaurs weren’t confined to the seas, they did inhabit freshwater. But the fossil record also suggests that after almost a hundred and fifty million years, the last plesiosaurs finally died out at the same time as the dinosaurs, 66 million years ago.

Reference:
Georgina Bunker, David M. Martill, Roy Smith, Samir Zourhi, Nick Longrich. Plesiosaurs from the fluvial Kem Kem Group (mid-Cretaceous) of eastern Morocco and a review of non-marine plesiosaurs. Cretaceous Research, 2022; 105310 DOI: 10.1016/j.cretres.2022.105310

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

Iceland volcano eruption opens a rare window into the Earth beneath our feet

he Fagradalsfjall eruption site viewed from above. The photo shows lava emanating from multiple vents. Tourists for scale.  Photograph: Alina V. Shevchenko and Edgar U. Zorn, GFZ Germany
he Fagradalsfjall eruption site viewed from above. The photo shows lava emanating from multiple vents. Tourists for scale.
Photograph: Alina V. Shevchenko and Edgar U. Zorn, GFZ Germany

The recent Fagradalsfjall eruption in the southwest of Iceland has enthralled the whole world, including nature lovers and scientists alike. The eruption was especially important as it provided geologists with a unique opportunity to study magmas that were accumulated in a deep crustal magma reservoir but ultimately derived from the Earth’s mantle (below 20 km).

A research team from University of Oregon, Uppsala University, University of Iceland, and Deutsches GeoForschungsZentrum (GFZ) took this exceptional opportunity to collect lava samples every few days in order to construct a time-integrated catalogue of samples and to monitor the geochemical evolution throughout the eruption to a degree of detail rarely achieved before. Usually, when volcano scientists look at past eruptions they work with a limited view of the erupted materials — for example older lava flows can get wholly or partially buried by newer ones. However, at Fagradalsfjall, the eruption was so well monitored and sampled that scientists had a chance to capture the evolution of an Icelandic eruption in near real-time.

The team were interested in oxygen isotopes. Why? Because oxygen makes up about 50% of all volcanic rocks and its isotope ratios are very sensitive tracers of mantle and crustal materials. In this way, oxygen isotopes can help scientists to determine if magma is mantle-derived or if it interacted with crustal materials as it made its way to the surface. However, in addition to oxygen, the other vast suite of elements making up the volcanic rocks threw up some surprises. For instance, the team observed that this single eruption contains roughly half of the entire diversity of mantle-derived magmas previously recorded for the whole of Iceland.

In brief, geochemical results show that the latest Iceland eruption was supplied by magmas derived from multiple sources in the Earth’s mantle, each with its own distinctive elemental characteristics. To the amazement of scientists, each of these domains had identical oxygen isotope ratios. This result was remarkable and has never been observed before at an active eruption. The study provides new and compelling evidence for distinct mantle-sourced magmas having uniform oxygen isotope ratios, which can help us to better understand mantle dynamics and refine mantle models for Iceland.

Reference:
I. N. Bindeman, F. M. Deegan, V. R. Troll, T. Thordarson, Á. Höskuldsson, W. M. Moreland, E. U. Zorn, A. V. Shevchenko, T. R. Walter. Diverse mantle components with invariant oxygen isotopes in the 2021 Fagradalsfjall eruption, Iceland. Nature Communications, 2022; 13 (1) DOI: 10.1038/s41467-022-31348-7

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

Rare deep-sea brine pools discovered in Red Sea

Brine pools are one of the most extreme environments on Earth, yet despite their high salinity, exotic chemistry, and complete lack of oxygen, these pools are teeming with life.
Brine pools are one of the most extreme environments on Earth, yet despite their high salinity, exotic chemistry, and complete lack of oxygen, these pools are teeming with life.

Researchers at the University of Miami (UM) Rosenstiel School of Marine and Atmospheric Science recently discovered rare deep-sea brine pools in the Gulf of Aqaba, a northern extension to the Red Sea. These salty underwater lakes hold secrets into the way oceans on Earth formed millions of years ago, and offer clues to life on other planets.

In partnership with OceanX, Sam Purkis, professor and chair of the UM Department of Marine Geosciences and team made their discovery more than one mile beneath the sea surface (1,770 meters) using a remotely operated underwater vehicle (ROV) on the OceanXplorer, a highly equipped research vessel capable of exploring the most unreachable places on Earth.

“Until we understand the limits of life on Earth, it will be difficult to determine if alien planets can host any living beings,” said Purkis. “Our discovery of a rich community of microbes that survive in extreme environments can help trace the limits of life on Earth and can be applied to the search for life elsewhere in our solar system and beyond.”

Brine pools are one of the most extreme environments on Earth, yet despite their high salinity, exotic chemistry, and complete lack of oxygen, these pools are teeming with life. Bioactive molecules with potential anticancer properties have previously been isolated from brine pool microbes in the Red Sea.

The research, published in Nature Communications, is the first discovery of brine pools in the Gulf of Aqaba.

“We were very lucky,” said Purkis. “The discovery came in the last five minutes of the ten-hour ROV dive that we could dedicate to this project.”

Located close to the coastline, these extremely salty, zero oxygen pools preserve information on tsunami, flashfloods, and earthquakes in the Gulf of Aqaba that took place thousands of years ago. There are many faults and fractures in the seabed associated with the tectonics of the region in this area of the Gulf of Aqaba.

Earlier this year, Purkis and team discovered evidence of a 500-year-old submarine landslide that likely spawned a sizable tsunami in the region, that could have implications for coastline development in Egypt and Saudi Arabia.

Reference:
Sam J. Purkis, Hannah Shernisky, Peter K. Swart, Arash Sharifi, Amanda Oehlert, Fabio Marchese, Francesca Benzoni, Giovanni Chimienti, Gaëlle Duchâtellier, James Klaus, Gregor P. Eberli, Larry Peterson, Andrew Craig, Mattie Rodrigue, Jürgen Titschack, Graham Kolodziej, Ameer Abdulla. Discovery of the deep-sea NEOM Brine Pools in the Gulf of Aqaba, Red Sea. Communications Earth & Environment, 2022; 3 (1) DOI: 10.1038/s43247-022-00482-x

Note: The above post is reprinted from materials provided by University of Miami Rosenstiel School of Marine & Atmospheric Science. Original written by Diana Udel.

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