back to top
27.8 C
New York
Friday, November 15, 2024
Home Blog Page 96

A hidden diversity of half-billion-year-old microscopic animal fossils

Credit: Uppsala universitet

A team of researchers from Uppsala University have uncovered a hidden diversity of microscopic animal fossils from over half a billion years ago lurking in rocks from the northern tip of Greenland.

The Cambrian explosion of animal diversity beginning ~541 million years ago is a defining episode in the history of life. This was a time when the seas first teemed with animal life, and the first recognisably modern ecosystems began to take shape.

Current accounts of this explosion in animal diversity rely heavily on records from fossilised shells and other hard parts, since these structures are the most likely to survive as fossils.

However, since most marine animals are soft-bodied this represents only a small fraction of the total diversity.

Rare sites of exceptional fossilisation, like the world-famous Burgess Shale, have revolutionised palaeontologists understanding of soft-bodied Cambrian life. Because of the special conditions of fossilisation at these localities, organisms that did not produce hard mineralized shells or skeletons are also preserved. Such sites offer a rare glimpse into the true diversity of these ancient seas, which were filled with a dazzling array of soft and squishy predatory worms and arthropods (the group containing modern crustaceans and insects).

One of the oldest of these truly exceptional fossil bonanzas is the Sirius Passet site in the far north of Greenland. Unfortunately, during their long history, the rocks at Sirius Passet have been heated up and baked to high temperatures as the northern margin of Greenland smashed into various tectonic plates and buried these rocks deep beneath the surface.

All this heating has boiled away the delicate organic remains that once formed the fossils of soft bodied animals at Sirius Passet, leaving only faint impressions of their remains.

Not far to the south of Sirius Passet, the rocks have escaped the worst effects of this heating. A team of palaeontologists from Uppsala (Ben Slater, Sebastian Willman, Graham Budd and John Peel) used a low-manipulation acid extraction procedure to dissolve some of these less intensively cooked mudrocks. To their astonishment, this simple preparation technique revealed a wealth of previously unknown microscopic animal fossils preserved in spectacular detail.

Most of the fossils were less than a millimetre long and had to be studied under the microscope. Fossils at the nearby Sirius Passet site typically preserve much larger animals, so the new finds fill an important gap in our knowledge of the small-scale animals that probably made up the majority of these ecosystems. Among the discoveries were the tiny spines and teeth of priapulid worms – small hook shaped structures that allowed these worms to efficiently burrow through the sediments and capture prey. Other finds included the tough outer cuticles and defensive spines of various arthropods, and perhaps most surprisingly, microscopic fragments of the oldest known pterobranch hemichordates – an obscure group of tube-dwelling filter feeders that are distant relatives of the vertebrates. This group became very diverse after the Cambrian Period and are among some of the most commonly found fossils in rocks from younger deposits, but were entirely unknown from the early Cambrian. This new source of fossils will also help palaeontologists to better understand the famously difficult to interpret fossils at the nearby Sirius Passet site, where the flattened animal fossils are usually complete, but missing crucial microscopic details.

“The sheer abundance of these miniature animal fossils means that we have only begun to scratch the surface of this overlooked resource, but it is already clear that this discovery will help to reshape our view of the non-shelly animals that crawled and swam among the early Cambrian seas more than half a billion years ago,” says Sebastian Willman, researcher at the Department of Earth Sciences, Uppsala University.

Reference:
Ben J. Slater et al. Widespread preservation of small carbonaceous fossils (SCFs) in the early Cambrian of North Greenland, Geology (2017). DOI: 10.1130/G39788.1

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

Oldest fossils ever found show life on Earth began before 3.5 billion years ago

An example of one of the microfossils discovered in a sample of rock recovered from the Apex Chert, a rock formation in western Australia that is among the oldest and best-preserved rock deposits in the world.
An example of one of the microfossils discovered in a sample of rock recovered from the Apex Chert, a rock formation in western Australia that is among the oldest and best-preserved rock deposits in the world. The fossils were first described in 1993 but a 2017 study published by UCLA and UW-Madison scientists used sophisticated chemical analysis to confirm the microscopic structures found in the rock are indeed biological, rendering them — at 3.5 billion years — the oldest fossils yet found. Credit: J. William Schopf, UCLA

Researchers at UCLA and the University of Wisconsin-Madison have confirmed that microscopic fossils discovered in a nearly 3.5 billion-year-old piece of rock in Western Australia are the oldest fossils ever found and indeed the earliest direct evidence of life on Earth.

The study, published today in the Proceedings of the National Academy of Sciences, was led by J. William Schopf, professor of paleobiology at UCLA, and John W. Valley, professor of geoscience at the University of Wisconsin-Madison. The research relied on new technology and scientific expertise developed by researchers in the UW-Madison WiscSIMS Laboratory.

The study describes 11 microbial specimens from five separate taxa, linking their morphologies to chemical signatures that are characteristic of life. Some represent now-extinct bacteria and microbes from a domain of life called Archaea, while others are similar to microbial species still found today. The findings also suggest how each may have survived on an oxygen-free planet.

The microfossils—so called because they are not evident to the naked eye—were first described in the journal Science in 1993 by Schopf and his team, which identified them based largely on the fossils’ unique, cylindrical and filamentous shapes. Schopf, director of UCLA’s Center for the Study of Evolution and the Origin of Life, published further supporting evidence of their biological identities in 2002.

He collected the rock in which the fossils were found in 1982 from the Apex chert deposit of Western Australia, one of the few places on the planet where geological evidence of early Earth has been preserved, largely because it has not been subjected to geological processes that would have altered it, like burial and extreme heating due to plate-tectonic activity.

But Schopf’s earlier interpretations have been disputed. Critics argued they are just odd minerals that only look like biological specimens. However, Valley says, the new findings put these doubts to rest; the microfossils are indeed biological.

“I think it’s settled,” he says.

Using a secondary ion mass spectrometer (SIMS) at UW-Madison called IMS 1280—one of just a handful of such instruments in the world—Valley and his team, including department geoscientists Kouki Kitajima and Michael Spicuzza, were able to separate the carbon composing each fossil into its constituent isotopes and measure their ratios.

Isotopes are different versions of the same chemical element that vary in their masses. Different organic substances—whether in rock, microbe or animal—contain characteristic ratios of their stable carbon isotopes.

Using SIMS, Valley’s team was able to tease apart the carbon-12 from the carbon-13 within each fossil and measure the ratio of the two compared to a known carbon isotope standard and a fossil-less section of the rock in which they were found.

“The differences in carbon isotope ratios correlate with their shapes,” Valley says. “If they’re not biological there is no reason for such a correlation. Their C-13-to-C-12 ratios are characteristic of biology and metabolic function.”

Based on this information, the researchers were also able to assign identities and likely physiological behaviors to the fossils locked inside the rock, Valley says. The results show that “these are a primitive, but diverse group of organisms,” says Schopf.

The team identified a complex group of microbes: phototrophic bacteria that would have relied on the sun to produce energy, Archaea that produced methane, and gammaproteobacteria that consumed methane, a gas believed to be an important constituent of Earth’s early atmosphere before oxygen was present.

It took Valley’s team nearly 10 years to develop the processes to accurately analyze the microfossils—fossils this old and rare have never been subjected to SIMS analysis before. The study builds on earlier achievements at WiscSIMS to modify the SIMS instrument, to develop protocols for sample preparation and analysis, and to calibrate necessary standards to match as closely as possible the hydrocarbon content to the samples of interest.

In preparation for SIMS analysis, the team needed to painstakingly grind the original sample down as slowly as possible to expose the delicate fossils themselves—all suspended at different levels within the rock and encased in a hard layer of quartz—without actually destroying them. Spicuzza describes making countless trips up and down the stairs in the department as geoscience technician Brian Hess ground and polished each microfossil in the sample, one micrometer at a time.

Each microfossil is about 10 micrometers wide; eight of them could fit along the width of a human hair.

Valley and Schopf are part of the Wisconsin Astrobiology Research Consortium, funded by the NASA Astrobiology Institute, which exists to study and understand the origins, the future and the nature of life on Earth and throughout the universe.

Studies such as this one, Schopf says, indicate life could be common throughout the universe. But importantly, here on Earth, because several different types of microbes were shown to be already present by 3.5 billion years ago, it tells us that “life had to have begun substantially earlier—nobody knows how much earlier—and confirms it is not difficult for primitive life to form and to evolve into more advanced microorganisms,” says Schopf.

Earlier studies by Valley and his team, dating to 2001, have shown that liquid water oceans existed on Earth as early as 4.3 billion years ago, more than 800 million years before the fossils of the present study would have been alive, and just 250 million years after the Earth formed.

“We have no direct evidence that life existed 4.3 billion years ago but there is no reason why it couldn’t have,” says Valley. “This is something we all would like to find out.”

UW-Madison has a legacy of pushing back the accepted dates of early life on Earth. In 1953, the late Stanley Tyler, a geologist at the university who passed away in 1963 at the age of 57, was the first person to discover microfossils in Precambrian rocks. This pushed the origins of life back more than a billion years, from 540 million to 1.8 billion years ago.

“People are really interested in when life on Earth first emerged,” Valley says. “This study was 10 times more time-consuming and more difficult than I first imagined, but it came to fruition because of many dedicated people who have been excited about this since day one … I think a lot more microfossil analyses will be made on samples of Earth and possibly from other planetary bodies.”

Reference:
J. William Schopf el al., “SIMS analyses of the oldest known assemblage of microfossils document their taxon-correlated carbon isotope compositions,” PNAS (2017). DOI: 10.1073/pnas.1718063115

Note: The above post is reprinted from materials provided by University of Wisconsin-Madison.

Ancient fossil microorganisms indicate that life in the universe is common

This is a 3.465 billion year-old fossil microorganism from Western Australia.
This is a 3.465 billion year-old fossil microorganism from Western Australia.
Credit: J. William Schopf/UCLA Center for the Study of Evolution and the Origin of Life

A new analysis of the oldest known fossil microorganisms provides strong evidence to support an increasingly widespread understanding that life in the universe is common.

The microorganisms, from Western Australia, are 3.465 billion years old. Scientists from UCLA and the University of Wisconsin-Madison report today in the journal Proceedings of the National Academy of Sciences that two of the species they studied appear to have performed a primitive form of photosynthesis, another apparently produced methane gas, and two others appear to have consumed methane and used it to build their cell walls.

The evidence that a diverse group of organisms had already evolved extremely early in the Earth’s history — combined with scientists’ knowledge of the vast number of stars in the universe and the growing understanding that planets orbit so many of them — strengthens the case for life existing elsewhere in the universe because it would be extremely unlikely that life formed quickly on Earth but did not arise anywhere else.

“By 3.465 billion years ago, life was already diverse on Earth; that’s clear — primitive photosynthesizers, methane producers, methane users,” said J. William Schopf, a professor of paleobiology in the UCLA College, and the study’s lead author. “These are the first data that show the very diverse organisms at that time in Earth’s history, and our previous research has shown that there were sulfur users 3.4 billion years ago as well.

“This tells us life had to have begun substantially earlier and it confirms that it was not difficult for primitive life to form and to evolve into more advanced microorganisms.”

Schopf said scientists still do not know how much earlier life might have begun.

“But, if the conditions are right, it looks like life in the universe should be widespread,” he said.

The study is the most detailed ever conducted on microorganisms preserved in such ancient fossils. Researchers led by Schopf first described the fossils in the journal Science in 1993, and then substantiated their biological origin in the journal Nature in 2002. But the new study is the first to establish what kind of biological microbial organisms they are, and how advanced or primitive they are.

For the new research, Schopf and his colleagues analyzed the microorganisms with cutting-edge technology called secondary ion mass spectroscopy, or SIMS, which reveals the ratio of carbon-12 to carbon-13 isotopes — information scientists can use to determine how the microorganisms lived. (Photosynthetic bacteria have different carbon signatures from methane producers and consumers, for example.) In 2000, Schopf became the first scientist to use SIMS to analyze microscopic fossils preserved in rocks; he said the technology will likely be used to study samples brought back from Mars for signs of life.

The Wisconsin researchers, led by geoscience professor John Valley, used a secondary ion mass spectrometer — one of just a few in the world — to separate the carbon from each fossil into its constituent isotopes and determine their ratios.

“The differences in carbon isotope ratios correlate with their shapes,” Valley said. “Their C-13-to-C-12 ratios are characteristic of biology and metabolic function.”

The fossils were formed at a time when there was very little oxygen in the atmosphere, Schopf said. He thinks that advanced photosynthesis had not yet evolved, and that oxygen first appeared on Earth approximately half a billion years later before its concentration in our atmosphere increased rapidly starting about 2 billion years ago.

Oxygen would have been poisonous to these microorganisms, and would have killed them, he said.

Primitive photosynthesizers are fairly rare on Earth today because they exist only in places where there is light but no oxygen — normally there is abundant oxygen anywhere there is light. And the existence of the rocks the scientists analyzed is also rather remarkable: The average lifetime of a rock exposed on the surface of the Earth is about 200 million years, Schopf said, adding that when he began his career, there was no fossil evidence of life dating back farther than 500 million years ago.

“The rocks we studied are about as far back as rocks go.”

While the study strongly suggests the presence of primitive life forms throughout the universe, Schopf said the presence of more advanced life is very possible but less certain.

One of the paper’s co-authors is Anatoliy Kudryavtsev, a senior scientist at UCLA’s Center for the Study of Evolution and the Origin of Life, of which Schopf is director. The research was funded by the NASA Astrobiology Institute.

In May 2017, a paper in PNAS by Schopf, UCLA graduate student Amanda Garcia and colleagues in Japan showed the Earth’s near-surface ocean temperature has dramatically decreased over the past 3.5 billion years. The work was based on their analysis of a type of ancient enzyme present in virtually all organisms.

In, 2015 Schopf was part of an international team of scientists that described in PNAS their discovery of the greatest absence of evolution ever reported — a type of deep-sea microorganism that appears not to have evolved over more than 2 billion years.

Reference:
J. William Schopf, Kouki Kitajima, Michael J. Spicuzza, Anatoliy B. Kudryavtsev, John W. Valley. SIMS analyses of the oldest known assemblage of microfossils document their taxon-correlated carbon isotope compositions. Proceedings of the National Academy of Sciences, 2017; 201718063 DOI: 10.1073/pnas.1718063115

Note: The above post is reprinted from materials provided by University of California – Los Angeles.

Computing the way to the center of the Earth

Using JSC's JUQUEEN supercomputer, University of Cologne researchers were able to simulate the structure of silicon dioxide at a variety of different pressures. The image shows how the the shape and structure of the atoms change as pressure increases.
Using JSC’s JUQUEEN supercomputer, University of Cologne researchers were able to simulate the structure of silicon dioxide at a variety of different pressures. The image shows how the the shape and structure of the atoms change as pressure increases.
Credit: Prescher, C., Prakapenka, V.B., Stefanski, J., Jahn, S., Skinner, L.B., Wang, Y.

In order to more fully comprehend the complexities of Earth’s interior, humanity has to dig deep — literally. To date, scientists have been able to bore a little over 12 kilometres deep, or about half the average depth of the Earth’s crust.

Why would researchers need to peer into deeper depths? Both to better understand how the earth formed and how the interior might have an effect on our life on the surface of the Earth today, such as by the magnitude and reversals of the Earth’s magnetic field.

However, experiments investigating materials at conditions deep in the Earth are challenging, meaning that to continue gaining insights into these phenomena, experimentalists must turn to modeling and simulation to support and complement their efforts.

To that end, researchers at the University of Cologne’s Institute for Geology and Mineralogy have turned to computing resources at the Jülich Supercomputing Centre (JSC) to help better comprehend how materials behave in the extreme conditions below the surface of the Earth.

The team, led by University of Cologne’s Prof. Dr. Sandro Jahn and Dr. Clemens Prescher, has been using JSC’s JUQUEEN supercomputer to simulate the structure of melts by studying silicate glasses as a model system for melts under ultra-high pressures. The team recently published its initial findings in the Proceedings of the National Academy of Sciences.

“Understanding properties of silicate melts and glasses at ultra-high pressure is crucial to understand how the Earth has formed in its infancy, where impacts of large asteroids led to a completely molten Earth,” said Prescher. “In fact, all of the internal layered structure we know today was formed in such events.”

It’s a glass

When most people think of the word glass, they think of windows or bottles. Glass, however, is a term describing a wide range of non-crystal solids. Atoms in a solid can organize themselves in a variety of ways, and materials considered glasses have some of the more “chaotic” atomic structures possible in solids.

A glass can also be seen as a frozen melt. Thus by understanding the properties of glasses at ultra-high pressures, researchers can gain insights into the melts’ properties in the deep Earth’s interior, providing a clearer view into the physical processes which made the Earth and might be still occurring today.

Using a variety of geophysics measurements and laboratory experiments, researchers are capable of gaining some degree of insight into material properties under certain pressure conditions without actually being able to make direct observations.

Enter supercomputing. As computing power has gotten stronger, geophysics researchers are able to complement and expand their studies of these inner-Earth processes through the use of numerical models.

In the case of the University of Cologne researchers, they wanted to get a more detailed insight into the structure of the silicate glass than their experimental efforts were able to provide. The team utilized ab initio calculations of atoms’ electronic structures and put these calculations in motion using molecular dynamics simulations. Ab initio calculations mean that researchers start with no assumptions in their mathematical models, making a simulation more computationally expensive but also more accurate.

Due to having many calculations for each atom’s structure and computationally demanding molecular dynamics calculations, the team keeps its simulations relatively small in scale — the team’s largest runs typically have between 200-250 atoms in the simulation. This size allows the team to run simulations under a variety of different pressure and temperature combinations, ultimately allowing it to calculate a small but representative sample of material interactions under a variety of conditions.

To test its model and lay the foundation for modeling increasingly complex material interactions, the team decided to simulate silicon dioxide (SiO2), a common, well-studied material, most well-known as the compound that forms quartz.

Among silicate materials, SiO2 is a good candidate on which to base computational models — researchers already understand how its atomic structure patterns and material properties change under a variety of pressure conditions.

The team chose to focus on a relatively simple, well-known material in order to expand the range of pressure it could simulate and attempt to validate the model with experimental data. Using JUQUEEN, the team was able to extend its investigation well beyond the experimentally achieved 172 Gigapascals, corresponding to 1.72 million times the Earth’s atmospheric pressure, or roughly the amount of pressure the Eiffel Tower would apply by pressing down on the tip of a person’s finger.

The researchers also found that at high pressures, oxygen atoms are much more compressible than silicon atoms. The varying size ratio between the two leads to hugely different glass structures of SiO2 at low and at high pressures.

Digging Deeper

By validating its model, the team feels confident that it can move on to more complex materials and interactions. Specifically, the team hopes to expand its investigations deeper into the realm of melts. Think of lava as a melt — molten rock erupts from below the earth’s surface, rapidly cools when it reaches the surface, and may form obsidian, a glassy rock.

In order to do more advanced simulations of melts, the team would like to be able to expand its simulations to account for a wider range of chemical processes as well as expand the number of atoms in a typical run.

As JSC and the other two Gauss Centre for Supercomputing (GCS) facilities — the High-Performance Computing Center Stuttgart and the Leibniz Supercomputing Centre in Garching — install next-generation supercomputers, the team is confident that they will be able to gain even greater insight into the wide range of complex material interactions happening many kilometres below the surface.

“A faster machine will enable us to simulate more complex melts and glasses, which is crucial to go from model systems, such as SiO2 glass in this study, to the real-world compositions we expect in the Earth’s interior,” Prescher said.

Prescher also noted that JSC support staff helped the team work more efficiently by assisting with implementing the team’s code.

This type of support represents GCS’ plans for the future. With the promise and opportunity connected to next-generation computing architectures, GCS centre leadership realizes that closer collaboration with users and application co-design will be a key component for ensuring researchers can efficiently solve bigger, more complex scientific problems.

Whether studying deep in space among the stars or deep below the surface of the Earth, the collaboration between supercomputing centres and researchers will play an increasingly important role in solving the world’s toughest scientific challenges.

This research used Gauss Centre for Supercomputing resources based at the Jülich Supercomputing Centre.

Reference:
Clemens Prescher, Vitali B. Prakapenka, Johannes Stefanski, Sandro Jahn, Lawrie B. Skinner, Yanbin Wang. Beyond sixfold coordinated Si in SiO2glass at ultrahigh pressures. Proceedings of the National Academy of Sciences, 2017; 114 (38): 10041 DOI: 10.1073/pnas.1708882114

Note: The above post is reprinted from materials provided by Gauss Centre for Supercomputing.

Primitive fossil bear with a sweet tooth identified from Canada’s High Arctic

Digital reconstruction of the Canadian Arctic fossil bear
Digital reconstruction of the Canadian Arctic fossil bear, Protarctos abstrusus.
Credit: Xiaoming Wang

Researchers from the Canadian Museum of Nature and the Natural History Museum of Los Angeles County have identified remains of a 3.5-million-year-old bear from a fossil-rich site in Canada’s High Arctic. Their study shows not only that the animal is a close relative of the ancestor of modern bears — tracing its ancestry to extinct bears of similar age from East Asia — but that it also had a sweet tooth, as determined by cavities in the teeth.

The scientists identify the bear as Protarctos abstrusus, which was previously only known from a tooth found in Idaho. Showing its transitional nature, the animal was slightly smaller than a modern black bear, with a flatter head and a combination of primitive and advanced dental characters. The results are published today in the journal Scientific Reports.

“This is evidence of the most northerly record for primitive bears, and provides an idea of what the ancestor of modern bears may have looked like,” says Dr. Xiaoming Wang, lead author of the study and Head of Vertebrate Paleontology at the Natural History Museum of Los Angeles County (NHMLA). “Just as interesting is the presence of dental caries, showing that oral infections have a long evolutionary history in the animals, which can tell us about their sugary diet, presumably from berries. This is the first and earliest documented occurrence of high-calorie diet in basal bears, likely related to fat storage in preparation for the harsh Arctic winters.”

The research team, which included co-author Dr. Natalia Rybczynski, a Research Associate and paleontologist with the Canadian Museum of Nature, were able to study recovered bones from the skull, jaws and teeth, as well as parts of the skeleton from two individuals.

The bones were discovered over a 20-year period by Canadian Museum of Nature scientists, including Dr. Rybczynski, at a fossil locality on Ellesmere Island known as the Beaver Pond site. The peat deposits include fossilized plants indicative of a boreal-type wetland forest, and have yielded other fossils, including fish, beaver, small carnivores, deerlets, and a three-toed horse.

The findings show that the Ellesmere Protarctos lived in a northern boreal-type forest habitat, where there would have been 24-hour darkness in winter, as well as about six months of ice and snow.

“It is a significant find, in part because all other ancient fossil ursine bears, and even some modern bear species like the sloth bear and sun bear, are associated with lower-latitude, milder habitats,” says co-author Dr. Rybczynski. “So, the Ellesmere bear is important because it suggests that the capacity to exploit the harshest, most northern forests on the planet is not an innovation of modern grizzlies and black bears, but may have characterized the ursine lineage from its beginning.”

Dr. Wang analyzed characteristics of fossil bear remains from around the world to identify the Ellesmere remains as Protarctos and to establish its evolutionary lineage in relation to other bears. Modern bears are wide-ranging, found from equatorial to polar regions. Their ancestors, mainly found in Eurasia, date to about 5 million years ago.

Fossil records of ursine bears (all living bears plus their ancestors, except the giant panda, which is an early offshoot) are poor and their early evolution controversial. The new fossil represents one of the early immigrations from Asia to North America but it is probably not a direct ancestor to the modern American black bear.

Of further significance is that the teeth of both Protarctos individuals show signs of well-developed dental cavities, which were identified following CT scans by Stuart White, a retired professor with the UCLA School of Dentistry. The cavities underline that these ancient bears consumed large amounts of sugary foods such as berries. Indeed, berry plants are found preserved in the same Ellesmere deposits as the bear remains.

“We know that modern bears consume sugary fruits in the fall to promote fat accumulation that allows for winter survival via hibernation. The dental cavities in Protarctos suggest that consumption of sugar-rich foods like berries, in preparation for winter hibernation, developed early in the evolution of bears as a survival strategy,” explains Rybczynski.

Reference:
Xiaoming Wang, Natalia Rybczynski, C. Richard Harington, Stuart C. White, Richard H. Tedford. A basal ursine bear (Protarctos abstrusus) from the Pliocene High Arctic reveals Eurasian affinities and a diet rich in fermentable sugars. Scientific Reports, 2017; 7 (1) DOI: 10.1038/s41598-017-17657-8

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

60 Million Year Old Meteorite Strike in Scotland

Thin section view of meteoritic ejecta deposit si
Thin section view of meteoritic ejecta deposit site 1. Note fractured quartz and pervasive fabric. Field of view 4 mm XPolars. Credit: Simon Drake.

Geologists exploring volcanic rocks on Scotland’s Isle of Skye found something out-of-this-world instead: ejecta from a previously unknown, 60 million-year-old meteorite impact. The discovery, the first meteorite impact described within the British Paleogene Igneous Province (BPIP), opens questions about the impact and its possible connection to Paleogene volcanic activity across the North Atlantic.

Lead author Simon Drake, an associate lecturer in geology at Birkbeck University of London, zeroed in on a meter-thick layer at the base of a 60.0 million-year-old lava flow. “We thought it was an ignimbrite (a volcanic flow deposit),” says Drake. But when he and colleagues analyzed the rock using an electron microprobe, they discovered that it contained rare minerals straight from outer space: vanadium-rich and niobium-rich osbornite.

These mineral forms have never been reported on Earth. They have, however, been collected by NASA’s Stardust Comet Sample Return Mission as space dust in the wake of the Wild 2 comet. What’s more, the osbornite is unmelted, suggesting that it was an original piece of the meteorite. The team also identified reidite, an extremely high pressure form of zircon which is only ever associated in nature with impacts, along with native iron and other exotic mineralogy linked to impacts such as barringerite.

A second site, seven kilometers away, proved to be a two-meter-thick ejecta layer with the same strange mineralogy. The researchers pin the impact to sometime between 60 million and 61.4 million years ago (Ma), constrained by a 60 Ma radiometric age for the overlying lava flow, and 61.4 Ma for a basalt clast embedded within the ejecta layer. The team published their discovery in Geology this week.

The discovery opens many questions. Is the same ejecta layer found elsewhere in the BPIP? Where exactly did the meteorite hit? Could the impact have triggered the outpouring of lava that began at the same time, or be related to volcanism in the larger North Atlantic Igneous Province? So far, Drake has collected samples from another site on Skye that also yield strange mineralogy, including another mineral strikingly similar to one found in comet dust.

Drake says he was surprised that the ejecta layer had not been identified before. After all, the Isle of Skye is famously well-trampled by geologists. The second site had not been sampled in years. As for the first site, Drake suspects the steep, rough, and very boggy terrain probably discouraged previous workers from sampling the layer. “We were sinking in up to our thighs. I distinctly recall saying to (co-author) Andy Beard, ‘this had better be worth it.'” Now, says Drake, “It was worth it.”

Reference:
Simon M. Drake, Andrew D. Beard, Adrian P. Jones, David J. Brown, A. Dominic Fortes, Ian L. Millar, Andrew Carter, Jergus Baca, Hilary Downes. Discovery of a meteoritic ejecta layer containing unmelted impactor fragments at the base of Paleocene lavas, Isle of Skye, Scotland. Geology, 2017; DOI: 10.1130/G39452.1

Note: The above post is reprinted from materials provided by Geological Society of America.

Residual strain despite mega earthquake

The Nazca plate moves eastwards with a rate of 6.6 cm per year.
The Nazca plate moves eastwards with a rate of 6.6 cm per year. Off the Chilean coast it collides with the South American plate and is submerged beneath it. In this process, strains build up between the plates – until they break and the earth trembles. Credit: Image reproduced from the GEBCO world map 2014.

On 22 May 1960, an earthquake shook the southern Chilean continental margin on a length of about 1,000 kilometers. Estimates suggest that around 1,600 people died as a direct result of the quake and the following tsunami, leaving around two million people homeless. With a strength of 9.5 on the moment magnitude scale, the Valdivia earthquake from 1960 still ranks number one on the list of strongest earthquakes ever measured.

More than half a century later, on 25 December 2016, the earth was trembling around the southern Chilean island of Chiloé. With a strength of 7,5 Mw this event can be described as rather moderate by Chilean standards. But the fact that it broke the same section of the Chilean subduction zone as the 1960 earthquake is quite interesting for scientists. As researchers from the GEOMAR Helmholtz Centre for Ocean Research Kiel and the Universidad de Chile have now published in the journal Geophysical Journal International, part of the energy of the 2016 quake apparently dates back to before 1960. “So, the 1960 quake, despite its immense strength, must have left some strain in the underground, ” says Dr. Dietrich Lange, geophysicist at GEOMAR and lead author of the study.

To understand why Chile is being hit so frequently by heavy earthquakes, one has to look at the seabed off the coast. It belongs to the so-called Nazca plate, a tectonic plate, which moves eastwards with a rate of 6.6 cm per year. Off the Chilean coast it collides with the South American plate and is submerged beneath it. In this process, strains build up between the plates — until they break and the earth trembles.

During such an earthquake, the strain is released within minutes. During the 1960 earthquake for example, the plates shifted by more than 30 meters against each other. As a result, landmasses were lifted up or down several meters with a fundamental change of Chilean landscapes and coastline. “The scale of the slip also gives information about the accumulated energy between the two plates,” explains Dr. Lange.

From the time interval (56 years), the known speed of the Nazca plate, and further knowledge of the subduction zone, the German-Chilean team has calculated the accumulated energy and thus the theoretical slip of the 2016 earthquake to about 3.4 meters. But the analysis of seismic data and GPS surveys showed a slip of more than 4.5 m. “The strain must have had accumulated for more than 56 years. It is older than the last earthquake in the same region,” says Dr. Lange.

Similar results have recently been obtained in another subduction zones. Along with them, the new study suggests that for risk assessment in earthquake-prone areas, not just a single seismic cycle from one earthquake to the next should be considered. “The energy can be greater than that resulting from the usual calculations, which can, for example, have an impact on recommendations for earthquake-proof construction,” says Dr. Lange.

Reference:
Dietrich Lange, Javier Ruiz, Sebastián Carrasco, Paula Manríquez. The Chiloé Mw 7.6 earthquake of 25 December 2016 in Southern Chile and its relation to the Mw 9.5 1960 Valdivia earthquake. Geophysical Journal International, 2017; DOI: 10.1093/gji/ggx514

Note: The above post is reprinted from materials provided by Helmholtz Centre for Ocean Research Kiel (GEOMAR).

Geologists report new discoveries about Kansas, Oklahoma earthquakes

The number of earthquakes striking south-central Kansas has skyrocketed
The number of earthquakes striking south-central Kansas has skyrocketed. This map shows the 2,522 earthquakes that occurred from May 2015 to July 2017 in all of Sumner County, small segments of Sedgwick County to the north and a portion of Harper County to the west. During this period, Sumner County alone experienced about 2,400 earthquakes, ranging from 0.4 to 3.6 magnitude. A 3.0 magnitude earthquake is usually felt by humans. Red circles indicate earthquakes. Triangles indicate sensors the geologists used to study the earthquakes. Citation: K.A. Nolte, G.P. Tsoflias, T.S. Bidgoli, W.L. Watney, Shear-wave anisotropy reveals pore fluid pressure-induced seismicity in the U.S. midcontinent. Credit: Sci. Adv. 3, e1700443 (2017).

As concern rises about earthquakes induced by human activity like oil exploration, geologists at the University of Kansas report a new understanding about recent earthquakes in Kansas and Oklahoma. This breakthrough may one day lead to a method for predicting where induced earthquakes might occur and may help the energy industry and regulators decide where they can safely place wells.

In a paper published online today in Science Advances, K. Alex Nolte, doctoral student in the Department of Geology; George Tsoflias, associate professor of the department; Tandis Bidgoli, assistant scientist at the Kansas Geological Survey, and Lynn Watney, senior scientific fellow at KGS, report they were able to use an array of sensors in the Wellington oil field in south-central Kansas to detect signals of local earthquakes that point to an increase in fluid pressure in particular areas of the subsurface. The ability to directly detect earthquake-causing pressure may enable geologists to develop methods of predicting which areas of the subsurface might be prone to induced earthquakes.

“It’s very promising, but we haven’t solved anything yet,” Nolte said. “There are still a lot of hurdles to cross.”

The published paper provides new insights, but it is also unusual because its lead author, Nolte, is still a student. Few scientists, let alone students, ever publish in one of the prestigious journals like Science Advances that are produced by the American Association for the Advancement of Science. The publication is Nolte’s first, and it deals with a problem affecting his hometown of Wichita.

The study was prompted by a startling increase in earthquakes in what had previously been the seismically quiet midcontinent. In the more than three decades between 1977 and 2012, only 15 earthquakes with a magnitude of 3.0 or greater were recorded in the entire state of Kansas. A magnitude 3.0 earthquake is typically felt by humans. Since 2012 more than 100 earthquakes of 3.0 or greater have been recorded in only two counties in the state, Sumner and Harper. These include the largest earthquake ever monitored in Kansas in November 2014, a magnitude 4.9 event near the Sumner County town of Milan. The frequency of earthquakes has continued to increase. Between May 2015 and July 2017 the KU array of sensors detected more than 2,400 earthquakes in Sumner County alone, ranging in magnitude from 0.4 to 3.6.

A number of researchers have already linked the increasing occurrence of earthquakes in the area with human activity, specifically an oil boom that has produced ever increasing amounts of wastewater. Every oil well produces wastewater. This is true of conventional wells and of wells that employ hydraulic fracturing (known popularly as fracking). The oil boom led to more oil wells being drilled in the area, which led to a sharp increase in the volume of wastewater. Researchers now believe the increased injection of wastewater into the salty aquifer in the subsurface, the Arbuckle, caused the increase in earthquakes.

Because conditions in the subsurface vary and a perfect storm of problems must be present for a wastewater injection well to induce an earthquake, only a relatively small fraction of injection wells cause tremors. This makes it difficult for regulators and the energy industry to determine where they can place wells.

Like sponges made of rock, aquifers store fluid in their pores. Injected wastewater increases the pressure of fluid in the aquifer’s pores and in fractures (cracks) in the rock. An earthquake is triggered when the fluid pushing against the rock affects an existing fault that is already close to slipping. If researchers can detect regions of elevated fluid pressure in the aquifer’s pores, they might be able to predict where induced earthquakes would likely occur.

The geologists tracked the increase in pore pressure by noticing a difference in the way seismic waves from recent earthquakes, presumably injection-induced, act compared with the way waves from older, naturally occurring earthquakes act. The group studied what geologists call shear-waves, or S-waves, looking closely at their anisotropy, a phenomenon where waves split in two with one component of the wave traveling along the fractures in the rock and the second component traveling perpendicular or nearly perpendicular to the orientation of the fracture.

In the naturally occurring earthquakes that do not involve high pressure, the wave component traveling along the fractures moves faster than the wave component moving perpendicularly to the fractures. In the induced earthquakes in Kansas, the geologists found the opposite.

“Such changes, or ‘flips’, in fast S-wave orientation had been previously documented in natural earthquakes and volcanic settings where there exist zones critically stressed by pore fluid pressure,” Tsoflias said. “Our observation of S-wave flips in recent southern Kansas earthquakes provides for the first time evidence of increasing pore pressure in the region from seismological data.”

Reference:
K.A. Nolte, G.P. Tsoflias, T.S. Bidgoli, W.L. Watney, Shear-wave anisotropy reveals pore fluid pressure-induced seismicity in the U.S. midcontinent. Sci. Adv. 3, e1700443 (2017). DOI: 10.1126/sciadv.1700443

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

Ancient penguin was as big as a (human) Pittsburgh Penguin

ancient giant penguin Kumimanu biceae
This illustration provided by Gerald Mayr shows the size of an ancient giant penguin Kumimanu biceae. On Tuesday, Dec. 12, 2017, researchers announced their find of fossils from approximately 60-55 million years ago, discovered in New Zealand, that put the creature at about 5 feet, 10 inches (1.77 meters) long when swimming, and 223 pounds (101 kilograms). (Gerald Mayr/Senckenberg Research Institute via AP)

Fossils from New Zealand have revealed a giant penguin that was as big as a grown man, roughly the size of the captain of the Pittsburgh Penguins.

The creature was slightly shorter in length and about 20 pounds (9 kilograms) heavier than the official stats for hockey star Sidney Crosby. It measured nearly 5 feet, 10 inches (1.77 meters) long when swimming and weighed in at 223 pounds (101 kilograms).

If the penguin and the Penguin faced off on the ice, however, things would look different. When standing, the ancient bird was maybe only 5-foot-3 (1.6 meters).

The newly found bird is about 7 inches (18 centimeters) longer than any other ancient penguin that has left a substantial portion of a skeleton, said Gerald Mayr of the Senckenberg Research Institute and Natural History Museum in Frankfurt, Germany. A potentially bigger rival is known only from a fragment of leg bone, making a size estimate difficult.

The biggest penguin today, the emperor in Antarctica, stands less than 4 feet (1.2 meters) tall.

Mayr and others describe the giant creature in a paper released Tuesday by the journal Nature Communications. They named it Kumimanu biceae, which refers to Maori words for a large mythological monster and a bird, and the mother of one of the study’s authors. The fossils are 56 million to 60 million years old.

That’s nearly as old as the very earliest known penguin fossils, which were much smaller, said Daniel Ksepka, curator at the Bruce Museum of Greenwich, Connecticut. He has studied New Zealand fossil penguins but didn’t participate in the new study.

The new discovery shows penguins “got big very rapidly” after the mass extinction of 66 million years ago that’s best known for killing off the dinosaurs, he wrote in an email.

That event played a big role in penguin history. Beforehand, a non-flying seabird would be threatened by big marine reptile predators, which also would compete with the birds for food. But once the extinction wiped out those reptiles, the ability to fly was not so crucial, opening the door for penguins to appear.

Birds often evolve toward larger sizes after they lose the ability to fly, Mayr said. In fact, the new paper concludes that big size appeared more than once within the penguin family tree.

What happened to the giants?

Mayr said researchers believe they died out when large marine mammals like toothed whales and seals showed up and provided competition for safe breeding places and food. The newcomers may also have hunted the big penguins, he said.

Reference:
Gerald Mayr et al. A Paleocene penguin from New Zealand substantiates multiple origins of gigantism in fossil Sphenisciformes, Nature Communications (2017). DOI: 10.1038/s41467-017-01959-6

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

The oldest plesiosaur was a strong swimmer

skeleton of Rhaeticosaurus
Paleontologists Tanja Wintrich and Martin Sander from the University of Bonn inspect the skeleton of Rhaeticosaurus in the laboratory of the LWL-Museum für Naturkunde in Münster (Germany).
Credit: Yasuhisa Nakajima

Plesiosaurs were especially effective swimmer. These long extinct “paddle saurians” propelled themselves through the World’s oceans by employing “underwater flight” — similar to sea turtles and penguins. Paleontologist from the University of Bonn, Germany, now describe the oldest plesiosaur in the journal Science Advances, together with colleagues from Japan and France. The find comes from the youngest part of the Triassic period and is about 201 million years old.

Instead of laboriously pushing the water out of the way with their paddles, plesiosaurs were gliding elegantly along with limbs modified to underwater wings. Their small head was placed on a long, streamlined neck. The stout body contained strong muscles keeping those wings in motion. Compared to the other marine reptiles, the tail was short because it was only used for steering. This evolutionary design was very successful, but curiously it did not evolve again after the extinction of the plesiosaurs” says paleontologist Prof. Martin Sander from the Steinmann Institute of Geology, Mineralogy, and Paleontology of the University of Bonn.

The long extinct paddle saurians easily could have held their own against today’s water animals. Whereas sea turtles mainly use their strong forelimbs for propulsion, the plesiosaurs moved all four limbs together, resulting in powerful thrust. These ancient animals did not have a shell like turtles, however. Plesiosaurs fed on fish. Numerous fossils document a global distribution of the group during the Jurassic and Cretaceous periods.

A private collector discovered the fossil in a clay pit

The private collector Michael Mertens discovered a truly exceptional specimen during quarrying operations in a clay pit in Westphalia, Germany, in 2013. The subsequent evaluation by the LWL-Museum für Naturkunde in Münster, Germany, revealed that the find represents a marine reptile from the Triassic, the period that predates the Jurassic. This news reached Prof. Sander of the University of Bonn while on sabbatical in Los Angeles. “I could not believe that there was a plesiosaur from the Triassic, given that these animals had been studied by paleontologist for nearly 300 years, and never was there one older than Jurassic” said Sander. He also notes that only through the timely and efficient cooperation between the private collector, the natural heritage protection agency, the Münster museum, and the scientists, the unique find could be described and published. The detailed research by Ph.D. student Tanja Wintrich of the Steinmann Institute of the University of Bonn revealed that the find indeed represent the oldest plesiosaur at an age of about 201 million years, which makes it the only plesiosaur skeleton from the Triassic period.

The reconstructed length of the skeleton is 237 cm (7′ 7″) (part of the neck was lost to quarrying). “We are looking at a relatively small plesiosaur” says Wintrich. The scientists bestowed the name Rhaeticosaurus mertensi on the unique fossil. The first part of the name refers to its geologic age (Rhaetian) and the second part honors the discoverer. Together with scientists from Osaka Natural History Museum, the University of Osaka, the University of Tokyo and the Paris Natural History Museum, the team from Bonn studied a bone sample. First, they “looked” into the interior of the bone using computed tomography, and then they cut thin sections for microscopic study from especially promising parts of the bone.

Scientists study the growth marks in the bones

Based on the growth marks in the bones, the researchers recognized that Rhaeticosaurus was a fast growing youngster. They compared the thin sections with those from young plesiosaurs from the Jurassic and Cretacous. “Plesiosaurs apparently grew extremely fast before reaching sexual maturity” Sander sums up the results. The paleontologists interprets this as a clear indication that plesiosaurs were warmblooded. Since plesiosaurs spread quickly all over the world, “they must have been able to regulate their body temperature to be able to invade cooler parts of the ocean” says the paleontologist. Because of their warmbloodedness and their efficient locomotion, plesiosaurs were extremely successful and widespread — until they disappeared from the face of the earth. Sander says “at the end of the Cretaceous, a meteorite impact together with volcanic eruptions lead to an ecosystem collapse, of which plesiosaurs were prominent victims.”

Reference:
Tanja Wintrich, Shoji Hayashi, Alexandra Houssaye, Yasuhisa Nakajima, P. Martin Sander. A Triassic plesiosaurian skeleton and bone histology inform on evolution of a unique body plan. Science Advances, 2017 DOI: 10.1126/sciadv.1701144

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

Chemical tipping point of magma determines explosive potential of volcanoes

bubbly magma in laboratory
This is bubbly magma in laboratory used as starting material for the viscosity experiments. Credit: Danilo Di Genova

Volcanic eruptions are the most spectacular expression of the processes acting in the interior of any active planet. Effusive eruptions consist of a gentle and steady flow of lava on the surface, while explosive eruptions are violent phenomena that can eject hot materials up to several kilometres into the atmosphere.

The transition between these eruptions represents one of the most dangerous natural hazards.

Understanding the mechanisms governing such transition has inspired countless studies in Earth Sciences over the last decades.

In a new study led by Dr Danilo Di Genova, from the University of Bristol’s School of Earth Sciences, an international team of scientists provide evidence, for the first time, that a subtle tipping point of the chemistry of magmas clearly separates effusive from explosive eruptions worldwide.

Moreover, they demonstrate that variabilities at the nanoscale of magmas can dramatically increase the explosive potential of volcanoes.

Dr Di Genova said: “The new experimental data, thermodynamic modelling and analysis of compositional data from the global volcanic record we presented in our study provide combined evidence for a sudden discontinuity in the flow behaviour of rhyolitic magmas that guides whether a volcano erupts effusively or explosively.

“The identified flow-discontinuity can be crossed by small compositional changes in rhyolitic magmas and can be induced by crystallisation, assimilation, magma replenishment or mixing.

“Composition-induced flow behaviour variations may also originate from changes in magmas intrinsic parameters such as temperature, pressure or oxygen fugacity.”

These can result in revitalization of a previously “locked” magma chamber via chemical fluidification or may hinder efficient degassing and lead to increased explosive potential via chemical “stiffening” of a magma.

Furthermore, the study showed how the sudden precipitation of iron-bearing nanocrystals, which have been recently found in volcanic rocks, can increase the explosive potential of a magma via both depletion of iron in the melt structure and providing nucleation points for gas bubbles which drive explosive eruption.

Reference:
D. Di Genova, S. Kolzenburg, S. Wiesmaier, E. Dallanave, D. R. Neuville, K. U. Hess, D. B. Dingwell. A compositional tipping point governing the mobilization and eruption style of rhyolitic magma. Nature, 2017; 552 (7684): 235 DOI: 10.1038/nature24488

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

Fossil orphans reunited with their parents after half a billion years

Pseudooides
This is an image of Pseudooides. Credit: University of Bristol

Everyone wants to be with their family over the holidays, but spare a thought for a group of orphan fossils that have been separated from their parents since the dawn of animal evolution, over half a billion years ago.

For decades, paleontologists have puzzled over the microscopic fossils of Pseudooides, which are smaller than sand grains.

The resemblance of the fossils to animal embryos inspired their name, which means ‘false egg’.

The fossils preserve stages of embryonic development frozen in time by miraculous processes of fossilisation, which turned their squishy cells into stone.

Pseudooides fossils have a segmented middle like the embryos of segmented animals, such as insects, inspiring grand theories on how complex segmented animals may have evolved.

A team of paleontologists from the University of Bristol’s School of Earth Sciences and Peking University have now peered inside the Pseudooides embryos using X-rays and found features that link them to the adult stages of another fossil group.

It turns out that these adult stages were right under the scientists’ noses all along: they have been found long ago in the same rocks as Pseudooides.

Surprisingly, these long-lost family members are not complex segmented animals at all, but ancestors of modern jellyfish.

Dr Kelly Vargas from the University of Bristol said: “It seems that, in trying to classify these fossils, we’ve previously been barking up the wrong branch of the animals family tree.”

Professor Philip Donoghue, also from the University of Bristol, co-led the research with Professor Xiping Dong of Peking University.

Professor Donoghue added “We couldn’t have reunited these ancient family members without the amazing technology which allowed us to see inside the fossilized bodies of the embryos and adults.”

The team used the Swiss Light Source, a gigantic particle accelerator near Zurich, Switzerland, to supply the X-rays used to image the inside of the fossils.

This showed that the details of segmentation in the Pseudooides embryos to be nothing more than the folded edge of an opening, which developed into the rim of the cone-shaped skeleton that once housed the anemone-like stage in the life cycle of the ancient jellyfish.

Luis Porras, who helped make the discovery while still a student at the University of Bristol, said: “Pseudooides fossils may not tell us about how complex animals evolved, but they provide insights into the how embryology of animals itself has evolved.

“The embryos of living jellyfish usually develop into bizarre alien-like larvae which metamorphose into anemone-like adults before the final jellyfish (or ‘medusa’) phase.

“Pseudooides did things differently and more efficiently, developing directly from embryo to adult. Perhaps living jellyfish are a poor guide to ancestral animals.”

Professor Donoghue added: “It is amazing that these organisms were fossilised at all.

“Jellyfish are made up of little more than goo and yet they’ve been turned to stone before they had any chance to rot: a mechanism which some scientists refer to as the ‘Medusa effect’, named after the gorgon of Greek mythology who turned into stone anyone that laid eyes upon her.”

The Bristol team are still looking for fossil remains of the rest of Pseudooides life cycle, including the ‘medusa’ jellyfish stage itself. However, jellyfish fossils are few and far between, perhaps ironically because the ‘Medusa effect’ doesn’t seem to work on them.

In the interim, the embryos of Pseudooides have been reunited with their adult counterparts, just in time for Christmas.

Reference:
Baichuan Duan, Xi-Ping Dong, Luis Porras, Kelly Vargas, John A. Cunningham, Philip C. J. Donoghue. The early Cambrian fossil embryo Pseudooides is a direct-developing cnidarian, not an early ecdysozoan. Proceedings of the Royal Society B: Biological Sciences, 2017; 284 (1869): 20172188 DOI: 10.1098/rspb.2017.2188

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

Oldest ice core ever drilled outside the polar regions

A joint research team from the United States and China ventured to the Guliya Ice Cap in Tibet in 2015
A joint research team from the United States and China ventured to the Guliya Ice Cap in Tibet in 2015. They drew a core from the ice that was more than 1,000 feet long, the bottom of which dates back to more than half a million years ago.
Credit: Photo by Giuliano Bertagna, courtesy of the Byrd Polar and Climate Research Center.

The oldest ice core ever drilled outside the polar regions may contain ice that formed during the Stone Age — more than 600,000 years ago, long before modern humans appeared.

Researchers from the United States and China are now studying the core — nearly as long as the Empire State Building is tall — to assemble one of the longest-ever records of Earth’s climate history.

What they’ve found so far provides dramatic evidence of a recent and rapid temperature rise at some of the highest, coldest mountain peaks in the world.

At the American Geophysical Union meeting on Thursday, Dec. 14, they report that there has been a persistent increase in both temperature and precipitation in Tibet’s Kunlun Mountains over the last few centuries. The change is most noticeable on the Guliya Ice Cap, where they drilled the latest ice core. In this region, the average temperature has risen 1.5 degrees Celsius (2.7 degrees Fahrenheit) in the last 50 years and the average precipitation has risen by 2.1 inches per year over the past 25 years.

Lonnie Thompson, Distinguished University Professor in the School of Earth Sciences at The Ohio State University and co-leader of the international research team, said that the new data lend support to computer models of projected climate changes.

“The ice cores actually demonstrate that warming is happening, and is already having detrimental effects on Earth’s freshwater ice stores,” Thompson said.

Earth’s largest supply of freshwater ice outside of the Arctic and Antarctica resides in Tibet — a place that was off limits to American glaciologists until 20 years ago, when Ohio State’s Byrd Polar and Climate Research Center (BPCRC) began a collaboration with China’s Institute of Tibetan Plateau Research. There, glaciologist Yao Tandong secured funding for a series of joint expeditions from the Chinese Academy of Sciences.

“The water issues created by melting ice on the Third Pole, along with that from the Arctic and Antarctica, have been recognized as important contributors to the rise in global sea level. Continued warming in these regions will result in even more ice melt with the likelihood of catastrophic environmental consequences,” Yao noted.

The name “Third Pole” refers to high mountain glaciers located on the Tibetan Plateau and in the Himalaya, in the Andes in South America, on Kilimanjaro in Africa, and in Papua, Indonesia — all of which have been studied by the Ohio State research team.

Of particular interest to the researchers is a projection from the Intergovernmental Panel on Climate Change that future temperatures on the planet will rise faster at high altitudes than they will at sea level. The warming at sea level is expected to reach 3 degrees Celsius by the year 2100, and possibly double that, or 6 degrees Celsius, at the highest mountain peaks in the low latitudes.

“The stable isotopic records that we’ve obtained from five ice cores drilled across the Third Pole document climate changes over the last 1,000 years, and contribute to a growing body of evidence that environmental conditions on the Third Pole, along with the rest of the world, have changed significantly in the last century,” Thompson said. “Generally, the higher the elevation, the greater the rate of warming that’s taking place.”

Around the world, hundreds of millions of people depend on high-altitude glaciers for their water supply. The Guliya Ice Cap is one of many Tibetan Plateau ice caches that provide fresh water to Central, South, and Southeast Asia.

“There are over 46,000 mountain glaciers in that part of the world, and they are the water source for major rivers,” Thompson said.

In September and October of 2015, the team ventured to Guliya and drilled through the ice cap until they hit bedrock. They recovered five ice cores, one of which is more than 1,000 feet long.

The cores are composed of compressed layers of snow and ice that settled on the western Kunlun Mountains year after year. In each layer, the ice captured chemicals from the air and precipitation during wet and dry seasons. Today, researchers analyze the chemistry of the different layers to measure historical changes in climate.

Based on dating of radioactive elements measured by scientists at the Swiss research center ETH Zurich, the ice at the base of the core may be at least 600,000 years old.

The oldest ice core drilled in the Northern Hemisphere was found in Greenland in 2004 by the North Greenland Ice Core Project and was dated to roughly 120,000 years, while the oldest continuous ice core record recovered on Earth to date is from Antarctica, and extends back 800,000.

Over the next few months, the American and Chinese research teams will analyze the chemistry of the core in detail. They will look for evidence of temperature changes caused by ocean circulation patterns in both the North Atlantic and tropical Pacific Oceans, which drive precipitation in Tibet as well as the Indian monsoons. For instance, one important driver of global temperatures, El Niño, leaves its chemical mark in the snow that falls on tropical glaciers.

Ultimately, researchers hope the work will reveal the linkages that exist between ice loss in tropical mountain glaciers and climate processes elsewhere on the planet. Thompson, Yao, and German ecologist Volker Mosbrugger are co-chairing a Third Pole Environment Program to focus on basic science and policy-relevant issues.

“The more we study the different components of the environment of the Third Pole, the better we understand climate change and its linkages among Earth’s three polar regions,” Yao said.

Note: The above post is reprinted from materials provided by Ohio State University. Original written by Pam Frost Gorder.

Dinosaur parasites trapped in 100-million-year-old amber tell blood-sucking story

Hard tick grasping a dinosaur feather preserved in 99 million-year-old Burmese amber.
Hard tick grasping a dinosaur feather preserved in 99 million-year-old Burmese amber. Modified from the open access article published in Nature Communications: ‘Ticks parasitised feathered dinosaurs as revealed by Cretaceous amber assemblages.’ Credit: Paper authors.

Fossilised ticks discovered trapped and preserved in amber show that these parasites sucked the blood of feathered dinosaurs almost 100 million years ago, according to a new article published in Nature Communications today.

Sealed inside a piece of 99 million-year-old Burmese amber researchers found a so-called hard tick grasping a feather. The discovery is remarkable because fossils of parasitic, blood-feeding creatures directly associated with remains of their host are exceedingly scarce, and the new specimen is the oldest known to date.

The scenario may echo the famous mosquito-in-amber premise of Jurassic Park, although the newly-discovered tick dates from the Cretaceous period (145-66 million years ago) and will not be yielding any dinosaur-building DNA: all attempts to extract DNA from amber specimens have proven unsuccessful due to the short life of this complex molecule.

“Ticks are infamous blood-sucking, parasitic organisms, having a tremendous impact on the health of humans, livestock, pets, and even wildlife, but until now clear evidence of their role in deep time has been lacking,” says Enrique Peñalver from the Spanish Geological Survey (IGME) and leading author of the work.

Cretaceous amber provides a window into the world of the feathered dinosaurs, some of which evolved into modern-day birds. The studied amber feather with the grasping tick is similar in structure to modern-day bird feathers, and it offers the first direct evidence of an early parasite-host relationship between ticks and feathered dinosaurs.

“The fossil record tells us that feathers like the one we have studied were already present on a wide range of theropod dinosaurs, a group which included ground-running forms without flying ability, as well as bird-like dinosaurs capable of powered flight,” explains Dr Ricardo Pérez-de la Fuente, a research fellow at Oxford University Museum of Natural History and one of the authors of the study.

“So although we can’t be sure what kind of dinosaur the tick was feeding on, the mid-Cretaceous age of the Burmese amber confirms that the feather certainly did not belong to a modern bird, as these appeared much later in theropod evolution according to current fossil and molecular evidence”.

The researchers found further, indirect evidence of ticks parasitising dinosaurs in Deinocroton draculi, or “Dracula’s terrible tick”, belonging to a newly-described extinct group of ticks. This new species was also found sealed inside Burmese amber, with one specimen remarkably engorged with blood, increasing its volume approximately eight times over non-engorged forms. Despite this, it has not been possible to directly determine its host animal.

“Assessing the composition of the blood meal inside the bloated tick is not feasible because, unfortunately, the tick did not become fully immersed in resin and so its contents were altered by mineral deposition,” explains Dr Xavier Delclòs, an author of the study from the University of Barcelona and IRBio.

But indirect evidence of the likely host for these novel ticks was found in the form of hair-like structures, or setae, from the larvae of skin beetles (dermestids), found attached to two Deinocroton ticks preserved together. Today, skin beetles feed in nests, consuming feathers, skin and hair from the nest’s occupants. And as no mammal hairs have yet been found in Cretaceous amber, the presence of skin beetle setae on the two Deinocroton draculi specimens suggests that the ticks’ host was a feathered dinosaur.

“The simultaneous entrapment of two external parasites – the ticks – is extraordinary, and can be best explained if they had a nest-inhabiting ecology as some modern ticks do, living in the host’s nest or in their own nest nearby,” says Dr David Grimaldi of the American Museum of Natural History and an author of the work.

Together, these findings provide direct and indirect evidence that ticks have been parasitising and sucking blood from dinosaurs within the evolutionary lineage leading to modern birds for almost 100 million years. While the birds were the only lineage of theropod dinosaurs to survive the mass extinction at the end of the Cretaceous 66 million years ago, the ticks did not just cling on for survival, they continued to thrive.

Reference:
Enrique Peñalver et al, parasitised feathered dinosaurs as revealed by Cretaceous amber assemblages, Nature Communications (2017). DOI: 10.1038/s41467-017-01550-z

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

Small earthquakes at fracking sites may be early indicators of bigger tremors to come

Small earthquakes (yellow stars) can be induced during hydraulic fracturing when high-pressure fluid (blue arrows) is pumped into horizontal wells to crack rock layers containing natural gas.
Small earthquakes (yellow stars) can be induced during hydraulic fracturing when high-pressure fluid (blue arrows) is pumped into horizontal wells to crack rock layers containing natural gas. Earthquakes (green stars) can also be induced by disposal of wastewater from gas and oil operations into deep vertical wells. Over time, the disposal layer migrates away from the well (dashed green arrows), destabilizing preexisting faults. Credit: Clara Yoon

Stanford geoscientists have devised a way of detecting thousands of faint, previously missed earthquakes triggered by hydraulic fracturing, or “fracking.”

The technique can be used to monitor seismic activities at fracking operations to help reduce the likelihood of bigger, potentially damaging earthquakes from occurring, according to the new study.

“These small earthquakes may act like canaries in a coalmine,” said study co-author William Ellsworth, a professor (research) of geophysics at Stanford’s School of Earth, Energy & Environmental Sciences. “When they happen, they should be viewed as cautionary indicators of underground conditions that could lead to larger earthquakes.”

Fracking involves injecting high-pressure fluid underground to crack open rocks and release the natural gas trapped inside. As the rocks crack, they produce tiny earthquakes that were typically too small to be detected – until now.

“In our study, you can actually see individual earthquakes occurring next to the section of a well that’s being fracked,” said Stanford PhD student Clara Yoon, lead author of the study published in the Journal of Geophysical Research.

Arkansas earthquakes

In October 2010, residents near an Arkansas natural gas field were shaken by a magnitude 4 earthquake that was followed by two larger aftershocks in February 2011.

Scientists say these large earthquakes were caused by injections of wastewater from fracking sites into deep underground wells, and not by fracking operations closer to the surface.

“These were some of the first earthquakes related to shale-gas development to draw national attention,” Ellsworth said.

Earthquakes of magnitude 4 and higher have subsequently rattled Oklahoma, Texas and other gas- and oil-producing states.

Data mining

Using an advanced data-mining algorithm developed by Yoon and her colleagues, the Stanford team conducted a retrospective analysis of seismic activity in Arkansas prior to the magnitude 4 event. The algorithm uses earthquake-pattern recognition to generate detailed records of seismicity.

The analysis tracked seismic events generated at production wells that utilized fracking and at deeper wastewater-disposal wells nearby.

“We were interested in how the sequence that led to the magnitude 4 earthquake got started,” Yoon said. “We looked at the earliest period of seismic activity in 2010, from June 1 to September 1, when wastewater injection was just beginning.”

When Yoon ran the algorithm on this dataset, she discovered more than 14,000 small, previously unreported earthquakes. By comparing the timing and location of the tremors with fluid-injection data provided by the state of Arkansas, Yoon was able to demonstrate that most of the earthquakes were the direct result of fracking operations at 17 of the 53 production wells.

“That was a surprise,” said co-author Gregory Beroza, the Wayne Loel Professor of Geophysics at Stanford. “It had been thought, and we thought, that early earthquakes in this area were related to wastewater injection. But we found that the majority were caused by fracking.”

Persistent quakes

Many of the fracking-induced earthquakes were also bigger and more persistent that expected – unusual properties indicating potential trouble ahead.

Earthquakes generated by fracking are typically no larger than magnitude 0. That’s equivalent to the amount of energy released when a milk carton hits the floor after falling off a counter.

But several earthquakes observed in the study were magnitude 1, which is 31 times stronger than a magnitude 0 quake. A few were above magnitude 2, which is 1,000 times stronger than magnitude 0.

Most fracking-induced quakes occur near the well and dissipate quickly. But some of the Arkansas earthquakes were located far from the wellbore and continued weeks after fracking operations had ended.

“We were particularly surprised by the size and persistence of the seismicity,” Ellsworth said. “When earthquakes during fracking operations are larger than expected and persist for weeks, it indicates a high level of stress in that area. Faults under high stress are unstable and can slip, triggering larger earthquakes.”

The fact that fracking near wastewater wells induced thousands of earthquakes – too many, too big and lasting too long – was a red flag that stress conditions deeper down were also primed to create the instability that triggered larger earthquakes, he added.

“We want to encourage continuous seismic monitoring before fracking operations start, while they’re in progress and after they’ve finished,” Beroza said. “The algorithm Clara developed offers an efficient, cost-effective method for getting more information out of existing data, so that in the future informed decisions can be made that reduce the chance of larger earthquakes from happening.”

Reference:
Clara E. Yoon et al. Seismicity During the Initial Stages of the Guy-Greenbrier, Arkansas, Earthquake Sequence, Journal of Geophysical Research: Solid Earth (2017). DOI: 10.1002/2017JB014946

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

New research improves understanding of ancient landscapes

The Rio San Juan transports sediment from the High Andes
The Rio San Juan transports sediment from the High Andes (the most distant mountains in the photo) across the Precordillera mountain range (foreground). Credit: Tomas Capaldi

Geologists use zircon mineral grains to reconstruct what the Earth and its landscapes looked like in ancient times. These microscopic grains, commonly the width of a human hair, record detailed information on when and where they formed, making them a standard tool for studying how our planet has changed through the ages.

A new study led by The University of Texas at Austin Jackson School of Geosciences suggests that scientists may be able to better leverage zircon data to understand how landscapes have evolved over time by considering a suite of factors that can skew zircon geochronologic data and interpretation of the origin of sediments.

The study, published on Dec. 1 in Earth and Planetary Science Letters, focused on a method called detrital zircon U-Pb (uranium-lead) geochronology. Zircon is an ideal mineral to trace landscape evolution because it is found in most crustal rocks, is very durable (harder than diamond), and contains three isotopic clocks (chronometers) that geoscientist can utilize.

The researchers found that estimates of landscape erosion and sediment dispersal could be improved by taking several factors into account:

Bedrock materials erode at different rates. This means sediment in rivers will be disproportionately enriched in zircon grains derived from weaker, erodible bedrock sources.
Zircon fertility, a term that indicates how many zircons are in a bedrock source region. Materials that produce less zircons can be underrepresented in a study unless this issue is accounted for.
Some zircons come from material that has been recycled over time. That means the zircons could contain complex signatures from multiple erosion events from different rocks.

Tomas Capaldi, a Ph.D. student in the Jackson School’s Department of Geological Sciences, led the study by collecting zircon grain samples from modern river watersheds in the Andes Mountains where the sediment sources and drainage networks are well known, which is not the case in ancient settings. Capaldi’s goal was to test whether zircons in the river sand accurately reflected the erosion patterns of the modern Andes, and to understand the extent that the aforementioned factors—zircon fertility, bedrock erosion rate, and sediment recycling— can impact results.

“We’re exploring how we can use sediment from modern rivers to calibrate ourselves for the ancient sedimentary record,” Capaldi said. The research involved collecting samples of river sands and bedrock from drainage basins in the Andes of western Argentina, across a region about one-fifth the size of Texas. Ph.D. student Margo Odlum and Ryan McKenzie, an assistant Professor at University of Hong Kong and former Jackson School Postdoctoral Fellow, assisted with the work. The team collected 21 river sand samples and 23 bedrock samples in the Rio Mendoza and Rio San Juan basins, dating about 120 zircon grains per sample.

The study found that the greatest difference between known upstream bedrock sources and downstream river sands was recorded by zircons in small, localized drainage catchments. Results varied by location. For example, researchers found that smaller, high elevation Andean river catchments eroded weaker bedrock units more easily and these sediment sources disproportionately contributedmore sand to the river than anticipated. In contrast, the zircons were more accurate when sampling larger river systems, which receive sand from the entire region and record the overall erosion of the Andes.

The findings are important because thousands of studies a year depend on detrital zircon U-Pb geochronology, said Jackson School Professor

Brian Horton, Capaldi’s advisor and a co-author on the paper.

“They all make an assumption that these sediments, these zircon grains, are accurate reflections or one-to-one tracers of their source regions,” Horton said. “It turns out there are some serious complications.”

The good news is that this can be largely accounted for by researchers in the field and lab, said co-author and Jackson School Professor Danny Stockli.

“You might have to take some of these complications that Tomas points out, maybe even leverage them, to obtain a better understanding of long-term landscape evolution,” he said.

Capaldi said that the study clarifies how these factors influence patterns of erosion and sediment dispersal, and warrant further research.

“This is the first stepping stone,” he said. “We’re trying to determine what these zircons, as potential erosional tracers, are really showing.”

Stockli said that the work is vital because studies of river sands have exploded over the past decade by researchers trying to reconstruct ancient landscapes, and oil and gas companies trying to determine the link between sand and the generation of offshore energy reservoirs.”If you understand how river drainage areas evolved you learn something about how the surface of the planet was shaped in the past,” Stockli said. “At the same time, people use these drainage areas to make predictions of how much sediment is delivered to the ocean. These sands provide a memory of landscape erosion as well as a predictor of what might be offshore.”

Reference:
Tomas N. Capaldi et al. Sediment provenance in contractional orogens: The detrital zircon record from modern rivers in the Andean fold-thrust belt and foreland basin of western Argentina, Earth and Planetary Science Letters (2017). DOI: 10.1016/j.epsl.2017.09.001

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

Ancient weakening of Earth’s crust explains unusual intraplate earthquakes

Distribution of intraplate earthquakes in central and eastern North America
Distribution of intraplate earthquakes in central and eastern North America with respect to ancient faulting from the assembly of supercontinent Rodinia and the Grenville orogeny (red lines) and from the breakup of Rodinia and opening of the Iapetus Ocean (green lines). Credit: Thomas and Powell

New research reveals that mysterious pockets of earthquake activity in the middle of North America all have one thing in common: Earth’s crust in these zones underwent significant deformation hundreds of millions of years ago, creating weak areas that are more susceptible to earthquakes. These fracturing features could help explain why some regions in central and eastern North America are more seismically active than others.

Earthquakes typically happen along fault lines, like California’s San Andreas fault, where the edges of Earth’s tectonic plates scrape against each other, releasing enough energy to shake the ground. Some seismic activity occurs in the middle of tectonic plates, but these earthquakes are generally random, occur rarely and are poorly understood.

But a few spots within the North American tectonic plate – thousands of kilometers away from the plate’s boundaries – experience earthquake activity frequently.

Seismologists have found geological evidence of past earthquakes greater than magnitude 7 in some regions in the eastern U.S. and Canada. For example, from December 1811 to February 1812, three magnitude-7 earthquakes shook southeastern Missouri, knocking down trees, damaging homes and disrupting the Mississippi River current.

Seismologists don’t know why these pockets of earthquakes occur in the middle of tectonic plates, but a new study suggests they happen in places where Earth’s crust experienced ancient fracturing events on top of old, buried fault lines.

It is important to better understand these intraplate seismic zones since the earthquakes associated with them have the potential to deal significant damage, said Christine Powell, a seismologist at the University of Memphis Center for Earthquake Research and Information in Memphis, Tennessee and co-author of the new study accepted for publication in Tectonics, a journal of the American Geophysical Union.

While California’s infrastructure is built to withstand large tremors, construction in central and eastern North America typically does not account for strong earthquakes. If a magnitude 7 earthquake happened within the North American tectonic plate today, communities would sustain serious injuries and face multi-billion-dollar damages to property, Powell said.

“We have to understand as much as we possibly can about why the earthquakes are here,” she said. “All of that information can then be used to help public safety and building construction.”

Waking up ancient faults

Seismologists know that many intraplate seismic zones overlap with ancient fault lines. But only parts of old fault lines in central and eastern North America show frequent earthquake activity. Unlike California, where earthquakes occur along the entire San Andreas Fault line, central and eastern North America experience seismic hiccups on only specific segments of old faults. The rest of the inner-North American faults are seismically inactive.

In the new study, Powell and her co-author Bill Thomas, an emeritus professor of geology at the University of Kentucky and now at the Geological Survey of Alabama in Tuscaloosa, reviewed the most active seismic spots in eastern and central North America to determine what geologic features may be involved with intraplate earthquakes.

Thomas and Powell examined three places in particular: the Charlevoix Seismic Zone (CSZ) in southeastern Canada, the Eastern Tennessee Seismic Zone (ETSZ), and the New Madrid Seismic Zone (NMSZ) along the Mississippi River valley between southeastern Missouri and western Tennessee. They surveyed the known geological characteristics of the three regions and soon realized each zone had experienced significant fracturing compared to other areas along the old faults.

The researchers reason that fracturing events from hundreds of millions of years ago have lowered the ability of Earth’s crust to withstand high levels of stress in these regions. This means that a weaker crust has a higher chance of breaking under the pressure of various geological forces, resulting in more seismic activity.

For example, roughly 357 million years ago, a large meteor hit the Charlevoix Seismic Zone, shattering rocks within the crust, likely creating the perfect conditions along the ancient fault to host future seismic activity, according to the researchers.

“You can look up and down the rest of those long faults and you don’t see the earthquake activity in other places. It’s just where that big meteorite smacked it,” Powell said.

An old fault line running through the Eastern Tennessee Seismic Zone is bent instead of straight, which created additional fracturing in the area as the North American Plate moved over time. The New Madrid Seismic Zone encompasses a segment of ancient fault lines where the two sides of the North American continent began to pull apart, but stopped short of making a significant break. The plates instead crunched back together, leaving the crust significantly faulted and fractured.

In each case, crustal deformation has weakened the crust along ancient fault lines, according to the researchers’ findings.

Past research has examined intraplate seismic zones individually, but no study has yet made an overall comprehensive attempt to explain all of them, Thomas said.

“This is the first [study] that actually answers the question: why do [intraplate earthquake zones] happen where they do,” Powell said.

The researchers point out that there are other spots within eastern and central North America that may have concentrated crustal deformation but lack significant seismic activity. Therefore, they suspect that crustal deformation is necessary for creating intraplate seismic zones, but intraplate earthquakes occur only in places with the right present-day crustal forces.

“If the various forces acting on the crust are oriented in the right direction, those faults down there will be reactivated,” Powell said.

This story is republished courtesy of AGU Blogs (http://blogs.agu.org), a community of Earth and space science blogs, hosted by the American Geophysical Union. Read the original story here.

Note: The above post is reprinted from materials provided by American Geophysical Union.

How much can 252-million-year-old ecosystems tell us about modern Earth? A lot

This map of Pangea shows the distribution of life during the late Permian period
This map of Pangea shows the distribution of life during the late Permian period. Many species exclusively thrived near the equator, including early amphibian tetrapods and early crocodiles and dinosaurs, while animals like dicynodonts (early mammal-relatives) were in greater abundance farther north and south. Credit: Brandon Peecook, The Field Museum, using illustrations from Wikimedia Commons

A whopping 252 million years ago, Earth was crawling with bizarre animals, including dinosaur cousins resembling Komodo dragons and bulky early mammal-relatives, a million years before dinosaurs even existed. New research shows us that the Permian equator was both a literal and figurative hotspot: it was, for the most part, a scorching hot desert, on top of having a concentration of unique animals. Here, you could find some of the first tetrapods to emerge from the water and live on land, living right next to newly evolved, dinosaur and crocodile-like reptiles. Many of these species were wiped out after an extinction which changed life on the planet forever.

In a paper published in Earth-Science Reviews, paleontologists studied fossil sites all over the world from the late Permian to get an idea of what lived where. They found an unusual assortment of species near the equator, and one that is comparable to the modern tropics — except that the array of large, carnivorous reptiles would look very out of place anywhere on Earth today.

“The tropics act as a diversity center — stuff that has gone extinct elsewhere is still alive there, and there’s new stuff evolving,” explains Postdoctoral Researcher Brandon Peecook, co-author of the paper. While it makes sense that the warm, wet rainforests we see now have incredible diversity, it seems counterintuitive that these fiery, hot deserts were home to an exceptional range of species, especially because diversity at the equator fluctuates so much historically.

These findings about the late Permian beg the question, “Why are we seeing so much biodiversity at the equator?” This is something scientists have yet to answer, but it shows us that biodiversity at the tropics isn’t intuitive, and isn’t consistent. What scientists know for sure is that regardless of desert or rainforest, climate change negatively impacts living things.

This unequaled comparison of Permian climate and species distribution to modern events shows us that while many changes are natural and we see them throughout our planet’s history, drastic changes like this can be triggered by something much larger — volcanic activity likely caused this in the Permian, and human activity is the suspected culprit today. After the Permian extinction, “it was almost as though the slate had been wiped clean, and all the ecosystems had to rebuild,” says Peecook. This event altered life permanently and while new animals evolved and thrived, the process of recovery took millions of years, and the animals that were lost never returned.

“If we want to know how Earth’s systems work, what’s expected and what’s normal, we need to look to the past,” and the fossil record is the best measure of ecosystem stability. As we already begin to face extinctions and carbon levels similar to those before the Permian extinction, examining these patterns over time gives us the evidence we need to measure and minimize our impact on climate, preventing further permanent damage to our planet’s ecosystems and animals.

Reference:
Massimo Bernardi, Fabio Massimo Petti, Evelyn Kustatscher, Matthias Franz, Christoph Hartkopf-Fröder, Conrad C. Labandeira, Torsten Wappler, Johanna H.A. van Konijnenburg-van Cittert, Brandon R. Peecook, Kenneth D. Angielczyk. Late Permian (Lopingian) terrestrial ecosystems: A global comparison with new data from the low-latitude Bletterbach Biota. Earth-Science Reviews, 2017; 175: 18 DOI: 10.1016/j.earscirev.2017.10.002

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

Nuclear technology unlocks 50-million-year-old time capsules

Sample of amber
Sample of amber. Credit: Monash University

A scientific analysis of fossilised tree resin has caused a rethink of Australia’s prehistoric ecosystem, and could pave the way to recovering more preserved palaeobiological artefacts from the time of dinosaurs or prehistoric mammals.

In a project that could be straight out of Jurassic Park, Monash University researchers and collaborators from the Deakin Institute of Frontier Materials (IFM) used nuclear magnetic resonance to investigate the make-up of 52 to 40-million-year-old amber samples recovered from sites in Anglesea, Victoria, and Strahan, Tasmania.

Study lead author, Andrew Coward, an Honours student from the Monash School of Earth, Atmosphere and Environment, said the amber captured a period in time during the Eocene Epoch (56 to 33.9 million years ago).

“This is an unparalleled method of preservation, and provides insights into past organisms, ecosystems and environments,” said Mr Coward.

Amber, also called resinite or fossilised resin, is organic material created through the fossilisation of the resins of seed plants.

“Our collaboration aimed to identify the original plant sources of amber at Anglesea and Strahan and to establish the way they degraded during their tens of millions of years underground,” said co-researcher Associate Professor Jeffrey Stilwell, also from the Monash School of Earth, Atmosphere and Environment.

Project collaborator Dr Luke O”Dell from IFM said this degradation could potentially have a major impact on the preserved palaeobiological information contained within the samples, and the sort of information we can recover about Earth’s ancient past.

By measuring how each sample absorbed and re-emitted electromagnetic radiation, Dr O”Dell, was able to probe the physical and chemical properties of the amber and identify distinct botanical sources.

Monash University researchers conducted their own chemical analysis using reflective and infrared spectroscopy.

“Nuclear magnetic resonance turned out to be extremely useful as it provided us with a unique fingerprint of the chemical structure of each piece of amber,” Associate Professor Stilwell said.

“This study, sponsored by the Australian Research Council Discovery Projects scheme (led by Stilwell), could represent the first unambiguous discovery of indigenous Class II amber in Australia,” he said.

“Amber can be separated into different classes based on which plants it came from, and the discovery of Class II amber from the Anglesea site could mean certain prehistoric plants capable of producing cadinene-based amber were native to Australia during the Eocene Epoch, which is something that has never been proven due to their absence from the fossil record.

“Another possibility is that there may even be an entirely new, previously unidentified botanical source capable of exuding cadinene resins.”

Associate Professor Stilwell said other outcomes of the study had important implications for the field of amber prospecting, by demonstrating how even visually altered amber could still be used to recover valid palaeobotanical and palaeobiological data.

Of particular note was the amount of amber that showed no significant chemical changes despite being extensively visibly altered during millions of years beneath the earth, suggesting such samples could still have preserved intact palaeobiological and palaeoenvironmental information.

Understanding which factors and reactions influence amber as it degrades and how this impacts stored biochemical information could make it much easier for the future collection of amber with intact palaeobiological data.

Dr O”Dell said the discovery was even more significant due to Australia’s sparse amber record.

“While there have been recent reports of amber stretching back 100 million years to the mid-Cretaceous period, the largest known deposits of Australian amber come from the Latrobe Valley coal measures in Victoria and are roughly 3 million to 23 million years old,” he said.

All amber samples that remained after IFM’s analysis are now being housed with Museums Victoria.

The project’s full findings, “Taphonomy and chemotaxonomy of Eocene amber from southeastern Australia,” have been accepted for publication in the Organic Geochemistry journal.

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

What geologists got wrong about the world’s biggest failed rift

Dramatic cliffs on the shores of Lake Superior.
Geologists have disproved a theory about what stopped the formation of the Midcontinent Rift, which is responsible for creating the dramatic cliffs on the shores of Lake Superior. Credit: Northwestern University

Geologists have corrected a mix-up that made an ancient geological structure in the central U.S. seem hundreds of miles shorter than it really is. The biggest failed rift known to geologists is even bigger than originally thought, according to research that will be presented at the American Geophysical Union fall meeting Dec. 11 in New Orleans.

The Midcontinent Rift, which started but failed to split North America in two pieces 1.1 billion years ago, is the biggest failed rift ever discovered. It was formed when 350,000 cubic miles of volcanic rock poured out of the rift and formed the beautiful cliffs around Lake Superior. South of Lake Superior, the volcanic rocks are covered by younger rocks, so it wasn’t clear how far the rift extended.

For decades, geologists believed the rift stopped in southern Michigan, but a joint study by geologists at the University of Illinois at Chicago (UIC), Northwestern University, the University of Oklahoma and the University of Göttingen, Germany, reveals the rift extends much farther – as far south as Oklahoma.

Successful geologic rifts cut through the Earth’s surface, splitting continents in two and forming new ocean basins, but something prevented the Midcontinent Rift from completing this process. Until now, geologists believed the Grenville Front halted the Midcontinent Rift’s growth.

“Geologists got confused by the Grenville Front, which appears in southeast Canada,” said Carol Stein, lead author of the study and professor of Earth and environmental sciences at UIC. “It marks where another continent collided with North America after the Midcontinent Rift formed.”

“Somehow the idea developed that the Grenville Front extended south into the U.S., cutting off the Midcontinent Rift in Southern Michigan,” explained coauthor Seth Stein, professor of Earth and planetary sciences in Northwestern’s Weinberg College of Arts and Sciences. “That didn’t make sense because there wasn’t any good reason for the rift to stop there.

To sort this out, the researchers used gravity data to “see” underground.

“The Midcontinent Rift shows up nicely,” explained coauthor Reece Elling, a graduate student in Earth and planetary sciences at Northwestern. “The rift’s volcanic rocks are very dense, so they pull downward strongly. In contrast, the Grenville Front doesn’t have these dense rocks, and so it doesn’t cause the gravity high we see.”

The gravity high shows that the underground rift has an east arm that extends south from Lake Superior through Michigan, Ohio, Kentucky, Tennessee and Alabama. The gravity high also maps a western arm that extends as far south as Oklahoma.

“This make sense in terms of how continents grow,” said coauthor Jonas Kley of the University of Göttingen, Germany.

The new analysis “makes the Midcontinent Rift great again,” explains coauthor Randy Keller, professor emeritus of geology and geophysics at the University of Oklahoma. “It’s a major structure and should be recognized accordingly.”

The results of the study will be published in GSA Today.

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

Related Articles