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Ancient carpet shark discovered with ‘spaceship-shaped’ teeth

One of the tiny fossilized teeth recovered from Galagadon, so named for the shape of its teeth, which resemble the spaceships in the video game Galaga. Credit: Copyright Terry Gates
One of the tiny fossilized teeth recovered from Galagadon, so named for the shape of its teeth, which resemble the spaceships in the video game Galaga. Credit: Copyright Terry Gates

The world of the dinosaurs just got a bit more bizarre with a newly discovered species of freshwater shark whose tiny teeth resemble the alien ships from the popular 1980s video game Galaga.

Unlike its gargantuan cousin the megalodon, Galagadon nordquistae was a small shark (approximately 12 to 18 inches long), related to modern-day carpet sharks such as the “whiskered” wobbegong. Galagadon once swam in the Cretaceous rivers of what is now South Dakota, and its remains were uncovered beside “Sue,” the world’s most famous T. rex fossil.

“The more we discover about the Cretaceous period just before the non-bird dinosaurs went extinct, the more fantastic that world becomes,” says Terry Gates, lecturer at North Carolina State University and research affiliate with the North Carolina Museum of Natural Sciences. Gates is lead author of a paper describing the new species along with colleagues Eric Gorscak and Peter J. Makovicky of the Field Museum of Natural History.

“It may seem odd today, but about 67 million years ago, what is now South Dakota was covered in forests, swamps and winding rivers,” Gates says. “Galagadon was not swooping in to prey on T. rex, Triceratops, or any other dinosaurs that happened into its streams. This shark had teeth that were good for catching small fish or crushing snails and crawdads.”

The tiny teeth — each one measuring less than a millimeter across — were discovered in the sediment left behind when paleontologists at the Field Museum uncovered the bones of “Sue,” currently the most complete T. rex specimen ever described. Gates sifted through the almost two tons of dirt with the help of volunteer Karen Nordquist, whom the species name, nordquistae, honors. Together, the pair recovered over two dozen teeth belonging to the new shark species.

“It amazes me that we can find microscopic shark teeth sitting right beside the bones of the largest predators of all time,” Gates says. “These teeth are the size of a sand grain. Without a microscope you’d just throw them away.”

Despite its diminutive size, Gates sees the discovery of Galagadon as an important addition to the fossil record. “Every species in an ecosystem plays a supporting role, keeping the whole network together,” he says. “There is no way for us to understand what changed in the ecosystem during the mass extinction at the end of the Cretaceous without knowing all the wonderful species that existed before.”

Gates credits the idea for Galagadon’s name to middle school teacher Nate Bourne, who worked alongside Gates in paleontologist Lindsay Zanno’s lab at the N.C. Museum of Natural Sciences.

Reference:
Terry A. Gates, Eric Gorscak, Peter J. Makovicky. New sharks and other chondrichthyans from the latest Maastrichtian (Late Cretaceous) of North America. Journal of Paleontology, 2019; 1 DOI: 10.1017/jpa.2018.92

Note: The above post is reprinted from materials provided by North Carolina State University.

Crocodiles have complex past

Representative Image

A new study throws into question the notion that today’s crocodiles and alligators have a simple evolutionary past.

Previous research has pointed to crocodiles and alligators starting with a land-based ancestor some 200 million years ago and then moving to fresh water, becoming the semi-aquatic ambush predators they are today.

But a new analysis, published online today in the journal Scientific Reports, offers a different story. Modern crocodiles and alligators came from a variety of surroundings beginning in the early Jurassic Period, and various species occupied a host of ecosystems over time, including land, estuarine, freshwater and marine.

As University of Iowa researcher and study co-author Christopher Brochu says, “Crocodiles are not living fossils. Transitions between land, sea, and freshwater were more frequent than we thought, and the transitions were not always land-to-freshwater or freshwater-to-marine.”

Brochu and colleagues from Stony Brook University pieced together crocodile and alligator ancestry by analyzing a large family tree showing the evolutionary history of living and extinct crocodylomorphs (modern crocodiles and alligators and their extinct relatives). The team was then able to predict the ancestral habitat for several divergence points on the evolutionary tree.

This suggests a complex evolutionary history not only of habitat, but of form. Those living at sea had paddles instead of limbs, and those on land often had hoof-like claws and long legs. These did not all evolve from ancestors that looked like modern crocodiles, as has long been assumed.

Reference:
Eric W. Wilberg, Alan H. Turner, Christopher A. Brochu. Evolutionary structure and timing of major habitat shifts in Crocodylomorpha. Scientific Reports, 2019; 9 (1) DOI: 10.1038/s41598-018-36795-1

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

Fossilized slime of 100-million-year-old hagfish shakes up vertebrate family tree

Tethymyxine tapirostrum, is a 100-million-year-old, 12-inch long fish embedded in a slab of Cretaceous period limestone from Lebanon, believed to be the first detailed fossil of a hagfish.
Tethymyxine tapirostrum, is a 100-million-year-old, 12-inch long fish embedded in a slab of Cretaceous period limestone from Lebanon, believed to be the first detailed fossil of a hagfish. Credit: Tetsuto Miyashita, University of Chicago

Paleontologists at the University of Chicago have discovered the first detailed fossil of a hagfish, the slimy, eel-like carrion feeders of the ocean. The 100-million-year-old fossil helps answer questions about when these ancient, jawless fish branched off the evolutionary tree from the lineage that gave rise to modern-day jawed vertebrates, including bony fish and humans.

The fossil, named Tethymyxine tapirostrum,is a 12-inch long fish embedded in a slab of Cretaceous period limestone from Lebanon. It fills a 100-million-year gap in the fossil record and shows that hagfish are more closely related to the blood-sucking lamprey than to other fishes. This means that both hagfish and lampreys evolved their eel-like body shape and strange feeding systems after they branched off from the rest of the vertebrate line of ancestry about 500 million years ago.

“This is a major reorganization of the family tree of all fish and their descendants. This allows us to put an evolutionary date on unique traits that set hagfish apart from all other animals,” said Tetsuto Miyashita, PhD, a Chicago Fellow in the Department of Organismal Biology and Anatomy at UChicago who led the research. The findings are published this week in the Proceedings of the National Academy of Sciences.

The slimy dead giveaway

Modern-day hagfish are known for their bizarre, nightmarish appearance and unique defense mechanism. They don’t have eyes, or jaws or teeth to bite with, but instead use a spiky tongue-like apparatus to rasp flesh off dead fish and whales at the bottom of the ocean. When harassed, they can instantly turn the water around them into a cloud of slime, clogging the gills of would-be predators.

This ability to produce slime is what gave away the Tethymyxine fossil. Miyashita used an imaging technology called synchrotron scanning at Stanford University to identify chemical traces of soft tissue that were left behind in the limestone when the hagfish fossilized. These soft tissues are rarely preserved, which is why there are so few examples of ancient hagfish relatives to study.

The scanning picked up a signal for keratin, the same material that makes up fingernails in humans. Keratin, as it turns out, is a crucial part of what makes the hagfish slime defense so effective. Hagfish have a series of glands along their bodies that produce tiny packets of tightly-coiled keratin fibers, lubricated by mucus-y goo. When these packets hit seawater, the fibers explode and trap the water within, turning everything into shark-choking slop. The fibers are so strong that when dried out they resemble silk threads; they’re even being studied as possible biosynthetic fibers to make clothes and other materials.

Miyashita and his colleagues found more than a hundred concentrations of keratin along the body of the fossil, meaning that the ancient hagfish probably evolved its slime defense when the seas included fearsome predators such as plesiosaurs and ichthyosaurs that we no longer see today.

“We now have a fossil that can push back the origin of the hagfish-like body plan by hundreds of millions of years,” Miyashita said. “Now, the next question is how this changes our view of the relationships between all these early fish lineages.”

Shaking up the vertebrate family tree

Features of the new fossil help place hagfish and their relatives on the vertebrate family tree. In the past, scientists have disagreed about where they belonged, depending on how they tackled the question. Those who rely on fossil evidence alone tend to conclude that hagfish are so primitive that they are not even vertebrates. This implies that all fishes and their vertebrate descendants had a common ancestor that — more or less — looked like a hagfish.

But those who work with genetic data argue that hagfish and lampreys are more closely related to each other. This suggests that modern hagfish and lampreys are the odd ones out in the family tree of vertebrates. In that case, the primitive appearance of hagfish and lampreys is deceptive, and the common ancestor of all vertebrates was probably something more conventionally fish-like.

Miyashita’s work reconciles these two approaches, using physical evidence of the animal’s anatomy from the fossil to come to the same conclusion as the geneticists: that the hagfish and lampreys should be grouped separately from the rest of fishes.

“In a sense, this resets the agenda of how we understand these animals,” said Michael Coates, PhD, professor of organismal biology and anatomy at UChicago and a co-author of the new study. “Now we have this important corroboration that they are a group apart. Although they’re still part of vertebrate biodiversity, we now have to look at hagfish and lampreys more carefully, and recognize their apparent primitiveness as a specialized condition.

Paleontologists have increasingly used sophisticated imaging techniques in the past few years, but Miyashita’s research is one of a handful so far to use synchrotron scanning to identify chemical elements in a fossil. While it was crucial to detect anatomical structures in the hagfish fossil, he believes it can also be a useful tool to help scientists detect paint or glue used to embellish a fossil or even outright forge a specimen. Any attempt to spice up a fossil specimen leaves chemical fingerprints that light up like holiday decorations in a synchrotron scan.

“I’m impressed with what Tetsuto has marshaled here,” Coates said. “He’s maxed out all the different techniques and approaches that can be applied to this fossil to extract information from it, to understand it and to check it thoroughly.”

The study, “A Hagfish from the Cretaceous Tethys Sea and a Reconciliation of the Morphological-Molecular Conflict in Early Vertebrate Phylogeny,” was supported by the National Science Foundation and the National Science and Engineering Research Council (Canada). Additional authors include Robert Farrar and Peter Larson from the Black Hills Institute of Geological Research; Phillip Manning and Roy Wogelius from the University of Manchester; Nicholas Edwards and Uwe Bergmann from the SLAC National Accelerator Laboratory; Jennifer Anné from the Children’s Museum of Indianapolis; and Richard Palmer and Philip Currie from the University of Alberta.

Note: The above post is reprinted from materials provided by University of Chicago Medical Center. Original written by Matt Wood.

Large volcanic eruption in Scotland may have contributed to prehistoric global warming

This is a false color electron-microscope image of a resorbed apatite crystal (green) in pitchstone glass (blue). The composition of the pitchstone glass and the characteristic mineral textures are identical in the studied pitchstone sites of the Sgùrr of Eigg and Òigh-sgeir, although over 30km apart, indicating a common origin, and thus a large and geographically widespread volcanic eruption. Credit: Valentin Troll
This is a false color electron-microscope image of a resorbed apatite crystal (green) in pitchstone glass (blue). The composition of the pitchstone glass and the characteristic mineral textures are identical in the studied pitchstone sites of the Sgùrr of Eigg and Òigh-sgeir, although over 30km apart, indicating a common origin, and thus a large and geographically widespread volcanic eruption. Credit: Valentin Troll

Around 56 million years ago, global temperatures spiked. Researchers at Uppsala University and in the UK now show that a major explosive eruption from the Red Hills on the Isle of Skye may have been a contributing factor to the massive climate disturbance. Their findings have been published in the journal Scientific Reports.

Large explosive volcanic eruptions can have lasting effects on climate and have been held responsible for severe climate effects in Earth’s history. One such event occurred around 56 million years ago when global temperatures increased by 5-8 °C. This event has been named the Paleocene-Eocene Thermal Maximum (PETM). The warm period was associated with volcanic activity in the North Atlantic region, especially in Greenland, the British Isles and the present day North Sea region. However, until now, no large-scale explosive eruptions had been confirmed in current-day Scotland.

A team of researchers at Uppsala University, Sweden, the Universities of Durham and St Andrews in the UK, and the Scottish Environmental Research Centre in Glasgow, now seem to have found a missing piece of the puzzle. By studying volcanic rocks called pitchstones from islands more than 30 kilometres apart in the Inner Hebrides off the west coast of Scotland, the researchers have found plausible evidence of a major eruption from what is today the Isle of Skye.

The researchers used several different methods to compare the pitchstones recovered from the two sites (Sgùrr of Eigg and Òigh-sgeir) including isotope geochemistry. Samples from the two pitchstone outcrops display identical textures and compositions in all analyses, confirming that the two outcrops represent deposits of a single, massive and explosive volcanic eruption. The researcher’s geochemical data identify the Red Hills on Skye, around 40 kilometres to the North, as the most likely vent area for this large eruption. Using this vent location, a reconstruction estimates the eruption to have been similar in magnitude to the infamous Krakatoa eruption of 1883, one of the deadliest and most destructive volcanic events in recorded history.

Earth scientists have long thought that the Scottish sector of the North Atlantic Volcanic province did not see any large explosive eruptions at the time of the PETM. This notion is now contradicted by the findings of the current study and the researchers conclude that large explosive volcanic events in the Scottish sector of the North Atlantic Volcanic Province were likely a major contributing factor to the climate disturbance of the PETM.

Around 56 million years ago, global temperatures spiked. Researchers at Uppsala University and in the UK now show that a major explosive eruption from the Red Hills on the Isle of Skye may have been a contributing factor to the massive climate disturbance. Their findings have been published in the journal Scientific Reports.

Large explosive volcanic eruptions can have lasting effects on climate and have been held responsible for severe climate effects in Earth’s history. One such event occurred around 56 million years ago when global temperatures increased by 5-8 °C. This event has been named the Paleocene-Eocene Thermal Maximum (PETM). The warm period was associated with volcanic activity in the North Atlantic region, especially in Greenland, the British Isles and the present day North Sea region. However, until now, no large-scale explosive eruptions had been confirmed in current-day Scotland.

A team of researchers at Uppsala University, Sweden, the Universities of Durham and St Andrews in the UK, and the Scottish Environmental Research Centre in Glasgow, now seem to have found a missing piece of the puzzle. By studying volcanic rocks called pitchstones from islands more than 30 kilometres apart in the Inner Hebrides off the west coast of Scotland, the researchers have found plausible evidence of a major eruption from what is today the Isle of Skye.

The researchers used several different methods to compare the pitchstones recovered from the two sites (Sgùrr of Eigg and Òigh-sgeir) including isotope geochemistry. Samples from the two pitchstone outcrops display identical textures and compositions in all analyses, confirming that the two outcrops represent deposits of a single, massive and explosive volcanic eruption. The researcher’s geochemical data identify the Red Hills on Skye, around 40 kilometres to the North, as the most likely vent area for this large eruption. Using this vent location, a reconstruction estimates the eruption to have been similar in magnitude to the infamous Krakatoa eruption of 1883, one of the deadliest and most destructive volcanic events in recorded history.

Earth scientists have long thought that the Scottish sector of the North Atlantic Volcanic province did not see any large explosive eruptions at the time of the PETM. This notion is now contradicted by the findings of the current study and the researchers conclude that large explosive volcanic events in the Scottish sector of the North Atlantic Volcanic Province were likely a major contributing factor to the climate disturbance of the PETM.

Reference:
Valentin R. Troll, C. Henry Emeleus, Graeme R. Nicoll, Tobias Mattsson, Robert M. Ellam, Colin H. Donaldson, Chris Harris. A large explosive silicic eruption in the British Palaeogene Igneous Province. Scientific Reports, 2019; 9 (1) DOI: 10.1038/s41598-018-35855-w

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

International Chronostratigraphic Chart “Version 2018/08”

International Chronostratigraphic Chart “Version 2018/08”
International Chronostratigraphic Chart “Version 2018/08”

Click here (PDF or JPG) to download the latest version (v2018/08) of the International Chronostratigraphic Chart.

Translations of the chart: Chinese  (v2018/08: PDF or JPG), Spanish (v2018/08: PDF or JPG), Belgium Dutch (v2018/08: PDF or JPG), Turkish (v2018/08: PDF or JPG), Netherlands Dutch (v2018/08: PDF or JPG), Catalan (v2018/08: PDF or JPG), Finnish  (v2017/02: PDF or JPG), American Spanish (v2017/02: PDF or JPG), Iberian Portuguese (v2017/02: PDF or JPG), Brazilian Portuguese (v2017/02: PDF or JPG), Russian (v2017/02: PDF or JPG), German (v2017/02: PDF or JPG), Basque (v2015/01: PDF or JPG), Norwegian (v2015/01: PDF or JPG), Lithuanian (v2015/01: PDF or JPG), Japanese (v2014/02: PDF or JPG) and French (v2012).

The old versions can be download at the following links: 2008 (PDF or JPG), 2009 (PDF or JPG), 2010 (PDF or JPG), 2012 (PDF or JPG), 2013/01 (PDF or JPG), 2014/02 (PDF or JPG) , 2014/10 (PDF or JPG), 2015/01 (PDF or JPG), 2016/04 (PDF or JPG), 2016/10 (PDF or JPG), 2017/02 (PDF or JPG), 2018/07 (PDF or JPG)  and the ChangeLog for 2012-2018.

 

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New study quantifies deep reaction behind ‘superdeep’ diamonds

Diamond
The Cullinan Diamond, the largest gem-quality diamond found, was discovered in South Africa in 1905. Superdeep diamonds have been uncovered at the same mine. Credit: Public Domain

Whether they are found in an engagement ring or an antique necklace, diamonds usually generate quick reactions from their recipients. Now, new research shows deep inside the Earth, fast reactions between subducted tectonic plates and the mantle at specific depths may be responsible for generating the most valuable diamonds.

The diamonds mined most often around the world are formed in the Earth’s mantle at depths of around 150-250 kilometers (93-155 miles). They are created by extreme pressure and temperature of at least 1050 degrees Celsius (1922 degrees Fahrenheit). Only a small amount of these diamonds make it to mineable regions since most are destroyed in the process of reaching the Earth’s crust via deep source volcanic eruptions.

But a tiny portion of mined diamonds, called sub-lithospheric or superdeep diamonds, are formed at much deeper depths than others, mostly in two rich zones at depths of 250-450 kilometers (155-279 miles) and 600-800 kilometers (372-497 miles). These diamonds stand out from others due to their compositions, which occasionally include materials from the deep Earth like majorite garnet, ferropericlase and bridgmanite.

“Although only composing 1 percent of the total mined diamonds, it seems lots of large and high-purity diamonds are superdeep diamonds, so they have good value as gems,” said Feng Zhu the lead author of the new study in Geophysical Research Letters, a journal of the American Geophysical Union, who was a post-doctoral geology researcher at the University of Michigan when he performed the research.

No previous theory has completely explained the reason why very few diamonds have been found near the surface from the area at depths of 450-600 kilometers (372-497 miles) – the region between the zones where most superdeep diamonds are formed.

The new study seeks to explain this phenomenon. Zhu, now a post-doctoral researcher at the University of Hawai’i, and his colleagues believe the two superdeep areas where diamonds are formed are rich in the gems due to high production rates. The new study explains what drives the diamond-producing reaction in some areas and what slows it down in other areas.

Diamond formation

According to the authors, diamonds can form anywhere in the mantle, which extends from about 35 to 2,890 kilometers (21-1,800 miles) below the Earth’s surface. However, humans rarely see most of the diamonds formed. Very few diamonds survive the volcanic trip to the Earth’s crust where we can sample them.

That means the chances of finding diamonds from deep regions in the mantle, which produce relatively few of the gems, is extremely small. Only 1 percent of mined diamonds come from superdeep regions.

“In our hypothesis, the production of diamonds at any depth in the mantle is possible, it’s just the production rate is different, so they have a different chance to be sampled in the crust,” Zhu said.

Creating diamonds

In order to mimic the extreme pressures experienced deep inside planets, the study’s authors used diamond anvil cells and a 1,000-ton multi-anvil apparatus at the University of Michigan. Both these devices allow researchers to compress sub-millimeter-sized material in extreme pressures. They compressed magnesium carbonate powder with iron foil in extreme heats and managed to create minuscule diamond grains visible through scanning electron microscopes.

They found that when conditions are right, diamond grains can form as quickly as every couple of minutes, and never took longer than a few hours to form, although the growth of gem diamonds may take much longer time in an actual melting fluid environment.

In the shallower region rich in superdeep diamond formation, 250-450 kilometers (155-279 miles) down, a subducting tectonic plate pushes under the Earth’s mantle. This supplies plenty of carbonate, which creates “factories on a conveyor belt” for diamonds when combined with the iron from the mantle, the authors said.

High temperatures promote reactions which form diamonds, but pressure does the opposite. At depths roughly 475 kilometers (295 miles) below the surface, the pressure increases, and the reactions slow down drastically, the authors said. That’s why few diamonds are found near the Earth surface coming from between 450-600 kilometers (372-497 miles).

“When your pressure reaches the diamond stable region, it will form. But when you increase pressure it will form at lower rates. You have a trade off there,” Zhu said.

One exception to this rule is in the deeper region of 600-800 kilometers (372-497 miles) beneath the surface. In this region, accumulation of carbonate due to the stagnation of tectonic slabs pushing downwards makes up for the overdose in pressure. So while the reactions slow down, higher temperatures and an abundance of carbonate makes for a diamond-rich region.

Zhu said the new study adds to scientists’ understanding of the Earth’s mantle, about which relatively little is known for sure.

“Superdeep diamond inclusions bring us the only mineral samples from the Earth’s deep mantle,” he said. “Seeing is believing, and these inclusions provide a solid ground for the studies on the inaccessible mantle.”

Reference:
Feng Zhu et al. Kinetic control on the depth distribution of superdeep diamonds, Geophysical Research Letters (2018). DOI: 10.1029/2018GL080740

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

Scientists find increase in asteroid impacts on ancient Earth by studying the Moon

Image depicts the change in impact rate modeled in this paper. Some of the craters used in the study on both the moon and Earth are highlighted in the background. Credit: Data from NASA GSFC / LRO / Arizona State University; Artwork by Rebecca Ghent
Image depicts the change in impact rate modeled in this paper. Some of the craters used in the study on both the moon and Earth are highlighted in the background. Credit: Data from NASA GSFC / LRO / Arizona State University; Artwork by Rebecca Ghent

An international team of scientists is challenging our understanding of a part of Earth’s history by looking at the Moon, the most complete and accessible chronicle of the asteroid collisions that carved our solar system.

In a study published today in Science, the team shows the number of asteroid impacts on the Moon and Earth increased by two to three times starting around 290 million years ago.

“Our research provides evidence for a dramatic change in the rate of asteroid impacts on both Earth and the Moon that occurred around the end of the Paleozoic era,” said lead author Sara Mazrouei, who recently earned her PhD in the Department of Earth Sciences in the Faculty of Arts & Science at the University of Toronto (U of T). “The implication is that since that time we have been in a period of relatively high rate of asteroid impacts that is 2.6 times higher than it was prior to 290 million years ago.”

It had been previously assumed that most of Earth’s older craters produced by asteroid impacts have been erased by erosion and other geologic processes. But the new research shows otherwise.

“The relative rarity of large craters on Earth older than 290 million years and younger than 650 million years is not because we lost the craters, but because the impact rate during that time was lower than it is now,” said Rebecca Ghent, an associate professor in U of T’s Department of Earth Sciences and one of the paper’s co-authors. “We expect this to be of interest to anyone interested in the impact history of both Earth and the Moon, and the role that it might have played in the history of life on Earth.”

Scientists have for decades tried to understand the rate that asteroids hit Earth by using radiometric dating of the rocks around them to determine their ages. But because it was believed erosion caused some craters to disappear, it was difficult to find an accurate impact rate and determine whether it had changed over time.

A way to sidestep this problem is to examine the Moon, which is hit by asteroids in the same proportions over time as Earth. But there was no way to determine the ages of lunar craters until NASA’s Lunar Reconnaissance Orbiter (LRO) started circling the Moon a decade ago and studying its surface.

“The LRO’s instruments have allowed scientists to peer back in time at the forces that shaped the Moon,” said Noah Petro, an LRO project scientist based at NASA Goddard Space Flight Center.

Using LRO data, the team was able to assemble a list of ages of all lunar craters younger than about a billion years. They did this by using data from LRO’s Diviner instrument, a radiometer that measures the heat radiating from the Moon’s surface, to monitor the rate of degradation of young craters.

During the lunar night, rocks radiate much more heat than fine-grained soil called regolith. This allows scientists to distinguish rocks from fine particles in thermal images. Ghent had previously used this information to calculate the rate at which large rocks around the Moon’s young craters — ejected onto the surface during asteroid impact — break down into soil as a result of a constant rain of tiny meteorites over tens of millions of years. By applying this idea, the team was able to calculate ages for previously un-dated lunar craters.

When compared to a similar timeline of Earth’s craters, they found the two bodies had recorded the same history of asteroid bombardment.

“It became clear that the reason why Earth has fewer older craters on its most stable regions is because the impact rate was lower up until about 290 million years ago,” said William Bottke, an asteroid expert at the Southwest Research Institute in Boulder, Colorado and another of the paper’s coauthors. “The answer to Earth’s impact rate was staring everyone right in the face.”

The reason for the jump in the impact rate is unknown, though the researchers speculate it might be related to large collisions taking place more than 300 million years ago in the main asteroid belt between the orbits of Mars and Jupiter. Such events can create debris that can reach the inner solar system.

Ghent and her colleagues found strong supporting evidence for their findings through a collaboration with Thomas Gernon, an Earth scientist based at the University of Southampton in England who works on a terrestrial feature called kimberlite pipes. These underground pipes are long-extinct volcanoes that stretch, in a carrot shape, a couple of kilometers below the surface, and are found on some of the least eroded regions of Earth in the same places preserved impact craters are found.

“The Canadian shield hosts some of the best-preserved and best-studied of this terrain — and also some of the best-studied large impact craters,” said Mazrouei.

Gernon showed that kimberlite pipes formed since about 650 million years ago had not experienced much erosion, indicating that the large impact craters younger than this on stable terrains must also be intact.

“This is how we know those craters represent a near-complete record,” Ghent said.

While the researchers weren’t the first to propose that the rate of asteroid strikes to Earth has fluctuated over the past billion years, they are the first to show it statistically and to quantify the rate.

“The findings may also have implications for the history of life on Earth, which is punctuated by extinction events and rapid evolution of new species,” said Ghent. “Though the forces driving these events are complicated and may include other geologic causes, such as large volcanic eruptions, combined with biological factors, asteroid impacts have surely played a role in this ongoing saga.

“The question is whether the predicted change in asteroid impacts can be directly linked to events that occurred long ago on Earth.”

The findings are described in the study “Earth and Moon impact flux increased at the end of the Paleozoic,” published in Science. Support for the research was provided by the National Science and Engineering Research Council of Canada, NASA’s Solar System Exploration Research Virtual Institute, and the Natural Environment Research Council of the United Kingdom.

Reference:
Sara Mazrouei, Rebecca R. Ghent, William F. Bottke, Alex H. Parker, Thomas M. Gernon. Earth and Moon impact flux increased at the end of the Paleozoic. Science, 2019 DOI: 10.1126/science.aar4058

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

Geological fingerprinting of volcanic ash

The Santiaguito volcano: The Santiaguito dome complex in Guatemala regularly spews out plumes of gas and volcanic ash.
The Santiaguito volcano: The Santiaguito dome complex in Guatemala regularly spews out plumes of gas and volcanic ash.

Volcanic ash consists of tiny particles containing minerals and glass. LMU researchers have now used a new analytical technique based on quantitative chemical analysis under a scanning electron microscope to link their surface composition to activity during volcanic eruptions.

The Santiaguito volcanic complex in Guatemala first emerged in 1922, and has grown steadily since then. Over this period, one of the magma domes has discharged lava almost continuously, and often explosively releases clouds of gas and ash. Santiaguito is the source of some of the volcanic ash samples that Dr. Adrian Hornby of the Department of Earth and Environmental Sciences at LMU is analyzing as part of his EU-funded project AVAST (Advanced Volcanic ASh characTerisation). In a long-standing collaboration with researchers at the University of Liverpool, he has now applied a novel imaging procedure to examine ash samples collected on the flanks of Santiaguito. The results appear in the online journal Scientific Reports.

Volcanic ash consists of particles with diameter of less than 2 mm, and is typically made up of fragments of crystalline material and glass that are derived from magma. In the new study, Hornby employed a technology known as QEMSCAN (Quantitative Evaluation of Minerals by Scanning Electron Microscopy) Particle Mineralogical Analysis to investigate ash that had been vented in an explosive plume and ash from a pyroclastic flow caused by the sudden collapse of part of the rim of the active crater at the Santiaguito complex. “How magma fragments depends on the type of volcanic activity involved in its production, and this also changes the mineralogy that is found at the surfaces of the ash particles,” Hornby explains.

The surfaces of both Guatemalan ash samples exhibited various combinations of feldspar and glass, but the particles generated by the dome collapse had more glass and less feldspar on their surfaces than within the particles. This variation most probably reflects differences in fragmentation conditions between the two samples. “Our findings make a significant contribution to a better understanding of the origin and composition of volcanic ash – which is necessary to enable the risks associated with eruptions to be assessed.” In 2010, following the eruption of the Eyjafjallajökull volcano in Iceland, commercial air traffic in Europe was severely affected as the ash released by the event could damage aircraft jet engines.

Reference:
A. J. Hornby et al. Phase partitioning during fragmentation revealed by QEMSCAN Particle Mineralogical Analysis of volcanic ash, Scientific Reports (2019). DOI: 10.1038/s41598-018-36857-4

Note: The above post is reprinted from materials provided by Ludwig Maximilian University of Munich.

Waiting for the complete rupture

Where plates collide: The main frontal thrust (red line) extends over the entire length of the Himalayas. Credit: NASA Earth Observatory
Where plates collide: The main frontal thrust (red line) extends over the entire length of the Himalayas. Credit: NASA Earth Observatory

In April 2015, Nepal — and especially the region around the capital city, Kathmandu — was struck by a powerful tremor. An earthquake with a magnitude of 7.8 destroyed entire villages, traffic routes and cultural monuments, with a death toll of some 9,000.

However, the country may still face the threat of much stronger earthquakes with a magnitude of 8 or more. This is the conclusion reached by a group of earth scientists from ETH Zurich based on a new model of the collision zone between the Indian and Eurasian Plates in the vicinity of the Himalayas.

Using this model, the team of ETH researchers working with doctoral student Luca Dal Zilio, from the group led by Professor Taras Gerya at the Institute of Geophysics, has now performed the first high-resolution simulations of earthquake cycles in a cross-section of the rupture zone.

“In the 2015 quake, there was only a partial rupture of the major Himalayan fault separating the two continental plates. The frontal, near-surface section of the rupture zone, where the Indian Plate subducts beneath the Eurasian Plate, did not slip and remains under stress,” explains Dal Zilio, lead author of the study, which was recently published in the journal Nature Communications.

Normally, a major earthquake releases almost all the stress that has built up in the vicinity of the focus as a result of displacement of the plates. “Our model shows that, although the Gorkha earthquake reduced the stress level in part of the rupture zone, tension actually increased in the frontal section close to the foot of the Himalayas. The apparent paradox is that ‘medium-sized’ earthquakes such as Gorkha can create the conditions for an even larger earthquake,” says Dal Zilio.

Tremors of the magnitude of the Gorkha earthquake release stress only in the deeper subsections of the fault system over lengths of 100 kilometres. In turn, new and even greater stress builds up in the near-surface sections of the rupture zone.

According to the simulations performed by Dal Zilio and his colleagues, two or three further Gorkha quakes would be needed to build up sufficient stress for an earthquake with a magnitude of 8.1 or more. In a quake of this kind, the rupture zone breaks over the entire depth range, extending up to the Earth’s surface and laterally — along the Himalayan arc — for hundreds of kilometres. This ultimately leads to a complete stress release in this segment of the fault system, which extends to some 2,000 kilometres in total.

Historical data shows that mega events of this kind have also occurred in the past. For example, the Assam earthquake in 1950 had a magnitude of 8.6, with the rupture zone breaking over a length of several hundred kilometres and across the entire depth range. In 1505, a giant earthquake struck with sufficient power to produce an approximately 800-kilometre rupture on the major Himalayan fault. “The new model reveals that powerful earthquakes in the Himalayas have not just one form but at least two, and that their cycles partially overlap,” says Edi Kissling, Professor of Seismology and Geodynamics. Super earthquakes might occur with a periodicity of 400 to 600 years, whereas “medium-sized” quakes such as Gorkha have a recurrence time of up to a few hundred years. As the cycles overlap, the researchers expect powerful and dangerous earthquakes to occur at irregular intervals.

However, they cannot predict when another extremely large quake will next take place. “No one can predict earthquakes, not even with the new model. However, we can improve our understanding of the seismic hazard in a specific area and take appropriate precautions,” says Kissling.

The two-dimensional and high-resolution model also includes some research findings that were published after the Gorkha earthquake. To generate the simulations, the researchers used the Euler mainframe computer at ETH Zurich. “A three-dimensional model would be more accurate and would also allow us to make statements about the western and eastern fringes of the Himalayas. However, modelling the entire 2,000 kilometres of the rupture zone would require enormous computational power,” says Dal Zilio.

Reference:
Luca Dal Zilio, Ylona van Dinther, Taras Gerya, Jean-Philippe Avouac. Bimodal seismicity in the Himalaya controlled by fault friction and geometry. Nature Communications, 2019; 10 (1) DOI: 10.1038/s41467-018-07874-8

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

Drilling deep for clues on earthquakes

Civil and Environmental Engineering Assistant Professor Hiroki Sone stands on the drilling vessel Chikyu’s heliport. Credit: Hiroki Sone

Lingering motion sickness is one of the occupational hazards of working at sea off the coast of Japan for three weeks. Hiroki Sone can attest to that, having spent part of the fall 2018 semester on the deepest scientific oceanic drilling project ever.

“Maybe I shouldn’t nod too much,” says the assistant professor of civil and environmental engineering at the University of Wisconsin-Madison, a day after returning stateside. “I’m feeling dizzy.”

Sone and Ph.D. student Zirou Jin are part of the international team of scientists working on the Nankai Trough Seismogenic Zone Experiment. In the final phase of the 11-year experiment, researchers are drilling below the Nankai Trough, the meeting point of the Eurasian and Philippine Sea tectonic plates and the source of repeated earthquakes. If successful, it would be the first time scientists have reached a depth at which earthquakes spawn in a subduction zone, where one plate (in this case, the Philippine Sea) pushes under another.

The drilling, which reached a record depth in early December 2018 and will continue until March 2019, will yield rock samples and allow the team to install sensors, potentially unearthing new clues about the processes that drive earthquakes.

“We want to understand what kind of forces are accumulating in this plate boundary, because that’s the driving force for ground motion during earthquakes,” says Sone. “To be directly in there and see the material really improves our understanding of what is actually happening.”

Sone grew up in a Japanese society that’s understandably wary of earthquakes, given the long history of seismic activity in the country. He remembers elementary school visits from a truck with a shaking room that enabled students to practice safety maneuvers.

He was a graduate student at Kyoto University working on a thesis about a deadly earthquake in Taiwan when he heard about plans for the first NanTroSEIZE Integrated Ocean Drilling Program expedition, which launched in 2007. Six years later, he joined his first expedition on the Nankai Trough.

This time, he’s leading the group’s physical properties team. When cuttings—the rock debris generated during drilling—come to the surface, Sone’s team examines their densities to calculate changes in porosity, the percentage of empty space in the rock that’s filled by water. Porosity typically decreases with depth, but the researchers look for exceptions to that trend that will indicate higher-than-expected fluid pressure. Scientists have long postulated that fluid pressure along tectonic plate interfaces is abnormally high, which could encourage a plate to slip like a puck on an air hockey table. But no one has measured that fluid pressure at this depth, Sone says.

“This is a good opportunity to test those hypotheses and validate theories or maybe disprove some of them,” he says.

Sone will helicopter back onto the drilling vessel Chikyu, whose name means earth in Japanese, again in January 2019, while Jin will work a pair of two-week shifts in February and March. Work days are long aboard the Chikyu, with 12-hour shifts and limited internet access.

But the promise of rock core samples—much larger and more useful than cuttings—at the end is a powerful motivator. Jin is studying cores from a previous expedition for her Ph.D. work on the viscoplastic properties—how materials flow and deform over time—in Nankai Trough’s accretionary prism, the collection of rocks and sediment formed during plate subduction.

“We try to see how the stress accumulates,” she says.

By taking cores from the plate interface and slowly deforming them in the lab, Sone says, scientists can better understand the forces building up during the 100 to 400 years between the earthquakes that generate tsunamis in the Nankai Trough.

“It’s important to understand how the earth ruptures during these large earthquakes that happen in a matter of minutes, and scientists have focused on that for many decades,” he says. “But what happens in between the 100 years? How does the force accumulate to get ready for the next earthquake? That is an equally, if not more, important questions to ask that we have not addressed in the community. We’d like to make a breakthrough there to better forecast seismic hazards around the world.”

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

New computer modeling approach could improve understanding of megathrust earthquakes

Years before the devastating Tohoku earthquake struck the coast of Japan in 2011, the Earth’s crust near the site of the quake was starting to stir. Researchers at The University of Texas at Austin are using computer models to investigate if tiny tremors detected near this site could be connected to the disaster itself.

The research could help enhance scientists’ understanding of forces driving megathrust earthquakes — the world’s most powerful type of earthquake — and improve earthquake hazard assessment. The study was published on Dec.15, 2018, in Earth and Planetary Science Letters.

Lead author Thorsten Becker, a professor at the UT Jackson School of Geosciences and researcher at the University of Texas Institute for Geophysics, said that this was the first comprehensive study showing changes in barely perceptible tremor activity before the Tohoku megathrust earthquake.

“The part of the crust that is close to the place that eventually ruptured changes stress state a couple of years before the event,” said Becker. “By demonstrating this, our work complements studies of crustal deformation and our understanding of the forces driving earthquakes.”

The Institute for Geophysics is a research unit of the Jackson School of Geosciences.

While the location of the tremors raises questions about their potential linkage to the quake, Becker said that it’s unknown at the moment if the two events relate. However, the seismic signature of the tremors is helping refine a computer model that could help untangle the connection. This new modeling technique allows scientists to create a four-dimensional image of the Earth’s crust and interactions between tectonic plates, showing how forces pushing at the fault change over time.

Once the seismic data was inputted, the model matched observations of how the plate deformed in the years before and after the earthquake. This allowed the scientists to make inferences about the kind of forces taking place at the plate boundary, the point where one plate dives into the Earth’s hot, viscous mantle. In this semi-molten layer, solid rocks ooze and behave in unexpected ways, so understanding the dynamics of the layer could help identify the connection between pressure along a fault before and after a major earthquake.

The new research is significant because the model was originally developed using a different dataset: geodetic information about the shape of the Earth’s surface. By gaining similar results using different data sets — seismic waves and changes in the planet’s shape — scientists can be much more confident about the accuracy of earthquake models.

Becker believes that with the right research and support, advanced computer models can be used to study the physics of earthquakes and perhaps contribute to improved forecasts.

Currently, scientists can at best offer hazard maps showing known earthquake zones and a vague probability of an earthquake in the coming decades. Knowing more about when and where such a quake might strike, even within a few years, would represent a significant improvement on current earthquake forecasting and perhaps allow authorities and industry adequate time to prepare for such an event.

To this end, the authors hope their study will contribute to global efforts to improve earthquake hazard assessment, such as the Modeling Collaboratory for Subduction RCN, a new UT-led research collaboration network funded by the National Science Foundation (NSF).

The study was supported by the NSF and the Japanese Ministry of Education, Culture, Sports, Science and Technology.

Reference:
Thorsten W. Becker, Akinori Hashima, Andrew M. Freed, Hiroshi Sato. Stress change before and after the 2011 M9 Tohoku-oki earthquake. Earth and Planetary Science Letters, 2018; 504: 174 DOI: 10.1016/j.epsl.2018.09.035

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

Robot recreates the walk of a 290-million-year-old creature

This image from video provided by John Nyakatura in January 2019 shows computer-generated and robotic simulations of an Orobates Pabsti dinosaur’s footprints while walking. Nyakatura has spent years studying the four-legged plant-eater, which lived before the dinosaurs, and fascinates scientists “because of its position on the tree of life.”. Researchers believe the creature is a “stem amniote”—a likely ancestor of several groups of land-dwelling animals that later differentiated into modern mammals, birds and reptiles. Credit: John Nyakatura/Humboldt University via AP

How did the earliest land animals move? Scientists have used a nearly 300-million-year old fossil skeleton and preserved ancient footprints to create a moving robot model of prehistoric life.

Evolutionary biologist John Nyakatura at Humboldt University in Berlin has spent years studying a 290-million-year-old fossil dug up in central Germany’s Bromacker quarry in 2000. The four-legged plant-eater lived before the dinosaurs and fascinates scientists “because of its position on the tree of life,” said Nyakatura. Researchers believe the creature is a “stem amniote”—an early land-dwelling animal that later evolved into modern mammals, birds and reptiles.

Scientists believe the first amphibious animals emerged on land 350 million years ago and the first amniotes emerged around 310 million years ago.

The fossil, called Orabates pabsti, is a “beautifully preserved and articulated skeleton,” said Nyakatura. What’s more, scientists have previously identified fossilized footprints left by the 3-foot-long (90 cm) creature.

Nyakatura teamed up with robotics expert Kamilo Melo at the Swiss Federal Institute of Technology in Lausanne to develop a model of how the creature moved. Their results were published Wednesday in the journal Nature.

The researchers built a life-size replica of the prehistoric beast—”we carefully modeled each and every bone,” said Nyakatura—and then tested the motion in various ways that would lead its gait to match the ancient tracks, ruling out combinations that were not anatomically possible.

They repeated the exercise with a slightly-scaled up robot version , which they called OroBOT. The robot is made of motors connected by 3D-printed plastic and steel parts. The model “helps us to test real-world dynamics, to account for gravity and friction,” said Melo. The team also compared their models to living animals, including salamanders and iguanas.

Technology such as robotics, computer modeling and CT scans are transforming paleontology, “giving us ever more compelling reconstructions of the past,” said Andrew Farke, curator at the Raymond M. Alf Museum of Paleontology in Claremont, California, who was not involved in the study.

Based on the robot model, the scientists said they think the creature had more advanced locomotion than previously thought for such an early land animal. (Think more scampering than slithering.)

“It walked with a fairly upright posture,” said Melo. “It didn’t drag its belly or tail.”

University of Maryland paleontologist Thomas R. Holtz, who was not involved in the study, said the research suggests “an upright stance goes further back than we originally thought.”

Stuart Sumida, a paleontologist at California State University in San Bernardino and part of the initial team that excavated Orobates fossils, called it “an exciting study.” Sumida, who was not involved in the robot project, said the work provided “a much more confident window in to what happened long ago. It isn’t a time machine, but Nyakatura and colleagues have given us a tantalizing peek.”

Reference:
John A. Nyakatura et al. Reverse-engineering the locomotion of a stem amniote, Nature (2019). DOI: 10.1038/s41586-018-0851-2

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

Fossil deposit is much richer than expected

CHW 189 from the private collection of Herman Winkelhorst (Netherlands). The neck of the animal is excellently preserved, but the rest is not. One possible explanation may be that this is the result of uneven colonization of the carcass by microorganisms and algae, which created a protective layer especially around the neck
CHW 189 from the private collection of Herman Winkelhorst (Netherlands). The neck of the animal is excellently preserved, but the rest is not. One possible explanation may be that this is the result of uneven colonization of the carcass by microorganisms and algae, which created a protective layer especially around the neck. Credit: © Photo: Jelle Heijne/Uni Bonn

It has long been known that a quarry near the Dutch town of Winterswijk is an Eldorado for fossil lovers. But even connoisseurs will be surprised just how outstanding the site actually is. A student at the University of Bonn, himself a Dutchman and passionate fossil collector, has now analyzed pieces from museums and private collections for his master’s thesis. He found an amazing amount of almost completely preserved skeletons, all between 242 and 247 million years old. The good condition is presumably due to particularly favorable development conditions. These make Winterswijk, which belongs to the so-called Germanic Basin, a cornucopia for paleontology. The study is published in the Paläontologische Zeitschrift.

Jelle Heijne examined exactly 327 remains of marine reptiles for his master’s thesis — collected partly from public museums, but primarily from about 20 private collections. He was particularly impressed by the high quality of the finds: “Among them were more than 20 contiguous skeletons,” he emphasizes. “Only very few complete skeleton finds are known from the other sites of the Germanic Basin, which stretches from England to Poland.”

In his study, the 25-year-old investigated the question of why the bones, which are over 240 million years old, have been preserved so well here. The reason is probably a combination of fortunate circumstances: At that time the Germanic Basin was a sea, which was extremely shallow in today’s Winterswijk. This is illustrated by the fossil footprints of terrestrial animals that were found not far from the reptile bones. The region probably resembled today’s Wadden Sea of the North Sea coast, but with a bottom that was not sandy but covered in lime silt.

The shallow depth ensured that cadavers quickly hit the ground, where they were then covered by sediment. If dead animals float in the water for a long time and are tossed back and forth by waves and currents, the probability increases that body parts, such as tail, limbs or head, are lost.

Another important factor was a process called “Stick’n’Peel” by paleontologists: The animal is colonized by microorganisms and algae that hold the skeleton together like a skin. “It was probably these two factors in particular that favored the occurrence of well-preserved finds,” explains Heijne.

In fact, there is some evidence for the Stick’n’Peel hypothesis. For example, some skeletons lack individual larger bones, while the small bones are complete — even though the latter are usually most likely to be carried away by the water. “Such unusual patterns typically occur when a skeleton is unevenly colonized and thus protected,” Heijne explains.

It has long been known that Winterswijk stands out among the sites of the Germanic Basin. Nevertheless, the large number of high-quality finds is likely to surprise even connoisseurs, especially since most of the finds are not accessible to the public. “I have been a member of an association of private collectors in the Netherlands for years,” Heijne explains. This was the ideal contact exchange for his study: “The collectors I approached were all proud to be able to contribute to the research on Winterswijk.”

Reference:
Jelle Heijne, Nicole Klein, P. Martin Sander. The uniquely diverse taphonomy of the marine reptile skeletons (Sauropterygia) from the Lower Muschelkalk (Anisian) of Winterswijk, The Netherlands. PalZ, 2019; DOI: 10.1007/s12542-018-0438-0

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

Sampling Hot Molten Lava

Lava is molten rock generated by geothermal energy and expelled through fractures in planetary crust or in an eruption, usually at temperatures from 700 to 1,200 °C (1,292 to 2,192 °F). The structures resulting from subsequent solidification and cooling are also sometimes described as lava. The molten rock is formed in the interior of some planets, including Earth, and some of their satellites, though such material located below the crust is referred to by other terms.

A lava flow is a moving outpouring of lava created during a non-explosive effusive eruption. When it has stopped moving, lava solidifies to form igneous rock. The term lava flow is commonly shortened to lava. Although lava can be up to 100,000 times more viscous than water, lava can flow great distances before cooling and solidifying because of its thixotropic and shear thinning properties.

Lava sampling: Why do we do it?

Hot lava samples provide important information about what’s going on in a volcano’s magma chambers.

We know from laboratory experiments that the more magnesium there is in magma, the hotter it is. Chemical analysis, therefore, provides the means not only to determine the crystallization history of lava but also to establish the temperature at which it was erupted.

For example, Kilauea’s 1997 lavas are chemically different from lavas erupted from 1985 to 1997. Chemical analyses show that magma was supplied by two distinct magma bodies.

Video Copyright © USGS

Bismuth Crystal “Artificially grown bismuth crystal”

Bismuth is a chemical element with symbol Bi and atomic number 83. It is a pentavalent post-transition metal and one of the pnictogens with chemical properties resembling its lighter homologs arsenic and antimony. Elemental bismuth may occur naturally, although its sulfide and oxide form important commercial ores. The free element is 86% as dense as lead. It is a brittle metal with a silvery white color when freshly produced, but surface oxidation can give it a pink tinge. Bismuth is marginally radioactive, and the most naturally diamagnetic element, and has one of the lowest values of thermal conductivity among metals.

Bismuth was long considered the element with the highest atomic mass that is stable, but in 2003 it was discovered to be extremely weakly radioactive: its only primordial isotope, bismuth-209, decays via alpha decay with a half-life more than a billion times the estimated age of the universe. Because of its tremendously long half-life, bismuth may still be considered stable for almost all purposes.

Bismuth metal has been known since ancient times, although it was often confused with lead and tin, which share some physical properties. The etymology is uncertain, but possibly comes from Arabic bi ismid, meaning having the properties of antimony or the German words weiße Masse or Wismuth (“white mass”), translated in the mid-sixteenth century to New Latin bisemutum.

Bismuth compounds account for about half the production of bismuth. They are used in cosmetics, pigments, and a few pharmaceuticals, notably bismuth subsalicylate, used to treat diarrhea. Bismuth’s unusual propensity to expand upon freezing is responsible for some of its uses, such as in casting of printing type. Bismuth has unusually low toxicity for a heavy metal. As the toxicity of lead has become more apparent in recent years, there is an increasing use of bismuth alloys (presently about a third of bismuth production) as a replacement for lead.

How to predict when a volcano will erupt

Findings about the effect of a volcano's age on its likelihood to erupt will be applied to the Merapi volcano in Indonesia, among others.
Findings about the effect of a volcano’s age on its likelihood to erupt will be applied to the Merapi volcano in Indonesia, among others. Credit: Jimmy McIntyre, licensed under CC BY-SA 2.0

The eruption of a volcano can have devastating consequences – killing people and destroying livelihoods, as well as releasing vast amounts of ash into the sky that disrupts air travel and alters the climate. Knowing what goes on underground, however, would facilitate better warnings for when an eruption will occur – and help save lives while keeping damage to a minimum.

“Understanding volcanoes is an international effort. The impact of eruptions does not stop at borders,” said volcanologist Dr. Catherine Annen of the University Savoie Mont Blanc in France.

Though relatively small, the eruption of the Eyjafjallajökull volcano in southern Iceland in 2010 sticks in many people’s memories. Its drifting plume of ash led to the widespread cancellation of flights across Europe.

Today, other, bigger volcanoes seem to be on the brink of eruption. Seismic observations suggest that Italy’s Campi Flegrei, a supervolcano close to millions of people living in and around Naples, is amassing magma in a dangerous ‘hot zone’.

But such observations only give rough forecasts – usually days, weeks or months in advance – of when a volcano will erupt. “The uncertainty arises from the fact that we cannot see what is happening underground,” said Dr. Annen.

Scientists such as Dr. Annen already have a fair idea of what goes on. Being less dense than surrounding rock, magma from deep within the Earth can rise up, potentially finding an outlet at thinner points – volcanoes – in the planet’s crust.

Foaming and freezing

Magma cools as it rises, and if we are lucky it will freeze, or solidify, before ever erupting. On the other hand, the pressure close to the surface drops too, and this liberates dissolved gases, which increase the chances of a foaming explosion – a bit like opening a shaken fizzy drink bottle.

Dr. Stephan Kolzenburg, a volcanologist at McGill University in Montreal, Canada, said: “These two processes – foaming and freezing – compete, and depending on which one wins, the volcano will or will not erupt.”

The foaming and solidification processes also lie at the heart of mathematical volcano models. Through a research project called DYNAVOLC, Dr. Kolzenburg hopes that by better understanding the competition between the two processes, and by linking them to geophysical signals recorded on the Earth’s surface, he will be able to improve the hazard maps depicting the areas most likely to be affected by volcanic eruptions.

Although his research project only began in April, it has already yielded results. In one study, Dr. Kolzenburg found that the faster magma and lava flows, the faster it solidifies – knowledge that could improve the volcano models.

Not all volcanoes behave in the same way, however. Having had longer to store magma, old volcanoes tend to be hotter than young volcanoes, and this determines, for instance, the level of ground swelling close to eruption.

Volcano’s age

Dr. Annen is interested in how a volcano’s age affects this and other potential warning signals. Through a project called MAGMATS, she is simulating on computers the interaction of magma and gases to understand how key volcano parameters change over thousands to hundreds of thousands of years.

Such parameters include temperature, gas content and magma content – none of which vary in a simple, linear fashion with one another. “Simulating the processes is challenging,” she said.

Nevertheless, the work should help the prediction of an eruption to be better tailored to a volcano’s age – and thus more accurate. Dr. Annen hopes to apply her findings to four active volcanoes: Campi Flegrei in Italy, Uturunku in Bolivia, Merapi in Indonesia and Krafla in Iceland.

“I would like to know if there are large volumes of magma ready to erupt close to the surface – or if, on the contrary, any eruption must first involve new magma transfer from deeper levels,” she said. Ultimately, she hopes that ‘any decision about evacuation will be better informed.”

Note: The above post is reprinted from materials provided by Horizon: The EU Research & Innovation Magazine.

Reconstruction of trilobite ancestral range in the southern hemisphere

Representative Image: A light photograph of a pyritized, egg-bearing specimen of Triarthrus eatoni.  Credit: Image courtesy of Western Illinois University

The first appearance of trilobites in the fossil record dates to 521 million years ago in the oceans of the Cambrian Period, when the continents were still inhospitable to most life forms. Few groups of animals adapted as successfully as trilobites, which were arthropods that lived on the seabed for 270 million years until the mass extinction at the end of the Permian approximately 252 million years ago.

The longer ago organisms lived, the more rare are their fossils and the harder it is to understand their way of life; paleontologists face a daunting task in endeavoring to establish evolutionary relationships in time and space.

Surmounting the difficulties inherent in the investigation of a group of animals that lived such a long time ago, Brazilian scientists affiliated with the Biology Department of São Paulo State University’s Bauru School of Sciences (FC-UNESP) and the Paleontology Laboratory of the University of São Paulo’s Ribeirão Preto School of Philosophy, Science and Letters (FFCLRP-USP) have succeeded for the first time in inferring paleobiogeographic patterns among trilobites.

Paleobiogeography is a branch of paleontology that focuses on the distribution of extinct plants and animals and their relations with ancient geographic features. The study was conducted by Fábio Augusto Carbonaro, a postdoctoral researcher at UNESP’s Bauru Macroinvertebrate Paleontology Laboratory (LAPALMA) headed by Professor Renato Pirani Ghilardi. Other participants included Max Cardoso Langer, a professor at FFCLRP-USP, and Silvio Shigueo Nihei, a professor at the same university’s Bioscience Institute (IB-USP).

The researchers analyzed the morphological differences and similarities of the 11 species of trilobites described so far in the genus Metacryphaeus; these trilobites lived during the Devonian between 416 million and 359 million years ago (mya) in the cold waters of the sea that covered what is now Bolivia, Peru, Brazil, the Malvinas (Falklands) and South Africa.

The Devonian Period is subdivided into seven stages. Metacryphaeus lived during the Lochkovian (419.2-410.8 mya) and Pragian (410.8- 407.6 mya) stages, which are the earliest Devonian stages.

The results of the research were published in Scientific Reports and are part of the project “Paleobiogeography and migratory routes of paleoinvertebrates of the Devonian in Brazil,” which is supported by São Paulo Research Foundation -FAPESP and Brazil’s National Council for Scientific and Technological Development (CNPq). Ghilardi is the project’s principal investigator.

“When they became extinct in the Permian, 252 million years ago, the trilobites left no descendants. Their closest living relatives are shrimps, and, more remotely, spiders, scorpions, sea spiders and mites,” Ghilardi said.

Trilobite fossils are found abundantly all over the world, he explained — so abundantly that they are sometimes referred to as the cockroaches of the sea. The comparison is not unwarranted because anatomically, the trilobites resemble cockroaches. The difference is that they were not insects and had three longitudinal body segments or lobes (hence the name).

In the northern hemisphere, the trilobite fossil record is very rich. Paleontologists have so far described ten orders comprising over 17,000 species. The smallest were 1.5 millimeters long, while the largest were approximately 70 cm long and 40 cm wide. Perfectly preserved trilobites can be found in some regions, such as Morocco. These can be beautiful when used to create cameos or intaglio jewelry. Trilobite fossils from Brazil, Peru and Bolivia, in contrast, are often poorly preserved, consisting merely of the impressions left in benthic mud by their exoskeletons.

“Although their state of preservation is far from ideal, there are thousands of trilobite fossils in the sediments that form the Paraná basin in the South region of Brazil, and the Parnaíba basin along the North-Northeast divide,” said Ghilardi, who also chairs the Brazilian Paleontology Society.

According to Ghilardi, their poor state of preservation could be due to the geological conditions and climate prevailing in these regions during the Paleozoic Era, when the portions of dry land that would one day form South America were at the South Pole and entirely covered by ice for prolonged periods.

During the Devonian, South America and Africa were connected as part of the supercontinent Gondwana. South Africa was joined with Uruguay and Argentina in the River Plate region, and Brazil’s southern states were continuous with Namibia and Angola.

Parsimonious analysis

The research began with an analysis of 48 characteristics (size, shape and structure of organs and anatomical parts) found in some 50 fossil specimens of the 11 species of Metacryphaeus.

“In principle, these characteristics serve to establish their phylogeny — the evolutionary history of all species in the universe, analyzed in terms of lines of descent and relationships among broader groups,” Ghilardi said.

Known as a parsimonious analysis, this method is widely used to establish relationships among organisms in a given ecosystem, and in recent years, it has also begun to be used in the study of fossils.

According to Ghilardi, parsimony, in general, is the principle that the simplest explanation of the data is the preferred explanation. In the analysis of phylogeny, it means that the hypothesis regarding relationships that requires the smallest number of characteristic changes between the species analyzed (in this case, trilobites of the genus Metacryphaeus) is the one that is most likely to be correct.

The biogeographic contribution to the study was made by Professor Nihei, who works at IB-USP as a taxonomist and insect systematist. The field of systematics is concerned with evolutionary changes between ancestries, while taxonomy focuses on classifying and naming organisms.

“Biogeographic analysis typically involves living groups the ages of which are estimated by molecular phylogeny, or the so-called molecular clock, which estimates when two species probably diverged on the basis of the number of molecular differences in their DNA. In this study of trilobites, we used age in a similar manner, but it was obtained from the fossil record,” Nihei said.

“The main point of the study was to use fossils in a method that normally involves molecular biogeography. Very few studies of this type have previously involved fossils. I believe our study paves the way for a new approach based on biogeographic methods requiring a chronogram [a molecularly dated cladogram] because this chronogram can also be obtained from fossil taxa such as those studied by paleontologists, rather than molecular cladograms for living animals.”

As a vertebrate paleontologist who specializes in dinosaurs, Langer acknowledged that he knows little about trilobites but a great deal about the modern computational techniques used in parsimonious analysis, on which his participation in the study was based. “I believe the key aspect of this study, and the reason it was accepted for publication in as important a journal as Scientific Reports, is that it’s the first ever use of parsimony to understand the phylogeny of a trilobite genus in the southern hemisphere,” he said.

Gondwanan dispersal

The results of the paleobiogeographical analyses reinforce the pre-existing theory that Bolivia and Peru formed the ancestral home of Metacryphaeus.

“The models estimate a 100% probability that Bolivia and Peru formed the ancestral area of the Metacryphaeus clade and most of its internal clades,” Ghilardi said. Confirmation of the theory shows that parsimonious models have the power to suggest the presence of clades at a specific moment in the past even when there are no known physical records of that presence.

In the case of Metacryphaeus, the oldest records in Bolivia and Peru date from the early Pragian stage (410.8-407.6 mya), but the genus is believed to have evolved in the region during the Lochkovian stage (419.2-410.8 mya).

Parsimony, therefore, suggests Metacryphaeus originated in Bolivia and Peru some time before 410.8 mya but not earlier than 419.2 mya. In any event, it is believed to be far older than any known fossils.

According to Ghilardi, the results can be interpreted as showing that the adaptive radiation of Metacryphaeus to other areas of western Gondwana occurred during episodes of marine transgression in the Lochkovian-Pragian, when the sea flooded parts of Gondwana.

“The dispersal of Metacryphaeus trilobites during the Lochkovian occurred from Bolivia and Peru to Brazil — to the Paraná basin, now in the South region, and the Parnaíba basin, on the North-Northeast divide — and on toward the Malvinas/Falklands, while the Pragian dispersal occurred toward South Africa,” he said.

Fossil trilobites have been found continuously in the Paraná basin in recent decades. Trilobites collected in the late nineteenth century in the Parnaíba basin were held by Brazil’s National Museum in Rio de Janeiro, which was destroyed by fire in September 2018.

“These fossils haven’t yet been found under the rubble and it’s likely that nothing is left of them. They were mere shell impressions left in the ancient seabed. Even in petrified form, they must have dissolved in the blaze,” Ghilardi said.

Reference:
Fábio Augusto Carbonaro, Max Cardoso Langer, Silvio Shigueo Nihei, Gabriel de Souza Ferreira, Renato Pirani Ghilardi. Inferring ancestral range reconstruction based on trilobite records: a study-case on Metacryphaeus (Phacopida, Calmoniidae). Scientific Reports, 2018; 8 (1) DOI: 10.1038/s41598-018-33517-5

Note: The above post is reprinted from materials provided by Fundação de Amparo à Pesquisa do Estado de São Paulo. Original written by Peter Moon.

Thin layers of sediment point to early arrival of life on land

Part of a quilted Ediacaran fossil is partly covered by ancient wind-drift from Namibia. Image courtesy of Greg Retallack.
Part of a quilted Ediacaran fossil is partly covered by ancient wind-drift from Namibia. Image courtesy of Greg Retallack.

New clues emerging from fossils found in the oldest soils on Earth suggest that multicellular, land-dwelling organisms possibly emerged much earlier than thought.

The evidence for such a conclusion emerged from fossil assemblages, previously considered to be ocean organisms, found in thin layers of silt and sand located between thicker sandstone beds in South Australia. The sediments date to between 542 million to 635 million years ago – during a geological period known as the Ediacaran.

“These Ediacaran organisms are one of the enduring mysteries of the fossil record,” said Greg Retallack, fossil collections director at the University of Oregon’s Museum of Natural and Cultural History. “Were they worms, sea jellies, sea pens, amoebae, algae? They are notoriously difficult to classify, but conventional wisdom has long held that they were marine organisms.”

Retallack’s new study, published online in November and in the January issue of the journal Sedimentary Geology, suggests otherwise based on a geochemical and microscopic re-examination of both the age and environmental associations in the thin, silty-to-sandy layers.

The sediments, known as interflag sandstone laminae, reveal telltale marks of ancient wind erosion—phenomena more closely associated with modern river banks than with oceans or seas. These thin, alternating layers, which are light in color and rich in fine grain sizes, appear similar to sheets of white paper between books bound in brown and red, Retallack noted.

“Such wind-drifted layers are widespread on river levees and sandbars today. They are present throughout the Flinders Ranges of South Australia and also in Ediacaran rocks of southern Namibia,” he said.

The emergence of multicellular life on land dates to about 565 million years ago, although there is debate on whether Ediacaran fossils of that age originated from organisms in the sea or on land, Retallack said.

If the sediments themselves were deposited on dry land, it would follow that the organisms fossilized there were land dwellers, said Retallack, who also is a professor in the UO’s Department of Earth Sciences. The organisms that left the fossils, he said, would have been from multicellular organisms visible with the naked eye. Such life would have preceded the emergence of green plant vegetation, which is believed to have started between 470 million and 583 million years ago.

Last November, Retallack and Nora Noffke of Old Dominion University had reported on traces of life left in 3.7 billion-year-old soils in a metamorphic rock formation in southwestern Greenland. In the journal Palaeogeography, Palaeoclimatology, Palaeoecology, they identified isotopic ratios of carbon potentially indicative of early land-dwelling microbes.

While the Ediacaran organisms remain enigmatic when it comes to biological classification, Retallack’s new study offers some important clues.

“The investigation points to a terrestrial habitat for some of these organisms, and combined with growing evidence from studies of fossil soils and biological soil crust features, it suggests that they may have been land creatures such as lichens,” Retallack said.

For the paper, Retallack also re-examined well-known interflag sandstone laminae at four southern Indiana locations, which date to the Pennsylvanian period, and a central Colorado site from the Eocene epoch. These locations and examination of modern rivers showed the same sedimentary processes seen in Ediacaran rocks of South Australia and Africa.

Reference:
Gregory J. Retallack. Interflag sandstone laminae, a novel sedimentary structure, with implications for Ediacaran paleoenvironments, Sedimentary Geology (2018). DOI: 10.1016/j.sedgeo.2018.11.003

Gregory J. Retallack et al. Multiple Early Triassic greenhouse crises impeded recovery from Late Permian mass extinction, Palaeogeography, Palaeoclimatology, Palaeoecology (2010). DOI: 10.1016/j.palaeo.2010.09.022

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

Medical scanner helps to unlock the mysteries of a giant prehistoric marine reptile

Life reconstruction of ichthyosaur skull. Credit: Bob Nicholls (Thinktank, Birmingham Science Museum)
Life reconstruction of ichthyosaur skull. Credit: Bob Nicholls (Thinktank, Birmingham Science Museum)

A nearly metre-long skull of a giant fossil marine ichthyosaur found in a farmer’s field more than 60 years ago has been studied for the first time.

Using cutting-edge computerised tomography (CT) scanning technology, the research reveals new information including details of the rarely preserved braincase.

The almost 200 million year old fossil, which was found in 1955 at Fell Mill Farm in Warwickshire, had never formally been studied prior to this research.

Now, thanks to data collected from CT scans, the research team were able to digitally reconstruct the entire skull in 3D. It is the first time a digital reconstruction of a skull and mandible of a large marine reptile has ever been made available for research purposes and to the public.

Although thousands of ichthyosaur fossils have been unearthed in the UK, this specimen is particularly important and unusual because it is three-dimensionally preserved and contains bones of the skull that are rarely exposed.

In 2014, as part of a project at Thinktank Science Museum, Birmingham, palaeontologists Dean Lomax, from The University of Manchester, and Nigel Larkin began to study the skull and its incomplete skeleton for the first time and were soon convinced of its importance.

Dean, the lead author and one of the world’s leading ichthyosaur experts, explains: “The first time I saw this specimen I was puzzled by its excellent preservation.

Ichthyosaurs of this age (Early Jurassic) are usually ‘pancaked’, meaning that they are squished so that the original structure of the skull is either not preserved or is distorted or damaged. So to have a skull and portions of the skeleton of an ichthyosaur of this age preserved in three dimensions, and without any surrounding rock obscuring it, is something quite special.”

The ichthyosaur was originally identified as a common species called Ichthyosaurus communis, but after studying it closer, Dean was convinced it was a rarer species. Based on various features of the skull, he identified it as an example of an ichthyosaur called Protoichthyosaurus prostaxalis. With a skull almost twice as long as any other specimen of Protoichthyosaurus, this is the largest specimen so far known of the species.

Co-author Nigel Larkin added: “Initially, the aim of the project was to clean and conserve the skull and partially dismantle it to rebuild it more accurately, ready for redisplay at the Thinktank Museum. But we soon realised that the individual bones of the skull were exceptionally well preserved in three dimensions, better than in any other ichthyosaur skull we’d seen. Furthermore, that they would respond well to CT scanning, enabling us to capture their shape digitally and to see their internal details. This presented an opportunity that couldn’t be missed”

The skull isn’t quite complete, but several bones of the braincase — which are rarely preserved in ichthyosaurs — are present. To unlock information contained in the skull, these bones were micro-CT scanned at Cambridge University in 2015 by expert palaeontologist and co-author, Dr Laura Porro of University College London (UCL).

The fossil only preserved bones from the left side of the braincase; however, using CT scans these elements were digitally mirrored and 3D printed at life size to complete the braincase. Finally, the entire skull was CT scanned at the Royal Veterinary College (RVC) using a scanner typically reserved for horses and other large animals.

Dr Porro added: “CT scanning allows us to look inside fossils — in this case, we could see long canals within the skull bones that originally contained blood vessels and nerves. Scans also revealed the curation history of the specimen since its discovery in the ’50s. There were several areas reconstructed in plaster and clay, and one bone was so expertly modelled that only the scans revealed part of it was a fake. Finally there is the potential to digitally reconstruct the skull in 3D. This is hard (and risky) to do with the original, fragile and very heavy fossil bones; plus, we can now make the 3D reconstruction freely available to other scientists and for education.”

The use of modern technologies, such as medical scanners, have revolutionised the way in which palaeontologists are able to study and describe fossils.

Dean added: “It’s taken more than half a century for this ichthyosaur to be studied and described, but it has been worth the wait. Not only has our study revealed exciting information about the internal anatomy of the skull of this animal, but our findings will aid other palaeontologists in exploring its evolutionary relationship with other ichthyosaurs.”

Reference:
Dean R. Lomax, Laura B. Porro, Nigel R. Larkin. Descriptive anatomy of the largest known specimen of Protoichthyosaurus prostaxalis (Reptilia: Ichthyosauria) including computed tomography and digital reconstruction of a three-dimensional skull. PeerJ, 2019; 7: e6112 DOI: 10.7717/peerj.6112

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

Deep low-frequency earthquakes indicate migration of magmatic fluids beneath Laacher See Volcano

Map of the locations and depths of the deep low-frequency (DLF) earthquakes beneath the Laacher See Volcano ("Lake Laach Volcano") in Germany. Brittle earthquakes are marked as circles, DLF events as stars. Credit: Hensch et al.
Map of the locations and depths of the deep low-frequency (DLF) earthquakes beneath the Laacher See Volcano (“Lake Laach Volcano”) in Germany. Brittle earthquakes are marked as circles, DLF events as stars. Credit: Hensch et al.

Magma could rise from the upper mantle into the middle and upper crust beneath the Laacher See Volcano (Rhineland-Palatinate). This is the result of a study conducted by the Seismological Survey of Southwest Germany (Erdbebendienst Südwest), together with GFZ German Research Centre for Geosciences, Karlsruhe Institute of Technology (KIT) and the Seismological Survey of North Rhine-Westphalia. For the first time, the scientists present evidence of deep and low-frequency earthquakes caused by magma movements under the Laacher See Volcano. However, there are presently no signs of any upcoming volcanic activity in the near future. The researchers report their findings in Geophysical Journal International.

“The detected earthquakes are generated at large depths and are characterized by unusually low frequencies. Their magnitudes are below the limit of human perception,” explains Professor Joachim Ritter of the Geophysical Institute (GPI) at KIT. The scientists speak of “deep low-frequency” (DLF) earthquakes. They are generated at depths between ten and over forty kilometres, i.e. in the Earth’s crust and upper mantle. Their dominant oscillation frequencies are between one and ten Hertz, which is significantly lower than tectonic earthquakes of comparable magnitude.

“DLF earthquakes are regarded worldwide as an indication of the movement of magmatic fluids at great depths,” explains Professor Torsten Dahm, head of the GFZ section Physics of Earthquakes and Volcanoes. “Such earthquakes can be observed regularly beneath active volcanoes, for example in Iceland, Japan or Kamchatka.” The results of the study in the East Eifel region suggest that magmatic fluids from the upper mantle of the Earth could rise into the Earth’s crust under the Laacher See Volcano. This can be interpreted as an indication for the existence and ongoing slow recharge of magma chambers in the crust beneath the volcano.

In their study, the scientists of KIT, GFZ, Erdbebendienst Südwest — the joint seismological services of Rhineland-Palatinate and Baden-Württemberg — and the State Seismological Service of North Rhine-Westphalia determined that these earthquakes occur episodically in groups that are narrowly limited in time and space and line up along a line between 10 and 45 kilometres depth The scientists conclude that fluids and magmas, i.e. molten rock, could rise from the upper mantle into the middle and upper crust of the earth beneath the Laacher See Volcano.

“Due to extensive improvements of the seismological monitoring networks in Rhineland-Palatinate and the adjacent regions, deep low-frequency earthquakes could be registered beneath the Laacher See Volcano for the first time in 2013,” says Dr. Martin Hensch, head of the study at the Erdbebendienst Südwest. “In the past five years, a total of four spatially well constrained clusters of such DLF earthquakes have been detected in the East Eifel region.” The clusters align along an approximately 80° southeast dipping line south of the Laacher See Volcano. In addition to the spatial separation, the temporal occurrence of the DLF earthquakes is also sharply limited: So far, the experts have observed eight episodes of DLF earthquakes lasting between 40 seconds and eight minutes.

However, the researchers do not interpret the observed DLF earthquakes as an immediate precursor signal of any upcoming volcanic activity in the near future. “The rise of magma into the shallow crust is usually accompanied by swarms of high-frequency earthquakes. Such activity has not yet been observed in the Eastern Eifel,” reports Joachim Ritter. “Further, there is no sign of deformation at the Earth’s surface, which should be clearly detectable during massive magma ascents,” adds Torsten Dahm. Dating of the magma produced during the last eruption 12,900 years ago show that the filling and differentiation of the upper magma chamber under Laacher See Volcano could have taken about 30,000 years before the actual eruption took place. This means that the magmatic processes take an extremely long time before an eruption occurs. As the technical requirements for the detection and localization of DLF earthquakes in the East Eifel region have only reached a sufficient quality in the last few years, it is not possible to determine retrospectively since when DLF earthquakes have occurred in the region. It can be assumed that this was already the case before 2013. Following the first observation of deep earthquakes in 2013, KIT, GFZ and Erdbebendienst Südwest installed a seismological research network. The joint use of seismic registrations now allows detailed scientific analysis of microseismicity.

In order to better investigate the interrelation of DLF earthquakes and possible magmatic activity beneath the East Eifel region, the researchers recommend to intensify geochemical monitoring to analyse emitted gases, as well as repeated geodetic measurements to detect possible deformations of the earth’s surface. Specific geophysical investigations should also be conducted to map and characterize possible magma reservoirs under the Laacher See Volcano. Further, the scientists advise a reassessment of the volcanic hazard of the Eifel.

Reference:
Martin Hensch, Torsten Dahm, Joachim Ritter, Sebastian Heimann, Bernd Schmidt, Stefan Stange, Klaus Lehmann. Deep low-frequency earthquakes reveal ongoing magmatic recharge beneath Laacher See Volcano (Eifel, Germany). Geophysical Journal International, 2019; DOI: 10.1093/gji/ggy532

Note: The above post is reprinted from materials provided by GFZ GeoForschungsZentrum Potsdam, Helmholtz Centre.

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