back to top
27.8 C
New York
Saturday, April 19, 2025
Home Blog Page 7

Could geometry offer a new explanation for why earthquakes happen?

San Andreas fault
San Andreas fault

Findings published in Nature by a team of Brown-led researchers challenge traditional beliefs about the cause of earthquakes and suggest that it depends not on friction, but on the ways faults are aligned.

By taking a close look at the geometrical makeup of rocks where earthquakes originate, researchers at Brown University are adding a new wrinkle to a long-held belief about what causes seismic quakes in the first place.

The work, described in the journal Nature, reveals that the way fault networks are aligned plays a critical role in determining where an earthquake will happen and its strength. The findings challenge the more traditional notion that it is primarily the type of friction happening at these faults that governs whether earthquakes happen or not, and they could improve current understandings of how earthquakes work.

“Our paper paints this very different sort of picture about why earthquakes happen,” said Brown geophysicist Victor Tsai, one of the paper’s lead authors. “And this has very important implications for where to expect earthquakes versus where to not expect earthquakes, as well as for predicting where the most damaging earthquakes will be.”

Fault lines are the visible boundaries on the planet’s surface where the rigid plates that make up the Earth’s lithosphere brush against each another. Tsai says that for decades, geophysicists have explained earthquakes as happening when stress at faults builds up to the point where the faults rapidly slip or break past each other, releasing pent-up pressure in an action known as stick-slip behavior.

Researchers theorized that the rapid slip and intense ground motions that follow are a result of unstable friction that can happen at the faults. In contrast, the thought is that when friction is stable, the plates then slide against each other slowly without an earthquake. This steady and smooth movement is also known as creep.

“People have been trying to measure these frictional properties, like whether the fault zone has unstable friction or stable friction and then, based on laboratory measurements of that, they try to predict if are you going to have an earthquake there or not,” Tsai said. “Our findings suggest that it might be more relevant to look at the geometry of the faults in these fault networks, because it may be the complex geometry of the structures around those boundaries that creates this unstable versus stable behavior.”

The geometry to consider includes complexities in the underlying rock structures such as bends, gaps and stepovers. The study is based on mathematical modeling and studying fault zones in California using data from the U.S. Geological Survey’s Quaternary Fault Database and from the California Geological Survey.

The research team, which also includes Brown graduate student Jaeseok Lee and Brown geophysicist Greg Hirth, offer a more detailed example to illustrate how earthquakes happen. They say to picture the faults that brush up against each other as having serrated teeth like the edge of a saw. When there are fewer teeth or teeth that are not as sharp, the rocks slide past each other more smoothly, allowing for creep. But when the rock structures in these faults are more complex and jagged, these structures catch on to one another and get stuck. When that happens, they build up pressure and eventually as they pull and push harder and harder, they break, jerking away from each other and leading to earthquakes.

The new study builds on previous work looking at why some earthquakes generate more ground motion compared to other earthquakes in different parts of the world, sometimes even those of similar magnitude. The study showed that blocks colliding inside a fault zone as an earthquake happens contributes significantly to the generation of high-frequency vibrations and sparked the notion that maybe geometrical complexity beneath the surface was also playing a role in where and why earthquakes happen.

Analyzing data from faults in California — which include the well-known San Andreas fault — the researchers found that fault zones that have complex geometry underneath, meaning the structures there weren’t as aligned, turned out to have stronger ground motions than less geometrically complex fault zones. This also means some of these zones would have stronger earthquakes, others would have weaker ones, and some would have no earthquakes.

The researchers determined this based on the average misalignment of the faults they analyzed. This misalignment ratio measures how closely the faults in a certain region are aligned and all going in the same direction versus going in many different directions. The analysis revealed that fault zones where the faults are more misaligned causes stick-slip episodes in the form of earthquakes. Fault zones where the geometry of the faults were more aligned facilitated smooth fault creep with no earthquakes.

“Understanding how faults behave as a system is essential to grasp why and how earthquakes happen,” said Lee, the graduate student who led the work. “Our research indicates that the complexity of fault network geometry is the key factor and establishes meaningful connections between sets of independent observations and integrates them into a novel framework.”

The researchers say more work needs to be done to fully validate the model, but this initial work suggests the idea is promising, especially because the alignment or misalignment of faults is easier to measure than fault frictional properties. If valid, the work can one day be weaved into earthquake prediction models.

That remains far off for now as the researchers begin to outline how to build upon the study.

“The most obvious thing that comes next is trying to go beyond California and see how this model holds up,” Tsai said. “This is potentially a new way of understanding how earthquakes happen.”

Reference:

Jaeseok Lee, Victor C. Tsai, Greg Hirth, Avigyan Chatterjee, Daniel T. Trugman. Fault-network geometry influences earthquake frictional behaviour. Nature, 2024; DOI: 10.1038/s41586-024-07518-6

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

Yowah Nut Opal

Yowah Nut Opal
Yowah Nut Opal

Introduction

Yowah Nut Opal is a unique and captivating gemstone known for its distinctive appearance and vibrant play of colors. Found exclusively in the Yowah opal field in Queensland, Australia, this gemstone is highly prized by collectors and jewelers alike. The name “Yowah Nut” derives from the opal’s resemblance to nuts or nodules, encapsulating the precious opal within a hardened outer shell. This article delves into the geological formation, history, and significance of Yowah Nut Opal, exploring its unique characteristics and the region from which it originates.

Geological Formation

The Origins of Opal

Opal is a mineraloid composed of silica and water, formed through a process of sedimentation. It typically occurs in areas with rich deposits of sandstone and volcanic ash, where water percolates through the earth, dissolving silica from the rocks. This silica-laden water then seeps into voids and cracks in the earth’s crust. Over time, the water evaporates, leaving behind silica deposits that gradually solidify to form opal. The unique play of colors in opal, known as opalescence, is due to the diffraction of light passing through these silica spheres.

Formation of Yowah Nut Opal

Yowah Nut Opal specifically forms within ironstone concretions, or nodules, often referred to as “nuts.” These nodules are typically spherical or ellipsoidal, ranging in size from a few millimeters to several centimeters in diameter. The formation process of Yowah Nut Opal involves several stages:

  1. Sedimentary Deposition: The region where Yowah Nut Opal is found was once a vast inland sea. Over millions of years, sedimentary layers, including sandstone and claystone, accumulated on the seabed.
  2. Silica Infusion: As water infiltrated these sedimentary layers, it dissolved silica from the surrounding rocks. This silica-rich water then filled cavities within the ironstone nodules.
  3. Opalization: Over time, the water evaporated, leaving behind deposits of silica. In favorable conditions, these silica deposits transformed into opal. The opal within Yowah Nuts often exhibits striking colors and patterns, encapsulated by the harder ironstone exterior.
  4. Fossilization and Erosion: Geological processes such as fossilization and erosion exposed these opal-filled nodules near the earth’s surface, making them accessible for mining.

The Yowah Opal Field

Location and Geology

The Yowah Nut Opal field is located in southwestern Queensland, Australia, approximately 130 kilometers west of Cunnamulla. This region is part of the larger Eromanga Basin, known for its rich deposits of opal. The Yowah field is characterized by its arid climate, sparse vegetation, and rugged terrain, typical of the Australian outback.

The geology of the Yowah Nut Opal field is dominated by sedimentary rock formations, primarily sandstone and claystone, dating back to the Cretaceous period. The presence of ironstone concretions, within which Yowah Nut Opal is found, is a distinctive feature of this area. These ironstone nodules are embedded within the sedimentary layers, and their opal content is revealed through mining and exploration.

Mining and Extraction

Mining in the Yowah Nut Opal field is a challenging and labor-intensive process, often carried out by small-scale miners and prospectors. The extraction of Yowah Nut Opal involves several steps:

  1. Prospecting: Miners use various techniques to locate opal-bearing nodules, including ground-penetrating radar, drilling, and surface exploration. The presence of ironstone nodules is a key indicator of potential opal deposits.
  2. Excavation: Once a promising area is identified, miners use excavators, jackhammers, and other tools to break through the overlying sedimentary layers. The ironstone nodules are carefully extracted to avoid damaging the opal inside.
  3. Processing: The extracted nodules are then split open, either manually or using mechanical saws, to reveal the opal within. This process requires skill and precision to ensure that the opal is not damaged during extraction.
  4. Sorting and Grading: The opal is sorted and graded based on its color, pattern, and overall quality. High-quality Yowah Nut Opal is characterized by its vibrant colors and intricate patterns, making it highly sought after in the gemstone market.

Unique Characteristics of Yowah Nut Opal

Color and Patterns

One of the most captivating features of Yowah Nut Opal is its vibrant play of colors. This phenomenon, known as opalescence, occurs when light interacts with the microscopic silica spheres within the opal. The diffraction of light results in a stunning display of colors, ranging from blues and greens to reds and oranges. The intensity and variety of colors in Yowah Nut Opal are often considered superior to other types of opal.

The patterns within Yowah Nut Opal are equally unique. The opal can form intricate and mesmerizing patterns, including:

  1. Pinfire Pattern: Characterized by small, pinpoint flashes of color.
  2. Harlequin Pattern: Featuring larger, angular patches of color.
  3. Floral Pattern: Resembling the shapes of flowers or petals.
  4. Mosaic Pattern: A complex arrangement of color patches, resembling a mosaic.

These patterns, combined with the vibrant colors, make each piece of Yowah Nut Opal a unique and highly desirable gemstone.

Ironstone Matrix

Unlike other types of opal, Yowah Nut Opal is often found encased within an ironstone matrix. This ironstone shell provides a striking contrast to the colorful opal inside, enhancing its visual appeal. The ironstone matrix also adds to the durability and stability of the opal, making it suitable for various types of jewelry and decorative items.

Cabochons and Freeform Pieces

Yowah Nut Opal is commonly cut and polished into cabochons, showcasing its vibrant colors and patterns. Cabochons are smooth, domed gemstones that highlight the opal’s natural beauty. Additionally, some Yowah Nut Opal pieces are left in their natural, freeform shapes, preserving the unique contours and features of the original nodule.

Historical and Cultural Significance

Indigenous Australian Connection

Opal has been cherished by Indigenous Australians for thousands of years. The gemstone holds cultural and spiritual significance, often associated with the Dreamtime, a central concept in Indigenous Australian mythology. According to Dreamtime stories, opal is the result of a rainbow touching the earth, imbuing the stone with its vibrant colors.

Yowah Nut Opal, with its distinctive appearance, has a special place in Indigenous Australian culture. The gemstone is sometimes used in traditional ceremonies and as a symbol of connection to the land and ancestral heritage.

Discovery and Early Mining

The Yowah opal field was discovered in the late 19th century, during a period of opal rushes in Australia. Prospectors and miners flocked to the region in search of opal, leading to the establishment of small mining communities. The discovery of Yowah Nut Opal brought attention to the unique and valuable gemstone, sparking interest from collectors and jewelers worldwide.

Early mining efforts were often rudimentary, relying on manual labor and basic tools. Despite the challenges, miners persevered, uncovering some of the most exquisite Yowah Nut Opal specimens ever found.

The Modern Yowah Opal Industry

Advances in Mining Technology

In recent years, advances in mining technology have improved the efficiency and safety of opal extraction in the Yowah field. Modern equipment, such as hydraulic excavators, drills, and saws, allows miners to access deeper and more remote opal deposits. Additionally, improved processing techniques enable the careful extraction and preservation of opal, minimizing damage and maximizing yield.

Environmental and Ethical Considerations

As the demand for opal continues to grow, there is an increasing focus on sustainable and ethical mining practices. Efforts are being made to minimize the environmental impact of opal mining, including land rehabilitation and water management. Ethical considerations also extend to the fair treatment of miners and the support of local communities.

Global Market and Demand

Yowah Nut Opal is highly prized in the global gemstone market, known for its exceptional quality and unique characteristics. The gemstone is sought after by collectors, jewelers, and enthusiasts, driving demand and market value. Yowah Nut Opal is often featured in high-end jewelry, including rings, pendants, and earrings, as well as in decorative art pieces.

Conclusion

Yowah Nut Opal is a truly remarkable gemstone, distinguished by its vibrant colors, intricate patterns, and unique formation within ironstone nodules. Found exclusively in the Yowah opal field in Queensland, Australia, this gemstone holds cultural, historical, and economic significance. From its geological origins to its modern-day extraction and global demand, Yowah Nut Opal continues to captivate and inspire those who encounter its natural beauty. As mining practices evolve and sustainability becomes a priority, the legacy of Yowah Nut Opal will endure, preserving its place as one of nature’s hidden gems.

T. Rex not as smart as previously claimed

Photograph of a T. rex skeletal cast at Senckenberg Museum Frankfurt, Germany. T. rex lived at the end of the Cretaceous (about 66 million years ago) and was exclusive to western North America. Credit: Kai R. CasparKai R. Caspar
Photograph of a T. rex skeletal cast at Senckenberg Museum Frankfurt, Germany. T. rex lived at the end of the Cretaceous (about 66 million years ago) and was exclusive to western North America. Credit: Kai R. CasparKai R. Caspar

Dinosaurs were as smart as reptiles but not as intelligent as monkeys, as former research suggests.

An international team of palaeontologists, behavioural scientists and neurologists have re-examined brain size and structure in dinosaurs and concluded they behaved more like crocodiles and lizards.

In a study published last year, it was claimed that dinosaurs like T. rex had an exceptionally high number of neurons and were substantially more intelligent than assumed. It was claimed that these high neuron counts could directly inform on intelligence, metabolism and life history, and that T. rex was rather monkey-like in some of its habits. Cultural transmission of knowledge as well as tool use were cited as examples of cognitive traits that it might have possessed.

However the new study, published today in The Anatomical Record, involving the University of Bristol’s Hady George, Dr Darren Naish (University of Southampton) and led by Dr Kai Caspar (Heinrich Heine University) with Dr Cristian Gutierrez-Ibanez (University of Alberta) and Dr Grant Hurlburt (Royal Ontario Museum) takes a closer look at techniques used to predict both brain size and neuron numbers in dinosaur brains. The team found that previous assumptions about brain size in dinosaurs, and the number of neurons their brains contained, were unreliable.

The research follows decades of analysis in which palaeontologists and biologists have examined dinosaur brain size and anatomy, and used these data to infer behaviour and lifestyle. Information on dinosaur brains comes from mineral infillings of the brain cavity, termed endocasts, as well as the shapes of the cavities themselves.

The team found that their brain size had been overestimated — especially that of the forebrain — and thus neuron counts as well. In addition, they show that neuron count estimates are not a reliable guide to intelligence.

To reliably reconstruct the biology of long-extinct species, the team argues, researchers should look at multiple lines of evidence, including skeletal anatomy, bone histology, the behaviour of living relatives, and trace fossils. “Determining the intelligence of dinosaurs and other extinct animals is best done using many lines of evidence ranging from gross anatomy to fossil footprints instead of relying on neuron number estimates alone,” explained Hady from Bristol’s School of Earth Sciences.

Dr Kai Caspar explained: “We argue that it’s not good practice to predict intelligence in extinct species when neuron counts reconstructed from endocasts are all we have to go on.”

“Neuron counts are not good predictors of cognitive performance, and using them to predict intelligence in long-extinct species can lead to highly misleading interpretations,” added Dr Ornella Bertrand (Institut Català de Paleontologia Miquel Crusafont).

“The possibility that T. rex might have been as intelligent as a baboon is fascinating and terrifying, with the potential to reinvent our view of the past,” concluded Dr Darren Naish. “But our study shows how all the data we have is against this idea. They were more like smart giant crocodiles, and that’s just as fascinating.”

Reference:
Kai R. Caspar, Cristián Gutiérrez‐Ibáñez, Ornella C. Bertrand, Thomas Carr, Jennifer A. D. Colbourne, Arthur Erb, Hady George, Thomas R. Holtz, Darren Naish, Douglas R. Wylie, Grant R. Hurlburt. How smart was T. rex? Testing claims of exceptional cognition in dinosaurs and the application of neuron count estimates in palaeontological research. The Anatomical Record, 2024; DOI: 10.1002/ar.25459

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

First ‘warm-blooded’ dinosaurs may have emerged 180 million years ago

    The artist’s impression shows a dromaeosaur, a type of feathered theropod, in the snow. This dinosaur group is popularly known as a raptor. A well-known dromaeosaur is Velociraptor, portrayed in the film Jurassic Park. Credit: Davide Bonadonna/Universidade de Vigo/UCL
The artist’s impression shows a dromaeosaur, a type of feathered theropod, in the snow. This dinosaur group is popularly known as a raptor. A well-known dromaeosaur is Velociraptor, portrayed in the film Jurassic Park. Credit: Davide Bonadonna/Universidade de Vigo/UCL

The ability to regulate body temperature, a trait all mammals and birds have today, may have evolved among some dinosaurs early in the Jurassic period about 180 million years ago, suggests a new study led by UCL and University of Vigo researchers.

In the early 20th century, dinosaurs were considered slow-moving, “cold-blooded” animals like modern-day reptiles, relying on heat from the sun to regulate their temperature. Newer discoveries indicate some dinosaur types were likely capable of generating their own body heat but when this adaptation occurred is unknown.

The new study, published in the journal Current Biology, looked at the spread of dinosaurs across different climates on Earth throughout the Mesozoic Era (the dinosaur era lasting from 230 to 66 million years ago), drawing on 1,000 fossils, climate models and the geography of the period, and dinosaurs’ evolutionary trees.

The research team found that two of the three main groupings of dinosaurs, theropods (such as T. rex and Velociraptor) and ornithischians (including relatives of the plant eaters Stegosaurus and Triceratops), moved to colder climates during the Early Jurassic, suggesting they may have developed endothermy (the ability to internally generate heat) at this time. In contrast, sauropods, the other main grouping which includes the Brontosaurus and the Diplodocus, kept to warmer areas of the planet.

Previous research has found traits linked to warm-bloodedness among ornithischians and theropods, with some known to have had feathers or proto-feathers, insulating internal heat.

First author Dr Alfio Alessandro Chiarenza, of UCL Earth Sciences, said: “Our analyses show that different climate preferences emerged among the main dinosaur groups around the time of the Jenkyns event 183 million years ago, when intense volcanic activity led to global warming and extinction of plant groups.

“At this time, many new dinosaur groups emerged. The adoption of endothermy, perhaps a result of this environmental crisis, may have enabled theropods and ornithischians to thrive in colder environments, allowing them to be highly active and sustain activity over longer periods, to develop and grow faster and produce more offspring.”

Co-author Dr Sara Varela, of the Universidade de Vigo, Spain, said: “Theropods also include birds and our study suggests that birds’ unique temperature regulation may have had its origin in this Early Jurassic epoch.

“Sauropods, on the other hand, which stayed in warmer climates, grew to a gigantic size at around this time — another possible adaptation due to environmental pressure. Their smaller surface area to volume ratio would have meant these larger creatures would lose heat at a reduced rate, allowing them to stay active for longer.”

In the paper, the researchers also investigated if sauropods might have stayed at lower latitudes to eat richer foliage unavailable in colder polar regions. Instead, they found sauropods seemed to thrive in arid, savannah-like environments, supporting the idea that their restriction to warmer climates was more related to higher temperature and then to a more cold-blooded physiology. During that time, polar regions were warmer, with abundant vegetation.

The Jenkyns event occurred after lava and volcanic gasses erupted from long fissures in the Earth’s surface, covering large areas of the planet.

Co-author Dr Juan L. Cantalapiedra, of the Museo Nacional de Ciencias Naturales, Madrid, Spain, said: “This research suggests a close connection between climate and how dinosaurs evolved. It sheds new light on how birds might have inherited a unique biological trait from dinosaur ancestors and the different ways dinosaurs adapted to complex and long-term environmental changes.”

The study involved researchers from UCL, University of Vigo, the University of Bristol and the Museo Nacional de Ciencias Naturales in Madrid, and received funding from the European Research Council, the Spanish Ministry of Research, the Natural Environment Research Council and the Royal Society.

Reference:
Alfio Alessandro Chiarenza, Juan L. Cantalapiedra, Lewis A. Jones, Sara Gamboa, Sofía Galván, Alexander J. Farnsworth, Paul J. Valdes, Graciela Sotelo, Sara Varela. Early Jurassic origin of avian endothermy and thermophysiological diversity in dinosaurs. Current Biology, 2024; DOI: 10.1016/j.cub.2024.04.051

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

Researchers discover hidden step in dinosaur feather evolution

The specimen under natural light (a) and UV light (b) showing distinct fluorescence hues for bone (cyan) and soft tissues (yellow) against a dark purple sedimentary matrix.
The specimen under natural light (a) and UV light (b) showing distinct fluorescence hues for bone (cyan) and soft tissues (yellow) against a dark purple sedimentary matrix.

Palaeontologists at University College Cork (UCC) in Ireland have discovered that some feathered dinosaurs had scaly skin like reptiles today, thus shedding new light on the evolutionary transition from scales to feathers.

The researchers studied a new specimen of the feathered dinosaur Psittacosaurus from the early Cretaceous (135-120 million years ago), a time when dinosaurs were evolving into birds. The study shows, for the first time, that Psittacosaurus had reptile-like skin in areas where it didn’t have feathers.

The study, published today in Nature Communications, was led by UCC palaeontologists Dr Zixiao Yang and Prof. Maria McNamara of UCC’s School of Biological, Earth and Environmental Sciences, who teamed with scientists based in Nanjing University (China).

The team used ultraviolet (UV) light to identify patches of preserved skin, which are invisible in natural light. Further investigation of the fossil skin using X-rays and infrared light revealed spectacular details of preserved cellular structure.

Dr Yang says:

“The fossil truly is a hidden gem. The fossil skin is not visible to the naked eye, and it remained hidden when the specimen was donated to Nanjing University in 2021. Only under UV light is the skin visible, in a striking orange-yellow glow.

“What is really surprising is the chemistry of the fossil skin. It is composed of silica — the same as glass. This type of preservation has never been found in vertebrate fossils. There are potentially many more fossils with hidden soft tissues awaiting discovery.”

The most exciting aspect of the discovery, however, is what it tells us about the evolution of feathers in dinosaurs. Prof. McNamara, senior author on the study, says:

“The evolution of feathers from reptilian scales is one of the most profound yet poorly understood events in vertebrate evolution. While numerous fossils of feathers have been studied, fossil skin is much more rare.

“Our discovery suggests that soft, bird-like skin initially developed only in feathered regions of the body, while the rest of the skin was still scaly, like in modern reptiles. This zoned development would have maintained essential skin functions, such as protection against abrasion, dehydration and parasites. The first dinosaur to experiment with feathers could therefore survive and pass down the genes for feathers to their offspring.”

The Psittacosaurus specimen NJUES-10 is currently housed in Nanjing University.

Reference:
Zixiao Yang, Baoyu Jiang, Jiaxin Xu, Maria E. McNamara. Cellular structure of dinosaur scales reveals retention of reptile-type skin during the evolutionary transition to feathers. Nature Communications, 2024; 15 (1) DOI: 10.1038/s41467-024-48400-3

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

Rock steady: Study reveals new mechanism to explain how continents stabilized

These ancient metamorphic rocks called gneisses, found on the Arctic Coast, represent the roots of the continents now exposed at the surface. The scientists said sedimentary rocks interlayered in these types of rocks would provide a heat engine for stabilizing the continents. Credit: Jesse Reimink. All Rights Reserved.
These ancient metamorphic rocks called gneisses, found on the Arctic Coast, represent the roots of the continents now exposed at the surface. The scientists said sedimentary rocks interlayered in these types of rocks would provide a heat engine for stabilizing the continents. Credit: Jesse Reimink. All Rights Reserved.

Ancient, expansive tracts of continental crust called cratons have helped keep Earth’s continents stable for billions of years, even as landmasses shift, mountains rise and oceans form. A new mechanism proposed by Penn State scientists may explain how the cratons formed some 3 billion years ago, an enduring question in the study of Earth’s history.

The scientists reported today (May 8) in the journal Nature that the continents may not have emerged from Earth’s oceans as stable landmasses, the hallmark of which is an upper crust enriched in granite. Rather, the exposure of fresh rock to wind and rain about 3 billion years ago triggered a series of geological processes that ultimately stabilized the crust — enabling the crust to survive for billions of years without being destroyed or reset.

The findings may represent a new understanding of how potentially habitable, Earth-like planets evolve, the scientists said.

“To make a planet like Earth you need to make continental crust, and you need to stabilize that crust,” said Jesse Reimink, assistant professor of geosciences at Penn State and an author of the study. “Scientists have thought of these as the same thing — the continents became stable and then emerged above sea level. But what we are saying is that those processes are separate.”

Cratons extend more than 150 kilometers, or 93 miles, from the Earth’s surface to the upper mantle — where they act like the keel of a boat, keeping the continents floating at or near sea level across geological time, the scientists said.

Weathering may have ultimately concentrated heat-producing elements like uranium, thorium and potassium in the shallow crust, allowing the deeper crust to cool and harden. This mechanism created a thick, hard layer of rock that may have protected the bottoms of the continents from being deformed later — a characteristic feature of cratons, the scientists said.

“The recipe for making and stabilizing continental crust involves concentrating these heat-producing elements — which can be thought of as little heat engines — very close to the surface,” said Andrew Smye, associate professor of geosciences at Penn State and an author of the study. “You have to do that because each time an atom of uranium, thorium or potassium decays, it releases heat that can increase the temperature of the crust. Hot crust is unstable — it’s prone to being deformed and won’t stick around.”

As wind, rain and chemical reactions broke down rocks on the early continents, sediments and clay minerals were washed into streams and rivers and carried to the sea where they created sedimentary deposits like shales that were high in concentrations of uranium, thorium and potassium, the scientists said.

Collisions between tectonic plates buried these sedimentary rocks deep in the Earth’s crust where radiogenic heat released by the shale triggered melting of the lower crust. The melts were buoyant and ascended back to the upper crust, trapping the heat-producing elements there in rocks like granite and allowing the lower crust to cool and harden.

Cratons are believed to have formed between 3 and 2.5 billion years ago — a time when radioactive elements like uranium would have decayed at a rate about twice as fast and released twice as much heat as today.

The work highlights that the time when the cratons formed on the early middle Earth was uniquely suited for the processes that may have led them to becoming stable, Reimink said.

“We can think of this as a planetary evolution question,” Reimink said. “One of the key ingredients you need to make a planet like Earth might be the emergence of continents relatively early on in its lifespan. Because you’re going to create radioactive sediments that are very hot and that produce a really stable tract of continental crust that lives right around sea level and is a great environment for propagating life.”

The researchers analyzed uranium, thorium and potassium concentrations from hundreds of samples of rocks from the Archean period, when the cratons formed, to assess the radiogenic heat productivity based on actual rock compositions. They used these values to create thermal models of craton formation.

“Previously people have looked at and considered the effects of changing radiogenic heat production through time,” Smye said. “But our study links rock-based heat production to the emergence of continents, the generation of sediments and the differentiation of continental crust.”

Typically found in the interior of continents, cratons contain some of the oldest rocks on Earth, but remain challenging to study. In tectonically active areas, mountain belt formation might bring rocks that had once been buried deep underground to the surface.

But the origins of the cratons remain deep underground and are inaccessible. The scientists said future work will involve sampling ancient interiors of cratons and, perhaps, drilling core samples to test their model.

“These metamorphosed sedimentary rocks that have melted and produced granites that concentrate uranium and thorium are like black box flight recorders that record pressure and temperature,” Smye said. “And if we can unlock that archive, we can test our model’s predictions for the flight path of the continental crust.”

Penn State and the U.S. National Science Foundation provided funding for this work.

Reference:
Jesse R. Reimink, Andrew J. Smye. Subaerial weathering drove stabilization of continents. Nature, 2024; DOI: 10.1038/s41586-024-07307-1

Note: The above post is reprinted from materials provided by Penn State. Original written by Matthew Carroll.

Can coal mines be tapped for rare earth elements?

Coal core
Coal core

Deposits of designated critical minerals needed to transition the world’s energy systems away from fossil fuels may, ironically enough, be co-located with coal deposits that have been mined to produce the fossil fuel most implicated in climate change.

Now, research led by the University of Utah has documented elevated concentrations of a key subset of critical minerals, known as rare earth elements, or REEs, in active mines rimming the Uinta coal belt of Colorado and Utah.

These findings open the possibility that these mines could see a secondary resource stream in the form of metals used in renewable energy and numerous other high-tech applications, according to study co-author Lauren Birgenheier, an associate professor of geology and geophysics.

“The model is if you’re already moving rock, could you move a little more rock for resources towards energy transition?” Birgenheier said. “In those areas, we’re finding that the rare earth elements are concentrated in fine-grain shale units, the muddy shales that are above and below the coal seams.”

This research was conducted in partnership with the Utah Geological Survey and Colorado Geological Survey as part of the Department of Energy-funded Carbon Ore, Rare Earth and Critical Minerals project, or CORE-CM. The new findings will form the basis for a grant request of an additional $9.4 million in federal funding to continue the research.

While these metals are crucial for U.S. manufacturing, especially in high-end technologies, they are largely sourced from overseas.

“When we talk about them as ‘critical minerals,’ a lot of the criticality is related to the supply chain and the processing,” said Michael Free, a professor metallurgical engineering and the principal investigator on the DOE grant. “This project is designed around looking at some alternative unconventional domestic sources for these materials.”

The association between coal and REE deposits has been well documented elsewhere, but little data had been previously gathered or analyzed in Utah and Colorado’s coal fields.

“The goal of this phase-one project was to collect additional data to try and understand whether this was something worth pursuing in the West,” said study co-author Michael Vanden Berg, Energy and Minerals Program Manager at the Utah Geological Survey. “Is there rare earth element enrichment in these rocks that could provide some kind of byproduct or value added to the coal mining industry?”

Researchers analyzed 3,500 samples from 10 mines, four mine waste piles, seven stratigraphically complete cores, and even some coal ash piles near power plants.

“The coal itself is not enriched in rare earth elements,” Vanden Berg said. “There’s not going to be a byproduct from mining the coal, but for a company mining the coal seam, could they take a couple feet of the floor at the same time? Could they take a couple feet of the ceiling? Could there be potential there? That’s the direction that the data led us.”

The team deployed two different methods to record levels of rare earths, expressed in parts per million, or ppm, in the samples. One was a hand-held device for quick readings in the field, the other used Inductively Coupled Plasma-Mass Spectrometry, or ICP-MS, in an on-campus lab.

“We’re mostly using this portable x-ray fluorescence device, which is an analysis gun that we hold to the rock for two minutes, and it only gives us five or six of the 17 rare earth elements,” Birgenheier said. If samples showed concentrations higher than 200 ppm, they ran a more complete analysis using the more costly mass spectrometry equipment.

The Department of Energy has set 300 ppm as the minimum concentration for rare earth mining to be potentially economically viable. But for the study, researchers deemed concentrations greater than 200 ppm to be considered “REE enriched.”

The study found the highest prevalence of such concentrations in coal-adjacent formations of siltstone and shale, while sandstone and the coal itself were mostly devoid of rare earths.

The team has analyzed 11,000 samples to date, far more than were used in the published study. Next steps include determining how much rare earth ore is present, likely to be done with colleagues at the University of Wyoming and New Mexico Institute of Mining and Technology.

Reference:
Haley H. Coe, Lauren P. Birgenheier, Diego P. Fernandez, Ryan D. Gall, Michael D. Vanden Berg, Andrew Giebel. Rare earth element enrichment in coal and coal-adjacent strata of the Uinta Region, Utah and Colorado. Frontiers in Earth Science, 2024; 12 DOI: 10.3389/feart.2024.1381152

Note: The above post is reprinted from materials provided by University of Utah. Original written by Brian Maffly.

Subduction zone splay faults compound hazards of great earthquakes

Magnified through a microscope, diatoms, which are a type of siliceous microalgae preserved within sediment, helped the researchers determine the salinity levels of the core samples. Photo courtesy of Jessica DePaolis.
Magnified through a microscope, diatoms, which are a type of siliceous microalgae preserved within sediment, helped the researchers determine the salinity levels of the core samples. Photo courtesy of Jessica DePaolis.

Groundbreaking research has provided new insight into the tectonic plate shifts that create some of the Earth’s largest earthquakes and tsunamis.

“This is the first study to employ coastal geology to reconstruct the rupture history of the splay fault system,” said Jessica DePaolis, postdoctoral fellow in Virginia Tech’s Department of Geosciences. “These splay faults are closer to the coast, so these tsunamis will be faster to hit the coastline than a tsunami generated only from a subduction zone earthquake.”

Subduction zones around the world, areas where one tectonic plate shifts under another, create the largest earthquakes — those over magnitude 8.0 — triggering tsunamis and altering ecosystems in their wake. DePaolis, along with Tina Dura, assistant professor of natural hazards, and colleagues from the United States Geological Survey, found evidence that splay faults, the crustal faults connected to the subduction zones, may shift during subduction zone earthquakes and contribute to local coastal destruction and ecological change more regularly than previously realized.

Such a shift of the splay fault underwater can create a tsunami that could reach the nearest shores in 30 minutes or less, DePaolis said.

Published in the Journal of Geophysical Research: Solid Earth, the study should affect hazard awareness at subduction zones around the world. Splay faults exist at subduction zones bordering Ecuador, Cascadia, Chile, and Japan, suggesting they may contribute to tsunami hazards at those locations as well.

When tectonic plates shift at a subduction zone, it occurs miles under the ocean surface. Because splay faults are connected to these zones, their location makes researching them a challenge.

Fortunately, secondary, or surface level, effects of these shifts have been geologically recorded on Montague Island in Prince William Sound in Alaska, making it the only current land mass to sit atop a splay fault to exhibit such effects in its soil.

Typically, the resultant lifting of land from the tectonic plate shifting beneath it, called uplift, from subduction zone earthquakes can be as much as 1 to 3 meters. This is true for most onshore locations impacted by the 1964 earthquake, which hit 9.2 on the Richter scale. However, on Montague Island, splay faults created 11 meters of uplift and initiated drainage of a coastal lagoon, effectively altering its ecosystem from a marine lagoon to a freshwater bog.

“The island is kind of stuck in the middle of these splay faults, so anytime these splay faults rupture, it’s actually recording the uplift,” DePaolis said. “It has this exaggerated uplift that’s just not common in subduction zone-only earthquakes.”

DePaolis and her team examined the effects of the splay fault ruptures on Montague Island. By analyzing 42 sediment cores, they found stratigraphic evidence of the 1964 earthquake and a secondary shift caused by the splay fault. They noticed there was a clear sedimentary change from pre-earthquake lagoon silt to post-earthquake rooted soil.

“There are definitely islands that uplift with subduction zone earthquakes, but they don’t necessarily have faults going through them causing that exaggerated uplift, so it’s a really unique place,” said Dura, an affiliated faculty member of the Global Change Center and the Fralin Life Sciences Institute.

Researchers have believed that a secondary shift from the splay faults was possible. But that idea has been only theoretical until now because this is the first known land mass to record the stratigraphic evidence.

Team members also utilized diatoms, a type of siliceous microalgae preserved within the sediments that is sensitive to changes in salinity, to reconstruct the paleoenvironmental changes that occurred following the 1964 earthquake. They found a clear shift from a highly saline marine lagoon environment out of the reach of tides, indicating uplift of the coast.

Comparing the findings of the 1964 earthquake core samples to samples deeper in the coastal stratigraphy, the research team discovered sedimentary and diatom evidence of three other instances where the splay fault ruptured. This evidence correlated with four of the last eight documented subduction zone earthquakes in the region.

“There’s a huge amount of displacement on these faults that can create those really quick, local, large tsunamis,” DePaolis said. “So you have that local tsunami coming in really quickly and right behind that, you’re going to have the tsunami that was created by the subduction zone itself. All of a sudden you’re having these massive and destructive tsunamis kind of coming in rapidly one after another.”

Reference:
Jessica M. DePaolis, Tina Dura, Robert C. Witter, Peter J. Haeussler, Adrian Bender, Janet H. Curran, D. Reide Corbett. Repeated Coseismic Uplift of Coastal Lagoons Above the Patton Bay Splay Fault System, Montague Island, Alaska, USA. Journal of Geophysical Research: Solid Earth, 2024; 129 (5) DOI: 10.1029/2023JB028552

Note: The above post is reprinted from materials provided by Virginia Tech. Original written by Felicia Spencer.

308-million-year-old arachnid discovered in the Mazon Creek locality

Fossilized Douglassarachne acanthopoda, noted for its up-armored spiny legs, might have resemblance to modern harvestmen, but with a more experimental body plan. Credit: Paul Selden
Fossilized Douglassarachne acanthopoda, noted for its up-armored spiny legs, might have resemblance to modern harvestmen, but with a more experimental body plan. Credit: Paul Selden

More than 300 million years ago, all sorts of arachnids crawled around the Carboniferous coal forests of North America and Europe. These included familiar ones we’d recognize, such as spiders, harvestmen and scorpions—as well as exotic animals that now occur in warmer regions like whip spiders and whip scorpions.

But there were also quite bizarre arachnids in these habitats belonging to now extinct groups. Even among these strange species now lost to time, one might have stood out for its up-armored legs.

The ancient critter was recently described in a new paper published in the Journal of Paleontology, co-written by Paul Selden from the University of Kansas and the Natural History Museum of London and Jason Dunlop from the Museum für Naturkunde Berlin.

“Douglassarachne acanthopoda comes from the famous Mazon Creek locality in Illinois and is about 308 million years old,” said lead author Selden. “This compact arachnid had a body length of about 1.5 centimeters and is characterized by its remarkably robust and spiny legs—such that it is quite unlike any other arachnid known, living or extinct.”

The KU researcher said Carboniferous Coal Measures are an important source of information for fossil arachnids, representing the first time in Earth’s history when most living groups of arachnids occurred together. Yet, the fauna was still quite different to today.

“Spiders were a rather rare group, only known at that time from primitive lineages, and they shared these ecosystems with various arachnids which have long since died out,” said co-author Dunlop.

“Douglassarachne acanthopoda is a particularly impressive example of one of these extinct forms. The fossil’s very spiny legs are reminiscent of some modern harvestmen, but its body plan is quite different from a harvestman or any other known arachnid group.”

This led the two scientists to conclude it doesn’t belong in any of the known arachnid orders.

“Unfortunately, details such as the mouth parts cannot be seen, which makes it difficult to say exactly which group of arachnids are its closest relatives,” Selden said. “It could belong to a wider group, which includes spiders, whip spiders and whip scorpions. Whatever its evolutionary affinities, these spiny arachnids appear to come from a time when arachnids were experimenting with a range of different body plans.

“Some of these later became extinct, perhaps during the so-called ‘Carboniferous Rainforest Collapse,’ a time shortly after the age of Mazon Creek when the coal forests began to fragment and die off. Or perhaps these strange arachnids clung on until the end Permian mass extinction?”

According to the team, Mazon Creek fossil locality is one of the most important windows into life in the late Carboniferous, producing a wide range of fascinating plants and animals. The present fossil was discovered in a clay-ironstone concretion in the 1980s by Bob Masek and later acquired by the David and Sandra Douglass Collection and displayed in their Prehistoric Life Museum.

“The genus name Douglassarachne acknowledges the Douglass family, who kindly donated the specimen to the Field Museum of Natural History in Chicago for scientific study once it became apparent that it represented an undescribed species,” Dunlop said. “Then, acanthopoda refers to the unique and characteristic spiny legs of the animal.”

Reference:
Paul A. Selden et al, A remarkable spiny arachnid from the Pennsylvanian Mazon Creek Lagerstätte, Illinois, Journal of Paleontology (2024). DOI: 10.1017/jpa.2024.13

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

Earth scientists describe a new kind of volcanic eruption

Telephoto view looking east of the active lava lake within Halema‘uma‘u at the summit of Kīlauea. Credit: N. Deligne / USGS / Public Domain
Telephoto view looking east of the active lava lake within Halema‘uma‘u at the summit of Kīlauea. Credit: N. Deligne / USGS / Public Domain

No two volcanic eruptions are exactly alike, but scientists think a series of explosive eruptions at Kīlauea volcano fit into a whole new category.

By analyzing the dynamics of 12 back-to-back explosions that happened in 2018, researchers describe a new type of volcanic eruption mechanism. The explosions were driven by sudden pressure increases as the ground collapsed, which blasted plumes of rock fragments and hot gas into the air, much like a classic stomp-rocket toy.

Researchers from the University of Oregon, United States Geological Survey and China’s Sichuan University report their findings in a paper published May 27 in Nature Geoscience.

The particular string of explosions at the summit of Kīlauea was part of a sequence of events that included lava flows erupting from lower on the flank of the volcano. Those lava flows destroyed thousands of homes and displaced residents on the Island of Hawai’i for months.

Understanding exactly what happened in past volcanic eruptions, colloquially called “hindcasting,” allows volcanologists to make better forecasts about future eruptions and give more accurate warnings to people in an eruption’s path.

For the most part, explosive volcanic eruptions are either primarily driven by rising magma, vaporized groundwater, or some combination of the two, according to Josh Crozier, who did this research as a doctoral student at the UO. But these eruptions didn’t quite fit the mold.

“These eruptions are quite interesting in that they don’t really seem to involve either of those,” Crozier said. “The eruptive material contained very little that looked like fresh magma that was blasted out, but there’s no evidence for significant groundwater being involved, either.”

The Hawaiian Volcano Observatory, part of the U.S. Geological Survey, keeps close tabs on Kīlauea. The volcano is covered with scientific instruments, from ground sensors that measure the shaking of the earth to tools that analyze the gases released from the volcano.

“A cool thing about these eruptions is that there were a bunch of them in sequence that were remarkably similar; that’s relatively unusual,” said Leif Karlstrom, a volcanologist at the UO. “Typically, volcanic eruptions don’t happen with as much regularity.”

So the team had more data than usual to work with, and they could dig deeper into the specific dynamics of the eruptions.

Putting all that data into a variety of atmospheric and subsurface models, the scientists pieced together a new story about what happened on Kīlauea during the string of events in 2018.

Before each explosion at the summit, magma was slowly draining from an underground reservoir. (This magma was feeding lava flows 40 kilometers away, on the eastern flank of the volcano.) As the reservoir depleted, the ground above it — the crater within the caldera at the volcano’s summit — suddenly collapsed.

That quickly increased the pressure in the reservoir. And because there was a pocket of accumulated magmatic gas sitting at the top of this reservoir, the pressure increase squeezed the magmatic gas and bits of rubble through a conduit and blasted them out of a vent in Kīlauea’s crater.

The researchers compare the eruption dynamic to a stomp-rocket toy, where stepping on an air bag connected to a hose launches a projectile into the air.

“The ‘stomp’ is this whole kilometer-thick chunk of rock dropping down, pressurizing the pocket, and then forcing material directly up,” Crozier said. And the ‘rocket’ is, of course, the gas and rocks erupting from the volcano.

Caldera collapse is fairly common, Crozier notes. So while this is the first time scientists have specifically spelled out this specific stomp-rocket mechanism, it’s probably not the only time it’s occurred.

The study was able to link geophysical observations to the properties of the volcanic plume in the atmosphere.

“This link is very rare,” said Joe Dufek, a volcanologist at the UO. “It points to new ways for us to observe eruptions and to combine sensor measurements with computer simulations to better assess hazards from eruptions.”

The fact that this was a series of smaller eruptions may have made it easier to see the underlying mechanism, Dufek said. Other complex processes weren’t overshadowing the stomp-rocket component.

But that’s not to say that Kīlauea is simple. A typical textbook drawing of a volcano shows magma moving upwards through chambers at different depths. But it’s rarely that straightforward, and a volcano like Kīlauea, decked out in scientific instruments, provides an opportunity to dig into the details.

“This is an example, and there’s an increasing number of these, where the pathways of magma ascent are quite geometrically complex,” Karlstrom said. “It gives us a much more nuanced picture of what volcanic plumbing systems look like.”

Reference:

Josh Crozier, Josef Dufek, Leif Karlstrom, Kyle R. Anderson, Ryan Cahalan, Weston Thelen, Mary Benage, Chao Liang. Explosive 2018 eruptions at Kīlauea driven by a collapse-induced stomp-rocket mechanism. Nature Geoscience, 2024; DOI: 10.1038/s41561-024-01442-0

Note: The above post is reprinted from materials provided by University of Oregon. Original written by Laurel Hamers.

Artificial geysers can compensate for our mineral shortages

Take a close look at these seabed minerals! Green copper minerals are seen here precipitated in a sectioned sulphide sample, retrieved from a scientific cruise conducted by the Norwegian Offshore Directorate across the Mohns Ridge in 2020. Credit: Øystein Leiknes Nag/Norwegian Offshore Directorate
Take a close look at these seabed minerals! Green copper minerals are seen here precipitated in a sectioned sulphide sample, retrieved from a scientific cruise conducted by the Norwegian Offshore Directorate across the Mohns Ridge in 2020. Credit: Øystein Leiknes Nag/Norwegian Offshore Directorate

By imitating nature, it may be possible to recover seabed minerals by extracting hot water from the Earth’s crust. We can harvest green energy and be sensitive to the environment—all at the same time.

Seabed minerals: Here’s something you probably don’t know. The copper found in the Norwegian mines at Røros and Løkken, and which once made the country very wealthy, was formed from smoking “chimneys” on the ocean floor.

In the Earth’s remote past, this copper was carried up through the crust by seawater that had originally been drawn downwards into the scorching depths. If we humans can learn to imitate part of this process, it may be possible to apply it to sensitively recover a variety of minerals from the oceans offshore Norway.

At SINTEF, we believe that seabed minerals should only be recovered if we can develop methods that minimize any negative environmental impacts. We are now in the process of identifying one such method.

Or, in other words, of obtaining the “building blocks” being called for by the green transition. At the same time, we can obtain valuable geothermal heat that we can convert into emissions-free energy.

From the scorching depths to the deck of a platform

In the heated debate currently raging about seabed minerals, now fueled once again by WWF’s recent notification to sue the Norwegian state, many people have expressed their fear of negative ecological consequences resulting from the exploitation of these resources.

At SINTEF, we believe that seabed minerals should only be recovered if we can develop methods that minimize any negative environmental impacts. We are now in the process of identifying one such method.

Our idea is to transport the mineral-rich water and bypass the process of precipitation on the seabed, recovering the minerals directly from the scorching depths in the Earth’s crust from where they originate. Extraction will take place on the deck of an offshore platform.

Water heated by molten rock

Below the sea surface, some distance from land, there are several locations where so-called black smoker geysers eject mineral-rich waters brought up from the depths of the crust.

This phenomenon is the result of water first having been drawn down into fractures in the volcanic rocks of the seabed and then all the way down into the mantle, which is the layer of molten rock lying beneath the crust. Here, the water is subject to intense heat and is able to take up particles of metals and minerals. These are exactly the materials we need to make our batteries, wind turbines and electric vehicle engines.

Then, the mineral-rich water rises from the mantle, through the crust, and up to the seabed, where it is ejected from the black smoker geysers.

Electricity from steam

At SINTEF, we are working on the idea of imitating part of this process by constructing artificial geysers. Firstly, by drilling wells for sending seawater down into the mantle—and then others for transporting the mineral-rich water back to the surface.

This water will be transported in pipes up to platforms where the particles will be separated.

The pressure at the Earth’s surface will cause the water to boil. Our idea is to use the steam to generate electricity, which will then be sent onshore. The revenues from selling the electricity will be used to pay for parts of the mineral recovery process.

Discovered in the 1970s

SINTEF has been here before—demonstrating that imitating nature can be a very fruitful venture. Specifically, that the properties of underwater shales are ideal for dealing with abandoned oil wells.

The phenomenon that we are seeking to imitate today—these “black smokers” on the seabed—was discovered in the 1970s in an area of the Pacific Ocean at the boundary between two tectonic plates.

Many underwater geysers of this type have been identified on the Mid-Atlantic Ridge in Norwegian waters. These are locations where molten magma still occurs close to the seabed. Some of them are probably still active today.

Sulfide minerals

The smoker chimneys are made up of particles that are precipitated when the hot, mineral-rich water is ejected from the geysers into the cold seawater. Other fractions of the ejected mass of particles have sunk to the seabed, forming great mounds of gravel at the base of the chimneys.

As time passes, many of the chimneys stop ejecting. They seal up and die, tipping over onto the “piles of gravel.”

These gravel piles represent the biggest and most concentrated occurrences of sulfide minerals on the seabed. The sulfide family is one of the two main groups of seabed minerals known from Norwegian oceans.

Key metals

According to the Norwegian Offshore Directorate, the natural geysers have deposited minerals containing key metals such as zinc, cobalt, nickel, vanadium, tungsten and silver. Not to mention copper, which occurs in concentrations much greater than those we encounter in mines onshore.

Our idea assumes that humans will succeed in drilling wells that can withstand the temperatures they will encounter close to bodies of molten rock. Experts are already working on this problem..

“Our concept will not be put into practice tomorrow, but it may not be too far into the future either. The timing will depend on the efforts that we are prepared to put into developing the idea. We still need more data about the subsurface, combined with some smart technological innovations.

Supply security for the green transition

If our idea succeeds, this will help the European Parliament, the Norwegian government and everyone else who is looking to safeguard supply security for the green transition.

We have great faith that our concept represents a sensitive and realistic approach to minerals recovery, and are looking forward to continuing with its development.

Note: The above post is reprinted from materials provided by Norwegian University of Science and Technology.

Exploring the Beauty and Mystery of Flower Agate

 

Flower Agate
Flower Agate

Introduction

There are several mesmerising minerals in the gemstone world, each with its own narrative to tell. Flower Agate is one gemstone that has piqued the interest of both collectors and enthusiasts. Flower Agate stands out as a beautiful work of nature’s art, with its exquisite flower designs and enticing colours. In this in-depth examination, we will look at the geological origins, features, formations, and importance of this fascinating mineral.

Geological Origins

Flower Agate, officially classed as a chalcedony variation, is a member of the vast quartz mineral family. Chalcedony is a microcrystalline form of quartz distinguished by its fine-grained structure and waxy lustre. Flower Agate is distinguished from other chalcedony kinds by its distinctive interior patterns like blossoming flowers, which give it an airy and appealing look.

The geological processes that create Flower Agate are as interesting as the gemstone itself. Flower Agate is thought to have formed as a result of volcanic activity, in which silica-rich fluids permeated voids within host rocks such as basalt. Over time, these fluids crystallise, resulting in complex formations within the voids. The abundance of impurities and mineral inclusions contributes to Flower Agate’s unique colours and patterns.

Description and Appearance

One of Flower Agate’s most outstanding aspects is its gorgeous interior patterns, which are very similar to blooming flowers. These patterns usually appear as dendritic structures or plumes that are elaborately intertwined into the transparent chalcedony matrix. Flower Agate’s colours span from subtle pastels to vivid hues, with pink, peach, white, and green being particularly frequent. The combination of colours and patterns within each specimen creates a sense of depth and dimension, adding to its attraction.

Flower Agate, in addition to its visual appeal, has favourable physical qualities that make it desirable as a gemstone. Its Mohs hardness ranges from 6.5 to 7, making it excellent for usage in a variety of jewellery and lapidary arts. Flower Agate’s relatively high resilience means it can resist the rigours of daily usage, making it a popular option for gemstone fans looking for both beauty and endurance.

Formation and Occurrence

Flower Agate is most commonly found in areas with a history of volcanic activity, where the geological conditions required for its creation exist. Madagascar, China, and the United States are notable suppliers of Flower Agate, with each producing specimens with distinct colours and patterns.

Madagascar is well-known for its broad variety of gemstones, but it is especially known for creating high-quality Flower Agate specimens. The deposits in Madagascar sometimes produce examples with vibrant pink and peach hues, covered with exquisite flower designs that equal the splendour of a botanical garden. Collectors and lapidary artists value these examples for their outstanding beauty and workmanship.

Flower Agate is most often found in Guangdong Province, China, and is recognised for its delicate pastel colours and beautiful dendritic structures. The examples from China have a tranquil grace evocative of cherry blossoms in full bloom. While not as well known as Madagascar examples, Chinese Flower Agate has a devoted following among gemstone enthusiasts.

Flower Agate has been discovered in various regions in the United States, including Oregon and Washington. Although less frequent than other sources, American Flower Agate has its own distinct beauty, with specimens varying in colour from gentle whites to bright greens. These examples are prized by local collectors and lapidary aficionados for their unique beauty and historical relevance.

Significance and uses

Beyond its visual appeal, Flower Agate has symbolic meaning in many civilizations and traditions. Flower Agate is thought to represent growth, rejuvenation, and abundance in metaphysical circles, making it an attractive option for spiritual healing and meditation activities. It is frequently connected with the heart chakra, which promotes peace, compassion, and emotional balance.

Flower Agate is highly valued in the jewellery and creative arts industries for its flexibility and beauty. Its exquisite patterns and calming colours make it an excellent material for making striking items like pendants, earrings, and rings. Flower Agate is also used by lapidary artisans to create beautiful artefacts like as carvings and sculptures, where its natural beauty can be fully appreciated.

Furthermore, Flower Agate demonstrates nature’s ongoing inventiveness and brilliance. Its creation over millions of years demonstrates the incredible durability and beauty of the Earth’s geological heritage. As a result, Flower Agate acts as a concrete reminder of the interdependence of geology, art, and culture, bridging the gap between the natural world and human creation.

Conclusion

Finally, Flower Agate reflects the natural world’s enchanting beauty and mystery. Flower Agate, with its geological roots in volcanic settings and gorgeous formations of blossoming flowers, continues to fascinate the imaginations of collectors, enthusiasts, and spiritual searchers alike. As we continue to uncover the mysteries of this enchanted diamond, we develop a greater appreciation for the wonderful diversity of Earth’s geological riches and the enduring fascination of nature’s workmanship.

Unraveling the Mysteries of Utroba Cave

Utroba Cave, Bulgaria
Utroba Cave, Bulgaria

Utroba Cave, located in Bulgaria’s gorgeous Rhodope Mountains, is a natural marvel that draws both explorers and scientists. This underground labyrinth, with its complex structures and timeless beauty, provides insight into the region’s geological past and the forces that formed it over millions of years.

The cave is located 20 kilometers from the city of Kardzhali near the village of Ilinitsa and it dates to 480 BC. It is also referred to as “The Cave Womb” or “Womb Cave” because the entrance is the shape of a vulva. The inside of the cave resembles a uterus. Locally it is also called “The Blaring Rock”.

The Origins of Utroba Cave

Utroba Cave, also known as “The Womb” in Bulgarian, is the result of a gradual yet constant dance between rock and water. The cave, formed in the core of limestone, began its journey aeons ago, when ancient oceans flooded most of what is now Bulgaria. As water percolated through the porous rock, it dissolved the limestone, forming enormous caverns under the surface.

A Geological Tapestry

Utroba Cave’s walls, a geological tapestry spanning millennia, tell its tale. The cave’s formations—stalactites, stalagmites, columns, and flowstones—are the result of water and time. Each drop of mineral-rich water leaves a small deposit of calcite, eventually forming these beautiful formations over thousands of years.

Time’s Impression

To really understand Utroba Cave, consider the massive periods required in its development. Stalactites, which dangle like icicles from the ceiling, develop at a pace of millimetres each century, whereas stalagmites rise almost imperceptibly from the cave floor. Together, they see nature’s slow, patient work, which unfolds across epochs too vast for the human intellect to completely comprehend.

Geological Processes in Play

The development of Utroba Cave demonstrates the complicated interaction of geological processes. It starts with the dissolving of limestone, also known as karstification, in which carbonic acid in rainfall combines with calcium carbonate in the rock, eventually eroding it away. Over time, this results in networks of underground corridors and chambers, such as those discovered in Utroba Cave.

The Role of Water

Water is the major sculptor in caverns like Utroba, forming the scenery both above and below earth. As it seeps through cracks and fissures in the rock, it dissolves the limestone, expanding existing passageways and generating new ones. Underground rivers and streams continue to carve out the cave system, transporting sediments and sculpting the formations we see today.

Geological Time in Perspective

Understanding the immensity of geological time requires confronting the humbling fact of our own fleeting existence. Utroba Cave has evolved over millions of years, long before people roamed the world. It demonstrates the persistent force of natural processes, which are still shaping our globe in subtle and deep ways.

Conclusion

Utroba Cave is a testament to nature’s everlasting beauty and the unstoppable march of geological time. Its structures, formed over millions of years, provide a glimpse into the Rhodope Mountains’ distant history and the forces that shaped it. As we explore the depths of Utroba Cave, let us marvel at nature’s grandeur and consider our role in the great fabric of time.

New step in tectonic squeeze that turns seafloor into mountains

The opening and closing of the Rocas Verdes Basin, a back-arc basin in Patagonia, as described by researchers at The University of Texas at Austin in a study published in Geology. Panels B and C illustrate the basin-closure process, in which an underlying portion of the oceanic crust is thrust into a magma chamber (B) and breaks off ahead of continental crust (C). The last two panels (C and D) show the oceanic plate and continental plate colliding together – squeezing the basin together into the Andes Mountains of Patagonia that we see today. Credit: Fernando Rey et al
The opening and closing of the Rocas Verdes Basin, a back-arc basin in Patagonia, as described by researchers at The University of Texas at Austin in a study published in Geology. Panels B and C illustrate the basin-closure process, in which an underlying portion of the oceanic crust is thrust into a magma chamber (B) and breaks off ahead of continental crust (C). The last two panels (C and D) show the oceanic plate and continental plate colliding together – squeezing the basin together into the Andes Mountains of Patagonia that we see today. Credit: Fernando Rey et al

Scientists use tiny minerals called zircons as geologic timekeepers. Often no bigger than a grain of sand, these crystals record chemical signatures of the geological environment where they formed. In a new study led by scientists at The University of Texas at Austin, researchers used them to describe what could be an overlooked step in a fundamental tectonic process that raises seafloors into mountains.

In a study published in the journal Geology, the researchers describe zircons from the Andes mountains of Patagonia. Although the zircons formed when tectonic plates were colliding, they have a chemical signature associated with when the plates were moving apart.

The researchers think that the unexpected signature could be explained by the mechanics of underlying tectonic plates that hasn’t yet been described in other models. This missing step involves a sort of geologic juicing in a magma chamber where zircons form before they reach the surface, with oceanic crust entering the chamber ahead of continental crust.

“If you put some oceanic basin below this magma, you have a change in the composition of this magma as it’s incorporated,” said the study’s lead author Fernando Rey, a doctoral student at the UT Jackson School of Geosciences. “This is something that was not documented before this study.”

This theory of oceanic magma mixing is important because it could represent a transitional step in the formation of back arc basins — an important geological structure that shapes landscapes, geologic records and helps regulate the planet’s climate.

These basins form between oceanic and continental tectonic plates, opening up as the plates move apart and closing as they come back together. While the opening of the basin creates oceanic crust, its closing squeezes the crust into mountains — bringing a geologic record of Earth history to the surface where humans can more easily access it, said coauthor Matt Malkowski, an assistant professor at the Jackson School’s Department of Earth and Planetary Sciences. What’s more, the weathering of the ocean crust is a major driver of natural carbon dioxide storage. “This is the Earth’s way of sequestering carbon. Very effective on its own, but it may take hundreds of thousands if not millions of years,” said Malkowski.

Malkowski collected the zircons examined in the study from rock and sediment samples at a field site in Patagonia. The samples captured the entire record of the back arc basin, called the Rocas Verdes Basin, from opening to closing.

When Rey started analyzing the chemical signatures of the zircons, nothing looked out of place at first. The zircons associated with an opening basin had the expected signature. However, when he started examining zircons associated with the closing of the basin, the signature didn’t undergo the expected chemical shift — known to scientists as a “pull down” because of the way data plotting the isotope ratios goes from steadily rising to falling down.

When that pull down signature didn’t show up until 200 million years later, appearing in zircons that formed 30 million years ago when the basin was already well into its closure phase, Rey and his collaborators hypothesized a scenario that could help explain the data.

In their paper, they propose a model where the same tectonic forces that squeeze the oceanic crust into mountains could be underthrusting parts of that crust and pushing it toward the magmatic chamber where the zircons are formed — influencing the chemical signatures recorded in the crystals during the early to middle stages of closure. As the continents continue to squeeze together, the oceanic crust is eventually replaced by continental crust, the source of the pulldown signal.

The researchers think this transitional phase where zircons are juiced by oceanic crust could be part of back arc basins around the world. But there’s a good reason why it hasn’t been observed before, said Rey. Most back arc basins close faster than Patagonia did — in a few million years rather than tens of millions of years — meaning a shorter window of time in which these zircons can form.

Now that scientists have discovered this zircon signal in Patagonia, they can start looking for signs of it in zircons from other places. Rey is currently analyzing zircons from the Sea of Japan — a modern back arc basin that’s in the early stages of closure — to see if there’s signs of oceanic crust influencing the zircon signature.

This research adds to a record of discovery about back arc basins at UT Austin, said Malkowski. Professor Ian Dalziel authored a well-known Nature paper in 1974 that first recognized the Andes of Patagonia as forming due to back arc basin closure.

“Here we are 50 years later, and we’re still learning new things about these rocks,” Malkowski said.

The research was funded by the National Science Foundation and UT Austin.

References:

  1. F.M. Rey, M.A. Malkowski, J.C. Fosdick, S.C. Dobbs, M. Calderón, M.C. Ghiglione, S.A. Graham. Detrital isotopic record of a retreating accretionary orogen: An example from the Patagonian Andes. Geology, 2024; DOI: 10.1130/G51918.1
  2. Ian W. D. Dalziel, Maarten J. de Wit, Keith F. Palmer. Fossil marginal basin in the southern Andes. Nature, 1974; 250 (5464): 291 DOI: 10.1038/250291a0

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

New geological study: Scandinavia was born in Greenland

The zircon crystals we found in river sand and rocks from Finland have signatures that point towards them being much older than anything ever found in Scandinavia, while matching the age of Greenlandic rock samples. Photo: Andreas Petersson.
The zircon crystals we found in river sand and rocks from Finland have signatures that point towards them being much older than anything ever found in Scandinavia, while matching the age of Greenlandic rock samples. Photo: Andreas Petersson.

In a Finnish outcrop nestled between some of Northern Europe’s oldest mountains, researchers have found traces of a previously hidden part of Earth’s crust that points more than three billion years back in time and north towards Greenland.

These traces were found in the mineral zircon, which after chemical analyses, indicated to researchers from the Department of Geosciences and Natural Resource Management that the “foundation” upon which Denmark and Scandinavia rest, was probably ‘born’ from Greenland approximately 3.75 billion years ago.

“Our data suggest that the oldest part of Earth’s crust beneath Scandinavia originates in Greenland and is about 250 million years older than we previously thought,” says Professor Tod Waight, a geologist at the Department of Geosciences and Natural Resource Management.

The researchers’ study of the zircon showed that, in several ways, its chemical fingerprint matches those of some of the oldest rocks on the planet found in West Greenland’s North Atlantic Craton.

“The zircon crystals we found in river sand and rocks from Finland have signatures that point towards them being much older than anything ever found in Scandinavia, while matching the age of Greenlandic rock samples. At the same time, the results of three independent isotope analyses confirm that Scandinavia’s bedrock was most likely linked to Greenland,” says Department of Geosciences and Natural Resource Management researcher Andreas Petersson.

A water world without oxygen

Denmark, Sweden, Norway and Finland rest atop a part of Earth’s crust known as the Fennoscandian Shield, or the Baltic Shield. The researchers believe that it broke away from Greenland as a “seed” and shifted for hundreds of millions of years until it “took root” where Finland is today.

Here, the plate grew as new geological material accumulated around it, until it became Scandinavia. At the time of the crust’s detachment from Greenland, the planet looked very different than today.

“Earth was probably a watery planet, like in the movie Waterworld, but without any oxygen in the atmosphere and without emergent crust. But, because that’s so far back in time, we can’t be really be sure about what it actually looked like,” says Tod Waight.

According to the researchers, the fact that Earth even has a continental crust composed of granite is quite special when they look out into space and compare it with other planets in our galactic neighborhood.

“This is unique in our solar system. And, evidence of liquid water and a granite crust are key factors when trying to identify habitable exoplanets and the possibility of life beyond Earth,” explains Andreas Petersson.

Continents are the key to life

The new study adds pieces to a primordial continental puzzle that began long before life on Earth truly blossomed, but which has largely paved the way for both human and animal life.

“Understanding how continents formed helps us understand why ours is the only planet in the solar system with life on it. Because without fixed continents and water in between them, we wouldn’t be here. Indeed, continents influence both ocean currents and climate, which are crucial for life on Earth,” says Andreas Petersson.

Furthermore, the new study contributes to a growing number of studies which reject the means used thus far to calculate how continents have grown — especially during the first billion years of Earth’s history.

“The most commonly used models assume that Earth’s continental crust began to form when the planet was formed, about 4.6 billion years ago. Instead, our and several other recent studies suggest that the chemical signatures showing growth of the continental crust can only be identified about a billion years later. This means that we may need to revise much of what we thought about how early continents evolved,” says Professor Waight.

At the same time, results of the study add to previous research that found similar “seeds” from ancient crusts in other parts of the world.

“Our study provides us with another important clue in the mystery of how continents formed and spread across Earth — especially in the case of the Fennoscandian Shield. But there is still plenty that we don’t know. In Australia, South Africa and India, for example, similar seeds have been found, but we’re unsure of whether they all come from the same “birthplace,” or whether they originated independently of one another in several places on Earth. This is something that we would like to investigate more using the method we used in this study,” concludes Professor Waight.

About the study

  • The study demonstrates that the oldest part of Earth’s crust beneath Scandinavia comes from Greenland and is about 250 million years older than once thought.
  • Therefore, Denmark and Scandinavia’s geologic foundation was most likely connected to Greenland approximately 3.75 billion years ago.
  • The researchers analysed zircons from modern river sand and rock samples from the remote Pudasjärvi and Suomujärvi regions of Finland, whose geological origins have been little studied.
  • The zircon crystals found in the Finnish river sand originally crystallized in granitic magmas deep within the crust. These granites were then lifted to the surface and eroded to eventually form sand.
  • The researchers used isotopic compositions of lead, hafnium and oxygen to trace the chemical fingerprint from the Fennoscandian Shield back to Greenland.
  • The study has been published in the scientific journal Geology.

Reference:
Andreas Petersson, Tod Waight, Anthony I.S. Kemp, Martin. J. Whitehouse, John W. Valley. An Eoarchean continental nucleus for the Fennoscandian Shield and a link to the North Atlantic craton. Geology, 2023; 52 (3): 171 DOI: 10.1130/G51658.1

Note: The above post is reprinted from materials provided by University of Copenhagen – Faculty of Science.

Mars attracts: How Earth’s interactions with the red planet drive deep-sea circulation

Mars
This is a mosaic image of Mars created from over 100 images taken by Viking Orbiters in the 1970s. Credit: NASA

Scientists from the Universities of Sydney and Sorbonne University have used the geological record of the deep sea to discover a connection between the orbits of Earth and Mars, past global warming patterns and the speeding up of deep ocean circulation.

They discovered a surprising 2.4-million-year cycle where deep currents wax and wane which, in turn, is linked to periods of increased solar energy and a warmer climate.

The study, published in Nature Communications, tackles the questions of how geological-timescale climate change affects ocean circulation and how this could help scientists to model future climates outcomes. The researchers looked to find if ocean-bottom currents become more vigorous or more sluggish in a warmer climate.

These cycles are not linked to the current rapid global warming caused by human greenhouse gas emissions.

Lead author ARC Future Fellow Dr Adriana Dutkiewicz from the University of Sydney EarthByte Group in the School of Geosciences and co-authors used more than half a century of scientific drilling data from hundreds of sites worldwide to understand the vigour of deep-sea currents through time.

In a collaboration with Professor Dietmar Müller (University of Sydney) and Associate Professor Slah Boulila (Sorbonne), Dr Dutkiewicz used the deep-sea sediment record to check for links between sedimentary shifts and changes in the Earth’s orbit.

They found that the vigour of deep-sea currents shifts in 2.4-million-year cycles.

These cycles are called “astronomical grand cycles,” predicted to occur due to the interactions of Earth and Mars orbits. However, evidence for this is rarely detected in the geological record.

Dr Dutkiewicz said: “We were surprised to find these 2.4-million-year cycles in our deep-sea sedimentary data. There is only one way to explain them: they are linked to cycles in the interactions of Mars and Earth orbiting the Sun.”

Co-author Professor Müller said: “The gravity fields of the planets in the solar system interfere with each other and this interaction, called a resonance, changes planetary eccentricity, a measure of how close to circular their orbits are.”

For the Earth it means periods of higher incoming solar radiation and warmer climate in cycles of 2.4 million years. The researchers found that the warmer cycles correlate with an increased occurrence of breaks in the deep-sea record, related to more vigorous deep ocean circulation.

The study has identified that deep eddies were an important component of earlier warming seas. It is possible these could partly mitigate ocean stagnation some have predicted could follow a faltering AMOC (Atlantic meridional overturning circulation) that drives the Gulf Stream and maintains temperate climates in Europe.

Professor Müller said: “We know there are at least two separate mechanisms that contribute to the vigour of deep-water mixing in the oceans. AMOC is one of them, but deep ocean eddies seem to play an important role in warm climates for keeping the ocean ventilated.

“Of course, this would not have the same effect as AMOC in terms of transporting water masses from low to high latitudes and vice-versa.”

These eddies are like giant whirlpools and often reach the abyssal seafloor, resulting in seafloor erosion and large sediment accumulations called contourites, akin to snowdrifts.

Dr Dutkiewicz said: “Our deep-sea data spanning 65 million years suggest that warmer oceans have more vigorous deep circulation. This will potentially keep the ocean from becoming stagnant even if Atlantic Meridional Overturning Circulation slows or stops altogether.”

How the interplay between different processes driving deep-ocean dynamics and ocean life may play out in the future is still not well known, but the authors hope that their new results will help with building better climate models.

Reference:
Adriana Dutkiewicz, Slah Boulila, R. Dietmar Müller. Deep-sea hiatus record reveals orbital pacing by 2.4 Myr eccentricity grand cycles. Nature Communications, 2024; 15 (1) DOI: 10.1038/s41467-024-46171-5

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

Do some mysterious bones belong to gigantic ichthyosaurs?

A reconstruction of a gigantic ichthyosaur - floating dead on the surface of the ocean. Remains of ichthyosaurs have been found in ocean sediment in various places around Europe. Credit: Marcello Perillo/University of Bonn
A reconstruction of a gigantic ichthyosaur – floating dead on the surface of the ocean. Remains of ichthyosaurs have been found in ocean sediment in various places around Europe. Credit: Marcello Perillo/University of Bonn

Several similar large, fossilized bone fragments have been discovered in various regions across Western and Central Europe since the 19th century. The animal group to which they belonged is still the subject of much debate to this day. A study carried out at the University of Bonn could now settle this dispute once and for all: The microstructure of the fossils indicates that they come from the lower jaw of a gigantic ichthyosaur. These animals could reach 25 to 30 meters in length, a similar size to the modern blue whale. The results have now been published in the journal PeerJ.

In 1850, the British naturalist Samuel Stutchbury reported a mysterious find in a scientific journal: A large, cylindrical bone fragment had been discovered at Aust Cliff — a fossil deposit near to Bristol. Similar bone fragments have since been found in various different places around Europe, including Bonenburg in North Rhine-Westphalia and in the Provence region of France. More than 200 million years ago, these areas were submerged beneath a huge ocean that covered vast swathes of Western and Central Europe. Fossil remains from the animal world of that time — including marine and coastal dwellers — have been preserved in the sediment.

There is still some debate to this day about the animal group to which these large, fossilized bones belonged. Stutchbury assumed in his examination of the first finds that they came from a labyrinthodontia, an extinct crocodile-like land creature. However, this hypothesis was questioned by other researchers, who believed instead that the fossils came from long-necked dinosaurs (sauropods), stegosaurs or a still completely unknown group of dinosaurs.

Unusual tissue made of protein fibers

“Already by the beginning of the 20th century, some other researchers had theorized that the fossils could possibly be from a gigantic ichthyosaur,” explains Marcello Perillo. The young researcher has been investigating this theory as part of his Master’s Thesis in the research group headed by Prof. Martin Sander in the Institute of Geosciences at the University of Bonn. As part of his work, he examined the microstructure of the fossilized bone tissue. “Bones of similar species generally have a similar structure,” he says. “Osteohistology — the analysis of bone tissue — can thus be used to draw conclusions about the animal group from which the find originates.”

Perillo first took samples from the bones that have so far not been classified. “I compared specimens from South West England, France and Bonenburg,” he says. “They all displayed a very specific combination of properties. This discovery indicated that they might come from the same animal group.” He then used a special microscope to prove that the bone wall had a very unusual structure: It contained long strands of mineralized collagen, a protein fiber, which were interwoven in a characteristic way that had not yet been found in other bones.

Ichthyosaur bones with a similar structure

Interestingly, fossils from large ichthyosaurs from Canada also have a very similar bone wall structure. “However, this structure is not found in fossil samples from other animal groups that I have studied,” emphasized Perillo. “Therefore, it seems highly probable that the fragments in question also belong to an ichthyosaur and that the findings refute the claim that the bones come from a land-living dinosaur.”

It is likely that the fossils come from the lower jaw of a sea creature. By comparing the size of the fragments with the jaws of other species in this animal group, it is possible to deduce the length of the animals: They could possibly have reached a length of 25 to 30 meters, as proponents of the ichthyosaur theory had originally speculated in an earlier study. “However, this number is only an estimate and far from certain — until, that is, we find more complete fossil remains,” says Perillo. Nevertheless, they were certainly exceptionally large.

The first ichthyosaur lived in the ancient oceans in the early Triassic period around 250 million years ago. Species as big as whales existed early on but the largest creatures only appeared around 215 million years ago. Almost all species of ichthyosaur then died out at the end of the Triassic period more than 200 million years ago.

The unusual structure of their bone walls — which is similar to carbon fiber reinforced materials — probably kept the bone very stable while allowing for fast growth. “These huge jaws would have been exposed to strong shearing forces even when the animal was eating normally,” says Perillo. “It is possible that these animals also used their snouts to ram into their prey, similar to the orcas of today. However, this is still pure speculation at this time.”

Reference:
Marcello Perillo, P Martin Sander. The dinosaurs that weren’t: osteohistology supports giant ichthyosaur affinity of enigmatic large bone segments from the European Rhaetian. PeerJ, 2024; 12: e17060 DOI: 10.7717/peerj.17060

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

Dinosaur study challenges Bergmann’s rule

Art by James HavensNanuqsaurus, standing in the background, and pachyrhinosaurus, skull in the foreground, were among the dinosaur species included in a new study led by scientists at the University of Alaska Fairbanks and the University of Reading that calls into question Bergmann’s rule.
Art by James Havens
Nanuqsaurus, standing in the background, and pachyrhinosaurus, skull in the foreground, were among the dinosaur species included in a new study led by scientists at the University of Alaska Fairbanks and the University of Reading that calls into question Bergmann’s rule.

When you throw dinosaurs into the mix, sometimes you find that a rule simply isn’t.

A new study led by scientists at the University of Alaska Fairbanks and the University of Reading calls into question Bergmann’s rule, an 1800s-era scientific principle stating that animals in high-latitude, cooler climates tend to be larger than close relatives living in warmer climates.

The fossil record shows otherwise.

“Our study shows that the evolution of diverse body sizes in dinosaurs and mammals cannot be reduced to simply being a function of latitude or temperature,” said Lauren Wilson, a UAF graduate student and a lead author of a paper published today in the journal Nature Communications.

“We found that Bergmann’s rule is only applicable to a subset of homeothermic animals (those that maintain stable body temperatures), and only when you consider temperature, ignoring all other climatic variables. This suggests that Bergmann’s ‘rule’ is really the exception rather than the rule.”

The study started as a simple question Wilson discussed with her undergraduate advisor: Does Bergmann’s rule apply to dinosaurs?

After evaluating hundreds of data points gleaned from the fossil record, the answer seemed a solid “no.”

The dataset included the northernmost dinosaurs known to scientists, those in Alaska’s Prince Creek Formation.

They experienced freezing temperatures and snowfall. Despite this, the researchers found no notable increase in body size for any of the Arctic dinosaurs.

Next the researchers tried the same evaluation with modern mammals and birds, the descendants of prehistoric mammals and dinosaurs.

The results were largely the same: Latitude was not a predictor of body size in modern bird and mammal species.

There was a small relationship between the body size of modern birds and temperature, but the same was not the case for prehistoric birds.

The researchers say the study is a good example of how scientists can and should use the fossil record to test current-day scientific rules and hypotheses.

“The fossil record provides a window into completely different ecosystems and climate conditions, allowing us to assess the applicability of these ecological rules in a whole new way,” said Jacob Gardner, a postdoctoral researcher at the University of Reading and the other lead author of the paper.

Scientific rules should apply to fossil organisms in the same way they do modern organisms, said Pat Druckenmiller, director of the University of Alaska Museum of the North and one of the co-authors of the paper.

“You can’t understand modern ecosystems if you ignore their evolutionary roots,” he said. “You have to look to the past to understand how things became what they are today.”

Reference:
Lauren N. Wilson, Jacob D. Gardner, John P. Wilson, Alex Farnsworth, Zackary R. Perry, Patrick S. Druckenmiller, Gregory M. Erickson, Chris L. Organ. Global latitudinal gradients and the evolution of body size in dinosaurs and mammals. Nature Communications, 2024; 15 (1) DOI: 10.1038/s41467-024-46843-2

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

Early dinosaurs grew up fast, but they weren’t the only ones

Herrerasaurus ischigualastensis is an early saurischian dinosaur. It shared a bipedal, running anatomy common to large carnivorous dinosaurs that would evolve in the future, but this dinosaur lived at a time when dinosaurs were small-bodied and rare. Credit: Kristina Curry Rogers (illustration by Jordan Harris, CC-BY 4.0 (creativecommons.org/licenses/by/4.0/)
Herrerasaurus ischigualastensis is an early saurischian dinosaur. It shared a bipedal, running anatomy common to large carnivorous dinosaurs that would evolve in the future, but this dinosaur lived at a time when dinosaurs were small-bodied and rare. Credit: Kristina Curry Rogers (illustration by Jordan Harris, CC-BY 4.0 (creativecommons.org/licenses/by/4.0/)

The earliest dinosaurs had rapid growth rates, but so did many of the other animals living alongside them, according to a study published April 3, 2024 in the open-access journal PLOS ONE by Kristina Curry Rogers of Macalester College, Minnesota and colleagues.

Dinosaurs grew up fast, a feature that likely set them apart from many other animals in their Mesozoic (252 to 66 million years ago) ecosystems.

Some researchers have proposed that these elevated growth rates were key to the global success of dinosaurs, but little is known about the growth strategies of the earliest dinosaurs.

In this study, Rogers and colleagues performed histological analysis, examining patterns of bone tissue growth in the fossilized leg bones of an array of animals in one of the earliest known Mesozoic ecosystems.

The studied fossils come from the Ischigualasto Formation of Argentina and date between 231-229 million years old.

Sampled fossils include several of the earliest known dinosaurs as well as several non-dinosaur reptiles and one early relative of mammals.

The analysis found that most of the examined species had elevated growth rates, more similar to some modern-day mammals and birds than to living reptiles.

The early dinosaurs all exhibited particularly fast growth, but they weren’t alone in this, as similar growth rates were seen in several of the non-dinosaur reptiles as well.

These results show that the earliest dinosaurs were already fast growers, supporting the idea that this feature was important to their later success.

But apparently dinosaurs were only one of multiple lineages evolving with elevated growth rates during the Triassic (252-201 million years ago), suggesting that this feature is only part of the story of dinosaurs’ eventual global prosperity.

The authors note that future studies could expand on these preliminary results by sampling a wider variety of ancient animals from additional early Mesozoic fossil sites.

The authors add: “Our sample comes from a time in which dinosaurs were the new kids on the block, restricted to relatively small, basic body plans, and evolving within a world rich with a diverse array of more specialized, non-dinosaur reptiles. We tackled the question of how all of these animals grew, and found that the earliest dinosaurs grew quickly, and that these rapid growth rates probably played a significant role in dinosaurs’ subsequent ascent within Mesozoic ecosystems; but dinosaurs weren’t unique — many of their non-dino sidekicks shared rapid growth 230 million years ago.”

Reference:
Kristina Curry Rogers, Ricardo N. Martínez, Carina Colombi, Raymond R. Rogers, Oscar Alcober. Osteohistological insight into the growth dynamics of early dinosaurs and their contemporaries. PLOS ONE, 2024; 19 (4): e0298242 DOI: 10.1371/journal.pone.0298242

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

3D mouth of an ancient jawless fish suggests they were filter-feeders, not scavengers or hunters

Reconstruction of fossil fish. Credit: Richard Dearden
Reconstruction of fossil fish. Credit: Richard Dearden

Early jawless fish were likely to have used bony projections surrounding their mouths to modify the mouth’s shape while they collected food.

Experts led by the University of Birmingham have used CT scanning techniques to build up the first 3D pictures of these creatures, which are some of the earliest vertebrates (animals with backbones) in which the mouth is fossilised. Their aim was to answer questions about feeding in early vertebrates without jaws in the early Devonian epoch — sometimes called the Age of Fishes — around 400 million years ago.

Feeding behaviours are commonly used by scientists to help piece together early evolution of vertebrates, and different jaw shapes and constructions can suggest a broad range of feeding strategies. In the absence of jaws, many competing theories have been developed ranging from biting and slicing, to filtering food from sediment or water.

In a new study, published in Proceedings of the Royal Society B, an international team of palaeontologists have been able to visualise the mouth parts of one of these jawless fish, called Rhinopteraspis dunensis, in detail. The images revealed the structure and arrangement of finger-like bones that project from the lower ‘lip’ of the animal’s mouth, which the scientists believe acted to control the mouth’s size and shape as it captured food particles from surrounding water.

Senior author and project lead Dr Ivan Sansom said: “The application of CT scanning techniques to the study of fossil fish is revealing so much new information about these ancient vertebrates and giving us the opportunity to study precious and unique specimens without destructive investigation.”

Lead author Dr Richard Dearden explained: “In this case, these methods have allowed us to fit all of the small bones of this animal’s mouth together, and try and understand how it fed from this integrated system rather than by using isolated bones. Instead of a steady trend towards ‘active food acquisition’ — scavenging or hunting — we see a real diversity and range of feeding behaviours among our earliest vertebrate relatives.”

The reconstruction produced by the team shows that the bony plates around the mouth would have had limited movement, making it unlikely that the animals were hunters capable of ‘biting’. In combination with an elongated snout, they would also have found it difficult to scoop and filter sediment directly from the bottom of the sea. However these plates would have allowed it to control opening of the mouth, and perhaps strain food from water in a way also used by animals such as flamingos or oysters.

The findings offer a new perspective on theories of vertebrate evolution, since current hypotheses argue that long term evolutionary trends move from passive food consumption to increasingly predatory behaviour. In contrast, the work outlined in this paper suggests that in fact, early vertebrates had a broad range of different feeding behaviours long before jawed animals started to appear.

The study was funded by the Leverhulme Trust and is part of a collaborative project between the University of Birmingham, the Natural History Museum, and the University of Bristol, in the UK, and Naturalis Biodiversity Centre, in the Netherlands.

Early jawless fish were likely to have used bony projections surrounding their mouths to modify the mouth’s shape while they collected food.

Experts led by the University of Birmingham have used CT scanning techniques to build up the first 3D pictures of these creatures, which are some of the earliest vertebrates (animals with backbones) in which the mouth is fossilised. Their aim was to answer questions about feeding in early vertebrates without jaws in the early Devonian epoch — sometimes called the Age of Fishes — around 400 million years ago.

Feeding behaviours are commonly used by scientists to help piece together early evolution of vertebrates, and different jaw shapes and constructions can suggest a broad range of feeding strategies. In the absence of jaws, many competing theories have been developed ranging from biting and slicing, to filtering food from sediment or water.

In a new study, published in Proceedings of the Royal Society B, an international team of palaeontologists have been able to visualise the mouth parts of one of these jawless fish, called Rhinopteraspis dunensis, in detail. The images revealed the structure and arrangement of finger-like bones that project from the lower ‘lip’ of the animal’s mouth, which the scientists believe acted to control the mouth’s size and shape as it captured food particles from surrounding water.

Senior author and project lead Dr Ivan Sansom said: “The application of CT scanning techniques to the study of fossil fish is revealing so much new information about these ancient vertebrates and giving us the opportunity to study precious and unique specimens without destructive investigation.”

Lead author Dr Richard Dearden explained: “In this case, these methods have allowed us to fit all of the small bones of this animal’s mouth together, and try and understand how it fed from this integrated system rather than by using isolated bones. Instead of a steady trend towards ‘active food acquisition’ — scavenging or hunti

Senior author and project lead Dr Ivan Sansom said: “The application of CT scanning techniques to the study of fossil fish is revealing so much new information about these ancient vertebrates and giving us the opportunity to study precious and unique specimens without destructive investigation.”

Lead author Dr Richard Dearden explained: “In this case, these methods have allowed us to fit all of the small bones of this animal’s mouth together, and try and understand how it fed from this integrated system rather than by using isolated bones. Instead of a steady trend towards ‘active food acquisition’ — scavenging or hunting — we see a real diversity and range of feeding behaviours among our earliest vertebrate relatives.”

The reconstruction produced by the team shows that the bony plates around the mouth would have had limited movement, making it unlikely that the animals were hunters capable of ‘biting’. In combination with an elongated snout, they would also have found it difficult to scoop and filter sediment directly from the bottom of the sea. However these plates would have allowed it to control opening of the mouth, and perhaps strain food from water in a way also used by animals such as flamingos or oysters.

The findings offer a new perspective on theories of vertebrate evolution, since current hypotheses argue that long term evolutionary trends move from passive food consumption to increasingly predatory behaviour. In contrast, the work outlined in this paper suggests that in fact, early vertebrates had a broad range of different feeding behaviours long before jawed animals started to appear.

The study was funded by the Leverhulme Trust and is part of a collaborative project between the University of Birmingham, the Natural History Museum, and the University of Bristol, in the UK, and Naturalis Biodiversity Centre, in the Netherlands.

Early jawless fish were likely to have used bony projections surrounding their mouths to modify the mouth’s shape while they collected food.

Experts led by the University of Birmingham have used CT scanning techniques to build up the first 3D pictures of these creatures, which are some of the earliest vertebrates (animals with backbones) in which the mouth is fossilised. Their aim was to answer questions about feeding in early vertebrates without jaws in the early Devonian epoch — sometimes called the Age of Fishes — around 400 million years ago.

Feeding behaviours are commonly used by scientists to help piece together early evolution of vertebrates, and different jaw shapes and constructions can suggest a broad range of feeding strategies. In the absence of jaws, many competing theories have been developed ranging from biting and slicing, to filtering food from sediment or water.

In a new study, published in Proceedings of the Royal Society B, an international team of palaeontologists have been able to visualise the mouth parts of one of these jawless fish, called Rhinopteraspis dunensis, in detail. The images revealed the structure and arrangement of finger-like bones that project from the lower ‘lip’ of the animal’s mouth, which the scientists believe acted to control the mouth’s size and shape as it captured food particles from surrounding water.

Senior author and project lead Dr Ivan Sansom said: “The application of CT scanning techniques to the study of fossil fish is revealing so much new information about these ancient vertebrates and giving us the opportunity to study precious and unique specimens without destructive investigation.”

Lead author Dr Richard Dearden explained: “In this case, these methods have allowed us to fit all of the small bones of this animal’s mouth together, and try and understand how it fed from this integrated system rather than by using isolated bones. Instead of a steady trend towards ‘active food acquisition’ — scavenging or hunting — we see a real diversity and range of feeding behaviours among our earliest vertebrate relatives.”

The reconstruction produced by the team shows that the bony plates around the mouth would have had limited movement, making it unlikely that the animals were hunters capable of ‘biting’. In combination with an elongated snout, they would also have found it difficult to scoop and filter sediment directly from the bottom of the sea. However these plates would have allowed it to control opening of the mouth, and perhaps strain food from water in a way also used by animals such as flamingos or oysters.

The findings offer a new perspective on theories of vertebrate evolution, since current hypotheses argue that long term evolutionary trends move from passive food consumption to increasingly predatory behaviour. In contrast, the work outlined in this paper suggests that in fact, early vertebrates had a broad range of different feeding behaviours long before jawed animals started to appear.

The study was funded by the Leverhulme Trust and is part of a collaborative project between the University of Birmingham, the Natural History Museum, and the University of Bristol, in the UK, and Naturalis Biodiversity Centre, in the Netherlands.

Reference:
Richard P. Dearden, Andy S. Jones, Sam Giles, Agnese Lanzetti, Madleen Grohganz, Zerina Johanson, Stephan Lautenschlager, Emma Randle, Philip C. J. Donoghue, Ivan J. Sansom. The three-dimensionally articulated oral apparatus of a Devonian heterostracan sheds light on feeding in Palaeozoic jawless fishes. Proceedings of the Royal Society B: Biological Sciences, 2024; 291 (2019) DOI: 10.1098/rspb.2023.2258

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

Related Articles