WFS News: Gualicho shinyae , Another Dinosaur with Short Arms

No one is sure what, exactly, Tyrannosaurus rex did with its short arms. But Argentinian and American scientists have discovered a new dinosaur species that had the same puzzling feature, they reported this week (July 13) in PLOS One.

Gualicho shinyae, whose 90 million-year-old fossil remains were found in Patagonia, Argentina, was 25 feet long and weighed about a ton—roughly the same size as a polar bear. Yet, full grown, this predator had arms the size of a child’s, New Scientist reported.

G. shinyae and T. rex stem from different evolutionary branches. T. rex’s earliest ancestors had arms that were actually long, study coauthor Peter Makovicky, a paleontologist at the Field Museum of Natural History in Chicago, told The New York Times.But for some reason, T. rex evolved to have stubby arms. Because this trait appears to have arisen independently in G. shinyae and T. rex, they may have served a purpose, according to Makovicky.

Another Dinosaur with Short Arms

Another Dinosaur with Short Arms

Scientists still don’t know what that purpose may have been. But theropods—a group of two-legged, flesh-eating dinosaurs—have been known to have forelimbs of questionable utility, Popular Science noted.

“There are a lot of different groups of theropods that tend to reduce the size of their hands and their arms or change the way that they’re used,” Lindsay Zanno, head of the North Carolina Museum of Natural Sciences’ Paleontology Research Lab who was not involved in the study, told The Christian Science Monitor.

“We don’t actually know what would have triggered a reduction in the forelimb in each individual lineage,” Makovicky told The New York Times. “But obviously there was some adaptive advantage because we see it multiple times in different lineages of theropods.”

Citation: Article  By Alison F. Takemura

Key: WFS,World Fossil Society,Riffin T Sajeev,Russel T Sajeev

WFS News: Dinosaur tail complete with its feathers trapped in a piece of amber

Researchers from China, Canada, and the University of Bristol have discovered a dinosaur tail complete with its feathers trapped in a piece of amber.The finding reported today in Current Biology helps to fill in details of the dinosaurs’ feather structure and evolution, which can’t be surmised from fossil evidence.

Photomicrographs and SR X-Ray μCT Reconstructions of DIP-V-15103 (A) Dorsolateral overview. (B) Ventrolateral overview with decay products (bubbles in foreground, staining to lower right). (C) Caudal exposure of tail showing darker dorsal plumage (top), milky amber, and exposed carbon film around vertebrae (center). (D–H) Reconstructions focusing on dorsolateral, detailed dorsal, ventrolateral, detailed ventral, and detailed lateral aspects of tail, respectively. Arrowheads in (A) and (D) mark rachis of feather featured in Figure 4A. Asterisks in (A) and (C) indicate carbonized film (soft tissue) exposure. Arrows in (B) and (E)–(G) indicate shared landmark, plus bubbles exaggerating rachis dimensions; brackets in (G) and (H) delineate two vertebrae with clear transverse expansion and curvature of tail at articulation. Abbreviations for feather rachises: d, dorsal; dl, dorsalmost lateral; vl, ventralmost lateral; v, ventral. Scale bars, 5 mm in (A), (B), (D), and (F) and 2 mm in (C), (E), (G), and (H). See also Figure S2.

Photomicrographs and SR X-Ray μCT Reconstructions of DIP-V-15103
(A) Dorsolateral overview.
(B) Ventrolateral overview with decay products (bubbles in foreground, staining to lower right).
(C) Caudal exposure of tail showing darker dorsal plumage (top), milky amber, and exposed carbon film around vertebrae (center).
(D–H) Reconstructions focusing on dorsolateral, detailed dorsal, ventrolateral, detailed ventral, and detailed lateral aspects of tail, respectively.
Arrowheads in (A) and (D) mark rachis of feather featured in Figure 4A. Asterisks in (A) and (C) indicate carbonized film (soft tissue) exposure. Arrows in (B) and (E)–(G) indicate shared landmark, plus bubbles exaggerating rachis dimensions; brackets in (G) and (H) delineate two vertebrae with clear transverse expansion and curvature of tail at articulation. Abbreviations for feather rachises: d, dorsal; dl, dorsalmost lateral; vl, ventralmost lateral; v, ventral. Scale bars, 5 mm in (A), (B), (D), and (F) and 2 mm in (C), (E), (G), and (H). See also Figure S2.

While the feathers aren’t the first to be found in amber, earlier specimens have been difficult to definitively link to their source animal, the researchers say.WFS News:Ryan McKellar, from the Royal Saskatchewan Museum in Canada, said: “The new material preserves a tail consisting of eight vertebrae from a juvenile; these are surrounded by feathers that are preserved in 3D and with microscopic detail.

“We can be sure of the source because the vertebrae are not fused into a rod or pygostyle as in modern birds and their closest relatives. Instead, the tail is long and flexible, with keels of feathers running down each side. In other words, the feathers definitely are those of a dinosaur not a prehistoric bird.”

SR μ-XFI Maps and Scanning Electron Micrographs of DIP-V-15103 (A) Elemental maps and region of interest (ROI) image for exposed soft tissue preservation in DIP-V-15103; black carbon film surrounds clay minerals infilling void between vertebrae or partially replacing them; milky amber related to decay surrounds vertebrae and plumage (ROI prior to clay flake removal is better visible in Figure S3H). (B) Patchy keratin preservation with traces of fibrous structure in DIP-V-15103 ventral feather. (C) Fibrous keratin sheets and isolated melanosomes from barb of modern Indian peafowl (Pavo cristatus; Galliformes). Scale bars, 2 mm in (A) and 1 μm in (B) and (C). See also Figure S3.

SR μ-XFI Maps and Scanning Electron Micrographs of DIP-V-15103
(A) Elemental maps and region of interest (ROI) image for exposed soft tissue preservation in DIP-V-15103; black carbon film surrounds clay minerals infilling void between vertebrae or partially replacing them; milky amber related to decay surrounds vertebrae and plumage (ROI prior to clay flake removal is better visible in Figure S3H).
(B) Patchy keratin preservation with traces of fibrous structure in DIP-V-15103 ventral feather.
(C) Fibrous keratin sheets and isolated melanosomes from barb of modern Indian peafowl (Pavo cristatus; Galliformes).Scale bars, 2 mm in (A) and 1 μm in (B) and (C). See also Figure S3.

The study’s first author Lida Xing from the China University of Geosciences in Beijing discovered the remarkable specimen at an amber market in Myitkyina, Myanmar in 2015.

The amber piece was originally seen as some kind of plant inclusion and destined to become a curiosity or piece of jewellery, but Xing recognized its potential scientific importance and suggested the Dexu Institute of Palaeontology buy the specimen.

The researchers say the specimen represents the feathered tail of a theropod preserved in mid-Cretaceous amber about 99 million years ago. While it was initially difficult to make out details of the amber inclusion, Xing and his colleagues relied on CT scanning and microscopic observations to get a closer look.

Photomicrographs of DIP-V-15103 Plumage (A) Pale ventral feather in transmitted light (arrow indicates rachis apex). (B) Dark-field image of (A), highlighting structure and visible color. (C) Dark dorsal feather in transmitted light, apex toward bottom of image. (D) Base of ventral feather (arrow) with weakly developed rachis. (E) Pigment distribution and microstructure of barbules in (C), with white lines pointing to pigmented regions of barbules. (F–H) Barbule structure variation and pigmentation, among barbs, and ‘rachis’ with rachidial barbules (near arrows); images from apical, mid-feather, and basal positions respectively. Scale bars, 1 mm in (A), 0.5 mm in (B)–(E), and 0.25 mm in (F)–(H). See also Figure S4.

Photomicrographs of DIP-V-15103 Plumage
(A) Pale ventral feather in transmitted light (arrow indicates rachis apex).
(B) Dark-field image of (A), highlighting structure and visible color.
(C) Dark dorsal feather in transmitted light, apex toward bottom of image.
(D) Base of ventral feather (arrow) with weakly developed rachis.
(E) Pigment distribution and microstructure of barbules in (C), with white lines pointing to pigmented regions of barbules.
(F–H) Barbule structure variation and pigmentation, among barbs, and ‘rachis’ with rachidial barbules (near arrows); images from apical, mid-feather, and basal positions respectively.
Scale bars, 1 mm in (A), 0.5 mm in (B)–(E), and 0.25 mm in (F)–(H). See also Figure S4.

The feathers suggest the tail had a chestnut-brown upper surface and a pale or white underside. The specimen also offers insight into feather evolution. The feathers lack a well-developed central shaft or rachis. Their structure suggests that the two finest tiers of branching in modern feathers, known as barbs and barbules, arose before a rachis formed.

Professor Mike Benton from the School of Earth Sciences at the University of Bristol, added: “It’s amazing to see all the details of a dinosaur tail — the bones, flesh, skin, and feathers — and to imagine how this little fellow got his tail caught in the resin, and then presumably died because he could not wrestle free.

“There’s no thought that dinosaurs could shed their tails, as some lizards do today.”

DIP-V-15103 Structural Overview and Feather Evolutionary-Developmental Model Fit (A and B) Overview of largest and most planar feather on tail (dorsal series, anterior end), with matching interpretive diagram of barbs and barbules. Barbules are omitted on upper side and on one barb section (near black arrow) to show rachidial barbules and structure; white arrow indicates follicle. (C) Evolutionary-developmental model and placement of new amber specimen. Brown denotes calamus, blue denotes barb ramus, red denotes barbule, and purple denotes rachis [as in 5, 12]. Scale bars, 1 mm in (A) and (B).

DIP-V-15103 Structural Overview and Feather Evolutionary-Developmental Model Fit
(A and B) Overview of largest and most planar feather on tail (dorsal series, anterior end), with matching interpretive diagram of barbs and barbules. Barbules are omitted on upper side and on one barb section (near black arrow) to show rachidial barbules and structure; white arrow indicates follicle.
(C) Evolutionary-developmental model and placement of new amber specimen. Brown denotes calamus, blue denotes barb ramus, red denotes barbule, and purple denotes rachis [as in 5, 12].
Scale bars, 1 mm in (A) and (B).

The researchers also examined the chemistry of the tail inclusion where it was exposed at the surface of the amber. The analysis shows that the soft tissue layer around the bones retained traces of ferrous iron, a relic left over from haemoglobin that was also trapped in the sample.The findings show the value of amber as a supplement to the fossil record. Ryan McKellar added: “Amber pieces preserve tiny snapshots of ancient ecosystems, but they record microscopic details, three-dimensional arrangements, and labile tissues that are difficult to study in other settings.

“This is a new source of information that is worth researching with intensity, and protecting as a fossil resource.”

The researchers say they are now “eager to see how additional finds from this region will reshape our understanding of plumage and soft tissues in dinosaurs and other vertebrates.”

Citation:Lida Xing, Ryan C. McKellar, Xing Xu, Gang Li, Ming Bai, W. Scott Persons IV, Tetsuto Miyashita, Michael J. Benton, Jianping Zhang, Alexander P. Wolfe, Qiru Yi, Kuowei Tseng, Hao Ran, Philip J. Currie. A Feathered Dinosaur Tail with Primitive Plumage Trapped in Mid-Cretaceous Amber. Current Biology, 2016; DOI: 10.1016/j.cub.2016.10.008

Key: WFS,World Fossil Society,Riffin T Sajeev,Russel T Sajeev

WFS News: Popcorn-rocks solve the mystery of the magma chambers

Since the 18th century, geologists have struggled to explain how big magma chambers form in Earth’s crust. In particular, it has been difficult to explain where the surrounding rock goes when the magma intrudes. Now a team of researchers from Uppsala University and the Goethe University in Frankfurt have found the missing rocks — and they look nothing like what they expected.

Researchers have previously proposed that the roofs and walls of magma chamber were either melted and assimilated into the magma, or that they would sink to the bottom of the magma chamber. However, enough evidence for either of these hypotheses have not been forthcoming, and researchers now propose a third possibility.

When rock fragments fall into the magma chamber, all fluids inside boil instantly. This is similar to what happens when a grain of corn turns into popcorn. Credit: Börje Dahrén

When rock fragments fall into the magma chamber, all fluids inside boil instantly. This is similar to what happens when a grain of corn turns into popcorn. Credit: Börje Dahrén

“We show that rock fragments from the roof of the magma chambers could have been expelled, similar to popcorn that is thrown out of a hot pan! We have found them in rocks that have been ejected in volcanic eruptions. The rock fragments are full of bubbles and have very low densities, and they look a lot like popcorn,” says Steffi Burchardt, researcher at the Department of Earth Sciences, Uppsala University.

When rock fragments fall into the magma chamber, they are rapidly heated by several hundred degrees, and all fluids inside boil instantly. This is similar to what happens when a grain of corn is put into the pan and the water inside boils — and we get popcorn.

Appearance and structure of examples of frothy xenolith fragments.

Appearance and structure of examples of frothy xenolith fragments.

Steffi and her colleagues have now managed to show how the popcorn-effect makes the rock fragments float and rise to the top of magma chambers rather than sink to the bottom. The floating rock fragments are then found among the erupted volcanic rocks, instead of inside the frozen magma chambers as previously expected. Furthermore, the gases released from the rock fragments as they boil also contribute to a higher pressure in the magma which can help explain some of the more explosive eruptions.

Appearance and structure of a frothy sandstone xenolith sample from the 2011 offshore eruption at El Hierro, Canary Islands, Spain

Appearance and structure of a frothy sandstone xenolith sample from the 2011 offshore eruption at El Hierro, Canary Islands, Spain

“Sometimes you can find the solution to age-old puzzles by looking in new places — in this case literally looking outside the box! The frozen magma chambers proved to be the wrong place to look,” Steffi explains.

Model results of thermomechanical processes associated with a xenolith sinking in a granitic magma chamber.

Model results of thermomechanical processes associated with a xenolith sinking in a granitic magma chamber.

Journal Reference:Steffi Burchardt, Valentin R. Troll, Harro Schmeling, Hemin Koyi, Lara Blythe. Erupted frothy xenoliths may explain lack of country-rock fragments in plutons. Scientific Reports, 2016; 6: 34566 DOI: 10.1038/srep34566

Citation:Uppsala Universitet. “Popcorn-rocks solve the mystery of the magma chambers.” ScienceDaily. ScienceDaily, 2 November 2016. <www.sciencedaily.com/releases/2016/11/161102080013.htm>.

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WFS News:New study describes 200 million years of geological evolution

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200 million years of geological evolution of a fault in Earth’s crust has recently been dated. Published in Nature Communications, these new findings may be used to shed light on poorly understood pathways for methane release from the heart of our planet.

Tectonic plates, big sections of Earth’s crust and blocks underneath them, are constantly moving. The areas where these sections meet and interact are called faults. They appear as scars on the outermost layer of Earth. A lot is going on along the largest of faults: mountains can grow, volcanoes can erupt, continents can separate and earthquakes happen.

Fault zone in Southern Norway shows 200 million years of reactivation history. Credit: Giulio Viola

                                  Fault zone in Southern Norway shows 200 million years of reactivation history.Credit: Giulio Viola

Also more discrete events are constantly happening close to faults: The emission of the greenhouse gas methane from ocean floor commonly occurs in gas hydrate provinces along tectonically active continental margins.

Active methane seepage happening frequently This is what makes brittle faults particularly alluring for CAGE/NGU researcher Jochen Knies. He is one of the coauthors of a new study in Nature Communications that, for the first time, precisely dates the evolution of a brittle fault from its initial formation to its later reactivation.

Brittle faults may be important because they open up pathways along which methane, released from the reservoirs deep under Earth’s crust, can migrate to shallower depths or even into the ocean itself.

(a) Location map of the study area in western Norway. Arrow indicates Goddo Island. (b) Hill-shaded LiDAR digital elevation model (DEM) of the southeasternmost Goddo Island illuminated from the northeast. Red line: trace of the Goddo Fault. (c) Stress tensor derived from the inversion of the quartz (±hematite) striated Goddo Fault principal slip surface (black great circles) and older, reactivated NW-SE-striking epidote-coated strike-slip faults (red great circles; equal area, lower hemisphere projection; inversion run with Win-Tensor60). E-W extension is indicated.

(a) Location map of the study area in western Norway. Arrow indicates Goddo Island. (b) Hill-shaded LiDAR digital elevation model (DEM) of the southeasternmost Goddo Island illuminated from the northeast. Red line: trace of the Goddo Fault. (c) Stress tensor derived from the inversion of the quartz (±hematite) striated Goddo Fault principal slip surface (black great circles) and older, reactivated NW-SE-striking epidote-coated strike-slip faults (red great circles; equal area, lower hemisphere projection; inversion run with Win-Tensor60). E-W extension is indicated.

“Active methane leakage from the sea floor happens episodically, and frequently. Some seeps activate annually, others become active on a millennial scale. We need to better identify and characterize timing and duration of these leaks. It is critical for our understanding of the role the natural gas emissions play on global climate.” says Jochen Knies, researcher at CAGE/NGU.

The story of the faults is the story of methane release Methane is a very potent greenhouse gas. The impacts of the industrial and agricultural release of the gas are well known and mapped. But the effects and quantities of the natural release of the gas, especially from the ocean floor, are poorly understood. Recent studies show that this natural release has been heavily underestimated.

The Nature Communications study focuses on brittle faults and fractures onshore in western Norway. Up to now, applications for directly fingerprinting the age of brittle faulting and reactivation — and thus potentially the timing of gas emission through the crust — did not exist.

(a) Sharp principal slip surface (PSS) overlain by 0.5–1 m of cataclasite (orange stripe). T. Scheiber for scale. (b) PSS overlain by greenish clay-rich gouge (sample BO-GVI-1) and phyllonite (sample BO-GVI-2), indicating top-to-the-E extensional kinematics. Hammer for scale. (c) Example of quartz (±hematite) striated PSS. (d) Example of pre-extension steeply dipping strike-slip fault plane, with steeper quartz striations (red) overprinting earlier and flatter epidote striae (blue). (e) Black dashed lines define the NNE-SSW fracture corridor dissecting the Goddo Fault PSS. (f) Sampling site for sample BO-OFR-1 consisting of strongly altered granodiorite. Note the subrounded shape of the granodiorite altered knobs, reminiscent of core stone formation and incipient saprolitization. Note spatula for scale (c. 200 mm long) in the upper part of the outcrop.

(a) Sharp principal slip surface (PSS) overlain by 0.5–1 m of cataclasite (orange stripe). T. Scheiber for scale. (b) PSS overlain by greenish clay-rich gouge (sample BO-GVI-1) and phyllonite (sample BO-GVI-2), indicating top-to-the-E extensional kinematics. Hammer for scale. (c) Example of quartz (±hematite) striated PSS. (d) Example of pre-extension steeply dipping strike-slip fault plane, with steeper quartz striations (red) overprinting earlier and flatter epidote striae (blue). (e) Black dashed lines define the NNE-SSW fracture corridor dissecting the Goddo Fault PSS. (f) Sampling site for sample BO-OFR-1 consisting of strongly altered granodiorite. Note the subrounded shape of the granodiorite altered knobs, reminiscent of core stone formation and incipient saprolitization. Note spatula for scale (c. 200 mm long) in the upper part of the outcrop.

“We have managed to precisely date several episodes of faulting and reactivation of brittle faults onshore Norway. Our study unravels and dates a complex evolution of the local brittle deformation, which straddles a 200 million year timespan.” says Giulio Viola, the lead-author of the study .

The onshore study gives scientists the necessary tools to understand the age of offshore faults, which are important for methane release from gas hydrate provinces.

Improving the models and estimates of methane release The innovative method behind the study combines a twofold approach: the detailed structural analysis of faults, and the dating of their history by applying potassium/argon dating of the clay mineral illite. The faulting causes deformations in which illite can form, and just a few milligrams of the clay mineral are enough to do this type of dating.

“Testing this toolbox on fault and fracture systems below active sites of methane leakages, would potentially provide an innovative and unique possibility: By constraining the timing of offshore faulting episodes, we may ultimately be able to identify the events of increased methane emission to the ocean and atmosphere. These episodes are not something that is restricted to the past. They are happening now, and will be happening frequently in the future,” concludes Knies.

Each of the represented stages was characterized by illite authigenesis. Selective preservation within the fault core of structural domains representative of all deformation stages made it possible to separate, characterize and date three different illite generations (illite colour: yellow: sample BO-GVI-2; orange: sample BO-GVI-1; red: sample BO-OFR-1) and to deconvolute the complex and long-lasting evolution of the Goddo Fault archive. (a) Permian faulting led to a phyllonitic, N-S trending normal fault that accommodated overall E-W to ESE-WNW extension. (b) Coaxial extension continued through the Triassic and into the Jurassic. By then the faulting style was entirely brittle with gouge formation and localized slip along a striated PSS. (c) The far-field stress effects related to NW-SE extension along the Mid-Norwegian margin caused localized fracturing, dilation, significant fluid ingress and fluid-rock interaction, leading to Early Cretaceous authigenesis of a third illite generation.

Each of the represented stages was characterized by illite authigenesis. Selective preservation within the fault core of structural domains representative of all deformation stages made it possible to separate, characterize and date three different illite generations (illite colour: yellow: sample BO-GVI-2; orange: sample BO-GVI-1; red: sample BO-OFR-1) and to deconvolute the complex and long-lasting evolution of the Goddo Fault archive. (a) Permian faulting led to a phyllonitic, N-S trending normal fault that accommodated overall E-W to ESE-WNW extension. (b) Coaxial extension continued through the Triassic and into the Jurassic. By then the faulting style was entirely brittle with gouge formation and localized slip along a striated PSS. (c) The far-field stress effects related to NW-SE extension along the Mid-Norwegian margin caused localized fracturing, dilation, significant fluid ingress and fluid-rock interaction, leading to Early Cretaceous authigenesis of a third illite generation.

The method and the findings may also improve current models that estimate the amounts of methane released from natural sources.

Citation: University of Tromso (Universitetet i Tromsø – UiT). “New study describes 200 million years of geological evolution.” ScienceDaily.

Key: WFS,World Fossil Society,Riffin T Sajeev,Russel T sajeev

WFS News: Earth’s deepest forearc basin discovered

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Geologists have for the first time seen and documented the Banda Detachment fault in eastern Indonesia and worked out how it formed.

Lead researcher Dr Jonathan Pownall from The Australian National University (ANU) said the find will help researchers assess dangers of future tsunamis in the area, which is part of the Ring of Fire — an area around the Pacific Ocean basin known for earthquakes and volcanic eruptions.

“The abyss has been known for 90 years but until now no one has been able to explain how it got so deep,” Dr Pownall said.

“Our research found that a 7 km-deep abyss beneath the Banda Sea off eastern Indonesia was formed by extension along what might be Earth’s largest-identified exposed fault plane.”

Geologists have for the first time seen and documented the Banda Detachment fault in eastern Indonesia and worked out how it formed. Credit: Image courtesy of Australian National UniversityClose

Geologists have for the first time seen and documented the Banda Detachment fault in eastern Indonesia and worked out how it formed.Credit: Image courtesy of Australian National University

By analysing high-resolution maps of the Banda Sea floor, geologists from ANU and Royal Holloway University of London found the rocks flooring the seas are cut by hundreds of straight parallel scars.

These wounds show that a piece of crust bigger than Belgium or Tasmania must have been ripped apart by 120 km of extension along a low-angle crack, or detachment fault, to form the present-day ocean-floor depression.

Dr Pownall said this fault, the Banda Detachment, represents a rip in the ocean floor exposed over 60,000 square kilometres.

“The discovery will help explain how one of Earth’s deepest sea areas became so deep,” he said.

Professor Gordon Lister also from the ANU Research School of Earth Sciences said this was the first time the fault has been seen and documented by researchers.

“We had made a good argument for the existence of this fault we named the Banda Detachment based on the bathymetry data and on knowledge of the regional geology,” said Professor Lister.

Dr Pownall said he was on a boat journey in eastern Indonesia in July when he noticed the prominent landforms consistent with surface extensions of the fault line.

“I was stunned to see the hypothesised fault plane, this time not on a computer screen, but poking above the waves,” said Dr Pownall.

He said rocks immediately below the fault include those brought up from the mantle.

“This demonstrates the extreme amount of extension that must have taken place as the oceanic crust was thinned, in some places to zero,” he said.

Dr Pownall also said the discovery of the Banda Detachment fault would help assesses dangers of future tsunamis and earthquakes.

“In a region of extreme tsunami risk, knowledge of major faults such as the Banda Detachment, which could make big earthquakes when they slip, is fundamental to being able to properly assess tectonic hazards,” he said.

Citation:Australian National University. “Biggest exposed fault on Earth discovered.” ScienceDaily. ScienceDaily, 28 November 2016. <www.sciencedaily.com/releases/2016/11/161128132928.htm>

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WFS News: X-raying the Earth with waves from stormy weather bomb

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Using a detection network based in Japan, scientists have uncovered a rare type of deep-earth tremor that they attribute to a distant North Atlantic storm called a “weather bomb.”

The discovery marks the first time scientists have observed this particular tremor, known as an S wave microseism. And, as Peter Gerstoft and Peter D. Bromirski write in a related Perspective, their observation “gives seismologists a new tool with which to study Earth’s deeper structure,” one that will contribute to a clearer picture of Earth’s movements, even those originating from the atmosphere-ocean system.

Faint tremors called microseisms are phenomena caused by the sloshing of the ocean’s waves on the solid Earth floor during storms. Detectable anywhere in the world, microseisms can be various waveforms that move through the Earth’s surface and interior, respectively.

An Atlantic "weather bomb," or a severe, fast-developing storm, causes ocean swells that incite faint and deep tremors into the oceanic crust. These subtle waves run through the earth and can be detected in places as far away as Japan, where facilities using a method called "Hi-net" measure the amplitude of the storm's P and S waves for the first time. Credit: Kiwamu Nishida and Ryota Takagi

An Atlantic “weather bomb,” or a severe, fast-developing storm, causes ocean swells that incite faint and deep tremors into the oceanic crust. These subtle waves run through the earth and can be detected in places as far away as Japan, where facilities using a method called “Hi-net” measure the amplitude of the storm’s P and S waves for the first time.Credit: Kiwamu Nishida and Ryota Takagi

So far, however, scientists analyzing microseismic activity in the Earth have only been able to chart P waves (those that animals can feel before an earthquake), and not their more elusive S wave counterpart (those that humans feel during earthquakes).

Here, using 202 Hi-net stations operated by the National Research Institute for Earth Science and Disaster Prevention in Japan’s Chugoku district, Kiwamu Nishida and Ryota Takagi successfully detected not only P wave microseisms triggered by a severe and distant North Atlantic storm, known as a weather bomb, but also S wave microseisms, too.

What’s more, the authors determined both the direction and distance to these waves’ origins, providing insight into their paths as well as the earthly structures through which they traveled. In this way, the seismic energy travelling from this weather bomb storm through the Earth illuminated many dark patches of its interior. Nishida and Takagi’s findings not only offer a new means by which to explore the Earth’s internal structure, but they may also contribute to more accurate detection of earthquakes and oceanic storms.

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Ref: K. Nishida, R. Takagi. Teleseismic S wave microseisms. Science, 2016; 353 (6302): 919 DOI: 10.1126/science.aaf7573

Citaion:American Association for the Advancement of Science. “X-raying the Earth with waves from stormy weather ‘bombs’.” ScienceDaily. ScienceDaily, 25 August 2016. <www.sciencedaily.com/releases/2016/08/160825151609.htm>.

WFS News: Keratin and melanosomes preserved in 130-million-year-old bird fossil Eoconfuciusornis

New research from North Carolina State University, the Chinese Academy of Sciences and Linyi University has found evidence of original keratin and melanosome preservation in a 130-million-year-old Eoconfuciusornis specimen. The work extends the timeframe in which original molecules may preserve, and demonstrates the ability to distinguish between ancient microstructures in fossils.

Eoconfuciusornis, crow-sized primitive birds that lived in what is now China around 130 million years ago, are the earliest birds to have a keratinous beak and no teeth, like modern birds. Previous studies argued that the feathers of these and other ancient birds and dinosaurs preserved small, round structures interpreted to be melanosomes — pigment-containing organelles that, along with other pigments, give feathers their color. However, without additional evidence, it was not possible to prove that these structures weren’t just microbes that had coated the feather during decomposition and fossilization.

Eoconfuciusornis. Credit: Dr. Xiaoli Wang

   Eoconfuciusornis.   Credit: Dr. Xiaoli Wang

Yanhong Pan, associate research fellow at the Chinese Academy of Sciences and corresponding author of a paper describing the research and co-author Mary Schweitzer, NC State professor of biology with a joint appointment at the North Carolina Museum of Natural Sciences, examined feathers from an Eoconfuciusornisspecimen taken from the Jehol Biota site in northern China, which is renowned for excellent fossil preservation.

“If these small bodies are melanosomes, they should be embedded in a keratinous matrix, since feathers contain beta-keratin,” Schweitzer says. “If we couldn’t find the keratin, then those structures could as easily be microbes, or a mix of microbes and melanosomes — in either case, predictions of dinosaur shading would not be accurate.”

Pan, Schweitzer and their team used both scanning and transmission electron microscopy to get microscopic details of the feather’s surface and its internal structure. They also utilized immunogold labeling — in which gold particles are attached to antibodies that bind to particular proteins in order to make them visible in electron microscopy — to show that filaments within the feathers were keratin.

Finally, they mapped copper and sulfur to these feathers at high resolution. Sulfur was broadly distributed, reflecting its presence in both keratin and melanin molecules in modern feathers. However copper, which is only found in modern melanosomes, and not part of keratin, was only observed in the fossil melanosomes. These findings both support the identity of the melanosomes and indicate that there was no mixing or leaching during decomposition and fossilization.

“This study is the first to demonstrate evidence for both keratin and melanosomes, using structural, chemical and molecular methods,” says Pan. “These methods have the potential to help us understand — on the molecular level — how and why feathers evolved in these lineages.”

Citation:North Carolina State University. “Keratin and melanosomes preserved in 130-million-year-old bird fossil.” ScienceDaily. ScienceDaily, 21 November 2016.

Key: WFS,World Fossil Society,Riffin T Sajeev,Russel T Sajeev

WFS News: Asteroid impacts could create niches for early life

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Scientists studying the Chicxulub crater have shown how large asteroid impacts deform rocks in a way that may produce habitats for early life.

Around 65 million years ago a massive asteroid crashed into the Gulf of Mexico causing an impact so huge that the blast and subsequent knock-on effects wiped out around 75 per cent of all life on Earth, including most of the dinosaurs. This is known as the Chicxulub impact.

Split drill cores collected from the peak ring of Chicxulub crater. The left two cores consist of basement granite. The right two cores are impact melt rocks that were created by the heat associated with the impact. Credit: E. Le Ber

Split drill cores collected from the peak ring of Chicxulub crater. The left two cores consist of basement granite. The right two cores are impact melt rocks that were created by the heat associated with the impact.Credit: E. Le Ber

In April and May 2016, an international team of scientists undertook an offshore expedition and drilled into part of the Chicxulub impact crater. Their mission was to retrieve samples from the rocky inner ridges of the crater — known as the ‘peak ring’ — drilling 506 to 1335 metres below the modern day sea floor to understand more about the ancient cataclysmic event.

Now, the researchers have carried out the first analysis of the core samples. They found that the impact millions of years ago deformed the peak ring rocks in such a way that it made them more porous, and less dense, than any models had previously predicted.

Porous rocks provide niches for simple organisms to take hold, and there would also be nutrients available in the pores, from circulating water that would have been heated inside the Earth’s crust. Early Earth was constantly bombarded by asteroids, and the team have inferred that this bombardment must have also created other rocks with similar physical properties. This may partly explain how life took hold on Earth.

The study, which is published today in the journal Science, also confirmed a model for how peak rings were formed in the Chicxulub crater, and how peak rings may be formed in craters on other planetary bodies.

The team’s new work has confirmed that the asteroid, which created the Chicxulub crater, hit the Earth’s surface with such a force that it pushed rocks, which at that time were ten kilometres beneath the surface, farther downwards and then outwards. These rocks then moved inwards again towards the impact zone and then up to the surface, before collapsing downwards and outwards again to form the peak ring. In total they moved an approximate total distance of 30 kilometres in a matter of a few minutes.

Professor Joanna Morgan, lead author of the study from the Department of Earth Science and Engineering, said: “It is hard to believe that the same forces that destroyed the dinosaurs may have also played a part, much earlier on in Earth’s history, in providing the first refuges for early life on the planet. We are hoping that further analyses of the core samples will provide more insights into how life can exist in these subterranean environments.”

The next steps will see the team acquiring a suite of detailed measurements from the recovered core samples to refine their numerical simulations. Ultimately, the team are looking for evidence of modern and ancient life in the peak-ring rocks. They also want to learn more about the first sediments that were deposited on top of the peak ring, which could tell the researchers if they were deposited by a giant tsunami, and provide them with insights into how life recovered, and when life actually returned to this sterilised zone after the impact.

Key:WFS,World Fossil Society,Riffin T Sajeev,Russel T sajeev

Citation:Imperial College London. “Asteroid impacts could create niches for early life, suggests Chicxulub crater study.” ScienceDaily. ScienceDaily, 17 November 2016.

WFS News: This oviraptorosaur may have met its end in a Chinese slush pit

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The workmen were building a high school, blasting out the site with dynamite in the southern Chinese city of Ganzhou when they saw it: the newly exposed fossil of a small, child-sized dinosaur. It was well preserved despite the construction, and it struck a curious pose: head elevated, neck arching upward, limbs splayed out to the side. The roughly meter-long fossil, researchers say today in Scientific Reports, represents a new species of oviraptorosaur, a group of feathered, birdlike dinosaurs that rapidly diversified in the few million years before an asteroid impact wiped out the dinosaurs 66 million years ago. Oviraptorosaurs inhabited much of the Northern Hemisphere, but they seem to have flourished in what is now Ganzhou. The new species, dubbed Tongtianlong limosus (or “muddy dragon on the road to heaven”), marks the sixth species of oviraptorosaur found in the Ganzhou area. T. limosus has slightly different skull features from its brethren, but a similarly short, deep, skull and a beak rather than teeth. Cretaceous-era Ganzhou was a hot, humid jungle with towering plants and the occasional mud pit, a richly diverse environment home to everything from duck-billed dinosaurs to long-nosed tyrannosaurs. Still, T. limosus may have met a sad end between 66 million and 72 million years ago: Its reaching neck and outstretched limbs hint at the final struggles of a creature hopelessly mired in mud.

Tongtianlong limosus (or “muddy dragon on the road to heaven”)

Tongtianlong limosus (or “muddy dragon on the road to heaven”)

 

Source: Article By Carolyn Gramling,Science mag.

Key: WFS,World Fossil Society,Riffin T Sajeev,Russel T sajeev

WFS News: Dinosaurs’ rise was ‘more gradual’

Researchers have discovered two small dinosaurs together with a lagerpetid, a group of animals that are recognized as precursors of dinosaurs. The discovery made in Brazil and reported in the Cell Press journal Current Biology on November 10 represents the first time that a dinosaur and a dinosaur precursor have ever been found together.

The new lagerpetid (Ixalerpeton) and saurischian dinosaur (Buriolestes) were unearthed from the ~230-million-year-old Carnian Santa Maria Formation — one of the oldest known rock units including dinosaur fossils anywhere in the world.

The skull of Buriolestes. Credit: Cabreira et al.

   The skull of Buriolestes.Credit: Cabreira et al.

“We now know for sure that dinosaurs and dinosaur precursors lived alongside one another and that the rise of dinosaurs was more gradual, not a fast overtaking of other animals of the time,” says Max Langer of Brazil’s Universidade de São Paulo.

The discovery clearly shows that these animals were contemporaries of each other during the earliest stages of dinosaurs’ evolution. The new lagerpetid specimen also preserves the first skull, scapular, and forelimb elements, plus associated vertebrae, known for the group, the researchers report. Tooth evidence also shows that the first dinosaurs most likely fed on “all kinds of small animals, but most probably not plants,” Langer says.

Those details help to reveal how dinosaurs acquired some of their characteristic anatomical traits. Their analysis also suggests that Buriolestes is one of the oldest known Sauropodomorpha, the group of long-necked dinosaurs that includes sauropods.

The two new animals have already helped to fill important gaps in the evolution of the key anatomical features of dinosaurs. But Langer and his colleagues aren’t done with them yet. They are using CT scans to characterize and describe the animals’ anatomy in even greater detail. They also hope to get an even more precise radioisotopic date on the oldest dinosaur-bearing rocks, and the search for more Triassic fossils continues.

Citation: Cell Press. “Dinosaurs’ rise was ‘more gradual,’ new fossil evidence suggests.” ScienceDaily. ScienceDaily, 10 November 2016. <www.sciencedaily.com/releases/2016/11/161110153112.htm>.

Key: WFS,World Fossil Society,Riffin T Sajeev,Russel T Sajeev