Category: 7. Science

  • NASA data reveals “lumpy” mantle inside Mars-Xinhua

    LOS ANGELES, Aug. 28 (Xinhua) — Rocky material from ancient impacts lies scattered in giant lumps throughout Mars’ mantle, offering new insights into the planet’s interior and its early history, according to a new study published on Thursday.

    Fragments from the aftermath of massive impacts on Mars that occurred 4.5 billion years ago have been detected deep below the planet’s surface by NASA’s InSight lander, which recorded the findings before its mission ended in 2022.

    The ancient impacts released enough energy to melt continent-size swaths of the early crust and mantle into vast magma oceans, simultaneously injecting the impactor fragments and Martian debris deep into the planet’s interior, according to the research, published in the journal Science.

    The remains of these impacts still exist as lumps up to four km across and scattered throughout the Martian mantle.

    “We’ve never seen the inside of a planet in such fine detail and clarity before,” said the study’s lead author, Constantinos Charalambous of Imperial College London. “What we’re seeing is a mantle studded with ancient fragments. Their survival to this day tells us Mars’ mantle has evolved sluggishly over billions of years. On Earth, features like these may well have been largely erased.”

    The InSight lander, which placed the first seismometer on Mars’ surface in 2018, has recorded 1,319 marsquakes during its mission, providing the detailed data that made these findings possible, according to NASA.

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  • Tricorder Tech: Stable Nitrogen Isotope Analysis of Amino Acids by Orbitrap Mass Spectrometry: Application for Extraterrestrial Samples

    Tricorder Tech: Stable Nitrogen Isotope Analysis of Amino Acids by Orbitrap Mass Spectrometry: Application for Extraterrestrial Samples

    Schematic of the GC-Orbitrap-IRMS instrumental setup: (A) GC–Orbitrap-IRMS mode, (B) the GC–SL–Orbitrap-IRMS mode, and (C) He–MS mode.– Rapid Communications In Mass Spectrometry (via PubMed)

    Background

    Obtaining isotopic data on soluble organic compounds, such as amino acids, in extraterrestrial samples is crucial for understanding their origins, prebiotic chemistry, and potential contamination. Conventional GC‐IRMS requires grams of material to measure isotopic compositions, limiting the analysis of low‐concentration organics in meteorites and other astromaterials. We present an Orbitrap‐based method optimized for nitrogen isotopic analysis of amino acids.

    Results

    This method determines δ15N values for picomole quantities (< 150 pmol) with 3%–8% precision and accuracy within 2% compared with elemental analysis. Our approach was validated using amino acid enantiomer standards and a CM2 Murchison meteorite sample. The Murchison results demonstrate that comparable precision can be achieved on analytes extracted from a total sample size representing less than 7% of the mass previously required for CSIA analysis of the same meteorite.

    Significance

    These results highlight the potential of Orbitrap mass spectrometry for δ15N measurements with less material and lower analyte concentrations. This technique improves our ability to trace the origins and synthetic pathways of amino acids, providing valuable insights into prebiotic chemistry and possible abiotic mechanisms for organic compound formation in primitive solar system materials. Nitrogen isotopes serve as a powerful tool for distinguishing biological from non‐biological sources, aiding in the identification of contamination in meteoritic samples and improving the reliability of analyses involving rare extraterrestrial materials.

    Astrobiology, Astrochemistry, Tricorder,

    Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻

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  • Autonomous, Miniature Research Station (lab-payload) For The Nanosatellite Biological Mission: LabSat

    Autonomous, Miniature Research Station (lab-payload) For The Nanosatellite Biological Mission: LabSat

    Conception of LabSat bio-nanosatellite with five basic functional blocks of lab-payload to conduct a biological experiment.– Nature

    There is an increase in demand for bio-nanosatellites and biomedical methodologies as a result of experiments conducted in microgravity and radiation conditions.

    Currently, the latest trend is to replace the experiments carried out by cosmonauts at the International Space Station (ISS) with research performed with the use of autonomous payload for nanosatellite.

    This paper describes the lab-payload for a biological nanosatellite of the CubeSat type with a size of 2U (10 × 10 × 20 cm3). The proposed payload enables the long-term cultivation of two different biological experiments simultaneously and provides suitable growth conditions.

    This lab-payload is equipped with lab-chips dedicated to each of the cultures, a container with a nutrient solution, a medium dosing system, an optical detection system, lighting, a heating system and sensors for measuring temperature, humidity, pressure and radiation inside a thermos.

    Autonomous, miniature research station (lab-payload) for the nanosatellite biological mission: LabSat, Science Reports (via PubMed)

    Autonomous, miniature research station (lab-payload) for the nanosatellite biological mission: LabSat, Nature (open access)

    Astrobiology, Space Biology, Tricorder,

    Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻

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  • World’s Most Powerful Solar Telescope Captures Its First Monster Flare in Astonishing Detail : ScienceAlert

    World’s Most Powerful Solar Telescope Captures Its First Monster Flare in Astonishing Detail : ScienceAlert

    The powerful NSF Inouye Solar Telescope has just delivered absolutely mind-blowing observations of its first X-class solar flare.

    On 8 August 2024, the telescope managed to capture one of the most powerful flares our Sun is capable of producing – at a remarkable resolution of just four Earths across. This level of detail reveals some of the finest structures we’ve ever seen associated with a solar flare, opening a new window into the Sun’s most extreme eruptions.

    “This is the first time the Inouye Solar Telescope has ever observed an X-class flare,” says astronomer Cole Tamburri of the University of California Boulder. “These flares are among the most energetic events our star produces, and we were fortunate to catch this one under perfect observing conditions.”

    Related: Staggering New Images of The Sun Are The Most Detailed Ever Taken

    Weather from our Sun can have some profound effects on our planet, with solar flares capable of knocking out radio communication for hours. We’re unlikely to be able to change what the Sun does, but if scientists understand how solar flares occur, they can develop better prediction tools that may allow us to prepare ourselves.

    frameborder=”0″ allow=”accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share” referrerpolicy=”strict-origin-when-cross-origin” allowfullscreen>

    Inouye is one of the most powerful solar observatories ever built, and it’s revealing structures on the Sun at scales finer than any we’ve seen.

    In its observations of the X1.3-class flare that took place in August 2024, Inouye captured the smallest coronal loops we’ve ever seen. On average, these loops were 48.2 kilometers (30 miles) wide, maybe as small as 21 kilometers, right at the telescope’s resolution limit of 24 kilometers.

    These loops are thin filaments of plasma that arc over the solar surface, following the magnetic field lines. They sometimes appear just before solar flares, which are powered by the energy released as magnetic field lines twist, snap, and reconnect.

    Coronal loops are deeply relevant to models of solar flare generation, but our telescopes have only been powerful enough to resolve loop bundles. Inouye has more than twice the resolving power of the next most powerful solar telescope, and its captures of the flare represent the first time scientists have been able to see individual loops.

    An annotated diagram of the flare captured by Inouye on 8 August 2024, showing the flare and the coronal loops. (NSF/NSO/AURA)

    “We’re finally peering into the spatial scales we’ve been speculating about for years. This opens the door to studying not just their size, but their shapes, their evolution, and even the scales where magnetic reconnection – the engine behind flares – occurs,” Tamburri says.

    “We’re finally seeing the Sun at the scales it works on.”

    The research has been published in The Astrophysical Journal Letters.

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  • ‘Punk rock’ dinosaur with metre-long spikes discovered

    ‘Punk rock’ dinosaur with metre-long spikes discovered

    BAKU  –  Scientists have discovered a bizarre armoured dinosaur, which had metre-long spikes sticking out from its neck, BBC reported. The species, called Spicomellus afer, lived 165 million years ago, and is the oldest example of a group of armoured dinosaurs called ankylosaurs.  The elaborateness and spikiness of the animal found in Morocco has come as a shock to experts, who now have to rethink how these armoured dinosaurs evolved. Prof Richard Butler, from the University of Birmingham who co-led the research, told BBC News that it was the “punk rocker” of its time. Punk rock is a sub-culture and music style that first emerged in the 1970s. Its followers often have spiky hair and accessories. “It is one of the strangest dinosaurs ever discovered,” said Prof Butler. Prof Butler’s project co-leader, Prof Susannah Maidment of the Natural History Museum, added that it was surprising that the spikes were fused directly on to the bone. “We don’t see that in any other animal, living or extinct,” she said. “It’s absolutely covered in really weird spikes and protrusions all over the back of the animal, including a bony collar that wraps around its neck and some sort of weapon on the end of its tail, so a most unusual dinosaur,” she said. The discovery is so unusual that the two professors are considering whether the discovery might force a rethink of theories on how ankylosaurs evolved. 

    These animals survived late into the time dinosaurs were on Earth, in a period known as the Cretaceous. This was between 145 to 66 million years ago. The end of this period saw the emergence of large carnivorous predators, such as T Rex, so it had been thought that ankylosaurs started off with simple small armoured plates on their back, which then became larger and more extensive to protect themselves from these big beasts, according to Prof Butler.

    “If you had asked me what I would have expected the oldest known ankylosaur to look like I would have said something with quite simple armour,” he told BBC News. “Instead, we have an animal bristling with spikes like a hedgehog, the most bizarre armour that we’ve ever found in any animal, far outside the range of armour seen in later ankylosaurs.” The researchers don’t have enough of the skeleton to be sure of the animal’s proportions, but they estimate it would have been about four metres long and one metre high, weighing around two tonnes. The discovery raises the possibility that ankylosaurs started off with elaborate armour in an earlier dinosaur period, known as the Jurassic, which evolved over tens of millions of years to become more simple and possibly more functional, according to Prof Maidment. “What we are speculating is that maybe these structures actually were used for display, and it was only later in the Cretaceous, when we start to see gigantic dinosaurs with huge jaws and crushing bites, that they actually then needed to co-opt these display structures as body armour.”

    The discovery was made by a local farmer in what is now the Moroccan town of Boulemane. It was the first ankylosaur to be found on the African continent. Prof Butler recalls the moment when he first saw the fossils. “It was a jaw dropping, spine-tingling moment, perhaps the most exciting in my career. It was clear right away that this animal was much weirder than we imagined and that we had enough of it to make sense of it,” he said. Prof Driss Ouarhache, who led the Moroccan team involved in the research, from the Université Sidi Mohamed Ben Abdellah, said: “This study is helping to drive forward Moroccan science. We’ve never seen dinosaurs like this before, and there’s still a lot more this region has to offer.”


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  • Planetary Assays: Testing A Computed Tomography Imaging Spectrometer for Earth Observations on the HEIMDAL Stratospheric Balloon Mission

    Planetary Assays: Testing A Computed Tomography Imaging Spectrometer for Earth Observations on the HEIMDAL Stratospheric Balloon Mission

    Shows the 0th order of CTIS images 11770-11800 overlaid on a corresponding RGB image during flight. The red arrow illustrates the motion of the balloon. – physics.ins-det

    Stratospheric High Altitude Balloons (HABs) have great potential as a remote sensing platform for Earth Observations that complements orbiting satellites and low flying drones.

    At altitudes between 20-35 kms, HABs operate significantly closer to ground than orbiting satellites, but significantly higher than most drones. HABs therefore offer a unique potential to deliver high spatial resolution imaging with large area coverage. Another two imaging parameters that are important for Earth Observation applications are spectral resolution and spectral range.

    In this paper, we therefore present the development and testing of a hyperspectral imaging system, able to record near-video-rate images in narrow contiguous spectral bands, from a HAB platform. In particular, we present the first stratospheric environmental tests and HAB flight of a snapshot hyperspectral camera, based on Computed Tomography Imaging Spectroscopy (CTIS), which is well suited to cope with the challenges posed by the motion of the HAB platform and the stratospheric environment.

    We have successfully acquired images with the system under both simulated stratospheric conditions in the Mars Simulation Laboratory at Aarhus University and during a 5 hour HAB flight mission named HEIMDAL from Kiruna in October 2024 as part of the REXUS/BEXUS 34/35 2024 campaign organized by DLR-SNSA. The study represents a step towards deploying the HAB platform for high quality land cover classification.

    Mads Juul Ahlebæk, Albertino Antonio Almeida Bach, Loui Collin-Enoch, Christian Cordes, Boas Hermansson, Christian Hald Jessen, Søren Peter Jørgensen, Tobias Jørgensen, Viktor Ulrich Kanstrup, Laurits Tværmose Nielsen, Jes Enok Steinmüller, Mads Svanborg Peters, Jonathan Merrison, René Lynge Eriksen, Christoffer Karoff, Mads Toudal Frandsen

    Comments: A review of the HEIMDAL experiment, launched as part of the REXUS/BEXUS 34/35 October 2024 stratospheric balloon flight campaign. 34 pages, 22 figures. As the experiment was being developed, this was presented at IASIM-2024 in Bilbao, Spain
    Subjects: Instrumentation and Detectors (physics.ins-det); Instrumentation and Methods for Astrophysics (astro-ph.IM); Biological Physics (physics.bio-ph); Optics (physics.optics)
    Cite as: arXiv:2508.19693 [physics.ins-det] (or arXiv:2508.19693v1 [physics.ins-det] for this version)
    https://doi.org/10.48550/arXiv.2508.19693
    Focus to learn more
    Submission history
    From: Mads Ahlebæk
    [v1] Wed, 27 Aug 2025 09:01:22 UTC (41,329 KB)
    https://arxiv.org/abs/2508.19693

    Astrobiology, Tricorder,

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  • TIME for Kids | Watching the Skies

    TIME for Kids | Watching the Skies

    Space is full of mysteries, from black holes to dark matter



    dark matter



    an invisible form of matter that astronomers believe makes up a large part of the universe
    (noun)



    . Now, astronomers have a new view of the universe. They can see the stars with the world’s largest digital camera.

    The device is called the Legacy Survey of Space and Time (LSST) camera. It is part of the Vera C. Rubin Observatory. It sits atop a mountain in Chile. The camera is part of a 27-foot telescope.

    On June 23, members of the Rubin team held a press conference. They released the camera’s first images. These images were all captured in just a few days. They showed stars, galaxies, and thousands of previously unseen asteroids.

    Colossal Camera

    The LSST camera took 10 years to build. Željko Ivezi directed its construction. During the June 23 press conference, he called the camera “the greatest astronomical discovery machine ever built.”

    P. HORÁLEK(INSTITUTE OF PHYSICS IN OPAVA)—RUBIN OBS/NOIRLAB/SLAC/NSF/DOE/AURA

    It’s certainly powerful. The new images reveal two nebulas



    nebulas



    a cloud of gas and dust in space
    (noun)



    . They’re located thousands of light-years from Earth. (A light-year is the distance light travels in a year, nearly 6 trillion miles.)

    Margaux Lopez is one of the camera’s mechanical engineers. She told TIME for Kids the camera is one of a kind. First of all, it’s huge. It’s about the size of a car. It’s also fast. The camera can take 1,000 images of the sky every 24 hours. That’s important, because space is vast.

    “We can only see a little bit of what’s out there, and everything’s really spread out,” Lopez says. “In the first year, we are going to take more data than every telescope in the history of humanity combined has ever taken.”

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  • New tool boosts speed in mineral analysis

    New tool boosts speed in mineral analysis

    Scientists introduced MIST, a new algorithm that quickly identifies minerals from chemical data. MIST automates a traditionally slow, expert-dependent process, streamlining exploration and mining.

    The study, published in a new issue of Computers & Geosciences, presents MIST—short for Mineral Identification by Stoichiometry—a computational tool that classifies minerals based on oxide compositional data. It replaces manual petrography and spectroscopy, offering a faster, standardized method to process vast datasets generated during exploration.

    The researchers who made the discovery and penned the article are a team of scientists at Rice University’s Department of Earth, Environmental and Planetary Sciences.

    Researchers note this represents a major advancement in geoscience data science as machine learning depends on high-quality data, and MIST ensures that the data is accurate and uniform. Available at mist.rice.edu, the tool is already being utilized in planetary science, including analyzing chemical data collected by NASA’s Mars rovers.

    One scientific researcher noted MIST was initially developed to interpret minerals on Mars and now it is proving just as useful for studying rocks here on Earth.

    In an interview with Phys.org, Kirsten Siebach, assistant professor of Earth, environmental and planetary sciences and lead author of the study, commented: “MIST takes a tedious, expertise-heavy process and makes it accessible in seconds. You don’t have to already know what mineral you’re looking at—MIST can figure it out from the chemistry.”

    Mineral identification is crucial for mining geology, affecting resource quantification and extraction techniques. Traditional methods rely on textures and optical properties, which, while accurate, are too slow for large deposits or early-stage exploration. Converting large analytical datasets into precise mineral IDs is complicated by mineral variability and elemental substitutions. Existing database-driven or machine learning approaches often lack consistency or require extensive training data.

    MIST addresses these issues by applying stoichiometric rules based on known mineral formulas. It provides a reproducible framework that transforms raw compositional data into reliable classifications.

    MIST analyzes oxide percentages, normalizes the data, and compares it against stoichiometric boundaries from established formulas. It accounts for natural substitutions—like Fe, Mg, or Ca—using rules aligned with International Mineralogical Association standards. The algorithm recalculates mineral formulas, filters out poor-quality or contaminated data, and assigns mineral identities or likely species. Implemented in MATLAB with an online version, MIST integrates smoothly into existing geochemical workflows.

    Applied to large repositories such as GEOROC, MIST identified over 200 mineral species from more than 875,000 analyses. It generated standardized formulas, flagged endmembers, and included quality checks comparing measured stoichiometry with ideal values. Case studies on igneous and metamorphic rocks demonstrated MIST’s ability to identify minerals like clinopyroxenes, feldspars, and sulfates such as anhydrite—accounting for elemental substitutions that impact mineral processing.

    The developers state that MIST improves mineral database reliability, enhances resource estimates, and provides cleaner data for machine learning models. Despite some limitations, like narrow criteria for certain minerals or difficulty handling mixed phases, the tool marks a significant step forward in large-scale mineral identification.

    MIST’s primary impact may lie in improving and annotating large mineral databases for machine learning applications. The team applied it to filter over a million analyses from the GEOROC geochemical database, converting 875,000 mineral records into a standardized format suitable for AI training and large-scale geological research.

    MIST enables faster interpretation of geochemical data, crucial during early exploration for prompt decision-making. It enhances quality control by detecting anomalies indicative of contamination or alteration, common in ore samples. Incorporating clearer mineralogical context improves resource estimates and guides more efficient processing strategies.

    The authors highlight that MIST complements traditional, texture-based identification, offering rapid first-pass classification to guide detailed analysis. The framework can evolve to include new mineral species and refine stoichiometric rules, keeping pace with industry advancements.

    By providing faster, scalable, and more consistent mineral identification, MIST supports a move toward data-driven mining practices—ultimately leading to more efficient and sustainable resource development.

    The article on MIST can be accessed here.


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  • Healing Ozone Layer Could Trigger 40% More Global Warming

    Healing Ozone Layer Could Trigger 40% More Global Warming

    Healing the ozone layer protects us from UV rays, but it may also fuel far more global warming than once thought, challenging assumptions about climate progress. Credit: Shutterstock

    As the ozone layer recovers, it’s also intensifying global warming. Researchers predict that by 2050, ozone will rank just behind carbon dioxide as a driver of heating, offsetting many of the benefits from banning CFCs.

    The planet is now expected to heat up more than scientists once predicted, and a major reason lies in the future behavior of ozone. This gas shields life on Earth from dangerous ultraviolet radiation, yet it also acts as a greenhouse gas by trapping heat in the atmosphere.

    The ban on ozone-depleting chemicals such as CFCs has allowed the protective layer to steadily recover. But researchers warn that when this rebound is combined with rising levels of air pollution, ozone could drive 40% more warming than earlier estimates suggested.

    Measuring Ozone’s Warming Impact

    Research led by the University of Reading shows that between 2015 and 2050, ozone will be responsible for an additional 0.27 watts per square meter (Wm⁻²) of trapped energy. This measurement refers to the amount of extra heat retained per square meter of the Earth’s surface. By mid-century, this would make ozone the second most important cause of warming, behind only carbon dioxide (1.75 W m⁻² of extra warming).

    Professor Bill Collins, who led the study, explained: “Countries are doing the right thing by continuing to ban chemicals called CFCs and HCFCs that damage the ozone layer above Earth. However, while this helps repair the protective ozone layer, we have found that this recovery in ozone will warm the planet more than we originally thought.

    “Air pollution from vehicles, factories, and power plants also creates ozone near the ground, causing health problems and warming the planet.”

    Simulating the Atmosphere’s Future

    The research, published on August 21 in Atmospheric Chemistry and Physics, used computer models to simulate how the atmosphere will change by the middle of the century. The models followed a scenario with low implementation of air pollution controls, but with CFCs and HCFCs being phased out as mandated by the Montreal Protocol (1987).

    The findings show that stopping CFC and HCFC production – done mainly to protect the ozone layer – provides less climate benefit than previously calculated. CFCs and HCFCs are greenhouse gases that warm the planet. Countries banned them to save the ozone layer, expecting this would also help fight climate change. But as the ozone layer heals, it creates more warming that cancels out most of the climate benefits from removing CFCs and HCFCs.

    Unavoidable Warming Ahead

    Countries that reduce air pollution will limit some ozone formation near the ground. However, the ozone layer will continue repairing itself for decades regardless of air quality policies, creating unavoidable warming.

    Protecting the ozone layer remains crucial for human health and preventing skin cancer. The ozone layer shields Earth from dangerous ultraviolet radiation that can harm people, animals and plants. However, the research suggests climate policies need updating to account for ozone’s larger warming effect.

    Reference: “Climate forcing due to future ozone changes: an intercomparison of metrics and methods” by William J. Collins, Fiona M. O’Connor, Rachael E. Byrom, Øivind Hodnebrog, Patrick Jöckel, Mariano Mertens, Gunnar Myhre, Matthias Nützel, Dirk Olivié, Ragnhild Bieltvedt Skeie, Laura Stecher, Larry W. Horowitz, Vaishali Naik, Gregory Faluvegi, Ulas Im, Lee T. Murray, Drew Shindell, Kostas Tsigaridis, Nathan Luke Abraham and James Keeble, 21 August 2025, Atmospheric Chemistry and Physics.
    DOI: 10.5194/acp-25-9031-2025

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  • 70-Million-Year-Old Fossils of Crocodile-Like Apex Predator Unearthed in Argentina

    70-Million-Year-Old Fossils of Crocodile-Like Apex Predator Unearthed in Argentina

    Paleontologists have unearthed a beautifully preserved skull and jaws as well as part of the postcranial skeleton of a previously unknown peirosaur species in Patagonia, Argentina.

    Life reconstruction of Kostensuchus atrox. Image credit: Gabriel Diaz Yanten.

    Kostensuchus atrox roamed Earth during the Maastrichtian age of the Cretaceous period, around 70 million years ago.

    The ancient species was a large predator, approximately 3.5 m (11.5 feet) long and 250 kg in weight.

    The animal had a wide, powerful jaw and big teeth capable of devouring large prey, likely including medium-sized dinosaurs.

    Kostensuchus atrox belonged to Peirosauridae, a Gondwanan family of crocodylomorphs within the suborder Notosuchia.

    “This new species belongs to the notosuchian clade Peirosauridae, representing the latest and southernmost record for this group of crocodyliforms,” said Dr. Fernando Novas, a paleontologist at the Museo Argentino de Ciencias Naturales ‘Bernardino Rivadavia,’ and his colleagues.

    The fossilized skull and bones of Kostensuchus atrox were found in the Chorrillo Formation, about 30 km south-west of the town of El Calafate in the province of Santa Cruz.

    “The Chorrillo Formation formed around 70 million years ago,” the paleontologists said.

    “At this time, southern Patagonia was a warm, seasonally humid landscape of freshwater floodplains, home to creatures like dinosaurs, turtles, frogs, and various mammals.”

    “The new fossil unearthed in this formation is largely intact, including a skull and jaws with visible details, as well as multiple bones from the body.”

    Kostensuchus atrox is the second-largest predator known to scientists from the Chorrillo Formation, and was likely one of the top predators in the region.

    The new species is also the first crocodyliform fossil found in this formation, and one of the most intact peirosaurid crocodyliforms ever found, giving scientists unique new insight into these prehistoric animals and their ecosystem.

    “The discovery of Kostensuchus atrox considerably expands the knowledge about the anatomy of broad-snouted peirosaurids, previously known from extremely fragmentary remains from South America and Madagascar,” the researchers said.

    “The new anatomical information sheds light on both, the similarities and differences between broad-snouted peirosaurids and baurusuchids, the other crocodyliform clade that independently evolved into apex predators during the Cretaceous of Gondwana.”

    Kostensuchus atrox formed part of the latest Cretaceous ecosystem of southern Patagonia, in a freshwater ecosystem under a temperate to warm climate with seasonal humidity, alongside a diverse fauna of dinosaurs, mammals, and other vertebrates,” they added.

    “The broad and high snout of Kostensuchus atrox, with notably large and robust ziphodont teeth, along with a broad adductor chamber in the skull and deep mandibular ramus, and robust forelimb anatomy suggests that the new species was capable of subduing large prey.”

    “These features imply that Kostensuchus atrox played the role of a top predator within this end-Cretaceous ecosystem.”

    The discovery of Kostensuchus atrox is described in a paper published this week in the journal PLoS ONE.

    _____

    F.E. Novas et al. 2025. A new large hypercarnivorous crocodyliform from the Maastrichtian of Southern Patagonia, Argentina. PLoS One 20 (8): e0328561; doi: 10.1371/journal.pone.0328561

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