Category: 7. Science

  • NASA Supercomputers Take on Life Near Greenland’s Most Active Glacier

    NASA Supercomputers Take on Life Near Greenland’s Most Active Glacier

    Simulating “biology, chemistry, and physics coming together” in even one pocket along Greenland’s 27,000 miles (43,000 kilometers) of coastline is a massive math problem, noted lead author Michael Wood, a computational oceanographer at San José State University. To break it down, he said the team built a “model within a model within a model” to zoom in on the details of the fjord at the foot of the glacier.

    Using supercomputers at NASA’s Ames Research Center in Silicon Valley, they calculated that deepwater nutrients buoyed upward by glacial runoff would be sufficient to boost summertime phytoplankton growth by 15 to 40% in the study area.

    More Changes in Store

    Could increased phytoplankton be a boon for Greenland’s marine animals and fisheries? Carroll said that untangling impacts to the ecosystem will take time. Melt on the Greenland ice sheet is projected to accelerate in coming decades, affecting everything from sea level and land vegetation to the saltiness of coastal waters.

    “We reconstructed what’s happening in one key system, but there’s more than 250 such glaciers around Greenland,” Carroll said. He noted that the team plans to extend their simulations to the whole Greenland coast and beyond.

    Some changes appear to be impacting the carbon cycle both positively and negatively: The team calculated how runoff from the glacier alters the temperature and chemistry of seawater in the fjord, making it less able to dissolve carbon dioxide. That loss is canceled out, however, by the bigger blooms of phytoplankton taking up more carbon dioxide from the air as they photosynthesize.

    Wood added: “We didn’t build these tools for one specific application. Our approach is applicable to any region, from the Texas Gulf to Alaska. Like a Swiss Army knife, we can apply it to lots of different scenarios.”

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  • Vulcan Centaur rocket to launch 1st national security mission on Aug. 12

    Vulcan Centaur rocket to launch 1st national security mission on Aug. 12

    United Launch Alliance’s (ULA) new Vulcan Centaur rocket will conduct its first-ever national security launch next week, if all goes according to plan.

    ULA announced on Tuesday (Aug. 5) that it’s targeting Aug. 12 for USSF-106, a U.S. Space Force mission that will lift off from Cape Canaveral Space Force Station in Florida.


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  • SpaceOps: Scientist Lobbies NASA For Closer Look An Interstellar Object

    The way Harvard astrophysicist Avi Loeb figures, rather than letting the Juno spacecraft end its mission with a suicidal plunge into Jupiter’s crushing atmosphere, why not use whatever propellant remains to get the orbiter into the most advantageous position to view a visiting object from another solar system.

    The apple of Loeb’s eye is a 6-12 mi.-wide rocky body discovered on July 1 with a telescope in Rio Hurtado, Chile, that is part of NASA’s Asteroid Terrestrial-impact Last Alert System (ATLAS) survey team.

    The comet-like object—although it currently lacks a distinctive comet-like tail—is just the third interstellar (3I) body discovered so far. Scientists suspect there could be many more similar objects zipping through the Solar System unobserved.

    At the time of its discovery, 3I/ATLAS was about 4.5 astronomical units (AU) from the Sun—inside the orbit of Jupiter—and traveling at a speed of 137,000 mph. One AU is the distance between Earth and the Sun, roughly 93 million mi.

    Hailing from the direction of the constellation Sagittarius and the central region of the Milky Way galaxy, 3I/ATLAS is in what is known as a hyperbolic orbit—too fast to be constrained by the gravity of the Sun and too elliptical for objects to loop back around it.

    3I/ATLAS will fly within 18 million mi. of Mars on Oct. 2, and reach perihelion—its closest point to the Sun—on Oct. 29-30 at a distance of about 1.4 AU, which is just inside the orbit of Mars.

    Before resuming its cold, dark journey in interstellar space, 3I/ATLAS will pass about 33 million mi. from Jupiter’s orbit on March 16. It is there and then Loeb and colleagues would like to put NASA’s Juno probe to work.

    “A close encounter between Juno and 3I/ATLAS will provide a once-in-a-lifetime opportunity to bring a human-made spacecraft within a short distance from a large interstellar object,” Loeb and colleagues wrote in a series of papers posted on arxiv.org.

    Built by Lockheed Martin and operated by NASA’s Jet Propulsion Laboratory, Juno launched from Cape Canaveral on Aug. 5, 2011, as part of the agency’s New Frontiers program. The spacecraft reached Jupiter and put itself into a polar orbit on July 5, 2016, to begin an extensive and extended scientific investigation of the planet.

    Juno is currently slated to cease operations in September when it will be tugged from orbit and then crushed by Jupiter’s immense gravity. The disposal protocol was designed in part to reduce chances any super-resilient, hitchhiking Earth microbes that somehow managed to stay alive on the spacecraft since launch could inadvertently seed life on a potentially habitable (and possibly inhabited) moon of Jupiter.

    Loeb and colleagues lay out an alternative plan for Juno. They propose using whatever propellant remains to reposition the spacecraft for 3I/ATLAS’s flyby on March 16.

    “We do not presume any specific amount of fuel. Instead, we show how close Juno can get to the path of 3I/ATLAS as a function of the amount of fuel left,” Loeb wrote in an email to Aviation Week.

    The instruments on Juno—a near-infrared spectrometer, magnetometer, microwave radiometer, gravity science instrument, energetic particle detector, radio and plasma wave sensor, UV spectrograph and visible light camera/telescope—“can all be used to probe the nature of 3I/ATLAS from a close distance far better than any observatories on Earth,” Loeb noted in an Aug. 2 post on Medium.

    NASA did not specifically say it had studied a mission extension for Juno. The agency is in the process of trimming 20% of its staff and preparing for a possible near-50% cut to science programs, including Juno.

    Instead, NASA spokeswoman Karen Fox told Aviation Week,  “From what I understand, the Juno spacecraft has significantly less propellant than assumed. The team says any remaining propellant is typically used for small spacecraft maneuvers, done via thrusters.”

    Rather than Juno, NASA says it is adding 3I/ATLAS observations to the Hubble and James Webb space telescopes’ schedules. “We are exploring whether some of our other telescopes can do so as well,” Fox said.

    For now, astronomers worldwide have the interstellar visitor in sight. 3I/ATLAS is visible to ground-based telescopes through September. It will then pass behind by the Sun, relative to Earth’s line of sight, and—if it survives close approach—reappear in early December.

    Interstellar objects are believed to be cosmic debris left over from the formation of planetary systems around their host stars. “As these remnants orbit their star, the gravity of nearby larger planets and passing nearby stars can launch them out of their home systems and into interstellar space, where they can cross paths with other solar systems,”  the U.S. National Science Foundation (NSF) wrote in a press release about 31/ATLAS observations with its Gemini North telescope in Hawaii.

    “These visitors from faraway regions of the cosmos are valuable objects to study since they offer a tangible connection to other star systems. They carry information about the chemical elements that were present when and where they formed, which gives scientists insight into how planetary systems form at distant stars throughout our galaxy’s history—including stars that have since died out,” the NSF added.

    3I/ATLAS is traveling much faster than two previous interstellar objects, 1I/‘Oumuamua and 2I/Borisov, discovered in 2017 and 2019, respectively. The newcomer may be older as well, likely predating the Solar System, which is 4.6 billion yrs old.

    Later this year, the Vera C. Rubin Observatory, jointly funded by the NSF and the U.S. Department of Energy’s Office of Science, is expected to join the hunt for more interstellar objects as part of its Legacy Survey of Space and Time program, a planned decade-long, all-sky survey of the southern hemisphere. 

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  • NASA’s Perseverance Rover Captures Mars Vista As Clear As Day

    ‘Float rocks,’ sand ripples, and vast distances are among the sights to see in the latest high-resolution panorama by the six-wheeled scientist.

    The imaging team of NASA’s Perseverance Mars rover took advantage of clear skies on the Red Planet to capture one of the sharpest panoramas of its mission so far. Visible in the mosaic, which was stitched together from 96 images taken at a location the science team calls “Falbreen,” are a rock that appears to lie on top of a sand ripple, a boundary line between two geologic units, and hills as distant as 40 miles (65 kilometers) away. The enhanced-color version shows the Martian sky to be remarkably clear and deceptively blue, while in the natural-color version, it’s reddish.

    “Our bold push for human space exploration will send astronauts back to the Moon,” said Sean Duffy, acting NASA administrator. “Stunning vistas like that of Falbreen, captured by our Perseverance rover, are just a glimpse of what we’ll soon witness with our own eyes. NASA’s groundbreaking missions, starting with Artemis, will propel our unstoppable journey to take human space exploration to the Martian surface. NASA is continuing to get bolder and stronger.”

    The rover’s Mastcam-Z instrument captured the images on May 26, 2025, the 1,516th Martian day, or sol, of Perseverance’s mission, which began in February 2021 on the floor of Jezero Crater. Perseverance reached the top of the crater rim late last year.

    “The relatively dust-free skies provide a clear view of the surrounding terrain,” said Jim Bell, Mastcam-Z’s principal investigator at Arizona State University in Tempe. “And in this particular mosaic, we have enhanced the color contrast, which accentuates the differences in the terrain and sky.”

    One detail that caught the science team’s attention is a large rock that appears to sit atop a dark, crescent-shaped sand ripple to the right of the mosaic’s center, about 14 feet (4.4 meters) from the rover. Geologists call this type of rock a “float rock” because it was more than likely formed someplace else and transported to its current location. Whether this one arrived by a landslide, water, or wind is unknown, but the science team suspects it got here before the sand ripple formed.

    The bright white circle just left of center and near the bottom of the image is an abrasion patch. This is the 43rd rock Perseverance has abraded since it landed on Mars. Two inches (5 centimeters) wide, the shallow patch is made with the rover’s drill and enables the science team to see what’s beneath the weathered, dusty surface of a rock before deciding to drill a core sample that would be stored in one of the mission’s titanium sample tubes.

    The rover made this abrasion on May 22 and performed proximity science (a detailed analysis of Martian rocks and soil) with its arm-mounted instruments two days later. The science team wanted to learn about Falbreen because it’s situated within what may be some of the oldest terrain Perseverance has ever explored — perhaps even older than Jezero Crater.

    Tracks from the rover’s journey to the location can be seen toward the mosaic’s right edge. About 300 feet (90 meters) away, they veer to the left, disappearing from sight at a previous geologic stop the science team calls “Kenmore.”

    A little more than halfway up the mosaic, sweeping from one edge to the other, is the transition from lighter-toned to darker-toned rocks. This is the boundary line, or contact, between two geologic units. The flat, lighter-colored rocks nearer to the rover are rich in the mineral olivine, while the darker rocks farther away are believed to be much older clay-bearing rocks.

    NASA’s Jet Propulsion Laboratory, which is managed for the agency by Caltech, built and manages operations of the Perseverance rover on behalf of NASA’s Science Mission Directorate in Washington, as part of NASA’s Mars Exploration Program portfolio. Arizona State University leads the operations of the Mastcam-Z instrument, working in collaboration with Malin Space Science Systems in San Diego, on the design, fabrication, testing, and operation of the cameras.

    For more about Perseverance:

    https://science.nasa.gov/mission/mars-2020-perseverance

    DC Agle
    Jet Propulsion Laboratory, Pasadena, Calif.
    818-393-9011
    agle@jpl.nasa.gov

    Karen Fox / Molly Wasser
    NASA Headquarters, Washington
    202-358-1600
    karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov

    2025-100

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  • Dwarf Galaxies Like the Magellanic Clouds Have Their Own Small Satellite Galaxies

    Dwarf Galaxies Like the Magellanic Clouds Have Their Own Small Satellite Galaxies

    Understanding the growth and evolution of galaxies is a critical part of cosmology. We know that massive galaxies like our own Milky Way grew over time by cannibalizing and merging with smaller satellite galaxies. That could be what’s happening right now with the Large and Small Magellanic Clouds, as they’re being tidally disrupted by the Milky Way.

    But researchers wonder if dwarf galaxies similar to the Magellanic Clouds have their own, much less massive satellites. New research by astronomers at Dartmouth College aims to broaden our understanding of dwarf galaxies and their satellites. The Lambda CDM model says that galaxies grow massive through mergers, and researchers want to test that idea.

    The research is “Identifying Dwarfs of MC Analog GalaxiEs (ID-MAGE): The Search for Satellites around Low-mass Hosts,” and it’s published in The Astrophysical Journal. The lead author is Laura Hunter, a research associate in the Physics and Astronomy Department at Dartmouth College.

    ID-MAGE is a survey of low-mass galaxies and their satellites between 4 and 10 megaparsecs away (13 million and 32.6 million light-years). It searched for satellite galaxies around 35 dwarf galaxies roughly as massive as the Large and Small Magellanic Clouds. ID-MAGE is based on data from the Dark Energy Spectroscopic Instrument (DESI) Legacy Imaging Surveys. ID-MAGE found 355 candidate satellite galaxies, 264 of which are new detections.

    The 35 galaxies were chosen because they’re different sizes and in different proximities to other galaxies. The idea is to discover how these factors influence the formation of satellite galaxies, and by casting a wide net, the results aren’t skewed by mass and proximity. “A robust sample of satellite galaxies around hosts with a wide range of masses is required to test ΛCDM models and our understanding of galaxy formation and evolution,” the researchers explain.

    This figure shows the surrounding environments for three representative low-mass galaxies in the survey. The galaxy on the left is in an isolated environment, while the environment gets more crowded in the middle image and on the right. “The central black point is the host galaxy, and the gray region is the 150 kpc radius search area,” the authors explain. “The green crosses are known galaxies that are less massive than our hosts, the pink squares are SMC-mass galaxies, and the orange diamonds are LMC-mass galaxies.” Image Credit: Hunter et al 2025 ApJ 989 58

    Observations show that larger galaxies host more dwarf galaxies, which makes intuitive sense. Their greater mass should allow them to attract and maintain their holds on smaller galaxies. But the question is, does this same relationship hold true for lower mass galaxies? Do they hold even smaller galaxies in thrall?

    “With this survey, we’ll be able to test whether those predictions hold true with much smaller host galaxies,” lead author Hunter said in a press release. “Astronomy is a field where you can’t run experiments; all you can do is observe and make as many measurements as you can, and then put that data into a simulation and see whether it reproduces your observations. If it doesn’t, that tells us that there’s something wrong with our assumptions or our model of the universe.”

    Determining which of the satellite candidates were actual satellite galaxies was a two-step process. First, the team used an algorithm to remove noise from the images, especially light from other stars or galaxies. Following that, they visually inspected images to eliminate things like image defects.

    This figure illustrates how the team's detection algorithm works. The first image on the left shows the candidate dwarf satellite galaxy. The second panel is the image after masking objects from the Guide Star Catalog. The third image is after further processing, and the final image shows the object detected above the background noise. After the algorithm processed the images, they are visually inspected. Image Credit: Hunter et al 2025 ApJ 989 58 This figure illustrates how the team’s detection algorithm works. The first image on the left shows the candidate dwarf satellite galaxy. The second panel is the image after masking objects from the Guide Star Catalog. The third image is after further processing, and the final image shows the object detected above the background noise. After the algorithm processed the images, they are visually inspected. Image Credit: Hunter et al 2025 ApJ 989 58

    Their results conform to current cosmological models.

    “Through a systematic visual inspection campaign, we classify the top candidates as high-likelihood satellites,” the researchers write. “On average, we find 4.0 ± 1.4 high-likelihood candidate satellites per LMC-mass host and 2.1 ± 0.6 per SMC-mass host, which is within the range predicted by cosmological models.”

    They also found that their 35 hosts have fewer satellites than Milky-Way mass hosts, and that SMC mass hosts have fewer satellites than LMC mass hosts. This also agrees with Lambda CDM predictions. “Our low-mass hosts also exhibit the trend observed among MW-mass hosts where satellite abundance correlates with host stellar mass, extending this relationship into the dwarf host galaxy mass range,” the researchers explain.

    Finding these candidates is just the first phase of the team’s research. Their follow-up work will more strongly confirm their candidate galaxies as actual satellites. It will also determine their masses, their distribution, the amount of gas and dust they contain, and how quickly they form new stars.

    “The ultimate goal of ID-MAGE is to create the first statistical view of dwarf satellites around low-mass hosts, substantially extending the range of host masses and environments probed by existing surveys, delivering quantitative constraints for galaxy formation physics in ΛCDM,” the authors explain.

    In their conclusion, the authors point out that their ID-MAGE survey already provides important observations into satellite galaxy populations and how they’re influenced by the mass of their host galaxies. “Moving forward, follow-up observations will refine our catalog, enabling detailed analysis of how host mass and environment affect satellite populations. This will lead to a deeper understanding of the galaxy formation and evolution processes in the ΛCDM paradigm,” the authors conclude in their paper.

    “Getting the answers will require a lot of resources and telescope time, but the impact will be incredible for understanding the nature of dark matter and galaxy formation at the smallest scale,” said study co-author Burçİn Mutlu-Pakdil, also from Dartmouth College. “Each one of them holds a little clue about the physics of how galaxies form.”

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  • Mystery of why sea stars keep turning into goo finally solved — and it’s not what scientists thought

    Mystery of why sea stars keep turning into goo finally solved — and it’s not what scientists thought

    Researchers have discovered the cause of a mysterious marine epidemic that has turned billions of sea stars into goo along the West Coast — and it’s not what they expected.

    Sea star wasting disease has been killing sea stars since 2013, causing catastrophic damage to ecosystems and driving the largest sea star species to the brink of extinction. Researchers thought a virus might be responsible for the disease, but after a four-year-long investigation, they’ve found that a strain of bacteria is to blame.

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  • Solar Powered Moon Brick Factory Could Build Future Lunar Cities

    Solar Powered Moon Brick Factory Could Build Future Lunar Cities

    Chinese scientists have developed a remarkable machine that could revolutionize how humans build structures on the Moon. The device works like a 3D printer powered by concentrated sunlight, turning lunar soil (known as regolith) into strong construction bricks without needing any materials from Earth.

    Astronaut Buzz Aldrin’s boot print in the lunar regolith (Credit : NASA)

    Developed by the Deep Space Exploration Laboratory in Hefei, the system functions as a 3D printing device using a parabolic reflector to gather solar radiation, which is then funnelled through fibre optic bundles. The technology is elegantly simple yet incredibly powerful, at the focus point, light intensity exceeds 3,000 times the standard level, reaching temperatures over 1,300 C to melt lunar regolith.

    The bricks produced are dense and robust, suitable not only for shelter construction but also for roads and platforms on the lunar surface. Imagine entire lunar cities built from nothing more than the ground beneath astronauts’ feet and the Sun’s energy. However, the engineers are realistic about the limitations, emphasising that lunar soil bricks alone cannot sustain pressure in the Moon’s vacuum and low gravity environment. Instead, the bricks will act as protective layers over pressure-retaining habitat modules made of rigid and inflatable structures. Think of it as creating a protective shell around pressurised living spaces, providing crucial shielding from radiation and meteorites.

    Leonid meteor captured here streaking through the Earth's atmosphere. Space rocks like meteor's are a great risk to lunar structures that any material will have to offer protection against (Credit : Navicore) Leonid meteor captured here streaking through the Earth’s atmosphere. Space rocks like meteor’s are a great risk to lunar structures that any material will have to offer protection against (Credit : Navicore)

    The two year development process wasn’t without challenges. Key challenges included transporting and melting variable lunar soil compositions and achieving efficient solar energy transmission. To address this, the team created multiple types of simulated lunar soil for extensive trials. This thorough testing approach ensures the technology will work reliably in the Moon’s harsh environment.

    What makes this breakthrough particularly impressive is its self sufficiency. According to senior engineer Yang Honglun, the machine uses no additives relying entirely on the lunar soil. This means future lunar settlers won’t need to transport heavy building materials from Earth, dramatically reducing the cost and complexity of establishing Moon bases.

    Due to the immense gravitational pull of the Earth, rockets like the mighty Saturn V are needed to transport materials to space. A costly enterprise if building materials had to be shipped to the Moon (Credit : NASA) Due to the immense gravitational pull of the Earth, rockets like the mighty Saturn V are needed to transport materials to space. A costly enterprise if building materials had to be shipped to the Moon (Credit : NASA)

    The vision extends far beyond just making bricks. Yang outlined a broader vision for lunar construction involving brick manufacturing, modular component integration, and structural validation under true lunar surface conditions. These efforts aim to enable full scale surface construction supported by automated robots and the brick making device.

    To ensure the technology works as expected, Chinese astronauts aboard the nation’s space station will expose simulated lunar bricks, delivered by the Tianzhou 8 cargo spacecraft in November 2024, to space conditions. This will assess thermal durability, mechanical integrity, and radiation shielding to inform future lunar base construction.

    Source : Lunar soil machine developed to build bricks using sunlight

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  • Evidence of World-Changing Comet Explosion 12,800 Years Ago Found in The Ocean : ScienceAlert

    Evidence of World-Changing Comet Explosion 12,800 Years Ago Found in The Ocean : ScienceAlert

    Microscopic grains of alien dust buried in the sediment at the bottom of the ocean could be evidence of a comet that exploded in Earth’s atmosphere 12,800 years ago.

    This hypothetical event, known as the Younger Dryas impact, was invoked to explain a sudden, 1,200-year period of rapid cooling to near-glacial conditions during a time when Earth’s climate was on a warm upswing. It’s a controversial proposal, to say the least, with many scientists roundly rejecting it while others remain more open to the possibility.

    One of the leading refutations is that no crater has been found, as one might expect from such a world-changing event… but the evidence may be much smaller than a crater.

    Related: Cosmic Shrapnel That Killed The Mammoth Is Buried Deep, Scientists Claim

    Led by geoscientist Christopher Moore of the University of South Carolina, a team of researchers puts forward a new line of evidence: four sediment cores from Baffin Bay near Greenland.

    These are cylinders of material excavated vertically that preserve layers upon layers of seafloor sediment that were deposited over many millennia.

    Some of the silica- and iron-rich microspherules found in the cores. (Moore et al., PLOS One, 2025)

    “We chose to analyze marine cores from Baffin Bay to determine if Younger Dryas impact proxies reported from dozens of terrestrial sites globally were present in ocean cores,” Moore explains in an interview with the science journal PLOS One.

    “The sites were significant because they were a considerable distance from potential anthropogenic [human] contamination, and in most cases, the cores were highly laminated, indicating that the record was relatively undisturbed.”

    The researchers used radiocarbon dating to determine the ages of the layers, and then used a technique called single-particle inductively coupled plasma time-of-flight mass spectrometry to look for signs of comet dust in the layers deposited during the time of the Younger Dryas cooling.

    Some of the metallic dust particles extracted from the cores. (Moore et al., PLOS One, 2025)

    This analysis revealed tiny particles of metal with compositions consistent with a cometary origin, including iron with low oxygen and high nickel content, and microspherules rich with iron and silica.

    These microspherules, the researchers say, consist mostly of material from Earth, but with a little bit of impactor material mixed in – likely from an airburst event as the comet exploded after atmospheric entry.

    “The Younger Dryas sediment layer in the Baffin cores contains multiple proxies consistent with an impact event. Microspherules, twisted and deformed metallic dust particles with chemistry consistent with comet or meteoritic material, meltglass, and identification of nanoparticle peaks in key elements (e.g., platinum and iridium) suggest an impact event,” Moore says.

    “This evidence is supported by the findings on terrestrial sites on multiple continents in both hemispheres. This work builds on other evidence that the Younger Dryas impact event was likely global in scale.”

    Impact meltglass particles found in the Baffin cores. (Moore et al., PLOS One, 2025)

    The researchers next plan to broaden the scale of their investigation by examining sediment cores from other ocean sites around the world.

    Their findings have been published in PLOS One.

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  • Earth’s Oldest Impact Crater Turns Out to Be Much Younger, Scientists Reveal in New Study

    Earth’s Oldest Impact Crater Turns Out to Be Much Younger, Scientists Reveal in New Study

    A location in Western Australia that used to be named as the oldest meteorite impact crater on Earth is now actually a lot younger than that, scientists announced today in Science Advances. The structure — previously dated to 3.5 billion years ago and located within Western Australia’s North Pole Dome region of the Pilbara — was believed to be older than any of Earth’s known impact craters. Today, new research published in the journal Geochemistry found that what we now call the Miralga impact structure is, in fact, much younger, at 2.7 billion years old, and considerably smaller in diameter. This recasts earlier ideas on the early Earth’s geological activity and questions previous theories regarding impact-driven crust formation or perhaps even early life.

    Miralga Crater Loses Oldest Impact Title but Gains New Scientific Relevance

    As per The Conversation article republished by Space.com, the teams that explored the crater could only point to one thing that was likely — it had been formed by an impact. However, they ultimately disagreed as to whether this event had been and how large it was. Younger rocks contain shatter cones, indicating Earth’s early continental geology shielded the impact to a specific 2.7 billion-400 million-year period despite earlier assertions.

    They made the determination to honour the cultural revision of one site from 100 km across to a more manageable 16 km wide crater named Miralga. It’s the site – still affected by seawater – of events too recent to influence the Earth’s crust.

    The Miralga basalt feature (unique to basalt) is a rare site for an instrument to practice on before heading to Mars, while advancing our understanding of impacts and early life prospects.

    Isotopic dating to clarify the crucial part played by this, the oldest crater on Earth and unique in a geological sense, in planetary science and early Earth history is presently ongoing at Miralga.

     

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  • Traces of dipnoan fish document the earliest adaptations of vertebrates to move on land

    Traces of dipnoan fish document the earliest adaptations of vertebrates to move on land

    Interpretation of the Reptanichnus acutori igen. et isp. nov

    The newly discovered trackway is a crucial trace fossil for the analysis presented in this paper. It was produced by a fish moving in extremely shallow water or even across exposed sediment, with at least part of its body emerging. In this state, buoyancy is either reduced or absent, preventing the fish from swimming. Under such conditions, all parts of the body involved in locomotion left different traces (Figs. 3, 4 and 5). The elongated depression was formed by the trunk being dragged across the sediment, partly due to lateral body twists, as reflected in the sinuous stretches, and partly by sliding in straighter stretches. Swimming is excluded because the sinuous pattern characteristic of swimming is absent, unlike in the well documented fish swimming trace Undichna. The various ichnospecies of Undichna are preserved on bedding surfaces of very fine-grained deposits and display single, paired, or tangled sinusoidal waves. The shape, amplitude, regularity and mutual relationship of these waves reflect the type of fins and manner of swimming of the fish that left them7.

    The longitudinal furrows (Fig. 6A, B), previously interpreted as the invertebrate locomotion trace fossil Protovirgularia4 are here reinterpreted as traces of fins that were raised and lowered, touching the bottom and leaving isolated impressions during the locomotion of the fish. The ribs in some of the furrows may reflect the structure of the fins. The bilobate depressions (low-angle Osculichnus) are traces of the snout, which was pushed into the sediment to anchor and create leverage for lifting the body. The fins were used as an auxiliary tool to adjust the movement.

    This interpretation of the trackway is supported by observations of the modern West African lungfish Protopterus annectens, which leaves characteristic traces when moving on land by rotating its body and supporting itself using its head8. The body and fins of primitive fishes rarely leave clear traces on the ground. The exception is when the fish slips during a rotational movement, in which case shallow, sinusoidal traces of the body dragging may appear on soft ground. On sand, due to the lack of cohesion of the substrate, the traces are more irregular and less distinct than on mud. The traces left during pauses in movement do not differ morphologically from those left during continuous movement. As a result, it produces circular headprints that form a left-right alternating series. These imprints are variable and can take the form of single semi-circular indentations or double, more elongated imprints when the fish has its mouth open, with the upper and lower jaws forming separate imprints. The spacing between the imprints is irregular, ranging from 1 to 15 cm, although it is most often around 10 cm8.

    Interpretation of the Broomichnium ujazdensis isp. nov

    The pairs of furrows were produced by ventral fins of a fish resting on the sediment with its body was raised at low angle enough that only one pair of fins left an impression (Fig. 6C). This corresponds to the behavior of modern lungfish, where the rear part rests on the sediment9. A few traces of this type were also found in double pairs. They are imprints of the pectoral and pelvic fins, formed when the entire fish rested on the bottom. It is likely that there are more resting traces, but the recognition of convincing pairs is difficult due to the high density and overlapping of the furrows.

    Similar trace fossils are known as Broomichnium flirii10 from late Pleistocene glacial lacustrine sediments. These are characterized by two bilaterally symmetrical two pairs of thin, linear or curved imprints corresponding to the pectoral and pelvic fins, with additional straight imprints in the middle, attributed to the anal fin. They occur either in a series or as solitary traces and have been interpreted as locomotion traces of a bony fish from the family Cottidae, using their pectoral and pelvic fins to “hop” or “crawl10.

    The trace maker

    The identification of the trace maker was discussed already at the stage of the description of the Osculichnus4. Characteristic features of the imprints that help to identify the trace maker are the trapezoidal outline of the snout in dorsal view, the deep, curved profile of the lower jaw in lateral view, and the presence of a pair of arches in the ventral margin of the upper lip. All of these characteristics match in short-snouted Devonian lungfishes such as Dipnorhynchus or ‘Chirodipterus’ australis4. Since Osculichnus is now one of the elements of the described trackway, their production by the same group seems obvious.

    Dipnoan fishes have a fascinating evolutionary history that began about 415 million years ago in an aquatic environment. During this time, they made the transition from marine environments to inland waters, where they continue to thrive today11,12. At the same time, their anatomical structure has undergone only minor changes, which is why they are sometimes referred to as “living fossils“11,13. Some representatives of this taxonomically small group (Protopterus and Lepidosiren) are capable of surviving in periodically drying water. reservoir. In particular, Protopterus8 can crawl in search of water and, as a last resort, dig a burrow where they enter torpor, awaiting favourable conditions. This ability has been known since the early Triassic, when they first appeared in the fossil record14. The fossil record of dipnoan fishes is sparse, particularly from the early stages of their appearance in the Early Devonian. Only a few forms are known from this time: Melanognathus15 Uranolophus16,17 Jessenia18 Sorbitorhynchus19 Tarachomylax20 and Dipnorhynchus21 preserved as more or less complete skull remains. Until the description of the hunting trace fossil Osculichnus tarnowskae4 details of the dipnoans’ way of life were inferred primarily from their skeletal remains.

    Adaptaions to invasion on land

    Adaptations of vertebrates for moving on land are complex and not limited to a single evolutionary lineage, having evolved independently in at least two groups of Devonian vertebrates. The ability to move in very shallow water, where part of the body is emerged and swimming is not efficient, may have been present in early/lower vertebrates22. Many fossil fish groups, such as the Late Devonian elpistostegids Tiktaalik, Panderichthys, and Elpistostege adapted to semi-terrestrial environments. Their elongated bodies and eyes positioned on top of their heads helped them to move with a semi-submerged body. Such adaptations suggesting a transition to land were observed in Tiktaalik23,24,25. The process of vertebrate terrestrialisation was therefore multi-staged, suggesting that the ability to walk and/or near-walking in very shallow water may have existed even before the appearance of tetrapods. In this context, morphological studies and molecular data on lungfishes show that they are a modern-day sister group to tetrapods26,27. These assumptions are strongly supported by the described trackway, which represents the oldest evidence of pre-tetrapod preadaptations and attempts to move in terrestrial or near-terrestrial conditions. By moving towards land, the fishes avoided competition and predation, gaining access to new feeding areas. Feeding was possible during low tide, while non-adapted taxa have had to retreat to the subtidal zone.

    Handedness of early dipnoans

    The presence of fish snout traces pushed into the sediment, coordinated with the body twisting to the left, was already reported4 as evidence of an almost exclusive left-handedness phenomenon based on ten trace fossils from the Ujazd section. These observations were later supplemented by an additional 26 traces from the Ujazd and Kopiec sections. The merged dataset of 35 left-turning traces appears to be statistically significant and may represent the earliest known instance of handedness among vertebrates.

    Asymmetries in whole-body actions, particularly those with a right-sided predominance, are common across various vertebrate groups, including amphibians, reptiles, birds, and mammals. Existing literature28 on the evolution of lateralization in vertebrates—the preference of one side of the body over the other—provides information on humans and marine mammals but lacks detailed data on fishes. This right-sided preference28 primarily controlled by the left hemisphere of the brain, may have originated in early vertebrates, possibly including fishes, even before the development of limbs. However, data from the studied sections suggest that the process of handedness in early vertebrates was more complex and that later right-handedness was not present from the outset.

    Overall significance

    The surfaces containing the described trace fossils are exceptionally well-preserved because they were covered by tuffite. This coverage prevented further bioturbation, which might have obliterated the traces left by fishes. As a result, the traces have been conserved, and the surfaces represent a form of “true substrate“29 capturing the original sediment-water or sediment-air interface and recording a period of stasis before subsequent deposition.

    The significance of the presented trackway Reptanichnus acutori igen. et isp. nov. lies in its documentation of both the locomotory abilities of fishes as well as their preadaptation to terrestrial conditions. It also presents the oldest known evidence of vertebrate movement in the transition between sea and land. Furthermore, it is relevant to the ongoing discussion regarding the interpretation of early tetrapod traces, such as those from Zachełmie2. The suggested possibility that these traces originated from fishes8,30 appears less likely in light of the evidence presented in this paper, as the morphology and development of these traces differ from the Middle Devonian material2,31.

    A neoichnological experiment showing that the tracks left by crawling Protopterus resemble those of tetrapods8 in light of our observations, demonstrated the identical behaviour of this creature on land to that of its Devonian ancestors.

    The pattern of tetrapod footprints is different from those of moving fishes primarily through the presence (someplace only subtle) of fingers imprints and regular alignment. However, the additional structures left by the fins and thorax are absent.

    An important characteristic of the traces left by the crawling dipnoans is the absence of a clear body midline, which is often present in quadruped traces. Additionally, the trackways of early fishes can display irregular distances between head imprints, although they may become more regular when the animal moved continuously in a single direction. In a palaeontological context, such traces—featuring alternating, evenly spaced, rounded impressions—can be mistaken for those of early tetrapods, particularly in the absence of distinct digit imprints.

    Some trace fossils record various behaviours of the trace-maker, with a classic example being the tellinacean bivalve trace fossil Hillichnus lobosensis32 whose morphological elements reflect locomotion, feeding, and ventilation. The described trackway exhibits different morphological elements that are genetically related, although only locomotion is inferred. Nevertheless, different parts of fish’s body played distinct roles during locomotion. Therefore, it can also be considered as compound trace fossil, which should be classified under a single ichnotaxonomic name. It further represents an example of structural and developmental complexity33.

    The described trackway Reptanichnus acutori igen. et isp. nov. suggests that Osculichnus is not necessarily a hunting trace when it forms a part of the trackway. Such trackways can be difficult to recognize if their remaining elements are less distinct. However, Osculichnus occurring outside of trackways can still be considered a hunting trace, as demonstrated by examples of younger, Late Devonian trace fossils from China4,7.

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