Category: 7. Science

  • In Honor Of World Asteroid Day, A Short History Of Planetary Defense

    In Honor Of World Asteroid Day, A Short History Of Planetary Defense

    World Asteroid Day started with a real bang.

    On June 30, 1908, an asteroid about 65 meters wide collided with Earth’s atmosphere and exploded several miles above Siberia; the force of the blast flattened and burned millions of trees over an area of more than 2,000 square kilometers. Today, the anniversary of the Tunguska blast has become World Asteroid Day: a science holiday co-founded by a rock music legend and an Apollo astronaut.

    In 2015, Apollo 9 lunar module pilot Rusty Schweickart helped launch World Asteroid Day with astrophysicist and Queen guitarist Brian May. The United Nations officially recognized the event a year later in 2016. Earlier this month, Arizona senator Mark Kelly – also a former astronaut – introduced a Senate resolution that, if passed, would officially recognize June 30 as World Asteroid Day in the U.S.

    I spoke with Kevin Schindler, resident historian at Lowell Observatory in Arizona, about the origins of World Asteroid Day, the history of planetary defense, and what asteroids can reveal about the history of our Solar System.

    Discovering the Danger from Outer Space

    Around 200 years ago, in the 1830s, geologists began to study fossils and figure out that several mass extinctions had wiped out whole ecosystems of species on Earth in the distant past.

    “In recent decades, they realized that those weren’t necessarily caused by something on Earth, but by something impacting from space – like the Cretaceous Tertiary boundary,” says Schindler.

    In the 1960s, geologist Walter Alvarez discovered a thin layer of black clay in rocks around the world. Below the black line, the rocks were rich in fossils; above it, they were nearly barren. The same layer of black clay showed up all around in the world: in rock outcroppings in Italy and New Zealand, and in samples from the floor of the Pacific Ocean. And it clearly marked a deadly before-and-after moment in Earth’s history – one that happened around 66 million years ago.

    Alvarez suspected that the black clay was something alien; it contained bizarrely large amounts of an element called iridium, which is vanishingly rare here on Earth but more common in asteroids. He began to realize that an asteroid or comet may have slammed into our planet 66 million years ago, kicking off a mass extinction and scattering iridium-rich black dust over the planet like a burial shroud.

    The pieces came together in 1978 when geophysicists Glen Penfield and Antonio Camargo discovered the outline of a crater hundreds of kilometers wide at the edge of Mexico’s Yucatan Peninsula. Its center lies at the bottom of the Gulf of Mexico. Penfield and Camargo named the crater for one of the communities that now lies within its boundaries: Chicxulub Pueblo.

    Other craters – smaller but still impressive – also make it obvious that our planet has had more than a few run-ins with meteors during its long history.

    “And while there’s not as much debris floating around in our Solar System as when it was newly-formed, there’s still stuff out there,” says Schindler. “And it’s inevitable that at some point that stuff will come back and get us again.”

    From Deep Impact to DART

    So we’ve known almost 60 years that asteroids and comets could threaten life on Earth.

    “In the 1980s and 1990s, there was a search to look for bodies that specifically could impact Earth,” says Schindler. “Phase one of all this started with, ‘okay, let’s look for these bodies that could hit us,’ and then a couple decades later is when we got to phase two, ‘what can we do about it if we do find these things?’”

    Strangely enough, it was a pair of high-budget, low-scientific-accuracy Hollywood blockbusters that really brought planetary defense to public attention, according to Schindler. The summer of 1998 featured not just one but two movies about humanity trying to save itself from extinction by blowing up an incoming chunk of space rock. In Armageddon, a wildly-improbable effort by a team of offshore drillers saves Earth from an asteroid impact; in Deep Impact, a similarly-improbable effort fails to save Earth from a comet (so the summer ends in a cinematic tie).

    “The good thing about those movies is that, even though they’re not scientifically accurate in every way, they certainly built awareness enough to where lawmakers said, you know, we should put some money aside to study this stuff more,” says Schindler. “Hollywood, in some ways, has helped the cause to learn more.”

    And, as science fiction often does, Deep Impact and Armageddon provided thought experiments (albeit not super-accurate ones, to put it mildly) for the ideas that would eventually become actual efforts at planetary defense. According to Schindler, theoretical ideas about whether we could destroy an incoming meteor eventually shifted to ideas about just nudging the deadly object off-course.

    “This is just something that’s really been developed in the last decade or so and – I wouldn’t say culminated, but really became well-known with the mission that went up to deflect the moon of an asteroid to see if it was possible,” says Schindler.

    That mission was NASA’s Double Asteroid Redirection Test, or DART, in which an intrepid little spacecraft flew 7 million miles to crash into the asteroid Dimorphos and knock it off-course. Dimorphos is actually a mini-moon that orbits another, larger asteroid called Didymos. Astronomers at Lowell carefully measured Dimorphos’s orbital path around its parent asteroid before and after the impact – and they saw evidence that DART had succeeded in knocking Dimorphos into a different orbit.

    It’s a long, long way from deflecting one tiny asteroid moonlet onto a different path around its parent asteroid to deflecting something the size of the Chicxulub impactor – or even Tunguska – as it’s barreling toward Earth. But the consensus seems to be that DART was a good start.

    “The biggest thing, I think, was that it is possible. This was a very controlled initial step,” says Schindler. “This was certainly promising enough that we should keep doing these tests in different sizes of body and different compositions, because depending on what it’s made of, a body might react differently to something impacting it.”

    Fossils of the Early Solar System

    Meanwhile, Schindler and World Asteroid Day also want the public to know that asteroids are more than potential threats: they’re an orbiting treasure trove of information about the history of our Solar System and even the origins of life.

    Most asteroids are chunks of rock that coalesced early in our Solar System’s history but never grew massive enough to become planets; they’re like the seeds of planets that might have been. Others are the debris left behind by collisions between objects in those chaotic early days of the Solar System, when planets were forming and gas giants migrated, scattering lesser objects in their wake.

    “They tell us what the early composition was and what a chaotic time it was in the early part of our Solar System,” says Schindler.

    Those clues are written not just in the chemical and physical makeup of asteroids, but in their orbital paths around the Sun. By studying and modelling how those paths have changed over the years, scientists can reconstruct how asteroids and planets may have interacted. The orbits of modern asteroids are like the “footprints” of planet formation, migrating gas giants, and long-ago collisions.

    Today, NASA’s Lucy mission is exploring the asteroid belt, getting up close and personal with several of these objects. Meanwhile, NASA’s OSIRIS-APEX mission is on its way to study the asteroid Apophis, which will pass close (but not too close!) to Earth in 2029.

    “And now we are studying planetary systems around other stars. Better understanding our Solar System, we can now look at others and see how typical we are,” says Schindler. “You don’t know that without knowing your own Solar System pretty well, so it really has helped us to learn about, sort of, our heritage, I guess.”

    World Asteroid Day

    World Asteroid Day aims to tie all of those things together, promoting awareness of planetary defense but also of the immense scientific value – and maybe monetary value, eventually – of asteroids.

    At Lowell Observatory, that awareness is hard to escape; the observatory stands just an hour’s drive from Meteor Crater – which is exactly what the name suggests, a 213-meter-deep, 1200-meter-wide crater where an object about the size of a Boeing 747 slammed into the desert floor around 50,000 years ago.

    “The proximity of Lowell Observatory, where we’re studying bodies in space, and Meteor crater, where we’ve seen the result of one of those bodies hitting Earth – how convenient is that? We’re looking at both ends of it, from when it’s still up in space to the final product if something like this hits.”

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  • Laughter lifts bonobo moods, offering clues to human emotion

    Laughter lifts bonobo moods, offering clues to human emotion

    When humans burst into laughter together, moods lift almost automatically. New research shows that a similar boost happens in our closest cousins.

    An international team led by Indiana University scientists has discovered that bonobos become more upbeat after hearing the giggles of their companions. This finding pushes the evolutionary history of positive emotions back millions of years.

    Laughter changed ape choices


    To explore laughter’s influence, the researchers designed a cognitive-bias test often used in animal psychology to gauge optimism or pessimism.

    First, they trained bonobos at the Ape Initiative in Des Moines, Iowa, to recognize two kinds of boxes: black ones that always contained a delicious snack and white ones that were always empty.

    Once the apes consistently chose black and ignored white, the experimenters introduced a third, ambiguous gray box. They then played one of two sounds: recorded bonobo laughter or a neutral control noise.

    “We know that other apes, like chimpanzees, have contagious laughter during play,” said lead author Sasha Winkler, a primatologist at Duke University. “We were wondering if that behavior could be explained by positive emotions produced from the sound itself.”

    If the bonobos felt a surge of good feeling after hearing laughter, the team expected them to treat the uncertain gray box as if it were the rewarding black one.

    That is exactly what happened. “Think of it like the rose-colored glasses effect,” Winkler said. “The bonobos were much more likely to approach the gray boxes after hearing laughter, treating them like the rewarded boxes, and indicating a more optimistic expectation of finding a treat.”

    Tracing optimism to our ancestors

    This study is the first experimental proof that great-ape laughter can shift mood and cognition the way human laughter does.

    “The tendency to behave more optimistically after hearing laughter suggests that the sound alone induced a positive emotional state in bonobos,” said senior author Erica Cartmill, the director of Indiana University’s Cognitive Science Program.

    “This is the first study of which we’re aware to measure a positive affect shift in nonhuman primates from a brief experimental intervention.”

    Great apes –  bonobos, chimpanzees, gorillas, orangutans – all emit play calls that acoustically resemble human chuckles. Earlier work tied those sounds to a common evolutionary origin. The new findings add a cognitive twist.

    “Our results suggest that laughter in other apes shares not only phylogenetic and behavioral similarities with human laughter but also perhaps some of the same cognitive-emotional underpinnings,” Winkler noted.

    “This emotional contagion appears to have been present in the primate lineage long before the evolution of language.”

    Laughter, empathy, and apes

    Emotional contagion is often described as a foundational element of empathy – the capacity to share another’s feelings. As Winkler put it, “studies like ours can help to untangle the evolutionary building blocks of empathy, communication, and cooperation in humans.”

    By revealing that a simple vocal cue can brighten outlooks in bonobos, the research suggests that the mechanisms linking social sound to positive mood were already in place in a common ancestor millions of years ago.

    Cartmill added that the work answers a long-standing bias in emotion research. “Our emotions influence many aspects of cognition, including memory, attention, and decision-making, but research has historically focused on negative emotions with clear behavioral correlates, like fear and aggression.”

    “We wanted to better understand the relationship between positive affect and cognition in our closest living relatives.”

    Kanzi and the future of empathy

    The experiments involved four bonobos, including the celebrated language-using ape Kanzi, who recently passed away.

    “I feel incredibly grateful to have had the opportunity to work with Kanzi while he was still alive,” Winkler said.

    “We hope this brings greater public awareness of the remarkable similarities between us and bonobos, who are an endangered species. We have so much to learn from these incredible animals.”

    Future studies will test whether laughter exerts similar cognitive effects in chimpanzees and other primates. They will also explore how social context – for example, hearing laughs from friends versus strangers – modulates optimism.

    For now, the discovery that bonobo giggles brighten expectations highlights a shared emotional heritage and hints that a simple laugh has been boosting group spirits since long before humans walked the Earth.

    The study is published in the journal Nature Scientific Reports.

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  • Scientists thought they found a ‘zombie’ in space. Turns out, it was something even stranger

    Scientists thought they found a ‘zombie’ in space. Turns out, it was something even stranger

    In June last year, astronomers scanning the sky from the remote deserts of Western Australia picked up a sudden, blinding burst of radio energy. The signal was so powerful, it temporarily outshone every other radio source in the sky, according to a report of CNN.

    At first, the team at Curtin University believed they had discovered something extraordinary — perhaps a new type of astronomical object or an ultra-rare fast radio burst (FRB) from within our galaxy.

    “We were really excited,” Dr. Clancy James, associate professor at Curtin’s Institute of Radio Astronomy, told CNN. “It looked like we had found an unknown object near Earth.”
    The data came from the ASKAP telescope, an advanced array of 36 large antennas spread across the Wajarri Yamaji Country in Western Australia. This setup is usually used to detect FRBs — intense, millisecond-long bursts of radio energy from distant galaxies, potentially caused by exotic phenomena like magnetars, the ultra-magnetic remains of dead stars.

    These bursts are not only puzzling but also powerful tools for mapping the “missing” matter in the universe. But this particular signal wasn’t behaving like a normal FRB.


    Unlike typical FRBs that originate billions of light-years away, this burst appeared to be shockingly close — just 4,500 kilometers (2,800 miles) from Earth. When the team zoomed into the data, the image became blurry — a telltale sign the source was much closer than expected.After sifting through satellite databases, the astronomers matched the source to Relay 2, a long-defunct U.S. communications satellite launched in 1964. Relay 2 had been orbiting silently since its instruments failed in 1967.But this sparked an even more bizarre question: Could a dead satellite suddenly burst back to life?

    A Flash from the Past
    The leading theory is an electrostatic discharge — a burst of energy caused by a buildup of electric charge on the satellite’s surface, similar to the shock you get from touching a doorknob after walking on carpet. When the charge releases, it can emit a sharp flash of radio energy.

    While these discharges are common and often harmless, the intensity and brevity of this one — just 30 nanoseconds long — was unprecedented. In fact, it was 2,000 to 3,000 times brighter than any other signal the ASKAP instrument typically detects.

    Another possibility, though less likely, is that a micrometeorite no larger than a grain of sand slammed into Relay 2 at extreme speed, causing a burst of plasma and radio waves. However, the team estimates there’s only about a 1% chance that was the cause.

    Why This Matters
    Although this turned out to be a human-made source, the discovery underscores a major challenge in space research: the interference of space junk with astronomical observations. With over 22,000 satellites launched since the dawn of the space age — and thousands no longer functional — Earth’s orbit is becoming a crowded and unpredictable place.

    Signals like the one from Relay 2 could easily be mistaken for cosmic phenomena, especially as ground-based observatories like ASKAP and upcoming arrays such as SKA-Low (Square Kilometre Array) continue to scan the skies for fast, faint signals.

    While this unexpected “zombie signal” turned out to be from a defunct satellite, it opens up new possibilities for using radio telescopes to monitor aging spacecraft for signs of unusual activity.

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  • Human fishing reshaped Caribbean reef food webs, 7000-year old exposed fossilized reefs reveal

    Human fishing reshaped Caribbean reef food webs, 7000-year old exposed fossilized reefs reveal

    video: 

    Fieldwork at an exposed fossilized Caribbean reef located in the Dominican Republic


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    Credit: Sean Mattson

    When we think of fossils, giant prehistoric creatures like dinosaurs may come to mind. But the fossil record also holds the remains of smaller organisms, such as fish and corals, that tell us about our oceans’ past.

    Scientists at the Smithsonian Tropical Research Institute (STRI) recently studied exposed fossilized coral reefs from Panama’s Bocas del Toro Province and the Dominican Republic, comparing them with nearby modern reefs. These exceptionally well-preserved reefs date back 7,000 years, offering a unique window into what Caribbean reefs looked like before human impact. Within the fine sediments of these ancient reefs, the team discovered thousands of tiny fish ear bones and shark scales, allowing them to reconstruct entire ancient fish communities.

    The results revealed a dramatic shift in fish communities over time: sharks have declined by 75% and human-targeted fish have become 22% smaller. But the real surprise came from the prey fish species — those eaten by predators like sharks. These have doubled in abundance and grown 17% larger on modern reefs. This study provides the first historical evidence for the “predator release effect” — where removing top predators allows their prey to flourish. Whilst scientists have long predicted such an effect, evidence for it was scarce without knowing what reefs looked like before human impact. Remarkably, the tiniest reef fish that shelter in coral crevices, showed no change in size or abundance over millennia. Their stability suggests a remarkable resilience to the multitude of changes occurring on reefs at higher layers of the food chain.

    To compare fossilized and modern reefs, scientists collected, quantified and measured thousands of skeletal remains, including the tiny tooth-like scales that give shark skin a sandpapery texture, called dermal denticles.

    To study the abundance and size of prey fish and small coral reef-sheltered fish (also known as cryptobenthic fishes), they also examined fish otoliths — the calcium carbonate structures found in fishes’ inner ears. Because otoliths grow in layers, scientists can estimate a fish’s size at death. In total, the team examined 807 denticles and 5,724 otoliths.

    The behavior of some organisms can also leave a fossil record. In this study, scientists measured the frequency and size of damselfish bite marks on coral branches from both fossilized and modern reefs. They found that the number of bites has increased in modern reefs — also indicating the rise in prey fish populations.

    These results illustrate an important change in food webs of modern Caribbean reefs: with fewer sharks and other predatory fish to control the population of exposed prey fishes, they have become bigger and more abundant, reflecting release from predation. On the other hand, small reef-sheltered fish remained unchanged in size and abundance over thousands of years, suggesting that the degradation of water quality and habitat in the region did not drive the changes in community structure.

    This study demonstrates the power of the fossil record for future conservation. By revealing what reefs looked like before intensive human fishing, these 7,000-year-old fossils provide the missing baseline critical to understand the food webs of pre-human coral reefs, and document which elements of reefs changed and which are resilient.

    This research, published in the Proceedings of the National Academy of Sciences, PNAS, was a collaboration among scientists from the Smithsonian Tropical Research Institute (STRI), the Sistema Nacional de Investigación (SENACYT) in Panama, the Marine Science Institute at the University of Texas at Austin, the Center for Biodiversity Outcomes at Arizona State University, the Graduate School of Oceanography at the University of Rhode Island, The Nature Conservancy, the Biodiversity Research Center at Academia Sinica in Taiwan, the Department of Earth & Environmental Sciences at Boston College, and the Cotsen Institute of Archaeology and Department of Anthropology at the University of California, Los Angeles.


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  • Groundbreaking analysis provides day-by-day insight into prehistoric plankton’s capacity for change

    Groundbreaking analysis provides day-by-day insight into prehistoric plankton’s capacity for change

    image: 

    Washed foraminifera being picked for computer tomography and geochemical analysis


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    Credit: University of Southampton

    27 June 2025

    UNDER EMBARGO UNTIL 20:00 UK TIME (15:00 U.S. EASTERN TIME) ON MONDAY JUNE 30, 2025

    Scientists at the University of Southampton have developed a new way of analysing fossils allowing them to see how creatures from millions of years ago were shaped by their environment on a day-to-day basis for the first time.

    The research published today [30 June] in Proceedings of the National Academy of Sciences could revolutionise our understanding of how character traits driven by environmental changes shaped evolutionary history and life on earth. 

    It could help scientists to understand how much of a species’ evolutionary journey is down to ‘nature vs nurture’.

    Researchers from the University of Southampton studied the fossilised remains of prehistoric plankton using high-resolution 3D scanning, like a medical CT scan, to examine tiny fossil shells about the size of a grain of sand.

    These plankton, called foraminifera or ‘forams’ for short, are tiny floating seashells that still live in the ocean today. Their shells are made of calcium carbonate and grow every few days by adding a new chamber to their shell in a spiralling pattern.

    These chambers act a little like the rings of a tree trunk, providing a permanent record of the growth and lived environment of forams over time.

    The shells’ chemical composition also tells us about the conditions the organism lived in, including the chemistry, depth and temperature of the water.

    “The fossil record provides the most powerful evidence of biodiversity change on Earth, but it traditionally does so at a scale of thousands and millions of years,” says Dr Anieke Brombacher, lead author of the paper how carried out the research at the University of Southampton and now works at the National Oceanography Centre.

    “These fossils however act a bit like chapter summaries of a species’ evolutionary story. This new way of analysing them lets us read the pages within each chapter – allowing us to see how individual organisms adapted to their changing environment, not over the course of generations but within an individual life span at day-to-day resolution.”

    The key advance the researchers developed was to combine highly advanced CT scanning with chemical analysis by laser ablation techniques. This combination of methods meant the team was able to ‘zoom in’ and ‘read’ the individual pages of those chapters to reveal how the forams grew and estimate the environment they experienced while growing.

    The growth rates of all three species were similar at low temperatures, but one species grew much faster in higher temperatures despite reaching the same average size.

    “If you’re a foram, temperature appears to be a bigger determinant of your growth rate than even how old you are,” says Dr Brombacher.

    “Temperatures change throughout the depth of the ocean water column so being able to optimise growth at different temperatures would have allowed each foram to live in a greater variety of habitats.”

    James Mulqueeney a PhD researcher from the University of Southampton and co-author of the study said: “We also found that of the two species with similar environmental sensitivities, one was able to reach the same size but with a thinner shell, indicating a lower energetic cost and potential evolutionary advantage.”

    Researchers say the same analysis techniques could be applied to other creatures which preserve their environmental and lifespan information including ammonoids, corals and bivalves like clams, oysters and mussels.

    “This sort of data is routine in how we study adaptation in modern populations but has only now been gathered for fossils. By bringing together experts and facilities across the University of Southampton, we’ve been able to make progress on a foundational question in biology that wouldn’t have been possible within a single discipline,” says Prof Thomas Ezard, supervising author on the paper from the University of Southampton.

    The research is part of a wider project which aims to scale up the analysis across a wider sample of two thousand plankton specimens to determine if a species’ adaptive flexibility is likely to lead it to diverge into separate, distinct species over time.

    Detecting environmentally dependent developmental plasticity in fossilised individuals is published in Proceedings of the National Academy of Sciences and is available online.

    The study was funded by the Natural Environment Research Council (NERC).

    Ends

    Contact

    Steve Williams, Media Manager, University of Southampton, press@soton.ac.uk or 023 8059 3212.

    Notes for editors

    1. Detecting environmentally dependent developmental plasticity in fossilised individuals will be published in Proceedings of the National Academy of Sciences. An advanced copy is available upon request.
    2. For Interviews with Prof Thomas Ezard please contact Steve Williams, Media Manager, University of Southampton press@soton.ac.uk or 023 8059 3212.
    3. Images and video available here:  https://safesend.soton.ac.uk/pickup?claimID=cttMNqAAKbarUFDw&claimPasscode=tHti2hkZabikVEtq

    All images and videos should be credited to University of Southampton

    Additional information

    The University of Southampton drives original thinking, turns knowledge into action and impact, and creates solutions to the world’s challenges. We are among the top 100 institutions globally (QS World University Rankings 2025). Our academics are leaders in their fields, forging links with high-profile international businesses and organisations, and inspiring a 22,000-strong community of exceptional students, from over 135 countries worldwide. Through our high-quality education, the University helps students on a journey of discovery to realise their potential and join our global network of over 200,000 alumni. www.southampton.ac.uk

    www.southampton.ac.uk/news/contact-press-team.page

    Follow us on X: https://twitter.com/UoSMedia

     


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  • Antarctic sea ice may be in terminal decline due to rising Southern Ocean salinity

    Antarctic sea ice may be in terminal decline due to rising Southern Ocean salinity

    The ocean around Antarctica is rapidly getting saltier at the same time as sea ice is retreating at a record pace. Since 2015, the frozen continent has lost sea ice similar to the size of Greenland. That ice hasn’t returned, marking the largest global environmental change during the past decade.

    This finding caught us off guard – melting ice typically makes the ocean fresher. But new satellite data shows the opposite is happening, and that’s a big problem. Saltier water at the ocean surface behaves differently than fresher seawater by drawing up heat from the deep ocean and making it harder for sea ice to regrow.

    The loss of Antarctic sea ice has global consequences. Less sea ice means less habitat for penguins and other ice-dwelling species. More of the heat stored in the ocean is released into the atmosphere when ice melts, increasing the number and intensity of storms and accelerating global warming. This brings heatwaves on land and melts even more of the Antarctic ice sheet, which raises sea levels globally.

    Our new study has revealed that the Southern Ocean is changing, but in a different way to what we expected. We may have passed a tipping point and entered a new state defined by persistent sea ice decline, sustained by a newly discovered feedback loop.

    A satellite image of Antarctica with sea ice and Southern Ocean noted.A satellite image of Antarctica with sea ice and Southern Ocean noted.

    The Southern Ocean surrounds Antarctica, which is fringed by sea ice. Nasa

    A surprising discovery

    Monitoring the Southern Ocean is no small task. It’s one of the most remote and stormy places on Earth, and is covered in darkness for several months a year. Thanks to new European Space Agency satellites and underwater robots which stay below the ocean surface measuring temperature and salinity, we can now observe what is happening in real time.

    Our team at the University of Southampton worked with colleagues at the Barcelona Expert Centre and the European Space Agency to develop new algorithms to track ocean surface conditions in polar regions from satellites. By combining satellite observations with data from underwater robots, we built a 15-year picture of changes in ocean salinity, temperature and sea ice.

    What we found was astonishing. Around 2015, surface salinity in the Southern Ocean began rising sharply – just as sea ice extent started to crash. This reversal was completely unexpected. For decades, the surface had been getting fresher and colder, helping sea ice expand.

    A line graph showing a steady and then sudden decline in sea ice extent.A line graph showing a steady and then sudden decline in sea ice extent.

    The annual summer minimum extent of Antarctic sea ice dropped precipitously in 2015. NOAA Climate.gov/National Snow and Ice Data Center

    To understand why this matters, it helps to think of the Southern Ocean as a series of layers. Normally, the cold, fresh surface water sits on top of warmer, saltier water deep below. This layering (or stratification, as scientists call it) traps heat in the ocean depths, keeping surface waters cool and helping sea ice to form.

    Saltier water is denser and therefore heavier. So, when surface waters become saltier, they sink more readily, stirring the ocean’s layers and allowing heat from the deep to rise. This upward heat flux can melt sea ice from below, even during winter, making it harder for ice to reform. This vertical circulation also draws up more salt from deeper layers, reinforcing the cycle.

    A powerful feedback loop is created: more salinity brings more heat to the surface, which melts more ice, which then allows more heat to be absorbed from the Sun. My colleagues and I saw these processes first hand in 2016-2017 with the return of the Maud Rise polynya, which is a gaping hole in the sea ice that is nearly four times the size of Wales and last appeared in the 1970s.

    What happens in Antarctica doesn’t stay there

    Losing Antarctic sea ice is a planetary problem. Sea ice acts like a giant mirror reflecting sunlight back into space. Without it, more energy stays in the Earth system, speeding up global warming, intensifying storms and driving sea level rise in coastal cities worldwide.

    Wildlife also suffers. Emperor penguins rely on sea ice to breed and raise their chicks. Tiny krill – shrimp-like crustaceans which form the foundation of the Antarctic food chain as food for whales and seals – feed on algae that grow beneath the ice. Without that ice, entire ecosystems start to unravel.

    What’s happening at the bottom of the world is rippling outward, reshaping weather systems, ocean currents and life on land and sea.

    An aerial view of sea ice.An aerial view of sea ice.

    Feedback loops are accelerating the loss of Antarctic sea ice. University of Southampton

    Antarctica is no longer the stable, frozen continent we once believed it to be. It is changing rapidly, and in ways that current climate models didn’t foresee. Until recently, those models assumed a warming world would increase precipitation and ice-melting, freshening surface waters and helping keep Antarctic sea ice relatively stable. That assumption no longer holds.

    Our findings show that the salinity of surface water is rising, the ocean’s layered structure is breaking down and sea ice is declining faster than expected. If we don’t update our scientific models, we risk being caught off guard by changes we could have prepared for. Indeed, the ultimate driver of the 2015 salinity increase remains uncertain, underscoring the need for scientists to revise their perspective on the Antarctic system and highlighting the urgency of further research.

    We need to keep watching, yet ongoing satellite and ocean monitoring is threatened by funding cuts. This research offers us an early warning signal, a planetary thermometer and a strategic tool for tracking a rapidly shifting climate. Without accurate, continuous data, it will be impossible to adapt to the changes in store.


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    This article is republished from The Conversation under a Creative Commons license. Read the original article.

    Alessandro Silvano is a Natural Environment Research Council (United Kingdom Research and Innovation) Independent Research Fellow.

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  • Was ancient Mars habitable? NASA’s Perseverance rover is grinding into a ‘weird, uncooperative’ rock to find out

    Was ancient Mars habitable? NASA’s Perseverance rover is grinding into a ‘weird, uncooperative’ rock to find out

    NASA’s Perseverance rover is digging deeper into Mars’ geologic past as it begins grinding into Red Planet rock surfaces to expose material that could hold clues to the planet’s ancient environment and habitability.

    Earlier this month, the Perseverance rover used its abrasion tool to scrape away the top layer of a rocky Martian outcrop nicknamed “Kenmore,” revealing a fresh surface for close-up analysis of the rock’s composition and history. The procedure, which involves a combination of mechanical grinding and gas-blast cleaning, allows scientists to study rock interiors that haven’t been altered by wind, radiation or dust over billions of years.

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  • City parks reveal surprising wildlife secrets from soil

    City parks reveal surprising wildlife secrets from soil

    As cities rapidly grow, expanding by an area almost double the size of France by 2030, natural spaces are being replaced by buildings and roads. This massive urban spread is hitting wildlife hard, wiping out their homes, cranking up temperatures, and creating dangerous concrete jungles.

    It’s a tough situation for many animals on the move. Cities can be tempting with easy food and fewer natural predators, but they also come with deadly risks like traffic and lost pathways.

    While past studies used cameras or sound to monitor urban wildlife, a new Yale study takes a different approach by analyzing environmental DNA (eDNA) from soil in 21 Detroit parks during winter and summer to uncover how mammal diversity changes with the seasons in urban landscapes.

    The study aimed to understand how human activity shapes mammal communities in urban areas. By sampling environmental DNA (eDNA) from soil across 21 Detroit parks, researchers uncovered subtle, park-specific shifts in species composition, influenced by both natural and human-related factors, and larger parks supported greater biodiversity.

    eDNA revealed seasonal changes and human presence effects on urban wildlife. These insights offer a promising tool for more adaptive and informed urban biodiversity planning, helping cities better balance green space with growing human footprints.

    Measuring the effects of natural events on wildlife

    Researchers analyzed soil samples from 21 urban parks in Detroit, Michigan, during February and July 2023. They detected DNA from 23 mammal species, including humans. They confirmed these results using iNaturalist wildlife sightings.

    The DNA samples revealed seasonal shifts in mammal presence. Hibernators like groundhogs and muskrats were absent in winter samples, reflecting seasonal behaviors. During winter, animals were more clustered, likely due to resource competition and limited movement.

    In summer, eDNA patterns revealed that mammals were more dispersed across landscapes, with fewer cross-species interactions due to abundant resources. Larger parks supported wider-ranging species, and coyotes appeared only in parks over 14.4 hectares.

    Human DNA made up about one-third of all samples, highlighting constant human presence. Domesticated animal DNA (from cats, dogs, pigs, and cattle) reinforced the idea that urban parks are shared socio-ecological spaces.

    Human presence influenced wildlife makeup, generalist and human-tolerant mammals thrived in busier areas, while more sensitive species were less commonly detected.

    To protect urban biodiversity, especially wide-ranging species, researchers recommend expanding green spaces and building wildlife corridors that link parks together.

    As cities continue to grow, these connected landscapes could be key to maintaining resilient ecosystems that support both nature and human well-being.

    Journal Reference

    1. Jane Hallam and Nyeema C. Harris. Network dynamics revealed from eDNA highlight seasonal variation in urban mammal communities. Journal of Animal Ecology. DOI: 10.1111/1365-2656.70082

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  • Algae pump toxins into the ocean. Can we catch them early?

    Algae pump toxins into the ocean. Can we catch them early?

    Credit: ZUMA Press, Inc./Alamy Stock Photo

    A sea lion shows symptoms of domoic acid poisoning during a harmful algae bloom in Malibu, California, on April 24, 2002.

    After starting her PhD studies in 2018, Monica Thukral would go for a swim off the coast of San Diego two to three times a week. The regular, physical connection with the waters helped to anchor her in her research at the University of California San Diego’s Scripps Institution of Oceanography.

    “I had an understanding of the physical processes: how the temperature and the wave energy change throughout the year,” Thukral recalls. “I was the first to know when an algae bloom was taking place.”

    In the laboratory, Thukral transformed that intuition into something more systematic. Using cutting-edge analytical tools, her team in the environmental systems biology lab of Andrew E. Allen—who also teaches at the nearby J. Craig Venter Institute, a genomics research foundation—strove to understand what was happening in the water on a molecular level.

    The scientists were working in the wake of a momentous oceanographic event. In 2015, a massive harmful algal bloom (HAB) had subsumed a stretch of Pacific coastline from southern California all the way to Alaska’s Aleutian Islands. It flooded the region’s waters with domoic acid, a neurotoxin so dangerous that it gives sea lions epilepsy; government regulators shuttered some commercial fisheries for months.

    How do you place a value on the loss of shellfish that you’ve been harvesting for centuries with your family?

    Vera Trainer, Director, University of Washington’s Olympic Region Harmful Algal Bloom program

    Produced by microalgae—namely, several species of marine diatoms known as Pseudo-nitzschia—domoic acid can bioaccumulate in the marine food web, eventually getting consumed by humans, in whom it can cause nausea, cardiac arrhythmia, and a condition called amnesic shellfish poisoning, which can include memory loss and disorientation. Once the acid has accumulated in shellfish tissues past an official threshold of 20 parts per million, regulators consider the meat unsafe for human consumption.

    The 2015 HAB affected the West Coast more than any other recorded bloom in history, costing an estimated $97 million dollars in damages to the Dungeness crab harvest alone. Just a few months ago, a HAB again sickened wildlife off the coast of Southern California.

    Domoic acid manifests in all of the world’s upwelling zones—coastal regions where winds push away warm surface water and draw cold, nutrient-rich waters to the surface. The neurotoxin is poised to become even more prevalent as warming oceans disturb the balance of nutrients available.

    For years, scientists have been working to understand the mechanisms behind these blooms. “We’ve long held a range of hypotheses in this field for what initiates blooms of this particular organism and its toxin production,” says Clarissa Anderson, one of Thukral’s collaborators and the director of the Southern California Coastal Ocean Observing System (SCCOOS). “We all want to know, What is that magic sauce?”

    Now Allen’s interdisciplinary team has figured out a way to potentially anticipate future toxic events. The researchers’ methods center around monitoring the algae-infused waters for environmental DNA (eDNA), material that is minute in concentration but rich in genetic information. In a paper published last year in Proceedings of the National Academy of Science, they pulled out all the stops to harvest, isolate, and analyze the genes behind the algal havoc (DOI: 10.1073/pnas.2319177121).

    The mechanics of a bloom

    Fans of classic cinema may already know domoic acid. In 1961, Alfred Hitchcock found himself inspired by a startling newspaper report about a frenzy of disoriented seabirds terrifying residents of coastal Santa Cruz, California. The director wove elements of that incident into his film The Birds 2 years later. Since then, similar incidents in Monterey Bay have linked addled avians to a diet temporarily infused with domoic acid, a product of Monterey Bay’s occasional HABs.

    When stressed, Pseudo-nitzschia may release domoic acid for a number of reasons, like to impede the growth of competing plankton or to stave off algae-grazing crustaceans. Also, domoic acid has been found to serve as an iron chelator. The element is critical to photosynthesis, so when it becomes scarce, Pseudo-nitzschia will release domoic acid extracellularly, where it can bind to iron in the environment and make it easier for the algae to absorb.

    HABs have likely always occurred as part of natural ecological cycles, but modern blooms appear to be becoming more toxic. Anderson says that over the past 20–30 years, deeper waters from the equatorial Pacific have seen rising levels of nitrogen and decreasing levels of silicate. These waters, which came up through the California undercurrent, likely contributed to the size and intense toxicity of 2015’s bloom.

    A chemical structure of domoic acid displaying its three carboxyl groups and a pyrrolidine ring.

    “This massive bloom exhausted silicate before nitrate,” explains John Ryan, a researcher at the Monterey Bay Aquarium Research Institute and coauthor of the paper. Each diatom needs silicate to build its tough cell walls, like a tiny suit of glassy armor. If they run out of silicate, the diatoms can’t divide, but the nitrogen-rich waters continue to fuel their metabolism.

    Faced with a silicon shortage threatening their ability to reproduce and an accompanying shortage in essential iron, the nitrogen-charged Pseudo-nitzschia along the Pacific coastline in 2015 took drastic action. The algae started producing as much as 10–20 times their usual amount of iron-scavenging domoic acid. As the compound built up in the Pseudo-nitzschia, each morsel of algae that nearby crustaceans ate became “phenomenally toxic,” Ryan says.

    In 2018, Thukral’s fellow researcher in Allen’s lab, Patrick Brunson, helped identify DabA, a key enzyme that kick-starts Pseudo-nitzschia’s biosynthesis of domoic acid (Science, DOI: 10.1126/science.aau0382). The paper “was a milestone study,” Allen says. It handed researchers a compass to seek out genes that, like dabA, express themselves as a Pseudo-nitzschia bloom takes shape. Now the team wanted to learn what was happening one step before that.

    Thukral, Brunson, and the rest of the team figured that because cells express genes before translating them into proteins, they could try to detect genes that Pseudo-nitzschia activated around the same time or even before dabA. These could serve as biological alarm bells that a HAB event was imminent.

    In the wake of that paper, Brunson found himself the beneficiary of scientific serendipity. Researchers at Moss Landing Marine Laboratories, 650 km up the US Pacific coast from his office at in San Diego, mentioned to Brunson’s team that they happened to have a year’s worth of plankton samples from 2015 sitting quietly in their freezers—including ones chock-full of Pseudo-nitzschia from the bloom.

    These were exactly the kind of time-indexed samples that the team needed to take the next step in their research, moving from understanding what caused HABs on a genetic level to identifying the warning signs leading up to a HAB. Things could have gone differently, Allen says. Many discoveries never see the light of day: viable samples languish in freezers, or data gather dust as they wait for robust analysis that never comes, he says.

    With the samples in hand, however, the researchers now faced a new challenge. From that slurry of biological material and miscellaneous sea gunk they needed to figure out how to extract and analyze the genetic data lying inside.

    Unveiling genetics

    The samples researchers netted during and leading up to the bloom—taken off a municipal wharf in nearby Monterey—provided a veritable goldmine of eDNA, genetic material that organisms shed into their surroundings. It has become an increasingly convenient and nonintrusive tool for researchers to get a picture of ecosystem dynamics.

    For example, a 2024 study swabbed hawk beaks and talons for DNA and identified what species of animals the birds preyed upon. And in 2022, biogeochemists extracted the oldest DNA ever from river sediments and reconstructed an ecosystem that had existed in the area millions of years ago.

    In addition to analyzing eDNA, Brunson and Thukral gleaned still more information using transcriptomics, a growing subfield of bioinformatics that catalogs the entirety of an organism’s RNA. By seeking out gene transcripts, such as ribosomal RNA, that differ between species, they could chart the evolution of the 2015 bloom—like how Pseudo-nitzschia australis had become the dominant diatom by April and had maintained its dominance into autumn.

    Aware of the ocean conditions in the days leading up to the bloom—low iron and low silicon concentrations—Brunson and Thukral started to put together the puzzle pieces. Thukral’s efforts uncovered dabA’s molecular coconspirator: the gene sit1, which helps transport silicon compounds into Pseudo-nitzschia cells. She found that when silicon was at its scarcest in early summer 2015, expression of sit1 skyrocketed as the algal cells tried to eke more silicon out of the water to build their cell walls and divide.

    Thukral figured out that when Pseudo-nitzschia express both genes at the same time—dabA when the algae are starting to synthesize domoic acid and sit1 as they struggle to divide themselves—it could serve as a “robust predictor” that the Pseudo-nitzschia are about to become a toxic powerhouse.

    Sorting through and properly analyzing this treasure trove of genetic data—along with data on oceanographic conditions, community composition, and metabolomics—took the team years. “But it becomes pretty beautiful when you’re able to see patterns that are linking them together, and trying to crack the code as to what is taking place in the ocean that we can’t really see with our naked eye,” Thukral says. “All of this data allows us to chip away at that.”

    A bit of notice

    The team’s metabolomic investigations fell under the umbrella of a US National Oceanic and Atmospheric Administration (NOAA) research program dedicated to the ecology and oceanography of HABs. Their discoveries from plumbing the depths of environmental genetic data are a step toward something coveted by scientists and fisheries alike: the ability to predict blooms as much as a week before they erupt.

    “It’s been exciting, because my field has always been prediction,” says SCCOOS’s Anderson, whose work has involved both remote sensing—such as monitoring HAB formation from space—and developing models that might help predict toxin formation. “But we’re always missing a lot of this fundamental knowledge. I’m really confident that now that we can do some of this molecular forecasting, that we’re a little closer towards a truly mechanistic understanding.”

    Vera Trainer, the director of the University of Washington’s Olympic Region Harmful Algal Bloom program, who was not involved with Thukral’s study, will be happy for any help she can get. In the Pacific Northwest of the US, the current warning system has its shortcomings because it requires physically counting phytoplankton cells in water samples and measuring their toxin concentration. By the time high concentrations of toxin can be detected, however, a HAB may already be in progress. “If we had a week’s early warning using these genetic approaches, that would be great,” Trainer says.

    She adds that toxic blooms also have an outsized impact on members of the Quinault Indian Nation, on the southwestern corner of Washington’s Olympic Peninsula, who have harvested razor clams for thousands of years. “How do you place a value on the loss of shellfish that you’ve been harvesting for centuries with your family?” Trainer asks. Genetic forecasting using eDNA could allow communities to harvest either before a bloom arrives or in unaffected locations.

    “It’s an element ingrained into their lives,” Trainer says. “And when they cannot harvest, it’s damaging not just to their economic well-being, but their cultural well-being.”

    Next steps

    One of the relative weaknesses of the team’s data had nothing to do with their abilities. Their limitation lay in not having enough samples from the beating heart—the initiation sites—of the HABs.

    “Where we really want to go next is more directed bloom sampling,” Brunson explains. For samples like those taken by the Moss Landing researchers at a local wharf, “you’re getting a unique environment that might not be precisely like the epicenter of the bloom.” As such, the gene expressions of the HAB that occurred on Moss Landing’s doorstep still need to be confirmed against those of other regions.

    Brunson and Thukral’s fellow researchers back at the Monterey Bay Aquarium Research Institute have spent years developing new ocean technology that could provide these genetic samples with robotic precision. Their autonomous underwater vehicles (AUVs) can zoom forth into the ocean depths at a moment’s notice and vacuum up eDNA like an Atlantean Roomba.

    The Monterey Bay Aquarium Research Institute’s long-range autonomous underwater vehicle floats underwater near the surface of a rolling blue ocean as it conducts autonomous sampling for real-time detection of algal toxins and the collection and preservation of environmental DNA (eDNA).

    Credit: MBARI/Monterey Bay Aquarium

    The Monterey Bay Aquarium Research Institute’s autonomous underwater vehicles can prowl water bodies for signs of harmful algal blooms. They take water samples and even do onboard chemical analysis.

    The AUV is outfitted with sensors that can continuously hunt for environmental markers so it can pilot itself into the thick of a HAB. This vehicle can then take “sips” of the surrounding water and store what it finds in one of dozens of filters. Researchers then have the choice to bring those samples ashore for hands-on analysis or have the AUV’s onboard systems get a quick look at their molecular components. Ryan says the AUV is “basically a laboratory in a can” that can lyse cells and analyze their contents using a light-based technique called surface plasmon resonance that can detect domoic acid.

    “Once you prepare that vehicle with all the reagents inside, you need to wait for the right moment,” Ryan says. “Maybe it’s a mortality event: you see animals dying from domoic acid poisoning. You then remotely send your AUV on its mission to 1) map the phytoplankton distributions, and 2) report back real-time detection information.”

    NOAA does, in fact, already have a fleet of ocean gliders monitoring the oceans, “but most of them aren’t out sniffing HABs,” Anderson explains.

    SCCOOS has also stationed along the California coastline a fleet of a dozen robotic microscopes, dubbed Imaging FlowCytobots, that can photograph and identify each phytoplankton in 15 mL of water every hour.

    Another set of approaches that could one day complement monitoring and data collection are prevention, control, and mitigation. In other words, scientists could use what they know to try to proactively intervene in natural processes to stop HABs from proliferating.

    That line of thinking raises pragmatic and philosophical questions: Will advances in molecular forecasting lead to techniques that can circumvent HAB formation, and can the consequences of this sort of geoengineering be known?

    The interior equipment of a Monterey Bay Aquarium Research Institute autonomous vehicle sits on a table, exhibiting a tangle of wires and pumps and a large barrel surrounded by dozens of sample containers.

    Credit: Todd Walsh © 2018 MBARI

    Inside the hull of Monterey Bay Aquarium Research Institute’s autonomous underwater vehicles is an onboard system that can collect water the samples for hands-on testing in the lab or do surface plasmon resonance analysis on site.

    “Once that horse has left the stable, it’s left the stable,” Anderson admits. In systems the size of the world’s oceans, preventive actions would require intervention on truly massive scales. “They’re much more effective in closed, freshwater systems, and there’s a ton of work being done in that field—with a lot of industry buy-in because they can make all kinds of chemicals that can effectively deal with this. But I do believe that [prevention, control, and mitigation] aspirations in the marine environment are a lot trickier.”

    Going forward, however, the transcriptomic techniques that Brunson and Thukral used will also continue to bloom. The sheer amount of biological data circulating through the environment provides more material than could be analyzed by any one laboratory or in any one lifetime.

    “That’s one of the amazing things about such a rich data set like this: there’s always so much to explore and learn,” Thukral says.

    Jonathan Feakins is a freelance science and history writer based in Chicago. A version of this story first appeared in ACS Central Science: cenm.ag/algalblooms.

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  • Great Britain to attempt to synthesize human genome • Mezha.Media

    Great Britain to attempt to synthesize human genome • Mezha.Media

    A five-year research project called Synthetic Human Genome (SynHG) has been launched in the UK, in which researchers plan to create large fragments of human DNA in the laboratory, The Guardian reports.

    The goal of the research is to gain a deeper understanding of how the genome functions and lay the foundation for new treatments for complex diseases, including autoimmune diseases and viral organ damage.

    The project is led by Professor Jason Chin from the Medical Research Council’s Laboratory of Molecular Biology (LMB) in Cambridge. The team also includes scientists from the universities of Cambridge, Kent, Manchester, Oxford and Imperial College London. The first stage involves the synthesis of individual sections of chromosomes, which the researchers will insert into human skin cells to observe their behaviour.

    This is the first large-scale attempt to rewrite the human genome from the bottom up, from molecule to cell. Previous experience synthesizing the complete genome of E. coli has prepared Chin’s team for the human genome, which is almost a thousand times larger, at over 3 billion base pairs.

    Researchers are paying particular attention to the so-called “dark matter of the genome” – sections of DNA whose function remains poorly understood. Their analysis may provide new answers about gene regulation, epigenetics, and the occurrence of hereditary diseases.

    Working alongside the scientific team will be an ethics team, led by Professor Joy Zhang from the University of Kent, to examine the social implications and potential risks of the research, including concerns about the use of the technology to create “designer babies” or modified organisms for domestic or industrial purposes.

    Bioethicists are also considering using synthetic mitochondria to prevent maternally transmitted diseases, a solution that could reduce the need for donors and simplify IVF procedures.

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