Category: 7. Science

  • NO KIDDING! Scientists want to use PAPER PLANES for space missions because…

    NO KIDDING! Scientists want to use PAPER PLANES for space missions because…

    Scientists in Japan have come up with a simple solution to the growing debris in low Earth orbit: a paper plane. No joke! A team of researchers from the University of Tokyo made a paper plane out of an A4 sheet and had it fly out of the International Space Station (ISS) in a simulation. Did it survive atmospheric reentry? The idea was put forward by the scientists in a paper published in Acta Astronautica. They showed how origami paper can solve the trash problem in space. The study argues that metals need not be solely relied upon to build spacecraft. A standard sheet of paper is also perfect for the job as it will burn up in the atmosphere during reentry. Typically, when a spacecraft reenters Earth’s atmosphere, it leaves behind metallic particles and chemicals that damage the ozone layer. The research aims to show how a more sustainable orbital environment can be created by using paper. Also Read: Wildlife exodus at Yellowstone National Park: Have animals sensed a disaster?

    A4 paper sheet plane in space?

    The experiment comprised a paper plane made of an uncoated A4 sheet, with an aluminium tail and placed in a wind tunnel to see what would happen to it in space. The layers at the nose were folded to shift its centre of mass upstream and ensure aerodynamic stability. The researchers clarified in the paper, “Such spacecraft have not yet flown in space. It is unclear whether their flight dynamics in the highly rarefied atmosphere in [low Earth orbit] would be similar to those of a usual ground-based origami plane, and whether the plane would survive or burn up during atmospheric entry.” However, they agreed that the entire plane cannot be made out of paper, and only specific parts can be built using the sustainable solution. Also Read: Scientists detect signs that mammoth rivers flowed in Antarctica 80 million years ago

    What will happen to paper plane if it flies out of ISS?

    The simulation had the paper plane being launched from the ISS at an altitude of 400 kilometres and a speed of 17,448 miles per hour. It remained stable and glided swiftly through the space-like environment. Then at a lower altitude of 120 kilometres above Earth’s surface, it started tumbling out of control. The paper states that this is expected at this position. Also, the severe aerodynamic heating would burn up the paper plane in the atmosphere at an altitude of around 90 to 110 kilometres. After this, a physical model of the plane was placed in the Kashiwa Hypersonic and High Enthalpy Wind Tunnel at the University of Tokyo. It was subjected to Mach 7 speeds for about seven seconds to see if it would disintegrate. The plane’s nose bent and the wings started charring, although it did not break apart. The researchers said it likely would have had they kept going. Also Read: Our Sun just inflicted a 400,000-kilometre-long scar on itself. Here’s what happened

    Shortcomings of paper plane in space

    However, an origami paper spacecraft has its challenges. It cannot be used for all kinds of missions. Researchers suggest a version could be used as a passive probe to measure atmospheric density. It could also be a platform for low-cost and short-lived missions in low Earth orbit. Besides, it would be really small and won’t reflect radar as strongly compared to a traditional spacecraft. A miniaturised position, navigation, and timing transceiver could be added to it, they stated. It would also be extremely sensitive to aerodynamic drag, and won’t be able to stay in orbit for long durations. So it can only be used for short-duration missions.

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  • Trading Options for Alien Tech. The research team of the new NSF-DOE… | by Avi Loeb | Jul, 2025

    Trading Options for Alien Tech. The research team of the new NSF-DOE… | by Avi Loeb | Jul, 2025

    Co-added image of 3I/ATLAS from 30-second exposures by the NSF-DOE Rubin Observatory. Each pixel is 0.2 arcseconds in size. During each exposure, the object had moved 0.625 arcseconds (3.125 pixels) on July 2, 2025, resulting in apparent smearing of the image along the direction of motion. (Image credit: Chandler et al. 2025)

    The research team of the new NSF-DOE Rubin Observatory just posted its first paper on 3I/ATLAS, reporting the first exquisite imaging data from an 8-meter class telescope, taken between June 21 and July 7, 2025. The Rubin data from 37 images of 3I/ATLAS yields a localization precision of about 0.02 arcseconds and a percent-level flux calibration, providing improved orbit solutions and showing no detectable flux variability on hourly timescales. The Rubin team recognized the elongation in their images as a result of smearing along the direction of motion of 3I/ATLAS (as noted in my previous essay), and detected a slight transverse broadening in the image of 3I/ATLAS beyond those of background stars. A coma around 3I/ATLAS might be much more apparent in forthcoming data from the Hubble and the Webb space telescopes.

    Given the discovery potential of the Rubin Observatory, it is an opportune time to reflect on the decade-long history of the frontier of interstellar objects. Astronomers discovered 1I/`Oumuamua on October 19, 2017, then 2I/Borisov on August 20, 2019 and finally 3I/ATLAS on July 1, 2025. But the new NSF-DOE Rubin Observatory is expected to discover a new interstellar object every few months, harvesting multiple interstellar objects every year. So far, each discovery was assigned a unique name. But in Rubin’s harvest, new interstellar objects will have to be distinguished by their discovery date, potentially labeled as 4I/Rubin-022626 for the fourth interstellar object detected on February 26, 2026, for example.

    For now, given the small number of known interstellar objects so far, we learn something fundamentally new from each of them. However, once our collection includes a large statistical sample, some groups of objects will belong to distinct classes, providing us with population statistics. There will always be outliers that do not resemble Solar System asteroids or comets. Among them, there might also be products of alien technologies, either in the form of space trash or functional devices.

    Today, I received a text message from a fan who after reading my essays on 3I/ATLAS over the past couple of weeks, decided to place an options trade on the Volatility Index (VIX) of the S&P 500 index that will expire on October 29, 2025, the date when 3I/ATLAS will arrive closest to the Sun — just in case this will turn out to be a civilization altering event. This bet against market uncertainty is the first time that my scientific research, in this case my third paper on 3I/ATLAS, affects investor trading in the stock market.

    (Image credit: Bloomberg/Getty Images)

    But even if 3I/ATLAS will turn out to be a bright comet similar to 2I/Borisov as it gets closer to the Sun, time is ripe to plan ahead and establish a new academic discipline for the study of the geopolitical and scientific implications of future interstellar visitors. In particular, a new brand of interstellar archaeologists will study interstellar asteroids, comets and meteors to learn about the formation and ejection processes of rocks our of planetary systems around different types of stars. If they uncover technological artifacts among the rocks, these interstellar archaeologists will explore their implications for the history of intelligent civilizations in the Milky-Way galaxy.

    One might expect space trash to be more abundant than functional devices based on experience. After all, our own young civilization launched five spacecraft: Voyager 1 & 2, Pioneer 10 & 11, and New Horizons, to interstellar space, but these devices will stop working by the time they exit the Oort cloud in about ten thousand years. However, a more mature civilization might aspire to launch functional interstellar probes that would explore other planetary systems to accomplish its ambitious long-term and long-distance goals. If functional devices were programmed to visit the habitable zone of the Solar System, then they might be more abundant near Earth than space trash on random trajectories. The interstellar archaeologists will be able to relate the statistics of space trash and functional devices near Earth to the technological maturity of the civilizations that launched them.

    Our interaction with functional interstellar probes will require the expertise of policy makers and experts in international diplomacy, since any response must be coordinated internationally based on its economic and geopolitical implications. Given the long duration of interstellar journeys, our visitors might not have had us in mind when starting the journey unless their arrival is in response to the electromagnetic signals that we broadcasted over the past century. Any message from the sky that we are not the smartest kid on the block will have to be moderated by Interstellar psychologists in order to reduce its harmful impact on the human ego.

    The skillset of this new cohort of interstellar professionals is needed to improve the survival likelihood of humanity when faced with a new reality from interstellar space. Before the past decade, humans were unaware of interstellar objects and this ignorance allowed us to focus our mind on terrestrial conflicts. Habits are difficult to break. The prophets of the day warn us of the existential threat from artificial intelligence, climate change or asteroid impact. But they neglect the security risk from alien tech. When a visitor to our backyard would knock on our door, it might be too late to decide how to respond. Our family of nations will be in disarray because governments may not be able to protect their citizens from advanced interstellar technologies. Whether such a visit will take place in the near future or will not happen in the next billion years, is unknown. We better use the Rubin data to reliably manage our risks rather than guess the answer.

    Our ability to cope with a threat from alien tech will depend on its intent and the extent of the gap between our technologies and theirs. As responsible scientists, we must abandon the “stone age” or “ice age” mindset of comet experts who assume that everything in the sky must be icy rocks. Interstellar archaeology can also be pursued on the surface of the Moon, which collected small impactors over the past billions of years without burning them in an atmosphere or burying them through geological activity.

    Here’s hoping that our new ability to detect interstellar objects with the NSF-DOE Rubin Observatory, will cultivate cooperation among all humans as we carefully explore any new interstellar package in our mailbox. If any packages are dropped on Earth by the interstellar delivery service, the three new Galileo Project observatories will use Machine Learning software under my leadership to figure out their nature.

    ABOUT THE AUTHOR

    (Image Credit: Chris Michel, National Academy of Sciences, 2023)

    Avi Loeb is the head of the Galileo Project, founding director of Harvard University’s — Black Hole Initiative, director of the Institute for Theory and Computation at the Harvard-Smithsonian Center for Astrophysics, and the former chair of the astronomy department at Harvard University (2011–2020). He is a former member of the President’s Council of Advisors on Science and Technology and a former chair of the Board on Physics and Astronomy of the National Academies. He is the bestselling author of “Extraterrestrial: The First Sign of Intelligent Life Beyond Earth” and a co-author of the textbook “Life in the Cosmos”, both published in 2021. The paperback edition of his new book, titled “Interstellar”, was published in August 2024.

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  • The $5.3 million sale of a precious rock from Mars belonging to Niger spurs outrage

    The $5.3 million sale of a precious rock from Mars belonging to Niger spurs outrage

    In November 2023, a meteorite hunter discovered NWA 16788 in the Agadez area of northern Niger.

    It weighs more than 24.6 kilograms (54 pounds) and is the biggest Martian rock ever recovered on Earth, according to Sotheby’s.

    Experts estimate it traveled 140 million miles from Mars’ surface, likely dislodged by an ancient asteroid impact, before landing in the Sahara sands.

    The auction started at $1.9 million and quickly jumped to $4.3 million, with premiums and fees bringing the total to $5.3 million.

    However, Sotheby’s has not revealed the identity of either the buyer or the seller, heightening speculation over how such an important alien item departed its nation of origin.

    The auction took place during the auction house’s “Geek Week,” which features goods related to natural history, science, and space.

    A private gallery in Tuscany, Italy, and the Italian Space Agency had both previously exhibited the rock.

    The specimen’s provenance remains a matter of debate, however, as reported by Forbes.

    “The NWA 16788 meteorite was shipped and transported in line with the standard procedure of all meteorites that come out of Niger.

    As with everything we sell, all relevant documentation was in order at each stage of its journey,” Sotheby’s tells Forbes Africa.

    According to Giovanni Pratesi, a professor at the University of Florence in Italy and one of the authors of two of the three papers referenced in the Sotheby’s catalogue, he was “only involved in the characterization and study of this specimen (NWA 16788), without having received, for a while, any information about provenance.”

    “In fact, the place of recovery of the meteorites is not so important for science because their real provenance, of course, is not the Earth but other bodies of the Solar System,” Pratesi says.

    “Anyway, there is no doubt that the Sahara represents a very important reservoir of extraterrestrial material.

    “A confirmation of this is given by the high number of meteorite specimens bearing the name NWA (North West Africa) that is used when the exact place of recovery is not known.

    In this respect, I believe that African countries should organize a network to recover and valorize these meteorites.”

    The sale has reignited concerns about the unregulated trade of meteorites, particularly those discovered in developing countries.

    Nigerien officials and international cultural watchdogs are now questioning the legality and ethics of the meteorite’s export, with many demanding its immediate return.

    “It was discovered in Niger? How come it ended up being sold in New York?” says Alia Baré, a fashion designer and daughter of former Nigerien president Ibrahim Baré Maïnassara, to Forbes Africa.

    “It is a crucial matter of sovereignty… This is a national treasure that shouldn’t have been sold. Things have to change,” she added.

    Social media users expressed concerns about the meteorite’s correct declaration to Nigerien authorities and the lack of action to prevent its sale.

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  • Astronomers have discovered 2020 VN40 moving in sync with Neptune

    Astronomers have discovered 2020 VN40 moving in sync with Neptune

    image: ©forplayday | iStock

    Astronomers from the Harvard-Smithsonian Centre for Astrophysics have discovered a rare trans-Neptunian object called 2020 VN40

    2020 VN40 is different from any other known object in the solar system as it moves in a synchronised rhythm with Neptune.

    By discovering 2020 VN40, scientists have new insights into the dynamics of our solar system’s outermost regions.

    A unique orbital pattern

    2020 VN40 is the first known object to orbit the Sun once for every ten orbits completed by Neptune, making it a 1:10 orbital resonance. Resonances like this happen when two bodies influence each other gravitationally, despite vast distances. This rare orbital behaviour suggests that Neptune’s gravitational reach extends much farther than previously understood.

    While many trans-Neptunian objects (TNOs) exist in similar resonances with Neptune, they typically reach their closest point to the Sun, called perihelion, when Neptune is on the opposite side of the solar system.

    However, 2020 VN40 goes against this traditional pattern. From a bird’s-eye view of the solar system, it appears to approach the Sun when Neptune is nearby. In reality, the two are never actually close to each other because 2020 VN40’s orbit is tilted steeply compared to the flat plane of the solar system.

    Exploring the distant edges

    This discovery is part of the Large Inclination Distant Objects (LIDO) survey, which is a project that studies objects with unusual, highly tilted orbits in the outer solar system.

    Using data from the Canada-France-Hawaii Telescope, along with follow-up observations from the Gemini Observatory and Magellan Baade Telescope, the LiDO team has been scanning the sky for elusive bodies in distant, unexplored regions.

    The 2020 VN40 travels on an orbit that is approximately 140 times farther from the Sun than the Earth. On average. Its steeply inclined orbit distinguishes it from many other known TNOs, which tend to follow flatter paths.

    Orbital dynamics

    The unusual behaviour of 2020 VN40 challenges some existing assumptions about orbital dynamics in the solar system.

    Most known objects in resonance with Neptune follow patterns that keep them out of close alignment with the planet when near the Sun. However, 2020 VN40’s alignment suggests a different kind of motion, previously unrecognised in solar system studies. This finding opens up the possibility that there may be many more objects following similarly unique orbits that haven’t yet been discovered.

    These resonant and inclined orbits could reveal a great deal about how objects migrate and evolve. These paths may be remnants of a more chaotic, early phase of the solar system, when planets were still shifting and scattering small bodies.

    Future discoveries

    So far, the LiDO survey has revealed more than 140 distant objects, and astronomers expect many more to follow. With future observations from facilities like the Vera C. Rubin Observatory, scientists hope to discover even more unusual trans-Neptunian objects and learn how their orbits were shaped.

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  • How an Ancient Ice Age Froze the Entire Earth—And Helped Humanity Flourish ‹ Literary Hub

    How an Ancient Ice Age Froze the Entire Earth—And Helped Humanity Flourish ‹ Literary Hub

    When you think of ice, maybe your mind first goes to an object. An ice cube, an icicle, a slushy. Something inert, a thing that can be handled. At a certain scale, ice does behave this way. But pile up enough of it, enough to create a glacier, and this material takes on its own agency. What once sat blank and unmoving begins to flow and creak and jerk beneath its own weight. Stress and tension crack into crevasses that yawn deep enough to end lives. These forces also spill out beauty, the most brilliant blues that glow like sapphires or hard candies. 

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    We live in a time of pity for glacial ice. It’s falling apart, it’s melting, it’s destabilizing. It’s retreating, giving in to warmth like prey to a predator.

    These words hold truth, but they also obscure the strength of this substance. Glacial ice is not simply a passive product of the planet’s climate; it is an engineer of it, and a ruthless agent of change. 

    We owe our own existence, in certain ways, to a series of ancient ice ages that spanned between 717 million and 635 million years ago. Strata from this geologic period tell us that life as we know it today may have bloomed in the wake of Earth’s coldest, hardest times. 

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    Remnants of these ancient ice ages rest on the mountainous slopes of Svalbard, a Norwegian archipelago located roughly 1,000 kilometers from the North Pole. A young British geologist named Brian Harland discovered these strata while out mapping that icy terrain last century. A photo captured during the first of more than forty expeditions he would take shows a scruffy-haired twenty-one-year-old with a wide, toothy grin and high cheekbones that frame earnest eyes. With shoulders pushed back and head leaned toward the camera, he looks totally in his element amid those mountains and fjords.

    We owe our own existence, in certain ways, to a series of ancient ice ages that spanned between 717 million and 635 million years ago.

    That was 1938. The outbreak of World War II the following year would prevent him from returning for some time. When he finally did make his way back a decade later, he did so as a professor of geology at the University of Cambridge, bringing a cadre of students along with him.

    As Harland and his students made their way across Svalbard’s frozen landscape, they pulled together evidence of another icy time that had taken place on that land hundreds of millions of years earlier. They found a few telltale signs of glacial activity in the ancient strata that they recognized as such thanks to their understanding of glacial activity in the modern world. For example, whereas rivers of water struggle to move debris larger than dinner plates in diameter, rivers of ice pluck up stones the size of golf carts and push them along like dust in a dustpan. These boulders get mixed in with much finer sand and clay to form what’s called a till. The randomness of glacial till distinguishes these deposits from those laid down by more delicate and organized movements, such as the flow of water through streams or out in the open ocean. Harland and his students recognized glacial till because it lay in plain sight among modern glaciers. 

    Unsorted mixes of sediments can also accumulate from other sorts of geologic activity, like landslides, and so they looked for a suite of other clues in the strata to weed out alternatives and affirm they had, indeed, found evidence of ancient ice. 

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    When glaciers move across the ground, they drag rubble beneath them, carving shallow, parallel grooves called striations through the bedrock. When icebergs drift out to sea, they melt out rubble that drops to the seafloor as pieces of debris called glacial dropstones. Because dropstones fall from above, they can pierce and depress the fine silty layers of the seafloor and cause those layers to warp around them, like a sofa cushion hugging a body.

    Of all the visual clues used to identify glacial deposits in the rock record, dropstones often provide the most convincing evidence of ice. Few other forces can send rocks dropping from above in a body of water. Uprooted trees can carry stones in their roots and release them as they get caught up in a current, but the strata Harland was studying had formed hundreds of millions of years before trees had even evolved.

    Check, check, and check. All of these signs of glaciers present in the modern sediments of Svalbard also appeared in the ancient strata. Harland understood that ice ages come and go, so evidence of ancient ice probably didn’t surprise him very much. But what did surprise him was what he and his students found interspersed among the glacial deposits: thick layers of yellow and gray carbonate rock. 

    Today, carbonates form the foundations of Australia’s Great Barrier Reef, the Bahama Banks, and other such tropical locations. They typically form only in the world’s warmest waters, which rush around the equator. If their interpretations were correct, Harland and his students had found evidence not only that Svalbard had once been closer to the equator but that, at some point while it was there, it had also been encased in ice.

    This, Harland realized, was odd. In today’s world, glacial ice can persist in equatorial regions such as the Andes and Indonesia, but only on mountainous slopes several miles above sea level. If ice had formed all the way at sea level in the warmest part of the world—the part with the most direct sunlight, around the equator—then ice probably would have smothered much of the rest of the planet as well. If that were the case, this would mark the most extreme ice age known in all of Earth’s history. At no other time had glacial ice made it to sea level that far from the poles. The most recent ice age that peaked some 20,000 years ago covered only about 8 percent of the planet; Harland’s ice age looked like it covered closer to 100 percent (though he wouldn’t come to this conclusion until years after his initial observations).

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    From outer space, this cryogenic version of Earth would have glistened white and bright. Beneath the surface of the frozen ocean, dark and briny currents would have stirred continuously from geothermal heat billowing out of cracks in the seafloor. Up above, winds would have howled around the equator in strong gusts, and tiny ice crystals would have settled out of air that remained below freezing everywhere. Life persisted through all this, but it couldn’t have been easy. Algae, bacteria, and simple protozoa would have squirmed around on top of or under the ice, and other specks of life would have swarmed alongside hydrothermal vents on the seafloor.

    This all may seem a bit fantastical, but Harland couldn’t see any other way to interpret the Svalbard strata. When he and colleagues conducted follow-up studies of magnetic minerals within these deposits, they found that those grains—which behave like fossilized compass needles—pointed to a near equatorial origin for the rocks as well.

    “It is concluded,” he wrote in a 1964 paper documenting his unusual finds, “that an ice age was sufficiently extreme to form marine tillites in the tropics.”

    That is, glacial tills. In the oceans. In the tropics. 

    Energized by these findings, Harland presented his theory to colleagues. But it was a hard sell. Rather than accept his seemingly fantastical ideas, some wove together alternative theories. They suggested that those sediments came not from ice but instead from something more mundane, like a series of widespread and robust mudflows. But Harland persisted. Mudflows, he argued, don’t drop uniformly over thousands of square miles, and they don’t leave behind dropstones. 

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    Further to his point, he wasn’t the only geologist finding evidence of ancient glaciers in rocks of roughly this age. As early as 1891, a Norwegian geologist reported deposits of a similar age along the shores of a fjord in northeastern Norway that had striations—those long grooves that form when glacial ice sandpapers the ground beneath it. Over the intervening decades, Harland and others identified some two dozen localities of similar randomly sorted, striated, dropstone-covered rocks across the world in deposits of a similar age, from East Asia to Western Africa to South Australia and Greenland—many with the same curious layers of carbonate capping them off. 

    Individually, the glacial interpretations of these rocks didn’t raise many concerns. But when they were taken all together, and the warm-water carbonates were thrown in, the story became harder to stomach.

    These glacial tills weren’t simply a blip here and a blop there. They were substantial. They measured between ten to one hundred meters thick, sometimes with boulders as large as baby rhinos. To Harland’s mind, these were all too expansive and widespread to have come from mudflows. The suggestion that they had was more outlandish to him than the possibility of ice at the tropics.

    Getting to the bottom of this global cooling event might reveal how the planet produced the complex multicellular beings that would one day evolve into us.

    The mudflow rebuttals drifted away over time, but many of his colleagues still couldn’t accept the idea of ice covering the turquoise waters and soft sand beaches that they thought of as the tropics. They couldn’t imagine a version of Earth that could ever get that cold, nor could they see how the planet would spin out of such a deep chill. They couldn’t, it seemed, grapple with the possibility that Earth was once much different than it is today. 

    These colleagues continued to come up with more alternatives. Some called for wandering magnetic poles that would have shuffled across the planet and brought cold snaps directly to continents, like a waiter serving drinks around a dining room. But that hypothesis, Harland wrote in a bristly 1964 Scientific American article, was not supported by any concrete evidence. “Indeed,” he and his coauthor, Martin Rudwick, lamented, “it seems to have been suggested only in order to avoid postulating the presence of ice in the tropics.” 

    Harland and Rudwick were not willing to be so avoidant. “Failing any other explanation,” they wrote, “we are prepared to accept that [ice] did exist there.”

    That those brilliant turquoise waves had flattened and hardened into muted whites and grays. That smells of salt gave way to ice’s absent scent. 

    The desperation with which Harland worked to understand this ice age stemmed not only from its strangeness but, perhaps even more so, from its timing in relation to another major event in Earth history. Relatively soon after the last of the ice deposits drift away, a burst of fossils appear around the world. This marked the beginning of the Cambrian period, when the majority of animal groups alive today first appear in the rock record. 

    “It can hardly be mere coincidence,” Harland and Rudwick wrote in their 1964 article, “that a geological event of such intensity was followed, after a relatively short interval, by a biological event of equally striking character.” 

    To their minds, the ice age could have instigated the explosion of life that followed. Getting to the bottom of this global cooling event might reveal how the planet produced the complex multicellular beings that would one day evolve into us.

    __________________________________

    Adapted from Strata: Stories from Deep Time by Laura Poppick. Copyright © 2025 by Laura Poppick. Used with permission of the publisher, WWNorton & Company, Inc. All rights reserved.

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  • Don’t Miss Jupiter And A Crescent Moon Shining Together This Week

    Don’t Miss Jupiter And A Crescent Moon Shining Together This Week

    There are few sights so fleeting, so delicate, and so beautiful than the moon when it’s about to sink into the sun’s glare. On Wednesday, July 23, just before sunrise, a whisper-thin crescent moon will appear just above the east-northeastern horizon — but that’s not all. Just a few degrees to its right will be brilliant Jupiter, just days after reappearing from the sun’s glare. Here’s how, when and where to catch these two solar system objects as their paths cross each other.

    Where And When To Look

    The delicate pairing of a barely 3%-lit waning crescent moon and Jupiter will take place low on the east-northeast horizon before sunrise. Jupiter will glow brightly at magnitude -1.8. The waning crescent moon, just 3% illuminated, will lie about five degrees to Jupiter’s left — roughly the width of three fingers at arm’s length. Both celestial bodies will fade quickly in the growing light of dawn.

    What You’ll See

    Seeing the moon when it’s this slender can be a bit of a challenge. However, if you struggle, bright Jupiter will be there to help you — just look to the left of the planet (binoculars will help), and a view of the moon’s final appearance before it slips into the sun’s glare will be yours. Above the pair will be Venus, shining noticeably brighter than Jupiter and the moon.

    Observing Tips

    Timing and preparation are crucial. Arrive early to give your eyes time to adjust to the dim twilight. Jupiter should be easy to find — once you do, look just to the left to spot the delicate crescent. You’ll need a clear sky and a good view down to the horizon. Stop observing before sunrise begins to avoid any risk to your eyes, especially if using binoculars or a telescope.

    What’s Next In The Night Sky

    The Delta Aquariid and Alpha Capricornid meteor showers peak overnight on July 29/30, bringing a gentle flurry of “shooting stars” in the pre-dawn hours. The Perseid meteor shower’s peak night will follow on Aug. 12-13 but be badly affected by strong moonlight.

    For exact timings, use a sunrise and sunset calculator for where you are, Stellarium Web for a sky chart and Night Sky Tonight: Visible Planets at Your Location for positions and rise/set times for planets.

    Wishing you clear skies and wide eyes.

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  • Newly Discovered ‘Infinity Galaxy’ Could Prove How Ancient Supermassive Black Holes Formed

    Newly Discovered ‘Infinity Galaxy’ Could Prove How Ancient Supermassive Black Holes Formed

    A team of astronomers have discovered a curious figure in the universe. It is two distant galaxies colliding with each other to form a larger structure. From Earth’s perspective, the junction of the disks resembles the number eight lying down, similar to the infinity symbol (∞).

    Because of this resemblance, the researchers—who are based at the universities of Yale and Copenhagen—have nicknamed it the “Infinity Galaxy” and have detailed their discovery in a paper published in the Astrophysical Journal Letters. Beyond its evocative shape, the structure intrigues the scientists because of its contents: Within it could be the first direct evidence of a newly formed primordial supermassive black hole.

    The images were taken through the James Webb Space Telescope and then enriched with information from the Chandra X-ray Observatory, the most powerful X-ray telescope ever created. Light from this galaxy comes from a time when the universe was only 470 million years old—roughly 13.5 billion years ago. In the dual galaxy’s structure, at least two consolidated black holes can be observed, each centered in a respective disk (the yellow points in the image below), and a region of compressed gas at the point of intersection suggests the presence of a supermassive object (the green point).

    The Infinity Galaxy, with three points marked where there could be black holes.

    Photograph: NASA, P. van Dokkum, G. Brammer

    The scientists think they might have viewed signs of a direct collapse black hole. Typically, black holes are formed when stars run out of fuel and collapse under their own gravity, but there’s an alternative formation phenomenon debated in astrophysics—where a black hole forms via the collapse of gigantic gas cloud, without a star having formed. Such a possibility has been theorized, but this type of black hole has yet to be observed.

    The largest black holes found in the universe, supermassive black holes, have been identified in galaxies that formed just a few hundred million years after the Big Bang. But what made their formation possible is not yet fully understood. Many supermassive black holes are believed to have come into being as a result of smaller black holes merging. But with very old supermassive black holes, there does not seem to have been enough time for the first stars in the universe to evolve, collapse into stellar-mass black holes, and then merge to colossal, supermassive sizes.

    So some astronomers have proposed an alternative origin for the universe’s first supermassive black holes. According to this hypothesis, the black holes would not need to form from a star or arise from mergers. Instead, the theory goes, dense clumps of matter that in other instances gave rise to galaxies could have compressed directly into massive black holes. Scientists are currently investigating this scenario, although conclusive evidence of this having happened is still lacking.

    It is possible that the Infinity Galaxy offers revealing clues about the possibility of this second formation pathway. “During the collision, the gas within these two galaxies shocks and compresses. This compression might just be enough to form a dense knot, which then collapsed into a black hole,” Pieter van Dokkum, a professor of astronomy and physics at Yale and a coauthor on the paper, said in a post on his university’s website. “While such collisions are rare events, similarly extreme gas densities are thought to have been quite common in the earliest cosmic epochs, when galaxies began to form,” Van Dokkum added.

    Scientists are also considering other, less spectacular alternatives as to what’s going on in the Infinity Galaxy. Rather than being created through a direct collapse of gas, that potential extra black hole—the green spot in the image above—could instead be the signs of a black hole ejected from another galaxy as “Infinity” passes through it. Another possible scenario is that this image actually shows the collision of three galaxies, with the third eclipsed by the other larger ones.

    For the moment, the team says the preliminary results are exciting. “We can’t say definitively that we have found a direct collapse black hole. But we can say that these new data strengthen the case that we’re seeing a newborn black hole, while eliminating some of the competing explanations,” Van Dokkum concluded in a blog for NASA.

    This story originally appeared on WIRED en Español and has been translated from Spanish.

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  • Recent Myanmar Earthquake Occurred at Supershear Velocity

    Recent Myanmar Earthquake Occurred at Supershear Velocity


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    The first studies of the 28 March 2025 magnitude 7.8 Myanmar earthquake suggest that the southern portion of its rupture occurred at supershear velocity, reaching speeds of 5 to 6 kilometers per second.

    In their paper published in The Seismic Record, seismologists Lingling Ye, Thorne Lay and Hiroo Kanamori share new details about the devastating earthquake, which caused widespread and severe damage in Myanmar and neighboring countries such as Thailand, with more than 5,000 confirmed casualties. The earthquake ruptured about 480 kilometers of the Sagaing Fault that extends north-south through the central part of the country.

    The researchers analyzed seismic and satellite imagery to conclude that the rupture had large slip of up to seven meters that extended about 85 kilometers north of the earthquake’s epicenter near the city of Mandalay. Slip along the 395 kilometers of rupture to the south of the epicenter was more patchy, from 1 to 6 meters and about 2 to 3 meters near the country’s capital of Nay Pyi Taw.

    Initial reports suggested that some parts of the rupture might have reached supershear—faster than the speed of shear waves—velocity, which the authors confirmed in this study.

    Measurements of strong ground motion recorded by a seismic station near Nay Pyi Taw roughly 5 kilometers km west of the Sagaing fault were “immediately convincing of supershear rupture given the time between the weak, dilational P wave first arrival and the arrival of large shear offset of the fault” at the station, said Lay. “That was unusually clear and convincing evidence for supershear rupture relative to other long strike-slip events that I have worked on.”

    “This is one of the closest seismic stations to record the rupture passage for a great earthquake. Earthquake seismologists have long desired to have near-fault records like this.” Ye added.

    The weak initial P waves hit the station about 36 seconds after the earthquake began, with much stronger motions starting just 12 seconds after that.

    The strong directivity of the rupture toward the south, combined with the supershear velocity, may have been responsible for the damaging impacts felt as far away as Bangkok, the researchers suggested.

    There have been several large earthquakes of magnitude 7 or larger in the 20th century along the Sagaing Fault, particularly along the northern portion of the fault. But the 28 March earthquake ruptured a part of the fault between Mandalay and Nay Pyi Taw that had been seismically quiet since 1912 and 1839.

    The characteristics of the preceding “seismic gap” are still unclear, said Lay.

    “The 2025 event appears to have ruptured a bit further north and further south than might be expected from the locations of prior events in 1956 in the north and 1930 in the south, but the precise locations and slip distributions for those events are not known,” he explained. “The overlap in the north and south with the ruptures in 1956 and 1930 may represent our lack of knowledge of precise strain release patterns for those two events, or incomplete strain release in those earlier events.”

    “Longer histories and better understanding of fault segmentation and geometry are needed to have any guidance for future event activity, but I would not expect the central area to fail again before a long period of rebuilding strain energy,” he added.

    The 2025 rupture is exceptionally long for a strike-slip rupture of this magnitude, the researchers noted. It is comparable to the roughly 400 kilometers-long 1906 San Francisco rupture, but longer than the 2023 East Anatolian Fault earthquake in Türkiye and the 2002 Denali earthquake in Alaska.

    “The length of the rupture is on the high end relative to the seismic moment, but I suspect that relative straightness of the fault in the southern two-thirds of the rupture helped enable rupture along the southern end, combined with the long time since prior large rupture of the central portion of the fault,” said Lay.

    Reference: Kearse J, Kaneko Y. Curved Fault Slip Captured by CCTV Video During the 2025 7.7 Myanmar Earthquake. Seis Rec. 2025. oi: 10.1785/0320250024


    This article has been republished from the following materials. Note: material may have been edited for length and content. For further information, please contact the cited source. Our press release publishing policy can be accessed here.

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  • This September, the UK will get to see a total lunar eclipse as the Blood Moon rises. Here’s all you need to know

    This September, the UK will get to see a total lunar eclipse as the Blood Moon rises. Here’s all you need to know

    On 7 September 2025, UK observers will be able to see a lunar eclipse rising above the horizon.

    If you saw the total lunar eclipse back in March 2025, you’ll remember that totality – when the entire disc of the Moon is covered in Earth’s shadow – occurred just a few minutes before the Moon set.

    We in the UK got to see the initial partial phase of the lunar eclipse, a hint of totality… and then the Moon was gone.

    Well, the good news is that on 7 September 2025 there’s another total lunar eclipse and it’s something of a mirror of the March event.

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    Why lunar eclipses happen

    A lunar eclipse takes place when the Sun, Earth and the Moon align in a straight line, with sunlight casting a reddish-brown hue on the Moon, hence the nickname ‘Blood Moon’.

    The dimming and change in colour of the Moon happen because Earth blocks direct sunlight from reaching the Moon.

    Only light that has been refracted, or bent, through Earth’s atmosphere manages to illuminate the Moon.

    This atmospheric bending of sunlight is what gives the Moon its red appearance during the eclipse, leading to the term ‘Blood Moon’.

    The total lunar eclipse of March 14, 2025 over Caracas, Venezuela. Photo by JUAN BARRETO/AFP via Getty Images

    How it will appear from the UK

    Whereas in March 2025, totality was reached just as the Moon set, the total lunar eclipse due on 7 September 2025 will see the Moon rise already in totality.

    It appears on the eastern horizon at about 19:45 BST (18:45 UT), around the time the Sun is setting.

    7 September 2025 lunar eclipse from UK, 20:00 BST
    Credit: Pete Lawrence

    This causes all sorts of viewing issues, because a totally eclipsed Moon is darker than a normal, uneclipsed Moon.

    How dark is unknown at this point, but it’s likely to be dark enough to make it tricky to see, low down in the evening twilight through a murky layer of atmosphere.

    Totality ends just as the Moon clears the horizon, so the experience for this eclipse, clouds willing, will be similar to what you saw in March, but in reverse.

    7 September 2025 lunar eclipse from UK, 20:15 BST
    Credit: Pete Lawrence

    Earth’s dark umbral shadow clears the Moon’s disc shortly after moonrise, and the first impression that’s likely to be evident will be an oddly shaped Moon, almost as if someone has taken a slice of regular Moon and placed it in the sky. 

    If totality is very dark, this can fool you at first.

    7 September 2025 lunar eclipse from UK, 20:30 BST
    Credit: Pete Lawrence

    You might spot the part of the Moon that’s coming out of totality, but – being both small and an unfamiliar shape – you might dismiss it.

    It’s quite possible that it’ll only be obvious as a part of the Moon when it rises higher in the sky, so be prepared for this, as failing to identify the Moon early could lead to missing an important part of the eclipse.

    7 September 2025 lunar eclipse from UK, 20:45 BST
    Credit: Pete Lawrence

    See the Belt of Venus

    The Moon will be rising in the Belt of Venus, a name given to the pink-topped grey band that sits just above the opposite horizon to where the Sun sets.

    As the evening progresses, the pink colour will reduce and the grey band will deepen. This is Earth’s shadow rising as the Sun sets in the opposite direction.

    As the evening darkens, the portion of the Moon that’s not covered by the umbral shadow will increase, this being the final partial phase of the eclipse.

    If you see or photograph the lunar eclipse on 7 September 2025, get in touch via contactus@skatnightmagazine.com

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  • First 3D Map of Glucose Metabolism Created in Cells

    First 3D Map of Glucose Metabolism Created in Cells


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    In a scientific first, researchers from Vanderbilt University and the University of California, San Diego, have generated a high-resolution metabolic “map” of how cells orchestrate glucose processing, revealing a hidden world where organelles and molecular complexes collaborate when responding to a rush of nutrients. This new study, published in Nature Communications, has redefined how glucose metabolism is visualized at the single-cell level. The pioneering work provides both a new method and insights into an organizational and molecular framework that can be used to study how metabolic processes are disrupted in diseases like diabetes, obesity, and cancer, as well as in aging and neurodegeneration.

    “This is a new field—we are at the forefront by integrating multiple microscopy modes into sophisticated pipelines to measure the fate of glucose atoms, from whole animals to organelles, and to show the underlying subcellular architecture associated with these processes in cells,” Rafael Arrojo e Drigo said. Arrojo e Drigo is an assistant professor of molecular physiology and biophysics and the corresponding author of the study. “We expect that this advance will propel a new program that exploits these advanced investigational strategies to study and better understand how nutrient metabolism is organized within the highly structured domains of cells and tissues, which allows for the precise regulation of organ function in the context of whole-animal physiology.”

    To date, what scientists know about how cells process nutrients like glucose has been derived from bulk metabolomics. Using metabolomics, researchers can analyze an entire set of small molecules within a biological sample, such as a tissue, but it’s done without consideration of the specific spatial or subcellular contexts in which they occur.

    “These bulk strategies do not reveal the spatial characteristics of cell metabolism at the single-cell level or how these aspects relate to the location of cells and organelles within the complexity of the tissue they reside within,” Arrojo e Drigo said.

    This gap in the field’s understanding drove a multidisciplinary team from Vanderbilt, the Vanderbilt University Medical Center, and UCSD to combine stable isotope tracing, multi-scale microscopy, and AI-powered image analysis to map glucose metabolites at animal, tissue, cellular, and organellar scales. The Vanderbilt team was led by co-first authors Christopher Acree and Aliyah Habashy from the Arrojo e Drigo lab and included scientists from the Vanderbilt Mouse Metabolic Phenotyping Center, the Mass Spectrometry Research Center, the Department of Cell and Developmental Biology, and the VUMC Department of Surgery. Researchers from Mark Ellisman’s group at the National Center for Microscopy and Imaging Research at UCSD rounded out the collaboration.

    Together, they determined the spatial organization of glucose metabolites, from inside whole animals to within liver cells and even in individual mitochondria. Using isotopically labeled glucose infusions in live mice, the researchers mapped how glucose-derived carbons were incorporated into glycogen, lipid droplets, and other cellular components over time.

    Among the major discoveries of this study, the team uncovered a previously unrecognized structural and functional interaction between lipid droplets and glycogen synthesis. In addition, the researchers mapped how contacts between mitochondria and the endoplasmic reticulum—two key organelles involved in energy production and nutrient sensing—shift dynamically in response to changes in blood glucose levels. These mitochondria-ER contacts form part of a broader organelle network that coordinates metabolic responses within the cell. By charting the timeline of these interactions, the study offers new insights into how organelles reorganize to adapt to different metabolic states, shedding light on fundamental mechanisms of glucose metabolism and cellular energy balance.

    This breakthrough was made possible by Vanderbilt’s characteristic interdisciplinary environment and the multi-scale, multi-modal imaging thrust of the NCMIR, an alliance that brought together experts in stable isotope tracing, in vivo animal metabolism, mass spectrometry imaging, AI, and computational modeling, Arrojo e Drigo said. Looking ahead, the team hopes to understand how the spatial organization of nutrients inside cells contributes to metabolic health and disease.

    Reference: Habashy A, Acree C, Kim KY, et al. Spatial patterns of hepatocyte glucose flux revealed by stable isotope tracing and multi-scale microscopy. Nat Commun. 2025;16(1). doi: 10.1038/s41467-025-60994-w

    This article has been republished from the following materials. Note: material may have been edited for length and content. For further information, please contact the cited source. Our press release publishing policy can be accessed here.

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