Category: 7. Science

  • A massive earthquake could be brewing beneath North America, study suggests

    A massive earthquake could be brewing beneath North America, study suggests

    A hidden tectonic fault in Canada’s Yukon could be gearing up to unleash a major earthquake of at least magnitude 7.5, according to a new study.

    The Tintina fault, which runs from northeastern British Columbia through to central Alaska, has been quietly accumulating strain for at least 12,000 years. Previously thought to be relatively benign, new analysis suggests it’s still very much active.

    Worryingly, scientists can’t say when the next major quake will strike – only that it almost certainly will.

    “Our findings indicate that the fault is active and continues to accumulate strain,” Dr Theron Finley, lead author of the study published in Geophysical Research Letters, told BBC Science Focus. “And so we anticipate that in the future, it will rupture again.” 

    Tintina is what’s known as a ‘right-lateral strike-slip fault’ – a type of fault where two blocks of the Earth’s crust slide past each other horizontally. If you stand on one side of the fault and the other side moves to your right during an earthquake, it’s called right-lateral.

    Over time, one side of the fault has slipped around 430km (270mi), mostly during the Eocene period – a geological epoch that occurred roughly 56 to 33.9 million years ago – when it’s thought to have been moving as much as 13mm (0.5in) a year.

    The Tintina fault extends 1,000km (600mi) from northeastern British Columbia into Alaska. – Credit: National Park Service

    Although small earthquakes have occasionally been recorded in the region, the Tintina fault was largely considered dormant.

    “There have been a few small earthquakes in the magnitude three to four range detected along or adjacent to the Tintina fault,” Finley said. “But nothing really suggests that it’s capable of larger ruptures.”

    That changed when Finley and his team used new technologies to re-examine the fault. Combining satellite surface models with drone-mounted Light Detection and Ranging (LIDAR) data, the researchers were able to see through the dense forest and uncover signs of a seismically active past – and future – in the Yukon.

    Scattered across the landscape were fault scarps – long, narrow landforms produced when an earthquake ruptures all the way to the surface. These can stretch for tens or even hundreds of kilometres, though they’re usually only a few metres high and wide.

    “In the case of the Tintina fault, the scarps appear as an interesting series of aligned mounds,” Finley said.

    By dating these surface features, the researchers found that while the fault has ruptured numerous times over the past 2.6 million years, it hasn’t produced a major earthquake in the last 12,000 years – all while slowly accumulating strain at a rate of 0.2 to 0.8 mm (0.008 to 0.03 in) per year.

    Fortunately, the region is sparsely populated. But when the fault does rupture, Finley warned that significant landslides, infrastructure damage, and impacts to nearby communities are likely.

    “I want to be clear that we don’t have a great sense of how imminent an earthquake is,” he said. “We just know that from our observations, it appears that a long time has elapsed since the last one. But there’s not really a way to tell whether another one is more likely in the coming days and weeks versus thousands of years from now.”

    Now that the fault has been confirmed as active, Finley says the next step is to better estimate how often large earthquakes occur there. While this won’t allow researchers to predict exactly when the next rupture will happen, it could provide a more reliable timescale for when one should be expected.

    “Earthquakes don’t necessarily occur periodically, but it would give us a better sense of how often we expect large earthquakes,” Finley said. Regardless, when Tintina finally does go, it won’t be a small one.

    Read more:

    About our expert

    Theron Finley is a surficial geologist at the Yukon Geological Survey. He recently graduated with a PhD from the University of Victoria, Canada, where he conducted research on active faults in western Canada using remote sensing, tectonic geomorphology and paleoseismology.

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  • Ancient viral DNA may play a key role in early human development, new study suggests

    Ancient viral DNA may play a key role in early human development, new study suggests

    The human genome is made up of 23 pairs of chromosomes, the biological blueprints that make humans … well, human. But it turns out that some of our DNA — about 8% — are the remnants of ancient viruses that embedded themselves into our genetic code over the course of human evolution.

    These ancient viruses lie in sections of our DNA called transposable elements, or TEs, also known as “jumping genes” due to their ability to copy and paste themselves throughout the genome. TEs, which account for nearly half of our genetic material, were once waved off as “junk” DNA, sequences that appear to have no biological function. Now, a new study offers support for the hypothesis that these ancient viral remnants play a key role in the early stages of human development and may have been implicated in our evolution.

    By sequencing TEs, an international team of researchers identified hidden patterns that could be crucial for gene regulation, the process of turning genes on and off. The findings were published July 18 in the journal Science Advances.

    “Our genome was sequenced long ago, but the function of many of its parts remain unknown,” study coauthor Dr. Fumitaka Inoue, an associate professor in functional genomics at Kyoto University in Japan, said in a statement. “Transposable elements are thought to play important roles in genome evolution, and their significance is expected to become clearer as research continues to advance.”

    There are many benefits to studying how TEs activate gene expression. It could help scientists understand the role that the sequences play in human evolution, reveal possible links between TEs and human diseases, or teach researchers how to target functional TEs in gene therapy, said lead researcher Dr. Xun Chen, a computational biologist and principal investigator at Shanghai Institute of Immunity and Infection of the Chinese Academy of Sciences.

    With more research, “we hope to uncover how TEs, particularly ERVs (endogenous retroviruses, or ancient viral DNA), make us human,” Chen added in an email.

    When our primate ancestors were infected with viruses, sequences of viral genetic information would replicate and insert themselves in various locations in the host’s chromosomes.

    “Ancient viruses are effective in invading our ancestral genomes, and their remnants become a big part of our genome. Our genome has developed numerous mechanisms to control these ancient viruses, and to eliminate their potential detrimental effects,” said Dr. Lin He, a molecular biologist and the Thomas and Stacey Siebel Distinguished Chair professor in stem cell research at the University of California, Berkeley, in an email.

    For the most part, these ancient viruses are inactive and are not a cause of concern, but in recent years, research has shown that some of the transposable elements may play important roles in human diseases. A July 2024 study explored the possibility of silencing certain TEs to make cancer treatment more effective.

    “Over the course of evolution, some viruses are degenerated or eliminated, some are largely repressed in expression in normal development and physiology, and some are domesticated to serve the human genome,” said He, who was not involved with the new study. “While perceived as solely harmful, some ancient viruses can become part of us, providing raw materials for genome innovation.”

    But because of their repetitive nature, transposable elements are notoriously difficult to study and organize. While TE sequences are categorized into families and subfamilies based on their function and similarity, many have been poorly documented and classified, “which could significantly impact their evolutionary and functional analyses,” Chen said.

    Ancient viral impact on human development and evolution

    The new study focused on a group of TE sequences called MER11 found within primate genomes. By using a new classification system as well as testing the DNA’s gene activity, researchers identified four previously undiscovered subfamilies.

    The most recently integrated sequence, named MER11_G4, was found to have a strong ability to activate gene expression in human stem cells and early-stage neural cells. The finding indicates that this TE subfamily plays a role in early human development and can “dramatically influence how genes respond to developmental signals or environmental cues,” according to a statement from Kyoto University.

    The research also suggests that viral TEs had a part in shaping human evolution. By tracing the way the DNA has changed over time, the researchers found that the subfamily had evolved differently within the genomes of different animals, contributing to the biological evolution that resulted in humans, chimpanzees and macaques.

    “To understand the evolution of our genome is one way to understand what makes humans unique,” said He. “It will empower us with tools to understand human biology, human genetic diseases, and human evolution.”

    Exactly how these TEs were implicated in the evolutionary process is still unclear, Chen said. It is also possible that other TEs that have yet to be identified played distinct roles in the evolutionary process of primates, he added.

    “The study offers new insights and potential leverage points for understanding the role of TEs in shaping the evolution of our genomes,” said Dr. Steve Hoffmann, a computational biologist at the Leibniz Institute on Aging in Jena, Germany, who was not involved with the study. The research also “underscores how much more there is to learn from a type of DNA once slandered as a molecular freeloader,” he added in an email.

    Hoffmann was the lead researcher of a scientific paper that first documented the nearly complete genome map of the Greenland shark, the longest-living vertebrate in the world that can survive until about 400 years old. The shark’s genome was made up of more than 70% jumping genes, while the human genome is composed of less than 50%. While primate genomes are different from those of a shark, “the study provides further evidence for the potential impact of TEs on genome regulation” and “is a message with relevance for all genome researchers,” Hoffmann said.

    By investigating how genomes have evolved, researchers can determine which DNA sequences have remained the same, which have been lost in time and which have emerged most recently.

    “Taking these sequences into account is often critical to understanding, e.g., why humans develop diseases that certain animals don’t,” Hoffmann said. “Ultimately, a deeper understanding of genome regulation can aid in the discovery of novel therapies and interventions.”

    Taylor Nicioli is a freelance journalist based in New York.

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  • Mixing Regolith With Polymer Saves Mass For 3D Printing

    Mixing Regolith With Polymer Saves Mass For 3D Printing

    3D printing is going to be a critical technology in space exploration, both for its ability to create almost any object, but also because it can utilize in-situ resources, at least in part. However, the more of those space resources are used in a print, the more the mechanical properties change from that on Earth, leading to problems with tensile or compressive strength. But a new paper from researchers at Concordia University hit a new milestone of how much lunar regolith can be used in a mixed feedstock for additive manufacturing, making it possible to use even more locally sourced material, and saving more launch cost, than ever before.

    The research mixed lunar regolith simultant, which is material created to mimic how the material on the surface on the Moon works, with polyether-ether-ketone, more commonly known as PEEK. PEEK is a thermoplastic already in wide use in 3D printing, but previous efforts to combine it with lunar regolith have faltered. They suffered from extrusion challenges, as the regolith, which is made up of hard individual particles, made it difficult to extrude without simply blowing dust all over. Additional problems resulted from the porosity of the material that was printed, which led to decreased tensile strength and increased brittleness.

    Modifications to the 3D printing method seemed to be the answer to those problems. There were two main advancements in technology discussed in the paper – a screw configuration and a different type of “raft” used to bond the printed material to the print bed.

    Fraser discusses how resources on the Moon are going to be so important to our expansion of the solar system.

    Combining lunar regolith simulant (LRS) with PEEK is a tricky business, so the researchers, led by Mohammed Azami of Concordia’s electrical engineering department, decided to use a novel “twin screw” configuration. Torque was a factor in previous iterations of the mixing machine, as higher regolith content meant higher torque, eventually limiting the total percentage of regolith mixed with the PEEK to around 30%. With the new configuration, the researchers were able to get concentrations of up to 50% of the regolith when combined with the PEEK.

    However, when those parts were printed, they started to delaminate and warp. While common in prints of just PEEK itself, the addition of the regolith exacerbated the problem. To solve it, the researchers used a “raft” – a type of intermediate layer to help the print bond to the main printing plate. In their case, they used a different type of thermopolymer, known as polyether-ketone-ketone (PEKK) as the raft, and implemented a dual-nozzle system, where the PEKK was printed using one nozzle and the combination LRS/PEEK was printed using the other.

    After they got the higher concentrations of LRS and overcame the delamination/warping problem, the researchers decided to anneal their samples. The annealing process seemed to improve some of the mechanical properties of the print, but only up to a point. At higher concentrations of LRS, the benefits of annealing were not as apparent due to breaks in PEEK’s polymer chain, which benefits from annealing, because of the increased number of regolith particles.

    Fraser discusses why 3D printing is so critical to space exploration.

    As with all good papers on 3D printing new material, the authors then looked at the mechanical properties of their output. While there was a noticeable increase in stiffness, there was a steady decrease in tensile strength, which was exacerbated at higher LRS concentrations. The combined material also had decreased “elongation at break” (i.e. increased brittleness), but ultimately the researchers determined that the best trade-off for using in-situ material was around a mix of 60% PEEK and 40% regolith. This mixture doesn’t suffer from some of the more severe degradation of mechanical properties while still utilizing as much local resources as possible.

    There is undoubtedly still room for improvement here, as this is very early on in experimentation with these materials. In the future, the researchers plan to try combining the LRS with different polymers, and do more of their testing / manufacturing in simulated lunar environments, such as a vacuum and decreased gravity. It will be a while before 3D printing makes up a large percentage of the material used on the Moon, but that time is surely on its way, and these first early steps at experimentation are how we will eventually get there.

    Learn More:

    M. Azami et al – Additive Manufacturing of PEEK/Lunar Regolith Composites for Sustainable Lunar Manufacturing

    UT – Quality Of 3D Printing With Lunar Regolith Varies Based On Feedstock

    UT – 3-D Printing on the Moon. From Regolith to Paste to Useful Objects and Structures

    UT – NASA Sends a 3D Printer for Lunar Regolith and More to the ISS

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  • New adhesive surface modeled on a remora works underwater

    New adhesive surface modeled on a remora works underwater

    What impressed the scientists the most, though, was the versatility of those disks. Reef-associated species of remora like Phtheirichthys lineatus are generalists and stick to various hosts, including other fish, sharks, or turtles. Other species living in the open sea are more specialized and attach to cetaceans, swordfish, or marlins. While most remoras attach to the external tissue of their hosts, R. albescens sticks within the oral cavities and gill chamber of manta rays.

    A close-up of the adhesive pad of a remora.


    Credit:

    Stephen Frink

    To learn what makes all these different disks so good at sticking underwater, the team first examined their anatomy in detail. It turned out that the difference between the disks was mostly in the positioning of lamellae. Generalist species have a mix of parallel and angled lamellae, while remoras sticking to fast-swimming hosts have them mostly parallel. R. albescens, on the other hand, doesn’t have a dominant lamellae orientation pattern but has them positioned at a very wide variety of angles.

    The researchers wanted to make an adhesive device that would work for a wide range of applications, including maritime exploration or underwater manufacturing. Their initial goal, though, was designing a drug delivery platform that could reliably stick to the inside walls of the gastrointestinal tract. So, they chose R. albescens disks as their starting point, since that species already attaches internally to its host. They termed their device an Mechanical Underwater Soft Adhesion System (MUSAS).

    However, they didn’t just opt for a biomimetic, copy-and-paste design. “There were things we did differently,” Traverso says.

    Upgrading nature

    The first key difference was deployment. MUSAS was supposed to travel down the GI tract to reach its destination, so the first challenge was making it fit into a pill. The team chose the size 000 capsule, which at 26 millimeters in length and 9.5 millimeters in diameter, is the largest Food and Drug Administration-approved ingestible form. MUSAS had a supporting structure—just like remora disks, but made with stainless steel. The angled lamellae with spinules fashioned after those on R. albescens were made of a shape memory nickel-titanium alloy. The role of remora’s soft tissues, which provide the suction by dividing the disk into compartments, was played by an elastomer.

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  • Scientists Discover a Deep Sea “Superhighway” in Australia

    Scientists Discover a Deep Sea “Superhighway” in Australia

    A recent study discovered that the deep sea isn’t as isolated as we once thought. Researchers believe it is way more globally connected than ever imagined. They call it a global, deep-sea superhighway where species have been migrating across entire oceans for millions of years.

    The groundbreaking research, published in Nature, focused on ancient spiny animals called brittle stars. These sea creatures are found from shallow coastal waters to the deepest depths.

    A research team led by Museums Victoria Research Institute analyzed the DNA of thousands of specimens preserved in museums globally to map the distribution and evolutionary relationships of brittle stars.

    A Deep-Sea Superhighway Connecting the World’s Oceans

    deep-sea superhighway
    Researchers discovered a deep-sea highway connection by studying brittle stars; Photo: CSIRO

    “You might think of the deep sea as remote and isolated, but for many animals on the seafloor, it’s actually a connected superhighway,” said Dr. Tim O’Hara, Senior Curator of Marine Invertebrates at Museums Victoria Research Institute.

    He added that deep-sea species have expanded their ranges by thousands of miles over time, a phenomenon that has gone unnoticed until now. Research shows that deep-sea communities are more closely related across regions than shallow-water communities. For example, the researchers explain, marine animals off Australia’s southern coast share evolutionary links with species in the North Atlantic.

    Researchers analyzed DNA from 2,699 brittle star species housed in 48 natural history museums. The study shows insights into how marine life evolved and dispersed over the past 100 million years.

    Temperature restricts marine life in shallow waters, making deep-sea environments more stable. This allows species like brittle stars to spread out over vast distances. A brittle star’s yolk-rich larvae aid their mobility because they can drift on deep ocean currents for extended periods.

    “These animals don’t have fins or wings, but they’ve still managed to span entire oceans,” said Dr. O’Hara. He adds that the secret lies in their biology. A brittle star’s larvae can survive for a long time in cold water because of their ability to ride deep-sea currents. 

    Despite the deep-sea being highly connected, researchers emphasize its fragility. Understanding how life is distributed and moves through the vast depths is crucial for its protection. It’s especially important because of the increasing threats of deep-sea mining and climate change.


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  • Venus and Jupiter conjunction: How to watch the 2 brightest planets ‘kiss’ on Aug. 12

    Venus and Jupiter conjunction: How to watch the 2 brightest planets ‘kiss’ on Aug. 12

    Just as the Perseid meteor shower approaches its peak, two luminous planets are getting in on the night-sky action.

    Venus and Jupiter, the two brightest planets in the sky, will meet in a conjunction very early on Tuesday morning (Aug. 12). On this morning, the two planets will be less than a degree apart — approximately the length of your pinkie when held up to the sky at arm’s length. Because they’ll appear close together, you’ll be able to view both simultaneously through skywatching binoculars or a backyard telescope.

    But if you want to see the conjunction, you’ll have to either stay out late or get up early: Venus and Jupiter rise together around 3 a.m. local time and set together around 6 a.m. local time. However, these times vary slightly depending on your exact location. You can use Time and Date to check the precise rise and set times for your area.

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  • Blame it on the moon. This year’s Perseids meteors won’t be as visible at their peak

    Blame it on the moon. This year’s Perseids meteors won’t be as visible at their peak

    The annual Perseids meteor shower will reach its peak next week. But astronomers say it won’t be as visible as it has been in recent years.

    A full moon is also expected during the peak — Aug. 12 into the 13th — and will likely wash out the view.

    “A few bright meteors may still be seen in the predawn hours, but viewing conditions are not ideal,” NASA said.

    If you still want to try to catch a glimpse, here’s what to know.

    Best viewing conditions

    This year, the Perseids began on July 17, and it will be visible until Aug. 23, NASA says. In an hour, one could see about 25 meteors. Characteristics of the Perseids include bright fireballs and long “wakes,” the streak of light and color that follow meteors.

    While NASA recommends trying to catch a glimpse of the Perseids before dawn, you may be able to see some meteors as early as 10 p.m. They are most visible in the Northern Hemisphere.

    Robert Lunsford, an observer with the American Meteor Society, recommends facing north and settling in.

    “Don’t go outside and stand,” he said. “You’ll get really tired and bored quick. Get a nice lounge chair where you’re comfortable.”

    And be patient.

    “Sometimes you go 10, 15 minutes without seeing anything, and all of a sudden, four or five will show up in the same minute. So they’re notorious for appearing in bunches like that,” he said.

    Where do they come from?

    As comets orbit the sun, they leave a trail of dust and particles, including meteors, behind them. The Perseids meteors originate from the Swift-Tuttle comet, which has a nucleus of about 16 miles wide, and takes more than 130 years to circle the Sun.

    The Swift-Tuttle comet last entered the solar system in 1992, during which observers could see about 200 meteors per hour. The comet leaves such a mess of debris when it comes, we’re able to catch the Perseids every year, Lunsford said.

    The Perseids is the most popular of the meteor showers, according to NASA. And while it’s not the strongest, people gravitate to it because it happens in the summer, Lunsford said.

    “Most of the other strong meteors occur in the late autumn or early winter, and it is really frigid outside. So that’s the bigger reason,” he said.

    Copyright 2025 NPR


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  • Paperclip probe could journey to nearby black hole within a century

    Paperclip probe could journey to nearby black hole within a century

    Paperclip probe could journey to nearby black hole within a century

    by Riko Seibo

    Tokyo, Japan (SPX) Aug 08, 2025






    It may sound like pure science fiction – a spacecraft no heavier than a paperclip racing toward a black hole at near-light speed – but astrophysicist Cosimo Bambi of Fudan University believes it could be achievable within decades.



    Writing in the journal iScience, Bambi presents a conceptual plan for sending a gram-scale nanocraft to a nearby black hole to probe the fabric of space-time and test general relativity under extreme conditions. The proposed journey, lasting 80 to 100 years, would require breakthroughs in both detection and propulsion technology.



    The first step is identifying a target. Based on stellar evolution models, a black hole may exist just 20 to 25 light-years away, but locating it will be difficult since black holes emit no light. Instead, astronomers must search for gravitational effects on nearby stars or light distortions.



    “There have been new techniques to discover black holes,” says Bambi. “I think it’s reasonable to expect we could find a nearby one within the next decade.”



    Once a target is confirmed, Bambi proposes using gram-scale probes equipped with a microchip and a light sail. Powerful Earth-based lasers would accelerate the craft to about one-third of light speed, enabling it to reach a black hole 20 to 25 light-years away in roughly 70 years. The data would arrive another 20 years later.



    At its destination, the probe could investigate questions central to physics, such as whether black holes have event horizons, how gravity behaves in extreme regimes, and whether Einstein’s theories remain valid under the universe’s most intense forces.



    Bambi estimates that the laser array alone would cost around one trillion euros today. However, he predicts that in 20 to 30 years, costs will drop and technology will catch up. “It may sound really crazy, and in a sense closer to science fiction,” he says. “But people said we’d never detect gravitational waves… Now, 50 years later, we have images of two.”



    Research Report:An interstellar mission to test astrophysical black holes


    Related Links

    Fudan University

    Understanding Time and Space


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  • Some young suns align with their planet-forming disks, others are born tilted

    Some young suns align with their planet-forming disks, others are born tilted

    Some young suns align with their planet-forming disks, others are born tilted

    by Sonia Fernandez for UCSB News

    Santa Barbara CA (SPX) Aug 08, 2025






    Researchers at UC Santa Barbara, The University of Texas at Austin, Yale University and National Taiwan Normal University have found that a fair number of sun-like stars emerge with their rotational axis tilted with respect to their protoplanetary disks, the clouds of gas and dust from which solar systems are born.



    “All young stars have these discs, but we’ve known little about their orientations with respect to the spin axis of the host stars,” said UCSB associate physics professor Brendan Bowler, who studies how planets form and evolve through their orbits and atmospheres, and is senior author of a study in the journal Nature. Based on the general alignment of our own sun’s rotational axis with those of the planets in our solar system, the assumption was that stars and their planet-forming disks emerge and rotate in or very close to alignment, he explained.



    “This work challenges these centuries-old assumptions,” Bowler said.



    Ever since exoplanetseart planets that orbit other stars were discovered in the early 1990s, the variety of spin orientations of host stars relative to the orbits of the planets closest to them had astrophysicists scratching their heads.



    “It came as quite a surprise that some planets were on orbits that were extremely inclined relative to the spin axis of the host star,” said Lauren Biddle, a postdoctoral researcher at UT Austin, and lead author of the study. Since then, there have been efforts to explain the dynamics that could lead to this planetary system architecture.



    “One idea is that after planets form, gravitational interactions with a passing star or maybe a companion star could incline the orbit of the planet relative to the host star,” Biddle said. “Or maybe after planets form, a particularly massive one on the outer edge of the system could gravitationally interact with planets closer to the star.” The leading idea has been that planetary systems and their suns begin life aligned but through interactions over billions of years, systems can become misaligned, she said. “But there was also this question about whether these orbits were inherited from their formation process.”



    To find out, the researchers took data from the Atacama Large Millimeter/submillimeter Array (ALMA), the Transiting Exoplanet Survey Satellite (TESS) and the repurposed exoplanet-seeking Kepler Mission (K2) to measure stellar and disk inclinations and obtain star-disk obliquity for a sample of 49 young isolated stars and their planet-forming disks.



    The result of their survey? About two-thirds of the stars and protoplanetary disks were found to be in alignment, while a third of them were misaligned. The modest number of misaligned stellar and planet-forming disk orientations hints at a more elegant model of the origin of planetary system tilts: some are just born that way.



    “It changes our interpretation,” he continued. “It means that we don’t need a ton of post-formation dynamics and interactions and planet-scattering events.” Certainly, there are suns and planetary systems that do undergo significant interactions, and can only be explained by complex dynamics, according to Bowler. And, he added, studying other stars and their solar systems gives context to our own six-degree misalignment between our own sun and solar system.



    “If we think of science as kind of an Occam’s razor where the least complex model ends up winning out, given the data, this is a nice example of the sun simply just fitting into this primordial, stellar obliquity distribution,” Bowler said.



    Future work in this realm may include further investigations into just how these sun-like stars and their protoplanetary disks create these tilted orientations during the earliest stages of solar system formation.



    “Now we know that at least a third of them are tilted,” said Bowler, but why this is the case remains unanswered.



    Research Report:One-third of Sun-like stars are born with misaligned planet-forming disks


    Related Links

    UC Santa Barbara

    Lands Beyond Beyond – extra solar planets – news and science
    Life Beyond Earth


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  • China advances crewed lunar mission with lander landing and takeoff trial

    China advances crewed lunar mission with lander landing and takeoff trial

    China advances crewed lunar mission with lander landing and takeoff trial

    by Riko Seibo

    Tokyo, Japan (SPX) Aug 08, 2025






    China has successfully carried out its first integrated landing and takeoff trial of a crewed lunar lander, marking a milestone in its manned lunar exploration program. The test took place Wednesday at a facility in Huailai county, Hebei province, the China Manned Space Agency confirmed Thursday.



    The spacecraft, called Lanyueeart – meaning embracing the mooneart – is composed of a landing module and a propulsion module. It is purpose-built for ferrying two astronauts between lunar orbit and the surface while transporting a rover and scientific instruments.



    Once on the moon, Lanyue will act as a life-support hub, power source, and communications and data center, enabling extended surface stays and operations for its crew.



    The agency emphasized the trial’s complexity, citing extended timelines and significant technical challenges. Officials described the achievement as a breakthrough in spacecraft design and technology for China’s crewed lunar initiatives.



    China plans to place astronauts on the lunar surface before 2030 to carry out scientific research and exploration.


    Related Links

    China Manned Space Agency

    Mars News and Information at MarsDaily.com
    Lunar Dreams and more


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