Category: 7. Science

  • Protein Misfolding Simulated in High Definition

    Protein Misfolding Simulated in High Definition

    UNIVERSITY PARK, Pa. — New computer simulations that model every atom of a protein as it folds into its final three-dimensional form support the existence of a recently identified type of protein misfolding. Proteins must fold into precise three-dimensional shapes — called their native state — to carry out their biological functions. When proteins misfold, they can lose function and, in some cases, contribute to disease. The newly spotted misfolding results in a change to a protein’s structure — either a loop that traps another section of the protein forms when it shouldn’t or doesn’t when it should — that disrupts its function and can persist in cells by evading the cell’s quality control system. The simulated misfolds also align closely with structural changes inferred from experiments that track protein folding using mass spectrometry, according to the team led by researchers at Penn State.

    “Protein misfolding can cause disease, including Alzheimer’s and Parkinson’s, and is thought to be one of the many factors that influence aging,” said Ed O’Brien, professor of chemistry in the Eberly College of Science, a co-hire of the Institute for Computational and Data Sciences at Penn State and the leader of the research team. “This research represents another step forward in our attempt to document and understand the mechanisms of protein misfolding. Our aim is to translate these fundamental discoveries into therapeutic targets that could help mitigate the impacts of these disorders and even aging.”

    A paper describing the research appeared today (Aug. 8) in the journal Science Advances.

    Proteins are composed of long strings of units called amino acids. A protein’s function relies on the sequence of those amino acids along the string, which determines how the string will fold into a three-dimensional structure. Sections of the protein can fold into helices, loops, sheets and various other structures which allows them to interact with other molecules and perform their functions. Any mistake during this folding process can disrupt these functions.

    The new class of misfolding, recently identified by the O’Brien Lab, involves a change in entanglement status in the protein’s structure. Entanglement refers to sections of the string of amino acids looping around each other like a lasso or a knot. Sometimes an entanglement can form when it shouldn’t be there and sometimes an entanglement that is part of the protein’s native structure doesn’t form when it should.

    “In our previous study, we used a coarser-grained simulation that only modeled the protein at the amino acid level not the atomic level,” said Quyen Vu, first author of the paper and a postdoctoral researcher in chemistry at Penn State who started the research as a graduate student at the Polish Academy of Sciences. “But there was concern in the community that such a model might not be realistic enough, as the chemical properties and bonding of the atoms that make up amino acids influence the folding process. So, we wanted to make sure we still saw this class of entanglement misfolding with higher-resolution simulations.”

    The team first used all-atom models of two small proteins and simulated their folding. They found that both small proteins could form the misfolds just like in their coarser-grained simulations. However, unlike in their previous simulations, which modeled normal-sized proteins, the misfolds in these small proteins lasted only a short time.

    “We think that the misfolds in our previous simulations persisted for two main reasons,” Vu said. “First, to fix the misfold required backtracking and unfolding several steps to correct to entanglement status, and second, the misfold can be buried deep inside the protein’s structure and essentially invisible to the cell’s quality control system. With the small proteins there were fewer steps and less to hide behind so the mistakes could be quickly fixed. So, we simulated a normal size protein at the atomic scale and saw misfolding that persisted.”

    The team also tracked folding of the proteins used in their simulations experimentally. While they couldn’t directly observe the misfolds in the experiments, structural changes inferred using mass spectrometry occurred in the locations that misfolded in their simulations.

    “Most misfolded proteins are quickly fixed or degraded in cells,” O’Brien said. “But this type of entanglement presents two major problems. They are difficult to fix as they can be very stable, and they can fly under the radar of the cell’s quality control systems. Coarse-grain simulations suggest that this type of misfolding is common. Learning more about the mechanism can help us understand its role in aging and disease and hopefully point to new therapeutic targets for drug development.”

    In addition to Vu and O’Brien, the research team includes Ian Sitarik, graduate student in chemistry; Yang Jiang, assistant research professor in chemistry; and Hyebin Song, assistant professor of statistics, at Penn State; Yingzi Xia, Piyoosh Sharma, Divya Yadav, and Stephen D. Fried at Johns Hopkins University; and Mai Suan Li at the Polish Academy of Sciences.

    The U.S. National Science Foundation, the U.S. National Institutes of Health and the Polish National Science Centre funded the research. The research was supported in part by the TASK Supercomputer Center in Gdansk, Poland; the PLGrid Infrastructure in Poland; and the Roar supercomputer in the Institute for Computational and Data Sciences at Penn State.

    /Public Release. This material from the originating organization/author(s) might be of the point-in-time nature, and edited for clarity, style and length. Mirage.News does not take institutional positions or sides, and all views, positions, and conclusions expressed herein are solely those of the author(s).View in full here.

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  • Apollo 13 astronaut Jim Lovell dies | US News

    Apollo 13 astronaut Jim Lovell dies | US News

    Retired astronaut and the commander of the famous Apollo 13 mission, Jim Lovell, has died aged 97.

    In a post on X, NASA said: “We are saddened by the passing of Jim Lovell, commander of Apollo 13 and a four-time spaceflight veteran.

    “Lovell’s life and work inspired millions. His courage under pressure helped forge our path to the Moon and beyond-a journey that continues today.”

    Image:
    File pic: AP

    Lovell helped turn the failed moon mission into a triumph after managing to get back to Earth safely after an oxygen tank explosion.

    NASA Administrator Sean Duffy said his the astronaut’s life and work “inspired millions of people across the decades”.

    “Jim’s character and steadfast courage helped our nation reach the moon and turned a potential tragedy into a success from which we learned an enormous amount,” he said. “We mourn his passing even as we celebrate his achievements.

    “From a pair of pioneering Gemini missions to the successes of Apollo, Jim helped our nation forge a historic path in space that carries us forward to upcoming Artemis missions to the moon and beyond.”

    This breaking news story is being updated and more details will be published shortly.

    Please refresh the page for the latest version.

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  • Spacecraft headed to DART asteroid crash site images 2 faint space rocks to boost planetary defense tactics

    Spacecraft headed to DART asteroid crash site images 2 faint space rocks to boost planetary defense tactics

    The Hera mission to follow-up on the aftermath of NASA’s DART asteroid crash has caught sight of two other asteroids in an important test of its camera ahead of its rendezvous its main target: the double space rock system of Didymos and Dimorphos.

    In September of 2022, NASA’s Double Asteroid Redirection Test, or DART for short, slammed into the small asteroid Dimorphos, which orbits the larger Didymos, to demonstrate how potentially hazardous asteroids that could one day be on a collision course with Earth could be bumped off their trajectories so they miss our planet.

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  • Ocean Planet Exploration: MBARI Researchers Deploy New Imaging System To Study The Movement Of Deep-sea Octopus

    Ocean Planet Exploration: MBARI Researchers Deploy New Imaging System To Study The Movement Of Deep-sea Octopus

    MBARI’s innovative EyeRIS camera system collects near real-time three-dimensional visual data about the structure and biomechanics of marine life. Filming deep-sea pearl octopus (Muusoctopus robustus) with this system has provided new insight into octopus locomotion that can contribute to the design of bioinspired robots in the future. Image: © 2022 MBARI Credit © 2022 MBARI

    Editor’s note: When we start to mount Astrobiology missions to explore ocean worlds we’ll need ways for our robotic submersibles to observe and interat with whatever life forms they may encounter. We’re going to our droids to be as smart and self-reliant as possible. This team at MBARI is doing that here on Earth – right now – as they study our own planet’s oceanic depths and the various life forms they encounter – known and unknown.


    MBARI researchers have developed an innovative imaging system that can be deployed at great depths underwater to study the movement of marine life. The team used the system to study deep-sea octopus and shared their findings in the scientific journal Nature.

    EyeRIS (Remote Imaging System) can capture detailed three-dimensional visual data about the structures and movement of marine life in their natural deep-sea habitat. MBARI researchers integrated EyeRIS on board a remotely operated vehicle to observe deep-sea pearl octopus (Muusoctopus robustus) at the famous Octopus Garden offshore of Central California.

    “In MBARI’s Bioinspiration Lab, we look to nature to find inspiration for tackling fundamental engineering challenges,” said Principal Engineer Kakani Katija. “Octopuses are fascinating subjects as they have no bones yet are able to move across complex underwater terrain with ease. Until now, it has been difficult to study their biomechanics in the field, but EyeRIS is a game changer for us.”

    “EyeRIS allowed us to follow several individuals as they moved, completely unconstrained, in their natural environment,” said Senior Research Specialist Crissy Huffard. “Our team was able to get 3D measurements of their arms in real-time as they crawled over the rough terrain of the deep seafloor.”

    EyeRIS uses a specialized, high-resolution camera with a dense array of microlenses that collects simultaneous views of any object in its sight. Software uses that data to create imagery where every pixel in an image is in focus. EyeRIS can create a three-dimensional reconstruction of an animal’s movements so researchers can observe individual features in stunning detail. MBARI researchers used EyeRIS to track the movements of specific points on an octopus’s arm, identifying areas of curvature and strain in real time as the animal crawled over the rugged seafloor.

    Developed by MBARI’s Bioinspiration Lab, EyeRIS (right) enables near real-time three-dimensional imaging and visualization in a compact payload that can be deployed to depths of 4,000 meters (13,100 feet). Image: Joost Daniels © 2021 MBARI

    “EyeRIS data showed that pearl octopus use temporary muscular joints in their arms when crawling, with strain and bend concentrated above and below the joint. This allows them to have simple, but sophisticated, control of their arms,” said Huffard. “The mechanisms of this simplified control could be valuable for designing octopus-inspired robots and other bioinspired technologies in the future.”

    EyeRIS is the latest example of how technology can help us better understand ocean life. This versatile new imaging system can study marine animals that live on the seafloor and in the water column.

    “There is still so much to learn about marine life. EyeRIS will allow us to continue to study the movement and behavior of octopuses and other deep-sea animals in their natural environment using non-invasive techniques. I’m excited to see how this growing body of research and new technology sparks future bioinspired engineering innovation,” said Katija.

    The development of EyeRIS was made possible by the David and Lucile Packard Foundation and the Gordon and Betty Moore Foundation.

    About MBARI

    MBARI (Monterey Bay Aquarium Research Institute) is a non-profit oceanographic research center founded in 1987 by the late Silicon Valley innovator and philanthropist David Packard. Our mission is to advance marine science and engineering to understand our changing ocean. Learn more at mbari.org.

    In situ light-field imaging of octopus locomotion reveals simplified control, Nature

    Astrobiology, Oceanography, robotics,

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  • Heaviest Black Hole Ever Found Pushes Limit of What’s Cosmologically Possible

    Heaviest Black Hole Ever Found Pushes Limit of What’s Cosmologically Possible

    The largest black hole ever detected is 36 billion times the mass of our Sun. It exists near the upper limit predicted by our cosmological models, leaving astronomers with burning questions surrounding the relationship between black holes and their galaxy hosts. 

    In a paper published August 7 in Monthly Notices of the Royal Astronomical Society, researchers announced the discovery of a black hole inside a supermassive galaxy 5 billion light-years from Earth, dubbed the Cosmic Horseshoe. The newly spotted monster is roughly 10,000 times heavier than the supermassive black hole at the Milky Way’s core, according to a statement. Theoretical predictions set the upper bound of a black hole’s mass at 40 to 50 billion times that of the Sun; this cosmic behemoth stands at 36 billion times the Sun’s mass, so it comes precariously close to what calculations allow.

    The Cosmic Horseshoe’s enormous size visibly warps spacetime, bending the light from nearby galaxies into a horseshoe-shaped glare called an Einstein Ring. This fortuitous celestial quirk, along with more traditional detection methods, allowed astronomers to spot the new black hole, which has yet to be named.

    “This is amongst the top 10 most massive black holes ever discovered, and quite possibly the most massive,” Thomas Collett, study co-author and a cosmologist at the University of Portsmouth in England, said in the statement. “Most of the other black hole mass measurements are indirect and have quite large uncertainties, so we really don’t know for sure which is biggest.” 

    Most large galaxies appear to host supermassive black holes at their core, including the Milky Way. Cosmological models predicted that bigger galaxies, like the Cosmic Horseshoe, might be capable of hosting even larger, “ultramassive” black holes. However, such ultramassive black holes were difficult to spot, as the conventional method of tracking the motion of stars around them—stellar kinematics—wasn’t effective for dormant, faraway black holes. 

    The researchers overcame this limitation with gravitational lensing, a method that doesn’t depend on necessarily “seeing” the motion of cosmic entities. They also took observational data from the Very Large Telescope and the Hubble Space Telescope to create a comprehensive model of the galaxy. This two-pronged approach allowed the team to spot a “dormant” black hole “purely on its immense gravitational pull and the effect it has on its surroundings,” explained Carlos Melo, study lead author and PhD student at the Universidade Federal do Rio Grande do Sul in Brazil, in the same statement.

    Another image of the Cosmic Horseshoe, but with the pair of images of a second background source highlighted. The faint central image forms close to the black hole, which is what made the new discovery possible. Credit: NASA/ESA/Tian Li (University of Portsmouth)

    “We detected the effect of the black hole in two ways,” Collett said. “It is altering the path that light takes as it travels past the black hole, and it is causing the stars in the inner regions of its host galaxy to move extremely quickly. By combining these two measurements, we can be completely confident that the black hole is real.”

    “What is particularly exciting is that this method allows us to detect and measure the mass of these hidden ultramassive black holes across the universe,” Melos added, “even when they are completely silent.”

    Another notable aspect of the Cosmic Horseshoe’s environment is that it’s a “fossil group.” These dark, massive systems are primarily driven by gravitational forces and usually come as the final product of a series of galaxy mergers.

    “It is likely that all of the supermassive black holes that were originally in the companion galaxies have also now merged to form the ultramassive black hole that we have detected,” said Collett. “So we’re seeing the end state of galaxy formation and the end state of black hole formation.”

    The new black hole is clearly impressive, and it’ll be exciting to see what else astronomers discover about it. It’s also a fantastic demonstration of multi-messenger astronomy—the coordination of different signal types from the same astronomical event. This has been essential in redefining phenomena that we supposedly “finished” studying, but it’s promising to see it support entirely new discoveries. Either way, there’s no doubt that we’re inching closer than ever to the core of our universe’s many mysteries.

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  • Diabolical mites kill record numbers of honeybees | Good Food

    Diabolical mites kill record numbers of honeybees | Good Food

    You’ve probably heard about colony collapse disorder and the many problems facing our bee population. These issues have persisted for nearly a decade but this winter was particularly disastrous for US beekeepers. Between June 2024, and January 2025, 62% of commercial honeybee colonies in the United States died. That’s the largest die off on record, and it comes on the heels of a 55% die-off the previous winter. What’s going on? 

    We decided to ask Adam Novicki, an agriculture supervisor at the University of California’s Agriculture and Natural Resources Department. He works at the Hansen Agricultural Research and Extension Center in Camarillo. He was also, for a few years, a hobbyist beekeeper

    Evan Kleiman: So let’s talk about this past winter and what happened. Why did so many hives have so much die-off? There appears to be a number one culprit, right? 

    Adam Novicki: I wish it was a single smoking gun, but it’s not. The Varroa destructor is the scientific name of the varroa mite, and that mite is not from the US. It came to America, the United States, in the early 90s, and it originally was from eastern Russia, and it coexisted with another bee called Apis cerana. There’s many different bee species, and Apis mellifera is the one that we know in the West. 

    Long story short is the Apis cerana had evolved with that mite, and one of the things is being very vigilant about keeping them off of other bees. It’s called grooming or hygienic. Unfortunately, the Western honeybee didn’t evolve with that so that mite was able to start to infiltrate and really take advantage of bees. And there’s a number of primary consequences. It’s a vector for many viruses that affect bees, the main one is called deformed wing virus. Basically, when you have bees being compromised their immune systems, like you and I, if we get sick. It’s like when COVID was happening, people with a compromised immune system were in greater danger of perishing. Same thing with the bees. When they start to get compromised, they can’t fight off just chilly weather or other things that might be affecting them, and then the hive suffers.

    How does the varroa mite operate?

    That’s a very good question. There are two stages. One is a really fancy word called phoretic, which really means running around, and those are mites that a beekeeper would see when they open the hive. And those mites are often either just running around, or they are attached to an adult bee, and they’re feeding on that bee and they feed off what the bee blood is, what we call hemolymph, and they feed off that, kind of like a tick. That’s how we see them. But how they reproduce is very diabolical. The female mites will hang around the brood chamber. And a modern hive that you see a white box in a field has 10 frames inside of it. But if you imagine three dimensionally, like a football, lying on its side in that box, then taking up that space, that is the brood chamber. So those mites, those female mites, hang around that area, and they go into the cells where eggs have been laid. And as that egg develops into a larva, they begin laying eggs of their own, which can develop very quickly.  So what they’ve done is they’re feeding off this larva, and they are passing that viral load into that larva. So it doesn’t kill the larva. It just diminishes its prospects. So when it’s born, it often has obvious signs of virus, deformed wing or paralysis, and those bees aren’t going to go anywhere. If you have a deformed wing, you can’t fly, so those bees will eventually die. But what’s even worse is the one that you see attached to the adult bees, those are still passing on the viral load too, but that’s called an asymptomatic transfer, and that, in and of itself, can also cause the bee to get sick.

    Adam Novicki, an agriculture supervisor and former beekeeper, attributes the drastic bee die-off to the varroa mite. Photo by Therese McLaughlin.

    And in a quest to fight off the mites, do bees sacrifice their own larva?

    Correct. Bees have very good hearing, through their antenna, their sensory apparatus. So the development of a bee is interesting, I can tell you very quickly, it takes 21 days to form a typical worker bee. Now a drone bee, which is a male bee that only goes out and mates with other new queens, those take 24 days. Well, these mites will go into those cells, like I mentioned, and they’re developing. They love to go into drone cells, because they’re big, fatter bees that take longer. So you know, it’s like having a buffet open longer. But let’s stick with the worker bees. 

    They go in right before that cell is capped. And as I mentioned, it takes 21 days. So you have an egg. For three days. It’s just an egg, then it develops into a larva, and about day 10, the bees cap it, and that allows the bee to build a cocoon and metamorphosize into an adult bee, which then is hatched by itself at 21 days. Now, without getting too complicated, that in and of itself, once they capped it, the other worker bees will sense that there’s something wrong with that cell, and they will open it, and they will destroy it. They’ll pull that larva out and throw it out of the hive. Now if that keeps happening over and over again, then, you know, bees only live 42 days, so your normal population is dying off. And if you are sacrificing your newbies, then your population is going to start to plummet.

    And once that starts to happen, once a hive reaches a tipping point where the mites can tell that the population is unsustainable, that it’s going to collapse, do they stay and collapse along with the bees, or do they hitch a ride out?

    You know, that’s a very good question. What happens is, and this is, again, sort of cruel fate, Apis mellifera, the race of bee that is most popular for honey production is the Italian honey bee, and it’s still Apis mellifera, but it’s called ligustica, is its subspecies. Long story short, is that particular race of bees is very good at producing honey, but also very good at stealing honey. So other hives, starting with the ones next to it, will notice that that hive is weak. So what are they going to do? They’re going to go into that hive and start stealing all the honey that happens to be left over. And if the hive was strong before, it might have quite a bit of honey. So when they go in to steal the honey, the mites that are on the bees, the remember, the phoretic ones, are running around, they’re going to jump onto the other bees. And those bees will then leave and go back to their own hive, and the life cycle will begin again.

    Can you briefly give us an idea of how huge this problem is?

    Well, there are 1.6 million acres of almonds [in California]. Of that, 1.2 are what they call bearing. The University of California has determined that the optimum number of hives per acre is two. You need 2.4 million hives to adequately pollinate the almonds. Each hive will have minimum of 12,000 bees in each hive, but ideally more. And remember that loss happened in January, and we pollinate February to March. So if you lost 60% of your hives, there were not enough bees to pollinate the crop.

    So in addition to the varroa mite, honeybees are facing two other major problems. The second issue is pesticide exposure, especially neonics. Can you tell us about that?

    The biggest problem with neonics is that, for instance, they’re using corn. Bees don’t pollinate corn, but they sometimes feed off the water that corn sweats. Neonics poison bees in a sub lethal way, and what that means is the bees can’t find their way home, and if they don’t find their way home, then the population is going to suffer.

    So this is fascinating to me. So first, explain what corn sweat is. I’ve seen pictures of it actually on social media. It’s startling.

    Every plant has evapotranspiration, and corn is a grass, and it’s a major crop in North Dakota, where all the bees are for honey production. And when it’s humid and hot, it will sweat all the water it’s taking up from the ground, it’s putting out through its leaves. And as I mentioned, bees don’t pollinate corn. However, they need water. If they’re flying over and they stop, they will grab that sweat, those drops of water that can have traces of neonicotinoids in the bees. And the challenge is that it’s what they call a sublethal dose, so the bees don’t even find a way back for us to determine that indeed what killed them, which offers the chemical company a very convenient defense.

    As you’ve pointed out, beehive die-off is caused by a host of interconnected factors, which isn’t surprising. All of Earth’s nature is just interconnected. Can you talk about how these three big issues, mites, pesticides, and also a decreasing lack of forage are all interconnected, and how they layer on top of each other?

    Again, let’s go back to North Dakota. It’s the number one producing state of honey in America. So when you’re in North Dakota, they have a lot of clover. That’s why, when you see clover honey, it’s generally from North Dakota or South Dakota. Here’s the catch. It used to be they would have marginal land that could not be farmed, and those farmers then would, say it’s 10% of the acreage. Well, that’s great for the bees, because if you have soybean or corn or wheat, they’re not going to go there. But they’ve got plenty of flowers. Well, the technology has caught up where now they can farm marginal land. So because farmers have very tight margins too, they and if anyone can do that, they will. Now the term they use in North Dakota is “ditch to ditch,” meaning there’s drainage ditches. And so now you’re farming nearly 100% of your land. So it really hurt the forage, which means all the flowers. And if you don’t have enough, you’re in really bad shape for the bees, because bees need multiple kinds of sugar and multiple kinds of pollen. The pollen is the protein, the carbohydrate is the nectar. So they need a variety. It’s like if you and I just had a Cliff Bar and 7-Up, you know, I mean, we’d have our protein and we’d have our carbohydrate, but we wouldn’t be very good if that’s all we, you know, wouldn’t be good for you and I.


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  • The Diversity Of Exoplanetary Environments And The Search For Signs Of Life Beyond Earth – astrobiology.com

    1. The Diversity Of Exoplanetary Environments And The Search For Signs Of Life Beyond Earth  astrobiology.com
    2. The search for biosignatures in the Milky Way  Astronomy Magazine
    3. Possible ‘Hints’ Of Life Found On Planet 124 Light-Years Away In James Webb Space Telescope Data  MSN
    4. Find life on other planets? We can’t even agree what it is  thenewworld.co.uk
    5. Potential life exists on K2-18B  The Campanile

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  • Flares On TRAPPIST-1 Reveal The Spectrum Of Magnetic Features On Its Surface

    Flares On TRAPPIST-1 Reveal The Spectrum Of Magnetic Features On Its Surface

    Stellar flares observed in JWST/NIRISS time-series spectroscopy of TRAPPIST-1. Each column shows one flare event during transits of the TRAPPIST-1c or TRAPPIST-1f planets. Tow row: Light curves with the total flux (integrated over the full spectral range and normalized to the mean out-of-transit flux). Colored points indicate pre-flare (green), flare (orange), maximum flare light (red), and post-flare (blue) phases. Green and blue dashed lines mark the average pre- and post-flare flux levels. Middle row: Light curves of the normalized Hα flux. Bottom row: Time-resolved spectrograms (wavelength vs. time) normalized to the pre-flare spectrum. The shaded blue region shows the drop in flux caused by the planetary transit. For comparison, the time axis in all panels are aligned such that t = 0 corresponds to the beginning of the maximum flare light phase. In all four events, the total flux in the post-flare phase is systematically elevated relative to the pre-flare level. — astro-ph.EP

    TRAPPIST-1 is an M8 dwarf hosting seven known exoplanets and is currently one of the most frequently observed targets of the James Webb Space Telescope (JWST).

    However, it is notoriously active, and its surface is believed to be covered by magnetic features that contaminate the planetary transmission spectra. The radiative spectra of these magnetic features are needed to clean transmission spectra, but they currently remain unknown.

    Here, we develop a new approach for measuring these spectra using time-resolved JWST/NIRISS observations. We detect a persistent post-flare enhancement in the spectral flux of TRAPPIST-1.

    Our analysis rules out lingering flare decay as the cause of the flux enhancement and, thus, points to structural changes on the stellar surface induced by flares. We suggest that the flaring event triggers the disappearance of (part of) a dark magnetic feature, producing a net brightening.

    This suggestion is motivated by solar data: flare-induced disappearance of magnetic features on the solar surface has been directly detected in high spatial resolution images, and our analysis shows that this process produces changes in solar brightness very similar to those we observe on TRAPPIST-1.

    The proposed explanation for the flux enhancement enables, to our knowledge, the first measurement of the spectrum of a magnetic feature on an M8 dwarf. Our analysis indicates that the disappearing magnetic feature is cooler than the TRAPPIST-1 photosphere, but by at most a few hundred kelvins.

    Valeriy Vasilyev, Nadiia Kostogryz, Alexander I. Shapiro, Astrid M. Veronig, Benjamin V. Rackham, Christoph Schirninger, Julien de Wit, Ward Howard, Jeff Valenti, Adina D. Feinstein, Olivia Lim, Sara Seager, Laurent Gizon, Sami K. Solanki

    Comments: accepted for publication in The Astrophysical Journal Letters
    Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Solar and Stellar Astrophysics (astro-ph.SR)
    Cite as: arXiv:2508.04793 [astro-ph.EP] (or arXiv:2508.04793v1 [astro-ph.EP] for this version)
    https://doi.org/10.48550/arXiv.2508.04793
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    Submission history
    From: Valeriy Vasilyev
    [v1] Wed, 6 Aug 2025 18:09:01 UTC (4,502 KB)
    https://arxiv.org/abs/2508.04793
    Astrobiology, Space Weather,

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  • The Possibility Of A Giant Impact On Venus

    The Possibility Of A Giant Impact On Venus

    Snapshots of a cross-sectional slice of a head-on collision between a non-rotating Venus and a 0.1 M⊕ impactor at 10 km s−1 . shown at multiple time steps. Initial energy deposition at the impact site generates pressure waves that converge at the antipode, causing significant heating and deformation. The outcome of this collisions is a merger. — astro-ph.EP

    Giant impacts were common in the early evolution of the Solar System, and it is possible that Venus also experienced an impact. A giant impact on Venus could have affected its rotation rate and possibly its thermal evolution.

    In this work, we explore a range of possible impacts using smoothed particle hydrodynamics (SPH). We consider the final major collision, assuming that differentiation already occurred and that Venus consists of an iron core (30% of Venus’ mass) and a forsterite mantle (70% of Venus’ mass). We use differentiated impactors with masses ranging from 0.01 to 0.1 Earth masses, impact velocities between 10 and 15 km/s, various impact geometries (head-on and oblique), different primordial thermal profiles, and a range of pre-impact rotation rates of Venus.

    We analyse the post-impact rotation periods and debris disc masses to identify scenarios that can reproduce Venus’ present-day characteristics. Our findings show that a wide range of impact scenarios are consistent with Venus’ current rotation. These include head-on collisions on a non-rotating Venus and oblique, hit-and-run impacts by Mars-sized bodies on a rotating Venus.

    Importantly, collisions that match Venus’ present-day rotation rate typically produce minimal debris discs residing within Venus’ synchronous orbit. This suggests that the material would likely reaccrete onto the planet, preventing the formation of long-lasting satellites – consistent with Venus’ lack of a moon.

    We conclude that a giant impact can be consistent with both Venus’ unusual rotation and lack of a moon, potentially setting the stage for its subsequent thermal evolution.

    Mirco Bussmann, Christian Reinhardt, Cedric Gillmann, Thomas Meier, Joachim Stadel, Paul Tackley, Ravit Helled

    Comments: Accepted for publication in A&A, 12 pages, 9 figures
    Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
    Cite as: arXiv:2508.03239 [astro-ph.EP] (or arXiv:2508.03239v1 [astro-ph.EP] for this version)
    https://doi.org/10.48550/arXiv.2508.03239
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    Submission history
    From: Mirco Bussmann
    [v1] Tue, 5 Aug 2025 09:12:48 UTC (5,186 KB)
    https://arxiv.org/abs/2508.03239
    Astrobiology,

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  • Scientists discover an organism that defies the definition of life

    Scientists discover an organism that defies the definition of life

    A tidy textbook definition of life has never existed, yet most biology lessons still lean on the idea that living things must grow, make energy, and reproduce on their own.

    That simple checklist leaves viruses outside the club, since their genetic shells activate only inside another organism and go dormant again when drifting alone.


    Ryo Harada of Dalhousie University and colleagues discovered a creature that forces us to redraw those lines on the fly.

    Their oddball microbe, provisionally named Sukunaarchaeum mirabile, was hiding in DNA scraped from a single plankton species off the Japanese coast.

    Sukunaarchaeum virus line blurs

    Biologists once leaned on André Lwoff’s dictum that “an organism is constituted of cells.” That rule pushed viruses into a separate realm of particles.

    That neat boundary already looked wobbly when giant viruses surfaced in the early 2000s, flaunting genomes larger than some bacteria.

    Sukunaarchaeum muddies the waters further. It is undeniably cellular, yet its playbook borrows many viral tricks. It retains the genes for building its own ribosomes and messenger RNA – parts no virus carries – but appears to outsource nearly every other task to a host cell.

    A record-breaking small genome

    The new organism’s entire genome fits into 238,000 base pairs – roughly the length of a medium-sized magazine article.

    For comparison, the minimalist archaeon Nanoarchaeum equitans holds the previous cellular record at about 490,000 base pairs, already microscopic by prokaryotic standards.

    Viruses can be both larger and smaller, yet they never lug around the full toolkit for protein synthesis. That is why Harada’s team calls Sukunaarchaeum “a cellular entity retaining only its replicative core.”

    A virus-like microbe emerges

    “Its genome is profoundly stripped-down, lacking virtually all recognizable metabolic pathways, and primarily encoding the machinery for its replicative core: DNA replication, transcription, and translation,” wrote Harada and co-authors in their report.

    The code resembles a viral instruction manual more than a self-sufficient microbe.

    Yet the creature sits within Archaea, one of the three great domains of life – not among viruses. Phylogenetic trees place it on a deep branch so distant from known groups that the authors propose creating a new phylum.

    Sukunaarchaeum and borrowed genes

    The team stumbled on the microbe while sequencing DNA from the dinoflagellate Citharistes regius. Nested in that plankton’s genetic debris was a tight loop of foreign DNA that refused to match any catalogued species.

    Marine symbiosis can be intimate: some plankton rely on bacterial partners for vitamins, while others house entire algal cells that photosynthesize for them.

    Sukunaarchaeum appears to take this intimacy to the extreme, shaving off every gene it can afford to lose and leaning on its host for nearly everything else a cell needs to stay alive.

    Redrawing the tree of life

    Because its ribosomal genes remain intact, the organism qualifies as cellular under the classic molecular litmus test.

    Yet its pared-down metabolism likely prevents it from harvesting nutrients, producing ATP, or fixing carbon without help – behaviors normally reserved for viral passengers.

    Phylogenetic analyses place Sukunaarchaeum as a deeply branching lineage within the tree of Archaea, representing a novel major branch distinct from established phyla. Environmental sequence data indicate that sequences closely related to Sukunaarchaeum form a diverse and previously overlooked clade in microbial surveys. Credit: JSPS
    Phylogenetic analyses place Sukunaarchaeum as a deeply branching lineage within the tree of Archaea, representing a novel major branch distinct from established phyla. Environmental sequence data indicate that sequences closely related to Sukunaarchaeum form a diverse and previously overlooked clade in microbial surveys. Click image to enlarge. Credit: JSPS

    Scientists debate whether life is a binary label or a spectrum; Sukunaarchaeum pushes the spectrum view to the forefront.

    The find suggests that many other stealth lineages may be hiding in environmental sequencing data, dismissed as contaminants or viral oddities.

    Defining the meaning of “alive”

    Words such as “alive” steer funding, public health policy, and even planetary protection rules for space probes.

    If more organisms like Sukunaarchaeum exist, biosecurity protocols that screen only for free-living microbes could miss entire classes of symbiotic parasites.

    The discovery also sharpens a practical question: What genetic load is the bare minimum for a cell to function? Synthetic biology groups pursuing engineered minimal cells may mine this archaeon’s blueprint for clues.

    “The discovery of Sukunaarchaeum pushes the conventional boundaries of cellular life and highlights the vast unexplored biological novelty within microbial interactions,” wrote the researchers.

    Harada’s team suspects that extreme genome pruning evolved because the host environment guaranteed nutrients, letting redundant pathways decay. 

    Paleobiologists see a glimpse of early evolution, when ancient cells likely shared genes and resources more freely than today.

    If so, today’s viruses and streamlined symbionts may echo an ancient lifestyle rather than representing biological outliers.

    Sukunaarchaeum may not be alone

    Scientists plan to investigate whether similar organisms exist in other marine ecosystems or symbiotic relationships.

    These searches may involve reanalyzing existing metagenomic databases that could contain overlooked sequences resembling Sukunaarchaeum.

    Another goal is to identify the specific host that enables Sukunaarchaeum to survive.

    Without knowing its exact partner, researchers can’t fully explain how the symbiosis functions or what evolutionary pressures shaped such an extreme dependency.

    The study is published in bioRxiv.

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