Category: 7. Science

  • Protein discovery could reverse Huntington’s disease damage, study finds

    Protein discovery could reverse Huntington’s disease damage, study finds

    In the complex world of neuroscience, Huntington’s disease remains a cruel mystery. It slowly strips away a person’s ability to think and move, yet scientists still don’t fully understand why. Researchers at the University at Buffalo have spent over ten years trying to unravel that mystery. Now, they’ve uncovered two tiny but powerful proteins that may hold the key to stopping the disease before it causes irreversible damage.

    What Happens in Huntington’s Disease?

    Huntington’s disease is a rare but devastating condition caused by a genetic mutation in the huntingtin (HTT) gene. This mutation happens when the gene’s DNA code repeats a sequence—cytosine, adenine, guanine (CAG)—too many times. In people with Huntington’s, the number of repeats often goes beyond 36. That small change has big consequences: the altered gene creates a mutated HTT protein that leads to the death of brain cells.

    Most people start to show symptoms around middle age. These can include trouble with movement, thinking, and mood. Eventually, the disease becomes fatal. For years, researchers knew that HTT helped with moving cell parts along thin structures called axons, which are like highways inside neurons. But no one could explain how the mutated version disrupted that process so badly.

    The proteomic network on HTT containing light membranes is dramatically altered in HD iPSC-derived neurons. (CREDIT: Nature Cell Death & Disease)

    Cell Traffic and Dead Ends

    In 2014, the same team at UB discovered that the normal HTT protein worked like a traffic controller. It helps move important cargo along the axons using tiny transport vehicles called vesicles. These vesicles travel thanks to motor proteins like kinesins and dyneins. Without HTT, that cargo gets stuck. Traffic jams form in the neurons, and cells begin to die.

    That early discovery led to a bigger question: What tells HTT when to go, stop, or change direction?

    This year, the team found the answer. Two signaling proteins, GSK3β and ERK1, help regulate that whole transport system. Both proteins are types of kinases, meaning they add small phosphate tags to other proteins to change how they function. But while both are involved, they have opposite effects.

    The Good and the Bad

    To test their theory, scientists used fruit flies genetically altered to have the same HTT mutation as in Huntington’s disease. When they blocked GSK3β, the flies showed fewer traffic jams in their neurons. Their cells were healthier, and the flies could even crawl better. But when they blocked ERK1, the opposite happened. More blockages formed, and more neurons died.

    “With these findings, we propose that ERK1 may protect neurons in the face of Huntington’s disease, while GSK3β may exacerbate it,” said Dr. Shermali Gunawardena, a senior author on the study and associate professor at UB.

    When the researchers increased ERK1 levels instead of blocking it, they saw reduced damage in the cells. That suggests that treatments boosting ERK1 or lowering GSK3β could one day help slow or even stop the disease.

    “There’s not much that can be done once cells have died,” Gunawardena said. “So our whole research is trying to figure out these key, early processes that lead to cell death and whether that can be prevented.”

    Pathogenic HTT triggers abnormal kinase associations with HTT and on membranes. (CREDIT: Nature Cell Death & Disease)

    Zooming in on the Cellular Map

    To dig deeper, the team used stem cell-derived neurons from people with and without the HTT mutation. They isolated membrane structures from the cells and used advanced mass spectrometry to analyze the proteins attached to HTT. What they found shocked them: mutant HTT caused a dramatic shift in the types of proteins it interacted with.

    In healthy neurons, HTT attached to proteins that support cell communication and transport. But in mutant cells, it was linked with different proteins—many of them involved in stress responses and cell death. This suggested that the mutated HTT protein wasn’t just broken. It was actively interfering with other essential cell processes.

    They also saw higher levels of GSK3β and lower levels of ERK1 in the diseased neurons. Even more, the active form of GSK3β was significantly elevated, while the helpful form of AKT1, another regulator protein, was lower. That’s important because AKT1 normally keeps GSK3β in check. When AKT1 is down and GSK3β is up, it creates the perfect storm for neuron damage.

    GSK3β and ERK phosphorylate non-pathogenic and pathogenic HTT in vitro. (CREDIT: Nature Cell Death & Disease)

    The fruit fly experiments confirmed these results. Blocking GSK3β in flies reduced both transport blockages and brain cell death. On the other hand, reducing ERK1 levels made things worse—more damage, more dysfunction. But when ERK1 was boosted, many of those problems improved.

    “The level of ERK1 is clearly important for Huntington’s disease,” said Thomas J. Krzystek, the study’s first author. “Even if we don’t know exactly how it works, the pathway clearly protects neurons.”

    A Path to Better Treatments

    Scientists now believe that the early stages of Huntington’s disease involve a disruption of HTT’s normal role as a scaffold. In healthy cells, HTT helps bring other proteins together at membranes, like parts on a workbench. These include the motor proteins that move cargo and the membrane proteins that receive signals from the rest of the body. But when HTT is mutated, it can no longer hold these pieces in place.

    As a result, entire signaling networks break down. The kinases that should be moving around the cell end up clumping together or disappearing from key areas. That makes it harder for neurons to maintain communication and health.

    GSK3 inhibition mitigates larval locomotion defects, axonal transport blockages, abnormal synaptic morphology, and elevated neuronal cell death elicited by pathogenic HTT. (CREDIT: Nature Cell Death & Disease)

    Among the biggest disruptions was in a group of pathways related to axon guidance, membrane trafficking, and vesicle transport. These pathways are vital for neuron survival. In the diseased cells, proteins like RAB7 and kinesin-1 showed abnormal patterns. That suggests they were either being trapped by the mutant HTT or unable to reach their proper locations.

    These findings are significant because both GSK3β and ERK1 are already targets in other areas of drug development. Small molecule inhibitors for GSK3β and activators for ERK1 exist and are being explored in diseases like Alzheimer’s and cancer.

    “Future treatment could potentially increase a patient’s levels of ERK1 to mitigate their neuronal cell death,” Gunawardena said. “That would need to be done carefully so it doesn’t affect other processes.”

    ERK does not play a major role in axonal transport regulation, unlike GSK3β. (CREDIT: Nature Cell Death & Disease)

    Published in the journal, Nature Cell Death & Disease, the work was funded by the National Institute of Neurological Disorders and Stroke, as well as support from UB’s Mark Diamond Research Fund, the Stephanie Niciszewska Mucha Fund, and the BrightFocus Foundation.

    Though Huntington’s disease has no cure today, the research brings new hope. By targeting key regulators like GSK3β and ERK1, scientists are getting closer to slowing or stopping the condition before damage becomes permanent. And with each new discovery, the tangled web of HTT and its deadly mutation becomes a little clearer.



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  • Titan Could Have An Alien Biosphere – But It Might Be Dog-Sized : ScienceAlert

    Titan Could Have An Alien Biosphere – But It Might Be Dog-Sized : ScienceAlert

    Titan, Saturn’s largest moon, could harbor life in its hidden underground ocean – yet Titan’s entire aquatic biosphere may weigh no more than a miniature poodle, according to new research.

    In disappointing news for alien hunters, the cycle of energy and nutrients in Titan’s hypothetical biosphere may barely be enough to satisfy a single fermenting cell per liter of the moon’s deep ocean, says evolutionary biologist Antonin Affholder from the University of Arizona.

    Tantalizing Titan is unique in the Solar System. Compared to other icy moons, some of which may also harbor life in subsurface oceans, Titan has plentiful organic content, Affholder says.

    Related: New Discovery Crushes Hopes of Finding Alien Life on Titan

    Hydrocarbons on its surface liquify at a frigid -179 degrees Celsius (-290 degrees Fahrenheit), collecting in rivers and pools as large as our own Great Lakes.

    Illustration showing Titan’s distinct layers, modeled on Cassini-Huygens data. (NASA)

    Titan also hides a subsurface water ocean beneath its icy crust. In cross-section, the 5,150-kilometer (3,200-mile) wide Titan may resemble a planetary-scale jawbreaker candy, with five distinct layers, according to Cassini-Huygens data.

    These layers hypothetically begin with a rocky core, then a layer of otherworldly ‘ice-VI’ – an alien ice that only exists at extremely high pressures. Above this sits the salty water ocean. The ocean is sealed by an outer layer of water-ice, which may be about 100 kilometers thick.

    This outer water-ice layer forms Titan’s bedrock, which is continually dusted by organic molecules that fall as raindrops from methane clouds, or settle as solid particles out of the hazy, yellowish atmosphere.

    Titan Could Have An Alien Ocean Biosphere That Weighs No More Than A Small Dog
    Titan’s organics are in constant flux. (NASA/ESA/ CSA/Elizabeth Wheatley (STScI))

    In the upper reaches of the atmosphere, molecules of nitrogen and methane are split apart by UV radiation from the Sun, and then recombine into a variety of heavy organic molecules rich in carbon and oxygen. As they gather on the surface they form tall, dark dunes that resemble mounds of coffee grounds as they fall back to the surface.

    This bounty of organic molecules may seep into Titan’s underground ocean through melt pools formed by meteorite impacts that crack and melt the ice crust. Organic molecules may also drift up into the watery ocean from Titan’s rocky core.

    In the new study, researchers used bioenergetic modeling to ascertain whether these organic molecules could offer the energy to sustain a community of microbes in Titan’s ocean. These microbes could have evolved to produce energy by breaking down glycine, not unlike the class of bacterium Clostridia does here on Earth.

    Titan Could Have An Alien Ocean Biosphere That Weighs No More Than A Small Dog
    A visual summary of organic nutrients seeping into Titan’s subsurface ocean. (Affholder et al., The Planetary Science Journal, 2025)

    Here on Earth, a diverse array of life forms have made use of oxygen as way to conveniently rearrange energetic compounds for growth and energy.

    Deprived of this powerful element, Titan’s microbes could utilize a process of anaerobic respiration similar to one here on Earth known as fermentation.

    Accordingly, the researchers say they chose this “simplest and most remarkable of all biological metabolic processes” because it does not require any speculations on wildly unknown alien metabolisms.

    Fermentation on other ocean worlds could be plausible because it’s a proven strategy on Earth; a ubiquitous and ancient process that now provides Earthlings with culinary favorites like sourdough, yogurt, and beer – yet also food spoilage if left unchecked.

    Additionally, glycine and its precursors are very common throughout the Universe. These molecules are embedded in asteroids, comets, and the clouds of gas and dust that condense into stars and planets.

    However, even though organic molecules like glycine have been enriching Titan’s ocean on geologic timescales, only a piddling portion of this organic inventory may be suitable for microbial consumption.

    This may mean that across Titan’s vast ocean, the overall weight of life could measure “only a few kilograms at most – equivalent to the mass of a small dog,” Affholder explains.

    In other metrics, researchers add that the biosphere would average much “less than 1 cell per kg [2.205 lb] of water over the entire ocean.” Or, the carbon content of a single, approximately 110-pound human.

    With such a Lilliputian population scattered throughout an expansive environment, discovering a living cell would be akin to finding a needle in a haystack – a haystack approximately 800 million miles away.

    This study was published in The Planetary Science Journal.

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  • Microscopic magnet powers search for dark matter in the universe

    Microscopic magnet powers search for dark matter in the universe

    In a chilled lab where temperatures drop close to absolute zero, a speck of magnet hovers in place. This tiny magnet, levitating silently inside a special trap, may hold answers to one of the greatest mysteries in science—dark matter. While no direct signals appeared in this first search, the experiment marks a bold step into a new frontier of physics.

    A New Way to Hunt the Invisible

    Dark matter doesn’t emit, absorb, or reflect light. You can’t see it, but scientists believe it makes up most of the universe’s mass. Without it, galaxies would spin apart. Yet, after decades of searching, no one has directly detected it.

    Now, researchers are turning to an unusual and delicate tool—a magnetically levitated particle. A new experiment led by scientists from Rice University has launched the first search for ultralight dark matter using this technique. The study focuses on a form of dark matter that behaves more like a soft background wave than a single particle.

    Christopher Tunnell is an associate professor of physics and astronomy at Rice and Postdoctoral researcher Dorian Amaral. (CREDIT: Jeff Fitlow)

    Ultralight dark matter, if it exists, might flow through Earth like a ripple in space. These ripples could tug very gently on certain types of matter. But this force would be incredibly small—so faint that only ultra-sensitive equipment could spot it.

    That’s why the team suspended a microscopic magnet inside a cold, superconducting trap. The magnet floated in midair, completely untouched by friction or heat. By creating such a quiet space, the magnet could wiggle if nudged by these ghostly dark matter waves.

    “Our approach brings dark matter detection into a new realm,” said physicist Christopher Tunnell, one of the study leaders. “By suspending a tiny magnet in a frictionless environment, we’re giving it the freedom to move if something nudges it.”

    Listening for the Quietest Whispers

    The experiment used a neodymium magnet less than a millimeter wide. This small piece was placed in a trap cooled to near -459.67°F. That’s almost as cold as anything can get. The setup reduced noise so much that it could detect movements smaller than the size of a single hydrogen atom.

    The researchers watched closely, searching for a signal at a specific frequency—26.7 cycles per second. That’s the rate at which ultralight dark matter in a certain mass range would likely cause oscillations, or tiny repeated movements. Despite the incredible precision, they found no signal.

    Still, this result helps. It sets a new limit on how dark matter can interact with regular matter. The study focused on interactions based on a property in particle physics known as “B minus L.” This stands for the difference between the number of baryons (like protons and neutrons) and leptons (like electrons). These numbers often stay constant during particle reactions.

    The experiment is designed to probe areas of the theoretical landscape that current detectors have not explored. (CREDIT: Rice University)

    In this study, the scientists searched for forces that would act differently depending on these numbers. By not finding any effect, they were able to narrow the possible strength of such dark matter interactions. They ruled out a coupling strength higher than 2.98 × 10⁻²¹, which is among the strictest limits ever set in this area.

    “Every time we don’t find dark matter, we refine the map,” said Tunnell. “It is like searching for a lost key in your house—when you do not find it in one place, you know to look elsewhere.”

    A Dance, a Protest, and a New Path Forward

    The idea for this novel experiment began in an unexpected place: a climate protest. Two physicists met there, talked about their ideas, and even danced a traditional dance known as the polonaise. That moment sparked the name for their next project—POLONAISE.

    Schematic of the experimental setup inside the dilution refrigerator. (CREDIT: Tunnell, et al.)

    This next-generation experiment will improve on the current design in several ways. It will use heavier magnets, which respond more to force. The team also plans to boost the stability of the levitation and scan a wider range of frequencies. That means they’ll be able to look for more types of dark matter than before.

    “Our future setup won’t just listen more closely, it’ll be tuned to hear things we’ve never even tried listening for,” said Tunnell. Dorian Amaral, the study’s lead author, helped lay the theoretical foundation for the measurement. He worked closely with other physicists to design this bold test.

    “We’re not just testing a theory, we’re laying the groundwork for an entire class of measurements,” said Amaral. “Magnetic levitation gives us a fundamentally new tool to ask the universe big questions.”

    This setup isn’t only useful for dark matter. It’s sensitive enough to detect forces as small as 0.2 femtonewtons per square root of hertz. That’s comparable to the weight of a single virus. Reaching this level of sensitivity opens the door to many kinds of future discoveries in physics.

    The force-power spectral density. (CREDIT: Tunnell, et al.)

    What Comes Next?

    The team hopes to improve their system over time. Short-term upgrades will help smooth the levitation and reduce noise. In the medium term, they’ll add better sensors and stronger magnetic materials. In the long run, the final version of POLONAISE could lead the world in dark matter sensitivity across a wide mass range.

    Even though this first attempt didn’t spot dark matter, the value of the experiment goes far beyond a single result. The setup proves that magnetic levitation in a superconducting trap works as a quantum sensor. And that opens up new paths in physics, many of which scientists haven’t yet explored.

    The research team worked with scientists from multiple universities and received support from the National Science Foundation. Together, they built something not just cutting-edge—but potentially revolutionary.

    Each new search like this one brings the world a little closer to understanding the unseen matter that shapes the universe. Whether or not it was found this time, the dark remains a little less mysterious now.



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  • Israeli science joins a global effort: Axiom’s Ax-4 mission

    Israeli science joins a global effort: Axiom’s Ax-4 mission

    Axiom Space’s fourth private mission, Ax-4, launched on June 25 after a series of delays. On June 26, the Dragon spacecraft successfully docked with the International Space Station (ISS), where its four crew members joined the seven astronauts already aboard the station. This Dragon spacecraft carries a new name — Grace — as announced at the time of separation from the upper stage.

    The mission doubles the number of official Indian representatives to have flown in space. Until now, the world’s most populous country had sent only one astronaut — more precisely, a cosmonaut – Rakesh Sharma, who spent a week aboard the Soviet Salyut 7 space station in 1984 as part of Soviet-Indian cooperation. Now, 39-year-old Indian pilot Shubanshu Shukla joins that legacy as a crew member of this private mission and the first Indian citizen to reach the International Space Station.

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    Preparing to enter a cooling phase until next year. An illustration of the spacecraft during its close approach to the Sun

    Preparing to enter a cooling phase until next year. An illustration of the spacecraft during its close approach to the Sun

    (Photo: Axiom Space)

    As with previous Axiom missions, command was assigned to a professional astronaut — Peggy Whitson, who holds the U.S. record for cumulative time in space at 675 days. A former senior NASA astronaut, Whitson joined Axiom after retiring from the agency. Axiom has been selected to develop a private space station to eventually replace the ISS, which is expected to retire by the end of the decade. For Whitson, 65, this marks her fifth visit to the space station, her second with Axiom — and possibly not her last.

    In addition to Whitson, the crew includes representatives from national space agencies, each from a country that previously sent only one astronaut to space during the Soviet era. Engineer Sławosz Uznański-Wiśniewski of the European Space Agency becomes Poland’s second astronaut, while 35-year-old engineer Tibor Kapu is Hungary’s second official astronaut. Hungary’s first unofficial representative was space tourist Charles Simonyi, a Hungarian-American entrepreneur who flew to the ISS twice — in 2007 and 2009 — on privately funded missions.

    Hungary is also collaborating in the continuation of Israeli research focused on detecting lightning sprites and other atmospheric phenomena. In experiments led by Prof. Yoav Yair of Reichman University, astronauts attempt to photograph these colorful, spectacular bursts of light that occur above thunderstorms.

    Though massive in scale, they often last only fractions of a second. Capturing them requires astronauts to aim their cameras with exceptional precision at active storm systems. This is made possible by data provided by Yair, who cross-references detailed storm forecasts with the space station’s orbital path, enabling him to direct the astronauts exactly where to point the camera at any given moment.

    Yair originally developed the experiment for the Columbia mission in 2003, alongside Israel’s first astronaut, Ilan Ramon, who successfully photographed sprites from space before the mission tragically ended with the shuttle’s disintegration. Since then, the experiment has been carried out several times aboard the ISS. In its current form, it was performed by Eytan Stibbe, Israel’s private astronaut on the Ax-1 mission in 2022 — with the Israeli segment named “Rakia Mission.”

    The Rakia Mission later became a public benefit corporation and helped facilitate the inclusion of the experiment in Axiom’s subsequent private missions. While the experiment ended in disappointment during Ax-2, it yielded interesting results in Ax-3. For Ax-4, it is being conducted in collaboration with Professor József Bór of the Hungarian Institute of Earth Physics and Space Science.

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    Preparing to enter a cooling phase until next year. An illustration of the spacecraft during its close approach to the SunPreparing to enter a cooling phase until next year. An illustration of the spacecraft during its close approach to the Sun

    Preparing to enter a cooling phase until next year. An illustration of the spacecraft during its close approach to the Sun

    (Photo: Axiom Space)

    “Kapu is the astronaut designated to lead the experiment, but we conducted a video training session with the entire crew, and everyone expressed interest in participating and capturing these phenomena,” Yair told the Davidson Institute website. He and his colleagues supply forecast data to the astronauts and hope the crew will find time to document as many events as possible. “We’ve already recorded dozens of brief electrical discharges, but we’ve yet to capture Gigantic Jets — massive, high-temperature lightning events,” he noted.

    He also added that the camera used in the experiment doesn’t remain on the space station but travels with the astronauts on each mission. “That’s ideal, since it has had minimal exposure to cosmic radiation, which helps maintain high image quality.” The Israeli experiment is one of about 60 scientific and medical experiments planned for the AX-4 crew during their approximately two-week stay aboard the ISS.

    “The Rakia Mission has been supporting the Hungarian space mission over the past two years,” added Hadar Vernik Shalev, CEO of the Rakia Mission. “We advised them on astronaut selection, candidate screening, and the setup of their mission control room.”

    The mission of Indian astronaut Shubanshu Shukla is generating widespread public interest across the country, which is also developing its own crewed spaceflight program. Sending a representative to the ISS is seen as an important first step.

    “As part of Rakia’s efforts to support space missions, we partnered with CMS School in Lucknow, northern India — Shukla’s alma mater,” said Hadar Vernik Shalev to the Davidson Institute website. “We assisted in developing educational content, translating it into local languages, and establishing a mission control room and visitor center. We’re one of the few organizations globally with the expertise to support missions of this kind, and from our perspective, this collaboration with India is just the beginning.”

    A European company developing spacecraft intended for cargo — and eventually human — transport into Earth orbit has lost its uncrewed spacecraft at the end of a mission it described as a “partial success.” The spacecraft Mission Possible, developed by The Exploration Company, was launched last Monday aboard a SpaceX Falcon 9 rocket from Vandenberg Space Force Base in California, along with other payloads.

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    Preparing to enter a cooling phase until next year. An illustration of the spacecraft during its close approach to the SunPreparing to enter a cooling phase until next year. An illustration of the spacecraft during its close approach to the Sun

    Preparing to enter a cooling phase until next year. An illustration of the spacecraft during its close approach to the Sun

    (Photo: SpaceX)

    Just under three hours after launch, Mission Possible separated from the rocket as planned and began a controlled re-entry over the northern Pacific Ocean. At that point, the spacecraft was operating normally, and mission control successfully activated several onboard experiments for in-space execution.

    The conical capsule, weighing 1.6 tons, survived atmospheric re-entry. Following a brief, expected signal loss caused by the intense heat and plasma buildup during the spacecraft’s re-entry, contact was reestablished. However, communication was lost again just minutes before the scheduled splashdown. The company suspects a malfunction in the parachutes may have caused the spacecraft to crash into the ocean.

    “We apologize to all our clients who entrusted us with their payloads,” the company said, adding that an investigation is underway into the root causes of the spacecraft’s loss.

    The company also stated that once findings are reviewed, it plans to move forward with a follow-up mission as soon as possible. Mission Possible was The Exploration Company’s second space mission. A year earlier, it launched a smaller demonstration craft that also faced setbacks — due to a second-stage malfunction during the maiden launch of the Ariane 6 rocket, the spacecraft became stranded in orbit and was unable to attempt atmospheric re-entry.

    The spacecraft lost last week was a prototype of Nyx, a vehicle the company is developing for orbital cargo transport. On June 16, at the Paris Air Show, the company also announced plans to develop a crewed version of the spacecraft.

    NASA’s Parker Solar Probe has completed another close flyby of the Sun, matching its previous flyby records for the closest approach to our star from December 2024 and March 2025, for both proximity and speed. The spacecraft came within just 6.2 million kilometers of the solar surface and reached a speed of approximately 690,000 kilometers per hour — equaling its own record for the fastest human-made object.

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    Preparing to enter a cooling phase until next year. An illustration of the spacecraft during its close approach to the SunPreparing to enter a cooling phase until next year. An illustration of the spacecraft during its close approach to the Sun

    Preparing to enter a cooling phase until next year. An illustration of the spacecraft during its close approach to the Sun

    (Photo: NASA)

    This marked Parker’s 24th solar flyby since its launch in 2018 — and the final one in this phase of the mission. Last week, mission controllers confirmed a successful pass, with all instruments fully operational, its heat shields enduring extreme temperatures exceeding 900°C. Parker will now shift to a more distant orbit, with no close passes planned until a decision about the mission’s next phase is made sometime next year.

    The data collected during the spacecraft’s flybys of the Sun are used to study solar wind and solar flares—phenomena that affect satellite operations, spacecraft systems, and astronaut health in space. Gaining a better understanding of these events, along with the development of the ability to predict powerful solar outbursts, is critical for planning and advancing deeper space missions, to the Moon, Mars and beyond.

    “Parker Solar Probe remains in excellent health, with both the spacecraft and its instruments ready to continue their groundbreaking mission,” said Arik Posner, Parker Solar Probe program lead scientist. “The spacecraft will keep exploring the solar atmosphere as the Sun enters the declining phase of its 11-year cycle, providing a unique opportunity to study how solar activity evolves and shapes the heliosphere during this pivotal period.”

    The new U.S. observatory named after astronomer Vera Rubin has released its first public images, showcasing its capabilities after entering a trial phase about two months ago. Located in Chile and built over nearly three decades at a cost exceeding one billion dollars, the Vera Rubin Telescope’s debut images reveal its exceptional imaging quality.

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    The world’s largest digital camera that will help unlock the secrets of the universe. The Vera Rubin Telescope at the summit of Cerro Pachón in Chile The world’s largest digital camera that will help unlock the secrets of the universe. The Vera Rubin Telescope at the summit of Cerro Pachón in Chile

    The world’s largest digital camera that will help unlock the secrets of the universe. The Vera Rubin Telescope at the summit of Cerro Pachón in Chile

    (Photo: RubinObs/NOIRLab/SLAC/NSF/DOE/AURA/P. Horálek (Institute of Physics in Opava))

    Equipped with an 8.4-meter primary mirror—not particularly large by today’s standards—the telescope’s true advantage lies in its state-of-the-art camera, roughly the size of a small car and weighing about three tons. Each image it captures is 3,200 megapixels in size, making it the world’s largest digital camera.

    The telescope features an exceptionally wide field of view—about 10 square degrees. Each image covers a portion of the sky roughly 45 times larger than the full Moon. Designed to take around 1,000 images per night, the telescope can survey the entire southern sky every three to four nights. This continuous, wide-field monitoring enables scientists to track changes and ongoing processes, detect previously unknown celestial objects, and, when needed, direct other telescopes toward them for follow-up observations.

    Researchers believe the telescope will identify more stars and planetary systems than any previous instrument, and will also significantly enhance planetary defense by detecting numerous asteroids, including those that could pose a future threat to Earth. Additionally, the observatory will contribute to research on cosmic mysteries such as dark matter and dark energy.

    The Vera Rubin Observatory will operate as part of a broad international scientific collaboration, working with a range of international partners. Among them is Israel’s ULTRASAT space telescope project, in development at the Weizmann Institute of Science and slated for launch in about two years.

    Like the Vera Rubin Telescope, ULTRASAT will have a wide field of view and repeatedly scan large portions of the sky—though in ultraviolet light, rather than in visible light, making the two projects scientifically complementary. As part of the partnership, U.S. scientists will gain access to ULTRASAT’s data, and Israeli researchers will be able to use data from the Vera Rubin Telescope


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  • Galaxies Had a “Thick Phase” – JWST Just Revealed How They Slimmed Down – SciTechDaily

    1. Galaxies Had a “Thick Phase” – JWST Just Revealed How They Slimmed Down  SciTechDaily
    2. Watch This Amazing 3D Visualization Fly Through View Of 5000 Galaxies From The James Webb Space Telescope  MSN
    3. How can the James Webb Space Telescope see so far?  The Conversation
    4. JWST’s early galaxies didn’t break the Universe. They revealed it.  Big Think
    5. Astro Brief: Cosmic Webb  KSMU

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  • Cygnus’ contrasting double star, Albireo

    Cygnus’ contrasting double star, Albireo

    This fan-favorite double star at the head of Cygnus the swan shows off stunning contrasting colors through a telescope.

    • Albireo, a double star in Cygnus, is easily seen with the naked eye.
    • Its two main stars appear gold and blue, though color perception varies.
    • The two stars are far apart and take 75,000 years to orbit each other.
    • “The two stars in this system are both a few times the mass of the Sun and take about 100 years to orbit each other!” said Jim Kaler.

    With the bright Moon lighting the sky our focus is on easy-to-spot targets tonight, such as Albireo at the head of Cygnus the Swan. Also cataloged as Beta (β) Cygni, Albireo is a stunning double star with contrasting colors that is a fan favorite at star parties. 

    Already flying high in the east after dark, the cross-shaped constellation Cygnus is easy to spot with its brightest star, Deneb, at the tail of the Swan and Albireo at the head in the southwestern corner Cygnus’ domain. About 380 light-years distant and shining with a combined magnitude of 3.1, the two components of Albireo are 34” apart — easy to split with any small scope. The brighter star, also called Beta1, is magnitude 3.4 and glows with a golden hue to most observers’ eyes. Beta2 is a fainter magnitude 5.1 but gives off a blue glow, indicating it is hotter than its brighter companion. 

    Take some time with this pair and consider which colors you see. While most report the gold-and-blue pairing, some people see the stars as white and blue, or even yellow and green! (Although that green is a trick of the eyes, as there are no green stars.) 

    Beta1 is a double star as well, but these components are too close to split in a telescope. The two stars in this system are both a few times the mass of the Sun and take about 100 years to orbit each other, according to the stellar expert Jim Kaler. By contrast, the visible components of Beta1 and Beta2 take 75,000 years to orbit each other! 

    Sunrise: 5:38 A.M.
    Sunset: 8:31 P.M.
    Moonrise: 5:19 P.M.
    Moonset: 1:54 A.M.
    Moon Phase: Waxing gibbous (84%)
    *Times for sunrise, sunset, moonrise, and moonset are given in local time from 40° N 90° W. The Moon’s illumination is given at 12 P.M. local time from the same location.

    For a look ahead at more upcoming sky events, check out our full Sky This Week column. 

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  • Meet the Gigantic Saber-Toothed Cat That Tracked Bison-Sized Prey 9 Million Years Ago

    Meet the Gigantic Saber-Toothed Cat That Tracked Bison-Sized Prey 9 Million Years Ago

    A new species of giant saber-toothed cat has been identified, providing fresh insights into the history of North America’s prehistoric predators. This remarkable animal, which lived between 5 million and 9 million years ago, weighed as much as 900 pounds and preyed on animals weighing 1,000 to 2,000 pounds. Researchers made this discovery after a thorough comparison of seven uncategorized fossil specimens with previously identified fossil and bone samples found around the world.

    The Role of Forearm Bones in Identifying New Species

    One of the most surprising aspects of this discovery was the role of the humerus, particularly the elbow region, in determining the species of this giant cat. Traditionally, researchers have used teeth as the primary means of identifying saber-toothed cats. However, in this case, the elbow bones were crucial to recognizing Machairodus lahayishupup. By comparing humerus fossils from various species of big cats, including modern lions, pumas, and tigers, researchers discovered that the large, muscular forearms of this new species were unlike any other known cat. This enabled them to confidently categorize it as a previously unidentified species of saber-toothed cat.

    Through detailed measurements and digital models of fossilized bones, the team was able to distinguish the unique characteristics of this new cat. The largest of the humerus fossils analyzed was more than 18 inches long, significantly larger than the humerus of a modern adult male lion, which averages around 13 inches in length. This difference in size and structure strongly suggests that Machairodus lahayishupup was a giant among the saber-toothed cats.

    A Powerful Predator of the Past

    Scientists estimate that Machairodus lahayishupup weighed an average of around 600 pounds, but it could have taken down prey as large as 6,000 pounds, based on the strength of its forelimbs and hunting habits. These cats likely preyed on large herbivores such as rhinoceroses, giant camels, and ground sloths, which were abundant in North America at the time.

    Study co-author Jonathan Calede, an assistant professor at Ohio State University, described these animals as regularly hunting bison-sized creatures. “This was by far the largest cat alive at that time.” He emphasized that Machairodus lahayishupup was by far the largest cat alive in North America during that period.

    Tracing the Evolution of Saber-Toothed Cats

    The identification of Machairodus lahayishupup raises intriguing questions about the evolution of saber-toothed cats across different continents. While giant saber-toothed cats have been known to exist in Europe, Asia, and Africa, this new find indicates that North America also hosted its own giant species during this period. The question of whether these large cats evolved independently on each continent or shared a common ancestral species is one that researchers are eager to explore further.

    Calede and co-author John Orcutt, who began this project as a graduate student, believe that their findings contribute significantly to the understanding of saber-toothed cat evolution. They propose that the discovery of similar large cats across multiple continents points to either a pattern of repeated independent evolution or a common ancestor that dispersed globally.

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  • Ice World Microbiology: Cryorhodopsins – Astrobiology

    Ice World Microbiology: Cryorhodopsins – Astrobiology

    Pentameric architecture of CryoRs and unusual central channel. (A) Overall view of the CryoR1 pentamer in detergent micelles and nanodiscs. (B) View at the CryoR1 pentamer from the cytoplasmic side. (C) Side view of the central channel in CryoR1. (D) Overall view of the CryoR2 pentamer in crystals. (E) View at the CryoR1 pentamer from the cytoplasmic side. (F) Side view of the central channel in CryoR1. C terminus is colored dark red. — Science Advances

    Imagine the magnificent glaciers of Greenland, the eternal snow of the Tibetan high mountains, and the permanently ice-cold groundwater in Finland. As cold and beautiful these are, for the structural biologist Kirill Kovalev, they are more importantly home to unusual molecules that could control brain cells’ activity.

    Kovalev, EIPOD Postdoctoral Fellow at EMBL Hamburg’s Schneider Group and EMBL-EBI’s Bateman Group, is a physicist passionate about solving biological problems. He is particularly hooked by rhodopsins, a group of colourful proteins that enable aquatic microorganisms to harness sunlight for energy.

    “In my work, I search for unusual rhodopsins and try to understand what they do,” said Kovalev. “Such molecules could have undiscovered functions that we could benefit from.”

    Cryorhodopsins are a group of proteins found in cold-loving microorganisms. They have the remarkable ability to turn cellular electrical activity on and off Credit Daniela Velasco/EMBL

    Some rhodopsins have already been modified to serve as light-operated switches for electrical activity in cells. This technique, called optogenetics, is used by neuroscientists to selectively control neuronal activity during experiments. Rhodopsins with other abilities, such as enzymatic activity, could be used to control chemical reactions with light, for example.

    Having studied rhodopsins for years, Kovalev thought he knew them inside out – until he discovered a new, obscure group of rhodopsins that were unlike anything he had seen before.

    As it often happens in science, it started serendipitously. While browsing online protein databases, Kovalev spotted an unusual feature common to microbial rhodopsins found exclusively in very cold environments, such as glaciers and high mountains. “That’s weird,” he thought. After all, rhodopsins are something you typically find in seas and lakes.

    These cold-climate rhodopsins were almost identical to each other, even though they evolved thousands of kilometres apart. This couldn’t be a coincidence. They must be essential for surviving in the cold, concluded Kovalev, and to acknowledge this, he named them ‘cryorhodopsins’.

    Rhodopsins out of the blue

    Kovalev wanted to know more: what these rhodopsins look like, how they work, and, in particular, what colour they are.

    Colour is the key feature of each rhodopsin. Most are pink-orange – they reflect pink and orange light, and absorb green and blue light, which activates them. Scientists strive to create a palette of different coloured rhodopsins, so they could control neuronal activity with more precision. Blue rhodopsins have been especially sought-after because they are activated by red light, which penetrates tissues more deeply and non-invasively.

    To Kovalev’s amazement, the cryorhodopsins he examined in the lab revealed an unexpected diversity of colours, and, most importantly, some were blue.

    The colour of each rhodopsin is determined by its molecular structure, which dictates the wavelengths of light it absorbs and reflects. Any changes in this structure can alter the colour.

    “I can actually tell what’s going on with cryorhodopsin simply by looking at its colour,” laughed Kovalev.

    Applying advanced structural biology techniques, he figured out that the secret to the blue colour is the same rare structural feature that he originally spotted in the protein databases.

    Phylogeny of CryoRs. (A) Maximum likelihood phylogenetic tree of MRs. The tree includes 2199 sequences reported in (1), 3 sequences of DSE rhodopsins reported in (17), and 40 sequences of CryoRs found in the present work. (B) Enlarged view of the tree branch containing CryoRs. Amino acid residues in helix B at the position corresponding to that of T46 in BR are shown at the tips. (C) Rectangular representation of the phylogenetic tree of the CryoRs and nearby DSE and ACI rhodopsins clades. The inset in the left bottom corner shows amino acids of the seven-letter motifs of CryoR1-5, DSE, and ACI rhodopsins (numbering corresponds to CryoR1). The unique arginine (R57 in CryoR1) is boxed for clarity. — Science Advances

    “Now that we understand what makes them blue, we can design synthetic blue rhodopsins tailored to different applications,” said Kovalev.

    Next, Kovalev’s collaborators examined cryorhodopsins in cultured brain cells. When cells expressing cryorhodopsins were exposed to UV light, it induced electric currents inside them. Interestingly, if the researchers illuminated the cells right afterwards with green light, the cells became more excitable, whereas if they used UV/red light instead, it reduced the cells’ excitability.

    “New optogenetic tools to efficiently switch the cell’s electric activity both ‘on’ and ‘off’ would be incredibly useful in research, biotechnology and medicine,” said Tobias Moser, Group Leader at the University Medical Center Göttingen who participated in the study. “For example, in my group, we develop new optical cochlear implants for patients that can optogenetically restore hearing in patients. Developing the utility of such a multi-purpose rhodopsin for future applications is an important task for the next studies.”

    “Our cryorhodopsins aren’t ready to be used as tools yet, but they’re an excellent prototype. They have all the key features that, based on our findings, could be engineered to become more effective for optogenetics,” said Kovalev.

    Evolution’s UV light protector

    When exposed to sunlight even on a rainy winter day in Hamburg, cryorhodopsins can sense UV light, as shown using advanced spectroscopy by Kovalev’s collaborators from Goethe University Frankfurt led by Josef Wachtveitl. Wachtveitl’s team showed that cryorhodopsins are in fact the slowest among all rhodopsins in their response to light. This made the scientists suspect that those cryorhodopsins might act like photosensors letting the microbes ‘see’ UV light – a property unheard of among other cryorhodopsins.

    “Can they really do that?” Kovalev kept asking himself. A typical sensor protein teams up with a messenger molecule that passes information from the cell membrane to the cell’s inside.

    Kovalev grew more convinced, when together with his collaborators from Alicante, Spain, and his EIPOD co-supervisor, Alex Bateman from EMBL-EBI, they noticed that the cryorhodopsin gene is always accompanied by a gene encoding a tiny protein of unknown function – likely inherited together, and possibly functionally linked.

    Kovalev wondered if this might be the missing messenger. Using the AI tool AlphaFold, the team were able to show that five copies of the small protein would form a ring and interact with the cryorhodopsin. According to their predictions, the small protein sits poised against the cryorhodopsin inside the cell. They believe that when cryorhodopsin detects UV light, the small protein could depart to carry this information into the cell.

    “It was fascinating to uncover a new mechanism via which the light-sensitive signal from cryorhodopsins could be passed on to other parts of the cell. It is always a thrill to learn what the functions are for uncharacterised proteins. In fact, we find these proteins also in organisms that do not contain cryorhodopsin, perhaps hinting at a much wider range of jobs for these proteins.”

    Why cryorhodopsins evolved their astonishing dual function – and why only in cold environments – remains a mystery.

    “We suspect that cryorhodopsins evolved their unique features not because of the cold, but rather to let microbes sense UV light, which can be harmful to them,” said Kovalev. “In cold environments, such as the top of a mountain, bacteria face intense UV radiation. Cryorhodopsins might help them sense it, so they could protect themselves. This hypothesis aligns well with our findings.”

    “Discovering extraordinary molecules like these wouldn’t be possible without scientific expeditions to often remote locations, to study the adaptations of the organisms living there,” added Kovalev. “We can learn so much from that!”

    Unique approach to unique molecules

    To reveal the fascinating biology of cryorhodopsins, Kovalev and his collaborators had to overcome several technical challenges.

    One was that cryorhodopsins are nearly identical in structure, and even a slight change in the position of a single atom can result in different properties. Studying molecules at this level of detail requires going beyond standard experimental methods. Kovalev applied a 4D structural biology approach, combining X-ray crystallography at EMBL Hamburg beamline P14 and cryo-electron microscopy (cryo-EM) in the group of Albert Guskov in Groningen, Netherlands, with protein activation by light.

    “I actually chose to do my postdoc at EMBL Hamburg, because of the unique beamline setup that made my project possible,” said Kovalev. “The whole P14 beamline team worked together to tailor the setup to my experiments – I’m very grateful for their help.”

    Another challenge was that cryorhodopsins are extremely sensitive to light. For this reason, Kovalev’s collaborators had to learn to work with the samples in almost complete darkness.

    CryoRhodopsins: a comprehensive characterization of a group of microbial rhodopsins from cold environments, Science Advances (open access)

    Astrobiology,

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  • exoatlas: Friendly Python Code For Exoplanet Populations

    exoatlas: Friendly Python Code For Exoplanet Populations

    Example exoatlas visualization placing the first discovered transiting exoplanet HD209458b in context with other transiting exoplanets and the eight major Solar System planets. Errorbars use a color intensity that scales inversely with quantity uncertainties, to avoid giving undue visual weight to the least precise data. — astro-ph.IM

    Planets are complicated. Understanding how they work requires connecting individual objects to the context of broader populations.

    Exoplanets are easier to picture next to their closest Solar System archetypes, and planets in the Solar System are richer when seen alongside a growing community of known exoplanets in the Milky Way.

    The exoatlas toolkit provides a friendly Python interface for retrieving and working with populations of planets, aiming to simplify the process of placing worlds in context.

    Zach K. Berta-Thompson, Patcharapol Wachiraphan, Autumn Stephens, Mirielle Caradonna, Catriona Murray, Valerie Arriero, Jackson Avery, Girish M. Duvvuri, Sebastian Pineda

    Comments: Submitted to the Journal of Open Source Software. Please try it at this link https://zkbt.github.io/exoatlas/ and submit GitHub Issues with bugs or suggestions for improvement!
    Subjects: Instrumentation and Methods for Astrophysics (astro-ph.IM); Earth and Planetary Astrophysics (astro-ph.EP); Solar and Stellar Astrophysics (astro-ph.SR)
    Cite as: arXiv:2507.02210 [astro-ph.IM] (or arXiv:2507.02210v1 [astro-ph.IM] for this version)
    https://doi.org/10.48550/arXiv.2507.02210
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    Submission history
    From: Zach K. Berta-Thompson
    [v1] Thu, 3 Jul 2025 00:14:38 UTC (250 KB)
    https://arxiv.org/abs/2507.02210
    Astrobiology

    Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻

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  • Diversity of Rocky Planet Atmospheres In The C-H-O-N-S-Cl System With Interior Dissolution, Non-ideality, and Condensation: Application to TRAPPIST-1e and Sub-Neptunes

    Diversity of Rocky Planet Atmospheres In The C-H-O-N-S-Cl System With Interior Dissolution, Non-ideality, and Condensation: Application to TRAPPIST-1e and Sub-Neptunes

    Atmospheric speciation of TRAPPIST-1e at 280 K above a planetary surface with stable condensates for atmospheres originally in equilibrium with a fully molten mantle. In all panels, the curve colours correspond to the gas species listed in the legend and condensate masses are relative to Earth oceans (EO). Upper panels show the percentage of models by dominant species (VMR > 50%) that satisfy the requirement of a minimum mass of (a) Water, (b) Graphite, (c) α-sulfur, and (d) Ammonium chloride. Lower panels illustrate the composition and total pressure of the atmosphere for (e) CO2-rich above a water ocean, (f) CH4-rich above graphite, (g) CO2-rich above α-sulfur, and (h) CH4-rich above ammonium chloride. Median values are indicated by lines and shaded regions bracket the first and third quartiles. Compare to the atmospheric speciation derived from a partially molten mantle in Figure A5. — astro-ph.EP

    A quantitative understanding of the nature and composition of low-mass rocky exo(planet) atmospheres during their evolution is needed to interpret observations.

    The magma ocean stage of terrestrial- and sub-Neptune planets permits mass exchange between their interiors and atmospheres, during which the mass and speciation of the atmosphere is dictated by the planet’s volatile budget, chemical equilibria, and gas/fluid solubility in molten rock.

    As the atmosphere cools, it is modified by gas-phase reactions and condensation. We combine these processes into an open-source Python package built using JAX called Atmodeller, and perform calculations for planet sizes and conditions analogous to TRAPPIST-1e and K2-18b.

    For TRAPPIST-1e-like planets, our simulations indicate that CO-dominated atmospheres are prevalent during the magma ocean stage, which, upon isochemical cooling, predominantly evolve into CO2-rich atmospheres of a few hundred bar at 280 K. Around 40% of our simulations predict the coexistence of liquid water, graphite, sulfur, and ammonium chloride-key ingredients for surface habitability.

    For sub-Neptune gas dwarfs, pressures are sufficiently high (few GPa) to deviate the fugacities of gases from ideality, thereby drastically enhancing their solubilities. This buffers the total atmospheric pressure to lower values than for the ideal case. These effects conspire to produce CH4-rich sub-Neptune atmospheres for total pressures exceeding around 3.5 GPa, provided H/C is approximately 100x solar and fO2 moderately reducing (3 log10 units below the iron-wüstite buffer).

    Otherwise, molecular hydrogen remains the predominant species at lower total pressures and/or higher H/C. For all planets at high temperature, solubility enriches C/H in the atmosphere relative to the initial composition.

    Dan J. Bower, Maggie A. Thompson, Kaustubh Hakim, Meng Tian, Paolo A. Sossi

    Comments: 41 pages, 10 figures in main text, 8 figures in appendices, submitted to ApJ
    Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
    Cite as: arXiv:2507.00499 [astro-ph.EP] (or arXiv:2507.00499v1 [astro-ph.EP] for this version)
    https://doi.org/10.48550/arXiv.2507.00499
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    Submission history
    From: Dan Bower
    [v1] Tue, 1 Jul 2025 07:14:10 UTC (12,751 KB)
    https://arxiv.org/abs/2507.00499
    Astrobiology

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