Category: 7. Science

  • SpaceX to perform a static fire test of its Falcon 9 rocket ahead of the Crew-11 launch – Spaceflight Now

    SpaceX to perform a static fire test of its Falcon 9 rocket ahead of the Crew-11 launch – Spaceflight Now

    SpaceX’s Falcon 9 rocket, topped with the Crew Dragon Endeavour, is pictured at sunset on Sunday, July 27, 2025. It will launch the Crew-11 mission, which is schedule to liftoff from Launch Complex 39A at NASA’s Kennedy Space Center on Thursday, July 31, 2025. Image: SpaceX

    SpaceX is preparing for a mid-afternoon demonstration on Monday to verify the health of the Falcon 9 rocket that will carry four humans up to the International Space Station this week. The three astronauts and one cosmonaut of the mission, dubbed Crew-11, will carry out a long-duration stay onboard the orbiting outpost with liftoff planned for Thursday, July 31.

    The launch company will fuel its 70-meter-tall rocket at Launch Complex 39A at NASA’s Kennedy Space Center before igniting the nine Merlin engines for a roughly 10-second-long burn. The operation is referred to as a static fire test, since the hold down clamps holding the rocket in place aren’t planned to release ahead of engine ignition as they will on launch day.

    Engine ignition is expected at 3:09 p.m. EDT (1909 UTC), three hours after the conclusion of a dry dress rehearsal in which the astronauts board the Dragon with the Falcon 9 un-fueled.

    Spaceflight Now will have live coverage of the static fire test beginning about 30 minutes prior to ignition.

    SpaceX is using Falcon 9 first stage booster serial number B1094 for the Crew-11 mission. The rocket is flying for a third time, having previously launched Starlink 12-10 on April 29 followed by Axiom Mission 4 on June 25.

    The fully integrated rocket rolled out of the hangar at LC-39A around midnight heading into Sunday morning. The rocket was brought into the launch position shortly before 10 a.m. EDT (1400 UTC) Sunday and the crew access arm swung out to position itself alongside the Crew Dragon Endeavour.

    Mission commander and NASA astronaut Zena Cardman and her three crew mates arrived at KSC on Saturday afternoon in the midst of their planned quarantine period, which is standard for missions to the ISS. She and Oleg Platonov, a Roscosmos cosmonaut and one of two mission specialists, will be flying to space for the first time.

    NASA astronaut and pilot Mike Fincke is returning to space for a fourth time. Japanese Aerospace Exploration Agency (JAXA) astronaut and mission specialist Kimiya Yui is making his second trip to the ISS.

    The crew will live and work onboard the station for at least six months. NASA and its international partners are considering extending the nominal mission to eight months to more closely align with the shifting timelines being put in place by Russia with its Soyuz missions.

    A final decision on the mission length isn’t expected until about a month or so after Crew-11 docks with the ISS.

    The three astronauts and cosmonaut of the SpaceX Crew-11 mission descend from a Gulfstream jet at Space Florida’s Launch and Landing Facility at NASA’s Kennedy Space Center. From bottom to top: Roscosmos cosmonaut Oleg Platonov, Japan Aerospace Exploration Agency (JAXA), NASA astronaut Mike Fincke and NASA astronaut Zena Cardman. Image: John Pisani/Spaceflight Now


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  • NIRPS, New Eye On Sky In Chile

    NIRPS, New Eye On Sky In Chile

    An international team of scientists, including UNIGE astronomers,

    publishes the first results from the new NIRPS near-infrared spectrograph.

    The instrument NIRPS is installed on the 3.6-metre telescope at La Silla Observatory in Chile. On this picture: a spectrum taken by NIRPS during preliminary tests in June 2023 of the star Proxima Centauri. © Etienne Artigau

    An international team led by the Universities of Geneva (UNIGE) and Montreal published the first results today from the NIRPS spectrograph installed on the European Southern Observatory’s (ESO) 3.6-meter telescope in La Silla, Chile. This new instrument, which operates in the near infrared, offers exceptional performance in detecting and characterising exoplanets, particularly around red dwarfs. By combining NIRPS with the HARPS spectrograph, which operates in visible light, astronomers have access to unrivalled spectral coverage for studying exoplanets. The first five scientific papers can be found in the journal Astronomy & Astrophysics.

    The Near-InfraRed Planet Searcher (NIRPS) is a high-resolution spectrograph designed to search for and study exoplanets around stars smaller and cooler than our Sun. Located on the 3.6-meter telescope at La Silla Observatory in Chile, NIRPS officially began scientific observations in April 2023. Its development and construction are the result of a large consortium of scientists and engineers from Canada, Switzerland, Spain, Portugal, France, and Brazil, with the support of the European Southern Observatory (ESO). More than 140 experts contributed to the project, including a large team from the Astronomy Department of the UNIGE Faculty of Science and the National Research Centre PlanetS.

    NIRPS is specially designed to observe in the near-infrared wavelengths. Next to it is the HARPS spectrograph, also designed by Swiss scientists, which has been hunting for exoplanets in visible light since 2003.

    “This new instrument is the result of technological innovations and the fruit of an international collaboration,” says François Bouchy, Associate Professor at the Department of Astronomy, co-leader of the NIRPS project and lead author of the paper describing the instrument’s performance and scientific objectives. “We are proud of the unique and unrivalled performance of NIRPS and excited by the first scientific results.”

    The combination of HARPS and NIRPS offers unique spectral coverage for studying and searching for exoplanets.

    The combination of HARPS and NIRPS offers outstanding spectral coverage for studying and searching for exoplanets. The unique performance of the HARPS+NIRPS tandem makes it one of ESO’s most requested astronomical instruments of the past semester. In parallel with this first-light paper, which accompanies the commissioning and science validation of the brand-new instrument, the consortium is publishing four papers in the journal A&A with the first astrophysical results from NIRPS observations.

    Scrutinising the atmosphere of exoplanets

    The precision of NIRPS in the near-infrared and the possibility of combining it with HARPS in the visible make it possible to study the atmospheres of planets as they pass in front of their star. For their first observations, the astronomers examined the atmospheres of two well-known gas giant exoplanets: WASP-189 b and WASP-69 b.

    The former has one of the most extreme atmospheres, so extreme that evaporated iron can be detected. However, it is only detected in the visible with HARPS and not in the near infrared with NIRPS. ”Iron also exhibits spectral signatures in the near infrared. So we should be able to detect it with NIRPS too!” explains Valentina Vaulato, PhD student at the Department of Astronomy and first author of the study conducted on WASP-189 b. ”Hence there must be another chemical element hiding the iron signature in the near infrared but not in the visible. The hydride anion – a hydrogen atom with two electrons instead of one – is our prime suspect,” concludes the researcher.

    NIRPS observations of the second exoplanet, WASP-69 b, reveal a long tail of helium gas escaping from its comet-like atmosphere. This observation, one of the most detailed of its kind, sheds new light on the evolution of planetary atmospheres under the effect of intense radiation from the host star.

    Detecting exoplanets in the infrared

    NIRPS’ prime targets are the cool red stars known as M dwarfs, by far the most common stars in the galaxy, as they shine more brightly in the near-infrared than in the visible. In its first months of operation, scientists from the NIRPS consortium were able to confirm with unprecedented accuracy the presence of Proxima Centauri b, an Earth-like planet located in the habitable zone of the red dwarf Proxima Centauri, the closest star to our solar system. The team also found evidence of a second, less massive planet orbiting this star.

    NIRPS is also the only near-infrared instrument to observe our Sun every day, to better understand stellar activity and how to limit its impact on the characterisation of exoplanet atmospheres and the detection of Earth-like exoplanets.

    /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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  • Fish in the deep sea help power the ocean’s carbon cycle

    Fish in the deep sea help power the ocean’s carbon cycle

    Mesopelagic fish, living hundreds of meters below the surface, play a quiet but powerful role in carbon cycling.

    A new study confirms that deep-sea fish excrete carbonate minerals, just like their shallow-water relatives. Their massive biomass and physiological traits make them a critical but overlooked part of ocean chemistry.


    Researchers from the University of Miami Rosenstiel School studied the blackbelly rosefish, a deep-sea species that tolerates lab conditions. They confirmed it produces ichthyocarbonate – a mineral excreted by the intestines to maintain salt and water balance.

    “Mesopelagic fish live in deep, cold, high-pressure environments, and until now, it was unclear if they produced carbonate like shallow water fish do – or at what rate,” said Martin Grosell, lead author of the study.

    “This study is the first to confirm that they do and that the mechanisms and characteristics of ichthyocarbonate formation are remarkably consistent across depths.”

    Deep-sea fish produce carbonate

    At 6°C, mirroring its native depth, the blackbelly rosefish excreted carbonate at about 5 mg/kg/hour. This aligns with predictions from previous models that connect metabolism, temperature, and depth.

    The study also tested how carbonate formation resists change. Even when held in laboratory settings far from their original pressure conditions, the fish continued producing carbonate. This suggests the process is robust and not sensitive to depth-induced pressure changes.

    Carbonate excretion comes from the gastrointestinal tract. It’s driven by ion transporters that move bicarbonate into the gut. There, it reacts with calcium and magnesium to form solid minerals. These are expelled into seawater and can later dissolve or sink.

    Deep fish and carbon cycling

    The researchers examined the carbonate composition of the blackbelly rosefish. They found that it matched the mineral makeup found in shallow-water species. Magnesium-rich calcite dominated, with minor aragonite and other forms. These materials dissolve at different rates, affecting their fate in the water column.

    The uniformity suggests that regardless of where fish live, their carbonate waste behaves similarly once expelled. This means deep-sea fish can contribute to upper-ocean carbonate chemistry even if they dwell much deeper.

    “This research fills a major gap in our understanding of ocean chemistry and carbon cycling,” said Amanda Oehlert, co-author and assistant professor.

    “With mesopelagic fish playing such a significant role, their contribution to carbonate flux – and how it might change with warming oceans – deserves greater attention.”

    Chemical engineers of the ocean

    By verifying carbonate production in mesopelagic fish, this work supports broader carbon flux models. Until now, those models included deep fish as contributors, but lacked direct measurements. This new data gives them firmer footing.

    “These results offer strong support for global models of fish-derived carbonate production, which had assumed – but not verified – that mesopelagic species contribute at similar rates,” Grosell said. “Mesopelagic fish aren’t just prey; they’re chemical engineers of the ocean.”

    The study also suggests that mesopelagic fish could influence carbon export. Their carbonates may either dissolve near the surface or fall deeper, adding to seafloor sediments.

    Implications for carbon budgets

    Carbonates affect seawater alkalinity and pH buffering. Fish-sourced minerals, especially from deep waters, could impact how oceans respond to acidification and warming.

    These particles interact with dissolved carbon and influence chemical stability at depth. The study’s results could help refine Earth system models used to forecast these changes.

    The researchers stress that ichthyocarbonate is not trivial waste. It is a steady mineral output with wide-scale consequences. It travels, dissolves, or settles, shaping carbon flow through ocean layers. With up to 94% of global fish biomass living in mesopelagic zones, their contributions matter.

    Understanding when and where this mineral is released is key. It could improve predictions of long-term carbon storage.

    “Ichthyocarbonate release by individual fish is episodic and under sophisticated endocrine control, but we know very little about the timing and frequency of release, offering an important area for future research,” concluded the study authors.

    The study was funded by the National Science Foundation and the University of Miami. The findings are published in the Journal of Experimental Biology.

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  • Lucia Perez Diaz: Expressing Earth with Art

    Lucia Perez Diaz: Expressing Earth with Art

    Lucia Perez Diaz always needed a creative outlet. She studied music from an early age and played the piano through her teens. She was always the one to be scolded for doodling in class.

    Wary that the hustle required by a professional career in music might be challenging and inspired by an influential Earth systems teacher, Perez Diaz chose a geology degree over a music degree when attending the Universidad de Oviedo in Spain. She then completed a master’s degree and Ph.D. in geodynamics at Royal Holloway, University of London, investigating the geologic formation and evolution of the South Atlantic Ocean.

    But Perez Diaz never let go of her creative side. After years of producing intricate illustrations for her own presentations, a pandemic-era refocusing spurred her to grow her illustration business. Now she’s a published children’s book author: Her first book, How the Earth Works, hit the shelves earlier this year.

    In a photograph of an illustration, two hands hold puzzle pieces that look like South America and Africa.
    Perez Diaz’s artwork includes a geosciences poster series. Credit: Lucia Perez Diaz

    “Science is full of inspiring stories,” she said. “Art is a really great vehicle to tell them.”

    Perez Diaz also works as a computational geodynamicist at Halliburton. Learning to program didn’t feel natural to Perez Diaz initially, and she required a lot of support from her peers. But the fact that she eventually succeeded and built a career using those skills motivated her to take on new, unfamiliar projects—like book publishing—with zeal.

    “It’s rarely about having all the skills—it’s more about giving ourselves space to learn and time to get there.”

    “People often ask me, ‘How did you manage to make a book?’” she said. “I’m like, ‘Honestly, because I thought, What’s the worst that could happen?’”

    She hopes to use what she’s learned to help others explore their own creativity. She hosts workshops to show aspiring illustrators that creating art isn’t as daunting as it may seem. “Often we look at others’ achievements and they make us feel like we don’t have their talent or their skills,” she said. “It’s rarely about having all the skills—it’s more about giving ourselves space to learn and time to get there.”

    —Grace van Deelen (@gvd.bsky.social), Staff Writer

    This profile is part of a special series in our August 2025 issue on science careers.

    Citation: van Deelen, G. (2025), Lucia Perez Diaz: Expressing Earth with art, Eos, 106, https://doi.org/10.1029/2025EO250261. Published on 28 July 2025.
    Text © 2025. The authors. CC BY-NC-ND 3.0
    Except where otherwise noted, images are subject to copyright. Any reuse without express permission from the copyright owner is prohibited.

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  • Biologists named a sex pheromone found in mouse urine after Mr. Darcy. ‹ Literary Hub

    Biologists named a sex pheromone found in mouse urine after Mr. Darcy. ‹ Literary Hub

    July 28, 2025, 9:25am

    If you’re anything like me, you’re constantly wondering, “How do these aloof and frankly cold male mice keep attracting partners?!” Science has an answer: Blame it on the darcin.

    Back in 2010, a team of biologists at the University of Liverpool studying major urinary proteins (MUPs) in mouse urine identified a male pheromone that “stimulates female memory and sexual attraction” to that male’s odor and named it darcin. So far so good, but you might be thinking that the name they chose sounds familiar. Well you’re right, and it’s ringing a bell for the exact reason you think. To quote the paper:

    In order to highlight its unusual characteristics compared to all other known MUPs, and its role in female sexual attraction (see below), we named this 18893Da MUP as darcin (after Jane Austen’s hero in Pride and Prejudice).

    Unusual, indeed! Well done, Sarah A Roberts, Deborah M Simpson, Stuart D Armstrong, et al, you found the perfect name for the urine you can’t help but fall for in the end.

    I came across this information while browsing the Mr. Darcy Wikipedia page, and was shocked to come across the phrase “mouse urine.” This led me to the page for “Major urinary proteins,” which amongst images of 3D protein renderings, dot plots, and native gel electrophoresis analyses has this amazing picture and caption:

    I’m not sure where pheromone research is these days, but if scientists ever find a pheromone that makes a male’s intentions extremely obvious to a mate, it could be named “colline.” Or maybe a pheromone that projects overconfidence to others could be “emmane.” Or if they find something that makes you good at hijacking the piano at parties, it could be “maryin.”

    I’m glad the scientists are reading Austen and having a laugh—or “taking the piss” as I’m sure the U of Liverpool PhDs are saying in more ways than one.

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  • Hubble Snaps Beautiful Image of NGC 1309

    Hubble Snaps Beautiful Image of NGC 1309

    The Hubble team has released a stunning new image snapped by the NASA/ESA Hubble Space Telescope of the face-on spiral galaxy NGC 1309.

    This Hubble shows NGC 1309, a spiral galaxy some 100 million light-years away in the constellation of Eridanus. The color image is made up of observations from Hubble’s Advanced Camera for Surveys (ACS) and Wide Field Camera 3 (WFC3) and in the ultraviolet, infrared, and optical parts of the spectrum. Four filters were used to sample various wavelengths. The color results from assigning different hues to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / L. Galbany / S. Jha / K. Noll / A. Riess.

    NGC 1309 is situated about 100 million light-years away in the constellation of Eridanus.

    Otherwise known IRAS 03197-1534, LEDA 12626 or TC 470, this galaxy has a diameter of 75,000 light-years.

    NGC 1309 was discovered by the German-British astronomer William Herschel on October 3, 1785.

    The galaxy is the brightest member of NGC 1309 group, a trio of galaxies that also includes MCG -03-09-027 and UGCA 71.

    “The stunning Hubble image encompasses NGC 1309’s bluish stars, dark brown gas clouds and pearly white center, as well as hundreds of distant background galaxies,” the Hubble astronomers said.

    “Nearly every smudge, streak and blob of light in this image is an individual galaxy.”

    “The only exception to the extragalactic ensemble is a star, which can be identified near the top of the frame by its diffraction spikes.”

    “It is positively neighborly, just a few thousand light-years away in the Milky Way Galaxy.”

    Much of NGC 1309’s scientific interest derives from two supernovae: SN 2002fk in 2002 and SN 2012Z in 2012.

    “SN 2002fk was a perfect example of a Type Ia supernova, which happens when the core of a white dwarf explodes,” the astronomers said.

    “SN 2012Z, on the other hand, was a bit of a renegade. It was classified as a Type Iax supernova: while its spectrum resembled that of a Type Ia supernova, the explosion wasn’t as bright as expected.”

    “Hubble observations showed that in this case, the supernova did not destroy the white dwarf completely, leaving behind a ‘zombie star’ that shone even brighter than it did before the explosion.”

    “Hubble observations of NGC 1309 taken across several years also made this the first time the white dwarf progenitor of a supernova has been identified in images taken before the explosion.”

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  • Tiny dinosaur chirped like birds, Jurassic-era throat bones reveal

    Tiny dinosaur chirped like birds, Jurassic-era throat bones reveal

    Researchers discovered a 163-million-year-old dinosaur that might have chirped like a bird, pushing the origins of birdsong back millions of years.

    In movies and demonstrations, if dinosaurs are depicted in motion, they typically roar as the ferocious beasts that they were. But maybe we cannot judge a book by its cover in this case.

    In a study published last week in PeerJ, researchers from the Chinese Academy of Sciences in Beijing described a brand-new dinosaur species found in 163-million-year-old rocks: the two-foot Pulaosaurus.

    The ancient fossil gave researchers a nearly complete view of its skeleton, which allowed them to identify the new dinosaur as an early member of the duck-billed hadrosaur and horned dinosaur, The New York Times reports.

    They found that it had an unusual throat, though the vocal capacity of dinosaurs has largely remained a mystery to scientists. Thus, it is one of two dinosaurs on record with a preserved throat.

    That area of the body typically doesn’t survive the millions of years it takes a scientist to dig it back up. Dr. Xu, lead author of the study, told The New York Times that “you don’t always have these isolated bones preserved with other skull elements,” even when the skeleton is preserved.

    In this extraordinary case, scientists could examine the Pulaousaurs’ throat bones. They concluded that it could have made birdlike sounds. There was only one other dinosaur found previously that seemed to possess this ability, and neither one of them was remotely related to birds.

    A mysterious aspect of the dinosaurs comes to light. What sound did they make? Were they tweeting and chirping, rather than roaring at one another? Maybe it was a mix of different sounds, but the latest discovery changes the entire image of the dinosaurs, even in theory.

    Were T. rexes tweeting at one another?

    In the study, scientists described a new fossil from the Upper Jurassic Tiaojishan Formation, County Qinglong, Province Hebei, China.

    The well-preserved snapshot of the small herbivore included “ossified laryngeal elements,” which suggests that “bird-like vocalization evolved early in non-avian dinosaur evolution,” as per the study in PeerJ.

    Scientists named it after a Chinese legend of the “Pulao,” a dragon that could shout loudly, so it will always be remembered as a dinosaur species that might have made sounds, though more like a bird.  

    Two terrestrial dinosaurs that could have sounded like birds

    When scientists compared the new specimen to the only other dinosaur to be discovered with its vocal anatomy intact—the armored ankylosaur Pinacosaurus—it appeared that the Pulaousaur shared a similar vocal set-up.

    Although they lacked a voice box like birds, their bony larynx was “large and mobile enough to possibly help produce birdlike noises,” according to the New York Times. However, the Pinacosaurus lived millions of years after the Pulaousaur, so this anatomical structure was less developed.

    Neither of these dinosaurs bears any relation to modern-day birds whatsoever. They aren’t related to any of their ancestors at all. Puzzling, as the discovery would suggest that this vocal capacity might have evolved in separate lineages. And it could have emerged in the earliest dinosaurs, over 230 million years ago.

    “We hope that in the future we can find more specialized structures relating to sound so we can do research on how dinosaurs produced their voices,” Dr. Xu concluded to The New York Times.

    Read the study in PeerJ.

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  • AI is taking scientific discovery from decades to minutes

    AI is taking scientific discovery from decades to minutes

    The hardest math in science has long been a bottleneck, delaying discoveries across physics, chemistry, and climate. But that’s starting to change, as AI slashes equation-solving times from years to minutes.

    Researchers who once waited a decade for enough computing power or clever tricks to tame complex formulas are now solving them in an afternoon.


    That leap is cataloged in a new 500-page review that maps out how learning algorithms are reshaping everything from drug design to climate modeling.

    Science’s equation problem

    Nature is divided into quantum, atomic, and continuum regimes, each governed by complex differential equations.

    “The goal of natural sciences is to understand the world on different temporal and physical scales, leading to three main systems: quantum, atomic, and continuum,” said study co-author Dr. Shuiwang Ji of Texas A&M University.

    Take Schrödinger’s equation, the backbone of quantum mechanics. It can be solved cleanly for two electrons but becomes hopeless when millions of particles interact.

    As the particle count rises, the number of variables grows exponentially, a curse of dimensionality that locks up even supercomputers.

    Traditional numerical tricks approximate the answers, yet they still demand weeks of high-performance computing time and deliver limited accuracy. That bottleneck slows fields that depend on quantum chemistry, such as battery design and catalyst screening.

    Teaching AI the hard math

    Machine learning models trained on known solutions learn to spot hidden patterns that humans miss. Once trained, they guess the wave functions or fluid pressures for new systems in seconds, often matching conventional solvers to within a percent.

    Unlike black-box predictors, the latest architectures bake in physical symmetries, so rotations or reflections leave the output unchanged. That makes the networks both faster and more trustworthy because they respect conservation laws by design.

    Ji and more than sixty collaborators detail strategies such as equivariant graph neural networks that treat atoms as nodes and bonds as edges.

    Their review also surveys large language models that write simulation code on demand, a trick already used inside Texas A&M’s RAISE Initiative labs.

    An early win came when graph neural nets replicated a month-long density functional theory run in under ten minutes on a laptop. That drop in cost means students can explore chemical space during an afternoon lab section instead of reserving cluster time.

    AI science breakthroughs in action

    The 2021 release of AlphaFold predicted shapes for roughly two hundred million proteins in about a year. Biologists who once waited months for an X-ray structure can now plan experiments the same morning.

    Materials scientists are using graph networks to screen millions of candidate battery electrolytes, pruning the list to a handful that survive expensive bench tests.

    Early prototypes have already pushed lithium-ion lifetimes past three thousand charge cycles in lab cells.

    Climate modelers plug neural solvers into global circulation codes, trimming the daily energy bill of a typical run by forty percent while keeping storm tracks intact. That saving frees funds to explore more emission scenarios instead of paying electricity costs.

    The limits of AI in science

    “We are using AI to accelerate our understanding of science and design better engineering systems,” said Ji. That ambition demands rigorous benchmarks, uncertainty estimates, and open data so other teams can replicate results.

    Data scarcity dogs many frontier problems, from fusion plasma turbulence to rare earth magnet phases. Researchers address this by augmenting sparse measurements with simulations, yet that may smuggle in the very biases they hope to escape.

    Ethical concerns loom as well, because AI that speeds drug discovery could just as easily accelerate toxin design.

    Leading groups advocate real-time screening of generated molecules against pathogen threat databases before any synthesis request reaches a vendor.

    Solving science together

    Ji’s team argues that no single lab can cover the sprawling space of quantum, atomistic, and continuum problems. Their paper itself is a proof, spanning fifteen universities and more than five hundred pages.

    The RAISE Initiative recruits over eighty-five faculty, pairing computer scientists with chemists, geologists, and civil engineers inside shared Slack channels. Weekly data-sharing sessions cut redundant efforts and seed joint grant proposals that draw on strengths across campus.

    Industry is leaning in, too, as pharmaceutical giants supply curated reaction data while earning early access to improved models.

    Start-ups license those models through cloud APIs, letting a small lab anywhere run high-end quantum chemistry without buying a single server.

    Science discovery at machine speed

    If the past four years are any guide, everyday researchers will soon treat AI solvers like they treat spreadsheets, a default tool that lives on every desktop.

    Once that happens, the defining question shifts from whether to trust AI to how to spend the freed-up creative energy.

    Young scientists might redirect their mornings from debugging Fortran toward framing deeper hypotheses, while seasoned engineers iteratively refine prototypes instead of waiting for a cluster queue slot.

    History suggests that when a method cuts cost by an order of magnitude, it sparks waves of experiments that nobody previously dared to attempt.

    Policymakers could feel the impact too, because faster simulations let agencies stress-test infrastructure plans against many more climate or seismic scenarios. More scenarios translate into codes that protect communities rather than average-case assumptions.

    Ji sees that horizon already, noting his own curiosity for fundamental science as the spark that keeps the collaboration moving. He and his colleagues hope that by teaching AI the language of physics, science can advance through better questions – not just faster answers.

    The study is published in the journal Foundations and Trends in Machine Learning.

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  • NASA Captures Haunting Photos of Lightning Illuminating a Tropical Storm

    NASA Captures Haunting Photos of Lightning Illuminating a Tropical Storm

    Lightning illuminates the cloud tops of Tropical Storm Erick as it stormed across the Pacific coast of central Mexico at approximately 3:38 a.m. local time on June 20 as the International Space Station orbited 258 miles above.

    Floating 258 miles above, NASA astronauts on board the International Space Station have a view like no other and can therefore photograph Earth in unique ways.

    Recently, the NASA Johnson Flickr page uploaded a dramatic set of photos showing the inside of a tropical cyclone. The picture was lit by thunder bolts.

    Category 1 Hurricane Erick brought heavy rainfall to parts of southern and southwestern Mexico in June 2025. It caused flash floods and mudslides that left at least 23 dead, 28 injured, and two missing. The total damage was estimated at $250 million, according to Wikipedia.

    Bright, swirling blue and white light forms a spiral pattern against a pitch-black background, resembling a glowing galaxy or nebula in space.
    The lightning dramatically illuminates Hurricane Erick for a unique photo.
    A glowing, cloud-like nebula with bright white and blue light at its center is surrounded by darkness, giving the appearance of a cosmic storm or a luminous cloud in deep space.
    NASA

    The awesome photos do not have an author ascribed to them, but we do know they were taken on June 20 at roughly 3.42 AM local time as Hurricane Erick stormed across the Pacific Ocean south of the Mexican state of Chiapas. The photos were uploaded just a few days ago.

    Astronauts onboard the ISS have become prolific photographers, and while the identity of the photograph’s author is unknown, we do know it was shot on a Nikon Z9 with a Nikon 200mm f/2 VR attached, set at 1/125 of a second, f/2.0, and 12,800 ISO.

    Dark storm clouds illuminated from within by a bright flash of lightning, surrounded by deep shadows, creating a dramatic and intense atmosphere in the night sky.

    The photos were likely taken by one of the Expedition 73 Crew, which includes NASA flight engineers Anne McClain, Nichole Ayers, and Jonny Kim. Out of the three, Nichole “Vapor” Ayers has proven to be the most accomplished photographer, having captured a spectacular image of a sprite — a rare form of lightning that shoots up from a thunderstorm — earlier this month.

    Don Pettit, who is arguably the best photographer to ever visit space, mentioned last year that he was on a mission to capture a photo of a sprite directly from above. Along with fellow talented photographer and astronaut Matthew Dominick, the pair were shooting thousands of photos while flying over lightning storms in the hope that a sprite would shoot up toward them. Sadly, it hasn’t been accomplished yet.


    Image credits: NASA

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  • Study Says This Sleep Factor May Matter More Than Sleep Quality

    Study Says This Sleep Factor May Matter More Than Sleep Quality

    As the study’s lead author Anita Lenneis, Ph.D., explains in a news release, “Our results found that how young people evaluated their own sleep was consistently linked with how they felt about their well-being and life satisfaction,” adding that when participants reported sleeping better than they normally did, for instance, they actually experienced more positive emotions and had a higher sense of life satisfaction the next day.

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