Category: 7. Science

  • Lead was turned into gold – but only for a trillionth of a second

    Lead was turned into gold – but only for a trillionth of a second

    The 17-mile Large Hadron Collider (LHC), located beneath the French-Swiss border, regularly slams heavy ions together at near light speed. But on July 30, 2025, researchers reported something many thought belonged to folklore: lead ions momentarily changed into gold before decaying back into more ordinary matter.

    The analysis shows that a single run of lead can produce gold nuclei with a cross section comparable to the total hadronic collision rate. This makes the “modern alchemy” far more common in the tunnel than anyone expected.


    “Usually in collider experiments, we make the particles crash into each other to produce lots of debris,” said Daniel Tapia Takaki, professor of physics at the University of Kansas and leader of the group on the ALICE experiment.

    His team developed the method that spots what happens when the ions merely graze, an interaction so clean that almost nothing else appears in the detectors besides a flash of light and an altered nucleus.

    Gold from lead, briefly

    Ultraperipheral collisions happen when two atomic nuclei pass close to each other without touching, but their powerful electromagnetic fields still interact.

    Instead of smashing apart, each ion showers the other with a burst of high-energy photons described by the Weizsäcker Williams method, allowing photons from one nucleus to probe or even transform its partner. That photon barrage can knock out one, two, or three protons.

    If three protons are lost, the lead-208 nucleus briefly becomes a gold-205 nucleus – fulfilling the alchemist’s dream, though only for about 10⁻²³ seconds. That’s just long enough to leave a signal in the forward calorimeters.

    Previous ALICE runs hinted that such clean events existed, but the detector was optimized for messy head on smash ups. Tapia Takaki’s team re-tuned readouts, added vetoes, and refined a two-stage fit to isolate neutron from proton peaks.

    What near miss collisions reveal

    Because photons carry no net charge, photon photon or photon nucleus interactions are free from the spray of hadronic debris that plagues central collisions. The clean environment allows physicists to study nuclear structure and test QED at previously unreachable energy scales.

    The Kansas-led analysis clocked a gold production cross section of 6.8 barns, only 12 percent shy of the 7.67 barn total inelastic rate for ordinary lead-lead interactions at the same energy.

    That means every time the LHC delivers a hadronic ion collision, there is roughly another event nearby where a lead ion quietly becomes gold and then disintegrates.

    The same data set pinned the 0 proton channel at 157.5 barns, the 1 proton channel at 40.4 barns, and the 2 proton channel at 16.8 barns. These results matched or exceeded theoretical predictions from the RELDIS photonuclear model within 25 percent.

    Discrepancies suggest existing models poorly capture pre-equilibrium emission and nucleon coalescence in single proton channels.

    Tracking alchemy at light speed

    The ALICE collaboration relies on zero degree calorimeters placed 369 feet downstream of the interaction point to record neutral and charged fragments.

    The KU team gated on events where proton energy fell within two standard deviations of the beam energy and at least one neutron hit the neighboring neutron calorimeter. This isolated a data set of just two million events from 2.05 million triggers.

    They corrected for acceptance, efficiency, and the small chance that a peripheral hadronic collision could imitate an electromagnetic event.

    Monte Carlo studies using RELDIS and the AAMCC-MST transport code showed that hadronic imposters contribute less than one percent to the single proton sample, leaving the photon driven signal essentially pure.

    The resulting fit revealed broad 1 proton and broad 2 proton peaks, about twice as wide as the corresponding neutron peaks. This is because relativistic protons can leak energy at the calorimeter edges or through interactions with beam line material.

    A modified Gaussian model with width scaling by proton count corrected smearing – now adopted by other heavy ion groups.

    Flash matters for future colliders

    Removing three protons turns lead into gold, but knocking out even one proton turns the ion into thallium, which bends differently in the LHC magnets.

    Secondary particle beams that aren’t properly controlled can hit cold components, shut down superconducting magnets, or trigger safety systems. These issues could limit the performance of future 27 TeV upgrades and the proposed 100-km Future Circular Collider.

    By measuring the full suite of 0- to 3- proton channels, the ALICE team provides essential inputs for loss maps that machine engineers use to design collimators and shielding.

    The data also feed into simulations for the U.S. Electron Ion Collider (EIC), where understanding photon induced breakup of nuclei is critical for background rejection in precision measurements.

    More than just gold

    Beyond gold, near-miss collisions can produce mercury, thallium, or platinum isotopes – each with unique decay paths and insights.

    Light-by-light scattering, axion-like particle searches, and studies of nuclear excitation all benefit from knowing exactly how often and how cleanly these channels occur.

    Tapia Takaki noted that the study may be crucial for designing the next generation of machines, because every lost beam ion costs days of accelerator time and significant operational money.

    In short, catching a blink of gold is less about getting rich and more about keeping billion dollar facilities running safely and efficiently.

    Next steps for gold physics

    The team plans to extend the analysis to four and five proton emissions once Run 3 data arrive, pushing sensitivity toward nuclei around hafnium and tantalum.

    They’re working with theorists to refine photonuclear models so neutron-to-proton ratios better match observations.

    A dedicated trigger for ultraperipheral collisions is in development. It combines existing calorimeter logic with real-time machine learning filters to capture rare events without overwhelming the data acquisition system.

    If successful, physicists could watch modern alchemy unfold almost as it happens, perhaps even identifying long lived isomers before they decay in flight.

    The study is published in the journal Physical Review C.

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  • The AI debate in student accommodation

    The AI debate in student accommodation

    Artificial Intelligence is quietly reshaping the student accommodation experience.rom chatbots answering late-night queries and streamlining bookings, to using data to provide a more personalised experience, AI is transforming how purpose-built student accommodation (PBSA) operators run their properties and the way in which students experience them.

    Across the industry, there are examples of operators using AI to improve operations, particularly the student booking experience. Operators are using AI-driven chatbots to provide instant responses to questions about rent payments, maintenance, or move-in dates. Booking platforms such as Student.com’s new AI-powered booking platform use AI to secure bookings almost instantly and reduce the process from days to minutes.

    AI is also being used to predict demand and occupancy, suggest personalised services and amenities for students based on each resident’s behaviour and preferences, streamline maintenance reporting and responses, and even to help prevent resident conflict through predictive analytics.

    AI is also being used to improve building operations – AI-enabled sensors can adjust lighting and temperature automatically, while predictive maintenance tools help building managers prevent disruptions before they occur.

    In some cases, AI is even being used to detect early signs of student distress, flagging social withdrawal or patterns that may suggest someone is struggling and prompting pastoral support.

    But as AI becomes more embedded in PBSA, it raises critical questions. What happens to the human touch? And how to balance efficiency with privacy?

    There are also growing concerns around surveillance. AI-powered security systems, facial recognition check-ins, and behaviour-tracking tools may enhance safety, but they can also create an atmosphere of constant monitoring. Add to that the ethical grey areas of data collection and privacy, and the picture becomes more complex.

    The challenge facing accommodation providers is not whether to adopt AI, but how. The most forward-thinking operators are using AI to support staff rather than replace them. By automating routine tasks, residential teams are freed up to build relationships, support wellbeing, and foster community. Implemented strategically, it is clear that AI can help student accommodation become more responsive, more inclusive, and more attuned to individual needs. AI is certainly the future of PBSA, but the kind of future it shapes depends on the choices made today.

    For a deeper dive into how AI is changing the student living sector and to hear from leaders across the PBSA sector about what is at stake, head over to the Summer Edition of Unlocked, GSL’s online magazine.


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  • Scientists have spotted the biggest explosions in the Universe since the Big Bang.

    Scientists have spotted the biggest explosions in the Universe since the Big Bang.

    Scientists from the University of Hawaii’s Institute for Astronomy (IfA) have discovered the most energetic cosmic explosions since the Big Bang.

    Extreme nuclear transients (ENTs) occur when massive stars several times larger than our Sun are torn apart by supermassive black holes.

    ENTs shine with intense luminosity, much brighter than supernovae, which originate from the violent death of massive stars.

    Animation showing a star being torn apart by a black hole

    Biggest explosions ever seen

    One ENT observed by the team at IfA emitted over 25 times more energy than the most energetic supernovae known, radiating the energy of around 100 Suns in a single year.

    “We’ve observed stars getting ripped apart as tidal disruption events for over a decade, but these ENTs are different beasts, reaching brightnesses nearly 10 times more than what we typically see,” says Jason Hinkle, the researcher at IfA who led the study.

    The vast amount of energy released by these explosions can be visible over huge distances.

    Hinkle first uncovered ENTs when searching for long-lived flares coming from galactic centres.

    Hubble Space Telescope image of galaxy located 600 million light-years away that is host to the telltale signature of a roaming supermassive black hole. The bright dot is tidal disruption event AT2024tvd, a flash of radiation caused by the supermassive black hole eating a star. Credit: NASA, ESA, STScI, Yuhan Yao (UC Berkeley); Image Processing: Joseph DePasquale (STScI)
    Hubble Space Telescope image of galaxy located 600 million light-years away that is host to the telltale signature of a roaming supermassive black hole. The bright dot is tidal disruption event AT2024tvd, a flash of radiation caused by the supermassive black hole eating a star. Credit: NASA, ESA, STScI, Yuhan Yao (UC Berkeley); Image Processing: Joseph DePasquale (STScI)

    The intense outbursts are examples of transients: astrophysical events that change brightness over a relatively short time.

    In his search of data from ESA’s Gaia mission, he discovered two particularly unusual events that brightened over a timescale longer than typical transients, and without their other characteristics.

    The researchers determined that ENTs could not be simple supernovae because they release far more energy.

    Instead, their unique characteristics suggest the involvement of a supermassive black hole.

    This is a new artist’s impression of our galaxy, the Milky Way, based on data from ESA’s Gaia space telescope. Credit: ESA/Gaia/DPAC, Stefan Payne-Wardenaar
    Artist’s impression of our galaxy, the Milky Way, based on data from ESA’s Gaia space telescope. Credit: ESA/Gaia/DPAC, Stefan Payne-Wardenaar

    Insights into black hole secrets

    “ENTs provide a valuable new tool for studying massive black holes in distant galaxies,” adds Benjamin Shappee, associate professor at IfA and the study’s co-author.

    “By observing these prolonged flares, we gain insights into black hole growth when the Universe was half its current age, when galaxies were happening places – forming stars and feeding their supermassive black holes 10 times more vigorously than they do today.”

    ENTs remain rare, occurring 10 million times less frequently than supernovae. As such, their detection is challenging.

    Future observatories like the Vera C Rubin Observatory and NASA’s Roman Space Telescope will aid in the search for these cosmic flashbangs.

    A small section of NSF-DOE Vera C. Rubin Observatory's total view of the Virgo cluster. Visible are two prominent spiral galaxies, three merging galaxies, several groups of distant galaxies and many stars in the Milky Way galaxy. Credit: NSF-DOE Vera C. Rubin Observatory
    A small section of NSF-DOE Vera C. Rubin Observatory’s total view of the Virgo cluster. Visible are two prominent spiral galaxies, three merging galaxies, several groups of distant galaxies and many stars in the Milky Way galaxy. Credit: NSF-DOE Vera C. Rubin Observatory

    Future study of ENTs

    Words: Chris Lintott

    To follow up on discoveries like these, you need a telescope capable of monitoring the whole sky, one that can ferret out unusual events.

    We’re about to get such an instrument, with the Vera C Rubin Observatory now starting operations as of summer 2025.

    With a mirror as large as some of the largest telescopes on Earth, the world’s largest camera and an ability to scan the whole sky every three nights, Rubin will help spot the ‘weird’ in the Universe.

    Producing 30 terabytes of data a night and issuing roughly 10 million alerts, it will revolutionise how astronomical research is conducted.

    We’re about to be surprised by more ENTs – and plenty of other novelties besides.

    This article appeared in the August 2025 issue of BBC Sky at Night Magazine

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  • August’s first Titan shadow transit

    August’s first Titan shadow transit

    The first of two Titan shadow transits this month occurs this morning — can you catch the big, black shadow crossing Saturn’s cloud tops?

    • Observers in the U.S. can witness the transit of Titan’s shadow across Saturn’s northeastern limb, beginning approximately 2:03 A.M. EDT on the specified date.
    • The shadow’s transit will last roughly an hour and fifty minutes, traversing Saturn’s disk from east to west, concluding around 5:12 A.M. MDT.
    • Concurrently, the moons Enceladus and Tethys will also be transiting Saturn’s rings, observable primarily through imaging due to their faint magnitudes (11.8 and 10.3, respectively).
    • Saturn’s rings, spanning 40″ end-to-end and only 2.5″ in thickness, will provide a striking backdrop to the celestial event; Saturn itself can be readily located in Pisces, below the Circlet asterism.

    U.S. observers can catch the first of two transits of Titan’s shadow across Saturn this month — and one of the last few of the year, before cosmic alignment that allows the shadow to cross the cloud tops comes to an end.

    Saturn now rises shortly after 10 P.M. local daylight time and is located in Pisces, hanging below the Circlet asterism. Shining at magnitude 0.8, it’s brighter than the nearby stars, making it easy to pick out in the sky. By local midnight, it is roughly 20° high in the east. Point your telescope at the ringed world, and you should also capture distant Neptune (magnitude 7.7) in your field of view. The ice giant is just over 1° north of Saturn, and will sit exactly due north of Saturn in just a few days.

    Saturn’s rings are, as always, stunning. They are also quite thin, with the narrow axis spanning just 2.5”. They stretch more than 40” from end to end. 

    But today, our attention is on the northeastern limb of Saturn. Note that Titan, easily visible at mid-8th-magnitude, lies some 15” from the planet. But at 2:03 A.M. EDT — note this is just after midnight in the Mountain time zone and still late on the 2nd in the Pacific time zone — Titan’s shadow begins to appear on the northeastern limb, taking nearly 20 minutes to fully appear. The shadow slowly crosses from east to west, reaching roughly midway on the disk around 4:30 A.M. EDT. Titan is now 10” from the planet. 

    The shadow finally reaches the northwestern limb and begins to disappear around 5:12 A.M.  MDT — after sunrise in the Midwest, leaving only the western half of the U.S. to view its exit. As with ingress, it takes about 20 minutes for the shadow to fully disappear.

    There’s an added bonus for imagers: During this time, two of Saturn’s smaller, fainter moons are also transiting. Enceladus (magnitude 11.8) and Tethys (magnitude 10.3) appear just north of the rings for much of the shadow’s transit. Timing-wise, Enceladus begins to transit around 2:10 A.M. EDT, while Tethys’ transit begins around 2:33 A.M. EDT. They take 2.5 hours to cross the disk and will be difficult to see visually, but may be picked up by imaging. 

    Sunrise: 6:01 A.M.
    Sunset: 8:11 P.M.
    Moonrise: 4:09 P.M.
    Moonset: 12:25 A.M.
    Moon Phase: Waxing gibbous (70%)
    *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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  • Potatoes were spawned by tomatoes: Researchers – NewsNation

    1. Potatoes were spawned by tomatoes: Researchers  NewsNation
    2. Scientists discover that tomato is the ‘mother’ of potato  news.cgtn.com
    3. The potato’s secret past: Scientists uncover ancient botanical romance that changed the world  The Economic Times
    4. What If We Told You the Potato Was Born from a Tomato? A 9-Million-Year Mystery Finally Cracked  Times Now
    5. Study reveals potato’s secret tomato heritage  canadian affairs

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  • 100 hours for an image: ESA releases the sharpest image of the Ultra Deep Field

    100 hours for an image: ESA releases the sharpest image of the Ultra Deep Field

    ESA’s official logo (Image source: ESA; cropped)

    NASA’s James Webb Space Telescope has taken a look at the Hubble Ultra Deep Field — one of the most iconic regions of the sky. The resulting image, showing thousands of distant galaxies, can help astronomers study how galaxies formed and evolved over billions of years.

    Webb, combining data from its Near-Infrared Camera (NIRCam) with its Mid-Infrared Instrument (MIRI), revealed sharp, detailed views of the Hubble Ultra Deep Field. Originally assembled from Hubble observations from 2003 to 2004, the Ultra Deep Field showcases over 10,000 galaxies, some of which date back to less than a billion years after the Big Bang.

    Webb’s latest look at the field focuses on the MIRI Deep Imaging Survey (MIDIS) region, using MIRI’s shortest-wavelength filter. The observation lasted nearly 100 hours, marking Webb’s longest observation of an extragalactic field in one filter. In this small patch of sky observed, Webb revealed more than 2,500 sources, including hundreds of extremely red galaxies. Many are likely huge galaxies buried in cosmic dust or evolved galaxies with mature stars that formed early in the Universe’s history.

    The image assigned colors based on infrared wavelengths, revealing distinct galaxy features. Orange and red indicate longer mid-infrared wavelengths, highlighting galaxies with features such as heavy dust, abundant star formation, or active galactic nuclei (AGN). Small greenish-white galaxies appear more distant due to redshift, making their light fall into the mid-infrared ranges. Most other galaxies shine brightest in shorter near-infrared wavelengths, shown as blue and cyan, as they lack mid-infrared enhancements.

    Webb’s view of the Hubble Ultra Deep Field is one of the deepest views of the Universe ever obtained. It is providing more insights into the formation of the first cosmic structures.

    The latest and clearest image of HUDF captured by JWST (Image source: NASA, ESA, and CSA)
    The latest and clearest image of HUDF captured by JWST (Image source: NASA, ESA, and CSA)

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  • 100-hour-long exposure: ESA releases the sharpest image of the Ultra Deep Field

    100-hour-long exposure: ESA releases the sharpest image of the Ultra Deep Field

    The James Webb Space Telescope (Image source: NASA)

    NASA’s James Webb Space Telescope has taken a look at the Hubble Ultra Deep Field — one of the most iconic regions of the sky. The resulting image, showing thousands of distant galaxies, can help astronomers study how galaxies formed and evolved over billions of years.

    Webb, combining data from its Near-Infrared Camera (NIRCam) with its Mid-Infrared Instrument (MIRI), revealed sharp, detailed views of the Hubble Ultra Deep Field. Originally assembled from Hubble observations from 2003 to 2004, the Ultra Deep Field showcases over 10,000 galaxies, some of which date back to less than a billion years after the Big Bang.

    Webb’s latest look at the field focuses on the MIRI Deep Imaging Survey (MIDIS) region, using MIRI’s shortest-wavelength filter. The observation lasted nearly 100 hours, marking Webb’s longest observation of an extragalactic field in one filter. In this small patch of sky observed, Webb revealed more than 2,500 sources, including hundreds of extremely red galaxies. Many are likely huge galaxies buried in cosmic dust or evolved galaxies with mature stars that formed early in the Universe’s history.

    The image assigned colors based on infrared wavelengths, revealing distinct galaxy features. Orange and red indicate longer mid-infrared wavelengths, highlighting galaxies with features such as heavy dust, abundant star formation, or active galactic nuclei (AGN). Small greenish-white galaxies appear more distant due to redshift, making their light fall into the mid-infrared ranges. Most other galaxies shine brightest in shorter near-infrared wavelengths, shown as blue and cyan, as they lack mid-infrared enhancements.

    Webb’s view of the Hubble Ultra Deep Field is one of the deepest views of the Universe ever obtained. It is providing more insights into the formation of the first cosmic structures.

    The latest and clearest image of HUDF captured by JWST (Image source: NASA, ESA, and CSA)
    The latest and clearest image of HUDF captured by JWST (Image source: NASA, ESA, and CSA)

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  • Overnight News Digest: Science Saturday, 8/2/25

    Overnight News Digest: Science Saturday, 8/2/25

    Welcome to the Overnight News Digest with a crew consisting of founder Magnifico, regular editors side pocket, maggiejean, Chitown Kev, eeff, Magnifico, annetteboardman, Besame, jck, and JeremyBloom. Alumni editors include (but not limited to) Interceptor 7, Man Oh Man (RIP), wader, Neon Vincent, palantir, Patriot Daily News Clearinghouse (RIP), ek hornbeck (RIP), rfall, ScottyUrb, Doctor RJ, BentLiberal, Oke (RIP) and jlms qkw.

    OND is a regular community feature on Daily Kos, consisting of news stories from around the world, sometimes coupled with a daily theme, original research or commentary. Editors of OND impart their own presentation styles and content choices, typically publishing each day near 12:00 AM Eastern Time.  

    Please feel free to share your articles and stories in the comments.

    I don’t know how many of these science editions we’ve got left. The shutdown of science funding by the federal government will have an effect on the amount of science news.

    Distorted Sound of the Early Universe Suggests We Are Living In a Giant Void

    A new study analyzing distorted sound waves from the early universe suggests we may live in a massive cosmic void “with roughly 20% lower than the average density of matter,” writes Indranil Banik in an article for The Conversation. “Not every physicist is convinced that this is the case. But our recent paper analyzing distorted sounds from the early universe, published in the Monthly Notices of the Royal Astronomical Society, strongly backs up the idea.” Slashdot reader alternative_right shares an excerpt from the report:

    My colleagues and I previously argued that the Hubble tension might be due to our location within a large void. That’s because the sparse amount of matter in the void would be gravitationally attracted to the more dense matter outside it, continuously flowing out of the void. In previous research, we showed that this flow would make it look like the local universe is expanding about 10% faster than expected. That would solve the Hubble tension. But we wanted more evidence. And we know a local void would slightly distort the relation between the BAO angular scale and the redshift due to the faster moving matter in the void and its gravitational effect on light from outside.

    So in our new paper, Vasileios Kalaitzidis and I set out to test the predictions of the void model using BAO measurements collected over the last 20 years. We compared our results to models without a void under the same background expansion history. In the void model, the BAO ruler should look larger on the sky at any given redshift. And this excess should become even larger at low redshift (close distance), in line with the Hubble tension. The observations confirm this prediction. Our results suggest that a universe with a local void is about one hundred million times more likely than a cosmos without one, when using BAO measurements and assuming the universe expanded according to the standard model of cosmology informed by the CMB.

    Our research shows that the ACDM model without any local void is in “3.8 sigma tension” with the BAO observations. This means the likelihood of a universe without a void fitting these data is equivalent to a fair coin landing heads 13 times in a row. By contrast, the chance of the BAO data looking the way they do in void models is equivalent to a fair coin landing heads just twice in a row. In short, these models fit the data quite well. In the future, it will be crucial to obtain more accurate BAO measurements at low redshift, where the BAO standard ruler looks larger on the sky — even more so if we are in a void. The average expansion rate so far follows directly from the age of the universe, which we can estimate from the ages of old stars in the Milky Way. A local void would not affect the age of the universe, but some proposals do affect it. These and other probes will shed more light on the Hubble crisis in cosmology.

    Your sleep schedule could be making you sick, says massive new study

    A global study of over 88,000 adults reveals that poor sleep habits—like going to bed inconsistently or having disrupted circadian rhythms—are tied to dramatically higher risks for dozens of diseases, including liver cirrhosis and gangrene. Contrary to common belief, sleeping more than 9 hours wasn’t found to be harmful when measured objectively, exposing flaws in previous research. Scientists now say it’s time to redefine “good sleep” to include regularity, not just duration, as biological mechanisms like inflammation may underlie these powerful sleep-disease links.

    Forget the Big Bang: Gravitational waves may have really created the Universe

    A team of scientists has proposed a groundbreaking new theory on the Universe’s origins, offering a fresh, radical take on the Big Bang’s early moments. Unlike the widely accepted inflationary model, which involves speculative assumptions, the new model starts with the established concept of De Sitter space, aligning with dark energy observations. The scientists believe gravitational waves—ripples in space-time—were the key to seeding the formation of galaxies and cosmic structure, eliminating the need for unknown elements.

    x

    Let me try to explain why it’s important to study the foundations of quantum mechanics. (1/n)

    (Have to do some breathing exercises, b/c to me it’s blindingly obvious that “understanding the most important theory in physics” is something physicists should care about, but apparently opinions differ.)

    — Sean Carroll (@seanmcarroll.bsky.social) 2025-07-30T16:35:19.343Z

    The real-life Kryptonite found in Serbia—and why it could power the future

    Deep in Serbia’s Jadar Valley, scientists discovered a mineral with an uncanny resemblance to Superman’s Kryptonite both in composition and name. Dubbed jadarite, this dull white crystal lacks the glowing green menace of its comic book counterpart but packs a punch in the real world. Rich in lithium and boron, jadarite could help supercharge the global transition to green energy.

    Deep-sea fish just changed what we know about Earth’s carbon cycle

    Mesopelagic fish, long overlooked in ocean chemistry, are now proven to excrete carbonate minerals much like their shallow-water counterparts—despite living in dark, high-pressure depths. Using the deep-dwelling blackbelly rosefish, researchers have demonstrated that carbonate production is consistent across ocean layers, bolstering global carbon cycle models. These findings reveal that these abundant fish play a hidden but crucial role in regulating Earth’s ocean chemistry and could reshape how we understand deep-sea contributions to climate processes.

    Drones reveal 41,000-turtle nesting mega-site hidden in the Amazon

    A team at the University of Florida used drones and smart modeling to accurately count over 41,000 endangered turtles nesting along the Amazon’s Guaporé River—revealing the world’s largest known turtle nesting site. Their innovative technique, combining aerial imagery with statistical correction for turtle movement, exposes major flaws in traditional counting methods and opens doors to more precise wildlife monitoring worldwide.

    Reversing Alzheimer’s damage: Two cancer drugs demonstrate surprising power

    In an exciting breakthrough, researchers have identified cancer drugs that might reverse the effects of Alzheimer’s disease in the brain. By analyzing gene expression in brain cells, they discovered that some FDA-approved cancer medications could reverse damage caused by Alzheimer’s.

    x

    On X, Masaki Nobushiro posts a recurring (and useful) drawing about how people wrongly think a 1m tsunami is a cresting wave when it’s actually a wall of water filled with dangerous and deadly debris that’s strong enough to sweep up a car.

    #tsunami

    — Unseen Japan (@unseenjapan.com) 2025-07-30T03:29:10.313Z

    Why cold feels good: Scientists uncover the chill pathway

    A newly mapped neural circuit shows how our skin senses cool temperatures and sends that info to the brain, revealing an unexpected amplifier in the spinal cord and offering insight into cold-related pain.

    The 0.05% RNA Process That Makes Cancer Self-Destruct

    A group of Australian scientists has uncovered a new way to fight some of the toughest cancers by targeting an overlooked cellular process called minor splicing. This tiny but vital mechanism turns out to be essential for the growth of certain tumors, especially those driven by KRAS mutations — a common but hard-to-treat culprit in cancer. By blocking minor splicing, researchers triggered DNA damage and activated the body’s own cancer-defense system, killing cancer cells while sparing healthy ones. The results in animal and human cell models are so promising that drug development is now underway, potentially paving the way for more effective and less toxic treatments across multiple cancer types.

    The pandemic’s secret aftershock: Inside the gut-brain breakdown

    A new global study reveals a striking post-pandemic surge in gut-brain disorders like IBS and functional dyspepsia. Researchers compared data from 2017 and 2023 and discovered sharp increases—IBS up 28% and dyspepsia nearly 44%. Those suffering from long COVID were especially vulnerable, reporting more anxiety, depression, and worse quality of life. These findings spotlight the urgent need for deeper investigation into the gut-brain axis and revised care models in a post-COVID world.

    Peacock Feathers Can Be Lasers

    Peacocks have a secret hidden in their brightly colored tail feathers: tiny reflective structures that can amplify light into a laser beam. After dyeing the feathers and energizing them with an external light source, researchers discovered they emitted narrow beams of yellow-green laser light. They say the study, published this month in Scientific Reports, offers the first example of a laser cavity in the animal kingdom. […]

    Scientists have long known that peacock feathers also exhibit “structural color” — nature’s pigment-free way to create dazzling hues. Ordered microstructures within the feathers reflect light at specific frequencies, leading to their vivid blues and greens and iridescence. But Florida Polytechnic University physicist Nathan Dawson and his colleagues wanted to go a step further and see whether those microstructures could also function as a laser cavity. After staining the feathers with a common dye and pumping them with soft pulses of light, they used laboratory instruments to detect beams of yellow-green laser light that were too faint to see with the naked eye. They emerged from the feathers’ eyespots, at two distinct wavelengths. Surprisingly, differently colored parts of the eyespots emitted the same wavelengths of laser light, even though each region would presumably vary in its microstructure.

    Just because peacock feathers emit laser light doesn’t mean the birds are somehow using this emission. But there are still ramifications, Dawson says. He suggests that looking for laser light in biomaterials could help identify arrays of regular microstructures within them. In medicine, for example, certain foreign objects — viruses with distinct geometric shapes, perhaps — could be classified and identified based on their ability to be lasers, he says. The work also demonstrates how biological materials could one day yield lasers that could be put safely into the human body to emit light for biosensing, medical imaging, and therapeutics. “I always like to think that for many technological achievements that benefit humans,” Dawson says, “some organism somewhere has already developed it through some evolutionary process.”

    Early Universe’s ‘Little Red Dots’ May Be Black Hole Stars

    After it began “peering into the distant universe” in 2022, NASA’s James Webb Space Telescope “has discovered a rash of ‘little red dots’,” reports Science magazine.  There’s “hundreds of them, shining within the first billion years of the 13.8-billion-year-old universe, so small and red that they defied conventional explanation.”

    “Only in the past few months has a picture begun to emerge. The little red dots, astronomers say, may be an entirely new type of object: a colossal ball of bright, hot gas, larger than the Solar System, powered not by nuclear fusion, but by a black hole…”The objects, which some astronomers are calling “black hole stars,” could be a missing link in the evolution of galaxies and help explain the rapid growth of supermassive black holes that lie at their hearts. “The big breakthrough of the past 6 months is actually the realization that we can throw out all these other models we’ve been playing with before,” says astronomer Anna de Graaff of the Max Planck Institute for Astronomy… JWST couldn’t resolve the dots into a recognizable shape, which meant they must have been tiny — less than 2% of the diameter of the Milky Way. “It was a mystery … as to why they were so spatially compact,” says Caitlin Casey of the University of Texas at Austin. An impossibly dense packing of stars would be needed to explain their brightness. “I was excited,” Casey says…

    For Mitch Begelman, a theoretical astrophysicist at the University of Colorado Boulder, the observations are a vindication. Earlier this month, he and a colleague posted a preprint on arXiv reviving a scenario for the formation of hypothetical “quasi-stars” that he and others had proposed 20 years ago.  The first generation of stars, they calculated, could have grown to colossal size in the early universe, which was made up almost entirely of hydrogen, the raw material of stars. When a giant star ran out of fuel, they said, its core would have collapsed into a black hole, but the outer envelope of hydrogen was so dense it survived the blast, enclosing the newborn black hole. As the black hole chewed at its shroud of gas, the entire system glowed as a quasi-star larger than the Solar System. “That’s what the quasi-star envelope is doing, it’s force-feeding the black hole by pushing matter into it,” Begelman says.

    Given how common little red dots appear to be in the early universe, theorists are beginning to wonder whether this giant-ball-of-gas phase is an essential part of black hole growth and the evolution of galaxies. “We’re probably looking at kind of a new phase of black hole growth that we didn’t know about before,” de Graaff says.
    “If the red dots do turn out to be black hole stars, it will be precisely the sort of breakthrough expected from JWST — and the kind of discovery astronomers live for.”

    Researchers Map Where Solar Energy Delivers the Biggest Climate Payoff

    A Rutgers-led study using advanced computational modeling reveals that expanding solar power by just 15% could reduce U.S. carbon emissions by over 8.5 million metric tons annually, with the greatest benefits concentrated in specific regions like California, Texas, and the Southwest. The study has been published in Science Advances. From the report:

    The study quantified both immediate and delayed emissions reductions resulting from added solar generation. For example, the researchers found that in California, a 15% increase in solar power at noon was associated with a reduction of 147.18 metric tons of CO2 in the region in the first hour and 16.08 metric tons eight hours later.

    The researchers said their methods provide a more nuanced understanding of system-level impacts from solar expansion than previous studies, pinpointing where the benefits of increased solar energy adoption could best be realized. In some areas, such as California, Florida, the mid-Atlantic, the Midwest, Texas and the Southwest, small increases in solar were estimated to deliver large CO2 reductions, while in others, such as New England, the central U.S., and Tennessee, impacts were found to be minimal — even at much larger increases in solar generation.

    In addition, the researchers said their study demonstrates the significant spillover effects solar adoption has on neighboring regions, highlighting the value of coordinated clean energy efforts. For example, a 15% increase in solar capacity in California was associated with a reduction of 913 and 1,942 metric tons of CO2 emissions per day in the northwest and southwest regions, respectively. “It was rewarding to see how advanced computational modeling can uncover not just the immediate, but also the delayed and far-reaching spillover effects of solar energy adoption,” said the lead author Arpita Biswas, an assistant professor with the Department of Computer Science at the Rutgers School of Arts and Sciences. “From a computer science perspective, this study demonstrates the power of harnessing large-scale, high-resolution energy data to generate actionable insights. For policymakers and investors, it offers a roadmap for targeting solar investments where emissions reductions are most impactful and where solar energy infrastructure can yield the highest returns.”

    The hidden climate battle between forests and the ocean

    Between 2003 and 2021, Earth saw a net boost in photosynthesis, mainly thanks to land plants thriving in warming, wetter conditions—especially in temperate and high-latitude regions. Meanwhile, ocean algae struggled in increasingly stratified and nutrient-poor tropical waters. Scientists tracked this global energy shift using satellite data, revealing that land ecosystems not only added more biomass but also helped stabilize climate by capturing more carbon.

    Einstein was wrong: MIT just settled a 100-year quantum debate

    MIT physicists have performed an idealized version of one of the most famous experiments in quantum physics. Their findings demonstrate, with atomic-level precision, the dual yet evasive nature of light. They also happen to confirm that Albert Einstein was wrong about this particular quantum scenario.

    The experiment in question is the double-slit experiment, which was first performed in 1801 by the British scholar Thomas Young to show how light behaves as a wave. Today, with the formulation of quantum mechanics, the double-slit experiment is now known for its surprisingly simple demonstration of a head-scratching reality: that light exists as both a particle and a wave. Stranger still, this duality cannot be simultaneously observed. Seeing light in the form of particles instantly obscures its wave-like nature, and vice versa.

    The original experiment involved shining a beam of light through two parallel slits in a screen and observing the pattern that formed on a second, faraway screen. One might expect to see two overlapping spots of light, which would imply that light exists as particles, a.k.a. photons, like paintballs that follow a direct path. But instead, the light produces alternating bright and dark stripes on the screen, in an interference pattern similar to what happens when two ripples in a pond meet. This suggests light behaves as a wave. Even weirder, when one tries to measure which slit the light is traveling through, the light suddenly behaves as particles and the interference pattern disappears.

    What happens when light smashes into itself? Scientists just found out

    Physicists have discovered that when beams of light interact at the quantum level, they can generate ghost-like particles that briefly emerge from nothing and affect real matter. This rare phenomenon, known as light-on-light scattering, challenges the classical idea that light waves pass through each other untouched.

    This spectrometer is smaller than a pixel, and it sees what we can’t

    Researchers have successfully demonstrated a spectrometer that is orders of magnitude smaller than current technologies and can accurately measure wavelengths of light from ultraviolet to the near-infrared. The technology makes it possible to create hand-held spectroscopy devices and holds promise for the development of devices that incorporate an array of the new sensors to serve as next-generation imaging spectrometers.

    “Spectrometers are critical tools for helping us understand the chemical and physical properties of various materials based on how light changes when it interacts with those materials,” says Brendan O’Connor, corresponding author of a paper on the work and a professor of mechanical and aerospace engineering at North Carolina State University. “They are used in applications that range from manufacturing to biomedical diagnostics. However, the smallest spectrometers on the market are still fairly bulky.

    Hidden gene in leukemia virus could revolutionize HIV treatment

    Scientists in Japan have discovered a genetic “silencer” within the HTLV-1 virus that helps it stay hidden in the body, evading the immune system for decades. This silencer element essentially turns the virus off, preventing it from triggering symptoms in most carriers. Incredibly, when this silencer was added to HIV, it made that virus less active too — hinting at a revolutionary new strategy for managing not just HTLV-1 but other deadly retroviruses as well. The discovery opens the door to turning the virus’s own stealth tactics against it in future treatments.

    Scientists just solved the 9-million-year mystery of where potatoes came from

    About 9 million years ago, a wild interspecies fling between tomato-like plants and potato relatives in South America gave rise to one of the world’s most important crops: the potato. Scientists have now traced its roots to a rare natural hybridization that created the tuber, a storage organ that allowed the plant to survive harsh Andean environments and spread rapidly.

    700,000 years ahead of their teeth: The carbs that made us human

    Long before evolution equipped them with the right teeth, early humans began eating tough grasses and starchy underground plants—foods rich in energy but hard to chew. A new study reveals that this bold dietary shift happened 700,000 years before the ideal dental traits evolved to handle it.

    Did drunk apes help us evolve? New clues reveal why we digest alcohol so well

    Ape behavior just got a name upgrade — “scrumping” — and it might help explain why humans can handle alcohol so well. Researchers discovered that African apes regularly eat overripe, fermented fruit off the forest floor, and this habit may have driven key evolutionary adaptations. By naming and classifying this behavior, scientists are hoping to better understand how alcohol tolerance evolved in our ancestors — and how it might have helped shape everything from safety in the trees to social drinking rituals.

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    If you want a weird but true fact to talk about:

    Dexter Holland, lead singer of The Offspring, was instrumental in this. His doctorial thesis in molecular biology was sequencing mRNA in HIV. The paper was also heavily cited in creating the COVID-19 vaccine.

    — Darryl Mott (@gamerstavernshow.com) 2025-08-01T13:53:42.445Z

    From the quoted post:

    It feels like we should be making a bigger deal of “we actually did in fact find a cure for AIDS”

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  • Moon phase today explained: What the moon will look like on August 3, 2025

    Moon phase today explained: What the moon will look like on August 3, 2025

    The moon is looking brighter every night, and we’re inching closer to the next full moon. But let’s take a look at where we are in the lunar cycle first.

    The lunar cycle is a series of eight unique phases of the moon’s visibility. The whole cycle takes about 29.5 days, according to NASA, and these different phases happen as the Sun lights up different parts of the moon whilst it orbits Earth. 

    What is today’s moon phase?

    As of Sunday, Aug. 3, the moon phase is Waxing Gibbous. According to NASA’s Daily Moon Observation, the moon will be 69% lit up tonight.

    It’s day 10 of the lunar cycle, and there’s a lot to see when we look up tonight. With just your naked eye (no visual aids required), you’ll be able to spot the Copernicus Crater, the Mare Fecunditatis, and the Mare Crisium.

    With binoculars, enjoy a glimpse of the Aphonsus Crater, Posidonius Crater, and the Mare Frigoris. With a telescope, you can also see the Rima Arladaeus, the Descartes Highlands, and Fra Mauro Highlands, a hilly region of the moon where the Apollo 14 landed.

    When is the next full moon?

    The next full moon will be on August 9. The last full moon was on July 10.

    What are moon phases?

    According to NASA, moon phases are caused by the 29.5-day cycle of the moon’s orbit, which changes the angles between the Sun, Moon, and Earth. Moon phases are how the moon looks from Earth as it goes around us. We always see the same side of the moon, but how much of it is lit up by the Sun changes depending on where it is in its orbit. This is how we get full moons, half moons, and moons that appear completely invisible. There are eight main moon phases, and they follow a repeating cycle:

    Mashable Light Speed

    New Moon – The moon is between Earth and the sun, so the side we see is dark (in other words, it’s invisible to the eye).

    Waxing Crescent – A small sliver of light appears on the right side (Northern Hemisphere).

    First Quarter – Half of the moon is lit on the right side. It looks like a half-moon.

    Waxing Gibbous – More than half is lit up, but it’s not quite full yet.

    Full Moon – The whole face of the moon is illuminated and fully visible.

    Waning Gibbous – The moon starts losing light on the right side.

    Last Quarter (or Third Quarter) – Another half-moon, but now the left side is lit.

    Waning Crescent – A thin sliver of light remains on the left side before going dark again.

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  • Solving a 13-Billion-Year-Old Mystery: Scientists Recreate the Universe’s First Chemical Reaction – SciTechDaily

    1. Solving a 13-Billion-Year-Old Mystery: Scientists Recreate the Universe’s First Chemical Reaction  SciTechDaily
    2. After the Big Bang: How the first stars lit up our universe  The Indian Express
    3. Chemistry at the beginning: How molecular reactions influenced the formation of the first stars  Phys.org
    4. New Insights into the Formation of Molecular Hydrogen in the Early Universe  AZoQuantum

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