Category: 7. Science

  • Do we all see the same thing? We looked at 100 years of research on perception and found something surprising.

    Do we all see the same thing? We looked at 100 years of research on perception and found something surprising.

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    It’s one of the deepest mysteries of the human mind: Do we all see the world the same way? In 1956, three social scientists set out to answer this question. From their offices at Northwestern University, Donald Campbell and Melville Herskovits teamed up with Marshall Segall, of Syracuse University, to coordinate an ambitious new investigation. They sent researchers on a mission to societies near and far, urban and rural: A gold mine in Johannesburg; a community of foragers in the Kalahari Desert; the Philippine island of Mindoro; and even their own college campus in Evanston, Illinois.

    Tucked into each of their suitcases was a booklet of drawings, including 12 examples of a prominent figure called the Müller-Lyer illusion. You may have seen it before: When two identical horizontal lines are capped with arrowheads pointing either inward or outward, the line with inward-facing arrowheads looks longer, even though it’s not.

    Courtesy of Dorsa Amir and Chaz Firestone

    At least, that’s how the illusion works here in the United States. But what about elsewhere? When the study was completed in 1961, the results shocked the scientific community: Not everyone was susceptible to this seemingly obvious illusion. While students in Illinois tended to report the top line as longer, Zulu pastoralists in South Africa had a much weaker response, barely experiencing the illusory effects. And the San foragers of the Kalahari seemed not to see anything remarkable at all, just two lines of equal length, as if the illusion simply wasn’t an illusion for them. This wasn’t like finding different shapes in a complicated abstract drawing, or even having different interpretations of a novel. It was as though something about human vision was fundamentally different from culture to culture. How was this possible?

    Before we unravel the mystery, let’s first explain why this matters to psychology researchers like us. Psychology aims to capture enduring truths about the human mind. But in the vast majority of cases, psychological studies explore narrow subject pools, such as college students taking introductory courses. The reason is mostly convenience; such test subjects are available in large numbers on college campuses (where most researchers are), and they are happy to give a little bit of their time in exchange for a bit of compensation, such as course credit. But there is good reason to worry about doing research this way. Who is to say that attitudes toward nationalism, or the prevalence of ADHD, or the best tricks for sticking to a new diet—or really, anything else psychologists study—generalize from one very specific group to the whole of humanity? Psychology has been around for a while, but it wasn’t until relatively recently that the field began to reckon with these concerns more seriously and systematically, under the banner of a clever acronym proclaiming most psychology research subjects are “WEIRD”: Western, Educated, Industrialized, Rich, and Democratic. The idea has gained steam over the past 15 years, and researchers are trying to do better.

    But which psychological principles should we expect to vary across groups? Which findings are cultural creations limited to WEIRD research subjects, and which reflect our common humanity—true for us and everyone else? Here’s where the illusion study becomes so consequential. It’s one thing to suppose that political attitudes or dietary practices differ around the world; any tourist can attest to this. But perception itself? Could it really be that our very eyes tell us something different about the world depending on where we grew up?

    Segall and colleagues thought so, and even went a step further. They proposed that Americans see the illusion only because of their overexposure to carpentry—straight lines and sharp angles that are present in urban environments and the Müller-Lyer figure, but are less prevalent in the Kalahari. Raise someone in an environment without boxy structures or rectangular windows and doors, the idea goes, and the illusion won’t exist for them. Contemporary anthropologists have further popularized this view, arguing that “the Müller-Lyer illusion is a kind of culturally evolved by-product.” Call it the Cultural Byproduct Hypothesis.

    This result and the theoretical apparatus built around it are now essentially part of the psychological canon. They are often taught to Psych 101 students as both a fascinating discovery about visual processing and a cautionary tale about unwarranted assumptions of universality. We shouldn’t assume that others experience the world like we do—that much seems true and even uncontroversial. And what better piece of evidence for this lesson than discovering that we literally see the world differently depending on where we grow up.

    We weren’t so sure about all this. In a new paper, we revisited over 100 years of research on perception and came to nearly the opposite conclusion: This particular visual illusion, and many other aspects of our perceptual system, arise from deep within us, are likely common to humans across the globe, and certainly aren’t mere cultural creations. As impressive as the cross-cultural studies seem (more on that in a moment), there are powerful clues suggesting that the Cultural Byproduct Hypothesis can’t really be true.

    Why not? For one thing, lots of other animals see the Müller-Lyer illusion. If you train a guppy to swim toward longer lines (yes, a real thing that can be done!), and then you show it the Müller-Lyer figure, it will swim towards the top line—suggesting that the guppy sees that line as longer. This is true for a veritable zoo of nonhuman creatures, including horses, parakeets, monkeys, and lizards, who all see the illusion as well. Did the guppies’ culture create the illusion for them too? Seems unlikely.

    Another clue: The illusion doesn’t even need to be made of straight lines in order to work. There are versions of the Müller-Lyer illusion composed entirely out of curves, or just groups of dots; there’s even a version that uses people’s faces. That observation calls into question the purported link with carpentry, since the whole idea was that the illusion relies on features such as straight lines present in precisely constructed environments.

    Straight lines of equal length but with half circles on the ends and cartoon faces facing out and facing in, with marks to show spacing.
    Courtesy of Dorsa Amir and Chaz Firestone

    Perhaps the strongest clue of all is also the most remarkable. A humanitarian and scientific project called Prakash recently offered free corrective surgery to children in North India who were born with congenital cataracts—cloudy lenses that prevent light from entering the eyes, blinding them since birth. With new, clear, artificial lenses, these children were now able to see for the first time in their lives. Astoundingly, when shown the Müller-Lyer illusion—mere hours after recovering from their operations—they reported the top line as longer than the bottom line. Not only had these children never seen carpentry, they had never seen anything.
    And yet they still experienced the illusory effects of the figure.

    All this and more suggests that the illusion really is a result of who we are, not the buildings we happen to grow up next to. Despite our differences, we really do see the world similarly, sharing something in common with humans across the globe and throughout history.

    But wait: If the evidence against the Cultural Byproduct Hypothesis is so overwhelming, then why did those three social scientists find different results in their cross-cultural study, with some groups seeming not to see the illusion at all?

    First, the cross-cultural studies were never all that consistent with one another. When we looked even deeper into the published record, it was surprisingly easy to find contradictory results: A study from the early 20th century found that a jungle-dwelling population in India showed a stronger illusion than a pastoralist community in the same country, and another study from 1970 similarly found stronger effects in a rural population indigenous to South Africa than in a nearby urban community. Even Segall, Campbell, and Herskovits’ more famous study contained contradictions within itself. For example, one of the samples showing the weakest illusion of all was a group of mineworkers. Mines, of course, are highly constructed, carpentered environments—exactly the kind of environment that should produce a large illusion, according to the theory.

    Second, studies of this sort are open to bias. For starters, you have to translate the task instructions into a local dialect, which is not always easy; many of these researchers even worried about this difficulty, writing that they “were not completely sure of exactly what was communicated to the respondents at all times.” There are also biases introduced by experimenters who know something about the research hypotheses and might—consciously or not—tilt the results accordingly. In another telling passage, one experimenter wrote that he “developed very strong expectations of what answer the respondents should give to a given item, and if a respondent gave the other answer, there was the impulse to correct the respondent to ask him to reconsider.” There is even evidence that some of the cross-cultural data were excluded if the reported illusion was too strong, and that this masked some findings that would have challenged the overall narrative. It may well be, then, that the illusion was present in these diverse populations, and the experimenters simply failed to fully capture it in their measurements.

    What does that mean for us today? Expanding psychological research to capture the diversity of human experience is a tide that lifts all boats, and is a project we wholeheartedly support (and engage in ourselves). But some experiences may well be universal.


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  • What a caterpillar’s quiet pose tells us about the biology of pain

    What a caterpillar’s quiet pose tells us about the biology of pain

    When most animals are hurt, they lash out or run away. It’s the classic fight-or-flight response. However, the tobacco hornworm caterpillar (Manduca sexta) has a very different strategy.

    When disturbed or in pain, it goes still, curling its head and upper body downward in a pose that researchers call the sphinx state, since it looks like the ancient Egyptian statue.

    Scientists have now discovered that this isn’t just a freeze response. The caterpillar is actually processing pain in this state, a finding that challenges what we thought we knew about how simple brains handle pain.

    “Our study is the first to characterize it as a behavioural state with associated physiological modulations. We show that this is a reversible, quiescent state that caterpillars assume when they experience mechanical disturbance in their surroundings,” the study authors note.

    This unusual caterpillar behavior reveals new insights about how animals process pain and could even help scientists rethink pest control and human pain relief.

    Decoding the pain processing mechanism

    Scientists at Tufts University wanted to know how tobacco hornworm caterpillars react when they feel pain or discomfort. Normally, animals respond through a reflex called nociception, an automatic response to painful stimuli. 

    For example, if you touch something hot, you pull your hand back before your brain even registers the pain. Researchers thought insects would behave the same way, and they performed a series of experiments with 20 tobacco hornworm caterpillars. However, the caterpillars surprised them.

    They gently stroked the caterpillars with a paintbrush, tapped on the surface where they were resting, and even moved the material under them. Each time, the caterpillars tucked their head and thorax downward and froze in the sphinx position. 

    The researchers then checked how this posture affected pain responses. When they applied heat to different parts of the caterpillars’ bodies, the insects showed less sensitivity than they normally would. To dig deeper, the scientists wanted to know whether the sphinx state was just a reflex or a conscious choice. 

    They performed surgery on the insects’ cerebral ganglion, a brain structure that controls movement and processes sensory information. Their experiments revealed that this part of the brain could not trigger the sphinx state on its own. 

    Instead, the behavior seemed to be actively chosen by the caterpillars, showing that they were not just passively reacting to pain but deliberately dampening their response. 

    “When they were separated from external mechanosensory stimuli for 24 hours, none of the 20 larvae entered the sphinx state. Instead, they were only observed engaging in crawling, feeding, and defecating. This suggests that the sphinx state is an ‘evoked’ response that is initiated on sensing an external stimulus,” the study authors said.

    “This discovery reveals a novel instance of active behavioural modulation in insects and highlights the flexibility of nociceptive responses, challenging the notion of nociception as strictly hard-wired and stereotyped,” they added.

    Why does the knowledge of such behavior matter?

    The humble caterpillar has taught science a big lesson. Pain isn’t always about fight or flight; sometimes, it’s about staying still and choosing silence.

    These findings could have various implications. For example, in the case of pest management, understanding how insects actively control their defensive behaviors could lead to smarter and safer ways to manage crop pests without relying solely on harmful pesticides. 

    The research also offers a window into the biology of pain. While the human brain is far more complex, studying a simple nervous system like that of the caterpillar allows researchers to pinpoint how decisions about pain suppression are made. 

    This could lead to novel ideas for developing new kinds of pain relief in humans, especially for conditions where the nervous system amplifies pain signals unnecessarily. The Tufts team now plans to explore how widespread this behavior is in the insect world and to trace the exact neural circuits responsible. 

    The study is published in the journal Biology Letters.

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  • Can black holes detonate stars? Rare supernova holds the clues

    Can black holes detonate stars? Rare supernova holds the clues

    Astronomers recorded a star merging with a black hole as it burst into a supernova. Thanks to AI-assisted technology, it was possible to study this extraordinary event as it unfolded.

    In July 2023, the Zwicky Transient Facility (ZTF) flagged an unusual cosmic flash while scanning the skies for anomalies. The explosion is now known as SN 2023zkd. 


    Further observations of its characteristics confirmed that this was no ordinary supernova.

    The discovery was made by a collaborative group conducting a survey known as the Young Supernova Experiment (YSE). The team consists of scientists from the Center for Astrophysics at Harvard & Smithsonian and MIT.

    A rarity in supernova history

    The supernova SN 2023zkd was likely the result of a heavyweight star locked in a tight orbit with a lurking black hole companion.

    Over time, the black hole’s gravity pulled out material, like gas and dust, from the star. This reduced the star’s angular momentum, bringing the star ever closer to the black hole.

    In close proximity to the black hole, the star was subjected to extreme gravitational stress. Over time, it partially merged with its companion in what astronomers call an instability-induced merger – a process that can prematurely trigger a star’s explosion.

    Study lead author Alexander Gagliano is a researcher at the NSF Institute for Artificial Intelligence and Fundamental Interactions.

    “This discovery shows how important it is to study how massive stars interact with companions as they approach the end of their lives,” Gagliano said in a news release.

    AI-detected star-black hole merger

    AI tools are trained on thousands of light curves – graphs that show how a star’s brightness changes over time – to detect subtle signs of an outburst. One of these tools is the Lightcurve Anomaly Identification and Similarity Search (LAISS).

    As the scientists were tracking SN 2023zkd’s decline, LAISS detected unusual color changes. Surprisingly, it eventually displayed two additional peaks of brightness following its detection. 

    The first peak came when the explosion’s shockwave hit the thin gas the star had shed earlier. The second, delayed peak arose as the ejecta slammed into a denser, disk-shaped cloud of material around the equator of the star.

    “Our machine learning system flagged SN 2023zkd months before its most unusual behavior, which gave us ample time to secure the critical observations needed to unravel this extraordinary explosion,” said Gagliano.

    Single star or a binary supernova?

    At first, astronomers considered single-star explanations because some characteristics were a match. The first possible explanation was a luminous blue variable (LBV), which is a massive, unstable star known for dramatic outbursts. 

    SN 2023zkd exhibited multi-year brightening that resembled LBV behavior. But it was far too bright. Its steady, persistent brightness is not compatible with the short bursts typical of LBVs.

    Similar to the LBV theory, other single-star theories also crumbled under the weight of the evidence. 

    The binary merger theory – the idea that the star collided with a black hole – explained the presence of the equatorial disk of debris, as well as the persistent brightness. 

    Opening the secrets of the universe

    SN 2023zkd offers a preview of what’s to come as large observatories and AI work together. This study relied on data from telescopes located in various parts of the world, including the United States, Australia, and Japan. 

    “We think this might be part of a whole class of hidden explosions that AI will help us discover,” said V. Ashley Villar, an assistant professor of astronomy at Harvard University.

    Future campaigns will track AI alerts using telescopes across the spectrum. Astronomers will map stellar gas in optical, infrared, X-ray, and radio wavelengths to piece together the chain of events that cause a star to explode.

    “We’re now entering an era where we can automatically catch these rare events as they happen, not just after the fact,” noted Gagliano. “That means we can finally start connecting the dots between how a star lives and how it dies, and that’s incredibly exciting.”

    The study was published in the August issue of The Astrophysical Journal.

    Image Credit: Melissa Weiss/CfA

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  • Giant Chunks of The Seafloor Are Mysteriously Upside Down, Scientists Find : ScienceAlert

    Giant Chunks of The Seafloor Are Mysteriously Upside Down, Scientists Find : ScienceAlert

    Deep beneath the waves of the North Sea, the seafloor is behaving in an unexpected way.

    There, scientists have discovered hundreds of vast sand mounds, some on the scale of several kilometers across, that, according to a release from the University of Manchester in the UK, “defy fundamental geological principles”.

    These mounds pile atop structures known as sinkites, the result of a process called stratigraphic inversion, and never before have they been found in such large numbers.

    Related: Mysterious Holes on The Ocean Floor Have a New Explanation

    “This discovery reveals a geological process we haven’t seen before on this scale,” says geophysicist Mads Huuse of the University of Manchester.

    “What we’ve found are structures where dense sand has sunk into lighter sediments that floated to the top of the sand, effectively flipping the conventional layers we’d expect to see and creating huge mounds beneath the sea.”

    A map of the strange mounds under the North Sea. (Rudjord & Huuse, Commun. Earth Environ., 2025)

    Geological layers are expected to follow a certain order consistent with the linear progression of time. Older layers are towards the bottom of the formation, growing progressively newer closer to the top, in the order of deposition.

    Stratigraphic inversion, or reverse stratigraphy, occurs when younger layers sink down, and the older ones rise to the top of the formation, and there are a number of ways this can happen, from rockslides to tectonic movements.

    Huuse and his colleague, geophysicist Jan Erik Rudjord of oil company Aker BP in Norway, identified the sinkites at the bottom of the North Sea using detailed seismic data. When acoustic waves travel through Earth, they propagate and reflect differently from materials with different density properties. Scientists can then analyze the seismic data and map the different types of rock the waves traveled through.

    In this data, Huuse and Rudjord found that large parts of the North Sea floor appeared to be upside down, with younger layers of sand buried beneath older layers.

    These younger layers are denser and heavier than the softer, lighter material that was below, so over time, they sank down, displacing the older, more porous material and forcing it upwards, where it sits atop the denser sinkite. The researchers have dubbed the porous rafts ‘floatites’.

    They believe this process probably took place around the boundary between the Miocene and the Pliocene, about 5.3 million years ago. The older material consisted of a lightweight, rigid, and porous layer predominantly made up of microscopic marine fossils, with a heavier layer atop.

    A map of the layers under the seafloor. (Rudjord & Huuse, Commun. Earth Environ., 2025)

    Disruptions such as earthquakes could have broken up the upper layer into sand, which sank down, switching places with the floatites. Over the ensuing millions of years, seafloor sediment dusted the entire structure over, producing the undulating seafloor that can be found there today.

    Now, the team are working to improve and validate their interpretation – one that could help better understand Earth’s crust under the ocean, where it is weak and where stable, and the processes that can dramatically alter these properties.

    “This research shows how fluids and sediments can move around in the Earth’s crust in unexpected ways. Understanding how these sinkites formed could significantly change how we assess underground reservoirs, sealing, and fluid migration – all of which are vital for carbon capture and storage,” Huuse says.

    “As with many scientific discoveries there are many skeptical voices, but also many who voice their support for the new model. Time and yet more research will tell just how widely applicable the model is.”

    The research has been published in Communications Earth & Environment.

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  • A Physicist Wants to Turn Jupiter’s Largest Moon Into a Gigantic Dark Matter Detector

    A Physicist Wants to Turn Jupiter’s Largest Moon Into a Gigantic Dark Matter Detector

    When searching for the unknown, classic physics wisdom holds that a bigger detector boosts the chances of discovery. A physicist is taking that advice to heart, advancing a bold plan to use none other than Ganymede—Jupiter’s largest moon—as a dark matter detector on an astronomical scale.

    Dark matter refers to the “invisible” mass that supposedly constitutes 85% of the universe. There’s considerable evidence that dark matter exists, but it’s “dark,” meaning it doesn’t respond to light and very weakly interacts with other matter. The search for dark matter has tested the limits of physicists’ creativity, but a proposal by William DeRocco, a physicist at the University of Maryland, may be the most extraordinary yet. In a preprint submitted to arXiv, Rocco suggests that Ganymede’s craters may store evidence of dark matter particles, which spacecraft like NASA’s Europa Clipper or ESA’s JUICE could observe during their respective missions.

    The paper, which has yet to be peer-reviewed, proposes that massive dark matter particles could have struck and penetrated Ganymede’s thick, icy surface, leaving deep, broad ruptures. Unlike the comparatively small-sized candidates for dark matter that ground-based detectors are searching for, these particles would be much larger. These extra-large dark matter particles would create “dark matter craters”—smaller dents on Ganymede’s surface comprised of distinctive minerals pulled to the surface from deep inside the moon’s oceans. 

    “If you used something like ground-penetrating radar, you might be able to see this column of melted ice going all the way down through the ice,” DeRocco explained in an interview with New Scientist. Studying Ganymede’s surface with this proposal in mind could uncover some unexpected insights about cosmic dark matter, according to the paper.

    In principle, the proposal sounds promising, Bradley Kavanaugh, an astrophysicist at the University of Cantabria in Spain who was not involved in the study, also told New Scientist. At the same time—like all dark matter experiments—there is still no definitive evidence that such heavy, massive dark matter particles actually exist.

    If all of this sounds bonkers, I don’t blame you. Still, it’s important to remember that, as many physicists are keen to point out, solving a physics mystery often means testing bold, unconventional ideas. And while there’s no decisive evidence that this particular proposal is correct, there isn’t any evidence to discount it, either. We’ll have to wait and see if NASA or ESA takes up DeRocco’s idea, and if they do, whether Ganymede really does have a surface dotted with dark matter craters.

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  • SpaceX launches 50th Dragon spacecraft to ISS on resupply mission for NASA

    SpaceX launches 50th Dragon spacecraft to ISS on resupply mission for NASA

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    SpaceX on Sunday launched a Commercial Resupply Services (CRS-33) mission to the International Space Station from Cape Canaveral in Florida, the Dragon spacecraft’s 50th time.

    Following stage separation, the first stage landed on the A Shortfall of Gravitas droneship, stationed in the Atlantic Ocean.

    According to SpaceX officials, the Dragon spacecraft is expected to dock with the ISS on Monday autonomously after an approximate 28-hour flight.

    The CRS-33 will then deliver 5,000 lbs (2268 kg) of food, supplies, and experiments to astronauts onboard the International Space Station—but according to SpaceX officials, this mission goes beyond being just a resupply mission.

    Some 50 different scientific studies critical for future human space exploration are to be conducted on the mission.

    “This research team is testing out the hypothesis that blocking a certain protein in the body that is known to promote bone loss or bone health changes may actually help reduce the overall bone loss that astronauts experience in space,” said Heidi Parris, associate program scientist for the ISS Program.

    While Sunday’s launch marked half a ton of SpaceX Dragon spacecraft visits to the space station; the first time was in May 2012 for a resupply demonstration.

    It was also the first-stage booster’s seventh flight and the third for the Dragon spacecraft as part of the resupply mission.

    In September, the Dragon spacecraft will be utilised to give the space station a boost. This will involve the adjustment of the space station’s altitude, according to Bill Spetch, the International Space Station Program’s Operations Integration Manager.

    “NASA contracted with SpaceX a few years ago to provide a reboost capability to the space station. As you know, the space station’s altitude slowly decays over time due to the thin amount of atmosphere still at our altitude,” Spetch said. 

    The Dragon spacecraft is expected to return to Earth no earlier than December.

    Video editor • Jerry Fisayo-Bambi

    Additional sources • AP

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  • Experts thrilled after deep-sea camera captures ‘first-ever record’ of elusive predator species

    Experts thrilled after deep-sea camera captures ‘first-ever record’ of elusive predator species

    It looked like a shadow at first — but after several minutes, a rare species of deep-sea shark had swum by an underwater camera 54 times, delighting researchers.

    The Miami Herald reported on the events, which happened in the Caribbean’s Cayman Islands. A group of scientists, conducting the area’s “first systematic investigation” of deep-sea biodiversity, lowered their camera to a depth of approximately 3,500 feet. They baited it with sardines and waited for sea life to appear — and sure enough, shortly thereafter, the roughskin dogfish appeared.

    Several of the small sharks proceeded to swim back and forth 54 times over several minutes as researchers captured high-quality footage of this normally “cryptic” predator.

    In their report published in the Journal of Fish Biology, the team called the recording “the first-ever record of the species” in the Cayman and central Caribbean. Not only is this helping in “adding a new species locality record,” they wrote, but it “expands our knowledge of the distribution of the roughskin dogfish in the region.”

    Considering that the roughskin dogfish are usually only seen as bycatch, accidentally captured and killed by fishing boats and deep-sea trawlers, this is a great achievement in order to better understand the species. And, the team added in their paper, it highlights that video systems are a great method for “enhancing and expanding our understanding of the biology and diversity of deep-sea sharks.”

    Finding effective, noninvasive ways to document the existence of species like the roughskin dogfish is key for scientists who are working to maintain biodiversity and species knowledge. This is particularly important in conservation efforts; after all, a team cannot help an endangered population thrive if they don’t know where and how they’re living.

    Watch now: Netflix chef and bestselling author talks about why she’s in love with new cooking technique

    Similar research has helped to repopulate critically endangered species such as eagles and ospreys, gray wolves, pygmy hogs, and Siamese crocodiles.

    Maintaining biodiversity is critical to ensuring that ecosystems stay healthy and functioning. As eminent scientific group The Royal Society puts it: “Biodiversity is essential for the processes that support all life on Earth, including humans. Without a wide range of animals, plants, and microorganisms, we cannot have the healthy ecosystems that we rely on to provide us with the air we breathe and the food we eat.”

    Join our free newsletter for good news and useful tips, and don’t miss this cool list of easy ways to help yourself while helping the planet.

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  • Researchers Turn Proteins Into Quantum Computing Unit

    Researchers Turn Proteins Into Quantum Computing Unit

    The University of Chicago reported a breakthrough in quantum technology using biological cells. Researchers from the university’s Pritzker School of Molecular Engineering transformed a protein from living cells into a functional quantum bit, or qubit. This significant achievement bridges the gap between biological systems and quantum technology.

    Traditionally, biological systems and quantum technology operate in vastly different environments. Living cells thrive in warm, dynamic environments, while quantum technology usually requires isolation and temperatures of almost 0 degrees Fahrenheit.

    Turning Proteins into Qubits

    Quantum protein
    Researchers turn living cells into a quantum bit; Photo: UChicago Pritzker School of Molecular Engineering / Jason Smith

    Researchers say the new protein-qubit functions as a quantum sensor and is capable of detecting minute changes within biological processes. The team’s approach was to develop a qubit from a biological system rather than trying to adapt a conventional quantum sensor to a biological environment.

    “Rather than taking a conventional quantum sensor and trying to camouflage it to enter a biological system, we wanted to explore the idea of using a biological system itself and developing it into a qubit,” said David Awschalom, a co-principal investigator.”

    Researchers believe that the cells could one day directly build protein-qubits that are stronger than existing quantum sensors.

    “Our findings not only enable new ways for quantum sensing inside living systems but also introduce a radically different approach to designing quantum materials,” said Peter Maurer, a co-principal investigator. “Specifically, we can now start using nature’s own tools of evolution and self-assembly to overcome some of the roadblocks faced by current spin-based quantum technology.”

    While the protein-based qubits do not match the sensitivity of the best quantum sensors, their ability to be genetically coded into living systems offers the potential to observe biological processes at the quantum level. Its potential capabilities range from protein folding to detecting early signs of diseases.

    “We’re entering an era where the boundary between quantum physics and biology begins to dissolve,” concluded first author Benjamin Soloway.


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  • Asteroid Bennu Is A Time Capsule Of Materials Bearing Witness To Its Origin And Transformation Over Billions Of Years – astrobiology.com

    1. Asteroid Bennu Is A Time Capsule Of Materials Bearing Witness To Its Origin And Transformation Over Billions Of Years  astrobiology.com
    2. Space weathering effects in Bennu asteroid samples  Nature
    3. Breakthrough for NASA: American space agency discovers material older than the Sun on asteroid 200 million  The Economic Times
    4. Particles older than solar system discovered in asteroid sample  WKEF
    5. Connolly: Bennu samples reveal clues to solar system origins, water-rock chemistry, space weathering  Rowan Today

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  • The Missing Giant: Do FAST Spectroscopic Observations Reveal a Scarcity of Large Polycyclic Aromatic Hydrocarbons in Astronomical Environments?

    The Missing Giant: Do FAST Spectroscopic Observations Reveal a Scarcity of Large Polycyclic Aromatic Hydrocarbons in Astronomical Environments?

    Fractional abundances of PAHs as a function of the number of carbon atoms 𝑁C. Dotted lines denote the estimated abundance upper limits of large quasi-symmetric PAHs in NGC 7027, and these values warrant cautious interpretation (refer to the contextual discussion). The solid curve shows the theoretical prediction from Draine & Lazarian (1998). For comparative analysis, values or upper limits from previous studies are overplotted. — astro-ph.GA

    The search for large polycyclic aromatic hydrocarbons (PAHs) with over 100 carbon atoms is crucial to resolving the origin of unidentified infrared emission (UIE) bands.

    These bands are commonly observed in nebulae and the interstellar medium, yet their spectroscopic assignment has remained unknown for decades. Using the Five-hundred-meter Aperture Spherical Radio Telescope (FAST), the world’s most sensitive instrument operating in the decimeter-wavelength range, we conducted a search for rotational transitions of large, quasi-symmetric PAHs.

    Our sample included two prototypical UIE sources, NGC 7027 and TMC-1, along with a non-UIE source, IRC+10216, for comparison. A matched filter technique was employed to isolate comb-like spectral features from quasi-symmetric PAHs containing 138 to 194 carbon atoms in the FAST spectra.

    This method significantly enhanced detection sensitivity to these astrophysically critical molecular signatures. Although no such features were detected, we derived upper limits on the abundance of large PAHs based on simplifying assumptions.

    These upper limits are lower than the values predicted by theoretical models, which might tentatively suggest that large PAHs may not be the primary carriers of UIE bands. However, this conclusion should be treated as tentative, given that it rests on simplistic assumptions which have not been empirically validated.

    Yi Shao, Yong Zhang, Xu-Jia Ouyang, Chuan-Peng Zhang

    Comments: 7 pages, 4 figures. Accepted for publication in MNRAS
    Subjects: Astrophysics of Galaxies (astro-ph.GA); Solar and Stellar Astrophysics (astro-ph.SR)
    Cite as: arXiv:2508.15302 [astro-ph.GA] (or arXiv:2508.15302v1 [astro-ph.GA] for this version)
    https://doi.org/10.48550/arXiv.2508.15302
    Focus to learn more
    Submission history
    From: Yong Zhang
    [v1] Thu, 21 Aug 2025 06:47:39 UTC (1,542 KB)
    https://arxiv.org/abs/2508.15302
    Astrobiology, Astrochemistry,

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