Category: 7. Science

  • Researchers identify a shared brain pattern behind feeling surprised

    Researchers identify a shared brain pattern behind feeling surprised

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    Whether it’s a surprise birthday cake or an underdog team suddenly stealing the ball, moments that violate our expectations tend to feel startling—and according to new research, the brain may respond to them in a surprisingly consistent way.

    Scientists at the University of Chicago built a whole‑brain “surprise network” that tracked how much a person’s expectations were violated and showed that the same pattern predicted surprise across three quite different scenarios: a laboratory learning game, the nail‑biting final minutes of college basketball, and short animated films that either followed or broke everyday rules. Their findings have been published in Nature Human Behaviour.

    The project began with a simple puzzle that has long preoccupied psychologists and neuroscientists. Surprise is one of the most vivid human feelings, but past studies rarely agreed on whether different kinds of surprise—social, physical, or purely informational—share a single neural signature. Study authors Ziwei Zhang and Monica Rosenberg reasoned that the best way to answer that question was not to look at one brain region at a time but to examine how hundreds of regions pulse together, moment by moment, whenever expectations are upended.

    To build their model, the researchers first revisited an open dataset collected at the University of Pennsylvania. Thirty‑two young adults lay in a brain scanner while playing an “adaptive learning” game. On each of 120 trials a cartoon helicopter hid behind the top edge of the screen and dropped a bag somewhere along a horizontal line. Before the drop the volunteers had to slide a bucket to the predicted landing spot.

    Most of the time the helicopter stayed in roughly the same place, but now and then it jumped to a new hidden position. The size of that jump, combined with uncertainty about whether a jump had just happened, provided an objective yardstick for how surprising each outcome should be to an ideal observer. While the game unfolded, the scanner recorded blood‑flow changes across 268 predefined brain parcels.

    Rather than calculate average connections over long intervals—a popular but slow‑moving approach—the team computed the “co‑fluctuation” between every pair of parcels at every single image frame. Each co‑fluctuation value captured whether two parcels’ signals rose and fell together in that instant. Feeding these high‑frequency edge traces into a leave‑one‑person‑out learning routine, the scientists identified two sets of connections. One set grew stronger when the modelled surprise level was high; the other did the opposite. Subtracting the average strength of the two sets yielded a single number each moment, the surprise network score, for each participant.

    Having trained the network on the game data, Zhang and Rosenberg next asked whether it would forecast surprise when the context changed completely. A separate group of twenty volunteers watched the last five minutes of nine National Collegiate Athletic Association tournament games while undergoing functional magnetic resonance imaging at Princeton University.

    For every possession change in each game an established sports‑analytics algorithm updated the home team’s win probability based on score difference, time remaining, possession, and team strength. Surprise was operationalised as the absolute change in that probability, but only when the change contradicted the prevailing belief about which team was likely to win.

    When the researchers aligned these probability swings with the surprise network score, the two rose and fell together even after accounting for visual and auditory features of the broadcasts, subtle head movements, court position, and remaining game time. In other words, the connection pattern forged in a joystick‑based learning task signalled belief‑inconsistent moments during real sports viewing, despite the switch from an interactive setting to passive spectatorship.

    To guard against the possibility that any large network might show the same property, the authors ran several control tests. Networks built from slower “sliding‑window” connectivity did not generalise. Networks made by averaging activity within established systems such as the default mode network or a well‑known sustained‑attention model failed to predict surprise in both directions.

    Models based only on activity of individual parcels, without considering how they interact, also stumbled. Even edge patterns tuned to the players’ motor predictions or to the reward signal in the learning game did not capture the basketball surprise metric. These comparisons suggest that moment‑to‑moment coordination across widely distributed regions contains information that simpler summaries miss.

    The team then flipped the analysis. They trained a new edge‑based network on the basketball data and tested it on the learning game. The flipped network again tracked surprise, confirming that the relationship was not tied to any one dataset.

    Interestingly, the edges that overlapped between the two independently trained networks concentrated in similar anatomical territories. Connections linking visual and parietal areas, the medial and lateral frontal cortices, and limbic zones repeatedly showed stronger co‑fluctuations when expectations were broken. In contrast, connections within primary sensory and motor systems tended to decrease in strength at those moments.

    A computational “lesioning” analysis—removing all edges tied to one functional system and rerunning the predictions—showed that eliminating links involving the frontoparietal control system or the default mode network markedly weakened performance, highlighting their importance for monitoring belief violations across contexts.

    For a final challenge the investigators examined a third open dataset collected at the Massachusetts Institute of Technology. Twenty‑nine adults watched brief videos in which cartoon agents either behaved logically or violated everyday psychology, such as walking straight through a solid wall, alongside clips that violated simple physics with no agents present, like objects passing through each other.

    The overlapping surprise network was significantly stronger when agents acted in unexpected ways compared with their expected counterparts, yet it did not distinguish between expected and unexpected physics clips. This outcome aligns with prior evidence that physical and social violations may rely on partly distinct brain mechanisms, and it hints that the surprise network is especially sensitive to belief shifts about intentions and actions.

    While the findings knit together three very different experimental worlds, the authors acknowledge several caveats. The network explains only a modest share of the moment‑to‑moment variance in surprise, meaning that other unmeasured factors also play large roles. Sample sizes, especially in the sports‑viewing dataset, were small by population standards. The magnetic resonance technique used is not optimised for deep brainstem nuclei that are thought to broadcast surprise signals, so those contributions remain blurry. Finally, the study depended on computational definitions of surprise rather than on each participant’s subjective reports, an issue future work could address with real‑time ratings or eye‑tracking.

    The study, “Brain network dynamics predict moments of surprise across contexts,” was published December 2024.

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  • These mysterious stars could glow forever using dark matter

    These mysterious stars could glow forever using dark matter

    A new kind of cosmic object could help solve one of the universe’s greatest mysteries: dark matter.

    Particle Astrophysicists have proposed the existence of a strange new type of star-like object, called a ‘dark dwarf’, which may be quietly glowing in the center of our galaxy.

    Far from being dark in appearance, these unusual objects are powered by dark matter (the invisible substance thought to make up about a quarter of the universe).

    The discovery comes from a UK-US research team and the full research findings has been published in the Journal of Cosmology and Astroparticle Physics (JCAP).

    Using theoretical models, the scientists suggest that dark matter can get trapped inside young stars, producing enough energy to stop them from cooling and turning them into stable, long-lasting objects they call dark dwarfs.

    Dark dwarfs are thought to form from brown dwarfs, which are often described as failed stars.

    Brown dwarfs are too small to sustain the nuclear fusion that powers most stars, so they cool and fade over time. But if they sit in a dense pocket of dark matter, like near the Milky Way’s center, they could capture dark matter particles.

    If those particles then collide and destroy each other, they release energy keeping the dark dwarf glowing indefinitely.

    The existence of these objects depends on dark matter being made of specific kinds of particles, known as WIMPs (Weakly Interacting Massive Particles).

    These are heavy particles that barely interact with ordinary matter, but could annihilate with one another inside stars, providing the energy needed to keep a dark dwarf alive.

    To tell dark dwarfs apart from other faint objects like brown dwarfs, the scientists point to a unique clue: lithium.

    The researchers believe dark dwarfs would still contain a rare form of lithium called lithium-7.

    In normal stars, lithium-7 gets burned up quickly. So, if they find an object that looks like a brown dwarf but still has lithium-7 that’s a strong hint it’s something different.

    Study co-author Dr Djuna Croon of Durham University, said: “The discovery of dark dwarfs in the galactic center would give us a unique insight into the particle nature of dark matter.”

    The team believes that telescopes like the James Webb Space Telescope could already be capable of spotting dark dwarfs, especially when focusing on the center of the galaxy.

    Another approach might be to look at many similar objects and statistically determine whether some of them could be dark dwarfs.

    Finding just one of these dark dwarfs, the researchers say, would be a major step towards uncovering the true nature of dark matter.

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  • Ocean World Exploration: New Autonomous Vehicle Studies Deep Ocean Critical Minerals – astrobiology.com

    1. Ocean World Exploration: New Autonomous Vehicle Studies Deep Ocean Critical Minerals  astrobiology.com
    2. Startup sets out to shed light on Earth’s dark and mysterious ocean floors: ‘The pot at the end of the rainbow’  The Cool Down
    3. Into The Abyss: Scientists Capture First-Ever Images of Ultra-Deep Waters Near the Mariana Trench  The Debrief
    4. Autonomous sub explores unexplored trench depths to reveal critical mineral clues  Space Daily

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  • Photodesorption Of SO2 And SO From UV-irradiated SO2 Ices

    Photodesorption Of SO2 And SO From UV-irradiated SO2 Ices

    Example of a simulated SO3 amorphous ice with 8 molecules in a cubic box with periodic boundary conditions. — astro-ph.GA

    The detection of high gas-phase abundances of SO2 and SO in the cold envelope of an intermediate mass protostar suggests that these molecules might form on icy dust grains and subsequently desorb to the gas phase by non-thermal desorption processes such as photodesorption.

    In this work we report photodesorption yields for SO2 and, tentatively, SO upon ultraviolet photon irradiation of SO2 ice samples at temperatures between 14 and 80 K. Photodesorption yields were measured directly in the gas phase using a calibrated quadrupole mass spectrometer.

    Yields of 2.3 x 10-4 molecule/photon and 6 x 10-5 molecule/photon were estimated for SO2 and SO at 14 K (respectively). The SO2 photodesorption yield increased with temperature up to a value of 3.8 x 10-4 molecule/photon at 70 K, followed by a decrease at 80 K that could be due to crystallization of the sample.

    The signal assigned to SO photodesorption did not significantly change with temperature. The estimated photodesorption yields were included in the Nautilus gas-grain chemical model to evaluate their contribution to the SO2 and SO gas-phase abundances in an astrophysical environment.

    In addition, we also present a theoretically estimated band strength for the 1395 cm-1 SO3 IR feature (A = 1.1 x 10-16 cm molecule-1). SO3 is the main detected product in irradiated SO2 ices, and a potential contributor to the 7.2 um band observed in some interstellar ice IR spectra.

    Rafael Martín-Doménech, Bruno Escribano, David Navarro-Almaida, Angèle Taillard, Héctor Carrascosa, Guillermo M. Muñoz Caro, Asunción Fuente

    Subjects: Astrophysics of Galaxies (astro-ph.GA); Solar and Stellar Astrophysics (astro-ph.SR)
    Cite as: arXiv:2507.06081 [astro-ph.GA] (or arXiv:2507.06081v1 [astro-ph.GA] for this version)
    https://doi.org/10.48550/arXiv.2507.06081
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    Submission history
    From: Rafael Martín-Doménech
    [v1] Tue, 8 Jul 2025 15:21:40 UTC (2,399 KB)
    https://arxiv.org/abs/2507.06081
    Astrobiology, Astrochemistry, interstellar,

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

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  • The Possibility of Hydrogen-Water Demixing in Uranus, Neptune, K2-18b and TOI-270d

    The Possibility of Hydrogen-Water Demixing in Uranus, Neptune, K2-18b and TOI-270d

    Potential interior structures of Uranus, Neptune, K2-18 b and TOI-270 d if they have undergone hydrogen-water demixing. We note that alternatives models are also possible (see Secs. 3 and 4). For Uranus and Neptune, the sketches correspond to the cases with Toffset = 1100 K, in which both planets are fully demixed. However, we can’t exclude scenarios in which demixing is still ongoing or does not occur at all. The sketch for K2-18 b shows a mini-Neptune scenario with ongoing demixing, while the one for TOI-270 d corresponds to a case of full demixing. — astro-ph.EP

    The internal structures of Uranus and Neptune remain unknown. In addition, sub-Neptunes are now thought to be the most common type of exoplanets.

    Understanding the physical processes that govern the interiors of such planets is therefore essential. Phase separation between hydrogen and water may occur in cold, water-rich intermediate-mass planets. We assess whether it could occur in Uranus, Neptune, K2-18 b and TOI-270 d, and investigate its effect on the planetary evolution and inferred internal structure.

    We couple planetary evolution models with recent ab initio calculations of the hydrogen-water phase diagram, allowing for temperature shifts to account for uncertainties in miscibility gaps.

    We find that demixing may occur and could lead to a complete depletion of water in the outermost regions of Uranus and Neptune. Temperature offsets of up to 1100~K lead to a depleted region comprising as much as 16% of the planet’s mass, and an increase in planetary radius by nearly 20%. For K2-18 b, our models suggest that hydrogen-water demixing is ongoing and may explain the absence of water features in its JWST spectrum.

    A temperature offset of 500~K is required to get a complete depletion of water in the atmosphere of K2-18 b. TOI-270 d may also have experienced hydrogen-water demixing. When applying a similar temperature offset on the phase diagram as for K2-18 b, we find a partial depletion of water in the atmosphere of TOI-270 d, consistent with JWST’s detection of water.

    Hydrogen-water immiscibility may play a key role in shaping the structure and evolution of both Solar System giant planets like Uranus and Neptune, and cold/temperate exoplanets such as K2-18 b and TOI-270 d. Accounting for such internal processes is crucial to accurately interpret atmospheric observations from current (e.g., JWST) and upcoming (e.g., ARIEL) missions.

    Saburo Howard, Ravit Helled, Armin Bergermann, Ronald Redmer

    Comments: Submitted to A&A
    Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
    Cite as: arXiv:2507.06288 [astro-ph.EP] (or arXiv:2507.06288v1 [astro-ph.EP] for this version)
    https://doi.org/10.48550/arXiv.2507.06288
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    Submission history
    From: Saburo Howard
    [v1] Tue, 8 Jul 2025 18:00:00 UTC (25,255 KB)
    https://arxiv.org/abs/2507.06288
    Astrobiology,

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  • TNO Colours Provide New Evidence For A Past Close Flyby Of Another Star To The Solar System

    TNO Colours Provide New Evidence For A Past Close Flyby Of Another Star To The Solar System

    Effect of flyby. (a) The pre-flyby colour gradient in the simulated disc is depicted by a false colour scheme representing very red to blue-grey TNOs. The same colour scheme is used throughout the paper. (b) Simulation snapshot of the flyby 128 years after periastron passage. The perturber star approached from the bottom right and already left the shown area. Disc matter is transported inwards and outwards along the spiral arms, with a fraction of the test particles injected into the planet region. Only the particles remaining bound to the Sun are shown. — astro-ph.EP

    Thousands of small bodies, known as trans-Neptunian objects (TNOs), orbit the Sun beyond Neptune. TNOs are remnants of the planets’ formation from a disc of gas and dust, so it is puzzling that they move mostly on eccentric orbits inclined to the planetary plane and show a complex red-to-grey colour distribution.

    A close stellar flyby can account for the TNOs’ dynamics, but it is unclear if this can also explain the correlation between their colours and orbital characteristics. Assuming an initial red-to-grey colour gradient in the disc, our numerical study finds that the spiral arms induced by the stellar flyby simultaneously lead to the observed TNOs’ colour patterns and orbital dynamics.

    The combined explanation of these TNO properties strengthens the evidence for a close flyby of another star to the young Solar System. Our study predicts that (1) small TNOs beyond 60 au will mostly be grey, and (2) retrograde TNOs will lack the colour most common to high-inclination TNOs. The anticipated TNO discoveries by the Vera Rubin telescope will be able to test these predictions. A confirmed flyby would allow us to reveal the chemical composition of the Solar System’s primordial disc.

    Susanne Pfalzner, Frank W. Wagner, Paul Gibbon

    Comments: 13 pages, 5 figures plus 4 in Appenidix, accepted for ApJ Letters
    Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Astrophysics of Galaxies (astro-ph.GA)
    Cite as: arXiv:2507.06693 [astro-ph.EP] (or arXiv:2507.06693v1 [astro-ph.EP] for this version)
    https://doi.org/10.48550/arXiv.2507.06693
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    Submission history
    From: Susanne Pfalzner Prof Dr
    [v1] Wed, 9 Jul 2025 09:37:35 UTC (22,112 KB)
    https://arxiv.org/abs/2507.06693
    Astrobiology, Astrochemistry, Astrogeology, Interstellar,

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

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  • bne IntelliNews – Israel successfully launches Dror 1 communications satellite joining space race

    bne IntelliNews – Israel successfully launches Dror 1 communications satellite joining space race

    Israel Aerospace Industries successfully launched the Dror 1 national communications satellite aboard a SpaceX Falcon 9 rocket from Cape Canaveral, Florida, marking a significant milestone in Israel’s space capabilities and technological independence.

    The 4.5-tonne satellite lifted off at 8:03am local time and separated from its launcher approximately 40 minutes after launch, beginning its independent orbit around Earth every 90 minutes. Dror 1 will reach its final geostationary orbit 36,000 kilometres above the equator within two weeks following a series of manoeuvres.

    Designed to meet Israel’s national communication needs for the coming years, Dror 1 represents the most advanced communications satellite ever built in Israel, featuring the largest transmission and reception antennas developed domestically. The satellite incorporates advanced Israeli technology and will provide flexible communication coverage for various government systems.

    The project stems from decisions made following the destruction of the Amos 6 satellite in a SpaceX explosion in September 2016, which prompted the Israeli government to establish an independent national communications capability. Israel invested approximately $200mn in developing Dror 1 since 2018 through collaboration between IAI, the Israel Space Agency and the Ministry of Innovation, Science and Technology.

    Dror 1 replaces the Amos satellite series and will serve Israeli communications companies whilst fulfilling security-related missions. The satellite will operate from a fixed point in space, providing continuous communication services for at least 15 years.

    IAI President Boaz Levy said Dror 1 was designed to preserve Israel’s national strategic capability whilst providing essential satellite communications for years to come. Innovation, Science and Technology Minister Gila Gamliel described the launch as a historic milestone in achieving complete communications independence.

    The Dror series is expected to continue with additional satellites to ensure Israel’s long-term communications sovereignty. The satellite features blue-and-white technology developed entirely in Israel, showcasing the country’s advanced space engineering capabilities and maintaining technological independence in this strategically vital sector.

     


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  • VLT Timelapse Of 3I/ATLAS, A New Interstellar Object – astrobiology.com

    1. VLT Timelapse Of 3I/ATLAS, A New Interstellar Object  astrobiology.com
    2. 3I/Atlas: Mystery interstellar object could be the oldest known comet  BBC
    3. A 7-Billion-Year-Old Ice Ball Just Entered Our Solar System  SciTechDaily
    4. Robotic Survey Camera at Caltech Observatory Spots “Interstellar Visitor”  Pasadena Now
    5. Astronomers have spotted an interstellar comet older than the Sun  The Economist

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  • Ancient Proteins from a 24 Million-Year-Old Rhino Open New Window into Evolution

    Ancient Proteins from a 24 Million-Year-Old Rhino Open New Window into Evolution

    Paleontologists have unlocked a groundbreaking discovery that brings clarity to the evolutionary history of rhinos. A recent study, published in Nature, reveals how ancient protein sequences recovered from the fossilized tooth of Epiaceratherium sp., a rhinocerotid from the Early Miocene period, are transforming our understanding of this species’ past. These ancient proteins, preserved for over 24 million years, have not only reshaped the timeline of the rhino family tree but have also raised new possibilities for exploring the deep past of evolutionary biology.

    This discovery challenges previous assumptions about the divergence of rhinocerotids and opens the door to studying evolution through a new lens—proteins. The research, which used sophisticated techniques like chiral amino acid analysis, demonstrates that ancient proteins can be preserved for millions of years, offering a unique window into evolutionary processes long before the advent of ancient DNA. With this groundbreaking research, scientists now have a more refined understanding of how rhinos evolved and diverged into different subfamilies.

    Uncovering Ancient Proteins in Rhino Fossils

    The discovery of ancient proteins in fossils has long been limited to specimens no older than four million years. However, this new study pushes that boundary dramatically by analyzing a tooth from Epiaceratherium sp., a rhinoceros species that lived in Canada’s High Arctic between 24 and 21 million years ago. Paleontologists, led by Dr. Marc Dickinson from the University of York, used chiral amino acid analysis to study the enamel of this ancient tooth. The remarkable aspect of this analysis is that it confirmed the proteins within the tooth were original, not a result of contamination or degradation. This provided a direct glimpse into the biochemical composition of a species that lived millions of years ago, giving researchers a tangible link to the distant past.

    As Dr. Dickinson noted, “It is phenomenal that these tools are enabling us to explore further and further back in time.” This statement reflects the immense potential of protein analysis as a tool for paleontologists. The ability to retrieve usable protein sequences from such an ancient sample challenges the limits of current methods and opens up exciting new avenues for paleobiological research. With further advancements, scientists may soon be able to piece together evolutionary histories for species whose genetic material is otherwise lost to time.

    The Implications for the Rhino Family Tree

    This new protein analysis provides fresh insights into the evolutionary split between two major subfamilies of rhinos: Elasmotheriinae and Rhinocerotinae. Prior studies based on bone structure suggested a much older divergence, but the findings from this study point to a more recent split occurring during the Oligocene, around 34 to 22 million years ago. This updated timeline could significantly alter our understanding of the evolutionary relationships between various rhino species, highlighting the complexity and variability of species’ evolutionary paths.

    By comparing the ancient proteins from Epiaceratherium sp. with previously studied rhinoceros fossils, researchers were able to refine these timelines. The divergence between the two subfamilies, once thought to be much older, is now understood to have occurred more recently than previously believed. Dr. Fazeelah Munir, also from the University of York, emphasized the significance of this new approach, stating, “Successful analysis of ancient proteins from such an old sample gives a fresh perspective to scientists around the globe who already have incredible fossils in their collections.” This insight reshapes how paleontologists approach fossil records, encouraging a broader exploration of protein-based analysis in ancient species.

    The Role of Ancient Proteins in Paleontological Research

    For decades, paleontologists have relied primarily on fossil shapes, structure, and, more recently, ancient DNA (aDNA) to trace the evolutionary lineage of extinct species. However, DNA degrades over time and rarely survives beyond one million years, making it difficult to study species from deeper geological periods. Proteins, on the other hand, are more stable and can persist for much longer under the right conditions. This study demonstrates the potential of ancient proteins to bridge the gap in studying species that existed millions of years ago, allowing scientists to access information that DNA analysis alone could not provide.

    Dr. Dickinson expressed the excitement of this discovery, saying, “Building on our knowledge of ancient proteins, we can now start asking fascinating new questions about the evolution of ancient life on our planet.” This new understanding will allow researchers to explore how ancient lifeforms adapted to changing environments, giving us deeper insight into the forces that shaped the diversity of life we see today.

    The Future of Ancient Protein Research

    With the success of this study, the door is now open for further exploration of ancient proteins, which could revolutionize our understanding of evolutionary biology. The ability to extract and analyze proteins from fossils that are millions of years old presents new opportunities for studying extinct species. This has profound implications not only for rhinoceros research but for the study of other ancient species as well. As Dr. Munir highlighted, “This important fossil helps us to understand our ancient past,” underscoring the value of expanding the tools available for paleontological research.

    With more fossils being analyzed using similar methods, it is likely that researchers will uncover even more revelations about the deep past. As technology continues to evolve, the field of paleontology may soon be able to answer questions that once seemed impossible to ask, shedding light on the origins of life on Earth and the intricate web of evolutionary relationships that has shaped our planet.

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  • Synaptic Plasticity Regulated by Protein Modifications Offer Path for Brain Therapeutics – Genetic Engineering and Biotechnology News

    1. Synaptic Plasticity Regulated by Protein Modifications Offer Path for Brain Therapeutics  Genetic Engineering and Biotechnology News
    2. How the Binding of Two Brain Molecules Creates Memories That Last a Lifetime  WIRED
    3. This tiny brain molecule could hold the key to learning, memory—and Alzheimer’s treatment  ScienceDaily
    4. Key brain protein may hold answers for memory loss and neurodegenerative diseases  Medical Xpress

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