NASA’s Io: Synchronized Volcanic Eruptions Indicate Cavernous Interior Structure

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Volcanic eruption on Io

Volcanic Eruption on Io Captured by the Galileo Spacecraft

NASA/JPL/DLR

In an unprecedented display, five volcanoes on Jupiter’s moon Io erupted simultaneously, indicating a potential connection to a shared underground magma network. This remarkable phenomenon may offer insights into the enigmatic interior of Io.

During late 2024, NASA’s Juno spacecraft provided crucial observations of a significant lava flow originating from Io’s south pole. “We noticed an enormous eruption with extensive lava flow, but upon closer inspection, all other hotspots were also glowing,” remarked Jani Radebaugh from Brigham Young University in Utah. “The abundance of magma is challenging to fully comprehend.”

This massive eruption impacted an area of about 65,000 square kilometers, releasing more energy than any previously recorded eruption on Io. “Imagine standing at the edge of a newly formed lava lake; behind you, a crevice opens, also flooding with lava. It would be both awe-inspiring and terrifying,” Radbaugh described. “Such beauty mixed with danger is captivating.”

The origin of this vast amount of magma remains a mystery, especially given current understanding of Io’s internal structure. Previous studies revealed that Io does not possess a global magma ocean beneath its crust, raising questions about how such a substantial volume of magma could erupt simultaneously.

Radbaugh and his team propose the existence of a ‘magmatic sponge’ beneath Io’s surface, consisting of networks of interconnected pores that can accumulate lava and erupt at hotspots. However, further observations are necessary to validate this theory, and with Juno moving away from Io, timely additional data may be scarce.

Despite its relatively small size, slightly larger than Earth’s moon, Io’s vigorous volcanic activity parallels eruptive phenomena observed on Earth. “Io provides a window into our planet’s past, reminiscent of an Earth that was hotter and more active,” Radebaugh noted. While the precise causes of these powerful eruptions remain elusive for now, resolving them may illuminate vital chapters in Earth’s geological history.

Exploring the Mysteries of the Universe: Cheshire, England

Join some of the brightest minds in science for a weekend dedicated to uncovering the mysteries of the universe, complete with a tour of the famed Lovell Telescope.

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Source: www.newscientist.com

Scientists Uncover Unique Internal Drum Structure in Odd-Looking Fish

The Armored Rockhead Poacher (Boslagonus Swanee) possesses a mysterious anatomical feature: a bowl-shaped cavity in its skull that has puzzled marine biologists for years. This unique trait is now believed to play a critical role in an innovative form of communication.



The Rockhead Poacher (Boslagonus Swanee) at the Oregon Coast Aquarium. Image credit: Rhinopias / CC BY-SA 4.0.

Originally described by Franz Steindachner in 1876, Boslagonus Swanee belongs to the family Agonidae. This fascinating fish can be found at depths of up to 18 meters in the eastern Pacific Ocean, from Alaska down to Carmel Bay in California.

Marine experts have long speculated about the purpose of the cavernous cranial fossa, which is roughly the size of the fish’s brain. Some theories suggest it aids in camouflage among rocky environments, while others propose it enhances hearing and sensory perception.

Recent advancements in imaging technology have led Louisiana State University student Daniel Geldof to propose a groundbreaking explanation. His findings suggest it might resonate with the rhythm of rock music rather than the serenity of coral reefs.

“My dissertation project aims to uncover the reasons behind this unique feature,” Geldof explained.

Utilizing a high-resolution micro-CT scanner, his team created an intricate 3D model of the rockhead poacher’s anatomy.

These scans indicated that the fish’s initial set of ribs are notably large, flat, and free-moving, positioned near the epigastric region of the skull without direct attachment.

Located at the base of these ribs are powerful muscles and tendons resembling drumsticks.

When these ribs vibrate against the skull’s calcified cavities, they create pulses of sound that can be transmitted through the substrate.

Geldof posits that this percussive mechanism likely evolved to facilitate communication among fish in their acoustically challenging intertidal habitats, where traditional underwater communication might be hindered by crashing waves and background noise.

In this rugged, shallow environment, using substrate vibrations may provide a more efficient means of communication aligned with the fish’s unique lifestyle.

Furthermore, Professor Geldof’s research combined contrast-enhanced soft tissue scans with data on bone structures to map the nerves, muscles, and microstructures within rockhead poachers, suggesting that the cranial fossa may serve sensory functions as well.

Branches of the dorsal lateral line nerve—a crucial component of the fish’s movement-sensing system—extend into the cavity, and the arrangement of microstructures suggests a role in mechanoreception, allowing the fish to sense movement and pressure.

Geldof concludes that this anatomical feature is multifunctional, serving both communicative and sensory purposes within the dynamic intertidal ecosystem.

“The intricate details of this small structure reflect not just a scientific inquiry, but a fundamental human curiosity,” he states.

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Daniel L. Geldof 2025. The Truth About Holes: The Morphology of Rockhead Poachers’ Skull Holes, Boslagonus Swanee (Agonidae). LSU Master’s Thesis 6270

Source: www.sci.news

Ancient Mammoth Bone Dwelling Uncovered in Ukraine: 18,000-Year-Old Circular Structure

The Upper Paleolithic site of Mezilich in Cherkasy Oblast, central Ukraine, features four remarkable mammoth bone structures, each ranging from 12 to 24 m2. These extensive constructions were meticulously crafted using hundreds of mammoth bones and tusks. Recent analyses of small mammal remains excavated directly from these archaeological formations indicate that one of these structures was in use for nearly 429 years, underscoring its role as a potential dwelling.



MBS 4 being excavated at the Upper Paleolithic site of Mezilich, Cherkasy Oblast, Ukraine. Image credit: Chu et al., doi: 10.12688/openreseurope.20112.1.

“Open-air Upper Paleolithic sites in east-central Europe, such as Mezilich, offer invaluable insights into human activities and biogeography during the Late Holistic Age—a period marked by significant environmental shifts,” stated Wei Chu, an archaeologist from Leiden University, and collaborators.

“These sites often exhibit deep loess sediment layers rich in lithic tools, faunal remains, and bone assemblages, serving as crucial environmental proxies for illuminating contemporary ecological conditions.”

“Notably, some of these locations have been discovered in direct association with mammoth bone deposits, representing some of the earliest known constructions showcasing both spatial and seasonal organization.”

“While many of these structures were historically viewed as domestic remnants,” they elaborated, “ongoing excavations have reignited debates about their primary functions—whether as dwellings or perhaps as ritualistic tombs, food storage areas, burial sites, religious landmarks, or primitive monuments.”

“Mezilich, situated in the mid reaches of the Dnieper River, is pivotal to this discourse due to its extraordinary conservation state, featuring four mammoth bone structures (MBS 1-4) that span heights of 12 to 24 m2 in diameter.

“These structures are complemented by surrounding features like artifact-filled pits, hunting tools, ivory, bone ornaments, and segmented areas rich in slaughtered animal remains and workshops with dense cultural deposits, each aligned around mammoth bone structures, revealing economic settlement units.”

In their latest study, the researchers scrutinized the dating and composition of MBS 4—the only Mezilich structure containing artifacts that can be directly dated within the archaeological layer.

By analyzing small mammal remains rather than mammoth bones, they established a more accurate age for MBS 4, estimated to be between approximately 18,248 and 17,764 years old.

Crucially, the findings indicate that this structure was actively occupied for 429 years.

These results suggest that Mezilich was a stable, long-term settlement rather than a transient camp used intermittently.

The structure likely served as a residence for multiple generations, enduring and being reused throughout the centuries.

“MBS 4 corresponds with the harshest conditions of the last Ice Age,” the researchers noted.

“Interestingly, the period of occupation appears brief—potentially comprising only a few visits over many centuries.”

“This implies that these mammoth bone shelters were practical solutions for survival, rather than established permanent settlements.”

“Why is this significant? Beyond the remarkable ingenuity of utilizing mammoth bones for construction, these findings alter our perspective on human resilience and adaptability,” they remarked.

“They illustrate how communities thrived even in extreme environments, transforming large animal remains into protective architecture.”

“As dating techniques improve, sites like Mezilich continuously challenge our preconceived notions about prehistoric existence,” they concluded.

“These societies were dynamic, resource-abundant, and deeply interconnected with their environments, and their lessons are relevant even today.”

For further insights, refer to the team’s published paper in Open Research Europe.

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W. Chu et al. 2025. Revised radiocarbon chronology of bone structures and related features of mammoths from Mezilich, Ukraine. Open Res Europe 5:198; doi: 10.12688/openreseurope.20112.1

Source: www.sci.news

Neuroscientists Discover Five Key Phases of Brain Structure Development Across the Human Lifespan

Recent findings from neuroscientists reveal that the brain’s structure divides into five main stages throughout a typical person’s life, marked by four significant turning points from birth to death where the brain undergoes reorganization. Brain topology in children evolves from birth up to a crucial transition at age 9, then shifts into adolescence, which generally lasts until around age 32. In your early 30s, the neural wiring transitions to adult mode, marking the longest phase that extends for over 30 years. The third turning point occurs at about age 66, indicating the start of an early aging phase of brain structure, while the late brain phase begins around age 83.

Masry et al. Using a dataset of MRI diffusion scans, they compared the brains of 3,802 individuals aged 0 to 90 years. The dataset maps neural connections by tracking the movement of water molecules through brain tissue. Image credit: Mously et al., doi: 10.1038/s41467-025-65974-8.

“While we know brain wiring plays a crucial role in our development, we still lack a comprehensive understanding of how and why it fluctuates throughout life,” explained Dr. Alexa Mausley, a researcher at the University of Cambridge.

“This study is the first to pinpoint essential stages in brain wiring throughout the human lifespan.”

“These epochs offer vital insight into our brain’s strengths and vulnerabilities at different life stages.”

“Understanding these changes could shed light on why certain developmental challenges arise, such as learning difficulties in early childhood or dementia later in life.”

During the transition from infancy to childhood, strengthened neural networks emerge as the excess of synapses (the connections between neurons) in a baby’s brain diminishes, allowing only the most active synapses to thrive.

The brain rewires in a consistent pattern from birth until approximately age 9.

In this timeframe, the volumes of gray and white matter grow swiftly, resulting in maximal cortical thickness (the distance from the outer gray matter to the inner white matter), with the cortical folds stabilizing.

By the first turning point at age 9, cognitive abilities begin to evolve gradually, and the likelihood of mental health issues becomes more pronounced.

The second stage, adolescence, is characterized by an ongoing increase in white matter volume, leading to an enhancement in the sophistication of the brain’s communication networks, measurable through water diffusion scans.

This phase is marked by improved connectivity efficiency across specific regions and swift communication throughout the brain, correlating with enhanced cognitive performance.

“As expected, neural efficiency is closely linked to shorter pathways, and this efficiency increases throughout adolescence,” Mausley notes.

“These advancements peak in your early 30s, representing the most significant turning point in your lifetime.”

“Around age 32, the change in wiring direction is the most pronounced, and the overall trajectory alteration is greater than at any other turning points.”

“Although the onset of puberty is clearly defined, the conclusion is far harder to identify scientifically.”

“Based solely on neural structure, we found that puberty-related changes in brain structure conclude by the early 30s.”

Post age 32, adulthood enters its longest phase, characterized by a more stable brain structure with no significant turning points for three decades. This aligns with findings indicating an “intellectual and personality plateau.”

Additionally, the researchers observed a greater degree of “segregation” during this phase, indicating a gradual fragmentation of brain regions.

The tipping point at age 66 is more gradual, lacking dramatic structural shifts; however, notable changes in brain network patterns were found around this age on average.

“Our findings indicate a gradual reconfiguration of brain networks that peaks in the mid-60s,” stated Dr. Mausley.

“This is likely linked to aging, as white matter begins to decline, reducing connectivity further.”

“We are currently facing an era where individuals are increasingly at risk for various health conditions impacting the brain, such as high blood pressure.”

The final turning point arises around age 83, ushering in the last stage of brain structure.

Data from this stage is scarce, but a key characteristic is the shift from global to local connectivity as interactions across the brain diminish while reliance on specific regions intensifies.

Professor Duncan Astle of the University of Cambridge remarked: “In reflection, many of us recognize that our lives encompass distinct stages.”

“Interestingly, the brain also navigates through these phases.”

“Numerous neurodevelopmental, mental health, and neurological conditions are tied to the brain’s wiring.”

“In fact, variations in brain wiring can predict challenges with attention, language, memory, and a wide array of other behaviors.”

“Recognizing that structural transformations in the brain occur not in a linear fashion but through several major turning points can assist us in identifying when and how brain wiring may be vulnerable to disruptions.”

a paper detailing the study was published in the journal on November 25. Nature Communications.

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A. Mausley et al. 2025. Topological turning points across the human lifespan. Nat Commun 16, 10055; doi: 10.1038/s41467-025-65974-8

Source: www.sci.news

Researchers Explore the Structure of Bacteriophages

The researchers employed cryo-electron microscopy to examine the structure of Bas63, a bacteriophage from the Ounabilinae subfamily. Felixona virus targets the genus Escherichia coli to explore their evolutionary relationships and functional adaptations.

Composite representation of the complete Bas63 virion. Image credit: Hodgkinson Bean et al., doi: 10.1126/sciadv.adx0790.

Bacteriophages classified as Caudobilites constitute the most prevalent group of viruses on the planet.

The Caudovirites encompass 7 orders, 74 families, and 121 subfamilies.

“Bacteriophages are of significant interest to researchers seeking alternatives to antibiotics in response to the growing threat of antimicrobial resistance,” stated Dr. James Hodgkinson-Bean from the University of Otago.

“These bacteriophage viruses pose no harm to multicellular organisms and can selectively target and eliminate specific bacteria.”

“This is why there is a surge in research and application of ‘phage therapy’ for treating highly drug-resistant bacterial infections.”

“Bacteriophages are intricate viruses that infect bacteria using a large mechanical structure known as a ‘tail.’

In this study, Dr. Hodgkinson-Bean and his team examined the structure of Bas63 at the molecular level to gain insights into the tail’s role during infection.

“This research is crucial for identifying optimal bacteriophages for treatment and understanding the variations in infection behavior observed in laboratory settings,” said Dr. Hodgkinson-Bean.

“As antibiotic resistance escalates and plant pathogens threaten global food security, bacteriophages represent a promising alternative,” remarked Dr. Mifnea Bostina, also from the University of Otago.

“Our comprehensive bacteriophage blueprint advances the strategic design of medical, agricultural, and industrial uses, from treating infectious diseases to combating biofilms in food processing and water systems.”

“Beyond the realm of science, the 3D data illustrating the virus’s unique whisker and collar combinations, hexameric decorative proteins, and varied tail fibers might inspire artists, animators, and educators.”

Understanding viral structure also enhances our comprehension of their evolution.

“While DNA generally serves as the primary marker of human evolution, the three-dimensional structure of a virus offers more nuanced information about its distant evolutionary ties to other viruses,” said Dr. Hodgkinson-Bean.

The authors identified features previously observed only in distantly related viruses, uncovering previously unrecognized evolutionary connections.

“Through structural research, we have established that bacteriophages are related to herpesviruses, and this connection is believed to date back billions of years, prior to the rise of multicellular life,” remarked Dr. Hodgkinson-Bean.

“Looking at the structure of bacteriophages is akin to viewing a living fossil, an ancient primordial entity.”

“There’s something profoundly beautiful about it.”

These findings were published in the Journal on November 12, 2025, in Scientific Progress.

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James Hodgkinson-Bean et al. 2025. Cryo-EM structure of bacteriophage Bas63 reveals structural conservation and diversity of bacteriophage Bas63. Felixona virus Genus. Scientific Progress 11(46); doi: 10.1126/sciadv.adx0790

Source: www.sci.news

Astronomers Reveal Pleiades Star Cluster is Integral to a Vast Stellar Structure

The Pleiades star cluster, also referred to as the Seven Sisters and Messier 45, is an open star cluster situated around 440 light-years away from Earth in the Taurus constellation. It forms the central core of a larger network that includes several known star clusters scattered over 600 parsecs (1,950 light-years). This network is known as the Greater Pleiades Complex and comprises at least 3,091 stars.



Pleiades star cluster. Image credit: NASA / ESA / AURA / California Institute of Technology / Palomar Observatory.

Stars originate from clouds of dust and gas. Clumps of this material come together and eventually collapse under their gravity, creating the hot core that becomes a star.

Star formation typically occurs in bursts, with numerous stars being born in rapid succession.

A collection of stars that form from the same molecular cloud is known as a star cluster.

These stars remain gravitationally bound to one another for thousands of years.

Over tens to hundreds of millions of years, the materials that birthed them are expelled by cosmic winds, radiation, and various astrophysical phenomena.

As this occurs, individual stars can merge into their host galaxies, making it complex to ascertain their relationships and trace their origins, especially after more than 100 million years have elapsed.

In a recent study, Dr. Luke Buuma from the Carnegie Institution for Science Observatory and his colleagues concentrated on the Pleiades star cluster.

Utilizing data from NASA’s TESS mission, ESA’s Gaia spacecraft, and the Sloan Digital Sky Survey (SDSS), they discovered that this cluster is the core of a broader structure of related stars spanning over 1,950 light-years.

“We refer to this as the Greater Pleiades Complex,” Dr. Bouma stated.

“It includes at least three known groups of stars, and likely two additional ones.”

“We confirmed that most members of this structure have origins in the same gigantic stellar nursery.”

A key aspect of their methodology is that a star’s rotation rate decreases with age.

The study utilized a combination of TESS’s stellar rotation data (made to detect exoplanets) and Gaia’s stellar motion observations (designed for mapping the Milky Way).

With this information, they developed a new method based on rotation to identify stars that share common origins.

“For the first time, by amalgamating data from Gaia, TESS, and SDSS, we confidently identified a new member of the Pleiades cluster,” reported Dr. Buma.

“Data from each mission alone was not enough to reveal the full scope of the structure.”

“However, when we integrated stellar motions from Gaia, rotations from TESS, and chemical data from SDSS, a coherent picture took shape.”

“It’s akin to piecing together a jigsaw puzzle, where every dataset provides a different piece of a larger whole.”

Besides their comparable ages, the authors highlighted that the stars in the Greater Pleiades cluster share similar chemical compositions and were once much closer to one another.

The fifth generation of SDSS data was employed for the chemical abundance analysis.

“The Pleiades star cluster has been pivotal in human observations of stars since ancient times,” Dr. Buma remarked.

“This research marks a significant advancement in understanding the changes in the Pleiades star cluster since its formation 100 million years ago.”

The researchers believe their findings carry broad implications.

The Pleiades is not merely an astrophysical benchmark for young stars and exoplanets but also a significant cultural symbol, referenced in the Old Testament and Talmud, celebrated as Matariki in New Zealand, and represented on the Subaru logo in Japan.

Professor Andrew Mann of the University of North Carolina at Chapel Hill stated, “We are starting to understand that many stars near the Sun belong to extensive star clusters with intricate structures.”

“Our study provides a novel method to uncover these hidden connections.”

A paper detailing the survey results has been published this week in the Astrophysical Journal.

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Andrew W. Boyle et al. 2025. Missing Sister Found: TESS and Gaia Reveal Dissolving Pleiades Complex. APJ 994, 24; doi: 10.3847/1538-4357/ae0724

Source: www.sci.news

Brain Structure Mapping Alone Fails to Capture Its Functionality

The human brain contains trillions of connections

Sherbrooke Connectivity Imaging Lab/Connect Images/Alamy

Is it possible to fully comprehend brain function if we can accurately map its structures? Researchers aim to develop a wiring diagram, or connectome, of our neural pathways, yet the task of unveiling the brain’s mysteries is proving to be complex.

The Connectome serves as a roadmap for nerve signal pathways, but Sophie Dovari from Princeton University and her team have found notable gaps in these pathways.

Researchers analyzed the connectome of the nematode worm, Caenorhabditis elegans, and compared it to recorded neural signals. They accomplished this by stimulating each neuron and observing how signals flowed through the connectome. This method is feasible with nematodes due to their relatively simple nervous system, composed of roughly 300 neurons.

Nematode worms are significantly simpler than humans, with approximately 300 neurons depicted in green

Heiti Paves / Alamy Stock Photo

By viewing these two datasets as mathematical networks, researchers can ascertain whether closely connected groups of neurons manifest a high frequency of signal exchanges. They uncovered that this correlation is not always evident.

Dvali notes instances of substantial connection density and overlapping signal exchanges, like how worms eat or the groups of neurons that correspond well. However, even in cases where they appeared significantly connected, a gap remained in understanding their respective functionalities across both networks. Overall, these findings suggest that the biological connectome is insufficient to predict all neural behaviors.

Team member Andrew Leifer, also from Princeton University, points out that signals do not always follow the shortest paths between neurons; some may communicate beyond their direct connections. “While we typically leverage connectomes for research, the multitude of useful connections calls for deeper comprehension,” he explains.

According to Albert Laslo Barabasi at Northeastern University, Massachusetts, criticism surrounding connectomics often revolves around its inability to provide action-oriented insights from structural data. This new paper seeks to address that challenge.

Looking forward, researchers aim to delve deeper into how signals disseminate through the connectome when multiple neurons are activated simultaneously, with aspirations to study more complex organisms, such as fruit fly larvae, recognized for their intricate neural networks. “We are on the verge of a revolution in brain mapping,” Barabasi concludes.

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Source: www.newscientist.com

The Brain’s Tiny Structure Influences Your Eating Habits

The bed nuclei of the stria terminalis comprise a larger, banded structure in the brain known as the stria terminalis.

My Box/Alamy

Brain regions that influence food intake may eventually be targeted to enhance weight loss or therapeutic interventions.

Studies indicate that activating neurons in this specific brain region leads to increased food intake in mice, particularly when consuming sunflower seed-sized food items. However, the impact of taste on neuronal activity remained ambiguous.

For deeper insights, refer to Charles Zuker from Columbia University, who, along with his team, conducted brain imaging on mice. Earlier research linked sweet taste neuron activity in the amygdala with the enjoyment of sweet substances.

These neurons stimulate other neurons in the BNST, sometimes referred to as the “expanded amygdala.” This marks the first evidence of taste signal reception by this brain structure, according to Haijiang Cai from the University of Arizona, who was not part of the study.

The researchers aimed to determine whether these activated BNST neurons influence dietary choices, so they genetically modified cells to prevent activation when mice tasted sweet substances. Over a 10-minute period, these modified mice exhibited significantly reduced consumption compared to their normal counterparts, indicating that BNST neuron activation encourages sweet taste consumption.

Interestingly, the researchers also discovered that this artificial activation led mice to consume more water and even seek out salty or bitter substances, which they typically avoid.

Further experiments indicated that more BNST neurons were activated by sweet and salty tastes in hungry or salt-depleted mice, suggesting that the BNST integrates taste signals along with nutrient deficiency cues to regulate food intake, according to Cai.

Given the similarities between human and mouse BNST, these findings are relevant for humans, says Cai. They suggest that developing drugs to activate BNST neurons could aid individuals experiencing severe appetite loss, like those undergoing cancer treatment.

Cai mentioned that numerous brain pathways regulate food intake, and some may compensate for long-term changes in BNST activity induced by drugs. Therefore, targeting multiple feeding circuits would likely be necessary.

This research also has implications for improving results from weight loss treatments, including the GLP-1 drug semaglutide. This drug binds to neurons in the BNST, and a clearer understanding of its effects on food consumption could enhance the effectiveness of such medications, according to Sarah Stern from the Max Planck Florida Institute for Neuroscience.

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Source: www.newscientist.com

Our Brains Don’t Change Structure After Amputation

Before entering the MRI scanner, Emily Weldon practiced moving a lost finger from her amputated arm, accompanied by a researcher.

Tamar Makin/Hunter Schone

Research suggests our brains may not reconfigure as much as previously believed following an amputation.

The somatosensory cortex, which processes sensory data like touch and temperature from the entire body, has been shown in various studies to have distinct regions mapped to different body parts. For instance, the sensation of burning your hands might activate regions corresponding to your toes.

There is evidence indicating that when a nerve is severed, the somatosensory cortex may reorganize. A study observing macaques with severed arm nerves revealed that neurons typically responding to hand stimuli were instead active when the face was touched. The researchers inferred that some cortical areas initially linked to the hands were repurposed to respond to facial sensations.

However, a team led by Tamar Makin from Cambridge University conducted a groundbreaking comparison of brain activity in individuals before and after amputation, revealing minimal changes.

Using MRI, researchers scanned the brains of three participants prior to their medically necessary arm amputations. During the scans, they were instructed to pucker their lips and attempt to move their fingers.

Interestingly, even after numerous attempts to willfully move fingers they no longer possessed, the brain signals remained unchanged. “To the best of our measurement, they remain the same,” Makin noted.

Long-term follow-ups on two participants, 18 months and 5 years post-surgery, indicated no significant alterations in brain signals since the initial scans.

The researchers utilized an AI model that was trained to correlate brain activity with specific finger movements. When participants imagined moving their fingers in a random sequence, the model accurately identified which finger they were trying to move, demonstrating consistent neural activity.

In another experiment segment, somatosensory cortical activity was assessed in 26 individuals, average 23 years post-amputation, during attempts to move their lips and fingers. The findings showed comparable activity levels.

“This study decisively challenges the notion that the brain can easily remap, rewire, or reorganize as initially thought,” remarked John Krakauer from Johns Hopkins University in Maryland.

The implications of these findings could significantly affect treatments for phantom limb pain, a common condition where amputees experience discomfort in limbs that are no longer present.

Some therapeutic approaches utilize virtual reality and visual stimuli to prompt brain reorganization, yet results have varied, sometimes influenced by placebo effects, according to Makin.

Researchers suggest that innovative methods, such as implanting nerves into new tissues during amputation, might help mitigate this condition. If remaining nerves are left unconnected, they can thicken, potentially contributing to phantom limb pain.

“The previous maladaptive plasticity theory regarding phantom pain relied on the belief that reorganization was possible, which now seems incorrect,” stated Krakauer. “This fundamentally alters our approach to treating phantom limb pain since its underlying theory has been disproven.”

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Source: www.newscientist.com

Webb Observations Reveal Two Stars Shape the Irregular Structure of NGC 6072

Astronomers captured a new high-resolution image of the planetary nebula NGC 6072 using two instruments on board the NASA/ESA/CSA James Webb Space Telescope.

This Webb/Nircam image depicts NGC 6072, a planetary nebula located about 4,048 light years away in the constellation of Scorpius. Photo credits: NASA/ESA/CSA/STSCI.

NGC 6072 is situated approximately 1,241 parsecs (4,048 light years) away from the southern constellations of Scorpius.

Also known by designations such as ESO 389-15, HEN 2-148, and IRAS 16097-3606, this nebula has a dynamic age of about 10,000 years.

It was first discovered by British astronomer John Herschel on June 7, 1837.

“Since their discovery in the 1700s, astronomers have learned that planetary nebulae, the expanding shells of luminous gases expelled by dying stars, can take on various shapes and forms,” noted Webb astronomers.

“While most planetary nebulae are circular, elliptical, or bipolar, the new Webb image of NGC 6072 reveals a more complex structure.”

Images captured by Webb’s Nircam (near-infrared camera) suggest that NGC 6072 displays a multipolar configuration.

“This indicates there are multiple oval lobes being ejected from the center in various directions,” the astronomers explained.

“These outflows compress the surrounding gas into a disk-like structure.”

“This suggests the presence of at least two stars at the center of this nebula.”

“In particular, a companion star appears to be interacting with an aging star, drawing in some of its outer gas and dust layers.”

The central area of the nebula glows due to hot stars, reflected in the light blue hue characteristic of near-infrared light.

The dark orange regions, composed of gas and dust, create pockets and voids appearing dark blue.

This material likely forms when dense molecules shield themselves from the intense radiation emitted by the central star.

There may also be a temporal aspect; for thousands of years, rapid winds from the main star could have been blowing away the surrounding material as it loses mass.

This web/milli image highlights the planetary nebula NGC 6072. Image credits: NASA/ESA/CSA/STSCI.

The long wavelengths captured by Webb’s Miri (mid-infrared instrument) emphasize the dust, unveiling a star that astronomers believe resides at the center of the nebula.

“The image appears as a small pink dot,” remarked the researchers.

“The mid-infrared wavelengths also reveal a concentric ring expanding outward from the central region.

“This might indicate the presence of a secondary star at the heart of the nebula, obscured from direct observation.”

“This secondary star orbits the primary star, creating rings of material that spiral outward as the original star sheds mass over time.”

“The red regions captured by Nircam and the blue areas highlighted by Miri track cool molecular gases (likely molecular hydrogen), while the central region tracks hot ionized gases.”

Source: www.sci.news

Webb Reveals the Atmospheric Structure of Sub-Neptune TOI-421B

Subneptin is a type of exoplanet characterized by high birth discharge thrombosis and lacks analogs within our solar system. Significantly smaller than gas giants, and typically cooler than Hot Jupiter exoplanets, these worlds were notably challenging to study before the launch of the NASA/ESA/CSA James Webb Space Telescope. Many subneptins are obscured by thick clouds and hazards, hindering our ability to analyze their atmospheric structures. Utilizing the Webb, astronomers have obtained the transmission spectrum of subneptin TOI-421B, unveiling its atmospheric chemical signatures.



Artist’s impression of Subneptune Exoplanet TOI-421B. Image credit: NASA/ESA/CSA/DANI player, STSCI.

TOI-421 is a solar-type star located approximately 245 light years away in the constellation of Repas.

Commonly known as BD-14 1137, this star is around 10 billion years old and hosts at least two giant exoplanets.

The inner planet, TOI-421B, is a subneptin with a radius of 2.65 times that of Earth and boasts a high equilibrium temperature of 647 degrees Celsius (1,197 degrees Fahrenheit).

“Prior to Webb, scientists had scant information regarding subneptins,” stated University of Maryland astronomer Brian Davenport and his team.

“These planets are several times larger than Earth, yet still much smaller than gas giants, usually cooler than hot Jupiters, and significantly harder to observe than their larger gas analogs.”

“A crucial finding before Webb was that many Neptune-like atmospheres exhibited flat or featureless transmission spectra.”

“This indicates that when scientists scrutinized the spectrum of planets transiting in front of a host star, they only observed flatline spectra, missing the details of the spectrum (chemical fingerprints revealing atmospheric composition).”

“Based on these flatline spectra observations, it was concluded that certain subneptins are extremely obscured, potentially due to clouds or haze.”

“Why did we focus on planet TOI-421B? Because we hypothesized it might be an exception,” said Eliza Kempton, an astronomer at the University of Maryland.

“This hypothesis stemmed from previous data suggesting that planets within specific temperature ranges were less likely to be shrouded in haze or clouds.”

“The temperature threshold is around 577 degrees (1,070 degrees Fahrenheit); beneath this, it was assumed that complex photochemical reactions occur between sunlight and methane gas, leading to haze.”

TOI-421B, with a temperature of approximately 727 degrees Celsius (1,340 degrees Fahrenheit), is significantly above this threshold.



The transmission spectra of subneptune TOI-421B uncover the presence of water and potential indications of sulfur dioxide and carbon monoxide, without signs of carbon dioxide or methane. Image credits: NASA/ESA/CSA/Joseph Olmsted, STSCI.

Without the interference of haze or clouds, astronomers anticipated observing a clear atmosphere.

“We identified spectral features attributable to various gases, which empowered us to ascertain the atmospheric composition,” explained Davenport.

“In many previously studied subneptins, although I inferred that their atmospheres contained specific gases, they remained obscured by haze.”

Researchers have identified atmospheric water vapor along with tentative signatures of carbon monoxide and sulfur dioxide.

However, they did not find molecules such as methane and carbon dioxide.

From the gathered data, they speculate a substantial amount of hydrogen constitutes the atmosphere.

This prevalence of lightweight hydrogen was an unexpected revelation for scientists.

“We recently came to grips with the notion that one of the initial subneptins observed by Webb has a significant molecular atmosphere.

“This implies that TOI-421B may have formed and evolved differently compared to other cooler subneptins.”

“The hydrogen-rich atmosphere is intriguing, as it resembles the composition of its host star TOI-421B.”

“By incorporating the same gases that formed the host star into the planet’s atmosphere, and cooling them, one could replicate the same gas combination.”

“This process aligns more closely with the giant planets of our solar system, differing from previously observed subneptins through Webb.”

The team’s research paper was published this week in the Astrophysical Journal Letters.

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Brian Davenport et al. 2025. TOI-421B: High-temperature Neptune with a low average molecular weight atmosphere, haze-free. apjl 984, L44; doi: 10.3847/2041-8213/ADCD76

Source: www.sci.news

Mapping the Three-Dimensional Structure of the Atmosphere of WASP-121B by Astronomers

An extreme class of planets not found in our solar system, Ultrahot Jupiters offers a unique window into atmospheric processes. Using four telescope units in ESO’s extremely large telescopes, astronomers are currently being investigated deep into the atmosphere of the Ultra Hot Jupiter ExoPlanet WASP-121B, revealing separate powerful winds in separate layers, We have formed a map of the 3D structure of the atmosphere.

This diagram shows the atmospheric structure and movement of the WASP-121B. Image credit: ESO/M. Kornmesser.

The WASP-121B is a gas giant exoplanet 1.87 times larger than Jupiter and 1.18 times larger.

First discovered in 2016, this alien world takes just 1.3 days to traverse the parent F6 star WASP-121 (TYC 7630-352-1).

The WASP-121 system is approximately 881 light years away from the puppy’s constellations.

The WASP-121B is what is called “Ultra Hot Jupiter” and takes only 1.3 days to get the WASP-121 into orbit. It’s so close to the parent star, that when it gets closer, the star’s gravity begins to tear it apart.

Astronomers estimate the planet’s temperature is about 2,500 degrees Celsius (4,600 degrees Fahrenheit), high enough to boil some metals.

“The WASP-121B atmosphere behaves in a way that challenges understanding of how the weather works not only on Earth, but on all planets,” says the astronomer at Lagrange Laboratory, an astronomer at ESO. said Dr. Julia Victoria Seidel. Cote d’Azur.

“It feels like something from science fiction.”

“What we found was amazing. The Jet River rotates material around the planet’s equator, and another flow at a lower level in the atmosphere moves the gas from the hot side to the cool side. “

“We’ve never seen this kind of climate on any planet.”

“The observed jet stream spans half the planet, gaining speed and thrusts the air in the sky hard as it crosses the hot side of the WASP-121B.”

“Even the strongest hurricanes in the solar system seem milder in comparison.”

Dr. Seidel and colleagues to reveal the 3D structure of the atmosphere of the WASP-121B Used Espresso equipment located in ESO’s extremely large telescopes (VLTs) combines the light from four large telescope units into a single signal.

This combination mode of VLT collects 4 times the light of an individual telescope unit and reveals the details of the feinder.

Espresso was able to detect signatures of multiple chemical elements by observing the planet’s complete passage in front of the host star, resulting in different layers of the atmosphere.

“The VLT has led to three different layers of the Exoplanet atmosphere falling on one side,” said Dr. Leonardo A. dos Santos, an astronomer at the Institute of Space Telescope Science.

Astronomers were able to track the movement of iron, sodium and hydrogen, and track winds in the deep, central and shallow layers of the Earth’s atmosphere, respectively.

“It’s a very challenging observation for space telescopes and highlights the importance of ground-based observations on exoplanets,” Dr. Dos Santos said.

Interestingly, observations are also It was revealed Titanium is present just below the jet stream.

This was another surprise, as previous observations of the planet showed that this element was absent, and perhaps hidden deep within the atmosphere.

“It’s truly amazing to be able to study the details of such vast distances such as the chemical composition and weather patterns,” said PhD Viviana Prinos. A student at Lund University.

____

JV Seidel et al. Vertical structure of the atmospheric jet stream of the exporanet. NaturePublished online on February 18th, 2025. doi:10.1038/s41586-025-08664-1

Source: www.sci.news

The Statistical Structure of the Humpback Whale Song Resembles Human Language

An international team of researchers analyzed moans, moans, whistles, bark, screams, and creaks in recordings of humpback whale songs collected over eight years in New Caledonia.

Arnon et al. We have revealed the same statistical structure of humpback whales (Megaptera novaeangliae) Songs are characteristic of human language. Image credits: Christopher Michelle / CC by 2.0.

“I found something really fascinating,” said Dr. Emma Carroll, a marine biologist at Auckland University.

In this study, Dr. Carol and colleagues apply quantitative methods that are usually used to evaluate infantile utterances, and that this applies to culturally evolved learning songs in human languages. I found it. Humpback whale (Megaptera novaeangliae).

In human language, structurally consistent units exhibit frequency distribution that follows the law of power. Zipfian distribution – Attributes that are likely to promote learning and enhance accurate conservation of language across generations.

The Humpback Whale Song is one of the most complex vocal displays in the Animal Kingdom and is passed down through cultural transmission, providing something compelling in parallel with human language.

These songs are highly structured, consisting of nested hierarchical components. The theme is combined with the sound elements that form the phrase, the phrases that are repeated in the theme, and the song.

If statistical properties of human language arise from cultural transmission, similar patterns should be possible to detect in whale songs.

The study authors analyzed recorded humpback whale song data over eight years using infant-inspired speech segmentation techniques.

They discovered a hidden structure in the whale song.

Specifically, these songs contain statistically coherent subsequences that fit the Zipfian distribution.

Furthermore, the length of these subsequences follows ZIPF's Law of Suspicion, an efficiency-driven principle found in many species, including humans.

This striking similarity between the two evolutionarily distant species emphasizes the deep role of learning and cultural communication in shaping communication across species, with such structural properties being exclusive to human language. It challenges the concept of being.

“The Whale Songs” at Griffith University, Dr. Jenny Allen, a leading expert on whale songs, said:

“This is why it offers such an exciting comparison.”

“These results provide unique insight into the importance of cultural communication in interspecies learning processes, particularly for learning complex communication systems.”

“A more interesting question is, rather than trying to adapt animal communication to holes in the form of “human language”? I think so. ”

“Using insights and methods from how babies learn languages ​​allowed us to discover structures that were previously undetected in whale songs,” says Professor Inval Arnon of Hebrew University. Ta.

“This work illustrates how learning and cultural communication can form the structure of communication systems. Find similar statistical structures when complex continuous behaviors are culturally transmitted. You can do it.”

“It raises the interesting possibility that humpback whales can track the transition odds between sound elements, like human babies, and learn songs by using dips to segment those odds. Masu.”

study It was published in the journal today Science.

____

Invalanon et al. 2025. The whale song shows a language-like statistical structure. Science 387 (6734): 649-653; doi: 10.1126/science.adq7055

Source: www.sci.news

OpenAI to Shift to For-Profit Company Structure, Announces Transition Plans

OpenAI has announced plans to reorganize its corporate structure in the coming year, noting that it will establish a public benefit corporation to oversee its expanding operations and alleviate constraints imposed by its current nonprofit parent company.

Speculations are circulating about OpenAI’s transition to a commercial entity. Details of the proposal have now been revealed for the first time.

According to the proposed framework, a for-profit public interest corporation will manage OpenAI’s business activities, while a nonprofit entity will oversee the organization’s philanthropic endeavors in fields like healthcare, education, and science.

This new structure grants greater authority to OpenAI’s commercial division. The company stated in a blog post that it aims to create a “more robust nonprofit entity supported by the accomplishments of a for-profit entity.” OpenAI also mentioned that this setup will enable them to “secure the necessary funding” comparable to other companies in the industry.

Initially established as a nonprofit research-focused organization in 2015, OpenAI is the creator of the popular ChatGPT chatbot and is considered one of the most valuable startups globally.

In pursuit of artificial general intelligence (AGI), a form of AI surpassing human intellect, OpenAI has been exploring structural modifications over the past year to attract additional investment. The success of the latest $6.6 billion funding round (valuing the company at $157 billion) hinged on restructuring and eliminating profit restrictions for investors.

“Investors are willing to back us, but at this scale of capital, we no longer require traditional funding with extensive structural constraints,” stated OpenAI in a blog post.

Microsoft holds the largest stake in OpenAI at 49%, a situation that could become intricate if OpenAI transitions into a commercial entity. Investment banks have been engaged to facilitate the process and determine Microsoft’s future ownership stake in the reorganized OpenAI. As reported by the Wall Street Journal.

OpenAI’s competitors in the generative AI sector, including Anthropic and Elon Musk’s xAI, have adopted a similar public benefit corporation model. OpenAI believes that adopting this structure can enhance its competitiveness in the market.

“The substantial investment being made by leading companies in AI development underscores the level of commitment needed for OpenAI to advance its mission,” mentioned OpenAI in a blog post. “We once again find ourselves in need of raising more funds than we had anticipated.”

Source: www.theguardian.com

Unusual dental structure discovered in Triassic lizard-like quasi-reptile

Paleontologists have identified a new species of procolophonid reptile from fossilized skull and jaw fragments found in southwest England.

rebuilding the life of Treodatos casmatos. Image credit: Mark Whitton.

The newly discovered species Treodatos casmatoslived during the Late Triassic period, approximately 220 to 210 million years ago.

The ancient creature is a member of Leptopleuroninaean extinct lizard-like quasi-reptilian subfamily within the clade Procolophonidae.

Luke Mead, a palaeontologist at the University of Birmingham, said: “Procolophoids appeared in the late Permian, persisted until the end-Permian extinction event, and were a notable element of the post-extinction fauna in the Triassic, on the supercontinent. They were small quasi-reptile species that were diverse throughout Pangea.” his colleagues.

“Procolophonid diversity decreased during the Late Triassic and is represented only by the late-divergent clade Leptopleuroninae, known for small occurrences in Brazil, North America, Scotland, England, and possibly Wales. ”

“Leptopleuronin procolophorids typically have a reduced number of laterally expanded bicuspid maxillary teeth and are often characterized by cranial decorations such as enlarged spines of the quadrate zygoma.”

“Leptopleuronins appear to be well adapted to a high-fiber herbivore, omnivore, or entomovore diet, and this group may represent the latest surviving clade of Parareptilia.” There is.”

Fossilized remains are Treodatos casmatos It was discovered at Cromhall Quarry in southern Gloucestershire, south-west England.

“The teeth and jaws of this small reptile exhibit features never before seen in this group,” said Dr. Mead, lead author of the paper. study Published in a magazine Paleontology Papers.

“They probably fed differently than their relatives, raising new questions about how these animals interacted with their environment during the Late Triassic. ”

Reptiles have tricuspid teeth in their upper jaws, each with three distinct points. The lower jaw, on the other hand, has compressed unicuspid teeth with unusual edentulous (toothless) tips.

These adaptations may have facilitated unique methods of food processing.

Dr Mark Jones, curator of fossil reptiles at the Natural History Museum, said: “The interaction between the upper and lower teeth is interesting and there are some mammalian similarities in the shape of the teeth.”

“The mandible was not fused at the jaw area; instead, the connection was held by soft tissue and was probably flexible.”

“This flexibility may have allowed the lower jaws to make contact in a way that made it easier to masticate food.”

“This feature is not seen in closely related species and may indicate a specialized diet or feeding strategy.”

“The Late Triassic was a period of dramatic environmental change when Pangea began to collapse.”

“The unique adaptation of teeth is Treodatos casmatos This suggests that they may have carved out a unique ecological niche in a changing climate, feeding on plants, insects, or other small prey that required specialized oral food processing. ”

Treodatos casmatos “They lived at a time when solar radiation was much lower than it is today, but there was much more carbon dioxide in the atmosphere,” Dr. Jones said.

“It has become generally hotter, global average sea levels have risen, and extreme rainfall events have occurred.”

“therefore, Treodatos casmatos And the communities it lived in may provide perspective on today's threatened ecosystems and the global emergency we face. ”

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Luke E. Mead others. 2024. A new protocolophonid with complex tooth rows that lived in the Late Triassic of southwestern England. paleontology papers 10 (6): e1605;doi: 10.1002/spp2.1605

Source: www.sci.news

Neanderthal Hearth Structure Unearthed in Gibraltar Dating Back 65,000 Years

Archaeologists have announced the discovery of a new type of Neanderthal hearth in Gibraltar’s Vanguard Cave. This hearth structure is consistent with predictions from theoretical studies that require the use of heating structures to obtain birch tar commonly used in hafting. Researchers suggest that this hearth was used to burn herbs and shrubs over guano mixed with sand and heat rockrose without oxygen.

Neanderthal hearth structures may have been constructed according to the following steps: Image credit: Ochando others., doi: 10.1016/j.quascirev.2024.109025.

“The use and control of fire would have provided important adaptive benefits.” Homo and even shaped its evolution,” said Clive Finlayson of Gibraltar National Museum and colleagues.

“Manufacturing fire technology has been shown to be common from 400,000 years ago to the present, and it has probably been around for much longer.”

“A variety of studies have demonstrated the ability of Neanderthals to create, protect, and carry fire.”

“The main functions of the use of fire are related to providing heat, light and the possibility of cooking food.”

“But it could also lead to the development of new technological innovations,” they added.

“These include deliberate heat treatment of stone artifacts, durable wood, smoking purposes, and the use of distillation of birch bark and adhesives from coniferous resins to create stone flakes on wooden elements. This may include the production of hafting multi-component tools.”

“Other innovations by Neanderthals were the construction of pits and the diversification of the types of fuels used with a variety of commonly used plants, liquid hydrocarbons, and lignite.”

“However, plants are the most common type of fuel and are therefore expected to have been subject to a selection process by Neanderthals among available resources in the nearby, and perhaps even beyond, landscape.”

Special combustion structures discovered by the Vanguard Cave team have revealed previously unknown ways in which Neanderthals managed and used fire.

The structure is 68,000 to 61,000 years old and is adapted for steam distilling essential oils from rockrose to obtain tar, a hafting substance proven to have been used by Neanderthals.

The researchers tested that interpretation experimentally by building structures with similar morphological and compositional characteristics to those excavated in the cave.

Distilling a small bunch of young rockrose leaves in a closed, nearly anoxic environment for a reasonable period of time produces enough to hold two spearheads using only locally available tools and materials. of tar could be produced.

“Neanderthals had to go through a series of thought processes to choose which plants and find a way to extract the resin without burning them,” Dr Finlayson said.

“Our extinct cousins ​​were not the brutal humans of the popular imagination,” said Dr. Fernando Muñiz, an archaeologist at the University of Seville.

“This human species has been shown to have cognitive abilities, as reflected in studies showing mastery of the industrial process of making resin as an adhesive for attaching stone points to spear handles. ”

This finding is reported in the following article: paper in a diary Quaternary Science Review.

_____

Juan Ochando others. 2024. Neanderthals' special combustion structure adapted to the acquisition of tar. Quaternary Science Review 346: 109025;doi: 10.1016/j.quascirev.2024.109025

Source: www.sci.news

New study uncovers common, mysterious I motif structure in human genome DNA

The so-called i-motif is a knot-like DNA structure that forms in the nuclei of human cells and is thought to provide important genome control. Garvan Institute of Medical Research Other studies have used immunoprecipitation and next-generation sequencing to identify i-motif structures in human DNA.

Peña Martinez othersIn total, we observed 53,000 i-motifs across three human cell lines (MCF7, U2OS, and HEK293T). Image courtesy of Peña Martínez. others., doi: 10.1038/s44318-024-00210-5.

The I motif is a DNA structure that differs from the iconic double helix shape.

These form when runs of cytosine letters on the same DNA strand pair up with each other to form a four-stranded twisted structure that juts out from the double helix.

In 2018, scientists at the Garvan Institute of Medical Research were the first to successfully directly visualize i-motifs inside living human cells, using new antibody tools they developed to recognise and bind to the i-motifs.

The new study expands on these findings by using the antibody to identify the location of i-motifs throughout the genome.

“In this study, we have mapped more than 50,000 i-motif sites in the human genome that are found in all three cell types we looked at,” said Professor Daniel Crist from the Garvan Institute of Medical Research, lead author of the study.

“This is a surprisingly high number for a DNA structure whose presence in cells was once a matter of debate.”

“Our findings confirm that the i-motif is not just an object of laboratory study, but is widespread and likely plays an important role in genome function.”

The researchers found that i-motifs are not scattered randomly, but are concentrated in important functional regions of the genome, including those that control gene activity.

“We found that the i-motif is associated with genes that are highly active at specific times in the cell cycle,” said lead author Cristian David Peña Martinez, PhD, also of the Garvan Medical Institute.

“This suggests that it plays a dynamic role in regulating gene activity.”

“We also discovered that i-motifs are formed in the promoter regions of cancer genes. For example, MYC Oncogenes encode one of cancer’s most notoriously ‘untreatable’ targets.”

“This opens up exciting opportunities to target disease-related genes through i-motif structures.”

“The widespread presence of the i-motif near these 'holy grail' sequences implicated in hard-to-treat cancers opens up new possibilities for novel diagnostic and therapeutic approaches,” said study co-author Sarah Kummerfeld, PhD, a researcher at the Garvan Medical Institute.

“It may be possible to design drugs that target the i-motif to affect gene expression, potentially expanding current treatment options.”

Team result Published in EMBO Journal.

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Christian David Peña Martinez othersi-motif structures are widely distributed in human genomic DNA. Embo JPublished online August 29, 2024, doi: 10.1038/s44318-024-00210-5

Source: www.sci.news

Study finds ancient genome structure preserved in 52,000-year-old mammoth skin

Scientists from Baylor College of Medicine and other institutions have announced the discovery of ancient chromosome subfossils in a female mammoth fossil.Mammutus primigeniusThe mammoth, a species of mammoth known as the pygmy mammoth, died 52,000 years ago in what is now Siberia. The fossil preserves the structure of its ancient chromosomes down to the nanometer (billionth of a meter) scale. Researchers hypothesize that the cold of Siberia naturally freeze-dried the mammoth's skin, causing a glass transition that preserved the fossil.

Sandoval Velasco othersAssembled the genome and 3D chromosome structure of a 52,000-year-old woolly mammoth. Image courtesy of Sandoval Velasco. others., doi: 10.1016/j.cell.2024.06.002.

“This is a new type of fossil, one whose scale far exceeds that of individual ancient DNA fragments, with sequences a million times larger,” said Dr. Erez Lieberman Aiden, director of the Center for Genome Architecture at Baylor College of Medicine.

“This is also the first time that an ancient sample has been karyotyped.”

Knowing the three-dimensional structure of a genome gives us a lot of additional information beyond its sequence, but most ancient DNA specimens are made up of very small, jumbled up pieces of DNA.

Building on their work mapping the 3D structure of the human genome, Dr Aiden and his colleagues reasoned that the same strategy could be used to assemble ancient genomes, provided suitable ancient DNA samples were found.

The researchers tested dozens of samples over a five-year period, eventually locating an unusually well-preserved woolly mammoth that was unearthed in September 2018 near Belaya Gora, in the Sakha Republic in northeastern Siberia.

“We believe that the freeze-drying occurred naturally shortly after death, and the nuclear structures in the dried samples can remain viable for an incredibly long period of time,” said Dr. Olga Dudchenko of the Center for Genome Structure at Baylor College of Medicine.

To reconstruct the mammoth's genome structure, the authors extracted DNA from skin samples taken from behind the mammoth's ears.

They are, High C This allows them to detect which parts of DNA are in spatial proximity and likely to interact in their natural state within the nucleus.

“Imagine having a puzzle with 3 billion pieces, but not having the final puzzle picture at hand,” said Professor Marc-Marty-Renom, a structural genomicist at the National Center for Genome Analysis and Genomic Regulation.

“Hi-C allows me to get a rough idea of ​​what the picture looks like before I start putting the puzzle pieces together.”

They then combined the physical information from the Hi-C analysis with DNA sequences to identify interacting DNA sections and produced a neat map of the mammoth genome using the modern elephant genome as a template.

The analysis revealed that mammoths had 28 chromosomes, the same number as modern Asian and African elephants.

Remarkably, the fossilized mammoth chromosomes retained a great deal of physical integrity and detail, including the nanoscale loops that contact transcription factors with the genes they control.

By examining the compartmentalization of genes within the nucleus, the scientists were able to identify active and inactive genes in the mammoth skin cells, a proxy for epigenetics and transcriptomics.

Compared with skin cells from the mammoth's closest relative, the Asian elephant, the mammoth's skin cells showed different gene activation patterns, including genes that may be related to fur and cold tolerance.

“For the first time we have mammoth tissue where we can roughly tell which genes are on and which are off,” said Professor Martti Renom.

“This is a surprising new type of data, the first time we've measured cell-specific genetic activity of genes in ancient DNA samples.”

Team result Published in today's journal cell.

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Marcela Sandoval Velasco others2024. A 52,000-year-old mammoth skin sample contains 3D genome structure. cell 187(14):3541-3562; doi:10.1016/j.cell.2024.06.002

Source: www.sci.news

New Hubble Space Telescope Images Reveal Classic Spiral Structure in NGC 3810

Astronomers have used the NASA/ESA Hubble Space Telescope to create a stunningly detailed image of NGC 3810, a spiral galaxy hosting a supernova.

This Hubble Space Telescope image shows NGC 3810, a spiral galaxy about 50 million light-years away in the constellation Leo. The color image is composed of infrared, visible, and ultraviolet observations from both the Hubble Space Telescope's Advanced Camera for Surveys (ACS) and Wide Field Camera 3 (WFC3) instruments. Nine filters were used to sample different wavelengths. Color is achieved by assigning a different hue to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / D. Sand / RJ Foley.

NGC 3810 It is located in the constellation Leo, about 50 million light years from Earth.

Also known as IRAS 11383+1144, LEDA 36243 and UGC 6644, the galaxy has a diameter of 60,000 light years.

NGC 3810 discovered It was discovered on March 15, 1784 by German-born British astronomer William Herschel.

The galaxy belongs to a small group of galaxies called the NGC 3810 group.

The bright central region of NGC 3810 thought Many new stars are forming and outshining the outer regions of the galaxy by a significant amount.

Even more distant galaxies show surprisingly abundant dust clouds along their spiral arms.

Far from the center, hot, young blue stars appear in huge clusters, with bright red giants scattered throughout the arms.

In 2022, a Type Ia supernova event called SN 2022zut was observed in NGC 3810.

“In early 2023, the Hubble Space Telescope will focus on this and several other galaxies to take a closer look at recent Type Ia supernovae,” Hubble astronomers said in a statement.

“These types of supernovae are produced by the explosion of a white dwarf star, and all of them maintain a very stable brightness.”

“This allows us to measure distances. We know how bright a Type Ia supernova is, so we can tell from how faint it appears how far away it is.”

“One uncertainty with this method is that intergalactic dust between Earth and the supernova will block some of the light.”

“How do we know how much of the light reduction is due to distance and how much is due to dust?”

“With the help of Hubble, we have a clever workaround: we can image the same Type Ia supernova in ultraviolet light, which is almost completely blocked by the dust, and in infrared light, which passes through the dust almost unaffected.”

“By carefully recording how much light is transmitted at each wavelength, we can calibrate the relationship between the supernova's brightness and distance, and take dust into account.”

“Hubble can observe both of these wavelengths of light in incredible detail with the same instrument.”

“That makes it the perfect tool for this experiment. In fact, some of the data used to create this beautiful image of NGC 3810 was focused on the SN 2022zut supernova, which you can see as a point of light just below the galactic nucleus.”

Source: www.sci.news

Strange crystal structure reveals incredibly complex maze

Can you find your way out of the red center of the maze? Scroll down for the answer

University of Bristol

An algorithm designed to find the most efficient path from atom to atom in a strange kind of crystal turns out to create incredibly complex mazes. In addition to building mazes, the technique could also be useful for speeding up certain industrial chemical reactions.

The crystals in question are called quasicrystals because their atoms are arranged in a repeating fashion like normal crystals, but they exhibit more complex and unpredictable symmetries. Although such crystals have been synthesized in laboratories and were produced during the first nuclear weapon detonation in 1945, only one natural source has been found so far: a meteorite found in Russia in 1985.

“Quasicrystals have all the symmetries that normal crystals don’t have. [normal] The crystals are very interesting.” Felix Flicker Professor at the University of Bristol in the UK. “It’s a very beautiful area of mathematics, but you can appreciate that beauty directly without knowing the details.”

Fricker and his colleagues developed an algorithm to quickly generate paths that contact every atom in a quasicrystal exactly once. Diagrams of these paths form beautiful maze-like structures.

Creating such a pathway is known in computer science as an NP-complete problem, a problem that becomes exponentially more complicated as the number of atoms increases. These problems can quickly become virtually impossible to compute at large scales, but the researchers have found that in some quasicrystals the problem is unexpectedly simple.

“This was quite surprising, since this problem in general is known to be essentially unsolvable and, since these quasicrystals do not have translational symmetry, it did not seem to offer any obvious simplifications,” Fricker says.

The solution to the maze is marked in red

University of Bristol

Developing such a pathway, Fricker says, could be put to practical use in a laboratory technique called scanning tunneling microscopy, in which an extremely sharp tip is maneuvered over a material to sense individual atoms one by one, building up an atomic-level picture. Creating complex images, such as one of the quasicrystal itself, can take up to a month, but Fricker says that time could be cut in half if a more efficient pathway could be found to capture each atom.

Fricker also believes the technique could be used to create crystalline catalysts for industrial chemical processes that are more efficient than current methods, making certain compounds faster or less costly to produce. But Fricker thinks other uses may also become apparent over time. “I hope the most interesting uses will be ones that we haven’t even thought of.”

Physical Review X
DOI: In press

Source: www.newscientist.com

Enormous Stone Age hunting structure uncovered in the Baltic Sea

A team of German archaeologists has discovered a gigantic Stone Age structure submerged at a depth of 21 meters in the Western Baltic Sea. This structure was probably built by hunter-gatherers over 10,000 years ago and was eventually sunk about 8,500 years ago. Since then, it has remained hidden under the sea, leading to pristine preservation that has inspired research into lifestyles and territorial development in the wider region.

An artist's reconstruction of the Brinker Wall in Mecklenburg Bay, Germany. Image credit: Michał Grabowski.

The massive Stone Age structure was discovered in Mecklenburg Bay, about 10 kilometers northwest of the German coast of Relic.

The stone wall is made up of 1,673 individual stones, typically less than 1 meter in height, arranged side by side over a distance of 971 meters in a way that refutes their natural origin through glacial movement or ice-intrusion ridges.

This wall, known as the Brinker Wall, was built by hunter-gatherers who roamed the area after humans left. viserian ice sheet.

Running adjacent to the sunken shoreline of a paleo-lake (or swamp), whose youngest stage dates to 9,143 years ago, the structure was probably used for hunting. Eurasian reindeer (Langifer Tarandus).

“At that time, the population of all of Scandinavia was probably less than 5,000,” said Dr. Marcel Bradmeler, a researcher at the University of Rostock.

“One of their main food sources was herds of reindeer, which moved seasonally across sparsely vegetated post-glacial landscapes.”

“This wall was probably used to guide reindeer into the bottleneck between the adjacent shore and the wall, or into the lake, allowing Stone Age hunters to kill reindeer more easily with their weapons. Ta.”

Form of a southwest to northeast oriented ridge with a blinker wall and adjacent mounds.Image credit: Geersen et al. everyone, doi: 10.1073/pnas.2312008121.

The Brinker Wall is one of the oldest recorded man-made hunting structures on Earth and one of the largest known Stone Age structures in Europe.

Dr Jacob Geersen, also from the University of Rostock, said: “Our research shows that the natural origin of the submarine stone walls or modern constructions associated with, for example, the laying of submarine cables or stone extraction is unlikely. ” he said. .

“The orderly arrangement of many small stones connecting large, immovable rocks opposes this.”

The researchers used modern geophysical methods to create detailed 3D models of the Brinker Wall and reconstruct the ancient landscape.

A team of scientific divers from the University of Rostock and the West Pomeranian Mecklenburg State Department of Culture and Monuments also visited the site once and inspected it.

The main purpose of the dive was to assess the nature of the stone wall and investigate possible archaeological remains on the surrounding seabed.

They concentrated in two places: the western edge of the structure and the large stone in the center where the blinker wall turns.

No artifacts or dateable organic material were found in the immediate vicinity of the two dive sites, but a small wood sample was recovered from Holocene deposits approximately 10 m south of the structure.

3D model of the section of blinker wall adjacent to the large boulder at the west end of the wall. The photo was taken by Philip Huy of the University of Rostock. The scale bar at the top right corner of the image is 50 cm. Image credit: Geersen other., doi: 10.1073/pnas.2312008121.

“A number of well-preserved Stone Age sites are known along the coast of Wismar Bay and Mecklenburg-West Pomerania, but these are located at much shallower depths, and most of them are Mesolithic and Neolithic. It dates from the Stone Age (7,000-2,500 BC),” said Dr. Jens Auer, a researcher at the Mecklenburg-West Pomeranian Department for the Preservation of Cultural Monuments.

“There is evidence that similar stone walls exist in other parts of Mecklenburg Bay. These will also be investigated systematically,” added Dr. Jens Schneider von Daimling, a researcher at the University of Kiel.

“Overall, this research could make a significant contribution to understanding the lives, organization, and hunting methods of early Stone Age hunter-gatherers.”

team's paper Published in this week's Proceedings of the National Academy of Sciences.

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Jacob Giesen other. 2024. Submerged Stone Age hunting architecture in the Western Baltic Sea. PNAS 121 (8): e2312008121; doi: 10.1073/pnas.2312008121

Source: www.sci.news

Study reveals new organizational structure of water molecules on the surface of salt water

The distribution of ions at the air-water interface plays a decisive role in many natural processes. Some studies suggest that large ions tend to exhibit interfacial activity, suggesting that the ions sit above the water surface, thereby inducing an electric field that determines the interfacial water structure. But new research by chemists at the University of Cambridge and the Max Planck Institute for Polymer Research casts doubt on this view. Their results show that ions in typical electrolyte solutions are actually located in subsurface regions and that such interfaces stratify into two characteristic aqueous layers.

Littman other. They show that the ions and water molecules at the surface of most aqueous salt solutions, known as electrolyte solutions, are organized in a completely different way than previously understood.Image credit: Littmann other., doi: 10.1038/s41557-023-01416-6.

Many important reactions related to climate and environmental processes occur where water molecules come into contact with air.

For example, ocean water evaporation plays an important role in atmospheric chemistry and climate science.

Understanding these responses is critical to efforts to reduce human impact on the planet.

The distribution of ions at the air-water interface can influence atmospheric processes. However, accurately understanding the microscopic reactions at these important interfaces has been hotly debated.

Dr. Yair Littman of the University of Cambridge and his colleagues set out to study how water molecules are affected by the distribution of ions at the very point where air and water meet.

Traditionally, this has been done with a technique called oscillatory sum frequency generation (VSFG).

Using this laser irradiation technique, it is possible to directly measure molecular vibrations at these key interfaces.

However, while the strength of the signal can be measured, this technique does not measure whether the signal is positive or negative, which has previously made the results difficult to interpret. Furthermore, using only experimental data can lead to ambiguous results.

The authors overcame these challenges by utilizing a more sophisticated form of VSFG, called heterodyne detection (HD)-VSFG, to study different electrolyte solutions.

We then developed sophisticated computer models to simulate the interface in various scenarios.

The combined results showed that both positively charged ions, called cations, and negatively charged ions, called anions, are depleted from the water-air interface.

The cations and anions of simple electrolytes orient water molecules both upward and downward.

This is a reversal of the textbook model that teaches that ions form an electric double layer, orienting water molecules in only one direction.

“Our study shows that the surface of a simple electrolyte solution has a different ion distribution than previously thought, and that the ion-rich subsurface determines the composition of the interface. .At the top you have a few layers of pure water, then you have the ions, the “dense layer,'' and finally the bulk salt solution,'' Dr. Littman said.

“Our paper shows that combining high-level HD-VSFG with simulation is a valuable tool that contributes to the molecular-level understanding of liquid interfaces,” said Max Planck Institute for Polymer Research researchers said Dr. Kuo-Yang Chiang. .

“These kinds of interfaces exist everywhere on Earth, and studying them not only helps our fundamental understanding, but can also lead to the development of better devices and technologies.” said Professor Misha Bonn, also of the Max Planck Institute for Polymer Research.

“We are applying these same methods to study solid/liquid interfaces, which could have applications in batteries and energy storage.”

of study It was published in the magazine natural chemistry.

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Y. Littman other. Surface stratification determines the structure of interfacial water in simple electrolyte solutions. nut.chemistry, published online on January 15, 2024. doi: 10.1038/s41557-023-01416-6

Source: www.sci.news

Hidden Secrets of Atomic Structure Uncovered by Scientists

Groundbreaking research led by Professor Motoki Shiga has unraveled the complex atomic structure of glass, revealing its unique patterns and anisotropy. This research paves the way for advanced exploration of glass materials using AI and machine learning techniques.Credit: Motoki Shiga

Glass is an essential material in our daily life and serves a variety of purposes, such as insulating our homes and forming the screens of our computers and smartphones. However, its widespread historical use stands in contrast to the scientific mystery posed by its disordered atomic structure. This puzzling arrangement of atoms complicates efforts to fully understand and manipulate the structural properties of glasses. Therefore, designing effective functional materials from glass remains a difficult challenge for scientists.

Advances in glass research

To further elucidate the structural regularities hidden in glassy materials, the research group focused on the ring shape of the chemically bonded glass network. A research group including Professor Motoki Shiga of Tohoku University’s unprecedented scale data analysis center has developed a new method to quantify the three-dimensional structure of the ring and the symmetry of the structure, “roundness” and “roughness.”

Spatial atomic density around rings of silica crystal (left) and glass (right). Blue and red regions indicate areas with high density of silicon and oxygen atoms, respectively.Credit: Motoki Shiga et al.

Breakthroughs and future directions

“Structural units and structural order beyond chemical bonds have long been inferred through experimental observations, but until now scientists have avoided identifying them,” Professor Shiga says. “Furthermore, our successful analysis contributes to the understanding of phase transitions such as vitrification and crystallization in materials and provides the necessary mathematical explanations to control the structure and material properties of materials.”

Looking to the future, Shiga and his colleagues plan to use these techniques to devise procedures for exploring glass materials, procedures based on data-driven approaches such as: machine learning And AI.

Reference: “Ring-derived anisotropy of local structural order in amorphous and crystalline silicon dioxide” by Motoki Shiga, Akihiko Hirata, Yohei Onodera, and Hirokazu Masai, November 3, 2023. Communication materials.
DOI: 10.1038/s43246-023-00416-w

Source: scitechdaily.com

Unveiling the Structure of Neurotransmitter Transporters: Scientists Finally Answer 40-Year-Old Question

Researchers at St. Jude Children’s Research Hospital have uncovered the structure of VMAT2, a crucial neurotransmitter transporter, shedding light on its interaction with drugs used to treat conditions like Tourette syndrome. This pioneering study offers insights into neurotransmitter transport and advances the field of neuropharmacology.

Neurons communicate through neurotransmitters, and experts at St. Jude Children’s Research Hospital have utilized their knowledge in structural biology to reveal the structure of vesicular monoamine transporter 2 (VMAT2), an essential component of neurotransmission.

By visualizing VMAT2 in different states, researchers can now better comprehend its function and how its different conformations impact drug binding. This knowledge is crucial for the development of drugs to treat hyperactivity disorders such as Tourette syndrome.

This work was recently published in the journal Nature. Monoamines, including dopamine, serotonin, and adrenaline, play a central role in neurotransmission by influencing various brain functions. Before they can be released, these molecules must be packaged into vesicles, which are compartments in cells that store neurotransmitters.

VMAT2 is a protein that moves monoamines into these vesicles, acting like a loading crane on a cargo ship. The study, led by researchers such as Dr. Chia-Hsueh Lee, Dr. Shabareesh Pidathala, and Dr. Yaxin Dai, utilized cryo-electron microscopy to analyze the structure of VMAT2 and its interactions with serotonin and drugs used to treat certain conditions.

The study revealed that different drugs bind to specific conformations of VMAT2, providing detailed insights that can aid in developing treatments for various disorders. The research also identified amino acids that facilitate neurotransmitter transport, laying the groundwork for future studies to fully understand the mechanisms involved.

The study was supported by grants from organizations such as the National Institutes of Health and the National Natural Science Foundation of China.

Source: scitechdaily.com

Unprecedented Level of Internal Structure Exposed by Groundbreaking Human Brain ‘Atlas’

Global collaboration has led to the creation of the world’s most comprehensive primate brain atlas, consisting of 4.2 million cells. This atlas has provided insights into region-specific functions, associations with neurological diseases, and has guided future brain research and disease intervention. The project aims to explore the evolution of the human brain and discover new targets for disease treatment. The initiative, known as the “Brain Initiative Cell Census Network” project by the National Institutes of Health, has been working towards mapping the cell groups and understanding their functions for over 21 years. The recent breakthrough discovery has allowed scientists to gain a deeper understanding of the brain and the medical mysteries behind disorders such as autism and depression. The research team, led by scientists from Arizona State University, the University of Pennsylvania, the University of Washington, and the Brotman Beatty Institute, created the largest atlas of the primate brain to date. The atlas consists of profiles of over 4 million cells, providing valuable information on the evolution of human cognition and behavior, as well as the occurrence of neurological diseases. The data collected has been made publicly available for the scientific community and the general public. The research team utilized state-of-the-art single-cell techniques and analyzed gene expression and DNA regulatory regions to identify molecularly distinct brain cell types and their functional characteristics. They also investigated the genetic architecture of neurological disease risk at the cellular level. The atlas serves as a crucial resource for further research on the human brain and potential interventions for neurological diseases.

Source: scitechdaily.com