Category: 7. Science

  • Whispers in the womb: How cells “hear” to shape the human body

    Whispers in the womb: How cells “hear” to shape the human body

    Like all complex organisms, every human originates from a single cell that multiplies through countless cell divisions. Thousands of cells coordinate, move and exert mechanical forces on each other as an embryo takes shape. Researchers at the Göttingen Campus Institute for Dynamics of Biological Networks (CIDBN), the Max Planck Institute for Dynamics and Self-Organisation, and the University of Marburg have now discovered a new way that embryonic cells coordinate their behavior. This involves molecular mechanisms previously known only from the process of hearing. The researchers attribute the fact that such different cells use the same proteins for two such different functions to their evolutionary origin. The results were published in Current Biology.

    The interdisciplinary research team used an unusual combination of methods from developmental genetics, brain research, hearing research and theoretical physics to make a surprising discovery in cell communication: they found that in thin layers of skin, cells register the movements of their neighboring cells and synchronize their own tiny movements with those of the others. Groups of neighboring cells thus pull together with greater force. Thanks to their high sensitivity, the cells coordinate very quickly and flexibly as these subtle forces are the fastest signals traveling across embryonic tissue. When the cells were genetically deprived of their ability to “listen” to each other, the entire tissue changed and development was delayed or failed altogether.

    The researchers integrated cellular coordination into computer models of the tissue . These models showed that the “whispering” among neighboring cells leads to an interwoven choreography of the entire tissue and protects it from external forces. Both effects were confirmed by video recordings of embryonic development and further experiments. “Using AI methods and computer-assisted analysis, we were able to examine about a hundred times more cell pairs than was previously possible in this field,” explains Dr Matthias Häring, group leader at the CIDBN and co-author of the study. “This big data approach gives our results the high level of accuracy needed to reliably get to the bottom of these delicate interactions between cells.”

    The mechanisms revealed here in embryonic development were already known to play a role in the process of hearing. For instance, when very quiet sounds are heard, the hair cells in the ear, which convert sound waves into nerve signals, react to tiny mechanical movements. At the threshold of hearing, the cell protrusions bend over distances of only a few atomic diameters. The ear is so sensitive because of special proteins that convert mechanical forces into electrical currents. Until now, almost no one suspected that such sensors of force also play an important role in embryonic development. In principle, this is possible because every cell in the body carries the genetic blueprints for all proteins and may use them as needed.

    The phenomenon could also provide insights into how the perception of force at a cellular level has evolved. “The evolutionary origin of these force-sensitive ion channel proteins probably lies in our single-celled ancestors, that we share with fungi and which emerged long before the origin of animal life,” explains Professor Fred Wolf, Director of the CIDBN and co-author of the study. “But it was only with the evolution of the first animals that the current diversity of this protein type emerged.” Future work should determine whether the original function of these cellular “nanomachines” was to perceive forces inside the body rather than, as in hearing, to perceive the outside world.

    Continue Reading

  • Ancient wooden tools uncovered in China shed new light on early human diet, cognitive abilities – The Jerusalem Post

    1. Ancient wooden tools uncovered in China shed new light on early human diet, cognitive abilities  The Jerusalem Post
    2. 361,000-year-old discovery in China: Oldest wooden tools shake up archaeology  Interesting Engineering
    3. Top Comments: Early Humans Ate Vegetables  Daily Kos
    4. Did Denisovans or Homo erectus make the oldest wooden tools in East Asia?  Ars Technica
    5. Rare wooden tools from Stone Age China reveal plant-based lifestyle of ancient lakeside humans  The Conversation

    Continue Reading

  • “We Got It All Wrong”: New Study Reveals Dinosaur Speeds Were Vastly Overestimated by Decades of Fossil Trackway Data

    “We Got It All Wrong”: New Study Reveals Dinosaur Speeds Were Vastly Overestimated by Decades of Fossil Trackway Data

    IN A NUTSHELL
    • 🦖 Fossil trackways have been crucial in studying dinosaur locomotion, but new research suggests they’ve led to overestimations of speed.
    • 🔍 Researchers at Liverpool John Moores University analyzed modern birds, specifically helmeted guineafowl, to understand how muddy substrates affect trackway interpretations.
    • 📉 Findings indicate that previous calculations of dinosaur speed, based on Alexander’s formula, may be significantly overstated when applied to soft surfaces.
    • 🧩 The study calls for more comprehensive research to refine our understanding of dinosaur movement, urging caution in speed-based behavioral reconstructions.

    The fascinating world of dinosaurs has always captured our imagination, painting vivid pictures of these magnificent creatures roaming the Earth. Recent research challenges some of our long-held beliefs about dinosaur speed. A study from Liverpool John Moores University provides new insights into how these ancient giants might have moved. By analyzing fossil trackways and comparing them with modern birds, scientists have unveiled surprising findings about dinosaur locomotion that could reshape our understanding of their behavior and lifestyle.

    Fossil Trackways: A Window into Dinosaur Movement

    Fossil trackways have long been a vital tool in understanding the behavior and locomotion of extinct animals. These preserved footprints offer a glimpse into how dinosaurs might have moved across varied landscapes. However, new research suggests that our previous interpretations of these trackways might have been flawed. Traditionally, calculations of dinosaur speeds were based on equations derived from mammalian data. This approach failed to account for the unique conditions under which these tracks were made.

    The Liverpool research team focused on theropods, one of the three major dinosaur groups. They discovered that trackways made in soft, muddied surfaces could significantly distort recorded speeds. In fact, the original equation by R. McNeill Alexander, used for decades to estimate dinosaur speed, was based on data from living animals moving on hard surfaces. The study reveals that speeds calculated from trackways on softer substrates might be dramatically overestimated.

    James Webb Telescope Unlocks the Deep Structural Secrets of Disk Galaxies, Revealing How the Universe Built Its Greatest Shapes

    Modern Birds Reveal the Secrets of Dinosaur Locomotion

    To test their hypothesis, researchers turned to modern birds, specifically the helmeted guineafowl. This bird was chosen because of its similarities to non-avian theropods like Velociraptor. By observing the guineafowl moving across different types of mud, scientists gained valuable insights into how substrate consistency affects trackway formation and perceived speed.

    High-speed video recordings of the guineafowl’s movements provided a wealth of data. The researchers found that the bird’s trackways, when analyzed using Alexander’s formula, significantly overstated their actual speed. This finding suggests that many dinosaur trackways might have been misinterpreted, leading to erroneous conclusions about their pace and behavior. The study emphasizes the need to consider the substrate’s role in trackway analysis, which could lead to more accurate reconstructions of dinosaur movement.

    “We’re Finally Hunting Aliens for Real”: James Webb Telescope Begins Deep-Space Search for Signs of Extraterrestrial Life

    Reconsidering Dinosaur Speeds and Behavior

    The implications of this research are far-reaching. If dinosaur speeds have been overestimated, it could alter our understanding of their behavior, including predator-prey dynamics and migration patterns. For example, a theropod trackway previously thought to indicate running might actually represent a walking pace. Similarly, a large ornithopod moving leisurely could have been mistakenly classified as running.

    This new perspective encourages scientists to reassess previous speed-based behavioral reconstructions. The research suggests that while some dinosaurs likely did run, the speeds at which they did so might have been much slower than previously believed. The team advocates for using trackway data to make broad comparisons of relative speeds rather than specific velocity estimates. This approach could lead to a more nuanced understanding of dinosaur ecology and their interactions with the environment.

    “Earthquake Moves in Slow Motion”: Scientists Capture Rare Seismic Event Crawling Miles Over Weeks Beneath Earth’s Surface

    The Future of Dinosaur Locomotion Studies

    While this study sheds new light on dinosaur locomotion, it also highlights the limitations of current research methods. The researchers acknowledge that their guineafowl model might not fully represent the dynamics of larger dinosaurs moving on different substrates. They call for further studies across a range of body sizes and sediment types to refine our understanding of dinosaur movement.

    Without additional research on modern animals moving on compliant substrates, calculating precise speeds from fossil trackways remains challenging. The study concludes with a call for more comprehensive investigations, emphasizing the importance of integrating data from extant taxa to enhance our interpretations of extinct species. Such efforts could pave the way for more accurate reconstructions of dinosaur locomotion and contribute to our broader understanding of ancient ecosystems.

    As we continue to unravel the mysteries of these ancient creatures, one thing remains certain: our quest to understand dinosaurs is far from over. This study is a reminder that science is ever-evolving, and each new discovery brings us closer to the truth. How will future research reshape our perception of these magnificent giants? What other surprises lie hidden in the fossil record, waiting to be uncovered?

    Our author used artificial intelligence to enhance this article.

    Did you like it? 4.4/5 (25)

    Continue Reading

  • Why does Mars show shades of yellow, orange in ESA’s dramatic new satellite image?

    Why does Mars show shades of yellow, orange in ESA’s dramatic new satellite image?



    The image shows planet Mars. — ESA/File

    Mars is commonly known as the Red Planet, but a recent satellite image from the European Space Agency (ESA) displays a vibrant blend of yellows, oranges, and browns. The striking view also highlights an impact crater and four dust devils moving across the terrain.

    Taken by the high-resolution camera on ESA’s Mars Express orbiter, the image features Arcadia Planitia — a key region for understanding Mars’ geological past and assessing its potential for future human habitation, reported Space.com.

    Located northwest of the solar system’s tallest volcanoes, Arcadia Planitia is notable for its ancient solidified lava flows, estimated to be up to 3 billion years old. Scientists also believe the area contains water ice just beneath the surface, making it a key target for upcoming Mars missions, according to ESA.

    The region frequently hosts “dust devils,” which are short-lived, whirlwind-like phenomena formed when warm surface air rises and lifts dust. In the image, four dust devils appear as faint white streaks, crossing from the darker to lighter regions of the plain.

    In the lower right corner of the photo, a large impact crater measuring about 9 miles (15 kilometres) wide is visible. The layered patterns surrounding the crater suggest that the ground contained significant water ice at the time of impact. The crater’s relatively intact appearance also indicates it formed recently in geological terms.

    Continue Reading

  • Phenomenal ‘lobster-like creatures’ discovered more than 1,500 feet into Antarctic ice

    Phenomenal ‘lobster-like creatures’ discovered more than 1,500 feet into Antarctic ice

    Scientists have made an astonishing discovery after finding lobster-like creatures beneath the depths of the Antarctic ice.

    It’s hard to comprehend how any living creature can survive freezing cold temperatures, but after drilling more than half a mile below the surface of an ice sheet, experts found an unexpected slow-moving river where animals are living.

    The subglacial river has been hidden for millennia but was uncovered during a recent expedition. Researchers drilled over 1,600 feet into the West Antarctic Ice Sheet, where they found the river below the Ross Ice Shelf.

    The river is about as deep as a 30-story building and is a blend of both fresh and seawater, and is slowly travelling towards the ocean.

    Expedition leader Huw Horgan explained: “We struck water at the end of the borehole and with the help of our camera, we even discovered a school of lobster-like creatures — 400 kilometres from the open ocean.”

      Craig Stevens

    Researchers believe that the river swells around once every decade – this occurs when nearby lakes drain into it. It’s thought the surges in the river could be causing an acceleration of ice melt as it carves out channels in the ice, moving around nutrients that help to sustain life.

    The discovery is an important one in terms of our understanding of ice melt and sea level rise.

    Experts fear that subglacial rivers such as this may be thinning glaciers from the bottom up, which may make it easier for land-based ice to get into the ocean and speed up sea-level rise, which may increase the risk of flooding in extreme weather and put pressure on food systems.

    Why not read…

    Mutated tribe can swim to bottom of ocean after developing ‘sea nomad gene’

    1,800-year-old tomb discovered with rare treasure inside

    ‘World’s oldest pyramid’ built 25,000 years ago was not made by humans, archaeologists claim

    Sign up for our free Indy100 weekly newsletter

    How to join the indy100’s free WhatsApp channel

    Have your say in our news democracy. Click the upvote icon at the top of the page to help raise this article through the indy100 rankings

    Continue Reading

  • Fossils in Sahara Desert reveal whales once had feet and toes

    Fossils in Sahara Desert reveal whales once had feet and toes

    A picture taken on January 14, 2015 shows fossil of a marine organism at the Wadi Al-Hitan Fossile and Climate Change Museum neara Cairo, Egypt.  —AFP 

    A desert site in Egypt known as Whale Valley, or Wadi Al-Hitan, holds more than 400 fossilised whale skeletons that show the remarkable evolutionary journey of whales from land to sea, Live Science reported.

    The site, located in the Egyptian Sahara, contains primitive whale remains dating back to the late Eocene epoch — between 55.8 million and 33.9 million years ago — when the area was submerged under the Tethys Ocean, according to UNESCO.

    “These fossils represent one of the major stories of evolution: the emergence of the whale as an ocean-going mammal from a previous life as a land-based animal,” UNESCO’s website states.

    The first major discovery at Whale Valley came in 1902, when paleontologists unearthed a previously unknown whale species, Basilosaurus isis (formerly Zeuglodon isis). This ancient whale grew up to 60 feet (18 metres) long and likely preyed on smaller whales, crushing their skulls before swallowing them whole, according to a 2019 study.

    General view of the natural reserve area of Wadi Al-Hitan, taken on January 14, 2016. — Reuters
    General view of the natural reserve area of Wadi Al-Hitan, taken on January 14, 2016. — Reuters

    “B. isis had a long snout and was armed with pointed incisors and sharp cheek teeth,” Manja Voss, a marine mammal expert at the Berlin Museum of Natural History and lead author of the 2019 study.

    In 1989, a team from the University of Michigan and the Egyptian Geological Museum discovered B. isis fossils with preserved hind limbs, feet and toes — a rare find that confirms whales once had legs, according to a 2023 review. Though modern whales lack hind limbs, they retain pelvic bones, indicating their terrestrial ancestry, University of Hawaii researchers noted.

    In 2005, a near-complete B. isis skeleton led UNESCO to declare Whale Valley a World Heritage Site. Since then, more marine fossils have been found, including ancient turtles, sharks, rays, sea cows, and crocodiles, preserved thanks to the area’s arid climate since the Pliocene.

    The site now functions as an open-air museum with ongoing research and strict protection.


    Continue Reading

  • Why does Mars appear yellow, orange in ESA striking new satellite image?

    Why does Mars appear yellow, orange in ESA striking new satellite image?

    Image of Mars captured by the ESA. — ESA/File

    Mars is often called the Red Planet, but a new satellite image from the European Space Agency (ESA) reveals a mix of swirling yellows, oranges, and browns. The colourful landscape also features an impact crater and four dust devils sweeping across the surface.

    Captured by the high-resolution camera aboard ESA’s Mars Express orbiter, the image showcases Arcadia Planitia — a region crucial to studying Mars’ history and its suitability for future human exploration, reported Space.com.

    Located northwest of the solar system’s tallest volcanoes, Arcadia Planitia is notable for its ancient solidified lava flows, estimated to be up to 3 billion years old. Scientists also believe the area contains water ice just beneath the surface, making it a key target for upcoming Mars missions, according to ESA.

    The region frequently hosts “dust devils,” which are short-lived, whirlwind-like phenomena formed when warm surface air rises and lifts dust. In the image, four dust devils appear as faint white streaks, crossing from the darker to lighter regions of the plain.

    In the lower right corner of the photo, a large impact crater measuring about 9 miles (15 kilometres) wide is visible. The layered patterns surrounding the crater suggest that the ground contained significant water ice at the time of impact. The crater’s relatively intact appearance also indicates it formed recently in geological terms.


    Continue Reading

  • Scientists discover a ‘second Earth’ twice the size of our planet near a red dwarf star, 154 light-years away |

    Scientists discover a ‘second Earth’ twice the size of our planet near a red dwarf star, 154 light-years away |

    In a significant step forward in the search for distant worlds, astronomers have discovered TOI-1846 b, a newly identified super-Earth exoplanet that may be rich in water. Located just 154 light-years away, this planet is nearly twice the size of Earth and orbits a cool red dwarf star. Though not considered habitable due to its high temperatures, TOI-1846 b’s dense, water-rich composition and close orbit offer valuable insights into the formation and evolution of rocky planets beyond our solar system. The discovery was made using data from NASA’s Transiting Exoplanet Survey Satellite (TESS) and confirmed with advanced ground-based observations. This planet adds to the growing catalogue of super-Earths that continue to reshape our understanding of planetary diversity in the galaxy.

    New super-Earth discovered orbiting red dwarf just 154 light-years away

    The new water-rich exoplanet, nearly twice the size of Earth, is orbiting a red dwarf star 154 light-years away. Named TOI-1846 b, this super-Earth may offer insights into the formation and evolution of rocky planets beyond our solar system. The discovery, detailed in a recent study published on the arXiv preprint server, was led by Abderahmane Soubkiou and his team at the Oukaimeden Observatory in Morocco.The planet was initially detected through NASA’s Transiting Exoplanet Survey Satellite (TESS) and later confirmed using a combination of ground-based photometry, high-resolution imaging, and spectroscopy.

    TOI-1846 b: A water-rich super-Earth with extreme heat and close orbit

    According to the reports, TOI-1846 b has a radius of approximately 1.792 times that of Earth and is about 4.4 times more massive. It orbits its host star once every 3.93 days, indicating an extremely close and swift orbit. The planet’s equilibrium temperature is estimated at 568.1 Kelvin (roughly 295°C), ruling out the possibility of surface habitability under known Earth-like conditions.Despite its high temperature, its size and density suggest a potentially water-rich composition, making it of interest to exoplanet researchers. This characteristic positions it among a growing class of rocky exoplanets that may contain substantial water content, possibly beneath thick atmospheres or layered beneath rocky crusts.

    How astronomers confirmed TOI-1846 b as a genuine super-Earth

    To validate the planet’s existence, the team relied on a robust set of techniques:

    • TESS data captured the planet’s transits.
    • Ground-based multicolor photometry helped refine its radius and orbital data.
    • High-resolution imaging and spectroscopy confirmed that the transit signal was planetary in nature and not a false positive.

    These observations collectively confirmed that TOI-1846 b is a genuine super-Earth, orbiting a relatively small and cool red dwarf star.

    TOI-1846 b faces atmospheric study challenges due to low TSM score

    Researchers assessed the planet’s Transmission Spectroscopy Metric (TSM) — a measure of how suitable a planet is for atmospheric study. TOI-1846 b scored a TSM of 47, which falls below the benchmark value of 90 typically used for sub-Neptune-sized planets. This suggests that its atmosphere may be challenging to analyze with current instruments.However, astronomers still consider TOI-1846 b a compelling candidate for future study, especially using radial velocity (RV) methods with high-precision instruments like MAROON-X. These observations could help refine its mass and reveal its internal structure and water content.

    TOI-1846 b vs HD 20794 d: How super-Earths differ in habitability and structure

    TOI-1846 b joins a growing catalog of recently discovered super-Earth exoplanets. For instance, earlier in 2025, astronomers identified HD 20794 d, a planet located just 20 light-years away, with a mass nearly six times that of Earth. Unlike TOI-1846 b, HD 20794 d lies within its star’s habitable zone, although its elliptical orbit may complicate the possibility of stable surface water.While TOI-1846 b is too hot to support life, it remains a valuable case study for astronomers seeking to understand planetary composition, water retention, and the atmospheric evolution of rocky worlds.

    What TOI-1846 b could reveal about water-rich exoplanets

    Though not habitable, TOI-1846 b’s possible water-rich interior, proximity to Earth, and detailed observational data make it a key object of interest. As telescope technology improves, particularly with next-gen observatories like the James Webb Space Telescope (JWST) and upcoming ground-based extremely large telescopes (ELTs), TOI-1846 b could play a role in shaping future models of planetary formation and composition.

    About the star orbiting around TOI-1846

    The star around which TOI-1846 b orbits is a red dwarf, with just 42% the mass of our Sun and approximately 0.4 solar radii. It is estimated to be around 7.2 billion years old, making it older than the Sun. Its relatively cool effective temperature of 3,568 K is characteristic of low-mass stars, which are known to have long lifespans and stable radiation output — ideal for exoplanet detection missions.Also Read | Is your brain 15 seconds behind? Study reveals you’re seeing the past, not the present


    Continue Reading

  • Astronomers Stunned by Dancing Planets Discovery

    Astronomers Stunned by Dancing Planets Discovery

    An international research team led by the University of Southern Queensland (UniSQ) has discovered two new planets performing a cosmic tango – orbiting their star in perfect rhythm.

    The findings, published in Nature Astronomy, reveal the two giant planets appear to be “dancing” around KOI-134, an F-type star 3,500 light-years from Earth.

    The remarkable discovery is the first planetary system of its kind ever found.

    The planets – dubbed KOI-134 b and KOI-134 c – are locked into a 2:1 orbital resonance, meaning the inner planet, KOI-134 c, completes two full orbits for every single orbit of the outer planet.

    What makes the system even more intriguing is that, unlike the planets in our Solar System, the giants don’t share the same orbital plane – they are tilted about 15 degrees relative to each other.

    Emma Nabbie, a UniSQ PhD student and lead author of the new research, said the discovery challenges long-held theories on planet formation.

    “The two planets are linked in a rhythmic orbit – drifting apart, then slowly coming back together, like dancers weaving around each other on a cosmic stage,” Ms Nabbie said.

    “While their orbital planes tilt back and forth over time, the gravitational pull from KOI-134 c causes KOI-134 b’s orbital period to shift by up to a day – speeding up and slowing down as the faster-orbiting KOI-134 c overtakes it from the inside.

    “This is the first time a system with such strong gravitational interactions and misaligned orbits has been observed – presenting a major puzzle for planet formation theories, as none currently explain how a system like this could form.”

    Using four years of data from the Kepler Space Telescope, the researchers discovered KOI-134 b to be a giant roughly the size of Jupiter and KOI-134 c to be slightly smaller than Saturn.

    KOI-134 c is considered an ‘invisible planet’ because it doesn’t pass in front of its host star, which makes it difficult for scientists to spot its presence using traditional detection methods.

    “The only way we could determine its mass was through its gravitational effect on KOI-134 b,” Ms Nabbie said.

    “KOI-134 b’s average orbital period is about 67 days – but it can vary between 66 and 68 days due to the gravitational influence of KOI-134 c.

    “That’s a remarkably large effect for a planet so close to its star. The variation was so extreme that it was initially denied to be a planet by the Kepler team.

    “If we scaled this to Earth’s orbit, it would be like our year fluctuating between 360 and 370 days.”

    As far as the researchers could tell, KOI-134 b and KOI-134 c are the only two planets orbiting KOI-134, which was first observed by NASA’s Kepler mission in 2009.

    The study, ‘A high mutual inclination system around KOI-134 revealed by transit timing variations’, was co-authored by Emma Nabbie, Professor Robert Wittenmyer, Dr Chelsea Huang, Associate Professor George Zhou and Alexander Venner from UniSQ and researchers from Lund University, University of Geneva, University of La Laguna, Chinese Academy of Sciences, Harvard and Smithsonian, Georgia Institute of Technology, University of California and Tsinghua University.

    /Public Release. This material from the originating organization/author(s) might be of the point-in-time nature, and edited for clarity, style and length. Mirage.News does not take institutional positions or sides, and all views, positions, and conclusions expressed herein are solely those of the author(s).View in full here.

    Continue Reading

  • Starwatch: Venus will pass through the ‘golden gate’ of two star clusters | Astronomy

    Starwatch: Venus will pass through the ‘golden gate’ of two star clusters | Astronomy

    This week, Venus will pass through the so-called Golden Gate of the Ecliptic. Although the name has risen to prominence with science popularisers in recent decades, its exact origin is unknown.

    It references two star clusters in the constellation Taurus, the Bull. The Hydes and the Pleiades lie on either side of the ecliptic, which is the plane of the solar system. As such, the sun, the moon and the planets all follow this line in their passage through the sky. The constellations the ecliptic passes through are known as the zodiacal constellations, referred to in popular culture as the signs of the zodiac.

    The chart shows the view looking east-north-east from London at 3.30am BST in the pre-dawn twilight of 8 July 2025. On this day, Venus will be approaching the “gate”. On subsequent mornings, the brilliant planet will move across the invisible line between the two clusters and on 12 and 13 July, it will clip the top of the Hyades star cluster, appearing 3 degrees away from the star Aldebaran.

    Venus will be a brilliant white beacon in the morning sky, contrasting with the blood-red light from Aldebaran, which represents the eye of the bull.

    The conjunction will also be easily visible from the southern hemisphere.

    Continue Reading