Category: 7. Science

  • Pollen Substitute Could Safeguard Honeybees and Global Food Security

    Honeybee populations have been steadily declining over the recent decades, facing unprecedented challenges such as habitat loss changing weather patterns, intensive farming patterns, air pollution and excessive use of pesticides. The rapid decline threatens not only bee populations but global food security, according to the Food and Agriculture Organisation (FAO) of the United Nations, a third of the world’s food production depends on bees.

    Until now, pollen substitutes have fallen short of providing honeybees with all the nutrients they need to healthily survive. Scientists at Oxford have developed a new supplement using a genetically modified yeast, Yarrowia lipolytica. This yeast produces essential nutrients called sterols, which are naturally found in pollen but missing from the conventional supplements beekeepers provide, typically made from protein flour, sugar, and oils. 

    Based on the researchers’ findings the honeybee colonies that were fed a diet enriched with Yarrowia lipolytica had 15 times more baby bees that made it to adulthood in comparison to those given diets without the nutrients. “When the bees have a complete nutrition they should be healthier and less susceptible to disease,” Professor Geraldine Wright said to the BBC. The researchers say the supplement could be available to farmers within two years potentially reducing competition between bee species for natural floral resources and helping population growth. 

    In the meantime, there is a lot to be done to continue supporting bees such as planting diverse wildflowers, reducing pesticide usage, preserving natural habitats, and promoting sustainable farming. By creating nutrient-rich foraging areas, honeybees and other pollinators can thrive, helping to maintain resilient ecosystems and the secure global food production in the face of climate change. 

    Read the full article here: https://www.nature.com/articles/s41586-025-09431-y  

    Continue Reading

  • Astronomers discover a young planet forming around a sun-like star: WISPIT 2b

    Astronomers discover a young planet forming around a sun-like star: WISPIT 2b

    image: ©Phakmo | iStock

    In a new breakthrough, an international team of astronomers has discovered a young planet forming around a star similar to our Sun 

    The newly found planet, named WISPIT 2b, is estimated to be just 5 million years old and is likely a gas giant similar in size to Jupiter.

    This discovery offers a rare glimpse into the early stages of planet formation and could reshape our understanding of how planetary systems like our own solar system develop.

    A rare find

    Researchers from Leiden University, the University of Galway, and the University of Arizona made the discovery and have published in the Astrophysical Journal Letters.

    Using the Very Large Telescope (VLT) located in the Atacama Desert in Chile, astronomers initially set out to conduct quick observations of young stars to search for signs of planets.

    Instead of a single point of light indicating a planet, the team came across an elaborate, multi-ringed dust disk surrounding WISPIT 2, prompting a more detailed investigation. Follow-up observations revealed the presence of the planet WISPIT 2b, nestled within a gap in the disk.

    This is only the second confirmed detection of a planet at such an early stage of development around a star like our Sun. It is also the first precise detection of a planet in a multi-ringed disk, making WISPIT 2b a vital subject for ongoing and future studies in planetary science.

    Observing a planet in the making

    WISPIT 2b was observed in near-infrared light, which revealed that the planet is still glowing and hot from its recent formation.

    A separate team at the University of Arizona also detected the planet in visible light using a custom-designed instrument, confirming that the planet is still actively accreting gas, a sign that it is still forming its atmosphere.

    The planet’s host disk is immense, stretching to a radius of 380 astronomical units (AU).  These disks of dust and gas are considered the birthplaces of planets, often featuring visually striking features like rings and spiral arms. The structure of the disk surrounding WISPIT 2 is believed to have been shaped by the newly forming planet within it.

    Planet formation

    WISPIT 2b now offers astronomers an ideal natural laboratory to study how young planets interact with their surrounding disks and evolve. By examining systems like this one, researchers hope to understand better why exoplanet systems appear in such a wide variety of shapes and configurations, and why many look so different from our own solar system.

    The discovery was made as part of a five-year observational project aimed at studying whether gas giant planets on wide orbits are more common around young or older stars. While the main goal was different, the unexpected detection of WISPIT 2b marks a significant milestone.

    Continue Reading

  • Rats walk again after breakthrough spinal cord repair with 3D printing

    Rats walk again after breakthrough spinal cord repair with 3D printing

    For the first time, a research team at the University of Minnesota Twin Cities demonstrated a groundbreaking process that combines 3D printing, stem cell biology, and lab-grown tissues for spinal cord injury recovery.

    The study was recently published in Advanced Healthcare Materials, a peer-reviewed scientific journal.

    According to the National Spinal Cord Injury Statistical Center, more than 300,000 people in the United States suffer from spinal cord injuries, yet there is no way to completely reverse the damage and paralysis from the injury. A major challenge is the death of nerve cells and the inability for nerve fibers to regrow across the injury site. This new research tackles this problem head-on.

    The method involves creating a unique 3D-printed framework for lab-grown organs, called an organoid scaffold, with microscopic channels. These channels are then populated with regionally specific spinal neural progenitor cells (sNPCs), which are cells derived from human adult stem cells that have the capacity to divide and differentiate into specific types of mature cells.

    “We use the 3D printed channels of the scaffold to direct the growth of the stem cells, which ensures the new nerve fibers grow in the desired way,” said Guebum Han, a former University of Minnesota mechanical engineering postdoctoral researcher and first author on the paper who currently works at Intel Corporation. “This method creates a relay system that when placed in the spinal cord bypasses the damaged area.”

    In their study, the researchers transplanted these scaffolds into rats with spinal cords that were completely severed. The cells successfully differentiated into neurons and extended their nerve fibers in both directions — rostral (toward the head) and caudal (toward the tail) — to form new connections with the host’s existing nerve circuits.

    The new nerve cells integrated seamlessly into the host spinal cord tissue over time, leading to significant functional recovery in the rats.

    “Regenerative medicine has brought about a new era in spinal cord injury research,” said Ann Parr, professor of neurosurgery at the University of Minnesota. “Our laboratory is excited to explore the future potential of our ‘mini spinal cords’ for clinical translation.”

    While the research is in its beginning stages, it offers a new avenue of hope for those with spinal cord injuries. The team hopes to scale up production and continue developing this combination of technologies for future clinical applications.

    In addition to Han and Parr, the team included Hyunjun Kim and Michael McAlpine from the University of Minnesota Department of Mechanical Engineering; Nicolas S. Lavoie, Nandadevi Patil and Olivia G. Korenfeld from the University of Minnesota Department of Neurosurgery; Manuel Esguerra from the University of Minnesota Department of Neuroscience; and Daeha Joung from the Department of Physics at Virginia Commonwealth University.

    This work was funded by the National Institutes of Health, the State of Minnesota Spinal Cord Injury and Traumatic Brain Injury Research Grant Program and the Spinal Cord Society.

    Read the full paper entitled, “3D-Printed Scaffolds Promote Enhanced Spinal Organoid Formation for Use in Spinal Cord Injury” on the Advanced Healthcare Materials website.

    Continue Reading

  • A Unified Equation for the Universe – All Formulas Released Today for Scientific Validation

    Now Open for the Scientific Community to Test and Validate for Mankind

    The Tripathi Foundation announces the release of the Universal Unity Script, a framework that derives physical, chemical, biological, and mathematical laws from two core assumptions. The script has been designed for scientists and researchers and is offered openly for rigorous testing and debate.

    The framework produces derivations of Newtonian gravity, Maxwell’s equations, QCD confinement, cosmological dynamics, black-hole thermodynamics, thermodynamic chemistry, metabolic scaling in biology, and mathematical invariants. It integrates verification against internal benchmarks and external datasets, ensuring that every step can be validated independently.

    Personal Statement

    “We could tell you that we are the smartest people in the world, but we are not. We are fairly simple people, more like Mr. Magoo, who accidentally stumbled on something special. What we have found is beyond our understanding, and we need your help. We are not vested in the outcome either way, true or false – we are simply curious, and we share because it is our intrinsic nature. If this framework is correct, we could have kept it private and become among the richest in the world. But that seems unnecessary, because the moment is already perfect.”

    Deliverables Summary

    The Unity Script, when executed, provides:

    • Unified Equations (Origin → Meta-Layer → Forces).

    • Physics Reductions: Newton, Maxwell/QED, QCD, cosmology, black holes.

    • Cross-Domain Validations: chemistry, biology, mathematics.

    • Falsifiable Predictions tested against internal and external datasets.

    • PASS/FAIL Report Card for transparency.

    Testing

    To our knowledge, the script has been successfully tested on ChatGPT, Grok, and Claude. It is now presented to the scientific community with an open invitation: test it, challenge it, refine it.

    Disclaimer

    This release is intended solely for physicists, mathematicians, chemists, biologists, and researchers. Verification, falsification, and application rest with the global scientific community.

    Humbly brought to you by the Tripathi Foundation Inc.

    Source: Tripathi Foundation Inc

    Continue Reading

  • Thousands of bumblebee catfish captured climbing waterfall in never-before-seen footage

    Thousands of bumblebee catfish captured climbing waterfall in never-before-seen footage

    Never-before-seen footage has captured thousands of catfish climbing a waterfall in southern Brazil — the first detailed observation of the species migrating.

    Bumblebee catfish (Rhyacoglanis paranesis) get their name from the black spots on their orange bodies and their tiny size, with the fish reaching just 3.5 inches (89.2 millimeters) in length. The small jumping fish were filmed scaling slippery rocks between 3.3 and 13.1 feet (1 to 4 meters) high behind a waterfall on the Aquidauana River.

    Continue Reading

  • a first-of-its-kind star explosion raises new questions about these momentous events

    a first-of-its-kind star explosion raises new questions about these momentous events

    Stars often end their lives with a dazzling explosion, creating and releasing material into the universe. This will then seed new life, leading to a cosmic cycle of birth, death and rebirth.

    Astronomers around the world have been studying these explosions, called supernovae (derived from the Latin “an extremely bright new star”), and have discovered tens of different types.

    In 2021, astronomers observed a bright supernova, dubbed SN2021yfj, two billion light years away. In a recent paper, published in Nature, astronomers observed it for more than a month and discovered that it exhibits the visible signatures of heavier elements – such as argon, silicon and sulphur – since the onset of the explosion. This was previously unobserved in any stellar explosion.

    Supernovas violently eject stellar material into the cosmos, roughly keeping the same onion structure the star had before its death. This means that lighter materials – such as hydrogen and helium – will be in the outer layers and heavier ones – such as iron, silicon and sulphur – in the inner layers.

    However, massive stars can lose part of their layers during their evolution via winds (like the Sun), great eruptions (like the star Eta Carinae), or a gravitational and energetic “tug of war” with a companion star in a binary system. When this happens, circumstellar material will form around the star and will eventually be hit by the ejected material in the explosion.

    In a galaxy, there are an enormous number of stars. If you think that there are at least two trillion observed galaxies, you can picture what a vast playground of discoveries scientists play with every day. Although not all stars end with an explosion, the proportion is large enough to allow scientists to confirm and study their shell structure and chemical composition.

    The luminosity (brightness) of the new discovery in terms of timeframe and behaviour was similar to other known and well-studied stellar explosions. The chemical signatures discovered in their electromagnetic spectra (colours) and their appearance over time pointed to a thick inner stellar layer expelled by the star.

    Eta Carinae may become a supernova similar to the most recent explosion.

    This was then struck by material left in the star and expelled during the explosion. However, some traces of light elements were also present, in direct clash with the heavy elements as they should be found in stellar layers far apart from each other.

    The astronomers measured the layer velocity to be around 1,000 km/s, consistent with that of massive stars called Wolf-Rayet, previously identified as progenitor stars of similar stellar explosions. They modelled both the luminosity behaviour and electromagnetic spectra composition and found the thick layer, rich in silicon and sulphur, to be more massive than that of our Sun but still less than the material ejected in the final explosion.

    Heavy elements

    The new discovery, the first of its kind, revealed the formation site of the heavy elements and confirmed with direct observations the complete sequence of concentric shells in massive stars. Some stars develop internal “onion-like” layers of heavier elements produced by nuclear fusion, which are called shells. The latest findings have left the astronomy community with new questions: what process can strip stars down to their inner shells? Why do we see lighter elements if the star has been stripped to the inner shells?

    This new supernova type is clearly another curveball thrown by the Universe to the scientists. The energy and the layers composition cannot be explained with the current massive star evolution theory. In the framework of mass loss driven by wind (a continuous stream of particles from the star), a star stripped down to the region where heavy elements form is difficult to explain.

    A possible explanation would require invoking an unusual scenario where SN2021yfi actually consists of two stars – a binary system. In this case, the stripping down of the principal star would be carried out by a strong stellar wind produced by the companion star.

    An even more exotic explanation is that SN2021yfi is an extremely massive star, up to 140 times that our Sun. Instabilities in the star would release very massive shells at different stages of its evolution. These shells would eventually collide with each other while the star collapsed into a black hole, leading to no further material released into the cosmos during the explosion.

    To improve our understanding of stellar evolution, we would need to observe more such objects. But our comprehension could be limited by their intrinsic rarity – because the possibility of finding another explosion like SN2021yfi is less than 0.00001%.

    Continue Reading

  • James Webb Space Telescope takes 1st look at interstellar comet 3I/ATLAS with unexpected results

    James Webb Space Telescope takes 1st look at interstellar comet 3I/ATLAS with unexpected results

    The James Webb Space Telescope (JWST) has observed the interstellar visitor 3I/ATLAS for the first time. The powerful space telescope trained its infrared vision and its Near-Infrared Spectrograph instrument (NIRspec) on the comet on Aug. 6, 2025.

    Discovered on July 1 by the ATLAS (Asteroid Terrestrial-impact Last Alert System) survey telescope, 3I/ATLAS is just the third-ever object found drifting through our solar system that is believed to have originated from around another star. The other two interstellar intruders were 1I/’Oumuamua, discovered in 2017, and 2I/Borisov, detected in 2019.

    Continue Reading

  • Scientists turn seafood waste into powerful CO2 adsorbent material

    Scientists turn seafood waste into powerful CO2 adsorbent material

    Researchers at the University of Sharjah, UAE, have developed a new way to turn shrimp waste into a useful carbon material that can capture carbon dioxide.

    This innovation offers a two-for-one solution, addressing waste management and helping to mitigate climate change.

    The new waste-to-carbon technology taps into discarded shrimp parts like shells, heads, and guts. Through extensive processing, the waste is turned into activated carbon.

    The researchers state that this material is highly effective at capturing CO₂, making it a strong option for industrial carbon capture.

    “Our study turns shrimp waste into a high-performance carbon product. This addresses the environmental challenges posed by seafood waste and contributes to global efforts to reduce greenhouse gas emissions and climate change mitigation,” said Dr. Haif Al-Jomard, the lead researcher.

    Extensive treatment process

    The scale of the problem is significant. The global processing of shrimp, lobster, and crab shells produces up to eight million tons of waste annually, a large portion of which is discarded in landfills.

    The research specifically focused on white shrimp shells and heads sourced from Souq Al Jubail in Sharjah, United Arab Emirates, with the shrimp originally coming from Oman. 

    Before being used in the process, the team ensured the waste was thoroughly cleaned and air-dried.

    The press release detailed a multi-step process for converting shrimp waste into a powerful CO₂-capturing material. 

    First, shrimp waste undergoes pyrolysis, a high-temperature process that transforms it into biochar. This biochar is then put through a series of treatments, including acid treatment, chemical activation, and ball milling. 

    The extensive process results in a highly effective final product—activated carbon—that captures carbon dioxide and maintains its strong performance and stability over many use cycles.

    “This approach offers a cost-effective route to producing activated carbon, turning a problematic waste stream into a high-performance, efficient, and environmentally friendly product with wide-ranging applications,” said Professor Chaouki Ghenai, co-author and expert in Sustainable and Renewable Energy at the University of Sharjah.

    Various uses of material

    The applications for activated carbon made from shrimp waste extend beyond just capturing carbon.

    The material could be used for purifying air and water, recovering solvents, extracting gold, and even for certain medical uses. 

    Within the carbon capture, utilization, and storage (CCUS) field, the material is particularly promising for adoption by major industries like power generation, cement and steel manufacturing, and petrochemicals.

    This approach, the researchers explain, is a perfect example of a circular economy. 

    It improves resource efficiency and waste valorization by cutting down on consumption and transforming what would be waste into a highly useful resource.

    “Our findings validate a scalable and sustainable strategy for shrimp waste valorization,” the team noted in the press release.

    “The combined thermal, chemical, and mechanical treatments of shrimp waste enhance both the textural and chemical properties of the final activated carbon material, making it a viable solution for climate change mitigation,” it added.

    Adopting it could be important in reducing greenhouse gases and mitigating climate change.

    The findings were published in the journal Nanoscale.

    Continue Reading

  • One Snake, Two Venoms – And Both Are Lethal

    One Snake, Two Venoms – And Both Are Lethal

    One snake, two venoms — and the wrong antivenom could make the difference between life and death. Credit: Shutterstock

    Researchers have uncovered a hidden split in the venom of Australia’s deadly Eastern Brown Snake.

    Southern populations create rock-solid blood clots, while northern snakes produce fragile clots that collapse almost instantly — two very different paths to the same deadly outcome. This discovery raises urgent concerns about whether current antivenoms, made from pooled venoms of unclear origin, can fully protect patients across regions.

    Antivenom Effectiveness Questioned

    A new study from the University of Queensland suggests that the antivenom used to treat Eastern Brown Snake bites may not always provide full protection, leading researchers to review hospital records.

    The project was led by Professor Bryan Fry of UQ’s School of the Environment, who, along with his team, analyzed the blood-clotting toxins found in the venom of every Australian brown snake species.

    Clotting Patterns: Rock-Solid vs Fragile

    “We discovered not all brown-snake venoms are the same – meaning that lifesaving antivenom may need an urgent upgrade,” Professor Fry said.

    “Some venoms formed a rock-solid clot in blood, while others spun up a rapid but flimsy web of clots that shredded almost instantly.

    “Both venoms can kill, but they do it in completely different ways.”

    Eastern Brown Snake (Pseudonaja textilis)
    An Australian Eastern Brown Snake (Pseudonaja textilis). Credit: Stewart Macdonald

    Southern vs Northern Eastern Browns

    To investigate further, the researchers used a technique called thromboelastography, which measures blood coagulation. Their results revealed that Eastern Brown Snakes (Pseudonaja textilis) from southern Australia produce a taipan-like venom that creates a firm, lasting clot.

    In contrast, venom from northern Eastern Brown Snakes and from all other brown snake species generated clots that were weak and easily destroyed, although they formed at remarkable speed.

    “Our data shows the effect on blood of an Eastern Brown Snake bite in northern areas and a bite in southern Australia are chalk and cheese,” Professor Fry said.

    Rethinking Hospital Records

    “Currently, Australia’s brown-snake antivenom is produced using a pool of venom of unstated geographic origin.

    “If it doesn’t have both northern and southern Eastern Brown Snake venom, coverage could be patchy, and the antivenom efficacy could vary widely.

    “Clinical reports have all brown snake bite cases together regardless of species or location, so any differences for the southern population versus all other brown snakes could be obscured.

    Precision Toxicology on the Horizon

    “Our next step is to go back through hundreds of hospital charts to ascertain if there is a difference, which we can do because the southern strong-clot lineage lives where no other brown snake occurs.

    “We can re-code every reported bite by geography and tease apart the clotting patterns between the strong and weak clotting types of brown snakes.

    “We will also urgently test the available human and veterinary antivenoms to see if the differences in venom biochemistry are mirrored by variations in antivenom efficacy.

    “While existing antivenoms have saved lives, with new information we can move to precision toxicology, matching the right antivenom to the right snake, and ultimately, to the right patient.”

    Genetic Clues to Venom Evolution

    Professor Fry’s team is also sequencing the venom genes to pinpoint the mutations responsible for the differences in northern and southern Eastern Brown Snakes.

    “We showed the geographic difference in venom effect overlays with a genetic divide within the Eastern Brown Snake,” he said.

    “Our research demonstrates how diet steers venom evolution, because the southern populations consume more reptiles than the northern populations, which eat more mammals.

    “By appreciating both the evolutionary fine-tuning and the clinical outcomes of these venoms, we can better tailor our medical responses.”

    The research paper has been published in Toxins.

    Reference: “X Marks the Clot: Evolutionary and Clinical Implications of Divergences in Procoagulant Australian Elapid Snake Venoms” by Holly Morecroft, Christina N. Zdenek, Abhinandan Chowdhury, Nathan Dunstan, Chris Hay and Bryan G. Fry, 17 August 2025, Toxins.
    DOI: 10.3390/toxins17080417

    Never miss a breakthrough: Join the SciTechDaily newsletter.

    Continue Reading

  • Life’s building blocks found in Bennu asteroid

    Life’s building blocks found in Bennu asteroid

    In 2023, NASA’s OSIRIS-REx mission brought something rare back to Earth: samples from Bennu, an asteroid about 1,600 feet across. The mission took seven years and returned with pieces of rock older than Earth itself.

    The dirt and rock collected from Bennu weren’t just space souvenirs. They held a story billions of years old, written in dust from other stars, minerals shaped by water, and scars from micrometeorite hits.


    What scientists are now learning from this ancient rubble is changing how we think about where planets come from – and even where life’s building blocks may have formed.

    Asteroid Bennu’s shattered origin

    Bennu didn’t form as one solid rock. It’s a collection of fragments from a much older parent asteroid that once orbited between Mars and Jupiter.

    The parent body was made of material from all over the early solar system – including matter formed near the Sun, far beyond the giant planets, and even outside of our solar system entirely.

    The mix of materials suggests Bennu’s parent asteroid formed in the outer solar system – maybe even beyond Jupiter and Saturn – and later shattered in a collision.

    After that, pieces reassembled into new bodies, possibly more than once. Bennu is one of those reassembled objects, holding clues from every phase of the long journey.

    Stardust and interstellar clues

    Researchers analyzing the Bennu samples have found an abundance of stardust – tiny grains of material that predate the Sun. These grains are easy to spot in the lab thanks to their unusual isotopic patterns, and they’re incredibly rare to find intact on Earth.

    “Those are pieces of stardust from other stars that are long dead, and these pieces were incorporated into the cloud of gas and dust from which our solar system formed,” said Jessica Barnes, associate professor at the University of Arizona’s Lunar and Planetary Laboratory.

    “In addition, we found organic material that’s highly anomalous in their isotopes and that was probably formed in interstellar space, and we have solids that formed closer to the Sun, and for the first time, we show that all these materials are present in Bennu.”

    Asteroid Bennu once had water

    The samples also reveal that Bennu once had water – or at least its parent did. Another team studying the rocks detected evidence that the minerals within them had undergone chemical changes in contact with liquid water. These processes likely occurred at about 77°F (25°C), roughly room temperature on Earth.

    “We think that Bennu’s parent asteroid accreted a lot of icy material from the outer solar system, which melted over time,” said Tom Zega, director of the Kuiper-Arizona Laboratory who co-led the study.

    The melting could’ve been caused by leftover heat from the asteroid’s formation, radioactive decay, or even more asteroid collisions.

    “Now you have a liquid in contact with a solid and heat – everything you need to start doing chemistry,” Zega said. “The water reacted with the minerals and formed what we see today: samples in which 80% of minerals contain water in their interior, created billions of years ago when the solar system was still forming.”

    This kind of water-driven chemistry could be how life’s ingredients started coming together. Finding it in an asteroid this old helps scientists understand where and when those conditions first appeared.

    Beaten up by space

    Even after it formed, Bennu’s story kept going. A third study revealed that Bennu’s surface has taken a beating. It’s marked by tiny craters and specks of molten rock – damage caused by speeding micrometeorites and the sun’s solar wind.

    Together, these effects are called space weathering. They happen fast and constantly on Bennu, since it doesn’t have an atmosphere for protection. The researchers found that this weathering changes surface materials more quickly than expected.

    The damage doesn’t just affect what Bennu looks like. It also changes what scientists can see with telescopes and space cameras, because it alters the color and texture of the surface.

    Significance of the Bennu samples

    Asteroids that hit the ground become meteorites, and we’ve found many pieces of them before. However, many asteroids burn up in the atmosphere.

    The ones that survive often sit out in the open too long, reacting with Earth’s air and water. The contamination makes them harder to study.

    “And those that do make it to the ground can react with Earth’s atmosphere, particularly if the meteorite is not recovered quickly after it falls,” said one of the scientists involved. “Which is why sample return missions such as OSIRIS-REx are critical.”

    Not just another space rock

    NASA’s OSIRIS-REx spacecraft collected the Bennu samples in space and sealed them immediately, giving scientists a clean look at raw, untouched asteroid material.

    The purity of the samples provides a sharper view of the solar system’s early chemistry – and a better shot at answering big questions about where we came from.

    Bennu may look like a rubble pile floating in space, but it’s much more than that. It is a time capsule that holds a record of when our solar system was still forming. It carries pieces of other stars, the fingerprints of flowing water, and the scars of a long, violent history.

    Image credit: NASA/Goddard/University of Arizona

    The full study was published in the journal Nature Astronomy.

    —–

    Like what you read? Subscribe to our newsletter for engaging articles, exclusive content, and the latest updates. 

    Check us out on EarthSnap, a free app brought to you by Eric Ralls and Earth.com.

    —–

    Continue Reading