Today's Image of the Day from the European Space Agency features the Eagle Nebula, also known as Messier 16, which is located about 7,000 light-years away in the constellation Serpens.



The Eagle Nebula is one of the most iconic star-forming regions in our galaxy. It’s a vast cloud of gas and dust stretching roughly 70 light-years across. 



<h2 class="wp-block-heading" id="h-pillars-of-creation-nbsp">Pillars of Creation&nbsp;</h2>



What makes it especially famous is a portion of the <a href="https://www.earth.com/news/six-rogue-worlds-discovered-inside-a-young-star-forming-nebula/">nebula</a> captured by the Hubble Space Telescope in 1995 - an area called the "Pillars of Creation."&nbsp;



Some of these towering columns of gas are several light-years tall. The towers resemble sculpted fingers reaching out into space. Inside these pillars, new <a href="https://www.earth.com/news/serpens-nebula-image-reveals-how-stars-are-born/">stars</a> are being born as gravity pulls material together into dense cores that eventually ignite nuclear fusion.



The Pillars of Creation are often cited as a poetic example of the cosmic cycle of birth and destruction - where new stars are born even as the surrounding material is slowly destroyed by radiation.



<h2 class="wp-block-heading" id="h-hubble-image-of-the-eagle-nebula-nbsp">Hubble image of the Eagle Nebula&nbsp;</h2>



“This towering structure of billowing gas and dark, obscuring dust might only be a small portion of the Eagle Nebula, but it is no less majestic in appearance for it,” said <a href="https://esahubble.org/images/heic2507a/">ESA</a>.



“The new Hubble image is part of ESA/Hubble’s 35th anniversary celebrations. The cosmic cloud shown here is made of cold hydrogen gas, like the rest of the Eagle Nebula. In such regions of space new stars are born among the collapsing clouds.”&nbsp;



The hot, energetic stars emit intense ultraviolet light and powerful stellar winds that erode and sculpt the surrounding gas. The result is the creation of fantastical structures - like the narrow pillar with a blossoming head featured in the new image.



<h2 class="wp-block-heading" id="h-light-and-shadow-in-the-eagle-nebula">Light and shadow in the Eagle Nebula</h2>



The thick material in the pillar blocks most light, appearing dark and heavy against the backdrop. However, its edges glow where light from the more distant nebula shines through.&nbsp;



The striking colors reflect the chemistry and physics at play: blues signal ionized oxygen, reds indicate glowing hydrogen, and orange shows where starlight has managed to pierce the dust.



<h2 class="wp-block-heading" id="h-a-structure-under-siege">A structure under siege</h2>



Just out of frame lie the very stars responsible for shaping this dramatic pillar. Their radiation and winds continue to batter the cloud, compressing the gas and potentially triggering the birth of even more stars within.



For now, the pillar holds firm, but this stability is temporary. Over time, the relentless energy from newly formed <a href="https://www.earth.com/news/fluffy-molecular-clouds-may-change-our-understanding-of-star-formation/">stars</a> will eventually erode the entire structure.



“While the starry pillar has withstood these forces well so far, cutting an impressive shape against the background, eventually it will be totally eroded by the multitude of new stars that form in the Eagle Nebula,” explained ESA.



<h2 class="wp-block-heading" id="h-life-cycle-of-the-milky-way">Life cycle of the Milky Way</h2>



The nebula’s location in the Sagittarius Arm - one of the Milky Way’s major spiral arms - places it in a zone bustling with similar star-forming regions. This highlights the role of the Eagle Nebula in shaping the structure and the future of our galaxy.



Studies of the Eagle Nebula have revealed that the region is rich in young, hot stars - some of which are only a few million years old. These stars are in various stages of development, providing a natural laboratory for astronomers to study stellar life cycles.&nbsp;



<h2 class="wp-block-heading" id="h-evolution-of-the-eagle-nebula-nbsp">Evolution of the Eagle Nebula&nbsp;</h2>



Within the Eagle Nebula, there is a variety of stellar processes occurring in close proximity. Some stars are still forming within dense clouds of gas, while others have already matured and begun to emit powerful ultraviolet radiation.&nbsp;



The ongoing interaction between <a href="https://www.earth.com/news/star-formation-reignited-in-the-galaxy-leo-p-after-billions-of-years/">young stars</a> and their environment drives the evolution of the nebula itself.&nbsp;



As newly formed stars heat and disperse the gas and dust around them, they trigger further waves of star formation - or in some cases, halt it altogether.&nbsp;



This feedback loop not only influences the pace of star birth in the Eagle Nebula but also contributes to the broader life cycle of matter within the <a href="https://www.earth.com/news/milky-way-collision-may-change-everything-we-know-about-our-galaxy/">Milky Way</a>, enriching the galaxy with heavier elements forged in stellar cores.



Image Credit: ESA/Hubble &amp; NASA, K. Noll



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Eagle Nebula: Carving light from darkness

Today's Image of the Day from the European Space Agency...

Today's Image of the Day from the European Space Agency features a portion of the Rosette Nebula, captured by the Hubble Space Telescope.



The Rosette Nebula is a vast cloud of gas and dust located in the constellation Monoceros, also known as the Unicorn.



Shaped like a blooming rose in deep space, it lies about 5,200 light-years from Earth and spans roughly 100 light-years in diameter.&nbsp;



<h2 class="wp-block-heading" id="h-image-of-the-rosette-nebula">Image of the Rosette Nebula </h2>



“<a href="https://www.earth.com/news/35-years-of-hubble-the-telescope-that-changed-our-view-of-the-universe/" target="_blank" rel="noreferrer noopener">Hubble</a> zooms into a small portion of the nebula that is only four light-years across (the approximate distance between our Sun and the neighboring Alpha Centauri star system),” noted <a href="https://www.esa.int/ESA_Multimedia/Images" target="_blank" rel="noreferrer noopener">ESA</a>.



“Dark clouds of hydrogen gas laced with dust are silhouetted across the image. The clouds are being eroded and shaped by the seething radiation from the cluster of larger stars in the center of the nebula.”&nbsp;



“An embedded star seen at the tip of a dark cloud in the upper right portion of the image is launching jets of plasma that are crashing into the cold cloud around it. The resulting shock wave is causing a red glow. The colors come from the presence of hydrogen, oxygen, and nitrogen.”



<h2 class="wp-block-heading" id="h-distinct-appearance-of-rosette">Distinct appearance of Rosette</h2>



Stellar winds and ultraviolet light are gradually carving out a cavity in the nebula’s center while simultaneously triggering new waves of <a href="https://www.earth.com/news/fluffy-molecular-clouds-may-change-our-understanding-of-star-formation/" target="_blank" rel="noreferrer noopener">star formation</a> along its dense edges.&nbsp;



The Rosette Nebula is often studied to understand the life cycle of stars and the complex interactions between radiation and interstellar material. 



Its intricate structure and visual appeal have made it a favorite target for both professional astronomers and astrophotographers.



<h2 class="wp-block-heading" id="h-nebulae-that-are-similar-to-rosette">Nebulae that are similar to Rosette</h2>



Compared to other famous nebulae, the Rosette Nebula stands out for its symmetry and floral appearance, which give it a distinct, iconic look. It's often compared to the Orion Nebula, which is much closer to Earth at about 1,300 light-years away and far brighter in the night sky. 



The <a href="https://www.earth.com/news/orion-nebula-destroys-an-oceans-worth-of-water-every-month/" target="_blank" rel="noreferrer noopener">Orion Nebula</a> is a bustling stellar nursery visible even to the naked eye, while the Rosette requires a telescope and is more diffuse and fainter despite being larger in actual size.



The Eagle Nebula, home to the famous "Pillars of Creation," shares a similar process of star formation and sculpting by radiation, but the Eagle has more dramatic, finger-like structures.&nbsp;



<h2 class="wp-block-heading" id="h-stellar-feedback-and-cosmic-evolution">Stellar feedback and cosmic evolution</h2>



The Lagoon Nebula and the Trifid Nebula, both in the constellation Sagittarius, also resemble the Rosette in that they are active star-forming regions, but they lie in a denser part of the <a href="https://www.earth.com/news/astronomers-found-something-strange-at-core-of-milky-way-galaxy-webb-meerkat/" target="_blank" rel="noreferrer noopener">Milky Way</a> and are often surrounded by a rich starfield.



What makes the Rosette Nebula particularly interesting scientifically is the clear interaction between its central star cluster and the surrounding gas, offering a textbook example of how massive stars influence their environment. 



It may not be as visually iconic as the Orion or as dynamic as the Eagle, but it's a beautiful and instructive example of stellar feedback and cosmic evolution.



<h2 class="wp-block-heading" id="h-history-of-the-rosette-nebula">History of the Rosette Nebula </h2>



The history of the Rosette Nebula, like many deep-sky objects, is a blend of observational discovery and increasing scientific understanding over time. 



Although it was likely spotted by earlier astronomers, its first documented observation was in the late 17th century by John Flamsteed, the first Astronomer Royal of England.&nbsp;



However, the <a href="https://www.earth.com/news/six-rogue-worlds-discovered-inside-a-young-star-forming-nebula/" target="_blank" rel="noreferrer noopener">nebula</a> itself was not fully recognized as a distinct object until the advent of astrophotography and improved telescopes in the 19th and 20th centuries.



<h2 class="wp-block-heading" id="h-star-clusters-of-the-enormous-cloud">Star clusters of the enormous cloud</h2>



The central star cluster, NGC 2244, was cataloged separately by William Herschel in the 18th century. Over time, astronomers realized that this cluster was embedded in a much larger, complex nebular structure.&nbsp;



As telescope technology advanced, astronomers identified several parts of the Rosette Nebula and gave them separate designations, including NGC 2237, NGC 2238, NGC 2239, and NGC 2246 - essentially referring to different regions of the same enormous cloud.



Observations from space-based telescopes like Chandra (X-rays) and Spitzer (infrared) helped map the energetic processes inside the nebula, revealing how radiation and stellar winds from NGC 2244 are triggering the birth of new stars in its surrounding regions.



Image Credit: ESA



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Rosette Nebula: A flower blooming in deep space

Today's Image of the Day from the European Space Agency features UGC 5460, a spiral galaxy that is located about 60 million light-years away in the constellation Ursa Major.&nbsp;



“This image combines four different wavelengths of light to reveal UGC 5460’s central bar of stars, winding spiral arms and bright blue star clusters. Also captured in the upper left-hand corner of this image is a far closer object: a star just 577 light-years away in our own galaxy,” said <a href="https://www.esa.int/ESA_Multimedia/Images" target="_blank" rel="noreferrer noopener">ESA</a>.



“UGC 5460 has hosted two recent supernovae named SN 2011ht and SN 2015as. It’s because of these two stellar explosions that Hubble targeted this galaxy, collecting data for three observing programmes that aim to study various kinds of supernovae.”&nbsp;



<h2 class="wp-block-heading" id="h-a-core-collapse-supernova-nbsp">A core-collapse supernova&nbsp;</h2>



SN 2015as is an example of a core-collapse supernova. This type of <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernova</a> occurs when the core of a massive star - typically with more than 8 times the mass of the sun - can no longer support its own gravity after exhausting its nuclear fuel. 



This causes the core to collapse under its own weight, leading to an extremely violent explosion. The collapse triggers the release of an enormous amount of energy, expelling the outer layers of the star into space.



In the aftermath of the explosion, a dense <a href="https://www.earth.com/news/shockingly-bright-carbon-monoxide-detected-in-supernova-remnant/" target="_blank" rel="noreferrer noopener">remnant</a> is created. This is often a neutron star or black hole, depending on the mass of the original star. Core-collapse supernovae are some of the most powerful events in the universe.



According to ESA, Hubble observations of SN 2015as will help researchers understand what happens when the expanding shockwave of a <a href="https://www.earth.com/news/supernova-dandelion-year-1181-leaves-behind-zombie-star-defying-death/" target="_blank" rel="noreferrer noopener">supernova</a> collides with the gas that surrounds the exploded star.



<h2 class="wp-block-heading" id="h-rare-stars-with-large-eruptions-nbsp">Rare stars with large eruptions&nbsp;</h2>



“SN 2011ht might have been a core-collapse supernova as well, but it could also be an impostor called a luminous blue variable. Luminous blue variables are rare stars that experience eruptions so large that they can mimic supernovae,” noted ESA.



“Crucially, luminous blue variables emerge from these eruptions unscathed, while stars that go supernova do not. Hubble will search for a stellar survivor at SN 2011ht’s location, and the explosion’s identity may be revealed at last.”



<h2 class="wp-block-heading" id="h-what-is-a-spiral-galaxy">What is a spiral galaxy?</h2>



Spiral galaxies are some of the most recognizable and beautiful structures in the universe. They are known for their distinctive arms that spiral outward from a central bulge.&nbsp;



These galaxies are typically composed of stars, gas, dust, and dark matter. The arms are often sites of intense <a href="https://www.earth.com/news/fluffy-molecular-clouds-may-change-our-understanding-of-star-formation/" target="_blank" rel="noreferrer noopener">star formation</a>, where clouds of gas collapse to form new stars. 



In the center of a spiral galaxy lies a dense concentration of older stars and, often, a supermassive black hole.



<h2 class="wp-block-heading" id="h-structure-of-a-spiral-galaxy-nbsp">Structure of a spiral galaxy&nbsp;</h2>



The structure of a spiral galaxy is generally divided into three main components: the disk, the bulge, and the halo.&nbsp;



The disk is where the spiral arms are located and contains most of the galaxy's visible stars and interstellar medium.&nbsp;



The bulge is a tightly packed region of older stars at the core, and the halo consists of a sparse collection of stars and globular clusters that surround the galaxy.&nbsp;



Spiral galaxies can be classified into different types based on the tightness and number of their spiral arms, as well as the size of their central bulge.



<h2 class="wp-block-heading" id="h-the-milky-way-galaxy">The Milky Way galaxy</h2>



Our solar system is located within a large spiral galaxy known as the Milky Way. The name refers to its appearance as a dim, milky band of light stretching across the night sky.&nbsp;



The term "Milky Way" comes from ancient Greek mythology, where it was associated the goddess Hera's milk spilling into the sky. In Greek, it was called "Galaxias Kyklos," meaning "milky circle."&nbsp;



Spanning about 100,000 light-years in diameter, the Milky Way is composed of stars, gas, dust, and dark matter. The galaxy has a distinct disk shape with spiral arms that wind outward from a central bulge, which houses a supermassive <a href="https://www.earth.com/news/milky-ways-black-hole-unleashes-mysterious-flares/" target="_blank" rel="noreferrer noopener">black hole</a>. 



Our sun is located in one of the spiral arms - known as the Orion Arm - positioned roughly halfway from the center to the outer edge.&nbsp;



The Milky Way is part of a small group of galaxies called the Local Group, which includes the Andromeda Galaxy and several smaller galaxies.



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Hubble views a spiral galaxy with stellar explosions

Today's Image of the Day from NASA Earth Observatory features Lake Chad in central Africa. The photograph was taken by an astronaut aboard the International Space Station.



According to <a href="https://earthobservatory.nasa.gov/images/154407/lake-chads-water-wetlands-and-dunes" target="_blank" rel="noreferrer noopener">NASA</a>, Lake Chad once ranked among the largest natural lakes in the world. It was a critical resource for millions of people and animals, supporting agriculture and fishing across the region.&nbsp;



Lake Chad straddles the borders of Chad, Nigeria, Niger, and Cameroon. The shallow <a href="https://www.earth.com/news/lakes-are-warming-toward-the-point-of-no-return/" target="_blank" rel="noreferrer noopener">lake</a> is primarily fed by the Chari River, which brings water from the Central African Republic. 



The water levels are also influenced by seasonal rainfall. The rainfall patterns vary significantly across the basin but generally follow a wet-dry seasonal cycle.



<h2 class="wp-block-heading" id="h-environmental-decline-and-shrinkage-nbsp">Environmental decline and shrinkage&nbsp;</h2>



From the 1960s to the early 2000s, the lake lost more than 90 percent of its surface area. It transformed from a vast expanse of open water into a patchwork of wetlands, reed beds, and scattered pools.&nbsp;



This environmental decline has had severe consequences for local communities, leading to food and <a href="https://www.earth.com/news/global-water-security-relies-on-the-origins-of-rainfall/" target="_blank" rel="noreferrer noopener">water insecurity</a>, loss of livelihoods, and increasing competition over scarce resources.



“Ongoing droughts and the rising demand for fresh water have shrunk the lake to less than a tenth of the area it covered in the middle of the last century,” noted NASA.



“Although the lake has experienced dry and wet periods for thousands of years, there has been a significant decline in the amount of lake water available since the 1960s.”



<h2 class="wp-block-heading" id="h-conflict-culture-and-economy">Conflict, culture, and economy</h2>



Lake Chad is a geopolitical hotspot. The region has been affected by conflict, including the insurgency led by Boko Haram, which has displaced millions and further complicated efforts to manage and protect the lake’s fragile ecosystem.&nbsp;



Despite these challenges, regional governments and international organizations are working to restore and sustain the lake, including ambitious proposals to divert water from the Congo River basin.



Culturally and economically, Lake Chad remains vital. It is a hub for trade and social exchange among diverse ethnic groups and continues to provide fish and fertile land despite its reduced size.&nbsp;



The future of Lake Chad hinges on sustainable water management, <a href="https://www.earth.com/news/climate-extremes-alter-how-sunlight-travels-through-clear-lakes/" target="_blank" rel="noreferrer noopener">climate</a> resilience, and political cooperation across national boundaries.



<h2 class="wp-block-heading" id="h-evolution-of-lake-chad-nbsp">Evolution of Lake Chad&nbsp;</h2>



According to NASA, the evolution of Lake Chad has been documented by astronaut photography over the past 60 years.&nbsp;



“During the Apollo 7 mission in 1968, an astronaut acquired an oblique <a href="https://eol.jsc.nasa.gov/SearchPhotos/photo.pl?mission=AS07&amp;roll=8&amp;frame=1932" target="_blank" rel="noreferrer noopener">photograph</a> of the lake as one large body of water. In 1982, another <a href="https://eol.jsc.nasa.gov/SearchPhotos/photo.pl?mission=STS005&amp;roll=39&amp;frame=1022" target="_blank" rel="noreferrer noopener">photo</a> from the space shuttle mission STS-5 recorded receding water levels and encroaching sand dunes.”



“A <a href="https://eol.jsc.nasa.gov/SearchPhotos/photo.pl?mission=ISS042&amp;roll=E&amp;frame=244403" target="_blank" rel="noreferrer noopener">photo</a> taken in 2015 during space station Expedition 42 captured the lake’s remaining waters and wetlands in dark green, blue, and brown, contrasting with the sandy shades of the surrounding land.”&nbsp;



<h2 class="wp-block-heading" id="h-wildlife-of-lake-chad">Wildlife of Lake Chad</h2>



Lake Chad still supports wildlife, though species diversity and abundance have declined significantly due to ecosystem degradation



The lake and its surrounding wetlands are home to several species of fish, including tilapia, catfish, and Nile perch, which are important both ecologically and economically.&nbsp;



These fish support a major regional fishing industry, although overfishing and changes in water conditions have put pressure on fish populations.



Birds are another key component of the ecosystem. The lake serves as a crucial habitat and stopover point for <a href="https://www.earth.com/news/birds-may-be-using-quantum-physics-for-migration/" target="_blank" rel="noreferrer noopener">migratory birds</a> traveling along the African-Eurasian flyway. 



Species such as herons, storks, ducks, and geese can be found in the region, especially during the wet season when parts of the lake flood and create rich feeding grounds.



Mammals that depend on the surrounding floodplains and wetlands include hippos and various antelope species, yet their numbers have declined.&nbsp;



<h2 class="wp-block-heading" id="h-conservation-efforts-and-challenges">Conservation efforts and challenges</h2>



Reptiles like Nile crocodiles and turtles also inhabit the lake's waters and marshy areas. In the past, larger wildlife such as elephants and lions may have roamed the wider Lake Chad basin, but they are now mostly gone from the immediate lake area due to habitat loss and human activity.



Despite these challenges, Lake Chad remains an important, yet increasingly fragile, refuge for wildlife in a region where water and natural habitats are becoming more scarce.&nbsp;



Conservation efforts aim to balance the needs of people and <a href="https://www.earth.com/news/thousands-of-freshwater-species-are-threatened-with-extinction/" target="_blank" rel="noreferrer noopener">wildlife</a>, but the success of such efforts depends on managing the lake’s limited resources in the face of climate change, political instability, and population growth.



Image Credit: NASA Earth Observatory&nbsp;



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Lake Chad: A vanishing lifeline in Central Africa

Today's Image of the Day from NASA Earth Observatory features...

Today's Image of the Day from the European Space Agency features NGC 5335 - a barred spiral galaxy located in the constellation Virgo. 



The photo was captured by the Hubble Space Telescope. According to <a href="https://www.esa.int/ESA_Multimedia/Images/2025/04/Barred_Spiral_Galaxy_NGC_5335" target="_blank" rel="noreferrer noopener">ESA</a>, thousands of distant galaxies are speckled throughout the image in a variety of colors.&nbsp;



Hubble is revealing how <a href="https://www.earth.com/news/hidden-galaxies-discovery-would-upend-current-understanding-of-universe/" target="_blank" rel="noreferrer noopener">galaxies</a> form, grow, and evolve over cosmic time by capturing detailed images of galaxies at various stages of development, from the nearby universe to billions of light-years away. 



Hubble images have shown us that galaxies collide and merge, that star formation varies across different types of galaxies, and that supermassive black holes often lie at their centers.



<h2 class="wp-block-heading" id="h-studying-ngc-5335">Studying NGC 5335</h2>



The galaxy NGC 5335 lies approximately 160 million light-years from Earth. It is classified as an SB(s)bc type galaxy, indicating a well-defined bar structure across its center with less distinct spiral arms. The galaxy was discovered by astronomer William Herschel on May 13, 1793.&nbsp;



Like many galaxies of its type, NGC 5335 features active <a href="https://www.earth.com/news/star-formation-reignited-in-the-galaxy-leo-p-after-billions-of-years/" target="_blank" rel="noreferrer noopener">star formation</a>, especially in its spiral arms, where interstellar gas and dust provide the raw material for new stars.&nbsp;



Observations in different wavelengths, including infrared and ultraviolet, help astronomers study its stellar population and the dynamics of its central bar.



<h2 class="wp-block-heading" id="h-hubble-s-view-of-the-spiral-galaxy-nbsp">Hubble’s view of the spiral galaxy&nbsp;</h2>



“NGC 5335 is categorized as a flocculent spiral galaxy with patchy streamers of star formation across its disk. There is a striking lack of well-defined spiral arms that are commonly found among galaxies, including our Milky Way,” noted ESA.



“A notable bar structure slices across the center of the galaxy. The bar channels gas inwards toward the galactic center, fueling star formation.”&nbsp;



“Such bars are dynamic in galaxies and may come and go over two-billion-year intervals. They appear in about 30 percent of observed galaxies, including our Milky Way.”



<h2 class="wp-block-heading" id="h-galactic-bar-in-the-milky-way-nbsp">Galactic bar in the Milky Way&nbsp;</h2>



The bar in the <a href="https://www.earth.com/news/astronomers-found-something-strange-at-core-of-milky-way-galaxy-webb-meerkat/" target="_blank" rel="noreferrer noopener">Milky Way</a> is a vast, elongated structure composed mostly of stars, stretching across the galaxy’s central region. It is a key feature of our galaxy’s architecture, spanning about 27,000 light-years and oriented at an angle relative to the galaxy’s spiral arms.&nbsp;



Astronomers believe the bar plays a crucial role in the dynamics and evolution of the Milky Way by funneling gas inward toward the galactic center. This can feed star formation and fuel the supermassive black hole at the core. 



The bar is thought to have formed from instabilities in the galactic disk and continues to influence the motion of stars and the overall gravitational balance of the galaxy.&nbsp;



Observations in infrared and radio wavelengths, which can pierce through the dust in the galactic plane, have helped scientists map the bar’s size, shape, and orientation.



<h2 class="wp-block-heading" id="h-the-constellation-virgo-nbsp">The constellation Virgo&nbsp;</h2>



Virgo is one of the most prominent and well-known constellations in the night sky, both astronomically and mythologically. It is the second-largest constellation by area and lies along the zodiac, making it one of the twelve constellations through which the <a href="https://www.earth.com/news/team-creates-video-showing-the-sun-in-gamma-rays-over-a-14-year-period/" target="_blank" rel="noreferrer noopener">Sun</a> appears to move during the year.&nbsp;



Virgo is most visible in the evening sky in the Northern Hemisphere during spring, particularly in April and May. Its name means “virgin” in Latin.



Virgo is traditionally associated with various fertility and agriculture goddesses across different cultures, including the Greek goddess Demeter and her daughter Persephone, as well as the Roman goddess Ceres.&nbsp;



In some myths, Virgo represents Astraea, the virgin goddess of justice who fled to the heavens during the corruption of mankind.



<h2 class="wp-block-heading" id="h-astronomical-significance-of-virgo">Astronomical significance of Virgo</h2>



Astronomically, Virgo is situated between Leo to the west and Libra to the east. One of its most notable stars is Spica, the brightest star in Virgo and one of the brightest in the night sky.&nbsp;



Spica is a blue-white giant, located approximately 250 light-years from <a href="https://www.earth.com/news/was-early-earth-a-purple-planet-scientists-say-its-possible/" target="_blank" rel="noreferrer noopener">Earth</a>. It has been important for navigation and agriculture for centuries, marking planting and harvest times in ancient calendars.



Virgo is also of great interest to astronomers because it hosts the Virgo Cluster, a massive cluster of galaxies about 65 million light-years away.&nbsp;



This cluster contains more than 1,000 galaxies, and it's part of the larger Virgo Supercluster, which also includes our own Local Group of galaxies. This makes Virgo a key area for studying large-scale structures in the universe.



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Barred spiral galaxy glows in the constellation Virgo

Today's Image of the Day from the European Space Agency features a stunning image of Andromeda, the nearest spiral galaxy to our Milky Way.



The extraordinary image was captured by ESA's <a href="https://www.earth.com/news/flyeye-telescope-will-spot-asteroids-faster-than-ever-before/" target="_blank" rel="noreferrer noopener">Flyeye telescope</a> in May 2025 during its first light campaign. This was not just a technical test - it became a powerful demonstration of the telescope’s capabilities. 



<h2 class="wp-block-heading" id="h-capturing-andromeda-in-a-single-frame">Capturing Andromeda in a single frame</h2>



The image was produced from 16 simultaneous 30-second exposures, each corresponding to one segment of the instrument’s view. What’s remarkable is that this relatively brief imaging session managed to capture the entire span of Andromeda in a single frame.&nbsp;



“For a dedicated astronomical telescope such as the NASA/ESA Hubble Space Telescope, viewing the whole Andromeda Galaxy requires stitching together hundreds of individual observations. This <a href="https://www.esa.int/ESA_Multimedia/Images/2025/01/Hubble_s_panoramic_view_of_the_Andromeda_Galaxy" target="_blank" rel="noreferrer noopener">Hubble image</a> of Andromeda, for example, took over 10 years and 600 snapshots to make,” noted <a href="https://www.esa.int/ESA_Multimedia/Images/2025/06/Flyeye_s_view_of_the_Andromeda_galaxy" target="_blank" rel="noreferrer noopener">ESA</a>.



“Flyeye, on the other hand, is a survey telescope designed to see as much of the sky at once as possible, and to rapidly scan for new near-Earth objects. This image of Andromeda takes up just one sixteenth of the telescope’s full field of view.”



<h2 class="wp-block-heading" id="h-viewing-the-sky-like-never-before">Viewing the sky like never before</h2>



The Flyeye telescope is a uniquely engineered wide-field survey instrument that gets its name from the compound eyes of insects. The ability to image a vast celestial object like Andromeda so quickly and efficiently speaks volumes about the future role of Flyeye.&nbsp;



While the telescope was primarily designed for planetary defense - specifically, detecting near-Earth objects like asteroids and comets - it is proving to be a versatile tool for wide-field astrophotography.&nbsp;



Once the full network of Flyeye telescopes is operational, ESA will be able to monitor two-thirds of the visible sky up to three times per night. This will greatly enhance our ability to detect moving objects, transient phenomena, and changes in the sky in near real-time.



Flyeye represents a major leap in how we scan and interpret the sky, combining the speed of modern survey telescopes with the breadth and automation required for planetary protection and astrophysical discovery. The image of Andromeda, captured so efficiently, is an early glimpse of that future.



<h2 class="wp-block-heading" id="h-a-closer-look-at-andromeda">A closer look at Andromeda</h2>



The Andromeda Galaxy is the most distant <a href="https://www.earth.com/news/is-the-milky-way-on-a-collision-course-new-clues-from-hubble/" target="_blank" rel="noreferrer noopener">object</a> visible to the naked eye from Earth.&nbsp;Located approximately 2.5 million light-years away in the constellation Andromeda, it spans more than 220,000 light-years across - making it more than twice the size of the Milky Way.&nbsp;



The galaxy contains an estimated one trillion stars, which is several times more than the number in our galaxy.



Andromeda is on a slow but steady <a href="https://www.earth.com/news/milky-way-collision-may-change-everything-we-know-about-our-galaxy/" target="_blank" rel="noreferrer noopener">collision course</a> with the Milky Way. Astronomers estimate that the two galaxies will begin to merge in about 4 billion years, eventually forming a single, much larger elliptical galaxy.&nbsp;



This future collision is not a threat to individual stars or planets, including our solar system, because of the immense distances between stars. Instead, it will be a dramatic and relatively gentle gravitational reshaping of both galaxies over billions of years.



<h2 class="wp-block-heading" id="h-an-important-object-of-study">An important object of study</h2>



Visually, Andromeda appears as a faint, elongated smudge in dark skies, best seen in the Northern Hemisphere during autumn. 



Through binoculars or a small telescope, more structure becomes visible, including its bright core and hints of spiral arms. It has several satellite galaxies of its own, including M32 and M110, both of which are dwarf elliptical galaxies.



As a member of the Local Group - a small cluster of about 80 galaxies that includes the <a href="https://www.earth.com/news/brightest-era-of-the-universe-reveals-how-the-milky-way-formed/" target="_blank" rel="noreferrer noopener">Milky Way</a>, Triangulum Galaxy, and numerous dwarf galaxies - Andromeda plays a key role in our understanding of galactic formation and evolution.&nbsp;



It has been studied extensively in multiple wavelengths, from radio to X-ray, revealing not only its stars and dust lanes but also a massive halo of hot gas surrounding it and evidence of past galactic mergers.



Andromeda remains an important object of study for both scientists and skywatchers. It gives us a glimpse of what the Milky Way might look like from the outside and helps us understand what could happen when our galaxy and Andromeda eventually collide.



Image Credit: ESA



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Andromeda: One trillion stars in a single frame

In a fascinating new study, scientists documented 34 attempts by wild killer whales to give food to humans. These rare cases spanned four oceans and 20 years. Some happened near boats, others in open water or even from the shore. 



The events highlight the <a href="https://www.earth.com/news/killer-whales-use-kelp-to-massage-and-groom-each-other/">orcas</a>’ possible interest in humans and raise important questions about whale intelligence, communication, and social behavior.



“Orcas often share food with each other - it’s a prosocial activity and a way that they build relationships with each other,” said study lead author Jared Towers, of <a href="https://baycetology.org" target="_blank" rel="noreferrer noopener">Bay Cetology</a> in British Columbia, Canada. “That they also share with humans may show their interest in relating to us as well.”



<h2 class="wp-block-heading" id="h-social-lives-of-killer-whales">Social lives of killer whales</h2>



Orcas live some of the most complex social lives in the animal kingdom. They stick together in tight-knit family groups called pods, usually led by an older matriarch. 



These family units aren’t just casual gatherings - they’re lifelong bonds. Calves stay with their mothers for life, swimming, hunting, and <a href="https://www.earth.com/news/photographer-captures-killer-whales-wearing-fish-hats/">playing together</a>. 



In some regions, pods form larger communities or clans that share unique vocal dialects, kind of like cultural accents passed down through generations. This tight social structure helps them coordinate during hunts and <a href="https://www.earth.com/news/killer-whales-use-kelp-to-massage-and-groom-each-other/">protect each other</a> from threats.



But it’s not all business. Orcas socialize for the joy of it too. They engage in what clearly looks like play - tossing kelp, breaching dramatically, or nudging one another during underwater games. 



They form friendships beyond their pods and even flirt, showing preferences and personalities. These interactions suggest that orcas have emotional lives and a sense of identity.



<h2 class="wp-block-heading" id="h-what-orcas-gave-humans">What orcas gave humans</h2>



The 34 incidents involved six distinct populations of killer <a href="https://www.earth.com/news/ai-helps-humans-have-20-minute-conversation-with-humpback-whale-named-twain/">whales</a>. They offered humans a total of 18 species: six fish, five mammals, three invertebrates, two birds, one reptile, and even one piece of seaweed.



In 97 percent of these cases, the orcas waited for a human response. Some hovered for several minutes. 



On several occasions, they tried again when the humans ignored or returned the offering. In two especially curious cases, whales retrieved birds after humans returned them, only to offer them again.



This behavior could be a form of interspecies curiosity, communication, or even social learning. As the authors suggest, these events might represent "generalized altruism" - an advanced trait observed in only a few social animals.



<h2 class="wp-block-heading" id="h-exploration-more-than-play">Exploration more than play</h2>



Though play was observed in 38 percent of the interactions, the researchers argue most cases were not playful. The age of the whales varied widely, and many offered whole, fresh prey. 



In over 75 percent of ignored cases, the whales later used the prey for themselves or their group. This suggests the offerings had purpose and value, not just entertainment.



Curiosity-driven behavior, distinct from play, seemed a stronger motivator. As the study explains, animals often explore to reduce uncertainty. 



Offering food to humans might help orcas learn how we respond, just as they would with unfamiliar members of their own <a href="https://www.earth.com/news/whales-blow-bubble-smoke-rings-near-humans-to-communicate/">species</a>.



<h2 class="wp-block-heading" id="h-deep-social-intelligence-at-work">Deep social intelligence at work</h2>



Some whales returned the same item to humans multiple times. Others acted in pairs or small groups. 



Most of the 34 events involved a single whale separating from a larger group. This suggests the act was not for show. Rather, it might reflect the whale's individual decision to interact.



Interestingly, killer <a href="https://www.earth.com/news/how-dolphin-brains-evolved-to-see-underwater-by-using-sound-echolocation/">whales</a> have also been documented cooperating with human fishers in places like Australia and Russia. The authors noted that this history could influence modern interactions, especially as human activity increases near their habitats.



<h2 class="wp-block-heading" id="h-whales-may-view-humans-as-companions">Whales may view humans as companions</h2>



Killer whales rank second only to humans in brain-to-body ratio. They also show advanced emotional and social behavior. 



These traits support complex social learning, reciprocal behavior, and possibly even empathy.



“Offering items to humans could simultaneously include opportunities for killer whales to practice learned cultural behavior, explore or play and in so doing learn about, manipulate or develop relationships with us,” the researchers wrote.



<h2 class="wp-block-heading" id="h-humans-should-not-approach-whales">Humans should not approach whales</h2>



Despite the remarkable nature of these encounters, the researchers urge caution. Orcas can show complex and sometimes unpredictable behavior. 



While no wild killer whale has killed a person, some interactions have been intense. They warn against seeking out such encounters or encouraging the behavior without proper permissions.



Most of these whales belonged to populations that hunt near the surface and share prey frequently. 



No deep-water, fish-only populations were involved. This suggests that cooperative surface hunting may lead to more frequent and visible interspecies interactions.



<h2 class="wp-block-heading" id="h-complex-minds-of-whales-and-humans">Complex minds of whales and humans</h2>



The findings challenge our assumptions about human-animal relationships. If orcas are experimenting with ways to relate to us, it means they recognize us not as threats, but as potential social partners.



These whales are not just predators. They are thinkers, observers, and maybe, in some way, explorers of culture, curiosity, memory, learning, and emotion. 



Their actions suggest complex minds in both whales and humans, capable of choice, empathy, and communication.



The study is published in the <a href="https://psycnet.apa.org/fulltext/2026-29805-001.html" target="_blank" rel="noreferrer noopener">Journal of Comparative Psychology</a>. 



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Killer whales are attempting to bond with humans, according to many observations

In a fascinating new study, scientists documented 34 attempts by...

Underwater volcanoes, in the area that is now South Africa, vented roughly 20,500 gigatons of carbon dioxide into the ocean-atmosphere system roughly 183 million years ago, crippling the oxygen cycle. 



Human activity between 1850 and 2019 has already pumped out about 2,390 gigatons of the gas. That’s 12 percent of the Jurassic total in less than two centuries.



<a href="https://www.gps.caltech.edu/people/francois-tissot" target="_blank" rel="noreferrer noopener">Professor François Tissot</a> of the California Institute of Technology studies what came next for the Jurassic seas and what it might tell us about the fate of today’s oceans.



<h2 class="wp-block-heading" id="h-sudden-loss-of-ocean-oxygen">Sudden loss of ocean oxygen</h2>



Bands of limestone from southern Italy record the <a href="https://www.sciencedirect.com/science/article/abs/pii/S0012825223003252" target="_blank" rel="noreferrer noopener">Toarcian Oceanic Anoxic Event</a> (T-OAE), a span when oxygen vanished from vast tracts of seawater and many marine species disappeared. 



During the event, only 6 to 8 percent of the seafloor lay under dead, oxygen-starved water. Yet that area was 28 to 38 times larger than today’s anoxic patches. 



“You can see lots of fossils within ocean sediments before the T‑OAE, and then suddenly they disappear,” said Tissot.



The <a href="https://www.sciencedirect.com/science/article/abs/pii/S0009254116305393" target="_blank" rel="noreferrer noopener">Karoo‑Ferrar</a> large igneous province triggered the event by pouring out vast amounts of carbon. It heated the planet, slowed ocean mixing, and altered chemistry enough to pull oxygen from the water.



The anoxic spell lasted roughly 300,000 to 500,000 years, eventually easing as volcanic pulses waned and natural feedbacks rebalanced carbon and <a href="https://www.earth.com/news/earths-oxygen-supply-may-have-been-kick-started-by-volcanoes/">oxygen cycles</a>.



<h2 class="wp-block-heading" id="h-carbon-disrupted-ocean-life">Carbon disrupted ocean life</h2>



Surging greenhouse gases warmed surface waters, strengthened stratification, and blocked the downward draw of fresh <a href="https://www.earth.com/news/dark-oxygen-discovery-deep-ocean-rocks-upends-centuries-of-scientific-beliefs/">oxygen</a>. 



Warmer water also holds less dissolved gas, so every degree of heating squeezed oxygen concentrations further.



Nutrient runoff from newly exposed volcanic ash likely spurred <a href="https://www.earth.com/news/green-algae-in-lake-erie-may-be-hiding-toxic-deadly-compounds/">algal blooms</a>. When that organic matter sank and decayed, it consumed even more oxygen in deeper layers.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/07/limestone-quarry_ancient-seabed_T-OAE-Map_credit-Tissot_1m.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/07/limestone-quarry_ancient-seabed_T-OAE-Map_credit-Tissot_1s.webp" alt="Map of localities in which the T-OAE was previously recognized, along with our study site. Local anoxia refers to sites where redox proxy data reveal locally dysoxic to anoxic conditions. The site of the MSS is shown by the star in the Inset. KFCA-LIP: Karoo–Ferrar–Chon Aike Large Igneous Province. Credit: Tissot" class="wp-image-1976065"/></a><figcaption class="wp-element-caption">Map of localities in which the T-OAE was previously recognized, along with our study site. Local anoxia refers to sites where redox proxy data reveal locally dysoxic to anoxic conditions. The site of the MSS is shown by the star in the Inset. KFCA-LIP: Karoo–Ferrar–Chon Aike Large Igneous Province. Click image to enlarge. Credit: Tissot</figcaption></figure>



The result was anoxia, a chemically reduced state that favors the precipitation of once‑soluble uranium isotopes into sediments, leaving a measurable fingerprint for modern geochemists.



Scientists use those isotopes, preserved in carbonate grains, to reconstruct ocean redox conditions long after the water is gone.



<h2 class="wp-block-heading" id="h-tracing-ancient-ocean-oxygen-change">Tracing ancient ocean oxygen change</h2>



Tissot’s team combined 30 limestone samples with a <a href="https://www.publichealth.columbia.edu/news/what-bayesian-modeling" target="_blank" rel="noreferrer noopener">Bayesian model</a> built by <a href="https://www.gmu.edu/" target="_blank" rel="noreferrer noopener">George Mason University</a> researcher <a href="https://www.researchgate.net/scientific-contributions/Michael-A-Kipp-2118354679" target="_blank" rel="noreferrer noopener">Michael Kipp</a> to convert uranium data into the size of past anoxic zones. 



The model showed oxygen loss peaking just after the first volcanic pulse, then gradually recovering as emissions slowed.



Because uranium mixes uniformly in seawater, its isotopic shift offers a global view rather than a local snapshot, sidestepping problems that plague black shale studies in restricted basins. 



Independent work on molybdenum and thallium isotopes points to the same magnitude of <a href="https://www.earth.com/news/jurassic-extinction-may-hold-clues-about-our-oceans-future/">Jurassic</a> deoxygenation, reinforcing confidence in the carbonate method. Multiple tracers show how fast oceans can suffocate when carbon overwhelms natural buffers.



<h2 class="wp-block-heading" id="h-rock-preserved-ocean-memory">Rock preserved ocean memory</h2>



The limestones sampled from Mercato San Severino in Italy belong to a 5,000-foot-thick sequence of shallow-water carbonates. These were laid down on the southern edge of the ancient <a href="https://www.sciencedirect.com/science/article/pii/S0012825223002830" target="_blank" rel="noreferrer noopener">Tethys Ocean</a>. 



These deposits are ideal for capturing uranium isotope signals because they formed under well-oxygenated conditions and remained chemically stable over time.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/07/limestone-quarry_ancient-seabed_Mercato-San-Severino_credit-Tissot_1m.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/07/limestone-quarry_ancient-seabed_Mercato-San-Severino_credit-Tissot_1s.webp" alt="A quarry illustrating bands of stratified limestone from the ancient seafloor in what is now Mercato San Severino in Italy. Credit: F. Tissot" class="wp-image-1976063"/></a><figcaption class="wp-element-caption">A quarry illustrating bands of stratified limestone from the ancient seafloor in what is now Mercato San Severino in Italy. Click image to enlarge. Credit: F. Tissot</figcaption></figure>



Geochemical screening confirmed the rocks remained largely unaltered after burial. Isotope ratios, trace elements, and sediment structure all supported the conclusion that these limestones faithfully recorded seawater chemistry from the time of deposition.



<h2 class="wp-block-heading" id="h-today-s-waters-mirror-the-past">Today's waters mirror the past</h2>



Modern measurements show that only about 0.2 percent of the seafloor is overlain by permanently anoxic water, mostly in marginal seas like the Black Sea. 



Yet the global inventory of dissolved oxygen has already fallen by roughly 2 percent since 1960. “Oxygen concentrations in both the open ocean and coastal waters have been declining since at least the middle of the 20th century,” said marine ecologist <a href="https://serc.si.edu/staff/denise-breitburg/breitburgd9302003?sort_bef_combine=field_pub_date_value%20ASC&amp;page=3" target="_blank" rel="noreferrer noopener">Denise Breitburg</a>.



A 2024 <a href="https://www.nature.com/articles/s41467-024-52197-6">study</a> warned that deoxygenation will accelerate this century as warming and stratification intensify. If emissions rise, mid-depth zones could lose 20 percent of oxygen by 2100, exceeding many species’ physiological limits.



Dead zones already plague more than 400 estuaries worldwide, harming fisheries and coastal economies and hinting at larger changes offshore.



<h2 class="wp-block-heading" id="h-action-needed-before-oceans-suffocate">Action needed before oceans suffocate </h2>



Past events show that once widespread anoxia takes hold, recovery can take tens of thousands of years even after carbon input stops. 



Unlike volcanic outbursts, human emissions are continuous and tightly linked to energy and food systems, making a quick cutoff challenging. 



Cutting fossil fuel use, protecting carbon‑storing ecosystems, and curbing nutrient runoff can slow oxygen loss before feedback amplifies the trend.



Satellites, autonomous floats, and seafloor sensors now track oxygen in near real time. This gives policymakers a chance to act before thresholds comparable to the <a href="https://www.earth.com/news/jurassic-rocks-reveal-new-details-about-earths-climate-system/">Jurassic</a> pulse are crossed.



Tissot’s limestone cores remind us that the ocean’s memory is long and its tolerance finite.



The study is published in <a href="https://www.pnas.org/doi/10.1073/pnas.2406032121" target="_blank" rel="noreferrer noopener">Proceedings of the National Academy of Sciences</a>.



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What happened in the ocean millions of years ago could happen again today

Underwater volcanoes, in the area that is now South Africa,...

Cell biology is a world of constant motion and hidden structures. Much of what we know about cells comes from decades of research using microscopes, stains, and models. Yet, even in this well-charted territory, surprises still emerge - enter the "hemifusome."



This previously unknown organelle may help explain how cells sort, recycle, and discard their internal cargo. This function is vital to life and is often disrupted in instances of genetic disease.



The discovery of this organelle, which was made by scientists at the <a href="https://www.virginia.edu" target="_blank" rel="noreferrer noopener">University of Virginia</a> and the National Institutes of Health (<a href="https://www.nih.gov" target="_blank" rel="noreferrer noopener">NIH</a>), offers a new lens through which to study the inner workings of the cell. 



It also presents a possible turning point for understanding diseases where cellular housekeeping breaks down. Using cutting-edge imaging tools, researchers have caught this <a href="https://www.earth.com/news/cambrian-explosion-fossils-push-back-the-rise-of-complex-life/">organelle</a> in action and outlined its potential impact on health and medicine.



<h2 class="wp-block-heading" id="h-introducing-the-hemifusome">Introducing the hemifusome</h2>



The hemifusome is not a static component but a temporary structure that appears and disappears depending on the cell’s needs. 



It consists of two vesicles joined together by a partial membrane connection called a hemifusion diaphragm.



In this configuration, the vesicles do not fully merge but maintain a shared boundary that allows them to interact without blending entirely.



"This is like discovering a new recycling center inside the cell," said researcher Seham Ebrahim, Ph.D., of UVA's Department of Molecular Physiology and Biological Physics. 



"We think the hemifusome helps manage how <a href="https://www.earth.com/news/third-state-of-existence-beyond-life-and-death-confirmed-by-scientists/">cells</a> package and process material, and when this goes wrong, it may contribute to diseases that affect many systems in the body."



These hemifused vesicles appear in two configurations. In the direct form, a smaller vesicle is attached to the outer side of a larger one, whereas in the flipped version, the smaller vesicle is embedded on the inner, or luminal, side. 



In both cases, a dense particle called a proteolipid nanodroplet anchors the structure at the junction, possibly guiding its formation and stability.



<h2 class="wp-block-heading" id="h-how-the-hemifusome-appears">How the hemifusome appears</h2>



To study hemifusomes, researchers turned to cryo-electron tomography (cryo-ET). This imaging method freezes cells rapidly, preserving them close to their natural state. 



Unlike traditional <a href="https://www.earth.com/news/watching-electrons-move-1-quintillionth-of-second-attoseconds-attomicroscopy/">electron microscopy</a>, which can distort or destroy delicate structures, cryo-ET allows scientists to see cellular architecture as it truly exists.



By scanning the outer edges of four mammalian cell types, COS-7, HeLa, RAT-1, and NIH/3T3, the team identified hundreds of hemifusomes. These organelles made up nearly 10 percent of all membrane-bound vesicles in those regions. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/07/hemifused-vesicles_cryo-electron-tomography_Nature-Communications_1m.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/07/hemifused-vesicles_cryo-electron-tomography_Nature-Communications_1s.webp" alt="Cryo-electron tomography observation of hemifused vesicles at the leading edge of cultured cells. Credit: Nature Communications (2025)" class="wp-image-1976051"/></a><figcaption class="wp-element-caption">Cryo-electron tomography observation of hemifused vesicles at the leading edge of cultured cells. Click image to enlarge. Credit: Nature Communications (2025)</figcaption></figure>



Their consistency across <a href="https://www.earth.com/news/why-millions-of-fungal-species-still-remain-unknown/">cell</a> types suggests they are not rare anomalies but common cellular components.



"You can think of vesicles like little delivery trucks inside the cell," said Ebrahim, of UVA's Center for Membrane and Cell Physiology. "The hemifusome is like a loading dock where they connect and transfer cargo. It's a step in the process we didn't know existed."



<h2 class="wp-block-heading" id="h-what-makes-the-hemifusome-unique">What makes the hemifusome unique</h2>



Hemifusomes stand out not just for their shape, but for what’s inside them. The larger vesicle usually contains granular material, similar to what is seen in <a href="https://www.earth.com/news/mitochondria-cells-batteries-leaking-causes-inflammation-diseases/">endosomes</a> and ribosome-associated vesicles.



But the smaller vesicle shows a smooth, translucent interior. This likely reflects a protein-free or dilute aqueous solution, setting it apart from other vesicles in the cell.



The hemifusion diaphragm itself is unusually large, about 160 nanometers in diameter, far bigger than the 10 nanometer diaphragms seen in standard vesicle fusion <a href="https://www.earth.com/news/gold-eating-fungus-discovery-could-revolutionize-the-search-for-metals-and-minerals-on-earth-asteroids-and-other-planets/">events</a>. These extended diaphragms appear stable, not fleeting, suggesting they may be designed to last. 



In some cases, the diaphragm grows large enough to engulf the entire smaller vesicle into the larger one’s bilayer, creating a lens-like shape known in simulations as dead-end hemifusion. Seeing this in actual cells challenges the idea that such formations are purely theoretical.



<h2 class="wp-block-heading" id="h-anchors-and-architects-of-the-organelle">Anchors and architects of the organelle</h2>



One consistent feature at the heart of hemifusomes is the dense proteolipid nanodroplet, or PND. About 42 nanometers in diameter, these droplets are lodged at the rim of the hemifusion site. 



Their content, lipids and proteins, suggests they may help build or stabilize the hemifused structure.



These PNDs have never been observed in such a role before. Some appear free in the cytoplasm, others are embedded in membranes. Researchers propose that PNDs may serve as scaffolds for assembling new vesicles. 



As the PND integrates into a membrane, it may kickstart the formation of the smaller vesicle seen in hemifusomes.



This process, described as <a href="https://www.sciencedirect.com/topics/neuroscience/vasculogenesis" target="_blank" rel="noreferrer noopener">de novo vesiculogenesis</a>, stands apart from classical vesicle fusion. The presence of a unique, translucent vesicle and the absence of known docking steps indicate the hemifusome may follow its own assembly path.



<h2 class="wp-block-heading" id="h-are-hemifusomes-related-to-endosomes">Are hemifusomes related to endosomes?</h2>



Given their location and size, hemifusomes resemble some endosomal structures. To investigate this further, the researchers traced the journey of gold nanoparticles, common markers used to map endocytic activity. 



The particles entered known endosomes and <a href="https://www.earth.com/news/tricking-cells-into-thinking-they-ate-less-food-can-slow-aging-process/">lysosomes</a> but never appeared inside hemifusomes. This absence suggests that hemifusomes do not belong to the classical endocytic pathway.



Instead, they may represent a separate system operating independently of the cargo sorting carried out by proteins like ESCRT. This distinction may have wide implications for how we understand vesicle traffic inside cells.



<h2 class="wp-block-heading" id="h-multivesicular-bodies-and-disease">Multivesicular bodies and disease</h2>



Some hemifusomes evolve into more complex structures. The study observed compound hemifusomes that contained multiple vesicles, all partially fused. 



These could be early versions of <a href="https://www.sciencedirect.com/topics/medicine-and-dentistry/multivesicular-body" target="_blank" rel="noreferrer noopener">multivesicular bodies</a> (MVBs), which cells use to break down and recycle internal material.



In the canonical model, ESCRT proteins form inward buds that eventually pinch off inside a larger vesicle. But in hemifusomes, vesicles grow inward through hemifusion and expand with the help of PNDs. 



This alternative route might explain how MVBs form in ways not covered by traditional theories.



One such condition affected by these pathways is Hermansky-Pudlak syndrome. It is a genetic disorder marked by defects in pigmentation, lung function, vision, and bleeding. <a href="https://www.earth.com/news/damaged-mitochondria-recycled/">Cellular recycling</a> issues are central to the disease.



Understanding the hemifusome may help explain these disruptions and lead to future treatments.



<h2 class="wp-block-heading" id="h-a-new-model-for-vesicle-formation">A new model for vesicle formation</h2>



The study proposes a full model where PNDs trigger the formation of translucent vesicles that partially fuse with larger ones, forming hemifusomes. 



These structures may then bud inward, transforming into flipped hemifusomes. Over time, they could scission off as free vesicles inside MVBs.



In contrast to the ESCRT system, which requires tight protein coordination, this mechanism relies on structural and biophysical cues. 



It also sidesteps the need for large lipid donations from other organelles, solving a long-standing puzzle in vesicle formation research.



"This is just the beginning," Ebrahim said. "Now that we know hemifusomes exist, we can start asking how they behave in healthy cells and what happens when things go wrong. That could lead us to new strategies for treating complex genetic diseases."



<h2 class="wp-block-heading" id="h-what-comes-next">What comes next</h2>



The implications of this discovery stretch far beyond cell biology. By offering a new pathway for how cells build and manage internal compartments, the hemifusome challenges decades of assumptions. 



It also invites new thinking about disease, especially conditions where cells fail to manage their waste.



Future research will focus on identifying what proteins guide hemifusome formation and how PNDs are created. 



Scientists also want to know if these structures exist in other parts of the cell, not just at the periphery. Advanced imaging tools and genetic models will be key to answering these questions.



In a field where many believed the major organelles were already mapped, the hemifusome serves as a reminder. The cell still holds secrets. And some of them could lead to cures.



The study is published in the journal <a href="https://www.nature.com/articles/s41467-025-59887-9" target="_blank" rel="noreferrer noopener">Nature Communications</a>.



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Scientists discover a new organelle inside human cells with huge potential impact on health

Cell biology is a world of constant motion and hidden...

A fresh set of numbers is changing what scientists thought happens when a city‑sized slab of ice dissolves into the sea. The target was <a href="https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2023GL104028">mega‑iceberg</a> A‑68A, a floating platform roughly twice the area of Delaware that drifted toward South Georgia in early 2021.



“We think this is the first time measurements have been made so close to an iceberg,” said <a href="https://www.bas.ac.uk/profile/nacas/" target="_blank" rel="noreferrer noopener">Natasha Lucas of the British Antarctic Survey</a>, lead author of the new study. 



For the first time, researchers steered robotic vehicles to within 14 mi of such a iceberg and kept them there long enough to watch meltwater, temperature, and life interact in real time.&nbsp;



<h2 class="wp-block-heading" id="h-tracking-the-a-68a-iceberg">Tracking the A-68A iceberg</h2>



A‑68A calved from the Larsen C Ice Shelf <a href="https://www.earth.com/news/iceberg-larsen-c-antarctica/">back in 2017</a>, then rode the currents of the <a href="https://www.asoc.org/learn/welcome-to-the-southern-ocean/" target="_blank" rel="noreferrer noopener">Southern Ocean</a> on a five‑year tour that ended near South Georgia. 



<a href="https://www.earth.com/news/small-satellites-are-monitoring-ocean-conditions-from-space/">Satellites</a> could trace its general route, but ships kept their distance because the iceberg’s smaller rifts and spins defied prediction.



That standoff ended when a six‑foot‑long glider slipped off the deck of the <a href="https://noc.ac.uk/facilities/ships/rrs-james-cook" target="_blank" rel="noreferrer noopener">research vessel RRS James Cook</a> and began diving and climbing through a 0.6‑mile‑deep column of water. 



Over 49 days it logged 265 vertical profiles, sending each packet of data to scientists piloting the craft from home offices locked down by COVID‑19 restrictions.



The adventure was not entirely smooth. One glider vanished in the melee of drifting growlers, and another spent 17 days wedged beneath the berg before currents spat it out, battery blinking but sensors intact. 



Still, the mission mapped a zone of ocean that had never been observed so closely or for so long.



<h2 class="wp-block-heading" id="h-sensors-beneath-a-68a">Sensors beneath A-68A</h2>



The glider recorded a frosty cap of freshwater spreading across the top 30 ft of the sea. Right below, the instruments found a band of cold winter water that had lost its usual punch, a sign that melt‑driven turbulence had chewed away the seasonal layer separating surface and depth.



As that barrier thinned, nutrient‑rich deep water began sliding upward, carrying iron and silica shaved from the iceberg’s base. 



The upheaval altered local stratification, flipping the normal stack of density and temperature that keeps layers neatly in place during the Antarctic summer.



Salinity told the same story. At barely two miles from A‑68A, the profiles showed tongue‑shaped intrusions of water warmer and saltier than their neighbors, hallmarks of <a href="https://www.earth.com/news/life-survived-when-earth-was-covered-in-ice-but-how/">meltwater</a> plumes that had raced up the iceberg’s base before fanning out sideways.



<h2 class="wp-block-heading" id="h-a-68a-fuels-ocean-life">A‑68A fuels ocean life</h2>



Plankton reacted almost immediately. Near the ice wall, the glider’s fluorometer logged low <a href="https://oceantracks.org/library/oceanographic-factors/chlorophyll" target="_blank" rel="noreferrer noopener">chlorophyll</a> and high backscatter, evidence that meltwater diluted existing blooms while also dumping silt that clouded the light.



Farther away, a spike in <a href="https://www.earth.com/news/shifting-ocean-color-is-pushing-marine-life-toward-the-poles/">chlorophyll</a> flared about 36 hours after the iceberg’s passage, matching lab‑measured growth rates for the local phytoplankton community.



The burst hints that the same plume which first thinned the bloom later primed the water with micronutrients, a one‑two punch that temporarily shuffled who eats whom in the surface ocean.



Because upwelling also lifts dissolved carbon and heat, even short‑lived events like this matter to krill, fur seals, and the economy of South Georgia’s fisheries.



<h2 class="wp-block-heading" id="h-carbon-questions-on-a-cold-frontier">Carbon questions on a cold frontier</h2>



The carbon sink south of 35° S absorbs roughly 40 percent of humanity’s <a href="https://www.earth.com/news/creating-forests-cant-realistically-cancel-out-fossil-fuel-emissions/">fossil‑fuel emissions</a>. How that service will fare as calving accelerates remains uncertain.



The new findings show giant bergs can raise near‑surface stratification yet also stir the mid‑depths, two adjustments that tug carbon uptake in opposite directions. 



Recent model work argues current estimates may already overshoot Southern Ocean uptake by up to 0.4 Pg C yr‑1. Field evidence like the A‑68A data set will help sort winners from losers in that accounting.



<h2 class="wp-block-heading" id="h-risk-reward-and-remote-control">Risk, reward, and remote control</h2>



Flying a glider next to a iceberg the size of Los Angeles is an exercise in calculated gamble. Lucas and colleagues guided their craft from desks more than 7,500 miles away, relying on patchy satellite snapshots to dodge smaller ice.



When the glider went missing under the berg, frustration turned to nervous excitement, then relief as it resurfaced with a <a href="https://www.earth.com/news/supergiant-gold-deposit-find-claims-to-be-the-worlds-largest-discovery-ever/">gold mine</a> of temperature and salinity profiles. 



That trove fixed the first real numbers on basal melt rate, pegging it at roughly 6.9 × 10^8 m³ per day, an estimate within a factor of two of satellite calculations derived from changes in the iceberg’s freeboard height.



<h2 class="wp-block-heading" id="h-icebergs-preview-ocean-changes">Icebergs preview ocean changes</h2>



A‑68A is gone now, splintered into shards tracked only by radar, but younger cousins are lining up. The trillion‑ton A‑23A grounded off South Georgia this <a href="https://earthobservatory.nasa.gov/images/154022/iceberg-grinds-to-a-stop-off-south-georgia-island" target="_blank" rel="noreferrer noopener">March</a>, parking just 43 miles from the shore.



Researchers expect more deep‑drafted icebergs to exit West Antarctica as warming currents nibble ice shelves. 



Each one represents a floating lab, a hazard to shipping, and an agent of surprise for ecosystems that evolved around predictable cycles of light and nutrients.



The new study proves those labs are accessible with today’s tools. It also shows that a single iceberg can redraw local physics and biology in days, a reminder that climate change sends ripple effects far beyond melting ice.



The study is published in <a href="https://www.nature.com/articles/s41561-025-01659-7" target="_blank" rel="noreferrer noopener">Nature Geoscience</a>.



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Scientists measure marine environment near melting mega-iceberg for first time

A fresh set of numbers is changing what scientists thought...

Far beneath the Pacific, where the Philippine Sea Plate dives under Japan, researchers have finally caught a peculiar kind of earthquake in the act.



Instead of lurching violently, the shallow end of the Nankai Trough crept for weeks, shifting only millimeters at a time while instruments buried in the seabed recorded every move.



“It's like a ripple moving across the plate interface,” said Josh Edgington, who analyzed the data while completing his PhD at the <a href="https://ig.utexas.edu/">University of Texas Institute for Geophysics</a> (UTIG).



The event - technically a slow-slip earthquake - was first spotted in autumn 2015 and repeated in 2020. Each episode unzipped roughly 20 miles of the fault in slow motion, starting about 30 miles off Japan’s Kii Peninsula and migrating seaward toward the <a href="https://www.earth.com/news/deep-ocean-trenches-holding-water/">ocean trench</a>.



Onshore seismometers and GPS receivers were oblivious. Only a new network of borehole observatories, drilled hundreds of feet into the seabed, was sensitive enough to detect motion so subtle.



<h2 class="wp-block-heading" id="h-detecting-earthquakes-from-below">Detecting earthquakes from below</h2>



Those boreholes are part of Japan’s ambitious scientific-<a href="https://www.earth.com/news/drilling-hole-reveals-significant-presence-of-high-grade-gold-and-silver-navidad-deposit/">drilling</a> program, which set out to plug the blind spot in global earthquake monitoring.



Land-based arrays can pinpoint sudden jolts but cannot “listen” to the shallows of subduction zones - precisely the places where tsunami-spawning ruptures begin. Installed sensors measure fluid pressure, strain and tilt with exquisite precision, allowing scientists to see how strain accumulates and releases in real time.



For UTIG director Demian Saffer, who led the study, the advantage is obvious. Slow-slip signals, he said, give researchers a direct view of how the shallow plate boundary behaves between major quakes.



If this creeping zone regularly releases stress, it could limit the size of future <a href="https://www.earth.com/news/650-foot-mega-tsunami-sends-seismic-waves-around-world-dickson-fjord-swot-mission/">tsunamis</a>. If not, the locked portion of the fault farther down-dip might still be primed for a magnitude-8 or 9 shock, similar to 1946, when a great Nankai earthquake leveled towns and killed more than 1,300 people.



<h2 class="wp-block-heading" id="h-water-helps-faults-slip">Water helps faults slip</h2>



Both slow-slip events tracked by the borehole array unfolded in regions where pore-fluid pressures are unusually high.



That correlation supports a popular but difficult-to-prove theory: overpressured fluids lubricate faults, allowing sections to move quietly rather than break catastrophically.



In the Nankai data, the link is as clear as it has ever been, offering a new metric for judging the tsunami potential of similar faults worldwide.



<h2 class="wp-block-heading" id="h-tsunami-signs-from-afar">Tsunami signs from afar</h2>



While parts of Nankai appear to “creak and groan” in slow motion, the equivalent shallow segment off the Pacific Northwest known as <a href="https://www.earth.com/news/most-dangerous-part-of-this-west-coast-earthquake-fault-cascadia-subduction-zone/">Cascadia</a> may be silent. 



That worries scientists, because a silent, locked interface stores energy that can unleash one of Earth’s rare magnitude-9 megathrusts and the devastating tsunamis that follow.



“This is a place that we know has hosted magnitude 9 earthquakes and can spawn deadly tsunamis,” Saffer said.



“Are there creaks and groans that indicate the release of accumulated strain, or is fault near the trench deadly silent? Cascadia is a clear top-priority area for the kind of high-precision monitoring approach that we’ve demonstrated is so valuable at Nankai.”



Installing similar borehole observatories along Cascadia, Chile, and Indonesia - other corners of the Pacific “Ring of Fire” - could reveal whether those margins harbor their own stealthy slow quakes or remain locked tight to the trench. 



The answer would refine tsunami-hazard forecasts and perhaps buy coastal communities critical minutes of warning.



<h2 class="wp-block-heading" id="h-creeping-fault-limits-big-earthquakes">Creeping fault limits big earthquakes</h2>



Taken together, the 2015 and 2020 Nankai slow-slip episodes suggest the shallow <a href="https://www.earth.com/news/most-dangerous-part-of-this-west-coast-earthquake-fault-cascadia-subduction-zone/">fault</a> functions more like a tectonic shock absorber than a ticking bomb. By periodically releasing energy, it might reduce how much strain transfers to deeper, more dangerous segments.



Yet the scientists caution against complacency. The deeper Nankai interface and neighboring segments could still fail suddenly, as history shows.



For now, geophysicists are analyzing the rich new dataset to model how fluids, <a href="https://www.earth.com/news/solar-heat-and-earthquake-activity-is-there-a-connection/">temperature</a>, and rock composition govern the transition from silent creep to violent rupture.



Each slow-slip event is another frame in an expanding time-lapse of the earthquake cycle - one that could eventually reveal when the next big snap is likely to occur.



<h2 class="wp-block-heading" id="h-hearing-earthquakes-before-they-roar">Hearing earthquakes before they roar</h2>



Catch a fault in the middle of a slow-motion glide and you learn a simple truth: not every earthquake shouts. Some only whisper, rippling quietly through kilometres of rock.



By wiring the seabed for sound, scientists have begun to hear those whispers and, with them, the hidden conversations that decide when Earth decides to roar.



The study is published in the journal <a href="https://www.science.org/doi/10.1126/science.ads9715">Science</a>.



Image Credit: Japan Meteorological Agency 



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Scientists detect a rare slow-motion earthquake along Japan’s tsunami fault

Far beneath the Pacific, where the Philippine Sea Plate dives...

Being cool can feel elusive and almost mythic - something we “know when we see it,” yet struggle to define.



A sweeping new investigation led by marketing scholars Todd Pezzuti of <a href="https://www.uai.cl/">Universidad Adolfo Ibáñez</a> and Caleb Warren of the <a href="https://www.arizona.edu/">University of Arizona</a> argues that the concept is far less mysterious than it seems.



Across twelve nations, nearly 6,000 participants independently picked out the same constellation of <a href="https://www.earth.com/news/personality-type-can-accurately-predict-your-relationship-status/">personality</a> traits when describing a cool person. 



The findings reveal not only what separates “cool” from “good” but also why cool people tend to become catalysts of social change.



<h2 class="wp-block-heading" id="h-mapping-cool-across-12-nations">Mapping cool across 12 nations</h2>



Between 2018 and 2022, the research team collected online responses from adults in the United States, Australia, Chile, mainland China, Hong Kong, Germany, India, Mexico, Nigeria, Spain, South Africa, South Korea, and Turkey.



Participants first confirmed that they understood the slang meaning of the word “cool,” then spent a few minutes imagining someone who embodied one of four labels: cool, uncool, good, or not good.



Afterward, volunteers evaluated that imagined person on a battery of personality dimensions drawn from psychology’s “Big Five” model and Schwartz’s theory of universal values.



Because all responses came from internet users in relatively urban settings, the sample leans toward technologically connected citizens. 



Still, it is one of the most culturally diverse datasets ever assembled to study reputational judgments. The result is a uniquely global snapshot of how people assign social prestige.



<h2 class="wp-block-heading" id="h-where-cool-and-good-part-ways"><a></a>Where cool and good part ways</h2>



When the investigators compared ratings, they found considerable overlap: both cool and good people scored high on <a href="https://www.earth.com/news/people-with-many-facial-expressions-seem-more-social-and-likeable/">likability</a>. Yet important divergences emerged.



In all the places they studied, people consistently perceived cool individuals as more extraverted, hedonistic, powerful, adventurous, open, and autonomous. 



Good people, by contrast, ranked as conforming, traditional, secure, warm, agreeable, universalistic, conscientious, and calm.



<h2 class="wp-block-heading" id="h-cool-people-aren-t-always-good">Cool people aren't always "good"</h2>



In Pezzuti’s view, the cool profile evokes a kind of charismatic boundary-pusher: energetic, novelty seeking, and unapologetically self-directed.



That explains why cool individuals can inspire fashion trends or launch creative movements - roles that sometimes require bending social rules rather than following them.



“To be seen as cool, someone usually needs to be somewhat likable or admirable, which makes them similar to good people," said Warren. "However, cool people often have other traits that aren’t necessarily considered ‘good’ in a moral sense, like being hedonistic and powerful.”



The cool persona therefore straddles acceptance and transgression: admired enough to influence peers, rebellious enough to feel fresh.



<h2 class="wp-block-heading" id="h-cool-traits-go-global">Cool traits go global</h2>



In the mid-20th century, “cool” circulated in small countercultures - from Black jazz clubs to Beatnik cafés. Over the decades, fashion labels, record companies and Hollywood studios harnessed the aura of cool, broadcasting certain looks and attitudes to a worldwide audience.



The new study suggests that process may have standardized the meaning of the term. Even participants who live 10,000 miles apart now recognize the same signature <a href="https://www.earth.com/news/personality-traits-linked-to-willingness-to-volunteer-or-donate/">traits</a>. As the authors note, the meaning of cool has crystallized on a similar set of traits and values around the world.



Pezzuti does not see commercialization as a death knell. “Coolness has definitely evolved over time, but I don’t think it has lost its edge. It’s just become more functional,” he said.



“The concept of coolness started in small, rebellious sub-cultures, including Black jazz musicians in the 1940s and the beatniks in the 1950s. As society moves faster and puts more value on creativity and change, cool people are more essential than ever.”



<h2 class="wp-block-heading" id="h-why-coolness-matters">Why coolness matters</h2>



Because cool people display power and autonomy while earning admiration, the researchers argue that coolness helps establish informal hierarchies. Instead of relying solely on wealth or institutional authority, communities also elevate figures who embody daring and originality.



These individuals, in turn, shape cultural norms by modeling alternative ways to dress, speak, or live. As Pezzuti puts it, “everyone wants to be cool, or at least avoid the stigma of being uncool, and society needs cool people because they challenge norms, inspire change, and advance culture.”



That dual role - both aspirational and disruptive - makes the cool persona uniquely influential. Marketers know this instinctively when they cast charismatic musicians in sneaker ads. Activists harness it when they infuse protest art with edgy style.



The study provides empirical backing for those intuitions: people from Lagos to Los Angeles consistently associate coolness with adventurous independence.



<h2 class="wp-block-heading" id="h-coolness-in-the-digital-age">Coolness in the digital age</h2>



The team notes their study excludes rural and offline groups, whose ideas of cool may differ significantly. They also restricted the study to cultures already familiar with the English slang term, potentially narrowing linguistic nuance.



Future projects could test whether the six-trait profile - extraverted, hedonistic, powerful, adventurous, open, and autonomous - holds in additional societies or emerges in other languages.



Researchers are likewise curious about how <a href="https://www.earth.com/news/social-media-pressure-is-straining-teen-friendships/">social media</a> platforms, which accelerate the spread of trends, might further synchronize or fragment global standards of cool. Does TikTok broaden identity through niche subcultures or reinforce the six-trait mold by favoring charismatic risk-takers?



For now, the evidence is striking: when people across five continents imagine someone undeniably cool, they picture remarkably similar qualities. 



Coolness, it turns out, may be one of the few cross-cultural constants - an unwritten code that transcends borders even as it keeps pushing boundaries.



The study is published in the <a href="https://psycnet.apa.org/doiLanding?doi=10.1037%2Fxge0001799">Journal of Experimental Psychology: General</a>.



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What makes people cool? Scientists tracked down the traits

Being cool can feel elusive and almost mythic - something...

For decades, oceanographers assumed the surface waters circling Antarctica were becoming progressively fresher - a shift that helped lock deep heat away and nurture expansive winter sea ice.



However, new observations show the opposite is now happening. An international team led by the <a href="https://www.southampton.ac.uk/">University of Southampton</a> reported a sudden rise in surface <a href="https://www.earth.com/news/salinity-is-rising-in-coastal-areas-and-hurting-farmlands/">salinity</a> south of 50° latitude. This shift coincided with the steepest drop in Antarctic sea-ice extent ever recorded.



The analysis combines European satellite data with readings from autonomous floats that profile the water column. The result reveals an unanticipated pivot in the Southern Ocean’s salt balance sometime after 2015.



<h2 class="wp-block-heading" id="h-excessive-salt-melts-sea-ice">Excessive salt melts sea ice</h2>



Cold, fresh surface water normally overlies warmer, saltier layers at depth, creating strong density “stratification” that traps heat below. When the surface grows saltier, that barrier weakens. Heat then mixes upward, <a href="https://www.earth.com/news/antarcticas-melting-ice-shelves-threaten-global-sea-levels/">melting sea ice</a> from beneath and preventing extensive winter growth.



“Saltier surface water allows deep ocean heat to rise more easily, melting sea ice from below," said lead author Alessandro Silvano, an oceanographer at the University of Southampton. "It's a dangerous feedback loop: less ice leads to more heat, which leads to even less ice.” 



Since 2015, the continent has shed sea ice equivalent to the area of Greenland. Researchers call it the largest environmental shift detected anywhere on Earth in recent decades.



<h2 class="wp-block-heading" id="h-sea-ice-hole-returns-after-decades">Sea ice hole returns after decades</h2>



One striking symptom is the re-opening of the <a href="https://www.earth.com/news/massive-hole-polynya-the-size-of-switzerland-appeared-in-the-antarctica-sea-ice/">Maud Rise polynya</a> - a yawning hole in the Weddell Sea ice cover. It spans nearly four times the size of Wales and last appeared in the late 1970s.



“The return of the Maud Rise polynya signals just how unusual the current conditions are,” Silvano said. “If this salty, low-ice state continues, it could permanently reshape the Southern Ocean - and with it, the planet.”



Reduced Antarctic ice darkens the ocean, absorbing more sunlight and already feeding back into the global climate system. This, as Silvano put it, will give rise to “stronger <a href="https://www.earth.com/news/rapid-antarctic-sea-ice-loss-is-causing-severe-storms-around-the-world/">storms</a>, warmer oceans, and shrinking habitats for Antarctic wildlife.”



<h2 class="wp-block-heading" id="h-old-predictions-fall-short">Old predictions fall short</h2>



Climate models had projected eventual Antarctic sea-ice loss under greenhouse forcing. However, many scientists believed that enhanced snowfall and increased melt from continental ice sheets would keep surface waters fresh for decades, delaying large declines. The new evidence challenges that assumption.



“While scientists expected that human-driven climate change would eventually lead to Antarctic sea ice decline, the timing and nature of this shift remained uncertain,” said co-author Aditya Narayanan, a physical oceanographer at the University of Southampton.



“Previous projections emphasized enhanced surface freshening and stronger ocean stratification, which could have supported sustained sea ice cover. Instead, a rapid reduction in sea ice - an important reflector of solar radiation - has occurred, potentially accelerating global warming.”



<h2 class="wp-block-heading" id="h-eyes-on-the-southern-ocean">Eyes on the Southern Ocean</h2>



Because this turnaround was detected only after <a href="https://www.earth.com/news/satellites-reveal-a-sudden-drop-in-global-freshwater-levels/">satellites</a> began tracking sea-surface salinity in detail, researchers worry that other rapid transitions might be missed without constant observation.



“The new findings suggest that our current understanding may be insufficient to accurately predict future changes,” said senior author Alberto Naveira Garabato, a professor of physical oceanography at the University of Southampton.



“It makes the need for continuous satellite and in-situ monitoring all the more pressing, so we can better understand the drivers of recent and future shifts in the ice-ocean system.”



<h2 class="wp-block-heading" id="h-sea-ice-loss-changes-the-planet">Sea ice loss changes the planet</h2>



Antarctic sea ice acts as a reflective shield, bouncing sunlight back to space and modulating heat exchange between ocean and atmosphere.



Its precipitous decline could amplify warming worldwide, disturb wind patterns, and alter the formation of the deep water masses that power global ocean circulation.



Saltier surface layers may also influence how much carbon the <a href="https://www.earth.com/news/carbon-storage-mystery-emerges-in-the-southern-ocean/">Southern Ocean</a> can absorb, potentially weakening one of Earth’s most important climate buffers.



<h2 class="wp-block-heading" id="h-heat-and-salt-reinforce-sea-ice-loss">Heat and salt reinforce sea ice loss</h2>



The study leaves open questions about what triggered the sudden salinity jump. Possibilities include shifts in wind patterns, changes in precipitation, or increased intrusion of warm Circumpolar Deep Water onto the continental shelf.



Whatever the cause, the new feedback between salt and sea ice could lock the region into a self-reinforcing cycle of warming and ice loss.



Scientists stress that only sustained measurements - combining satellites, autonomous floats, and ship-based surveys - will reveal whether the Southern Ocean snaps back to its former fresher state or continues toward an unfamiliar, saltier future.



For now, the message is clear: Antarctica’s floating fringe, once thought relatively resistant to near-term change, is undergoing a rapid transformation that matters far beyond the frozen continent.



The study is published in the journal <a href="https://www.pnas.org/doi/10.1073/pnas.2500440122">Proceedings of the National Academy of Sciences</a>.



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Antarctic sea ice collapse linked to a sudden surge in ocean salt

For decades, oceanographers assumed the surface waters circling Antarctica were...

Scientists are transforming chocolate into a functional food by infusing it with probiotics and prebiotics, aiming to create a treat that satisfies cravings while supporting gut health. 



The challenge lies in maintaining chocolate's beloved texture and flavor while adding health benefits.



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Probiotics - beneficial microbes that balance gut bacteria and aid digestion - are typically fragile and can be destroyed by stomach acid or processing. 



Prebiotics act as food for these microbes, helping them thrive. Together, they form "synbiotics," a powerful health combination.



Researchers Smriti Gaur and Shubhi Singh from India's Jaypee Institute of Information Technology took an innovative approach, using natural prebiotics like corn and honey instead of complex processing methods. 



They created five chocolate varieties: a control and four synbiotic versions containing different combinations of prebiotics, probiotics (Lactobacillus strains), and flavor enhancers (cinnamon or orange).



Laboratory simulations of human digestion showed the probiotics remained viable for over five hours, suggesting they could survive long enough to benefit gut health.



Taste tests were positive, with researchers particularly enjoying the orange-flavored variety, describing it as having "vibrant citrus notes" complementing the "rich cocoa" with a "luxurious" texture.



This research represents just the beginning. With further refinement of strains, textures, and flavors, chocolate could evolve beyond mere indulgence to become a functional food that nourishes while it delights.



The study is published in the journal <a href="https://pubs.acs.org/doi/10.1021/acsfoodscitech.4c00741" target="_blank" rel="noreferrer noopener">ACS Food Science &amp; Technology</a>.

Is chocolate the next nutritional powerhouse?

Scientists are transforming chocolate into a functional food by infusing...

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Nushagak Bay, a large estuary in southwest Alaska. Nushagak runs mainly north to south and exits in Bristol Bay, a large body of water in the Bering Sea.



"The bay is primarily fed by the Nushagak River, which begins in the Alaska Range and flows southwest approximately 450 km. The bay is also fed by several additional rivers including the Wood, Igushik, Snake and Weary rivers," says ESA.



"The dark colors of the Nushagak River are most likely due to tannins or lignins (chemical substances found in plants). Tannins and lignins from roots, leaves, seeds, bark and soil can leach into the water and give it a brown or even black colour. The sediments then flow southwards where it is mixed with the bluer waters of the bay."



Video/ Image Credit: ESA



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By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer

Nushagak Bay in southwest Alaska

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Today's Video of the Day from the <a href="https://www.acs.org/">American Chemical Society</a> (ACS) reveals that proteins on flu viruses are actually flexible, tilting and waving in a “breath-like” motion. According to the experts, these proteins could be used to better defend against the flu.



"The main antigenic targets of influenza virus are two surface glycoproteins, hemagglutinin (HA) and neuraminidase (NA). Whereas the structural and dynamical properties of both glycoproteins have been studied previously, the understanding of their plasticity in the whole-virion context is fragmented," wrote the researchers.



To investigate, the team conducted detailed simulations of the influenza A H1N1 virion, or the swine flu. The experts concluded that the visualizations show many new vulnerable states of flu viruses, which could improve future vaccines and antiviral drugs.



Video/ Image Credit: American Chemical Society&nbsp;



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By <a href="mailto:csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Editor



Check us out on <a href="https://www.earth.com/earthsnap/">EarthSnap</a>, a free app brought to you by Eric Ralls and Earth.com.

Flu viruses are more flexible than expected

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Lake Trasimeno, which is located west of Perugia in central Italy. It is the fourth largest lake in the country. While Trasimeno’s water level varies, it has a maximum depth of approximately six meters.&nbsp;



"In this Copernicus Sentinel-2 image, captured on 6 August 2022, the lake’s emerald green colour is likely due to the presence of phytoplankton. Streaks in the water, particularly visible in the west, indicate the presence of soil and sediments which have been stirred up by winds. Dark colored waters in the southern part of the lake indicate a presence of submerged and floating macrophytes (aquatic plants) as well as algae," says ESA.



"Surrounded by hills on three sides, Trasimeno is subject to heavy storms created by winds, especially from the north and west. There are three islets in the lake: Maggiore, Minore and Polvese (the largest). The lake’s shores are sparsely inhabited with only two popular villages: Castiglione del Lago and Passignano sul Trasimeno."



"Italy is experiencing its worst drought in 70 years which has affected drinking water supplies, hydroelectric power and agricultural production. High temperatures, hot winds and lack of rainfall are the main causes of drought in the Umbrian region which saw Lake Trasimeno’s drop 1.3 m, reaching the limit of the hydrometric zero in July 2022."



Video/Image Credit: ESA&nbsp;



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By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer

Lake Trasimeno in Central Italy

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Today's Video of the Day from the <a href="https://www.acs.org/">American Chemical Society</a> describes a new self-powered nanosensor that can instantly detect mercury contamination with the tap of a finger.&nbsp;



The oxidized form of mercury can be harmful when it is ingested through contaminated water or food. This makes it necessary for experts to develop sensors that can quickly and accurately detect the presence of mercury.&nbsp;



Zong-Hong Lin and colleagues have now created a triboelectric nanosensor (TENS) that can detect mercury by simply by touching a sample. According to the researchers, their TENS could serve as the basis for similar devices to safely and remotely monitor other pollutants.



Video Credit: American Chemical Society&nbsp;



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By <a href="mailto:csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Editor



Check us out on <a href="https://www.earth.com/earthsnap/">EarthSnap</a>, a free app brought to you by Eric Ralls and Earth.com.

Detecting mercury contamination with the tap of a finger

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Kainji Lake, a reservoir on the Niger River.



In 1968, Kainji Lake was created by the construction of the Kainji Dam. The Niger River, the third longest in Africa, enters the lake in the north.&nbsp;



According to <a href="https://www.earth.com/news/rivers-in-the-american-west-are-a-lifesaving-resource-for-birds/">ESA</a>, the creation of the lake submerged Foge Island and the town of Bussa and permanently flooded other riverine settlements, leaving around 50,000 people displaced.&nbsp;



Large parts of Foge Island are temporarily exposed during low water tides, and the land is often used by migrating fishermen. Kainji Dam is a dam across the Niger River in Niger State of Central Nigeria. 



Wild mammals occur at relatively low densities due to illegal hunting. Lake Kainji has suffered a dramatic decline as a fishery due to the high numbers of artisanal and subsistence fisherfolk using the lake. It has been suggested that a period of closure, together with controlled fishing rights may help improve fish stocks.



Kainji Lake National Park is the oldest of its kind in Nigeria. The park contains three distinct areas: a part of the Kainji Lake, the Borgu Game Reserve to the west of the lake, and the Zugurma Game Reserve to the southeast. The park is home to around 65 mammal species, 350 bird species, and 30 species of reptiles and amphibians. 



Video/ Image Credit: European Space Agency&nbsp;



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By <a href="mailto:csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Editor



Check us out on <a href="https://www.earth.com/earthsnap/">EarthSnap</a>, a free app brought to you by Eric Ralls and Earth.com.

Kainji Lake in north central Nigeria

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“Lewisham is one of the poorest boroughs in London and this mass dumping of carrots at Goldsmiths is beyond insensitive. It’s a massive slap in the face,&#8221; read one Instagram post. Soon, critics grew louder.

Slap in the Face

News coming your way