Today's Image of the Day from the European Space Agency features the barred spiral galaxy NGC 3783, which is located about 130 million light-years away in the constellation Centaurus. 



NGC 3783 is also the most prominent of a galaxy group (by the same name) that contains 47 galaxies.&nbsp;



<h2 class="wp-block-heading" id="h-galaxy-groups">Galaxy groups</h2>



“Like galaxy clusters, galaxy groups are aggregates of gravitationally bound galaxies. Galaxy groups, however, are less massive and contain fewer members than <a href="https://www.earth.com/news/titanic-galaxy-cluster-collision-defies-all-current-understanding-of-the-universe/" target="_blank" rel="noreferrer noopener">galaxy clusters</a> do: where galaxy clusters can contain hundreds or even thousands of constituent galaxies, galaxy groups do not typically include more than 50,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



“The Milky Way is actually part of a galaxy group, known as the Local Group, which contains two other large galaxies (Andromeda and the Triangulum galaxy), as well as several dozen satellite and dwarf galaxies.”



<h2 class="wp-block-heading" id="h-a-blue-giant-star">A blue giant star</h2>



The bright object that appears to the right of the galaxy is the star HD 101274. “The perspective in this image makes the star and the galaxy look like close companions, but this is an illusion. HD 101274 lies only about 1,530 light-years from Earth, meaning it is about 85 thousand times closer than NGC 3783,” explained ESA.&nbsp;



The star is part of the NGC 3766 cluster, sometimes referred to as the Pearl Cluster, which is known for its richness in bright stars and its relatively young age.



Characterized by its high temperature and luminosity, HD 101274 is categorized as a blue giant star.



<h2 class="wp-block-heading" id="h-significance-of-blue-giants">Significance of blue giants</h2>



Blue giants are massive stars that have left the main sequence phase of stellar evolution and are burning helium or heavier elements in their cores. These stars are known for their short lifespans relative to smaller stars due to their rapid consumption of nuclear fuel.



<a href="https://www.earth.com/news/dark-stars-scientists-discover-a-new-type-of-star-powered-by-dark-matter/" target="_blank" rel="noreferrer noopener">Stars</a> like HD 101274 are important for astronomers because they help in studying the properties of stellar populations in clusters and the dynamics of stellar evolution in different environments. 



Observations of blue giant stars can provide valuable insights into the characteristics of their atmospheres, internal structures, and the processes occurring within and around them.



<h2 class="wp-block-heading" id="h-bright-central-region-of-ngc-3783">Bright central region of NGC 3783</h2>



One of the most interesting aspects of NGC 3783 is that it harbors an active galactic nucleus. This means that its central region is exceptionally luminous, likely due to the presence of a supermassive black hole. 



The black hole is actively accreting material, which emits a substantial amount of radiation as it spirals inward and heats up.



The galaxy has been studied extensively in the ultraviolet and X-ray light spectra to understand better the properties of the accretion disk around the black hole and the complex dynamics of the material surrounding it. 



These studies are crucial for understanding the physics of active galactic nuclei and the role they play in <a href="https://www.earth.com/news/galaxies-like-our-own-milky-way-are-not-unique/" target="_blank" rel="noreferrer noopener">galaxy evolution</a>.



According to ESA, NGC 3783 is a&nbsp;Type I Seyfert galaxy. “In this image it is recorded by Hubble in incredible detail, from its glowing central bar to its narrow, winding arms and the dust threaded through them, thanks to five separate images taken in different wavelengths of light," noted ESA.



“In fact, the galactic center is bright enough to Hubble that it exhibits diffraction spikes, normally only seen on stars such as HD 101274.”



<h2 class="wp-block-heading" id="h-ngc-3783-galaxy-group">NGC 3783 galaxy group</h2>



The NGC 3783 group is part of the larger Hydra-Centaurus Supercluster, which itself is a massive collection of <a href="https://www.earth.com/news/shapes-of-one-million-galaxies-hint-at-the-universes-origins/" target="_blank" rel="noreferrer noopener">galaxies</a> and galaxy clusters located primarily in the constellations of Hydra and Centaurus.



The NGC 3783 group consists of several galaxies that are gravitationally bound and interact with each other. These interactions can influence the galaxies' evolution through mechanisms like tidal forces and merger events, which can trigger star formation, fuel central black holes, and reshape the galaxies' structures.



Studying the NGC 3783 group helps astronomers understand how <a href="https://www.earth.com/news/ceers-2112-ancient-galaxy-looks-strikingly-similar-to-ours/" target="_blank" rel="noreferrer noopener">galaxies</a> evolve together in a common gravitational environment, offering insights into the dynamics and evolution of structures on cosmic scales.



Image Credit: ESA/Hubble &amp; NASA



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Luminous spiral galaxy and a blue giant star

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

Today's Image of the Day from the European Space Agency features a pair of interacting spiral galaxies known as the Antennae Galaxies. They are located approximately 45 million light-years away in the constellation Corvus.&nbsp;



<h2 class="wp-block-heading" id="h-antennae-galaxies-in-a-deadly-embrace">Antennae Galaxies in a deadly embrace </h2>



“The NASA/ESA Hubble Space Telescope has snapped the best ever image of the Antennae Galaxies. Hubble has released images of these stunning galaxies twice before, once using observations from its Wide Field and Planetary Camera 2 (WFPC2) in 1997, and again in 2006 from the Advanced Camera for Surveys (ACS),” noted <a href="https://esahubble.org/images/potw1345a/" target="_blank" rel="noreferrer noopener">ESA</a>.



“The galaxies - also known as NGC 4038 and NGC 4039 - are locked in a deadly embrace. Once normal, sedate spiral galaxies like the Milky Way, the pair have spent the past few hundred million years sparring with one another.”



According to ESA, the clash of the Antennae Galaxies is so violent that stars have been ripped from their host <a href="https://www.earth.com/news/galaxy-collision-2-million-mph-stephans-quintet-captured-unprecedented-detail/" target="_blank" rel="noreferrer noopener">galaxies</a> to form a streaming arc between the two.&nbsp;



The name of the galaxy pair comes from this long stream of stars and gas, which resembles insect antennae.



<h2 class="wp-block-heading" id="h-intense-bursts-of-star-formation-nbsp">Intense bursts of star formation&nbsp;</h2>



The collision has triggered intense bursts of star formation, making the Antennae Galaxies one of the nearest and most dramatic examples of a starburst galaxy.&nbsp;



Many of the newly formed stars are concentrated in massive star clusters, some of which are expected to evolve into globular clusters over millions of years.



“This new image of the Antennae Galaxies shows obvious signs of chaos. Clouds of gas are seen in bright pink and red, surrounding the bright flashes of blue star-forming regions - some of which are partially obscured by dark patches of dust,” explained ESA.



“The rate of star formation is so high that the Antennae Galaxies are said to be in a state of starburst, a period in which all of the gas within the galaxies is being used to form stars.”&nbsp;



“This cannot last forever and neither can the separate galaxies; eventually the nuclei will coalesce, and the galaxies will begin their retirement together as one large elliptical galaxy.”



<h2 class="wp-block-heading" id="h-significance-of-the-antennae-galaxies">Significance of the Antennae Galaxies</h2>



The Antennae Galaxies are one of the most well-studied examples of galaxy collisions - offering insight into the processes that shape galaxies over time.



Astronomers study the Antennae Galaxies using a range of telescopes across different wavelengths, including visible light, infrared, and X-rays.&nbsp;



Observations in X-rays have revealed evidence of supernovae and <a href="https://www.earth.com/news/black-holes-may-talk-to-galaxies-through-energetic-winds/" target="_blank" rel="noreferrer noopener">black holes</a>, while infrared studies highlight regions of dust and star formation.&nbsp;



<h2 class="wp-block-heading" id="h-the-milky-way-s-collision-course-nbsp">The Milky Way's collision course&nbsp;</h2>



The Antennae Galaxies provide a glimpse into the future of our <a href="https://www.earth.com/news/uma3-u1-faintest-star-system-found-orbiting-milky-way-galaxy/" target="_blank" rel="noreferrer noopener">Milky Way</a>, which is expected to eventually merge with the Andromeda Galaxy - our closest spiral galaxy neighbor.



The cosmic collision course of the Milky Way and Andromeda will reshape both galaxies over billions of years.&nbsp;



This event is expected to occur in about 4.5 billion years. Both galaxies are part of the Local Group, a cluster of galaxies bound together by gravity. Their mutual gravitational pull is drawing them closer at a speed of approximately 110 kilometers per second.



<h2 class="wp-block-heading" id="h-the-birth-of-an-elliptical-galaxy-nbsp">The birth of an elliptical galaxy&nbsp;</h2>



When the two galaxies collide, their individual stars will largely avoid direct collisions due to the vast distances between them. However, the gravitational forces involved will create dramatic effects.&nbsp;



These forces will distort the galaxies' <a href="https://www.earth.com/news/shapes-of-one-million-galaxies-hint-at-the-universes-origins/" target="_blank" rel="noreferrer noopener">shapes</a>, triggering intense bursts of star formation as gas clouds collide and compress. Over time, the galaxies will settle into a new, larger elliptical galaxy often referred to as "Milkomeda" or "Milkdromeda" by astronomers.



<h2 class="wp-block-heading" id="h-galaxy-merger-and-the-solar-system">Galaxy merger and the solar system</h2>



Despite the seemingly destructive nature of the collision, the solar system is unlikely to face direct harm. Our Sun may find itself flung into a new orbit within the merged galaxy or even cast into intergalactic space.&nbsp;



The merger will also significantly alter the night sky, with the Andromeda Galaxy becoming increasingly prominent before blending into the unified structure.



This event is part of the natural <a href="https://www.earth.com/news/galaxies-are-much-bigger-than-we-originally-believed-gas-clouds/" target="_blank" rel="noreferrer noopener">evolution of galaxies</a> and serves as a fascinating reminder of the dynamic and ever-changing nature of the universe. 



While the collision is still billions of years away, studying it helps astronomers understand galactic interactions and the long-term future of our cosmic neighborhood.



Image Credit: ESA/Hubble &amp; NASA



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Violent clash of the Antennae Galaxies  

Today's Image of the Day from the European Space Agency features a Copernicus Sentinel-2 photograph of South Georgia, a remote and rugged island located in the southern Atlantic Ocean. 



"Linked with the South Sandwich Islands to form a British Overseas Territory, this southern Atlantic island is a haven for a vast array of wildlife," said <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"Around five million seals call the islands home, as well as 65 million birds of 30 different species. Migrating whales and various fish species populate the surrounding waters and there is a large penguin population."



<h2 class="wp-block-heading" id="h-climate-and-wildlife-of-south-georgia">Climate and wildlife of South Georgia </h2>



The island is dominated by mountains, glaciers, and fjords. Its highest peak, Mount Paget, rises to 2,935 meters, making it one of the tallest in the region.



South Georgia’s location within the Antarctic Convergence gives it a cold, maritime climate. Although not part of the Antarctic Treaty System, its environment and <a href="https://www.earth.com/news/conservation-efforts-are-not-enough-to-save-antarctic-wildlife/" target="_blank" rel="noreferrer noopener">wildlife</a> are closely linked to Antarctica. 



The island is home to vast colonies of penguins, seals, and seabirds. The surrounding waters are rich with krill, providing an abundant food source for marine life.



<h2 class="wp-block-heading" id="h-penguins-adapted-to-harsh-environments">Penguins adapted to harsh environments </h2>



The most notable species found here are the king penguins, which are the second-largest penguin species in the world. South Georgia also hosts large populations of <a href="https://www.earth.com/news/what-makes-the-gentoo-penguin-the-worlds-fastest-swimming-bird/" target="_blank" rel="noreferrer noopener">gentoo</a> and macaroni penguins. 



The island's harsh climate, characterized by strong winds, snow, and cold temperatures, makes it a tough environment, but the penguins have adapted well. 



Their colonies - some of which number in the hundreds of thousands - can be found along the island's rugged coasts and beaches. 



The island’s isolation, combined with its plentiful food supply, makes it a critical breeding ground for these penguins.



<h2 class="wp-block-heading" id="h-history-of-south-georgia">History of South Georgia </h2>



The island has a history of exploration and exploitation. Captain James Cook first claimed South Georgia for Britain in 1775. 



During the late 19th and early 20th centuries, it became a hub for the <a href="https://www.earth.com/news/echoes-of-the-past-whalings-long-term-impact-on-genetic-diversity/" target="_blank" rel="noreferrer noopener">whaling</a> industry, with stations like Grytviken serving as operational centers. These stations have since been abandoned, and the island is now a haven for scientific research and ecotourism.



South Georgia is also notable for its role in Ernest Shackleton’s famed Endurance expedition. His crew reached the island in 1916 after an extraordinary open-boat journey from Elephant Island. Shackleton later died on South Georgia in 1922 and is buried in Grytviken.



<h2 class="wp-block-heading" id="h-pristine-nature-of-the-island">Pristine nature of the island</h2>



Today, South Georgia is a focus of conservation efforts. The eradication of invasive species, such as rats and reindeer, has been a significant success, allowing native wildlife to recover. 



Rats and mice were responsible for the decline of ground-nesting birds, including the South Georgia pipit, the island's only endemic bird. 



<a href="https://www.earth.com/news/reindeer-use-ultraviolet-vision-to-find-food-in-the-winter/" target="_blank" rel="noreferrer noopener">Reindeer</a>, which had been introduced for farming in the 19th century, caused extensive damage to the island’s vegetation, disrupting the habitat for native species.



South Georgia is uninhabited except for a small number of scientists and staff working at research stations and administrative facilities, emphasizing its role as a protected wilderness area and an essential site for understanding global environmental changes.



Its uninhabited status has helped preserve its pristine nature. Visitors to South Georgia must follow strict environmental guidelines to minimize human impact on this extraordinary island.



<h2 class="wp-block-heading" id="h-scientific-significance-of-remote-islands">Scientific significance of remote islands </h2>



Remote <a href="https://www.earth.com/news/plant-life-on-islands-loses-diversity-when-humans-arrive/" target="_blank" rel="noreferrer noopener">islands</a> are scientifically significant for several reasons. They often serve as unique ecosystems that can provide insights into evolutionary processes, biodiversity, and adaptation. 



Due to their isolation, species on remote islands may evolve differently from their mainland counterparts, resulting in the development of endemic species that exist nowhere else in the world. 



These islands also act as natural laboratories for studying the effects of climate change, human activity, and ecological interactions, as they are more vulnerable to disturbances. 



Moreover, remote islands can offer valuable information on the health of marine and terrestrial ecosystems, as their ecosystems are often less impacted by human-induced factors. This makes them ideal for studying natural processes in relatively undisturbed environments. 



The isolation of these islands can also help scientists study the patterns of species migration, colonization, and extinction.



Image Credit: ESA 



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South Georgia: One of the most remote islands in the world

Today's Image of the Day from the European Space Agency features NGC 6744 - a large, barred spiral galaxy located approximately 30 million light-years away in the constellation Pavo.&nbsp;



The galaxy is often considered a close analog to the <a href="https://www.earth.com/news/uma3-u1-faintest-star-system-found-orbiting-milky-way-galaxy/" target="_blank" rel="noreferrer noopener">Milky Way</a> due to its similar structure and size, spanning about 175,000 light-years across.&nbsp;



<h2 class="wp-block-heading" id="h-euclid-space-mission-nbsp">Euclid space mission&nbsp;</h2>



The image was captured by the <a href="https://www.esa.int/Science_Exploration/Space_Science/Euclid" target="_blank" rel="noreferrer noopener">Euclid</a> space telescope. NGC 6744 stands out as a prime example of the galaxies currently forming the majority of stars in the nearby universe, making it an ideal subject for study with the Euclid mission.&nbsp;



Euclid’s extensive field-of-view allows it to capture the entire galaxy, showcasing not only its large-scale spiral structure but also revealing intricate details on smaller scales across various wavelengths. These details include feather-like dust lanes, known as “spurs,” emerging from the spiral arms.



<h2 class="wp-block-heading" id="h-star-formation-in-ngc-6744">Star formation in NGC 6744</h2>



Euclid's observations enable scientists to count individual stars within NGC 6744, trace the distribution of stars and dust throughout the galaxy, and map the dust associated with the gas that fuels the development of new stars.&nbsp;



<a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">Star formation</a> is a key process in the growth of galaxies, making these studies crucial for understanding galaxy evolution.



Researchers are utilizing Euclid’s data to explore the relationship between dust, gas, and star formation; to map the distribution of different stellar populations and identify regions of active star formation; and to investigate the underlying physics of spiral galaxy structures.&nbsp;



Spiral arms play a significant role in star formation by compressing gas, yet the precise mechanisms behind this process are still unclear. The presence of “spurs” along NGC 6744’s spiral arms offers valuable insights into the dynamics of star formation within these structures.



<h2 class="wp-block-heading" id="h-discovering-new-dwarf-galaxies-nbsp">Discovering new dwarf galaxies&nbsp;</h2>



Additionally, Euclid's dataset will help scientists identify clusters of old stars (globular clusters) and discover new dwarf galaxies around NGC 6744. 



Remarkably, Euclid has already identified a new dwarf satellite galaxy of NGC 6744 - a surprising discovery given that the galaxy has been studied extensively.



With Euclid’s detailed observations, scientists are gaining a deeper understanding of the processes shaping galaxies, providing essential clues to the evolution and appearance of the <a href="https://www.earth.com/news/universes-expansion-rate-hubble-tension-puzzles-astronomers/" target="_blank" rel="noreferrer noopener">universe</a>.



<h2 class="wp-block-heading" id="h-more-about-ngc-6744">More about NGC 6744</h2>



NGC 6744's disk is rich in star-forming regions and contains numerous young, bright blue stars. The galaxy's nucleus is slightly elongated and has a bar structure, which influences the motion of the stars and gas within it.&nbsp;



The spiral arms of NGC 6744 are well-defined and extend outward, wrapping around the central bar. 



Additionally, NGC 6744 has a smaller companion galaxy, NGC 6744A, which is interacting with it, adding to the complexity and interest of this distant system. 



<h2 class="wp-block-heading" id="h-types-of-spiral-galaxies">Types of spiral galaxies</h2>



<a href="https://www.earth.com/news/the-mesmerizing-beauty-of-spiral-galaxies/" target="_blank" rel="noreferrer noopener">Spiral galaxies</a> are one of the most common types of galaxies in the universe, characterized by their distinct, spiral-shaped structure.&nbsp;



The galaxies typically consist of a flat, rotating disk containing stars, gas, and dust, along with a central concentration of stars known as the bulge. This bulge is often surrounded by a halo of older stars.&nbsp;



The spiral arms, which extend from the central bulge, are regions of active star formation and are rich in young, hot stars, giving them a bright, bluish appearance.&nbsp;



These arms are also sites where interstellar gas and dust are concentrated, leading to the formation of new stars.&nbsp;



Spiral galaxies are classified into different types based on the tightness of their spirals and the size of their central bulge, with classifications ranging from tightly wound arms in Sa galaxies to more loosely wound arms in Sc galaxies. The <a href="https://www.earth.com/news/large-amount-of-dark-matter-may-be-missing-from-the-milky-way/" target="_blank" rel="noreferrer noopener">Milky Way</a>, our home galaxy, is a prime example of a spiral galaxy.



<h2 class="wp-block-heading" id="h-the-constellation-pavo">The constellation Pavo</h2>



Pavo, which means "peacock" in Latin, is a constellation in the southern sky. It was named by the Dutch astronomer Petrus Plancius in the late 16th century, based on observations made during the Dutch explorations of the southern hemisphere. 



Pavo is one of the 12 constellations created by Plancius from the records of explorers Pieter Dirkszoon Keyser and Frederick de Houtman. 



The constellation is known for its distinctive shape, resembling a peacock with a long, curved tail. Pavo is not visible from most of the northern hemisphere, but it can be seen from the southern hemisphere, particularly during the winter months.



The constellation contains several interesting celestial objects, including the star Peacock, also known as Alpha Pavonis, which is the brightest star in the constellation. This star is a blue-white subgiant located about 179 light-years from Earth.



Image Credit: <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>/Euclid/Euclid Consortium/NASA&nbsp;



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Young stars illuminate a spiral galaxy in the constellation Pavo

Today's Image of the Day from the European Space Agency features the galaxy I Zwicky 18, which was captured in remarkable detail by the James Webb Space Telescope.



I Zwicky 18 is a blue compact dwarf <a href="https://www.earth.com/news/newly-discovered-stars-milky-way-are-old-as-universe/" target="_blank" rel="noreferrer noopener">galaxy</a> located approximately 59 million light-years away in the constellation Ursa Major.&nbsp;



<h2 class="wp-block-heading" id="h-star-formation-in-i-zwicky-18">Star formation in I Zwicky 18</h2>



The galaxy is notable for its relatively young appearance and the fact that it contains very few heavy elements. These characteristics indicate that it has experienced little <a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">star formation</a> compared to other galaxies of similar age.



“The galaxy was first identified by Swiss astronomer Fritz Zwicky in the 1930’s and resides roughly 59 million light-years from Earth,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>. “This galaxy has gone through several sudden bursts of star formation.”&nbsp;



According to ESA, I Zwicky 18 is typical of the kinds of galaxies that inhabited the early universe and is much smaller than our <a href="https://www.earth.com/news/runaway-star-j1249-36-spotted-trying-to-escape-our-milky-way-galaxy/" target="_blank" rel="noreferrer noopener">Milky Way</a>.



<h2 class="wp-block-heading" id="h-webb-telescope-image-of-the-galaxy">Webb telescope image of the galaxy</h2>



“Two major starburst regions are embedded in the heart of the galaxy. The wispy brown filaments surrounding the central starburst region are bubbles of gas that have been heated by stellar winds and intense ultraviolet radiation unleashed by hot, young stars,” said ESA.



“A companion galaxy resides nearby to the dwarf galaxy, which can be seen at the bottom of the wider-field image. The companion may be interacting with the dwarf galaxy and may have triggered that galaxy's recent star formation.”&nbsp;



ESA explained that the “orange blobs” surrounding the galaxy are the dim glow from ancient fully formed galaxies at much larger distances.



<h2 class="wp-block-heading" id="h-key-characteristics-of-i-zwicky-18">Key characteristics of I Zwicky 18</h2>



As previously mentioned, the galaxy has a very low abundance of elements heavier than hydrogen and helium, suggesting that it has not undergone significant stellar processing.



<h3 class="wp-block-heading" id="h-young-stellar-population-nbsp">Young stellar population&nbsp;</h3>



Despite its old age, I Zwicky 18 contains many young, hot stars. This suggests that it might have experienced a burst of <a href="https://www.earth.com/news/hubble-detects-awe-inspiring-newborn-star/" target="_blank" rel="noreferrer noopener">star formation</a> relatively recently in its history.



<h3 class="wp-block-heading" id="h-interstellar-medium-nbsp">Interstellar medium&nbsp;</h3>



The galaxy has a high density of gas, which is a prime ingredient for star formation. This gas is mostly in the form of hydrogen.



<h3 class="wp-block-heading" id="h-unusual-characteristics">Unusual characteristics</h3>



Its characteristics are more typical of primordial galaxies found in the early universe, making it a valuable object of study for understanding galaxy formation and evolution.



Ultimately, I Zwicky 18 provides insights into the conditions and processes that might have been prevalent in the early universe.



<h3 class="wp-block-heading" id="h-life-cycles-of-stars-and-dust">Life cycles of stars and dust</h3>



The image was captured as part of a Webb program to study the life cycle of dust in I Zw 18.&nbsp;



“Scientists are now building off of previous research with Hubble obtained at optical wavelengths, studying individual dusty stars in detail with Webb’s equivalent spatial resolution and sensitivity at infrared wavelengths.”&nbsp;



ESA noted that this galaxy is of particular interest as its content of elements heavier than helium is one of the lowest of all known <a href="https://www.earth.com/news/early-galaxy-formation-occurred-much-faster-than-we-thought/" target="_blank" rel="noreferrer noopener">galaxies</a> in the local universe.&nbsp;



“Such conditions are thought to be similar to those in some of the first star-forming galaxies at high redshift, so the Webb study of I Zw 18 should shed light on the life-cycle of stars and dust in the early universe.”



<h2 class="wp-block-heading" id="h-the-constellation-ursa-major">The constellation Ursa Major </h2>



Ursa Major, also known as the Great Bear, is one of the most prominent and easily recognizable constellations in the northern sky. 



Its name, "Ursa Major," means "Great Bear" in Latin, and it has been a significant part of various mythologies and star lore across cultures for thousands of years. 



One of the most famous asterisms within Ursa Major is the Big Dipper, a group of seven bright stars that form a shape resembling a ladle or dipper. The Big Dipper is often used as a navigation tool because it points to Polaris, the North Star, located in the nearby constellation Ursa Minor.



Ursa Major is best viewed in the northern hemisphere and is circumpolar, meaning it is visible year-round for much of the Northern Hemisphere. Its position changes with the seasons, rotating around Polaris, the North Star.



Image Credit: NASA/ESA/CSA James Webb Space Telescope



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Dwarf galaxy provides a window into the early universe

Today's Image of the Day from the European Space Agency features the barred spiral galaxy NGC 1559, located around 35 million light-years away in the southern constellation Reticulum. The image was captured by the James Webb Space Telescope. 



"The data featured in this portrait make use of two of Webb’s instruments: the Mid-InfraRed Instrument (MIRI) and Near-InfraRed Camera (NIRCam)," noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"Here MIRI captures the glow of interstellar dust grains, which trace out the interstellar medium, the fuel for future star formation. NIRCam shows the light from stars, even young stars hidden behind prodigious amounts of dust. NIRCam also captures emission from ionized nebulae around young stars."



<h2 class="wp-block-heading" id="h-webb-reveals-galaxies-in-new-light">Webb reveals galaxies in new light</h2>



According to ESA, the data was collected by the <a href="https://sites.google.com/view/phangs/home">PHANGS team</a> as part of a program in which Webb will observe 55 <a href="https://www.earth.com/news/james-webb-captures-galaxies-that-are-too-old-to-exist/">galaxies</a> that have also been mapped by the Atacama Large Millimeter/submillimeter Array (ALMA) radio telescope, the Hubble Space Telescope, and more.&nbsp;



"By combining Webb’s unprecedented view of the dust and stars with data from these other facilities, the team aims to obtain a new, highly detailed view of how stars are born, live, and die in galaxies across the Universe."



<h2 class="wp-block-heading" id="h-ngc-1559-a-loner-in-space">NGC 1559: A loner in space</h2>



Although NGC 1559 appears to sit close to one of our nearest neighbors in the sky - the Large Magellanic Cloud (LMC) - this is just a trick of perspective, noted ESA.



While it is part of the Reticulum constellation, NGC 1559 is not part of the Local Group of galaxies but instead resides in a more distant region of space.



"In reality, NGC 1559 is physically nowhere near the LMC in space; in fact it truly is a loner, lacking the company of any nearby galaxies or membership of any galaxy cluster."



<h2 class="wp-block-heading" id="h-star-formation-in-ngc-1559">Star formation in NGC 1559</h2>



NGC 1559 is notable for its active star formation and strong magnetic fields. It has also been the site of several <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernovae</a>, making it of particular interest to astronomers who study stellar evolution and the life cycle of stars.



The structure of NGC 1559 includes well-defined spiral arms that contain young, hot stars and regions of ionized gas, indicative of ongoing <a href="https://www.earth.com/news/black-hole-is-starving-its-host-galaxy-of-star-forming-fuel/" target="_blank" rel="noreferrer noopener">star formation</a>.



<h2 class="wp-block-heading" id="h-an-extragalactic-wonder">An extragalactic wonder</h2>



Despite being relatively small compared to larger galaxies like the Milky Way, NGC 1559 is an important object for understanding how barred spiral galaxies evolve and the processes that trigger supernovae.



The galaxy’s remote location and active nature make it a fascinating subject of study in the field of extragalactic astronomy. 



The isolation of NGC 1559 allows for a clearer view of its structure without much interference from neighboring galaxies.



<h2 class="wp-block-heading" id="h-barred-spiral-galaxies">Barred spiral galaxies</h2>



Barred spiral galaxies are a type of spiral galaxy characterized by a central bar-shaped structure composed of stars. This bar extends out from the core and connects to the galaxy's spiral arms, which swirl outward in a graceful pattern.



Scientists believe that the bar plays a crucial role in the evolution of the galaxy, funneling gas towards the core and potentially triggering star formation or feeding a central black hole. 



The <a href="https://www.earth.com/news/newly-discovered-stars-milky-way-are-old-as-universe/" target="_blank" rel="noreferrer noopener">Milky Way</a>, our own galaxy, is an example of a barred spiral. These galaxies are quite common in the universe, making up about two-thirds of all observed spiral galaxies.



The bar itself is thought to be a temporary feature, developing as the galaxy matures and possibly disappearing over time as the dynamics of the stars change. 



<h2 class="wp-block-heading" id="h-the-reticulum-constellation">The Reticulum constellation</h2>



The Reticulum constellation is a small, faint constellation in the southern sky. Its name means "the reticle" in Latin, which refers to the crosshairs in an eyepiece of a telescope. 



The constellation was named in the 18th century by the French astronomer Nicolas Louis de Lacaille to honor the reticle he used in his scientific instruments. It is one of the 88 modern constellations recognized by the International Astronomical Union.



Image Credit: ESA/Webb, NASA &amp; CSA, A. Leroy, J. Lee and the PHANGS Team



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Spiral galaxy NGC 1559 is a loner in outer space

Jupiter's striking size, swirling gases, and dramatic bands in its atmosphere set it apart from every other planet. One of its most iconic features is the Great Red Spot, a storm so vast that it has defined the planet’s appearance for centuries.



Until now, much of the discussion has centered on the spectacle of that colossal storm itself. Recent observations are shining a new light on what happens above this famous vortex. 



These details open a fresh perspective on Jupiter’s upper atmosphere, revealing unexpected structures and patterns.



These findings have been led by team leader Henrik Melin of the <a href="https://le.ac.uk/" target="_blank" rel="noreferrer noopener">University of Leicester</a> in the United Kingdom. 



By focusing on the region above the Great Red Spot, researchers have broadened our understanding of ionospheric activity on the gas giant.



<h2 class="wp-block-heading" id="h-fresh-insights-on-jupiter-s-atmosphere">Fresh insights on Jupiter’s atmosphere</h2>



Astronomers used the NASA/ESA/CSA James Webb Space Telescope (<a href="https://science.nasa.gov/mission/webb/" target="_blank" rel="noreferrer noopener">JWST</a>) to look at a portion of Jupiter once thought to be nondescript. 



The instrument’s infrared capabilities allowed scientists to analyze the gas giant’s upper atmosphere, an area where sunlight plays a role but had been assumed to be uniform. 



They found that Jupiter’s distance from the Sun means it receives only 4% of the sunlight hitting Earth, so it came as a surprise to see a host of intricate activity at these heights.



The team studied this region using Webb’s Near-Infrared Spectrograph (<a href="https://science.nasa.gov/mission/webb/nirspec/" target="_blank" rel="noreferrer noopener">NIRSpec</a>). After targeting the area above the <a href="https://www.earth.com/news/jupiters-great-red-spot-shrinks-and-expands-like-a-stress-ball/" target="_blank" rel="noreferrer noopener">Great Red Spot</a>, they identified dark arcs and bright points, distributed across the field of view in ways never documented before. 



“We thought this region, perhaps naively, would be really boring,” shared team leader Henrik Melin. “It is in fact just as interesting as the northern lights, if not more so. Jupiter never ceases to surprise.”



<h2 class="wp-block-heading" id="h-wave-patterns-and-the-great-red-spot">Wave patterns and the Great Red Spot</h2>



Although solar illumination drives the light coming from this zone, something else seems to be shaping the patterns. 



“One way in which you can change this structure is by gravity waves - similar to waves crashing on a beach, creating ripples in the sand,” explained Melin. 



“These waves are generated deep in the turbulent lower atmosphere, all around the Great Red Spot, and they can travel up in altitude, changing the structure and emissions of the upper atmosphere.”



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/04/Jupiter_Great-Red-Spot_mysterious-shapes_JWST-NIRSpec_ESA_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/04/Jupiter_Great-Red-Spot_mysterious-shapes_JWST-NIRSpec_ESA_1s.webp" alt="New observations of the Great Red Spot on Jupiter have revealed that the planet’s atmosphere above and around the infamous storm is surprisingly interesting and active. This graphic shows the region observed by Webb — first its location on a NIRCam image of the whole planet (left), and the region itself (right), imaged by Webb’s Near-InfraRed Spectrograph (NIRSpec). Credit: ESA" class="wp-image-1963902"/></a><figcaption class="wp-element-caption">New observations of the Great Red Spot on Jupiter have revealed that the planet’s atmosphere above and around the infamous storm is surprisingly interesting and active. This graphic shows the region observed by Webb — first its location on a NIRCam image of the whole planet (left), and the region itself (right), imaged by Webb’s Near-InfraRed Spectrograph (NIRSpec). Click to enlarge. Credit: ESA</figcaption></figure>



The fact that Earth also experiences these phenomena is intriguing, though the effect here at home is much weaker. 



The group behind these observations hopes to follow up on these wave patterns to see how they migrate through Jupiter’s upper atmosphere and affect the energy balance of that region. 



By observing these shifts over time, scientists can refine their ideas about Jupiter’s atmospheric mechanics.



<h2 class="wp-block-heading" id="h-jupiter-s-upper-atmosphere">Jupiter's upper atmosphere</h2>



Tom Stallard, Professor of Planetary Astronomy at <a href="https://www.northumbria.ac.uk/" target="_blank" rel="noreferrer noopener">Northumbria University</a>, worked on this effort and has been studying the upper layers of gas giants for many years. 



“We used to think of a planet’s aurora as the only interesting place in terms of ionospheric activity, but these new images show that is not always the case," Stallard explained. 



“Even spacecraft which have gone to Jupiter, such as the <a href="https://science.nasa.gov/mission/juno/" target="_blank" rel="noreferrer noopener">NASA Juno mission</a>, have not had the sensitivity required to pull out this level of ionospheric detail.”



The images taken by Webb highlight features that were once simply too faint for ground-based equipment or earlier missions to spot. 



Stallard continued, “In future it would be interesting to observe how the patterns we see over the Great Red Spot change, and how these waves move throughout Jupiter’s upper atmosphere.”



<h2 class="wp-block-heading" id="h-why-does-any-of-this-matter">Why does any of this matter?</h2>



Jupiter’s magnetic field is much more intense than Earth’s, yet there are parallels in the way ionospheres behave. 



“Although Jupiter appears very different to Earth there is actually much we can learn about our own planet by studying Jupiter. The processes going on are very similar, but Jupiter’s magnetic field is much stronger, and stranger," Stallard concluded.



By investigating these <a href="https://www.earth.com/news/discovery-about-jupiters-clouds-not-ammonia-ice-leaves-astronomers-astonished/" target="_blank" rel="noreferrer noopener">processes on a bigger stage</a>, scientists can apply fresh insights to our own world. 



When features are magnified on Jupiter, it can offer straightforward ways to test models that might be more subtle in Earth’s environment.



<h2 class="wp-block-heading" id="h-waiting-for-the-juice">Waiting for the Juice</h2>



These discoveries may also help guide work on ESA’s Jupiter Icy Moons Explorer, <a href="https://www.esa.int/Science_Exploration/Space_Science/Juice" target="_blank" rel="noreferrer noopener">Juice</a>, which lifted off on April 14, 2023. 



That mission carries instruments designed to learn more about Jupiter and its icy satellites, specifically Ganymede, Callisto, and Europa. 



The goal is to assess these worlds as potential habitats while exploring the planet’s broader surroundings. 



The insights from Webb could prove vital when Juice measures the structures of Jupiter’s magnetic and atmospheric environment up close.



Researchers plan to examine Jupiter’s entire system to see how it compares to other gas giants across the universe. 



By focusing on wave patterns near the planet’s equatorial belt and looking at how <a href="https://www.earth.com/news/what-is-causing-the-mysterious-haze-at-jupiters-poles/" target="_blank" rel="noreferrer noopener">charged particles behave</a>, the mission might provide further clarity on what drives the weather patterns and emissions in Jupiter’s upper layers.



<h2 class="wp-block-heading" id="h-learning-from-jupiter-s-atmosphere">Learning from Jupiter's atmosphere</h2>



With the Webb telescope’s remarkable precision, scientists have found another layer of interest that is changing the way we think about ionospheric activities in the outer solar system. 



Each new image confirms there are still stories unfolding above that swirling red storm. 



The spotlight now shifts to exploring these atmospheric waves, the structures they create, and the lessons that might await our own planet. 



By mapping these patterns and testing how they evolve, researchers are poised to gain a deeper understanding of giant planets both close to home and beyond.



The full study was published in the journal <a href="https://www.nature.com/articles/s41550-024-02305-9" target="_blank" rel="noreferrer noopener">Nature Astronomy</a>.



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Surprising 'shapes' discovered near Jupiter’s Great Red Spot

Jupiter's striking size, swirling gases, and dramatic bands in its...

Every summer feels hotter than the last. News reports cover deadly heatwaves, rising humidity, and collapsing infrastructure under soaring temperatures. But while climate models predict extreme weather, a deeper question lingers: how much heat can the human body actually tolerate?



A recent study from the University of Ottawa’s Human and Environmental Physiology Research Unit (<a href="https://hepru.ca" target="_blank" rel="noreferrer noopener">HEPRU</a>) has provided fresh insights. 



The team, led by Dr. Robert D. Meade and Professor Glen Kenny, set out to measure the biological limits of thermoregulation - our body’s ability to control internal <a href="https://www.earth.com/news/extreme-heat-is-pushing-parts-of-earth-beyond-human-survival/" target="_blank" rel="noreferrer noopener">temperature</a> under conditions of environmental stress.



This research does more than update old data. It redefines our understanding of human survival in a warming world.



<h2 class="wp-block-heading" id="h-heat-tolerance-is-lower-than-expected">Heat tolerance is lower than expected</h2>



Until recently, scientists assumed that humans could tolerate “wet bulb” temperatures - where humidity and heat combine - up to 35 °C. This threshold was widely cited as the maximum point for survival. However, new experiments have challenged that belief.



“The conditions under which humans can effectively regulate their body temperature are actually much lower than earlier models suggested,” said Professor Kenny.



This revelation comes from a series of precise laboratory experiments that exposed volunteers to controlled <a href="https://www.earth.com/news/astonishing-global-heat-in-january-2025-defied-climate-expectations/" target="_blank" rel="noreferrer noopener">heat</a> and humidity. 



The research team applied a method called thermal-step protocols, where air temperature or relative humidity is increased in steps to determine when the body loses control over its internal temperature. 



This point, called the “core temperature inflection,” was assumed to mark the edge of thermoregulation. Yet, until now, no study had tested this assumption directly.



<h2 class="wp-block-heading" id="h-testing-human-thermoregulation-limits">Testing human thermoregulation limits</h2>



To validate the threshold, researchers subjected 12 healthy adults to extreme conditions in a climate-controlled chamber. First, each participant underwent a humidity-step protocol. 



They were gradually exposed to increasing levels of <a href="https://www.earth.com/news/ocean-warming-broke-records-for-450-straight-days/" target="_blank" rel="noreferrer noopener">heat</a> or moisture to determine their personal inflection point - the moment when their core temperature started climbing sharply.



But the experiment didn’t stop there. Each participant returned for two additional 9-hour trials. In one session, they were exposed to a wet bulb temperature just below their individual limit (around 30.9 °C). 



In the other, they faced a temperature just above it (approximately 33.7 °C). The goal was to see whether the body could adapt and stabilize, or whether it would succumb to the heat.



<h2 class="wp-block-heading" id="h-when-the-body-fails-to-cool-itself">When the body fails to cool itself</h2>



The outcome was decisive. “The results were clear. The participants’ core <a href="https://www.earth.com/news/global-warming-is-accelerating-beyond-control-as-co2-levels-rise/" target="_blank" rel="noreferrer noopener">temperature</a> streamed upwards unabated, and many participants were unable to finish the 9-hour exposure,” Dr. Meade explained.



These extended trials confirmed that even slightly exceeding the inflection point leads to dangerous, unmanageable rises in body temperature. Heat stroke levels (around 40.2 °C core temperature) could be reached in under 10 hours under “Tabove” conditions. 



Even in the “Tbelow” trials, where conditions were slightly milder, the body struggled. It would take more than 24 hours to reach heat stroke, but the trajectory was still upward.



<h2 class="wp-block-heading" id="h-predicting-heat-impacts-on-humans">Predicting heat impacts on humans</h2>



This research does more than confirm a theory - it validates a method.



Thermal-step protocols have been used for decades to estimate limits for thermoregulation, but they lacked direct validation. Now, with this study, scientists can confidently rely on these models when projecting future human risks.



“Our findings [are] especially timely, given estimated limits for thermoregulation are being increasingly incorporated into large scale <a href="https://www.earth.com/news/clouds-have-become-less-reflective-making-global-warming-worse/" target="_blank" rel="noreferrer noopener">climate</a> modeling,” noted Dr. Meade.



By testing human physiology in real-world simulations, this study connects lab science with global climate data. It also provides detailed measurements of physiological strain during prolonged exposure.



Even when core temperature didn’t immediately reach lethal levels, participants showed signs of uncompensated heat stress - rapid heart rates, fatigue, and inability to finish the trial.



<h2 class="wp-block-heading" id="h-global-climate-map">Global climate map</h2>



As climate models grow more detailed, they are beginning to include human physiological limits. This study adds confidence to those models by showing that the lab-based thermal-step method can predict real-life responses. 



It also shifts expectations: survivability thresholds now fall between 26 °C and 31 °C wet bulb temperature, which is much lower than the previously cited 35 °C mark.



“By integrating physiological data with climate models, we hope to better predict and prepare for heat-related health issues,” said Professor Kenny.



In other words, this isn’t just about lab numbers. It’s about how cities will respond to heat emergencies, how healthcare systems can adapt, and how urban planning must change. Policies can now draw on data that reflect the actual stress on human bodies under conditions of rising temperature.



<h2 class="wp-block-heading" id="h-heat-exposure-may-exceed-human-capacity">Heat exposure may exceed human capacity</h2>



What makes this study urgent is the projection that large regions across the globe will soon experience these dangerous conditions. 



Some of these zones include densely populated areas where millions may face extended periods of wet bulb temperatures of above 32 °C. With each degree rise, the margin for survival shrinks.



These findings serve as both a warning and a guide. They remind us that biological systems - unlike machines - can only adapt so far. The limits are real, measurable, and fast approaching.



Human survival under climate stress will depend not only on environmental policy but on understanding and respecting the boundaries of our own physiology.



This research marks a turning point. It shows that the future of climate adaptation must start with the human body. It is not a matter of theory, but of the unmistakable rise of core temperatures, the lab data collected over nine sweltering hours, and the shared vulnerability of every person facing a hotter planet.



The study is published in the journal <a href="https://www.pnas.org/doi/10.1073/pnas.2421281122" target="_blank" rel="noreferrer noopener">PNAS</a>.



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Humans have a much lower heat tolerance than expected

Every summer feels hotter than the last. News reports cover...

Why would prehistoric humans carry their youngest children deep into the winding, pitch-black recesses of ancient caves - places riddled with danger, low oxygen, and claustrophobic tunnels? 



A new study from researchers at <a href="https://english.tau.ac.il/" target="_blank" rel="noreferrer noopener">Tel Aviv University</a> suggests an answer that goes beyond simple tradition or education: these children weren’t just tagging along - they were spiritual participants.



A paper recently published in <a href="http://dx.doi.org/10.3390/arts14020027" target="_blank" rel="noreferrer noopener">Arts</a>, a journal from MDPI, presents an innovative interpretation of children’s presence at cave art sites. The study proposes that small children were believed to serve a powerful spiritual function - acting as mediators between humans and the unseen world.



The research was conducted by Dr. Ella Assaf, Dr. Yafit Kedar, and Professor Ran Barkai from Tel Aviv University's Jacob M. Alkow Department of Archaeology and Ancient Near Eastern Cultures.



<h2 class="wp-block-heading" id="h-children-participated-in-cave-art">Children participated in cave art</h2>



Cave paintings, particularly those found in France and Spain, date back between 40,000 and 12,000 years and continue to mystify archaeologists.&nbsp;



While previous studies have focused on the adult creators of these artworks, there’s growing evidence that children were also involved. Handprints and finger paintings left by young ones, some as young as two years old, are scattered among the animal figures and abstract shapes. 



Footprints and hand impressions found near these ancient <a href="https://www.earth.com/news/worlds-oldest-cave-painting-discovered-in-indonesia/" target="_blank" rel="noreferrer noopener">paintings</a> suggest that children didn’t merely observe - they actively took part.



“There is solid evidence of children’s participation in the artwork,” Assaf said. “This naturally raises the question: why were very young children taken on exhausting and hazardous journeys deep into the dark, meandering caves with low oxygen levels - crawling through crevices, descending shafts, and climbing rocks to reach their destination?”



So far, most hypotheses have leaned toward the educational. The assumption was that adults brought children along to pass on cultural knowledge - traditions, myths, artistic skills. But the experts believe there’s more to the story.



<h2 class="wp-block-heading" id="h-children-as-powerful-figures">Children as powerful figures</h2>



“Despite extensive research on cave art, few studies have focused on the presence of children,” Kedar said. “The prevailing hypothesis is that their participation served an educational purpose. In our study, we argue that children’s involvement had an additional meaning.”



Drawing on ethnographic studies of indigenous societies and recent insights into the nature of cave rituals, the researchers suggest that small children were considered spiritually potent. 



In many traditional cultures, children are not seen merely as passive observers or learners, but as powerful figures in their own right - what the researchers call “active agents.”



“Children possess a range of unique mental and cognitive traits, For this reason, indigenous cultures worldwide, throughout history and prehistory, have viewed children as 'active agents' - mediators between this world and the entities inhabiting the natural world, the underworld, and the cosmos as a whole,” Assaf said.&nbsp;



“In this way, children made a vital contribution to their communities - <a href="https://www.earth.com/news/stone-age-hunter-gatherers-had-a-very-organized-domestic-life/" target="_blank" rel="noreferrer noopener">hunter-gatherers</a> who lived in nature and sought to maintain continuous, respectful relationships with various entities: animals and plants that served as food sources, stones used for <a href="https://www.earth.com/news/chimpanzees-select-the-best-materials-for-termite-fishing/" target="_blank" rel="noreferrer noopener">toolmaking</a>, ancestral spirits, and more.”



By involving children in cave rituals and artwork, ancient communities may have believed they were strengthening their connection to spiritual entities - animals, ancestral spirits, or cosmic forces - that governed their survival. 



These were communities deeply reliant on nature, where food, tools, and spiritual meaning were derived from the landscape around them.



<h2 class="wp-block-heading" id="h-children-delivered-messages-in-cave-art">Children delivered messages in cave art</h2>



According to Barkai, caves themselves were often seen as liminal spaces - gateways to the underworld. For prehistoric societies, descending into the earth was not merely physical but symbolic. Within the depths, shamanic rituals could be performed to communicate with unseen forces.



“Young children were perceived as liminal beings - belonging to both the realm they had left just recently (before birth) and the world they currently inhabit,” he said. “Thus, small children were considered particularly suited to bridging the gap between the worlds and delivering messages to non-human entities.”



By this logic, children were not just extras in a ceremonial performance, but integral players. Their presence, their touch, even their handprints may have been believed to amplify the ritual’s power.&nbsp;



Thus, children joined adults on journeys into the depths of caves and participated in painting and rituals as part of their role in the community - as ideal mediators with entities from the beyond.



<h2 class="wp-block-heading" id="h-childhood-and-spiritual-connection-nbsp">Childhood and spiritual connection&nbsp;</h2>



This study contributes to a growing body of work that rethinks the role of children in prehistory. Rather than viewing them as mere bystanders or apprentices, researchers are beginning to see young members of ancient communities as active participants in shaping both social life and spiritual practices.



By blending archaeological evidence with cultural anthropology and religious studies, the scientists opened a new window into how <a href="https://www.earth.com/news/early-humans-had-surprising-diets-3-5-million-years-ago/" target="_blank" rel="noreferrer noopener">early humans</a> understood the roles of the youngest among them.&nbsp;



It’s a theory that paints childhood not just as a period of learning, but as a time of spiritual connection - and children, not just as learners, but as vital messengers between worlds.



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Children played a spiritual role in prehistoric cave art

Why would prehistoric humans carry their youngest children deep into...

An international team of researchers took advantage of a rare chance encounter to explore a massive new expanse of seafloor exposed by the breakup of an Antarctic ice shelf in the Bellingshausen Sea.&nbsp;



On January 13, 2025, an iceberg named A-84 - which was the size of the city of Chicago - broke off from the George VI Ice Shelf, which sits along the Antarctic Peninsula. 



This event uncovered roughly 209 square miles (540 square kilometers) of seafloor that had previously been concealed under floating ice.



The team arrived aboard <a href="https://schmidtocean.org/" target="_blank" rel="noreferrer noopener">Schmidt Ocean Institute</a>’s R/V Falkor (too) at this newly exposed site on January 25, making them the first to study such a large underwater area that had previously been covered by an ice shelf.&nbsp;



Their effort marks the first large-scale interdisciplinary exploration of geologic, oceanographic, and biological features hidden beneath an extensive floating <a href="https://www.earth.com/news/astonishing-glacier-retreat-in-the-arctic-signals-climate-disaster/" target="_blank" rel="noreferrer noopener">glacier</a> front.



<h2 class="wp-block-heading" id="h-rapidly-shifting-expedition-goals">Rapidly shifting expedition goals</h2>



Co-chief scientist Patricia Esquete is a researcher in the <a href="https://www.cesam-la.pt/en/" target="_blank" rel="noreferrer noopener">Center for Environmental and Marine Studies</a> (CESAM) and the Department of Biology (DBio) at the <a href="https://www.ua.pt/" target="_blank" rel="noreferrer noopener">University of Aveiro</a> in Portugal.&nbsp;



"We seized upon the moment, changed our expedition plan, and went for it so we could look at what was happening in the depths below,” said Esquete.



“We didn’t expect to find such a beautiful, thriving <a href="https://www.earth.com/news/how-environmental-stress-strengthens-ecosystems/" target="_blank" rel="noreferrer noopener">ecosystem</a>. Based on the size of the animals, the communities we observed have been there for decades, maybe even hundreds of years.”



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/Antarctic-iceberg-detached_seafloor-study_credit-SOI_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/03/Antarctic-iceberg-detached_seafloor-study_credit-SOI_1s.webp" alt="The newly exposed Antarctic seafloor also allowed the team to gather critical data on the past behavior of the ice sheet. The ice sheet has been shrinking and losing mass over the last few decades due to climate change. Credit: Alex Ingle / Schmidt Ocean Institute" class="wp-image-1963228"/></a><figcaption class="wp-element-caption">The newly exposed Antarctic seafloor also allowed the team to gather critical data on the past behavior of the ice sheet. The ice sheet has been shrinking and losing mass over the last few decades due to climate change. Credit: Alex Ingle / Schmidt Ocean Institute</figcaption></figure>



Originally, the science mission did not include venturing beneath a freshly fractured portion of the ice shelf. 



However, the movement of this newly calved <a href="https://www.earth.com/news/massive-iceberg-that-broke-away-from-antarctica-sparks-concerns/" target="_blank" rel="noreferrer noopener">iceberg</a> offered a rare opportunity to explore a site that, until recently, had never been examined by any human.



<h2 class="wp-block-heading" id="h-antarctic-seafloor-reveals-lush-communities">Antarctic seafloor reveals lush communities</h2>



Using Schmidt Ocean Institute’s remotely operated vehicle, ROV SuBastian, the science team spent eight days surveying the seafloor at depths down to 1,300 meters (4,265 feet).&nbsp;



The experts discovered an unexpectedly rich ecosystem that was teeming with corals, sponges, icefish, giant sea spiders, and <a href="https://www.earth.com/news/octopuses-could-dominate-earth-if-humans-vanish/" target="_blank" rel="noreferrer noopener">octopuses</a> - an indication that marine life can flourish under ice-covered regions of the Antarctic in ways not previously documented.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/Antarctic-iceberg-detached_seafloor_octopus-resting_credit-SOI_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/03/Antarctic-iceberg-detached_seafloor_octopus-resting_credit-SOI_1s.webp" alt="An octopus rests on the seafloor 1150 meters deep, in the Bellingshausen Sea off Antarctica, at an area where the shelf break and slope are cut by several underwater gullies. Credit: ROV SuBastian / Schmidt Ocean Institute" class="wp-image-1963224"/></a><figcaption class="wp-element-caption">An octopus rests on the seafloor 1150 meters deep, in the Bellingshausen Sea off Antarctica, at an area where the shelf break and slope are cut by several underwater gullies. Credit: ROV SuBastian / Schmidt Ocean Institute</figcaption></figure>



According to the researchers, these observations offer insight into how ecosystems function beneath the Antarctic ice sheet.&nbsp;Such an ecosystem has seldom been accessed. 



Earlier findings, notably by <a href="https://www.bas.ac.uk/" target="_blank" rel="noreferrer noopener">British Antarctic Survey</a> researchers in 2021, revealed possible bottom-dwelling life beneath ice, but the present study marks the first time an ROV survey has thoroughly documented wide areas of this vibrant seabed.



The experts were surprised by the large biomass and biodiversity in the ecosystem and suspect they have discovered several new species.



<h2 class="wp-block-heading" id="h-how-marine-life-survives-in-darkness">How marine life survives in darkness</h2>



Deep-sea ecosystems generally depend on nutrients trickling down from surface waters. However, these Antarctic seafloors had been buried under ice some 150 meters (nearly 500 feet) thick for centuries.&nbsp;



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/Antarctic-iceberg-detached_seafloor_Sponge_Anemone_credit-SOI_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/03/Antarctic-iceberg-detached_seafloor_Sponge_Anemone_credit-SOI_1s.webp" alt="A large sponge, a cluster of anemones, and other life is seen nearly 230 meters deep at an area of the seabed that was very recently covered by the George VI Ice Shelf, a floating glacier in Antarctica. Credit: Schmidt Ocean Institute" class="wp-image-1963226"/></a><figcaption class="wp-element-caption">A large sponge, a cluster of anemones, and other life is seen nearly 230 meters deep at an area of the seabed that was very recently covered by the George VI Ice Shelf, a floating glacier in Antarctica. Credit: Schmidt Ocean Institute</figcaption></figure>



With no direct sunlight, how such abundant organisms manage to feed is still uncertain. The scientists propose that ocean currents under the ice may be funneling essential nutrients to these communities.



<h2 class="wp-block-heading" id="h-antarctic-ice-sheet-behavior">Antarctic ice sheet behavior</h2>



Apart from their ecological discoveries, the international group - which included scientists from Portugal, the United Kingdom, Chile, Germany, Norway, New Zealand, and the United States - examined geological samples to gain knowledge about past changes in the Antarctic ice sheet.



The ice sheet has been shrinking and losing mass for decades in response to climate change.&nbsp;



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/Antarctic-iceberg-detached_modis-satellite-view_NASA_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/03/Antarctic-iceberg-detached_modis-satellite-view_NASA_1s.webp" alt="The MODIS Corrected Reflectance satellite imagery showing the iceberg calved from George VI Ice Shelf in the Bellingshausen Sea on 19 January 2025. Credit: Schmidt Ocean Institute" class="wp-image-1963222"/></a><figcaption class="wp-element-caption">The MODIS Corrected Reflectance satellite imagery showing the iceberg calved from George VI Ice Shelf in the Bellingshausen Sea on 19 January 2025. Credit: Schmidt Ocean Institute</figcaption></figure>



“The ice loss from the Antarctic Ice Sheet is a major contributor to sea level rise worldwide,” said co-chief scientist Sasha Montelli of <a href="https://www.ucl.ac.uk/" target="_blank" rel="noreferrer noopener">University College London</a>, who is also a 2019 Schmidt Science Fellow.&nbsp;



“Our work is critical for providing longer-term context of these recent changes, improving our ability to make projections of future change - projections that can inform actionable policies. We will undoubtedly make new discoveries as we continue to analyze this vital data.”



<h2 class="wp-block-heading" id="h-samples-from-the-antarctic-seafloor">Samples from the Antarctic seafloor </h2>



During this mission, the team collected both biological and geological samples. 



In addition, they deployed autonomous underwater vehicles, called gliders, to analyze how meltwater from the ice shelf impacts the region’s physical and chemical properties.&nbsp;



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/antarctic-iceberg_Solitary-Hydroid_unseen-ecosystem_credit-SOI_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/03/antarctic-iceberg_Solitary-Hydroid_unseen-ecosystem_credit-SOI_1s.webp" alt="A solitary hydroid drifts in currents approximately 380 meters deep at an area of the seabed that was very recently covered by the George VI Ice Shelf, a floating glacier in Antarctica. Solitary hydroids are related to corals, jellyfish, and anemones, but do not form colonies. Credit: SOI" class="wp-image-1963895"/></a><figcaption class="wp-element-caption">A solitary hydroid drifts in currents approximately 380 meters deep at an area of the seabed that was very recently covered by the George VI Ice Shelf, a floating glacier in Antarctica. Solitary hydroids are related to corals, jellyfish, and anemones, but do not form colonies. Click image to enlarge. Credit: SOI</figcaption></figure>



Preliminary measurements hinted at high biological productivity and strong meltwater flow from the George VI ice shelf, providing further context for how such deep-sea populations may thrive in these surroundings.



<h2 class="wp-block-heading" id="h-part-of-a-larger-global-initiative">Part of a larger global initiative</h2>



The expedition is part of Challenger 150, a global cooperative dedicated to deep-sea biological study, and recognized by the Intergovernmental Oceanographic Commission of UNESCO (<a href="https://www.ioc.unesco.org/en" target="_blank" rel="noreferrer noopener">IOC/UNESCO</a>) as an Ocean Decade Action.&nbsp;



This alignment ensures that findings from the George VI Ice Shelf breakage feed into broader international efforts to understand and safeguard <a href="https://www.earth.com/news/climate-change-is-impacting-marine-life-more-than-we-realized/" target="_blank" rel="noreferrer noopener">marine life</a>.



“The science team was originally in this remote region to study the seafloor and ecosystem at the interface between ice and sea,” noted Schmidt Ocean Institute’s executive director, Jyotika Virmani.&nbsp;



“Being right there when this iceberg calved from the ice shelf presented a rare scientific opportunity. Serendipitous moments are part of the excitement of research at sea - they offer the chance to be the first to witness the untouched beauty of our world.”



Looking ahead, the researchers plan to continue analyzing the collected data for insights into both ice sheet behavior and the unique marine life that has flourished unseen for centuries beneath the ice.&nbsp;



With accelerating climate change, the study’s findings about species adaptability and the resilience of Antarctic habitats carry implications for future conservation and policy decisions on a global scale.



<a href="https://schmidtocean.photoshelter.com/galleries/C0000QszlkoaNkKU/G0000p4LRtGEAfWo/I0000X_S5KjUr4QU/FKt250110-20250126-IceScanningCollectionAndIcebergViewing-Ingle-0202-jpg" target="_blank" rel="noreferrer noopener">See more of the photos taken on this mission by the Schmidt Ocean Institute here...</a>



Images Credit: Schmidt Ocean Institute



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Antarctic iceberg breaks away and reveals ecosystem never seen by humans

An international team of researchers took advantage of a rare...

Memories don't follow a straight, linear path, even though we often recall them like tidy stories. Researchers are now embracing this complexity, using smartphones to explore how memories shift over time, how they become richer or fade, and how we might intentionally strengthen them.&nbsp;



These digital tools are allowing scientists to track real-life experiences in ways that lab studies can’t, revealing how actions like trying something new, replaying moments before sleep, or feeling strong emotions may enhance our memory.



These insights are being shared at the <a href="https://www.cns.org/annualmeeting?gad_source=1&amp;gclid=Cj0KCQjwna6_BhCbARIsALId2Z32nZKBwJfBW1xlk4p1DeZXQCu-j2lAYuBjcMNte24oAjQO4Thu2rEaAj5-EALw_wcB" target="_blank" rel="noreferrer noopener">annual meeting of the Cognitive Neuroscience Society (CNS)</a>, where researchers are highlighting a range of smartphone-based studies that explore how memory is shaped by daily life.&nbsp;



“Smartphones are an incredible tool for understanding patterns of feelings, behavior, and experiences in daily life, and how different types of everyday events stay with us in memory,” said Elizabeth Goldfarb from <a href="https://www.yale.edu/" target="_blank" rel="noreferrer noopener">Yale University</a>, who is chairing a session on the topic. 



“Real experiences have so much more salience and self-relevance than anything I can generate in the lab, and being able to quantify how people remember those events is very exciting.”



<h2 class="wp-block-heading" id="h-sleep-dreams-and-the-timing-of-memory">Sleep, dreams, and the timing of memory</h2>



One line of research being presented comes from Morgan Barense at the <a href="https://www.utoronto.ca/" target="_blank" rel="noreferrer noopener">University of Toronto</a>, who is examining how <a href="https://www.earth.com/news/sleep-rewires-the-brain-to-strengthen-memories/" target="_blank" rel="noreferrer noopener">sleep</a> and dreams affect memory retention. This work emerged unexpectedly, when a previous study showed that memory recall was significantly affected by when material was reviewed in relation to sleep.&nbsp;



“We found that the timing of when someone first reviews material relative to sleep had an enormous effect on how well they later remembered it,” Barense said.&nbsp;



“The effect was so striking that I initially didn’t believe it. That discovery made me realize that sleep is something all memory scientists should be paying close attention to.”



Barense’s team, led by graduate student Nelly Matorina, developed a smartphone app called HippoCamera to test how a night of sleep impacts memories from the day before.&nbsp;



<h2 class="wp-block-heading" id="h-memories-following-sleep-are-more-vivid">Memories following sleep are more vivid</h2>



Participants recorded two events each day - one in the morning, one in the evening - for two weeks. The researchers then tested <a href="https://www.earth.com/news/memory-isnt-only-stored-in-our-brains-other-cells-can-remember-too/" target="_blank" rel="noreferrer noopener">recall</a> after 12-hour intervals, comparing the effects of sleep versus wakefulness. 



Their earlier findings were confirmed. “Memories following sleep were more vivid, felt temporally closer, and were easier to recall, suggesting that a single night of sleep helps preserve the richness of autobiographical memory,” Barense explained.



Participants also recorded dreams and identified any that related to events captured with the app. “Interestingly, memories that were dreamt about were also rated as feeling temporally closer and were more likely to be recalled from a first-person perspective,” she added.



The team followed up by testing those same memories a year later to see how they changed, particularly in relation to the event's location.&nbsp;



“Our pattern of results suggests that the link between an event and its location may initially weaken after a night’s sleep to allow for memory reorganization, but over the long term, a year later, our memory is strongly connected to where it took place,” Matorina said.



<h2 class="wp-block-heading" id="h-smartphones-improve-memory-research-nbsp">Smartphones improve memory research&nbsp;</h2>



While studying memory outside the lab comes with challenges, Barense sees great value in this approach.&nbsp;



“Real-world data collection introduces variability that is difficult to control, and tracking sleep and memory over time requires careful methodological design,” she said.&nbsp;



“However, these challenges are also what make smartphone-based research so promising - it allows us to move beyond artificial settings and study memory as it naturally unfolds in daily life.”



Looking ahead, Barense’s team will partner with Ken Paller’s lab at <a href="https://www.northwestern.edu/" target="_blank" rel="noreferrer noopener">Northwestern University</a> to see if memory retention can be boosted during sleep. They plan to combine HippoCamera with targeted memory reactivation, which uses sound cues tied to events and plays them during specific sleep stages.&nbsp;



“While our previous work has shown that HippoCamera strengthens autobiographical memory in older adults, we believe that incorporating sleep-based memory reactivation will further amplify its benefits,” Barense said.



<h2 class="wp-block-heading" id="h-smartphone-app-tests-recall">Smartphone app tests recall</h2>



Lila Davachi of <a href="https://www.columbia.edu/" target="_blank" rel="noreferrer noopener">Columbia University</a> is also using smartphone-based research to explore memory, inspired by the mental and emotional effects of the pandemic.&nbsp;



“The lab had already published several papers on the impact of context representations on associative memory and here we all were sitting in our homes, meeting on Zoom, with very little change in our contexts,” she said.&nbsp;



“It was natural to wonder how this was going to impact our long-term memories and, perhaps by consequence, our <a href="https://www.earth.com/news/mental-health-crisis-half-of-the-worlds-population-will-be-affected-by-age-75/" target="_blank" rel="noreferrer noopener">mental health</a>.”



Davachi and her team used a “daily diary” smartphone app, asking participants to report and categorize daily events over two weeks as “novel,” “routine,” or “periodic.” Two weeks later, they tested recall.&nbsp;



With the help of artificial intelligence to analyze responses, the researchers found that novel events were remembered with greater vividness and detail.&nbsp;



“Perhaps more exciting, we found that routine and periodic events that happened on the same day as a novel event were also better remembered than routine and periodic events that took place on days with less novelty,” Davachi explained. “This suggests a penumbra-like effect of novelty.”



This effect hints at the value of “experiential diversity” in strengthening memory. By mixing up daily routines with new experiences, people might be able to enhance not just specific memories but their overall ability to recall an entire day.&nbsp;



“Being able to sample and record data from individuals in the real world, along with the use of AI-based large language models to help us analyze large amounts of complex data, is a solid stepping stone,” Davachi said.



<h2 class="wp-block-heading" id="h-exploring-the-role-of-emotion-and-addiction">Exploring the role of emotion and addiction </h2>



Goldfarb is also using smartphones to investigate how people remember emotionally intense experiences, particularly in the context of substance use. In one study, she is examining the role of memory in alcohol addiction.&nbsp;



Memory is an important factor in <a href="https://www.earth.com/news/zapping-the-brain-with-ultrasound-waves-may-cure-drug-addiction/" target="_blank" rel="noreferrer noopener">addiction</a>, since, for instance, someone can’t relapse in a place where they used to drink if they have no memories of drinking there. “Yet we know very little about what people remember about their time drinking that drives this behavior,” Goldfarb said.



Using smartphone recordings, her team is able to compare real-life memories of drinking events with patterns seen in lab studies.&nbsp;



“We’re uncovering some similarities with what we measure in the lab, which is great for establishing ecological validity,” she said. However, these real-world observations are also revealing new insights.&nbsp;



“We are seeing that people are more likely to link different parts of a positive event together in memory,” she said. “As a researcher, the effects of real emotions are so much stronger than what we can create in the lab.”



Goldfarb believes this emerging body of work - from <a href="https://www.earth.com/news/dream-recall-who-remembers-their-dreams-and-why/" target="_blank" rel="noreferrer noopener">dreams</a> to novelty to emotions - is opening new doors in memory research. As she concludes, these new tools and findings are a significant step forward in helping people build stronger and more detailed memories.



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Smartphones are teaching us how to supercharge our memory

Memories don't follow a straight, linear path, even though we...

Single-celled organisms that group together can generate stronger water currents to pull in food, a benefit that may have encouraged early life forms to assemble into colonies, according to a new study. This could have set the stage for more complex, multicellular life.



Ultimately, the research suggests that the evolution of multicellular organisms may have been shaped by the fluid dynamics of cooperative feeding.



“So much work on the origins of <a href="https://www.earth.com/news/past-snowball-earth-conditions-drove-evolution-complex-multicellular-life/" target="_blank" rel="noreferrer noopener">multicellular life</a> focuses on chemistry,” said Shashank Shekhar, lead author of the study and assistant professor of physics at <a href="https://www.emory.edu/home/index.html" target="_blank" rel="noreferrer noopener">Emory University</a>. “We wanted to investigate the role of physical forces in the process.”&nbsp;



Shekhar was inspired by observing the feeding behavior of stentors - large, trumpet-shaped, single-celled organisms. He began exploring how their movements through liquid might provide clues about the transition from single cells to complex life. 



“The project started with beautiful images of the fluid flows,” Shekhar said. “Only later did we realize the evolutionary significance of this behavior.”



<h2 class="wp-block-heading" id="h-the-physics-of-feeding">The physics of feeding</h2>



Stentors are visible to the naked eye and are commonly found floating near the surface of freshwater <a href="https://www.earth.com/news/ponds-release-more-greenhouse-gases-than-they-store/" target="_blank" rel="noreferrer noopener">ponds</a>. These organisms can grow up to two millimeters in length - roughly the size of a pencil tip.&nbsp;



They attach to leaves, twigs, or other floating matter using a sticky secretion from one end of their body, while the wider, open end is surrounded by cilia - tiny hair-like structures that beat rhythmically to create water currents and pull in food particles.



Using microscope video, Shekhar captured how a single stentor feeds by creating twin vortices at its mouth, which effectively draw in food like bacteria and algae.&nbsp;



To make the fluid motion visible, he added plastic beads small enough to trace the currents. This experiment revealed the efficiency of the cilia-generated flow in solitary feeding.



However, Shekhar noticed that stentors sometimes clustered together, forming pairs or even colonies in a semi-spherical shape. When he recorded the feeding dynamics of these groups, he discovered something intriguing:&nbsp;



“I call that movement ‘I love you, I love you not,’” Shekhar said, referring to how pairs of stentors would sway toward and away from each other. When their heads drew closer together, their fluid flows merged into a single, stronger vortex that attracted food from a larger area.



<h2 class="wp-block-heading" id="h-single-celled-organisms-working-together">Single-celled organisms working together </h2>



The feeding advantage increased further when stentors joined larger groups. <a href="https://www.earth.com/news/larger-ant-colonies-drove-the-evolution-of-worker-castes/" target="_blank" rel="noreferrer noopener">Colonies</a> were able to generate currents significantly more powerful than individual organisms or even pairs, drawing in more food from farther away. 



This finding raised a question: if cooperation improved feeding, why did some stentors occasionally leave the group?



The team proposed that not all stentors gained equally from forming colonies. “The colonies are dynamic as the stentors keep changing partners,” Shekhar explained. “The stronger ones are being taken advantage of, in a sense. They change partners often so that everyone benefits similarly.”&nbsp;



This suggested that stronger individuals might temporarily withdraw from the group to avoid being exploited by weaker ones, while the weaker stentors had more to gain by staying attached.



<h2 class="wp-block-heading" id="h-cooperation-in-organisms-without-a-brain">Cooperation in organisms without a brain</h2>



To test these ideas, the researchers turned to mathematical modeling. Co-authors Eva Kanso of the <a href="https://www.usc.edu/" target="_blank" rel="noreferrer noopener">University of Southern California</a> and Haniliang Guo of <a href="https://www.owu.edu/" target="_blank" rel="noreferrer noopener">Ohio Wesleyan University</a> helped construct simulations that reproduced the dynamics seen in the lab.&nbsp;



The models confirmed that in pairings, one organism always had a greater advantage. Meanwhile, larger groups, especially those in which members periodically changed positions, increased the overall food intake for each member on average.



These findings suggest that the benefits of forming temporary colonies - especially the ability to draw in more food - could have played a role in the early transition from single cells to complex life. 



“It’s amazing that a single-celled organism, with no brain or <a href="https://www.earth.com/news/first-complete-map-of-every-neuron-in-the-brain-revealed/" target="_blank" rel="noreferrer noopener">neurons</a>, developed behaviors for opportunism and cooperation,” Shekhar said. “Perhaps these kinds of behaviors were hard-wired into organisms much earlier in evolution than we previously realized.”



<h2 class="wp-block-heading" id="h-the-evolution-of-multicellular-organisms">The evolution of multicellular organisms </h2>



The research emerged from a decade-long journey that began in 2014, when Shekhar joined a summer program at the <a href="https://www.mbl.edu/" target="_blank" rel="noreferrer noopener">Marine Biological Laboratory</a> (MBL) in Woods Hole, Massachusetts. There, he was able to collaborate with scientists from various universities.&nbsp;



“Renowned scientists come there every summer from around the world for organic collaborations,” Shekhar said. “You have the time and resources to explore extreme questions that capture your interest.”



Marshall’s research on stentors and their ability to regenerate has sparked even greater curiosity about these unique cells. Their remarkable properties and visible behaviors made them ideal subjects for studying physical phenomena that could drive evolutionary change.



“You can chop up a stentor and each tiny piece will become a complete organism within 12 hours,” said Shekhar.&nbsp;



<h2 class="wp-block-heading" id="h-from-single-cells-to-complex-life">From single cells to complex life</h2>



Though Shekhar is known for his work on actin, a protein essential to cell mobility, this project marked a new direction for his lab.&nbsp;



“The stentor work was a passion project,” he said. “It’s wonderful to work at your own pace, over many years, on a question that fascinates you and wind up with such beautiful and significant results.”



The study offers a fresh perspective on how simple, physical interactions between organisms could have contributed to the emergence of complex life.&nbsp;



While chemistry has long dominated theories about the origins of multicellularity, these results highlight the potential role of fluid mechanics and cooperation in shaping the earliest stages of biological organization.



The study is published in the journal <a href="http://dx.doi.org/10.1038/s41567-025-02787-y" target="_blank" rel="noreferrer noopener">Nature Physics</a>.



Image Credit: Shashank Shekhar



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From single cells to complex life: Was cooperation the first step?

Single-celled organisms that group together can generate stronger water currents...

Clothing rental has been pitched as a way to curb the fashion industry’s massive environmental impact. But so far, many of these ventures haven’t lasted long. 



What could make this idea work? It turns out that focusing on a specific market and building strong relationships with suppliers could be the key.



A recent study investigated whether clothing rental is a possible solution to the fashion industry's footprint. The research was led by <a href="https://www.chalmers.se/en/" target="_blank" rel="noreferrer noopener">Chalmers University of Technology</a>, along with experts at the University of Borås and the research institute RISE.



The team explored what has and hasn’t worked for companies trying to make renting clothes a practical, long-term business.



<h2 class="wp-block-heading" id="h-rental-clothes-and-sustainable-consumption">Rental clothes and sustainable consumption </h2>



The <a href="https://www.earth.com/news/fashion-industrys-plastic-waste-is-a-major-environmental-threat/" target="_blank" rel="noreferrer noopener">fashion industry</a> is one of the top contributors to <a href="https://www.earth.com/news/unprecedented-increase-in-global-ocean-plastic-pollution-since-2005/" target="_blank" rel="noreferrer noopener">global pollution</a>. In Sweden alone, over 90% of the climate impact from clothing comes from newly produced garments.



Renting instead of buying could keep clothes in circulation longer and reduce the need for constant production.



"Many people have clothes hanging in the closet that are rarely or never used. Renting clothes can extend the use of each garment and thus contribute to more sustainable consumption," said study co-author Professor Frida Lind.



<h2 class="wp-block-heading" id="h-types-of-fashion-rental-models">Types of fashion rental models</h2>



The researchers examined nine Swedish clothing rental companies. Some were still active, while others had shut down. Through this, they identified three common types of rental models.



The first model is membership-based. Customers sign up and borrow clothes for a set period of time, similar to how a library works. These companies were often founded by individuals who were driven by an interest in sustainability.



The second approach is subscription-based. In this model, customers pay a monthly fee and receive a rotating selection of garments to wear. Companies using this model usually aimed to expand quickly and attract investors.



The third model focuses on individual rentals. These businesses typically offered clothing for specific purposes - such as renting out ski jackets along with ski equipment - creating a bundled, purpose-driven experience.



<h2 class="wp-block-heading" id="h-why-fashion-rental-companies-struggle">Why fashion rental companies struggle </h2>



Despite genuine interest from consumers, many of the businesses struggled to stay afloat.



"What struck us was that it seemed so difficult for them to make their business profitable. Several had had to end their investments for various reasons," said Professor Lind.



Running a <a href="https://www.earth.com/news/people-were-already-making-clothing-120000-years-ago/" target="_blank" rel="noreferrer noopener">clothing</a> rental service involves multiple layers of effort. Every garment needs to be returned, cleaned, inspected, and prepared before it can be sent out again. This process is time-consuming and costly. 



Many companies also had high overhead expenses related to storage, transportation, and laundry. For those using a subscription model, raising early-stage investment proved difficult. 



The researchers found that most of these models simply require more time and support to take root in the market.



"Renting out <a href="https://www.earth.com/news/the-dark-side-of-donating-clothes-to-charity/" target="_blank" rel="noreferrer noopener">clothes</a> involves many steps where each item of clothing needs to be handled and inspected before it can be rented out again, which takes time. Companies also struggled with high costs for warehousing, logistics and laundry, for example," said Professor Lind.



"Especially for the subscription models, there were also difficulties in obtaining venture capital to be able to survive financially through the first phase of building the company. All this shows that these business models need time to establish themselves in the market."



<h2 class="wp-block-heading" id="h-niche-markets-are-more-promising">Niche markets are more promising</h2>



Not all of the business models fared poorly. Companies that targeted a narrow and specific market - such as outdoor gear - had better outcomes, especially when they operated near places where such clothing was needed.



"They seem to have found their niche and seen that there is a specific need that the customer is willing to pay for each time they need to use that type of clothing," said Professor Lind.



Companies that collaborated closely with clothing designers, manufacturers, and suppliers tended to do better as they gained useful insights that helped improve both product quality and customer satisfaction.



"Rental companies that worked closely with clothing manufacturers and suppliers, such as designers with a sustainability profile, benefited greatly from this as they were able to quickly get feedback on which types of clothing were most popular," said Professor Lind.



"They also gained valuable information about the quality of the garments, for example if there was something that often broke."



<h2 class="wp-block-heading" id="h-why-these-efforts-matter">Why these efforts matter</h2>



The researchers didn’t measure the environmental impact of each business model in this particular study. But earlier findings from Chalmers show that 70 percent of a garment’s climate impact comes from production, while 22 percent is linked to the shopping trips consumers make to buy them. 



In the U.S., an average person throws away about 81 pounds of clothing per year. In the EU, that number is about 26 pounds per person.



If people buy fewer new clothes and use existing garments for longer, that shift could bring major environmental benefits. And if those changes happen without extra travel emissions - even better.



<h2 class="wp-block-heading" id="h-changing-habits-one-attempt-at-a-time">Changing habits, one attempt at a time</h2>



While some of the companies examined for the study didn’t survive, Professor Lind believes the broader effort is still important. She noted that even failed attempts help shift public attitudes around how we view clothing ownership and consumption. They also provide useful lessons for future ventures.



"All initiatives that can contribute to the sustainability transition are important. Not least because they help to change attitudes about clothing consumption and increase knowledge about what can and cannot work," said Professor Lind.



"Our study can be an important contribution to the fashion industry's sustainability transition, as it shows the possibilities of new business models in this industry." 



"We hope that it can have an impact on decision-makers who need a basis for establishing incentives and financial motivation for a more <a href="https://www.earth.com/news/wealthy-nations-are-making-more-progress-toward-sustainable-development/" target="_blank" rel="noreferrer noopener">sustainable</a> fashion industry."



The full study was published in the journal <a href="https://www.emerald.com/insight/content/doi/10.1108/jbim-04-2024-0281/full/html" target="_blank" rel="noreferrer noopener">Journal of Business and Industrial Marketing</a>.



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Borrow clothes, save the planet? The reality of fashion rental

Clothing rental has been pitched as a way to curb...

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

[sendtonews key="G9bUoxcjr4-2511624-12187" type="single"] Today's Video of the Day from the...

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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

[sendtonews key="LvS8v8bp9z-2564889-12187" type="single"] Today's Video of the Day from the...

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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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They found the fifth cub in poor condition, but as they arrived at the vet, the experts knew exac​tly what to do. Still, one question lingered in their mind – What were they to do once they cubs were healthy? They couldn’t bottle feed forever.

Tough Decision

News coming your way