Today's Image of the Day from NASA features the spiral galaxy NGC 2566, which is located 76 million light-years away in the constellation Puppis. The image was captured by the NASA/ESA Hubble Space Telescope.



“A prominent bar of stars stretches across the center of this galaxy, and spiral arms emerge from each end of the bar. Because NGC 2566 appears tilted from our perspective, its disk takes on an almond shape, giving the galaxy the appearance of a cosmic eye,” said <a href="https://phys.org/news/2024-12-hubble-spies-spiral-galaxy-ngc.html" target="_blank" rel="noreferrer noopener">NASA</a>.



“As NGC 2566 appears to gaze at us, astronomers gaze right back, using Hubble to survey the galaxy's star clusters and star-forming regions.”



<h2 class="wp-block-heading" id="h-complex-appearance-of-ngc-2566">Complex appearance of NGC 2566</h2>



NGC 2566 lies at a considerable distance from Earth, making it a challenging object for amateur astronomers to observe in detail without powerful telescopes.&nbsp;



It can be seen in the Southern Hemisphere sky and is better observed from locations with minimal <a href="https://www.earth.com/news/how-light-pollution-influences-interest-in-astronomy/" target="_blank" rel="noreferrer noopener">light pollution</a>.&nbsp;



The galaxy's arms are populated with young, bright stars, regions of active star formation, and interstellar gas and dust - giving it a dynamic and complex appearance.



<h2 class="wp-block-heading" id="h-measuring-the-ages-of-stars">Measuring the ages of stars</h2>



According to NASA, data from Hubble is especially valuable for studying stars that are just a few million years old. “These stars are bright at the ultraviolet and visible wavelengths to which Hubble is sensitive.”



“Using these data, researchers can measure the ages of NGC 2566's stars, which helps piece together the timeline of the galaxy's star formation and the exchange of gas between star-forming clouds and the stars themselves.”



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



Star formation in <a href="https://www.earth.com/news/shapes-of-one-million-galaxies-hint-at-the-universes-origins/" target="_blank" rel="noreferrer noopener">galaxies</a> is a fascinating and complex process that unfolds over millions of years. It begins in vast clouds of gas and dust, known as molecular clouds, which are often found in the spiral arms of galaxies or in regions of irregular or starburst galaxies.&nbsp;



These clouds provide the raw material for star formation, consisting primarily of hydrogen and helium, with trace amounts of heavier elements.



As the molecular clouds collapse under their own gravity, regions within them begin to condense and fragment, forming dense clumps. Within these clumps, protostars emerge. Their formation is driven by the gravitational pull drawing in surrounding gas. 



During this process, the gas heats up due to increasing pressure, eventually igniting nuclear fusion in the core, signaling the birth of a new star.



<h2 class="wp-block-heading" id="h-rate-of-star-formation-nbsp-across-galaxies">Rate of star formation&nbsp;across galaxies</h2>



The rate of star formation varies across galaxies is influenced by numerous factors. In spiral galaxies like the Milky Way, star formation is most active in the spiral arms, where density waves compress gas and dust, triggering the collapse of molecular clouds. 



In contrast, elliptical galaxies, which often have little cold gas and dust, typically exhibit low rates of star formation or none at all.



Starburst galaxies, on the other hand, experience episodes of exceptionally high star formation, often triggered by <a href="https://www.earth.com/news/webb-captures-a-galaxy-collision-with-a-radiant-smile/">galactic collisions</a> or interactions. 



These events can funnel large amounts of gas into central regions, leading to intense star-forming activity. However, such bursts are usually short-lived on cosmic timescales, exhausting the available gas quickly.



The environment within a galaxy also plays a significant role. Stellar winds and supernova explosions from existing stars can both inhibit and promote star formation. They may disperse gas, preventing further collapse, or compress nearby clouds, triggering new star formation.&nbsp;



Over time, as galaxies evolve, the availability of gas diminishes, leading to a gradual decline in star formation activity.



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



The Puppis constellation in the southern sky represents the stern of a ship. It was once part of a larger constellation known as Argo Navis, which depicted the mythical ship of Jason and the Argonauts. 



However, Argo Navis was later divided into three separate constellations: Puppis, Carina (the keel), and Vela (the sails). Puppis is the largest of these three and contains many notable celestial objects.



This constellation is home to several bright stars, including Naos (Zeta Puppis), a hot, massive star that emits intense ultraviolet radiation. Puppis also hosts a wide variety of deep-sky objects, such as open <a href="https://www.earth.com/news/stunning-star-clusters-captured-in-the-extreme-outskirts-of-the-milky-way/" target="_blank" rel="noreferrer noopener">star clusters</a> and nebulae. 



Among these, Messier 46 and Messier 47 stand out. Both are beautiful star clusters that are visible through binoculars or small telescopes. The region is dense with stars because it lies along the <a href="https://www.earth.com/news/milky-way-collision-may-change-everything-we-know-about-our-galaxy/" target="_blank" rel="noreferrer noopener">Milky Way</a>, making it a prime area for stargazing and astrophotography. 



Image Credit: NASA



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NGC 2566: A cosmic eye in the Puppis constellation

Today's Image of the Day from NASA features the spiral...

Today's Image of the Day from the European Space Agency features the Cat's Eye Nebula (NGC 6543), located about 3,300 light-years from Earth in the constellation Draco.&nbsp;



The nebula's name comes from its eye-like appearance when viewed through a telescope. This particular image, which reveals the <a href="https://www.earth.com/news/horsehead-nebula-webb-telescope-captured-unprecedented-detail/" target="_blank" rel="noreferrer noopener">nebula</a> in stunning detail, was captured by the NASA/ESA Hubble Space Telescope.



<h2 class="wp-block-heading" id="h-planetary-nebulae-nbsp">Planetary nebulae&nbsp;</h2>



According to ESA, the Cat's Eye Nebula is one of the most complex planetary nebulae that has ever been discovered.



“A planetary nebula forms when Sun-like stars gently eject their outer gaseous layers to form bright nebulae with amazing twisted shapes," explained <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"Until recently, it was thought that shells around planetary nebulae were a rare phenomenon. However, astronomers have instead shown that these rings are likely to be the rule rather than the exception."



<h2 class="wp-block-heading" id="h-appearance-of-the-cat-s-eye-nebula-nbsp">Appearance of the Cat's Eye Nebula&nbsp;</h2>



The central focus of the Cat's Eye is a hot, dying star that has shed its outer layers to form the <a href="https://www.earth.com/news/dragons-egg-nebula-is-a-truly-stunning-sight-to-behold/" target="_blank" rel="noreferrer noopener">nebula</a>. It is surrounded by concentric gas shells, jets of high-speed gas, and unusual shock-induced knots of gas.



“Although the rings may be the key to explaining the final ‘gasp’ of the dying central star, the mystery behind the Cat’s Eye Nebula’s nested ‘Russian doll’ structure remains largely unsolved,” noted ESA.



<h2 class="wp-block-heading" id="h-rings-around-the-cat-s-eye">Rings around the Cat’s Eye</h2>



“This image, taken with Hubble's Advanced Camera for Surveys (ACS), reveals the full pattern of eleven or more concentric rings, or shells, around the Cat’s Eye. Each ‘ring’ is actually the edge of a spherical bubble seen projected onto the sky - which is why it appears bright along its outer edge.”



According to ESA, observations suggest that the star ejected its mass in a series of pulses at 1,500-year intervals. “These convulsions created dust shells that each contains as much mass as all of the planets in our solar system combined.”



Several explanations have been proposed for this phenomenon, including cycles of magnetic activity similar to our Sun's sunspot cycle, the influence of companion stars orbiting the <a href="https://www.earth.com/news/dying-stars-may-be-a-source-of-gravitational-waves/" target="_blank" rel="noreferrer noopener">dying star</a>, or stellar pulsations.&nbsp;



Another theory suggests that the material is ejected smoothly from the star, with the rings forming later due to the creation of waves in the outflowing material.



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



<a href="https://www.earth.com/news/extrasolar-ocean-planet-discovered-in-the-draco-constellation/" target="_blank" rel="noreferrer noopener">Draco</a> is a constellation in the northern sky that represents a dragon. It's one of the largest constellations, winding between the Big and Little Dippers.&nbsp;



In Greek mythology, Draco is often identified as the dragon Ladon, who guarded the golden apples in the garden of the Hesperides.



Draco is a circumpolar constellation for most northern hemisphere observers, meaning it never sets below the horizon and can be seen all year round.



<h2 class="wp-block-heading" id="h-famous-planetary-nebulae">Famous planetary nebulae </h2>



Planetary nebulae are some of the most beautiful and intriguing objects in the universe.&nbsp;



One of the most famous is the Ring Nebula, or M57, located in the constellation Lyra. This nebula is renowned for its nearly perfect ring shape, which is the result of a dying star shedding its outer layers.&nbsp;



Another well-known planetary nebula is the Helix Nebula, or NGC 7293, often referred to as the "Eye of God" due to its eye-like appearance. The Helix Nebula is one of the closest planetary nebulae to Earth, making it a popular target for amateur astronomers.&nbsp;



The Dumbbell Nebula, or M27, in the constellation Vulpecula, is another striking example. It is named for its resemblance to a dumbbell and is notable for being the first planetary nebula ever discovered, by Charles Messier in 1764.&nbsp;



The Butterfly Nebula, or NGC 6302, is located in the constellation Scorpius. Its name comes from its distinctive bipolar structure, resembling the wings of a butterfly. The nebula's central star is one of the hottest known, with a surface temperature of around 250,000 degrees Celsius.&nbsp;



The Eskimo Nebula, or NGC 2392, in the constellation Gemini, is known for its resemblance to a face surrounded by a fur parka, which gives it its name. Its intricate structure, including filaments and bubble-like shapes, makes it a fascinating object of study. 



These nebulae not only captivate us with their beauty but also provide valuable insights into the life cycles of stars and the processes that shape our galaxy.



Image Credit: NASA/ESA Hubble Space Telescope



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Cat's Eye Nebula in the constellation Draco

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

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 NASA Earth Observatory features the Messak Settafet, a rocky plateau located in the central Sahara Desert. It is part of the greater Messak Plateau, which stretches between the Erg Uan Kasa and the Murzuq Sand Sea.&nbsp;



The plateau's surface is characterized by blackened sandstone, sculpted by thousands of years of wind erosion. This dark patina, often referred to as "desert varnish," adds to its distinctive appearance. The region is starkly beautiful but harsh, with extreme temperatures and minimal <a href="https://www.earth.com/news/even-desert-plants-are-not-immune-to-climate-stress/" target="_blank" rel="noreferrer noopener">vegetation</a>.



<h2 class="wp-block-heading" id="h-image-of-the-messak-settafet">Image of the Messak Settafet</h2>



“Towering over the desert in southwestern Libya, the Messak Settafet plateau resembles the wall of a giant fortress, with its dark, erosion-resistant sandstone separating the Ubari Sand Sea to the north and the Marzūq Sand Sea to the south,” noted NASA.



“The large outcrop of Cretaceous rock features a sharp escarpment on its north side. The cliff, some 300 meters (1,000 feet) high in places, is lined with a thin dark shadow.”&nbsp;



“Dark debris from rockfalls is visible to the north. Note that an optical illusion called relief inversion can make high-elevation areas appear low and vice versa when shadows appear on the northern side of a feature.”



<h2 class="wp-block-heading" id="h-archaeological-significance-of-the-plateau-nbsp">Archaeological significance of the plateau&nbsp;</h2>



Messak Settafet is often referred to as the "land of stone tools" because it is one of the world's largest sites for prehistoric tools.&nbsp;



The area is littered with countless <a href="https://search.app?link=https%3A%2F%2Fwww.earth.com%2Fnews%2Fstone-tool-discovery-challenges-entire-theory-of-human-evolution%2F&amp;utm_campaign=aga&amp;utm_source=agsadl2%2Csh%2Fx%2Fgs%2Fm2%2F4" target="_blank" rel="noreferrer noopener">stone tools</a> and artifacts dating back to various prehistoric periods, including the Acheulean and Neolithic. These tools offer insights into early human technology and adaptation to desert environments.



“Signs of ancient tool making cover much of the plateau’s surface,” said <a href="https://www.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA</a>. “According to one archaeological survey, people discarded so many stone tools and rock fragments on the plateau over hundreds of thousands of years that roughly 75 artifacts per square meter now carpet the surface.”&nbsp;



“That makes this one of the earliest known examples of hominins modifying an entire landscape, according to the University of Cambridge archaeologists who conducted the survey.”



“Other signs of ancient activity include the bright spots that dot the image. These areas were likely quarrying pits where people dug up rocks and crafted them into tools, the archaeologists reported.”&nbsp;



<h2 class="wp-block-heading" id="h-rock-art-on-the-plateau-nbsp">Rock art on the plateau&nbsp;</h2>



The plateau is home to numerous petroglyphs and <a href="https://www.earth.com/news/negev-petroglyphs-ancient-art-rock-carvings-face-erosion-fungi-lichens/" target="_blank" rel="noreferrer noopener">carvings</a>. These engravings depict animals, humans, and symbolic designs, providing valuable clues about the lives, beliefs, and environments of the region's ancient inhabitants.&nbsp;



“For instance, Wadi Mathendous, a prehistoric archaeological site located in the southern part of the plateau, contains engravings of rhinoceroses, crocodiles, hippopotamuses, fighting cats, giraffes, long-horned buffaloes, and elephants. The art is thought to be about 8,000 years old,” said NASA.



Some of the animals depicted, such as giraffes and elephants, indicate that the Sahara was once a <a href="https://search.app?link=https%3A%2F%2Fwww.earth.com%2Fnews%2Fa-lush-green-sahara-desert-helped-early-humans-migrate-out-of-africa%2F&amp;utm_campaign=aga&amp;utm_source=agsadl2%2Csh%2Fx%2Fgs%2Fm2%2F4" target="_blank" rel="noreferrer noopener">much wetter</a> and more hospitable environment.



<h2 class="wp-block-heading" id="h-cultural-significance-of-the-messak-settafet">Cultural significance of the Messak Settafet</h2>



Messak Settafet forms part of the Rock-Art Sites of Tadrart Acacus, a UNESCO World Heritage Site since 1985. This designation highlights the area's importance for understanding early human culture and environmental changes in the Sahara.



The plateau has been a critical area for studying the migration and adaptation of early humans. Its archaeological richness offers a glimpse into how humans thrived in this region during periods when the climate was wetter.



“Although the plateau now receives less than 0.4 inches of rain annually, clues in the landscape make clear it was once much wetter,” noted NASA.



“Deeply incised dried stream valleys, or wadis, crisscross the plateau, indicating significant past water flow. The small, bright features scattered across the plateau are sand and silt deposits left where water once pooled.”



The Messak Settafet, like many remote <a href="https://www.earth.com/news/sahara-desert-dust-storms-carry-harmful-bacteria-and-fungi-around-the-globe/" target="_blank" rel="noreferrer noopener">desert</a> regions, faces challenges such as erosion, vandalism of ancient rock art, and the potential impacts of development. 



Efforts to preserve its archaeological treasures are vital for protecting its cultural and scientific significance.



The image was captured November 17, 2024 by the Operational Land Imager-2 (OLI-2) on Landsat 9 on&nbsp;



Image Credit: NASA Earth Observatory



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Messak Settafet plateau in the Sahara Desert

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

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. 



<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.&nbsp;



<h2 class="wp-block-heading" id="h-spiral-galaxies">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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Spiral galaxy NGC 6744 in the constellation Pavo

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 "Antennae" 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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The violent clash of the Antennae Galaxies  

Today's Image of the Day from <a href="https://earthobservatory.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA Earth Observatory</a> features Tropical Cyclone Tej as it approached the Arabian Peninsula on October 23, 2023.



"The VIIRS (Visible Infrared Imaging Radiometer Suite) sensor on the NOAA-20 satellite acquired this image of the storm at approximately 10:00 Universal Time on October 23 as it began to move over land," said NASA.



"The storm is forecast to weaken rapidly upon making landfall and meeting the cool, dry air over the peninsula. Still, it threatens to drop up to 500 millimeters (20 inches) of rain in some locations. In a region that receives less than 100 millimeters (4 inches) on average in an entire year, intense rains can cause damaging flash floods."&nbsp;



"In southern Yemen, authorities declared a state of emergency and suspended schools. In Salalah, Oman, the port was temporarily shut down and a hospital evacuated because of the storm, according to news reports."



Cyclonic storms in the Arabian Sea were once considered rare, but have become more common in the last decade. This is likely the result of rising ocean temperatures.



Tropical Cyclone Tej made landfall over the southern coast of Al Mahrah Governorate in eastern Yemen on October 24. According to media reports, at least seven people have died and more than 1,000 people have been displaced.&nbsp;



The storm is expected to produce heavy rainfall in desert regions of eastern Yemen and western Oman on Wednesday.&nbsp;



Image Credit: NASA Earth Observatory



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Tropical Cyclone Tej is dumping water in the desert

Denali,(also,Known,As,Mount,Mckinley,,Its,Former,Official,Name)

The rugged landscape of Alaska often leaves people spellbound with its soaring peaks and dramatic valleys. 



Many geologists believe that these mountains and valleys are more than scenic wonders. Interestingly, the Denali Fault plays a critical role in shaping this awe-inspiring Alaskan terrain. Recent work has given a fresh perspective on how entire land masses may have drifted, collided, and fused, over long stretches of time, to form what we recognize today as the North American landscape.



<h2 class="wp-block-heading" id="h-the-denali-fault-in-alaska">The Denali Fault in Alaska</h2>



Scientists have debated how <a href="https://www.earth.com/news/parker-solar-probe-will-fly-through-suns-atmosphere-tomorrow-for-the-first-time/" target="_blank" rel="noreferrer noopener">ancient fragments</a> of the western margin of North America joined together. The Denali Fault, a <a href="https://earthobservatory.nasa.gov/features/denali" target="_blank" rel="noreferrer noopener">massive feature</a> that slices through Alaska, has been at the center of many investigations.



New <a href="https://pubs.geoscienceworld.org/gsa/geology/article-abstract/52/12/933/649182/Orogen-scale-inverted-metamorphism-during?redirectedFrom=fulltext" target="_blank" rel="noreferrer noopener">findings</a> suggest that three, seemingly separate geologic sites, spread along roughly 620 miles (1,000 kilometers), were once a smaller unit that signaled the final bonding of far-flung pieces of Earth's crust.



Geologists propose that these linked sites were torn apart again over millions of years.



<h2 class="wp-block-heading" id="h-unraveling-tectonic-mysteries">Unraveling tectonic mysteries</h2>



Experts have long focused on the northern <a href="https://www.researchgate.net/publication/329259890_The_Dynamic_History_of_220_Million_Years_of_Subduction_Below_Mexico_A_Correlation_Between_Slab_Geometry_and_Overriding_Plate_Deformation_Based_on_Geology_Paleomagnetism_and_Seismic_Tomography" target="_blank" rel="noreferrer noopener">North American Cordilleran margin</a>, which has been tectonically active for <a href="https://www.uvic.ca/science/seos/assets/docs/afgreadings13.pdf" target="_blank" rel="noreferrer noopener">over 200 million years</a>. Large fragments, known as exotic terranes, are present along the margin. They were once separate pieces of crust that occurred in locations far from the site where they now rest. 



<a href="https://www.researchgate.net/publication/240674082_Wrangellia-A_displaced_terrane_in_northwestern_North_America" target="_blank" rel="noreferrer noopener">Wrangellia</a> is among the biggest of these terranes; it was an oceanic plate that formed far away before docking with North America, tens of millions of years ago. Over time, complex strike-slip faults like the Denali Fault have shifted and displaced these <a href="https://www.earth.com/news/earths-crust-is-dripping-under-turkey/" target="_blank" rel="noreferrer noopener">bits of crust</a>, masking the full story of how they first fused to the continent.



“We’re starting to recognize those primary features involved in the stitching, or the suturing, of once-distant land masses to the North American plate,” said <a href="https://scholar.google.com/citations?user=Lrz_LL8AAAAJ&amp;hl=en&amp;oi=ao" target="_blank" rel="noreferrer noopener">Regan</a>, an associate professor at the University of Alaska Fairbanks' <a href="https://www.gi.alaska.edu/" target="_blank" rel="noreferrer noopener">Geophysical Institute</a> and the UAF College of Natural Science and Mathematics (<a href="https://www.uaf.edu/cnsm/" target="_blank" rel="noreferrer noopener">CNSM</a>). 



<h2 class="wp-block-heading" id="h-shared-tectonic-history-of-alaska-and-yukon">Shared tectonic history of Alaska and Yukon</h2>



A major clue in these findings is something called inverted metamorphism. 



Typically, deeper rocks show higher temperatures and pressures, while shallower rocks show lower ones. Sometimes the order reverses, and <a href="https://www.earth.com/news/mantle-heat-shaped-earths-crust-3-billion-years-ago/" target="_blank" rel="noreferrer noopener">rocks</a> formed in hotter conditions appear above the cooler layers.



According to researchers, this phenomenon appears in the Clearwater Mountains of Southcentral Alaska, the Kluane Lake area of Canada’s southwestern Yukon, and the Coast Mountains near Juneau. 



It became clear that all three of these independent, inverted metamorphic belts formed at the same time under similar conditions. Inverted metamorphic belts often point to <a href="https://pubs.usgs.gov/publication/70012246" target="_blank" rel="noreferrer noopener">intense thrusting events</a>, where layers of rock get shoved over one another in ways that defy the usual temperature and pressure patterns.



<h2 class="wp-block-heading" id="h-how-the-denali-fault-shook-things-up">How the Denali Fault shook things up</h2>



Before this <a href="https://pubs.geoscienceworld.org/gsa/geology/article-abstract/52/12/933/649182/Orogen-scale-inverted-metamorphism-during?redirectedFrom=fulltext" target="_blank" rel="noreferrer noopener">study</a>, some geologists suspected that each region had its own separate story. 



Regan’s analysis indicates that the three sites were once part of a single zone where the final merging of an ancient oceanic plate and the North American continent took place <a href="https://dggs.alaska.gov/pubs/id/29785" target="_blank" rel="noreferrer noopener">between 72 million and 56 million years ago</a>.



The Denali Fault came into play when post-collision shifting rearranged these pieces, scattering what had been one geologic feature across hundreds of miles. 



Researchers suggest that analyzing the movement along the fault reveals how these fractured pieces still fit together.



<h2 class="wp-block-heading" id="h-monazite-holds-the-key">Monazite holds the key</h2>



Monazite is at the core of identifying the shared history of these three sites. This mineral contains lanthanum, cerium, neodymium, and sometimes yttrium. “It is just the most special little mineral; it can participate in a lot of reactions, so we can use it as a way to track the mineralogical evolution of a rock,” explained Sean Regan. 



Specialists measure slight changes in <a href="https://pure.port.ac.uk/ws/portalfiles/portal/4085484/In_situ_LA_ICP_MS_dating_of_monazite_from_aluminous_gneisses_insights.pdf" target="_blank" rel="noreferrer noopener">monazite’s composition</a> to determine the timing and conditions of its formation.



<h2 class="wp-block-heading" id="h-denali-fault-and-earth-s-tectonic-activity">Denali Fault and Earth’s tectonic activity</h2>



Beyond their technical significance, these discoveries remind us that Earth’s surface is far from static. 



North America’s western margin has lived through episodes of oceanic plates, volcanic arcs, and shifted terrains that continue to shape the mountains and valleys seen today. Researchers see the Denali Fault as a record of long-distance transport of <a href="https://www.earth.com/news/claim-earth-has-six-continents-not-seven-north-america-europe-connected/" target="_blank" rel="noreferrer noopener">crustal fragments</a>, revealing the final act in the complicated docking of the Wrangellia Composite Terrane.



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



Many wonder how these findings will inform geological models of Alaska and Western Canada in future.



Geologists stress that further fieldwork, improved dating methods, and more collaborations are necessary to verify the timing and extent of major tectonic shifts.



Some plan to re-examine old mapping data or look at newly exposed <a href="https://www.earth.com/news/nasa-swot-satellite-mission-maps-earths-ocean-floors-from-space-in-stunning-detail/" target="_blank" rel="noreferrer noopener">rocks</a> for additional clues. Even small details, like determining a rock’s age down to the nearest million years, may one day yield a clearer history of ancient movements.



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Scientists have finally learned how America's tallest mountain formed

The rugged landscape of Alaska often leaves people spellbound with...

Astronomers have identified a remarkable water reservoir hidden in a corner of the cosmos, circling a quasar more than 12 billion light-years away.



At that distance, the light we see today began its journey not too long after the universe itself formed. 



The water supply in this distant place is huge, containing the equivalent of about 140 trillion times all the water in Earth’s oceans combined.



This supply is sitting near a supermassive black hole that is about 20 billion times more massive than our sun. 



<a href="https://www.earth.com/news/oldest-black-hole-ever-discovered-dates-back-to-the-dawn-of-time/" target="_blank" rel="noreferrer noopener">The black hole</a> is surrounded by a quasar named APM 08279+5255, which pumps out as much energy as a thousand trillion suns. 



This quasar, according to astronomers, holds the farthest and largest known reservoir of water anywhere in the universe.



<h2 class="wp-block-heading" id="h-quasar-apm-08279-5255-and-its-water">Quasar APM 08279+5255 and its water</h2>



Matt Bradford, a scientist at NASA’s <a href="https://www.jpl.nasa.gov/" target="_blank" rel="noreferrer noopener">Jet Propulsion Laboratory</a> in Pasadena, Calif., leads one of the teams involved in the observations.



“The environment around this quasar is very unique in that it’s producing this huge mass of water,” said Matt Bradford. “It’s another demonstration that water is pervasive throughout the universe, even at the very earliest times.”



Both Bradford’s group and a separate team of astronomers studied APM 08279+5255 and its <a href="https://www.earth.com/news/massive-black-hole-is-seen-taking-a-nap-after-eating-too-much/" target="_blank" rel="noreferrer noopener">black hole</a>, which sits at the center and draws matter inward. 



As it does, it warms the surrounding gas and dust, forming an area filled with molecules that have never before been detected at such an immense distance.



<h2 class="wp-block-heading" id="h-understanding-quasars-the-basics">Understanding quasars -- the basics</h2>



Quasars were first noticed more than half a century ago when telescopes revealed puzzling sources of intense brightness in <a href="https://www.earth.com/news/hubble-took-the-closest-ever-image-of-a-quasar-and-captured-some-weird-things/" target="_blank" rel="noreferrer noopener">distant areas of space</a>. 



These objects are unlike any ordinary star. They shine brightly from the center of distant galaxies, outshining all their galaxy’s stars combined.



At their heart sit supermassive black holes, millions or billions of times heavier than our sun. As gas and dust spiral in toward one of these black holes, the swirling material heats up and <a href="https://www.earth.com/news/black-hole-jet-crashes-into-an-unidentified-object/" target="_blank" rel="noreferrer noopener">releases energy</a>. 



This energy blasts out across all kinds of wavelengths, making quasars some of the brightest, most energetic phenomena ever seen.



Observing quasars helps astronomers understand what the universe looked like long ago, since the light we see now began its journey billions of years in the past. 



Quasars can show how galaxies formed, how matter spread out, and how the earliest structures in the cosmos came together.



They can even help map the distribution of matter between galaxies, shining light on the regions that would otherwise remain unseen. 



Some quasars also launch <a href="https://www.earth.com/news/black-hole-jets-are-like-million-light-year-long-jedi-lightsabers/" target="_blank" rel="noreferrer noopener">huge jets of high-speed particles</a> that stretch across enormous distances. These jets can affect how stars form, influencing entire neighborhoods of cosmic material.



<h2 class="wp-block-heading" id="h-strange-place-to-find-water">Strange place to find water</h2>



Astronomers observed that water vapor is present in this quasar’s environment. It occupies a region spanning hundreds of light-years, with one light-year at around six trillion miles. 



Although the gas is thin by Earth standards, it is surprisingly warm and dense compared to what is typical in places like our <a href="https://www.earth.com/news/milky-ways-black-hole-formed-through-a-merger/" target="_blank" rel="noreferrer noopener">Milky Way</a>.



The temperature hovers around minus 63 degrees Fahrenheit, and the gas is roughly 300 trillion times less dense than Earth’s atmosphere. 



Still, it is about five times hotter and tens to hundreds of times denser than the gas seen in normal galaxies. With its unusual conditions, this region stands out as an unexpected find.



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



<a href="https://www.earth.com/news/oceans-of-water-vapor-may-be-involved-in-planet-formation/" target="_blank" rel="noreferrer noopener">Water vapor</a> is not just a molecule. Its presence here suggests that the quasar is bathing its environment in radiation that keeps the gas relatively warm. 



Astronomers also spotted other molecules, like carbon monoxide, hinting that there is an abundance of raw material that can feed the black hole as it continues to grow.



They estimate that there is enough gas for the <a href="https://www.earth.com/news/largest-map-of-supermassive-black-holes-unveiled/" target="_blank" rel="noreferrer noopener">black hole</a> to increase in size by about six times, although what actually happens next is not certain. 



Some of this gas may form new stars, while some might be thrown out into space instead. Either way, these measurements open a window into what conditions were like when the universe was still young.



<h2 class="wp-block-heading" id="h-quasars-water-and-life-s-building-blocks">Quasars, water, and life's building blocks</h2>



Detecting water vapor in such a distant quasar expands our knowledge of how <a href="https://www.earth.com/news/did-the-building-blocks-of-life-replicate-on-their-own/" target="_blank" rel="noreferrer noopener">building blocks</a> appear across vast stretches of time and space. 



Water is essential for life as we know it, and its presence billions of years ago suggests that the elements needed for life have been around for a very long time.



Beyond that, water plays a key role in shaping how stars and galaxies evolve. When gas clouds cool, water helps by allowing those clouds to collapse more easily, leading to star birth. 



By spotting it this far back, astronomers get new clues about how galaxies changed as the universe aged and matured.



<h2 class="wp-block-heading" id="h-how-they-found-the-water-quasar">How they found the water quasar</h2>



Bradford’s team began collecting data in 2008 with an instrument called Z-Spec at the California Institute of Technology’s Submillimeter Observatory (<a href="https://www.cso.caltech.edu/" target="_blank" rel="noreferrer noopener">CSO</a>). 



This 33-foot telescope sits near the summit of Mauna Kea in Hawaii. They later confirmed their findings using the Combined Array for Research in Millimeter-Wave Astronomy (<a href="https://www.mmarray.org/" target="_blank" rel="noreferrer noopener">CARMA</a>), a set of radio dishes located high in the Inyo Mountains of Southern California.



Meanwhile, another group led by Dariusz Lis, senior research associate in physics at Caltech and deputy director of the Caltech Submillimeter Observatory, used the Plateau de Bure Interferometer in the French Alps. 



In 2010, Lis’s team found hints of water in this quasar by detecting a single signature, while Bradford’s team uncovered multiple signals that revealed the massive amount of water present.



<h2 class="wp-block-heading" id="h-where-do-we-go-from-here">Where do we go from here?</h2>



To sum it all up, this discovery shows that even at a time when the universe was young, water formed and gathered in places we never would have guessed. 



Instead of seeing just cold, empty darkness out there, astronomers have spotted a real treasure -- an enormous reservoir of water swirling around a quasar more than 12 billion light-years away. 



This water vapor, along with the intense radiation from the black hole at the quasar’s center, paints a picture of an environment that is far denser, warmer, and more active than ordinary parts of the cosmos.



By studying this distant quasar, scientists can learn how the earliest galaxies came together and evolved. They can see how matter spread out, how black holes grew, and how even tiny molecules like water played a role in shaping the universe. 



Every new detail uncovered by these long-ago signals traveling through time and space helps make sense of the vast cosmic story we are all a part of.



***



Other authors on the Bradford paper, "The water vapor spectrum of APM 08279+5255," include Hien Nguyen, Jamie Bock, Jonas Zmuidzinas and Bret Naylor of JPL; Alberto Bolatto of the University of Maryland, College Park; Phillip Maloney, Jason Glenn and Julia Kamenetzky of the University of Colorado, Boulder; James Aguirre, Roxana Lupu and Kimberly Scott of the University of Pennsylvania, Philadelphia; Hideo Matsuhara of the Institute of Space and Astronautical Science in Japan; and Eric Murphy of the Carnegie Institute of Science, Pasadena. Funding for Z-Spec was provided by the <a href="https://www.nsf.gov" target="_blank" rel="noreferrer noopener">National Science Foundation</a>, <a href="https://www.nasa.gov" target="_blank" rel="noreferrer noopener">NASA</a>, the Research Corporation and the partner institutions.



The full study was published in the <a href="https://iopscience.iop.org/article/10.1088/2041-8205/738/1/L6/meta" target="_blank" rel="noreferrer noopener">Astrophysical Journal Letters</a>.



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Enough water to fill trillions of Earth-size oceans found circling a black hole

Astronomers have identified a remarkable water reservoir hidden in a...

Scientists have long studied Antarctica's icy frontiers to predict how our warming world could reshape coastlines everywhere. Their attention recently turned to an unexpected ally: an Antarctic octopus that inhabits the chilly waters around the continent.



This Antarctic octopus species, known among experts for its unique distribution, has offered vital clues about a time in the past when ice retreated, ocean passages opened, and sea levels rose. 



Its DNA carries signals of events that may happen again if global temperatures continue to rise.



<h2 class="wp-block-heading" id="h-antarctic-ice-and-turquet-s-octopus">Antarctic ice and Turquet’s octopus</h2>



Lead author Sally Lau of <a href="https://www.jcu.edu.au/" target="_blank" rel="noreferrer noopener">James Cook University</a> in Australia explained that the genetic markers in this marine invertebrate link to shifts in Antarctica’s ice sheets thousands of years ago. 



She said, “I understand and then apply DNA and biology as a proxy of changes to Antarctica in the past.”



Researchers focused on a species commonly called Turquet’s octopus (<a href="https://www.earth.com/wp-content/uploads/2024/12/Turquets-octopus_Pareledone-turqueti_west-Antarctic-ice-sheet_wais_credit-SAEF_1m.webp" target="_blank" rel="noreferrer noopener">Pareledone turqueti</a>), which is widespread around Antarctica and has been recognized for around four million years.



This cephalopod measures about half-a-foot (15 centimeters) long excluding its arms and weighs approximately 1.3 pounds (600 grams).



Because it lays relatively few large eggs that must be tended carefully on the seafloor, the animal tends not to wander far, making each population’s genetic signatures more distinct. Circular sea currents trap different groups in separate regions.



<h2 class="wp-block-heading" id="h-understanding-turquet-s-octopus-the-basics">Understanding Turquet’s octopus - the basics</h2>



Known for its adaptability to the icy environment, Turquet’s octopus (Pareledone turqueti) is a master of camouflage, using its ability to change color and texture to blend into its surroundings. 



It thrives at depths of around 200 to 500 meters, where sunlight barely reaches, making it an elusive creature for scientists to study. 



Despite living in such a harsh environment, Turquet’s octopus is well-equipped to survive, thanks to its remarkable physiology and unique behaviors.



For such a small creature, it plays an outsized role in the <a href="https://www.earth.com/news/akarotaxis-gouldae-new-banded-dragonfish-species-discovered-reveals-antarctic-ecosystem/" target="_blank" rel="noreferrer noopener">Antarctic ecosystem</a>. It’s a predator, feeding on smaller fish and invertebrates, and is an important part of the food web.



<h2 class="wp-block-heading" id="h-octopus-dna-and-antarctic-ice-sheet-melt">Octopus DNA and Antarctic ice sheet melt</h2>



Scientists analyzed genetic data across 96 samples taken over three decades from museum collections. Findings showed clear evidence that this octopus once traveled between the Weddell, Amundsen, and Ross seas.



The only way for that to have happened was if massive expanses of ice vanished, opening channels where water (and octopuses) could move freely.



Genetic mixing placed those moments of ice sheet collapse in the mid-Pliocene, roughly 3-3.5 million years ago, and again during the <a href="https://www.earth.com/news/accelerating-coastal-retreat-in-alaska-the-triple-threat/" target="_blank" rel="noreferrer noopener">Last Interglacial period</a>, between 129,000 and 116,000 years ago.



“This was the last time the planet was around 1.5 degrees warmer than pre-industrial levels,” said Lau.



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



Scientists report that human activity has so far raised global temperatures by 1.2C relative to late 1700s benchmarks.



Experts warn that the <a href="https://www.earth.com/news/west-antarctic-ice-sheet-melting-will-accelerate-regardless-of-climate-action/" target="_blank" rel="noreferrer noopener">West Antarctic Ice Sheet</a> (WAIS) could be unstable under current climate targets, with the potential to add around 10-15 feet (3.3-5 meters) of sea level rise long term.



This study provides empirical evidence indicating that the WAIS collapsed when the global mean temperature was similar to that of today, suggesting that the tipping point of future WAIS collapse is "close."



Another contribution described the analysis as “pioneering,” noting that “and this latest piece of evidence from octopus DNA stacks one more card on an already unstable house of cards.”



<h2 class="wp-block-heading" id="h-many-more-questions-remain">Many more questions remain</h2>



The researchers emphasized in their study that many factors can influence how quickly an <a href="https://www.earth.com/news/antarctica-is-greening-at-an-unprecedented-rate/" target="_blank" rel="noreferrer noopener">ice sheet melts</a>, including changing ocean currents and the interaction between ice and the underlying bedrock.



Additional mysteries include whether the sea level rise would stretch over many centuries or appear in a series of faster surges.



They also highlighted ongoing research into whether various forces, beyond warmer temperatures, triggered the previous collapses.



Low-lying coastlines face the brunt of these possibilities. Even a modest rise can reshape communities and infrastructure on a global scale.



Researchers point to growing data on past sea levels, combined with the new genetic work, as motivation for further studies into climate dynamics.



<h2 class="wp-block-heading" id="h-more-clues-from-the-southern-ocean">More clues from the Southern Ocean</h2>



Questions about Antarctica’s future intersect with the behavior of the <a href="https://www.earth.com/news/southern-ocean-absorbs-more-co2-than-previously-thought/" target="_blank" rel="noreferrer noopener">Southern Ocean</a>. 



Recent analysis led by <a href="https://scholar.google.com/citations?user=b-RiXNQAAAAJ&amp;hl=en" target="_blank" rel="noreferrer noopener">Professor Simon Josey</a>, an expert on ocean-atmosphere interaction at the UK’s National Oceanography Centre (<a href="https://noc.ac.uk/" target="_blank" rel="noreferrer noopener">NOC</a>), connected shrinking Antarctic sea ice to more powerful winter storms and major changes in ocean structure.



According to the findings, years with minimal sea ice are likely to experience heightened storm activity and notable shifts in how heat and nutrients move through the water.



One crucial observation centers on water density. When <a href="https://www.earth.com/news/rapid-antarctic-sea-ice-loss-is-causing-severe-storms-around-the-world/" target="_blank" rel="noreferrer noopener">surface waters lose heat</a>, they become heavier and sink more readily.



“The massive increase in ocean heat loss to the atmosphere is increasing the density of water at the sea surface to values not previously seen,” said Professor Josey.



This diving of denser water can alter how the ocean circulates, which then affects temperatures and nutrient flows over great distances.



<h2 class="wp-block-heading" id="h-antarctic-ice-turquet-s-octopus-and-the-future">Antarctic ice, Turquet’s octopus, and the future</h2>



Long-term changes in these deep currents might ripple through wider ocean basins, impacting weather patterns on other continents.



While many questions remain, scientists who investigate these signals from both ice sheets and marine life say the findings underscore the delicate balance of the <a href="https://www.earth.com/news/earth-polar-regions-changing-fundamental-alarming-ways/" target="_blank" rel="noreferrer noopener">polar environment</a>.



Observations from octopus DNA, past sea level data, and new measurements of ocean heat exchange all add to the conversation about how warming may influence global coastlines and climates.



Researchers continue searching for more clues. Some look to ocean sediments, others to geological evidence. Each piece offers a small glimpse into cycles of warming and cooling that have repeated over millennia.



The common thread is the realization that Antarctica, though distant for many, is entwined with planetary systems in ways that affect all of us.



The full study was published in the journal <a href="https://www.science.org/doi/10.1126/science.ade0664?ftag=YHF4eb9d17" target="_blank" rel="noreferrer noopener">Science</a>.



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Octopus DNA tells scientists that total collapse of the Antarctic ice sheet is 'close'

Scientists have long studied Antarctica's icy frontiers to predict how...

Peyote dots the southern tip of Texas, emerging amidst the dusty aridity and cracked earth like otherworldly creations. These bluish-green cacti, found only here and in northern Mexico, are no ordinary plants.



To the local Native American Church members, peyote is less of a plant and more of a holy presence. Places where peyote plants flourish are reverently referred to as the "peyote gardens."



Within the DNA of this modest plant lies a critical aspect of Native American culture. 



Peyote cacti have been steadfast companions to Indigenous communities, serving as healers for the physical and mental afflictions wrought by colonization, displacement, and the erosion of culture, religion, and language.



<h2 class="wp-block-heading" id="h-sacred-plant-with-a-controlled-substance">Sacred plant with a controlled substance</h2>



One might wonder what makes the peyote plant coveted. It contains a spectrum of psychoactive alkaloids, primarily the <a href="https://www.earth.com/news/hallucinogen-use-is-on-the-rise-among-young-adults/" target="_blank" rel="noreferrer noopener">hallucinogen</a> mescaline, which is known for its psychedelic properties.



Despite being a controlled substance under federal law, a 1994 amendment to the American Indian Religious Freedom Act allows Native Americans to use peyote for traditional religious purposes.



However, for the past two decades, access to this "medicine," as it is called, has been an escalating concern for the Native American practitioners of peyotism.



These practitioners, which make up a large group of 400,000 individuals in the United States, have raised concerns about their lack of access to peyote.



They attribute the dwindling availability of the slow-growing cactus to poaching, excessive harvesting, agricultural activities, housing developments, wind farms, the border wall, and the burgeoning <a href="https://www.earth.com/news/study-offers-new-explanation-for-how-psychedelic-drugs-work/" target="_blank" rel="noreferrer noopener">psychedelic</a> renaissance.



<h2 class="wp-block-heading" id="h-diverse-opinions-on-peyote-conservation">Diverse opinions on peyote conservation</h2>



While most agree about the dire need for peyote conservation, the Native American Church community houses a diversity of opinions on how to achieve this.



Some members are suspicious of investors' intentions and prefer government funding to safeguard the plant. Peyote, after all, represents more to them than a plant; it embodies the Creator's spirit.



Among many poignant anecdotes that highlight the spiritual significance of peyote, one stands out. 



Adrian Primeaux from the Yankton Sioux and Apache lineage recalls a tale of a malnourished Apache woman who was guided by a peyote plant to survival during a forced relocation by the U.S. government.



This plant wasn't merely a source of sustenance; it was a spiritual guide and a north star for the Native community navigating years of traumatic history.



<h2 class="wp-block-heading" id="h-the-return-of-peyote-gardens">The return of peyote gardens</h2>



In 2017, the National Council of Native American Churches purchased land in Hebbronville, Texas, to establish the Indigenous Peyote Conservation Initiative (IPCI). 



This non-profit organization oversees a peyote preserve that is not harvested but naturally propagated in its habitat.



Steven Benally, an IPCI board member, recalls his emotional return to the peyote gardens after years of disconnection, stating: "This is real!"



His words encapsulate the deep bond between the Native Americans and the peyote gardens.



<h2 class="wp-block-heading" id="h-the-delicate-balance-of-peyote-conservation">The delicate balance of peyote conservation</h2>



The debate on peyote conservation isn't a simple one. While some argue that cultivation outside of its natural <a href="https://www.earth.com/news/fossil-reveals-how-plants-use-winged-seeds-to-expand-their-habitats/" target="_blank" rel="noreferrer noopener">habitat</a> is necessary for the species's survival, many Native American Church members contest that such a move would dilute its sacred nature.



Hershel Clark, secretary for the Teesto chapter of the Azee Bee Nahagha of Diné Nation, explained that the ceremonial protocols were bestowed by the Creator. 



This is why growing peyote outside of its natural habitat or synthesizing it into pills is not supported.



<h2 class="wp-block-heading" id="h-funding-and-future-of-peyote-preservation">Funding and future of peyote preservation</h2>



Funding has been a significant challenge for peyote preservation efforts. While the Native American Church of North America seeks financial support from the U.S. government, IPCI has taken a different route.



The non-profit kick-started their endeavours with funding from the Riverstyx Foundation run by Cody Swift, a psychotherapist and psychedelic therapy research supporter. 



The organization continues to seek philanthropic dollars to propel its mission while remaining open to government funding.



However, there is a degree of skepticism about the intentions of Swift and other investors among some members of the Native American Church. 



Regardless, there is an indisputable consensus: the sacred peyote plant must be protected.



<h2 class="wp-block-heading" id="h-limited-supply-and-rising-demand">Limited supply and rising demand</h2>



It is clear that opening peyote up to a broader market could create a supply crisis that favors those with financial resources.



Native American Church members might find themselves struggling to access their <a href="https://www.earth.com/news/the-real-impact-of-burning-magic-herbs-in-spiritual-rituals/" target="_blank" rel="noreferrer noopener">sacred plant</a> while witnessing others use it in ways they consider profane. 



Zulema "Julie" Morales, one of only three licensed peyoteros legally allowed to harvest the plant for sale to church members, sympathizes with this sentiment.



Morales recalls a time when her father could fill a dozen large trays with peyote, but now she can barely fill one, not because of ethical harvesting practices, but because of illegal poaching.



As the <a href="https://www.earth.com/news/theory-of-native-american-origins-undermined/" target="_blank" rel="noreferrer noopener">Native American</a> communities continue to cherish, protect, and conserve the sacred peyote plant, the rest of the world must extend their understanding and respect for the unique spiritual bond shared by the communities and this modest, yet powerful, plant. 



Let it be a lesson to us all about the harmonious coexistence of man and nature, and the profound sacredness that can spring from such a bond.



Information for this article comes from a <a href="https://www.nbcdfw.com/news/local/texas-news/psychedelic-renaissance-development-threaten-peyote/3728887/#:~:text=An%20initiative%20to%20conserve%20and%20protect%20peyote&amp;text=He%20recalls%20losing%20access%20to,to%20Native%20American%20Church%20members.">release</a> by the Associated Press.



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Sacred peyote gardens: A cultural legacy under threat

Peyote dots the southern tip of Texas, emerging amidst the...

Quantum,Computing,Concept.,Digital,Communication,Network.,Technological,Abstract.

Northwestern University engineers made a remarkable advance in quantum computing and communication, demonstrating quantum teleportation over a standard fiber optic cable that already carries everyday Internet traffic.



This development shows that quantum communication might not require dedicated lines, which clears the path for easier and more widespread integration of quantum and classical data sharing.



<h2 class="wp-block-heading" id="h-path-for-quantum-networking">Path for quantum networking</h2>



The news centers around the idea that <a href="https://www.earth.com/news/parker-solar-probe-will-fly-through-suns-atmosphere-tomorrow-for-the-first-time/" target="_blank" rel="noreferrer noopener">quantum signals</a> -- information carried by delicate particles of light known as photons -- can travel alongside everyday Internet traffic without losing their integrity. This breakthrough demonstrates quantum teleportation, a process where the state of a particle (like a photon) is transferred to another distant particle without the initial particle moving physically.



<h2 class="wp-block-heading" id="h-science-behind-quantum-teleportation">Science behind quantum teleportation</h2>



By using entangled photons, this method enables secure, near-instantaneous data sharing and paves the way for future quantum networks.



The research team successfully tested a setup that allows <a href="https://www.earth.com/news/negative-time-observed-measured-tangible-in-new-quantum-experiments/" target="_blank" rel="noreferrer noopener">quantum</a> information to weave through the bustling flow of regular Internet data without interference. 



This achievement overcomes one of the biggest hurdles in making quantum networks a practical reality.



<a href="https://www.mccormick.northwestern.edu/research-faculty/directory/profiles/kumar-prem.html" target="_blank" rel="noreferrer noopener">Prem Kumar</a>, who oversaw the research, is a professor of electrical and computer engineering at Northwestern’s <a href="https://www.mccormick.northwestern.edu/" target="_blank" rel="noreferrer noopener">McCormick School of Engineering</a>. 



He is known for his contributions to quantum communication and serves as the director of the Center for Photonic Communication and Computing. In their recent work, Kumar and his collaborators introduce a new way of thinking about quantum signals alongside their classical counterparts.



<h2 class="wp-block-heading" id="h-entanglement-in-quantum-communication">Entanglement in quantum communication</h2>



Quantum teleportation stands out because it uses entanglement as a way to exchange information without physically sending matter across a distance. The concept traces back to <a href="https://journals.aps.org/pr/abstract/10.1103/PhysRev.47.777" target="_blank" rel="noreferrer noopener">Einstein,</a> <a href="https://journals.aps.org/pr/abstract/10.1103/PhysRev.47.777" target="_blank" rel="noreferrer noopener">Podolsky</a>, and Rosen in 1935. Scientists have since <a href="https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.70.1895" target="_blank" rel="noreferrer noopener">tested</a> quantum entanglement in labs, culminating in the formal proposal for quantum teleportation in 1993.



One of the biggest appeals of quantum teleportation is that it can occur almost as fast as light travels. Photons can become entangled so that performing a measurement on one instantaneously affects its partner, no matter how far away it is. “This is incredibly exciting because nobody thought it was possible; our work shows a path towards next-generation quantum and <a href="https://www.earth.com/news/elusive-quantum-negative-entanglement-entropy-deciphered-in-the-lab/" target="_blank" rel="noreferrer noopener">classical networks</a> sharing a unified fiberoptic infrastructure. Basically, it opens the door to pushing quantum communications to the next level,” enthused Kumar.&nbsp;



<h2 class="wp-block-heading" id="h-protecting-delicate-photons">Protecting delicate photons</h2>



Securing a clear route for single photons involves more than just adding them to an active cable. Ordinary Internet traffic typically relies on millions of light particles, so a handful of <a href="https://www.earth.com/news/google-record-shattering-quantum-ai-chip-accesses-parallel-universes/" target="_blank" rel="noreferrer noopener">quantum</a> photons can easily get lost or overwhelmed. The <a href="https://www.northwestern.edu/" target="_blank" rel="noreferrer noopener">Northwestern</a> team performed detailed studies on how light scatters inside the cable to see if there was a specific wavelength that experiences less clutter. 



They pinpointed that sweet spot and added special filters to reduce the noise generated by normal data traffic.



“Quantum teleportation has the ability to provide quantum connectivity securely between geographically distant nodes,” said Kumar. Past work suggested that large-scale <a href="https://www.earth.com/news/functioning-quantum-internet-makes-giant-stride-closer-to-reality/" target="_blank" rel="noreferrer noopener">quantum networks</a> might need specialized systems. Now, his findings reveal that this might not be strictly necessary, if signals are positioned in just the right place in the spectrum.



<h2 class="wp-block-heading" id="h-first-test-run-in-busy-channels">First test run in busy channels</h2>



Earlier demonstrations of quantum teleportation typically involved pristine settings or dedicated fibers. 



Some <a href="https://www.science.org/doi/10.1126/science.aan3211">researchers</a> believed that real-world cables, teeming with signals, would smother the faint quantum light. That assumption has been proven wrong.



In tests at Northwestern, the researchers ran quantum signals and classical communications over the same fiber optic cable without them colliding. 



They measured how well the <a href="https://www.earth.com/news/electrons-can-follow-neat-paths-even-in-chaotic-quantum-systems/" target="_blank" rel="noreferrer noopener">quantum information</a> arrived at its destination and confirmed that it was still correct at the other end. “Our work shows a path towards next-generation quantum and classical networks,” Kumar summarized.



<h2 class="wp-block-heading" id="h-real-world-infrastructure">Real-world infrastructure</h2>



The immediate plan is to scale the system to longer runs and then transition to underground fiber connections. 



The group believes that an eventual shift to real-world cables could be next. Building on single-pair teleportation, they also want to experiment with multiple pairs of <a href="https://www.earth.com/news/quantum-dance-entangled-photons-wave-functions-captured-real-time/" target="_blank" rel="noreferrer noopener">entangled photons</a> to achieve another crucial step known as entanglement swapping.



If that milestone is reached, quantum networks could begin to take shape across regions rather than only between two points. For critical operations in finance, defense, and data management, such networks could offer more secure connections thanks to the inherent secrecy of quantum methods, where any tampering is immediately noticeable.



<h2 class="wp-block-heading" id="h-broader-applications">Broader applications</h2>



The capacity to support <a href="https://www.earth.com/news/quantum-computer-can-instantly-execute-a-task-that-would-normally-take-47-years/" target="_blank" rel="noreferrer noopener">quantum connections</a> without setting up special cables makes many new ideas more viable. 



Distributed quantum computing, which relies on linking multiple quantum computers in different locations, would be simpler to establish. 



Distance-sensing tasks and advanced metrology could also benefit from more stable quantum links.



Even beyond computing, quantum networks have the potential to spur new technologies in encryption, imaging, and fundamental physics experiments. Researchers have also discussed using quantum entanglement to <a href="https://watermark.silverchair.com/020011_1_online.pdf?token=AQECAHi208BE49Ooan9kkhW_Ercy7Dm3ZL_9Cf3qfKAc485ysgAAAzAwggMsBgkqhkiG9w0BBwagggMdMIIDGQIBADCCAxIGCSqGSIb3DQEHATAeBglghkgBZQMEAS4wEQQMxOCNBnzx99LUOAbXAgEQgIIC41_WikXKemGuhWdzU4OnkQXRNjdQ5jj8bK5la7lzZlWPVXgV6KM-mv4frQgdokiIKWhEiPaL2MBMicf8FXjC7C9DHm7cmfKlXHX0RsBGMmNFXIf3tnlSoygfD_3DsxoPrGUO5slXsAOpR2nNcOJqQMHxOtS2vZo885BZQmEF8j2Tdz7Eih6K3tmVzUTRmYwHJ4KtMk-RjD1JHXfFwUnnQ0B-Qk9VmP_s05zipejBq28CbQySyGw7Mi-SfxNEW7qC-VEEFHy__hVKeExMG4HmltzHbp-k_zPnwktK7eEojGWH17mX6qfBGSE_fSGYQYHh82x6TLx2HdMBx2RVuTZIxpClItEPUEuHXIn4ZM4QBHWUlhzFcnm5moZmsfIxN9II_S8v4fKN3hCeAp8QpjjhQyT3coqB4S80iIXBN3V1wpJMknK0WwKpuekyl7Tpcv1zPchLng2_lN8TuajzF8lyuBSRFWKGg4nKkdwtCV3OnUweAUfYwNrQdUgY769pFqspGxXh7VPhcgDe8hcdc9-EX2Y7uz7jMMmDyc9q7sJ0jW1tM2tUVkXYpOvSVkcuFN5Qa4ud5D8xdQ4UUL1nvGnhvJuTvT1kv2WiRlSy-3_uhi75BUEPppoyIv22JtpjkcAmQYEmLgcSdROYaB7LB5ySLLQ1rRZW7BFQvI5W7Zv0FX64VIvx1sNCubj1HvROm9OR026h8Kt-VuE8YZwoGgUP4DPycn_gwFHMguRZfU_bbMIBnLyufXePFSsPB0Nfv_gpwYN6lNzD3oyZPbo5BumjsspwgrOmvZADcEM6hyqkhAOGBm5gf5QiFtGWxvY9pYT2xSR9LI6C8cxxDNl8VMtRCK2pwJ_e2sg6h3sdILLYVzHuF4DO7SWTW0unBeit2cvJtDSN-PcPRtsTvI5eYgQkwouAfEZ3o4fKme-h8q4Ik1RVGvz3kMW2bnGOvgK0LeIer5Frkr3op85V1mpuWR1-l-Jjq6M">synchronize distant clocks</a> or to share random numbers for cryptography at unprecedented levels of security.



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



Quantum teleportation has matured from a fascinating theory to a tool that is becoming more practical. 



While it is never straightforward to integrate delicate <a href="https://www.earth.com/news/unbreakable-encryption-brings-quantum-internet-communication-closer-to-reality/" target="_blank" rel="noreferrer noopener">quantum signals</a>, the Northwestern group’s accomplishment raises confidence that such integration is within reach.



Many experts have believed that building specialized infrastructure was an unavoidable cost of quantum networking. 



According to Kumar’s report, if wavelengths are picked carefully, classical signals and quantum information can coexist just fine. This line of thinking spares organizations from installing entire new grids of cables.



<h2 class="wp-block-heading" id="h-future-work-on-quantum-teleportation">Future work on quantum teleportation</h2>



In upcoming work, the researchers plan to expand the scope of their approach in longer segments to confirm that the method remains stable as cables stretch far past the lab. They will also design a multi-node demonstration to verify it can handle more than a single link. There is much excitement that existing communication channels, once tuned just right, could <a href="https://www.earth.com/news/artificial-atoms-qkd-quantum-communication-revolutionizing-data-protection-privacy/" target="_blank" rel="noreferrer noopener">carry quantum data</a> to distant points.



With such possibilities on the horizon, quantum teleportation may shift from a theoretical concept to a tool that transforms communication. 



The future might see quantum and classical networks working side by side in ways that once sounded unlikely.



The study is published in the journal <a href="https://opg.optica.org/optica/fulltext.cfm?uri=optica-11-12-1700&amp;id=565936" target="_blank" rel="noreferrer noopener">Optica</a>.



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"Impossible" quantum teleportation achieved on normal internet cables

Northwestern University engineers made a remarkable advance in quantum computing...

Have you ever wondered about the magic behind the formation of raindrops or picturesque snowflakes? Or maybe about the creation of the otherworldly rings surrounding Saturn? These processes are all tied to the intricate dance of aggregating particles in fluid dynamics.



Now, researchers from Skoltech are adding a new chapter to the understanding of this cosmic dance. The team has proposed innovative mathematical equations that promise to push the frontiers of both our natural and technological worlds.



This advancement addresses natural and engineered phenomena, ranging from rain and snow formation to the creation of planetary rings and industrial fluid flows.



<h2 class="wp-block-heading" id="h-simplified-approach-to-fluid-dynamics">Simplified approach to fluid dynamics </h2>



Fluid <a href="https://www.earth.com/news/quasiparticle-is-seen-for-the-first-time-and-only-has-mass-moving-in-one-direction/" target="_blank" rel="noreferrer noopener">aggregation</a> is a critical process observed in both natural and technological systems. 



In nature, water droplets come together to form rain, ice crystals merge into snowflakes, and particles orbiting planets coalesce into structures like Saturn's rings. These processes demonstrate how particles in fluids aggregate to create larger entities.



In technology, fluid aggregation plays a significant role in activities like aerosol painting (where particles form a smooth layer), powder transport in industries, and controlled explosions that rely on particle behaviors.



Understanding and predicting these phenomena are essential for improving various applications.



<h2 class="wp-block-heading" id="h-models-of-aggregating-particles">Models of aggregating particles</h2>



Physicist Marian Smoluchowski’s equations, developed in the early 20th century, were a major step in understanding how <a href="https://www.earth.com/news/particles-are-forming-in-the-atmosphere-in-an-unexpected-way/" target="_blank" rel="noreferrer noopener">particles</a> combine in fluids. 



For example, these equations could describe how small droplets in a mist merge to form larger drops, or how tiny ice crystals in clouds come together to create snowflakes. The equations calculated the rate at which particles of different sizes combined, providing insights into the overall aggregation process.



However, these equations assumed that the environment was uniform - meaning that there were no changes in temperature, pressure, or fluid movement.



For instance, the equations worked well in theoretical situations like a calm, evenly distributed mist but failed to account for real-world <a href="https://www.earth.com/news/strange-high-energy-cosmic-rays-did-something-outside-our-galaxy-send-them-here/" target="_blank" rel="noreferrer noopener">complexities</a>, such as turbulent winds in a storm cloud or uneven temperature distributions in the atmosphere.



To address these shortcomings, the research team tried combining Smoluchowski's equations with models of fluid dynamics like the&nbsp;Euler equations&nbsp;(for ideal fluids) and the&nbsp;Navier-Stokes equations&nbsp;(which include viscosity and other forces).



For example, in atmospheric science,&nbsp;they might use Smoluchowski’s equations to predict how raindrops grow while using the Navier-Stokes equations to simulate airflows in a storm cloud.



In industrial processes, they could use these models together to simulate how fine powder particles mix and aggregate in a turbulent airflow inside a factory.



The challenge, however, was that these two sets of equations were developed for entirely different purposes and mathematical frameworks. 



<h2 class="wp-block-heading" id="h-limitations-of-past-models">Limitations of past models</h2>



Smoluchowski’s equations focus on particle merging rates, while the Navier-Stokes equations focus on fluid movement. Merging them without a unified foundation sometimes caused errors. 



For example, in air pollution studies, combining the equations might incorrectly predict how soot particles cluster in turbulent air.



In planetary science, using these hybrid models could lead to inaccurate predictions about how particles form rings around planets like Saturn.



The root problem was that the mathematical assumptions of these two frameworks were not compatible, leading to unreliable results in complex scenarios.



For example, in a turbulent environment where particle sizes and motion vary significantly, the models could miscalculate aggregation rates or fail to predict certain behaviors, limiting their usefulness in both research and <a href="https://www.earth.com/news/tire-particles-must-be-recognized-as-a-distinct-environmental-threat/" target="_blank" rel="noreferrer noopener">practical applications</a>.



<h2 class="wp-block-heading" id="h-the-skoltech-solution-hydrodynamic-equations">The Skoltech solution: Hydrodynamic equations</h2>



Skoltech researchers <a href="https://crei.skoltech.ru/ai/people/alexanderosinsky" target="_blank" rel="noreferrer noopener">Alexander Osinsky</a> and Professor <a href="https://faculty.skoltech.ru/people/nikolaybrilliantov" target="_blank" rel="noreferrer noopener">Nikolay Brilliantov</a> addressed these challenges by developing new hydrodynamic equations. 



Instead of merging incompatible systems, they derived a unified framework from fundamental principles. Their novel equations incorporate coefficients that account for both reaction rates and fluid transport - essentially blending the best aspects of traditional approaches.



"Surprisingly, these are neither the reaction-rate, nor the transport coefficients familiar from the Navier-Stokes equations, but a combination of both in the form of kinetic coefficients of a new nature," explained Professor Brilliantov.



"They are as fundamental for aggregating fluids as viscosity and thermal conductivity are for ordinary fluids."



"Using extensive computer simulations, we have shown the accuracy and relevance of our novel Smoluchowski-Euler hydrodynamic equations with the new coefficients for some of the technologically important aggregating fluids."



<h2 class="wp-block-heading" id="h-scientific-and-industrial-applications">Scientific and industrial applications</h2>



This breakthrough has implications for both natural systems and human technologies. By enhancing the precision of fluid aggregation models, the new equations will improve predictions in the areas listed below.



<ul class="wp-block-list">
<li>Air pollution analysis: To understand how solid particles aggregate and disperse in the atmosphere.</li>



<li>Granular flow dynamics: To optimize processes involving powders and other granular materials.</li>



<li>Powder technology: To develop more efficient methods for handling and transporting powders.</li>



<li>Aircraft and automotive design: To refine fluid dynamics for better performance and safety.</li>
</ul>



The researchers validated their equations through extensive computer simulations, demonstrating their applicability to real-world systems. This unified approach eliminates the errors introduced by previous hybrid models, paving the way for more reliable analyses.



<h2 class="wp-block-heading" id="h-a-step-forward-in-fluid-dynamics">A step forward in fluid dynamics</h2>



The new equations represent a fundamental shift in how scientists model aggregation in fluids. By addressing long-standing limitations, Skoltech researchers have provided a tool that bridges gaps between theory and application. 



As Brilliantov noted, these kinetic coefficients hold the same significance for aggregating fluids as traditional properties like viscosity do for ordinary fluids.



This advance not only deepens our understanding of natural processes but also enhances engineering capabilities. Whether analyzing atmospheric phenomena, improving industrial processes, or designing vehicles, the implications are vast and far-reaching.



The unified framework developed by Skoltech promises to revolutionize fields where fluid aggregation plays a critical role.



The study is published in the journal <a href="https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.133.217201" target="_blank" rel="noreferrer noopener">Physical Review Letters</a>.



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From rain to Saturn’s rings: New equations push the boundaries of fluid dynamics

Have you ever wondered about the magic behind the formation...

For nearly 10 years, California’s offshore seafloors have been missing a once-abundant, vividly colored predator: the sunflower sea star. 



This large starfish - capable of stretching over 3 feet wide - cruises the ocean floor in hues of orange, yellow, or purple, gliding swiftly on thousands of tube feet. Its multiple arms, which can number up to 24, allow for remarkable mobility.



<h2 class="wp-block-heading" id="h-restoring-sunflower-sea-stars">Restoring sunflower sea stars</h2>



When a mysterious disease almost wiped out sunflower sea stars in 2013, a domino effect ensued. A large number of purple sea urchins devoured nearly all of Northern California's iconic kelp forests. 



Now, however, scientists are hopeful that the sunflower sea star might soon reclaim its place in the region’s marine environment. 



Several pioneering labs, including ones in the Bay Area and Monterey County, are successfully growing these starfish with the goal of bolstering the species and <a href="https://www.earth.com/news/sunflower-sea-stars-could-help-save-kelp-forests/" target="_blank" rel="noreferrer noopener">restoring balance</a> to local ecosystems.



<h2 class="wp-block-heading" id="h-sunflower-sea-stars-raised-in-tubs">Sunflower sea stars raised in tubs</h2>



At the <a href="https://www.calacademy.org/" target="_blank" rel="noreferrer noopener">California Academy of Sciences</a> in San Francisco, behind a closed exhibit and through a locked door, biologist Riah Evin has been overseeing 137 sunflower sea stars raised in saltwater jars and tubs. In these containers, the starfish are fed bits of herring to sustain their growth.



These juvenile stars are among the remnants of 11 million embryos that Evin began working with in February. "These are the survivors,” said Evin. “That's way better than I had hoped for.”



Eventually, many of them will be displayed at the Academy of Sciences, giving the public a rare glimpse of a starfish that has all but disappeared from California’s coastal waters.



<h2 class="wp-block-heading" id="h-scientific-value-and-conservation-goals">Scientific value and conservation goals</h2>



More importantly, these sunflower stars are crucial to research. By raising them from infancy, Evin and other scientists are contributing to an international conservation effort to better understand the species and protect it from future crises.&nbsp;



Named critically endangered in 2020, sunflower sea stars were the subject of a conservation roadmap in 2022 that called on labs to breed and study them.



If scientists manage to decode the genetics behind their resistance (or susceptibility) to the disease that nearly eradicated them, they may eventually release healthy individuals back into the Pacific Ocean.&nbsp;



The hope is that reintroduced sunflower sea stars could help control the region’s exploding purple urchin populations, paving the way for devastated <a href="https://www.earth.com/news/sea-otters-have-protected-california-kelp-forests-for-a-century/" target="_blank" rel="noreferrer noopener">kelp forests</a> to regrow.



“There's a lot of promise in where the research will head,” said Andrew Kim, a research scientist at <a href="https://mlml.sjsu.edu/" target="_blank" rel="noreferrer noopener">Moss Landing Marine Laboratories</a> on Monterey Bay, who is also growing sunflower sea stars. “I'm very hopeful.”



<h2 class="wp-block-heading" id="h-a-species-on-the-brink-of-extinction">A species on the brink of extinction</h2>



The statistics are sobering: since 2013, an estimated six billion sunflower sea stars have died from Baja California to Alaska because of an ailment known as sea star wasting disease.&nbsp;



With this critical predator absent, <a href="https://www.earth.com/news/gray-whales-struggle-as-purple-sea-urchins-destroy-kelp-forests/" target="_blank" rel="noreferrer noopener">purple sea urchins</a> have proliferated, ravaging entire undersea forests of bull kelp. Scientists say 96% of Northern California’s kelp forests have disappeared over that period.



Kelp forests are essential habitats for numerous marine creatures - from fish and abalone to sea otters. Otters, found south of the Bay, play a protective role by feeding on urchins, but their range does not extend far enough to rescue Northern California’s compromised kelp.



<h2 class="wp-block-heading" id="h-reintroducing-natural-predators">Reintroducing natural predators </h2>



While volunteers have tried “seeding” kelp and removing urchins by hand in select coves, experts believe that reintroducing natural predators like sunflower sea stars (and possibly <a href="https://www.earth.com/news/sea-otters-use-tools-to-access-larger-prey-and-protect-their-teeth/" target="_blank" rel="noreferrer noopener">sea otters</a>) would be more sustainable and far-reaching. 



Sunflower sea stars are exceptionally effective hunters, moving quickly across the seabed to overtake urchins before extending their stomachs to digest the prey externally. Afterward, only a clean shell remains.



<h2 class="wp-block-heading" id="h-maximizing-survival-and-preventing-cannabilism">Maximizing survival and preventing cannabilism </h2>



Yet researchers like Evin remain unsure of exactly how to keep these starfish flourishing. Scientists still do not fully understand the disease that decimated them, despite working on the puzzle for over a decade. In labs across the state, only six adult sunflower stars exist, and breeding techniques remain experimental.



“There's a little bit of a 'Thunderdome' going on,” Evin joked while describing the fiercely competitive environment in which younger stars can devour each other if food is scarce. One particularly aggressive individual managed to consume hundreds of its siblings.



Evin is also investigating what diet optimally sustains these stars, testing everything from urchins to prawns. This feeding research aims to maximize survival, preventing the cannibalism that can occur if the starfish lack adequate nutrition.



<h2 class="wp-block-heading" id="h-challenges-with-sunflower-sea-star-larvae">Challenges with sunflower sea star larvae </h2>



Back in February, Evin traveled to <a href="https://aquarium.ucsd.edu/" target="_blank" rel="noreferrer noopener">Birch Aquarium</a> in San Diego, where she helped spawn an adult male and female sunflower sea star using a hormone injection. The pair produced billions of eggs and sperm, which fused into embryos. 



Those offspring, divvied up among institutions like the Academy of Sciences and Moss Landing Marine Laboratories, are the foundation for current breeding trials.



Maintaining healthy conditions for tiny sea star larvae proved challenging - until Evin discovered they thrived in jars of saltwater spun by automated stirrers purchased from kitchen supply stores. 



The larvae eventually sprouted five arms, but many soon turned on each other, forcing Evin to fine-tune her feeding strategies.



<h2 class="wp-block-heading" id="h-understanding-the-mysterious-wasting-disease">Understanding the mysterious wasting disease </h2>



Scientists are also eager to analyze the starfish’s DNA to gain insights into the genetics behind the wasting disease. 



Before any reintroduction to the wild can happen, they must ensure they are not inadvertently reintroducing the pathogen into marine environments. Regulatory agencies want a clearer picture of the disease’s causes and transmission pathways.



“What we don’t want to do is reintroduce (the disease) to recovered sea star populations,” said Ian Kelmartin, an environmental scientist with the California Department of Fish and Wildlife. “To get a handle on that, we need to understand what the disease is.”



<h2 class="wp-block-heading" id="h-a-glimpse-of-hope-in-the-lab">A glimpse of hope in the lab</h2>



Until more is known, the starfish remain confined to facilities like Evin’s. Ashley Kidd, a project manager with the Sunflower Star Lab in Moss Landing, sees these labs as living arks - safe havens for a species on the brink.&nbsp;



“Zoos and aquariums are living arks,” she said. “It is tragic in a way, but very useful if you can use it in time.”



By nurturing sunflower sea stars in captivity, researchers aim to one day restore a key predator to the Pacific Ocean, where it can help rein in purple urchins and nurture the revival of kelp forests.&nbsp;



Whether that vision comes to fruition depends on cracking the mystery of sea star wasting disease and ensuring enough of these starfish can survive - and thrive - back in their underwater realm.



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Sunflower sea stars are nearly extinct, but scientists are growing them

For nearly 10 years, California’s offshore seafloors have been missing...

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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



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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



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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



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Kainji Lake in north central Nigeria

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Today’s Video of the Day from <a href="https://www.igb.illinois.edu/">Carl R. Woese Institute for Genomic Biology</a> reveals how scientists can modify common crops like soybean, rice, and wheat to protect them from heat stress.



“We need to double crop production by 2050 to feed a growing global population, and not only are we not on track to do that, but climate change is further complicating things,” said Amanda Cavanagh, a lecturer at the University of Essex. 



The study is part of Realizing Increased Photosynthetic Efficiency (RIPE), an international research project that aims to develop food crops that turn the sun’s energy into food more efficiently.



“Using an engineering approach we designed multiple alternative metabolic pathways to photorespiration. Testing them in the field showed increases in productivity which led Amanda to significantly move the project forward by showing our engineered plants can withstand pretty extreme temperature stress,” said study co-author and RIPE researcher Paul South.&nbsp;



“As the climate changes and temperature stresses increase the pressure on our global food supply, farmers will need every tool available including engineering approaches like the synthetic biology used here to maintain safe and productive harvests.”



The experts tested plants modified to have more efficient photorespiration to see if they were better adapted to warmer temperatures.&nbsp;



The team found that the engineered plants produced 26 percent more biomass than the wild-type plants exposed to the same temperatures, and had 15 percent less yield loss under the higher temperatures.



Video Credit: Amanda Nguyen/University of Illinois



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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



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Designing crops that can beat the heat

[sendtonews key="QGPzYnXEtN-1712599-12187" type="single"] Today’s Video of the Day from Carl...

Today&#8217;s Image of the Day from <a href="https://earthobservatory.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA Earth Observatory</a> features a false-color image of Hurricane Otis on October 24, 2023. The following day, the storm slammed into Acapulco in the state of Guerrero as a category 5 storm. 



At the time this photo was captured by the VIIRS (Visible Infrared Imaging Radiometer Suite) sensor on the NOAA-20 satellite, Otis was still a tropical storm with sustained winds of 65 miles per hour, and was located about 210 miles south of Acapulco.&nbsp;



&#8220;Otis remained a tropical storm until the afternoon of October 24. Then, in a matter of hours, it rapidly intensified into a major hurricane. By 06:25 Universal Time (12:25 a.m. in Acapulco) on October 25, Otis made landfall near the beach resort town with sustained winds of 165 miles per hour,&#8221; said NASA.



&#8220;According to news reports, Otis was the strongest hurricane on record to hit Mexico’s Pacific Coast, and the fastest-strengthening storm on record in the northeast Pacific.&#8221;



Major damage to infrastructure, flooding, and mudslides have been reported in the state of Guerrero, and the extent of the destruction is still not clear. The government is scrambling to provide relief to those affected, deploying 8,400 members of Mexico&#8217;s army, air force and national guard to help in the cleanup efforts.&nbsp;



Scott Braun, a research meteorologist at NASA’s Goddard Space Flight Center, said that Otis had “all the right ingredients” for rapid intensification.&nbsp;



“Conditions were present for rapid intensification, but it is hard to say at this time why the rate and magnitude of intensification were so great,” said Braun.



Image Credit: NASA Earth Observatory



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Hurricane Otis slammed into Acapulco as a category 5 storm

Today's Image of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features the galaxy ESO 300-16, which is located 28.7 million light-years from Earth in the constellation Eridanus



According to ESA, the galaxy is a ghostly assemblage of stars which resembles a sparkling cloud.&nbsp;



"A rogue’s gallery of distant galaxies and foreground stars complete this astronomical portrait, which was captured by the Advanced Camera for Surveys," said ESA.



"This observation is one of a series which aims to get to know our galactic neighbors; around three quarters of the known galaxies suspected to lie within 10 megaparsecs of Earth have been observed by Hubble in enough detail to resolve their brightest stars and establish the distances to these galaxies."



"A team of astronomers proposed using small gaps in Hubble’s observing schedule to acquaint ourselves with the remaining quarter of the nearby galaxies."



ESO 300-16 is a relatively small and remote dwarf galaxy. It is sometimes known as a "compact blue dwarf galaxy" because of its size and the intense blue colors indicating active star formation.&nbsp;



These galaxies are typically small, but they have high star-forming rates for their size. This kind of galaxy can provide insights into the process of star formation as well as galaxy evolution in general.



Dwarf galaxies are of particular interest to astronomers because they can help to provide understanding about the formation and evolution of galaxies in the early universe. They're also thought to play a role in the assembly of larger galaxies over cosmic time.



By studying galaxies like ESO 300-16, astronomers can hope to better understand how galaxies grow, evolve, and interact over time.&nbsp;



Image Credit: ESA



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