Today's Image of the Day from NASA Earth Observatory features an active landslide zone that has been shifting for decades on the Palos Verdes Peninsula in Los Angeles County.



This area, particularly in Portuguese Bend, experiences ongoing ground movement, with land sliding toward the ocean at varying rates of up to several feet per year. 



The instability is largely due to weak, water-saturated bedrock and the effects of <a href="https://www.earth.com/news/rising-seas-sinking-cities-land-subsidence-on-the-east-coast/">human activity</a>, including road construction and irrigation, which have exacerbated the natural movement.



<h2 class="wp-block-heading" id="h-analysis-of-the-landslide-zone">Analysis of the landslide zone</h2>



According to a recent report from NASA, the landslide zone on the Palos Verdes Peninsula has expanded.&nbsp;



“Researchers at NASA’s Jet Propulsion Laboratory in Southern California used data from an airborne radar to measure the movement of the slow-moving landslides on the Palos Verdes Peninsula in Los Angeles County,” the <a href="https://earthobservatory.nasa.gov/images/153893/los-angeles-area-landslide-expands">report</a> stated.



“The analysis determined that, during a four-week period in the fall of 2024, land in the residential area slid toward the ocean by as much as 4 inches (10 centimeters) per week."



“Portions of the peninsula, which juts into the Pacific Ocean just south of the city of Los Angeles, are part of an ancient complex of landslides that has been moving for at least the past six decades, affecting hundreds of buildings in local communities.”&nbsp;



NASA noted that the motion accelerated and the active area expanded following record-breaking rainfall in Southern California in 2023 and heavy <a href="https://www.earth.com/news/rainfall-is-increasingly-unpredictable-due-to-climate-change/" target="_blank" rel="noreferrer noopener">precipitation</a> in early 2024.



<h2 class="wp-block-heading" id="h-visualization-of-the-landslide-zone">Visualization of the landslide zone</h2>



To create the image, the Advanced Rapid Imaging and Analysis (ARIA) team used data from four flights of NASA’s Uninhabited Aerial Vehicle Synthetic Aperture Radar (UAVSAR) collected between September 18 and October 17, 2024.&nbsp;



“The UAVSAR instrument was mounted to a Gulfstream III jet flown out of NASA’s Armstrong Flight Research Center in Edwards, California, and the four flights were planned to estimate the speed and direction of the landslides in three dimensions,” explained NASA.



“In the image above, colors indicate how fast parts of the landslide complex were moving in late September and October, with the darkest reds indicating the highest speeds." 



"The arrows represent the direction of horizontal motion. The white solid lines are the boundaries of the active landslide area as defined in 2007 by the California Geological Survey.”



<h2 class="wp-block-heading" id="h-accelerating-land-movement-and-risks">Accelerating land movement and risks</h2>



Alexander Handwerger is a landslide scientist at the Jet Propulsion Laboratory who performed the analysis. “In effect, we’re seeing that the footprint of land experiencing significant impacts has expanded, and the speed is more than enough to put human life and infrastructure at risk,” said Handwerger.&nbsp;



The landslide activity in this region dates back to the 1950s, when road construction projects disturbed the already <a href="https://www.earth.com/news/two-billion-people-are-threatened-by-land-subsidence/">unstable terrain</a>, accelerating movement.&nbsp;



Since then, shifting ground has led to significant damage to infrastructure, including cracked roads, broken utility lines, and distorted buildings. The instability has made it difficult for the city to maintain roads and essential services in the affected areas.



Despite efforts to slow the movement, including drainage improvements and engineering solutions, the land continues to shift. Homeowners and city officials have had to adapt, with some structures built to withstand slow movement, while others have been abandoned.&nbsp;



The situation remains a challenge, with scientists monitoring the landslide to better understand its <a href="https://www.earth.com/news/landslide-predictions-could-become-94-percent-more-accurate/">behavior</a> and explore potential mitigation strategies.



Portuguese Bend is a well-known example of a continuously active landslide, highlighting the complex interaction between geology, human development, and environmental forces.



Image Credit: NASA Earth Observatory&nbsp;



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Landslide zone in Los Angeles County is expanding

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

Today's Image of the Day from the European Space Agency features the Southern Ring Nebula, also known as NGC 3132.



The nebula is located about 2,000 light-years away from Earth in the constellation Vela. This remarkably detailed image was created using data from Webb’s Near-Infrared Camera (NIRCam).



The Southern Ring Nebula is one of the more famous examples of planetary nebulae. It is often studied for its beauty and valuable insights into the end stages of stellar evolution.



<h2 class="wp-block-heading" id="h-stars-power-the-southern-ring-nebula-nbsp">Stars power the Southern Ring Nebula&nbsp;</h2>



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> is powered by two central stars in a binary system. The brighter star is actually a less massive companion. The fainter, dimmer star is the dying, hot central star that has shed its outer layers to form the nebula. 



The dimmer star is a white dwarf and is responsible for the ionization of the gas in the nebula, causing it to glow.



“The bright star at the center of NGC 3132, while prominent when viewed by NASA’s Webb Telescope in near-infrared light, plays a supporting role in sculpting the surrounding nebula," noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"A second star, barely visible at lower left along one of the bright star’s diffraction spikes, is the nebula’s source. It has ejected at least eight layers of gas and dust over thousands of years.” 



“But the bright central star visible here has helped ‘stir’ the pot, changing the shape of this planetary nebula’s highly intricate rings by creating turbulence." 



ESA explained that the pair of stars are locked in a tight orbit, which leads the dimmer star to spray ejected material in a range of directions as they orbit one another, resulting in these jagged rings.



<h2 class="wp-block-heading" id="h-characteristics-of-the-southern-ring-nebula">Characteristics of the Southern Ring Nebula </h2>



The Southern Ring Nebula displays a complex structure with multiple layers of gas and dust. 



The outer shells of the nebula consist of hydrogen and other elements that were ejected from the dying star in previous stages of its <a href="https://www.earth.com/news/young-stellar-objects-observing-the-early-lives-of-stars/" target="_blank" rel="noreferrer noopener">evolution</a>.&nbsp;These layers are illuminated by ultraviolet radiation from the central white dwarf.



<h3 class="wp-block-heading" id="h-coloration">Coloration</h3>



The colors seen in the Southern Ring Nebula come from the different gases present. For example, hydrogen emits red light, while oxygen emits blue-green light. 



These colors help astronomers study the composition and dynamics of the nebula.



<h3 class="wp-block-heading" id="h-size-and-shape">Size and shape</h3>



The nebula spans about half a light-year in diameter. Its intricate, symmetrical structure provides valuable insights into the late stages of <a href="https://www.earth.com/news/star-collapse-black-hole-instead-of-supernova-vanish-from-sky/" target="_blank" rel="noreferrer noopener">stellar evolution</a>, especially the processes involved in the shedding of outer layers by dying stars.



<h2 class="wp-block-heading" id="h-spotlights-from-a-bright-star">Spotlights from a bright star</h2>



ESA noted that hundreds of straight, brightly-lit lines pierce through the rings of gas and dust. “These ‘spotlights’ emanate from the bright star and stream through holes in the nebula like sunlight through gaps in a cloud."



“But not all of the starlight can escape. The density of the central region, set off in teal, is reflected by how transparent or opaque it is. Areas that are a deeper teal indicate that the gas and dust are denser - and light is unable to break free.”



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



According to ESA, this is not only a crisp image of a planetary nebula - it also shows us objects in the vast distances of space behind it. The transparent red sections of the nebula are filled with distant <a href="https://www.earth.com/news/galaxies-have-hearts-and-lungs-that-help-them-live-longer/" target="_blank" rel="noreferrer noopener">galaxies</a>.



“Look for the bright angled line at the upper left. It is not starlight - it is a faraway galaxy seen edge-on. Distant spirals, of many shapes and colors, also dot the scene. Those that are farthest away - or very dusty - are small and red,” said ESA.



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



Vela is a southern constellation that represents the sails of a ship. It was once part of a larger constellation called Argo Navis, which depicted the ship of the mythological hero Jason and the Argonauts. 



In the 18th century, Argo Navis was divided into three separate constellations: Vela (the sails), Carina (the keel), and Puppis (the stern).



Vela is notable for containing several interesting astronomical features. One of its most prominent stars is Gamma Velorum, also known as Suhail or Regor, which is a bright, massive star system consisting of multiple stars.&nbsp;



The constellation also hosts the Vela Supernova Remnant, the remains of a <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernova</a> explosion that occurred about 11,000 years ago. 



This remnant is associated with the Vela Pulsar, a neutron star that formed during the supernova explosion, which is one of the brightest pulsars in the sky.



Vela is best observed in the Southern Hemisphere, where it can be seen in the summer months. Its position along the Milky Way makes it a popular region for both amateur and professional astronomers to explore.



Image Credit: NASA, ESA, CSA, STScI



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Southern Ring Nebula in the constellation Vela 

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

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA/Hubble &amp; NASA



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Luminous spiral galaxy and a blue giant star

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA/Hubble &amp; NASA



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Violent clash of the Antennae Galaxies  

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA 



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

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Young stars illuminate a spiral galaxy in the constellation Pavo

Each year, billions of animals migrate in search of better conditions. These journeys shape ecosystems, drive evolution, and challenge individual survival. 



Migration, however, is not a simple instinctual response. It demands a blend of physical traits and behavioral choices. In <a href="https://www.earth.com/news/worlds-oldest-fish-coelacanth-presumed-extinct-for-60-million-years-before-rediscovery/" target="_blank" rel="noreferrer noopener">fish</a>, even a subtle anatomical difference - like eye size - can influence who migrates and who stays behind.



Recent research from <a href="https://www.lunduniversity.lu.se" target="_blank" rel="noreferrer noopener">Lund University</a> reveals that the European roach (Rutilus rutilus), a common freshwater fish, shows a surprising link between eye structure and migration behavior.



Specifically, roach that migrate between lakes and streams tend to have larger pupils than those who remain year-round in a single habitat. This physical feature helps them see better in murky water and boosts their ability to find food, a vital edge in the energy-intensive act of migration.



<h2 class="wp-block-heading" id="h-what-makes-a-fish-migrate">What makes a fish migrate</h2>



Roach are partial <a href="https://www.earth.com/news/native-fish-species-are-facing-double-trouble/" target="_blank" rel="noreferrer noopener">migrants</a>. That means only some individuals in a population leave the lake each winter to enter connected streams. 



The rest stay put, braving seasonal changes in place. This difference in behavior offers researchers a unique lens through which to understand how physical traits affect life strategies.



The research team, led by biologist Kaj Hulthén, tracked more than 2,000 roach across two Danish lakes - Loldrup Sø and Søgård Sø - over several years. 



They photographed the <a href="https://www.earth.com/news/climate-change-is-pushing-freshwater-fish-toward-the-poles/" target="_blank" rel="noreferrer noopener">fish</a>, implanted each one with a tiny transponder, and monitored <a href="https://www.earth.com/news/small-fish-species-are-the-big-catch-of-the-future/" target="_blank" rel="noreferrer noopener">movements</a> using underwater antennas placed at stream inlets and outlets.



“We started by taking photos of the fishes’ eyes and then followed the migration patterns of 2,000 individual roaches over several years and in two different lakes by using implanted electronic transponders,” said Hulthén, who is a biology researcher at Lund University.



“It was shown that roach that migrated had larger pupils relative to individuals that chose to stay in the lake throughout the year.” 



<h2 class="wp-block-heading" id="h-eye-size-matters-for-fish-that-migrate">Eye size matters for fish that migrate</h2>



Larger pupils allow more light into the eye, improving vision in low-light conditions. For roach, this visual boost helps detect tiny prey like zooplankton. Using simulations, the researchers showed that roach with larger pupils could see farther - especially in dim twilight conditions, when many <a href="https://www.earth.com/news/bleaching-effect-coral-loss-threatens-fisheries-and-livelihoods/" target="_blank" rel="noreferrer noopener">fish</a> feed.



Even a 1-4% increase in pupil diameter led to as much as a 5% increase in the volume of water a <a href="https://www.earth.com/news/fish-diversity-has-changed-dramatically-on-the-great-barrier-reef/" target="_blank" rel="noreferrer noopener">fish</a> could visually scan.



That matters because in aquatic environments, visual range often dictates feeding success. These small gains are enough to help migratory roach gather the energy reserves they need before entering food-poor winter streams.



In twilight, detection range for 1 mm prey reached up to 20 cm - enough for practical foraging. The advantage fades under starlight but remains relevant during dusk and dawn, which are key feeding times.



<h2 class="wp-block-heading" id="h-feeding-now-to-survive-later">Feeding now to survive later</h2>



Migrating roach face a trade-off. Streams have fewer predators but offer less food. To survive the winter, migrants must build up fat stores beforehand. Larger pupils may be a tool to gather more food before departure and to stay active longer each day by foraging in low light.



This connection between eyesight and feeding has deep evolutionary roots. Eye size reflects both opportunity and cost. Bigger eyes offer better vision, but they require more energy to build and maintain. For a migrating roach, the benefits seem to outweigh the cost.



“The fact that migrating individuals have an improved ability to detect visual objects such as zooplankton indicates strong selection for effective food searches. This is crucial to cover the energy needs that migration requires," said Hulthén.



"These results correspond well with previous research, which showed that migrating roach with insufficient energy reserves run a higher risk of dying in the streams."



<h2 class="wp-block-heading" id="h-fish-with-big-eyes-are-likely-to-migrate">Fish with big eyes are likely to migrate</h2>



In both study lakes, researchers found a clear pattern: roach with larger relative pupil sizes were more likely to migrate. 



The correlation was strongest in Søgård Sø, where murkier water creates a dimmer visual environment. This suggests that visual demands may vary by location, shaping individual behaviour accordingly.



On average, migrant roach in Søgård Sø had pupils 4.2% larger than residents. In Loldrup Sø, the difference was smaller at 1.1%. While modest, these changes are functionally significant. Larger pupils helped fish see better, especially in the dim light that dominates northern winters.



Roach are planktivores. They feed on small, fast-moving prey that require sharp eyesight to detect. Under experimental conditions, fish given more food before winter were more likely to migrate, did so earlier, and stayed in streams longer. Those with less food died more often. 



This supports the idea that strong visual skills, like those enabled by larger pupils, help fish meet their energy needs.



<h2 class="wp-block-heading" id="h-a-migratory-syndrome-takes-shape">A migratory syndrome takes shape</h2>



The study’s findings contribute to a growing view that migration is not just a behavioral choice. It’s a full-body strategy involving vision, body shape, energy storage, and risk-taking.



Together, these traits form a “migratory syndrome” - a suite of characteristics that help fish survive the challenges of moving between habitats.



The eye, often taken for granted in ecological studies, now appears central to this survival kit. By enhancing foraging efficiency, it helps determine who has the resources to leave and who stays behind.



“Roach play an important role in the ecosystem. By understanding why some individuals migrate and other don’t, we can gain a deeper insight into how fish populations respond to environmental changes, which in turn could affect both fish stocks and the lake dynamics as a whole,” said Hulthén.



<h2 class="wp-block-heading" id="h-fish-eyes-can-change-shape">Fish eyes can change shape</h2>



Whether these differences in eye morphology are genetic or a response to the environment remains unknown. 



However, past studies show that fish eyes can change shape depending on food availability and predator pressure. That means both nature and nurture could play roles in shaping eye size and which fish migrate.



Interestingly, the benefits of bigger eyes seem to matter most in moderate turbidity. In very clear water, all fish see well. In extremely dark or muddy water, vision may become useless. This window of usefulness hints at why migration-related eye differences show up more clearly in some lakes than others.



<h2 class="wp-block-heading" id="h-eye-size-and-fish-migration">Eye size and fish migration</h2>



Roach migration has ecological ripples beyond the fish themselves. Migrants affect predators, prey, and nutrient cycles. 



Understanding how physical traits like pupil size influence migration choices can help scientists predict how fish populations may respond to environmental change.



In this study, a tiny difference in pupil size revealed a key factor in migratory success. It highlights the tight link between form, function, and behavior.



Eyes, often symbols of awareness and insight, prove once again to be more than just windows to the world—they are tools of survival, helping fish decide whether to stay or go.



The study is published in the <a href="https://besjournals.onlinelibrary.wiley.com/doi/10.1111/1365-2656.70015" target="_blank" rel="noreferrer noopener">Journal of Animal Ecology</a>.



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Bigger pupils help migrating fish survive

Each year, billions of animals migrate in search of better...

Insects quietly run the world. They pollinate crops, recycle organic matter, and feed countless animals. Despite their importance, scientists know very little about how most insect species are doing. 



There are about one million known insect species. Yet only 1% - roughly 12,100 species - have been assessed by the International Union for Conservation of Nature (<a href="https://iucn.org" target="_blank" rel="noreferrer noopener">IUCN</a>). Among these, around 20% face threats of extinction.



Monitoring efforts have mostly focused on butterflies, dragonflies, and bumblebees in North America and Europe. Other regions, especially Africa, Asia, and South America, remain largely unstudied. The <a href="https://www.earth.com/news/insect-populations-dramatically-declining-around-the-world-rising-temperatures/" target="_blank" rel="noreferrer noopener">global picture</a> of insect health is still blurry.



<h2 class="wp-block-heading" id="h-urgent-plan-to-track-insect-declines">Urgent plan to track insect declines</h2>



To address this, scientists from the UK Centre for Ecology &amp; Hydrology (<a href="https://www.ceh.ac.uk" target="_blank" rel="noreferrer noopener">UKCEH</a>) and the Zoological Society of London (<a href="https://www.zsl.org" target="_blank" rel="noreferrer noopener">ZSL</a>) propose a broader method. Their goal is to act quickly before climate change, pollution, land use shifts, and invasive species cause irreversible harm.



The new method integrates several ways of studying insects. It includes long-term tracking of <a href="https://www.earth.com/news/insects-boost-plant-evolution-in-surprising-ways/" target="_blank" rel="noreferrer noopener">diversity</a> and abundance, comparisons across different habitats, structured expert input, and controlled experiments. The researchers believe this mix offers a more complete view than any single approach.



Dr. Rob Cooke is an ecological modeler at UKCEH and joint lead author of the study.



“We need to find out whether insect declines are widespread and what’s causing them. The challenge is like a giant jigsaw puzzle where there are thousands of missing pieces, but we do not have decades to wait to fill these gaps and then act,“ noted Dr. Cook.



“There is a lot of interest in monitoring charismatic <a href="https://www.earth.com/news/future-of-farming-insect-waste-reshapes-soil-health/" target="_blank" rel="noreferrer noopener">species</a> such as bees and butterflies, but few people care about the supposedly unpleasant insects, even though they too provide benefits for us." 



"For example, earwigs feed on aphids and other garden pests while cockroaches eat decaying material and keep soils healthy.”



<h2 class="wp-block-heading" id="h-an-insect-monitoring-system-that-works">An insect monitoring system that works</h2>



The framework combines time series trends, such as counting how butterfly <a href="https://www.earth.com/news/robotic-insects-may-be-the-future-of-farming-and-plant-pollination/" target="_blank" rel="noreferrer noopener">populations</a> shift over a decade. It also uses spatial comparisons to see how insects vary between forests, grasslands, or farms. 



Researchers conduct experiments that test insect responses to threats, like removing pesticides or invasive species from certain areas. When hard data is missing, they gather expert judgments to predict how insects may react to different pressures.



This layered approach lets scientists make more informed decisions while still being open about gaps and uncertainties. It balances speed and precision in a way that single-method studies cannot match.



<h2 class="wp-block-heading" id="h-case-for-insect-inclusion">Case for insect inclusion</h2>



“Insects are an incredibly important part of our ecosystems, pollinating around 80% of flowering plant species and vital for 35% of global food production, yet they are undervalued and understudied,“ noted Dr. Charlotte Outhwaite of ZSL’s <a href="https://www.zsl.org/what-we-do/institute-of-zoology" target="_blank" rel="noreferrer noopener">Institute of Zoology</a>, joint lead author of the study.



“With a million described species it would take too long to figure what works best for each species. Instead we want to find large-scale actions that benefit the most insects. For this, we need to use all the available information we have.”



To meet this goal, the scientists propose using known responses from well-studied insects to estimate how lesser-known species might respond under similar conditions. This gives policymakers a usable way forward, even if some data is still missing.



<h2 class="wp-block-heading" id="h-next-phase-of-the-glitrs-project">Next phase of the GLiTRS project</h2>



The new framework will now guide the Global Insect Threat-Response Synthesis (GLiTRS) project. Researchers aim to model insect responses to major threats across many environments. 



By combining all sources of data - field studies, expert insights, and experiments - they hope to build a reliable picture of insect health worldwide. This new framework doesn’t pretend to be perfect.



But it offers something we desperately need: a way to understand insect declines in real time, using every piece of information available. It also shows how science can adapt when faced with complex, global challenges.



Insects have been quietly supporting life on Earth for hundreds of millions of years. Now they need our attention. The question is not whether we care, but whether we will act before it's too late.



The project is backed by the&nbsp;Natural Environment Research Council (<a href="https://www.ukri.org/councils/nerc/" target="_blank" rel="noreferrer noopener">NERC</a>). It involves teams from the&nbsp;<a href="https://www.nhm.ac.uk/" target="_blank" rel="noreferrer noopener">Natural History Museum</a>,&nbsp;<a href="https://www.ucl.ac.uk/" target="_blank" rel="noreferrer noopener">University College London</a>, the&nbsp;<a href="https://www.cam.ac.uk/" target="_blank" rel="noreferrer noopener">University of Cambridge</a>, and&nbsp;<a href="https://www.imperial.ac.uk/" target="_blank" rel="noreferrer noopener">Imperial College London</a>.



The study is published in the journal <a href="https://www.science.org/doi/10.1126/science.adq2110" target="_blank" rel="noreferrer noopener">Science</a>.



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Very little is known about 99% of all insects on Earth

Insects quietly run the world. They pollinate crops, recycle organic...

The image of a cold Coca-Cola bottle on a summer day is iconic. But behind that image lies an escalating crisis. By 2030, Coca-Cola’s plastic waste could reach 1.33 billion pounds annually in oceans and waterways. 



That staggering figure comes from a new analysis by <a href="https://oceana.org/" target="_blank" rel="noreferrer noopener">Oceana</a>, a nonprofit focused on marine protection. The weight is enough to fill the stomachs of 18 million whales. 



It’s not just a problem of pollution anymore. It’s a symptom of unchecked growth and a warning sign of deeper environmental neglect.



The report lands at a time when microplastics have become nearly impossible to ignore. These tiny particles now <a href="https://www.earth.com/news/ocean-currents-may-soon-clean-up-waste-thanks-to-space-tech/" target="_blank" rel="noreferrer noopener">infiltrate ecosystems</a>, drinking water, and even human organs. Their presence is no longer surprising. 



What shocks scientists now is how quickly they’ve become a global threat.



<h2 class="wp-block-heading" id="h-health-risks-hidden-in-every-sip">Health risks hidden in every sip</h2>



The spread of microplastics brings real health concerns. Researchers increasingly link <a href="https://www.earth.com/news/how-scientists-are-using-air-to-recycle-plastic/" target="_blank" rel="noreferrer noopener">plastic particles</a> to cancer, infertility, and cardiovascular problems. 



As plastic breaks down in the ocean, it doesn’t disappear - it transforms into particles small enough to enter the human body. The food chain, starting from marine life, now carries traces of our packaging choices.



"<a href="https://www.coca-colacompany.com" target="_blank" rel="noreferrer noopener">Coca-Cola</a> is by far the largest manufacturer and seller of beverages in the world. Because of that, they really matter when it comes to the impact of all this on the ocean," said Matt Littlejohn, who leads Oceana's campaigns targeting corporate polluters.



That impact, as recent data show, is no longer hypothetical. It’s measurable, predictable, and expanding.



<h2 class="wp-block-heading" id="h-coca-cola-leads-plastic-pollution-rankings">Coca-Cola leads plastic pollution rankings</h2>



Coca-Cola ranks first among the world’s top plastic polluters. This ranking comes from a 2024 study published in Science Advances. 



Following closely behind are other major players like&nbsp;<a href="https://www.pepsico.com/" target="_blank" rel="noreferrer noopener">PepsiCo</a>,&nbsp;<a href="https://www.nestle.com/" target="_blank" rel="noreferrer noopener">Nestlé</a>,&nbsp;<a href="https://www.danone.com/" target="_blank" rel="noreferrer noopener">Danone</a>, and&nbsp;<a href="https://www.altria.com/" target="_blank" rel="noreferrer noopener">Altria</a>.&nbsp;Oceana&nbsp;used Coca-Cola’s own public data, from 2018 to 2023, and combined it with future sales projections. The picture it paints is not optimistic.



If current trends continue, Coca-Cola will exceed 4.13 million metric tonnes of plastic use per year by 2030. That translates to over 9.1 billion pounds of plastic annually. 



Using a peer-reviewed method published in the journal Science, researchers estimate that 1.33 billion of those pounds will end up in aquatic ecosystems. That equals nearly 220 billion half-liter plastic bottles.



<h2 class="wp-block-heading" id="h-insufficient-efforts-by-coca-cola">Insufficient efforts by Coca-Cola </h2>



Reusable packaging once appeared to be Coca-Cola’s answer to this crisis. In 2022, the company declared that reusable packaging was "among the most effective ways to reduce waste." 



They even announced a target: 25% of all packaging would be reusable by 2030. But in December 2024, that pledge vanished from their sustainability roadmap.



Instead of reuse, Coca-Cola’s current strategy focuses on recycling and collection. While those efforts sound helpful, environmental experts see them as insufficient. 



Recycling, especially when dealing with thin single-use plastic, often costs more energy than it saves. And worse, it shifts the burden from corporations to consumers.



"Recycling is great, don't get me wrong," said Littlejohn. "But if you're going to use recycled <a href="https://www.earth.com/news/plastic-treaty-is-a-historic-opportunity-to-stop-a-human-health-crisis/" target="_blank" rel="noreferrer noopener">plastic</a> to produce more single-use plastic, that's a problem."



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



The value of reusable packaging lies in its durability. A single glass bottle can be reused up to 50 times. Thicker PET plastic containers allow up to 25 uses before needing replacement. 



Each reuse reduces plastic waste, production emissions, and energy use. Despite this, major brands like Coca-Cola continue to push for recycling as the primary solution.



The company’s quiet withdrawal from its reuse goals weakens global efforts to reduce plastic output. Refillable systems demand infrastructure and planning, but they offer a long-term way out of the plastic loop. 



Recycling, in contrast, often serves as a short-term patch on a broken system.



<h2 class="wp-block-heading" id="h-coca-cola-s-plastic-use-and-climate-change">Coca-Cola’s plastic use and climate change</h2>



Plastic is not just a litter issue. It’s a carbon issue. Nearly all plastic is made from fossil fuels. That means every bottle contributes to climate change - from its production to its disposal.



The connection between plastic waste and rising global temperatures grows stronger with each report. Companies that produce single-use plastic on a massive scale add to both crises: environmental and climatic.



Yet Coca-Cola has shown that change is possible. In several countries, they already operate large-scale refillable systems. Brazil, Germany, Nigeria, and even regions in the United States, like southern Texas, have adopted these models.



"They have the largest reusable infrastructure of any beverage company, and they have the ability to grow that and show the way for the rest of the industry," said Littlejohn.



<h2 class="wp-block-heading" id="h-will-coca-cola-follow-through">Will Coca-Cola follow through?</h2>



Coca-Cola says it's still invested in refillable options. In a statement to AFP, a spokesperson shared: "We have been investing and remain committed to expand our refillable packaging options, and this work will continue as part of our consumer-centric strategy."



The words suggest hope, but critics remain skeptical. Without public targets or timelines, such promises risk becoming just another footnote in a <a href="https://www.earth.com/news/surprise-study-some-scientists-call-for-halting-ocean-plastic-cleanup-efforts/" target="_blank" rel="noreferrer noopener">growing crisis</a>. 



Real progress demands transparency and follow-through. The oceans are already paying the price of delay.



<h2 class="wp-block-heading" id="h-convenience-vs-commitment">Convenience vs. commitment</h2>



Coca-Cola, with its vast global reach, has the tools to drive real change. The company’s influence over supply chains, consumer habits, and industry trends makes it a key player in solving the <a href="https://www.earth.com/news/is-it-still-possible-to-save-the-ocean-from-plastic-pollution/" target="_blank" rel="noreferrer noopener">plastic crisis</a>. 



But leadership requires more than statements. It needs bold decisions that value long-term sustainability over short-term gain.



Recycling is not enough. The solution lies in reuse, reduction, and rethinking how beverage packaging works. As the world grapples with rising plastic levels and declining ocean health, Coca-Cola stands at a crossroads. 



What it chooses next could define its legacy - for better or worse.



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Coca-Cola is on pace to dump 1.3 billion pounds of plastic into our oceans each year

The image of a cold Coca-Cola bottle on a summer...

A single bad food experience can be enough to change eating habits for a lifetime. Now, researchers have identified the precise brain region responsible for this powerful type of memory in mice, offering insights into how the brain links cause and effect when there's a delay between them - like getting sick hours after a meal.&nbsp;



This discovery may not only explain why certain foods suddenly become unpalatable but could also inform research into other lasting memory associations, including those involved in trauma and PTSD.



The new findings come from neuroscientists at <a href="https://www.princeton.edu/" target="_blank" rel="noreferrer noopener">Princeton University</a> who set out to explore the brain mechanisms behind “one-shot learning,” where a single event creates a <a href="https://www.earth.com/news/how-does-our-brain-form-long-term-memories/" target="_blank" rel="noreferrer noopener">long-term memory</a>.&nbsp;



“I haven't had food poisoning in a while, but now whenever I talk to people at meetings, I hear all about their food poisoning experiences,” said lead author Christopher Zimmerman, a postdoctoral fellow at the Princeton Neuroscience Institute.&nbsp;



Inspired by such anecdotes, Zimmerman and his colleagues developed an experiment to understand how the <a href="https://www.earth.com/news/brain-health-and-diet-nutrition-helps-lower-dementia-risk/" target="_blank" rel="noreferrer noopener">brain</a> forms food aversions even when illness sets in long after eating.



<h2 class="wp-block-heading" id="h-effects-of-food-poisoning-in-the-brain">Effects of food poisoning in the brain</h2>



Working in the lab of professor Ilana Witten, Zimmerman began by introducing mice to a new flavor - grape Kool-Aid. “It's a better model for how we actually learn,” he explained.&nbsp;



“Normally, scientists in the field will use sugar alone, but that's not a normal flavor that you would encounter in a meal. Kool-Aid, while it's still not typical, is a little bit closer since it has more dimensions to its flavor profile.”



Mice were trained to poke their noses into a port to receive a drop of the drink. Half an hour later, they were given an injection to induce temporary illness, mimicking food poisoning.&nbsp;



When offered a choice two days later between Kool-Aid and plain water, they strongly avoided the former - evidence that the unpleasant outcome had left a strong impression.&nbsp;



But what most intrigued the team was discovering which part of the brain was responsible for this aversive memory: the central amygdala.



“If you look across the entire brain, where novel versus familiar flavors are represented, the amygdala turns out to be a really interesting place because it's preferentially activated by novel flavors at every stage in <a href="https://www.earth.com/news/secrets-of-learning-how-the-brain-stores-new-information/" target="_blank" rel="noreferrer noopener">learning</a>,” Zimmerman said.&nbsp;



“It’s active when the mouse is drinking, when the mouse is feeling sick later, and then when the mouse retrieves that negative memory days later.”



<h2 class="wp-block-heading" id="h-memories-of-food-poisoning-in-the-brain">Memories of food poisoning in the brain</h2>



The central <a href="https://www.earth.com/news/lizard-brain-shapes-social-abilities-in-humans/" target="_blank" rel="noreferrer noopener">amygdala</a> is a small structure located deep within the brain, known for processing emotional learning, particularly fear. 



The amygdala also receives a wide range of sensory information, including taste and smell, making it a logical - but previously unconfirmed - candidate for processing food-related memories.



Zimmerman recalled the thrill of the discovery: “I remember making the plot from the first animal and sharing it on Slack with Ilana. She was at my desk a minute later to talk about how exciting this is.”&nbsp;



That initial result was just the beginning. With more data, the researchers confirmed that the central amygdala plays a central role at every point in the learning process - when the flavor is first encountered, when sickness occurs, and when the memory is retrieved later.



<h2 class="wp-block-heading" id="h-from-the-gut-to-the-brain">From the gut to the brain</h2>



To understand how the feeling of illness connects to memory, the team followed clues from earlier studies. They identified specialized cells in the hindbrain that produce a protein called CGRP. These cells send direct signals to the central amygdala, forming a neural bridge between the gut and the brain.&nbsp;



When the researchers stimulated these cells 30 minutes after the mice had tasted Kool-Aid - without inducing actual illness - the mice still developed the same aversion.



Even more striking was the finding that sickness appeared to reactivate the same neurons that had responded to the Kool-Aid in the first place.&nbsp;



“It was as if the mice were thinking back and remembering the prior experience that caused them to later feel sick,” Witten said. “It was very cool to see this unfolding at the level of individual neurons.”



The researchers propose that novel flavors may “tag” neurons in the amygdala, priming them to remain sensitive to signals from the body for several hours after eating.&nbsp;



If the animal then experiences sickness during this window, the brain reactivates the tagged neurons and forges a lasting association between the flavor and the illness.



<h2 class="wp-block-heading" id="h-implications-beyond-the-dinner-table">Implications beyond the dinner table</h2>



Although the study focused on food aversion, the findings point to a broader framework for how the brain learns to link events separated by time - a process that's not well understood.&nbsp;



“Often when we learn in the real world, there's a long delay between whatever choice we’ve made and the outcome. But that’s not typically studied in the lab, so we don't really understand the neural mechanisms that support this kind of long delay learning,” Zimmerman said.&nbsp;



“Our hope is that these findings will provide a framework for thinking about how the brain might leverage memory recall to solve this learning problem in other situations.”



In addition to shedding light on everyday behaviors - like swearing off oysters after one bad experience - this research could have implications for how we understand <a href="https://www.earth.com/news/childhood-trauma-can-cause-muscle-decline-adult-life/" target="_blank" rel="noreferrer noopener">trauma</a>. 



Much like food poisoning, traumatic events are often followed by symptoms only after a delay, and yet they still form vivid, persistent memories in the brain.



By identifying the precise brain pathways involved in one-shot memory formation, scientists are a step closer to understanding how such associations are wired - and possibly how they might be rewired in the future.



The study is published in the journal <a href="http://dx.doi.org/10.1038/s41586-025-08828-z" target="_blank" rel="noreferrer noopener">Nature</a>,



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Food poisoning triggers lifelong changes in the brain

A single bad food experience can be enough to change...

A newly discovered species of parasitic wasp that lived alongside dinosaurs nearly 100 million years ago may have evolved a bizarre and highly specialized mechanism to trap other insects and turn them into unsuspecting incubators for its offspring.&nbsp;



Preserved in amber, the wasp appears to have used a Venus flytrap-like structure on its body to grasp potential hosts, offering scientists a fascinating glimpse into prehistoric parasitic behavior.



<h2 class="wp-block-heading" id="h-parasitic-wasp-like-no-other">Parasitic wasp like no other</h2>



The species, Sirenobethylus charybdis, was identified from 16 remarkably preserved specimens found in Cretaceous-period amber from Myanmar’s Kachin region. The research describes a novel grasping appendage located on the abdomen of the female <a href="https://www.earth.com/news/unexpected-find-inside-the-eye-of-a-tiny-wasp-megaphragma-viggianii/" target="_blank" rel="noreferrer noopener">wasps</a>.



“When I looked at the first specimen, I noticed this expansion at the tip of the abdomen, and I thought this must be an air bubble. It’s quite often you see air bubbles around specimens in amber,” said Lars Vilhelmsen, study co-author and a curator at the <a href="https://snm.dk/en" target="_blank" rel="noreferrer noopener">Natural History Museum of Denmark</a>.&nbsp;



“But then I looked at a few more specimens and then went back to the first one. This was actually part of the animal.”



The structure’s purpose quickly intrigued the research team, especially once they observed its mobility across different specimens. 



"Sometimes the lower flap, as we call it, is open, and sometimes it’s closed,” Vilhelmsen said. “It was clearly a movable structure and something that was used to grasp something.”



<h2 class="wp-block-heading" id="h-ancient-wasp-like-a-venus-flytrap">Ancient wasp like a Venus flytrap</h2>



While nothing quite like this structure exists among <a href="https://www.earth.com/news/stick-and-leaf-insects-have-all-evolved-the-same-basic-body-parts/" target="_blank" rel="noreferrer noopener">modern insects</a>, the researchers found the best comparison in an entirely different kingdom: the Venus flytrap.&nbsp;



“There’s no way you can know how an insect that died 100 million years ago was living. So you look for analogs in modern insect fauna. Do we have anything among wasps or other groups that looks like this?” Vilhelmsen said.&nbsp;



“And there’s no real analog within insects. We had to go all the way out of the animal kingdom into the plant kingdom to find something that remotely resembled this.”



Although the structure resembles a <a href="https://www.earth.com/news/well-built-fences-keep-predators-from-harming-livestock/" target="_blank" rel="noreferrer noopener">predator</a>’s trap, the team believes it was not used to kill. Instead, they propose that the wasp used it to seize other insects just long enough to lay eggs into their bodies.&nbsp;



Once released, the unwitting hosts would carry the wasp larvae, which would eventually consume them from the inside out. According to Vilhelmsen, the likely hosts were flying insects of similar size.



<h2 class="wp-block-heading" id="h-a-window-into-ancient-parasitism">A window into ancient parasitism</h2>



Modern <a href="https://www.earth.com/news/fruit-flies-have-a-new-weapon-to-defend-against-parasitic-wasps/" target="_blank" rel="noreferrer noopener">parasitoid wasps</a> engage in comparable reproductive strategies. For instance, cuckoo wasps lay their eggs in the nests of other species, leaving their offspring to feed on the host’s young.&nbsp;



Yet the unique abdominal trapping mechanism seen in Sirenobethylus charybdis has no true parallel in living insects, adding to its mystery.



The amber in which the fossils were preserved provided an exceptionally detailed view of the wasp’s anatomy. In addition to Sirenobethylus charybdis, other remarkable finds from Myanmar amber have included everything from dinosaur tails and ancient spiders to crab and ant fossils.&nbsp;



The specimen of this wasp was purchased by a fossil collector and later donated to <a href="https://eng.cnu.edu.cn/" target="_blank" rel="noreferrer noopener">Capital Normal University</a>’s Key Laboratory of Insect Evolution and Environmental Changes in 2016.



However, the use of Myanmar amber in scientific research has become controversial in recent years due to ethical concerns surrounding the country’s political instability and military conflicts. 



Some paleontologists have called for a halt on studying these specimens until issues around their provenance and trade are resolved.



<h2 class="wp-block-heading" id="h-speculation-over-the-wasp-s-flytrap">Speculation over the wasp’s flytrap </h2>



The peculiar form and function of Sirenobethylus charybdis has captured the attention of entomologists and paleontologists alike. Phil Barden, an associate professor at the <a href="https://www.njit.edu/" target="_blank" rel="noreferrer noopener">New Jersey Institute of Technology</a> who studies amber fossils, described the wasp as a “Cretaceous weirdo.”&nbsp;



“This is significant because there are around a million known insect species - even with all of that living diversity, there are still lots of unexpected surprises in the fossil record that are beyond imagination,” he said.



While Barden acknowledges the wasp flytrap hypothesis as “plausible,” he also expressed caution, noting it remains speculative.&nbsp;



“There appears to be clear evidence that the abdominal components would have had range of motion. There are also a number of setae, or hairs, that look to be in the right position to detect hosts and potentially immobilize them.”&nbsp;



Still, Barden suggested alternative possibilities, such as using the structure to sense prey in the soil or even to transport young wasps.



He also questioned why Sirenobethylus charybdis would need such a structure at all when many living parasitoid wasps rely solely on stingers or mouthparts to capture and manipulate hosts. This makes the discovery all the more intriguing.



<h2 class="wp-block-heading" id="h-unanswered-questions-and-new-possibilities">Unanswered questions and new possibilities</h2>



Vilhelmsen and his team believe a key clue lies in the wasp’s reproductive anatomy. The egg-laying organ, or ovipositor, is located directly adjacent to the clasping structure, supporting the theory that the mechanism was used during reproduction.&nbsp;



Yet all the known specimens are female, so scientists can’t rule out other functions, such as roles in mating.



“This is something unique, something I never expected to see, and something I couldn’t even imagine would be found,” Vilhelmsen said. “It’s a 10 out of 10.”



With every amber discovery, paleontologists inch closer to understanding the rich complexity of ancient ecosystems. And sometimes, as in the case of Sirenobethylus charybdis, they uncover something so strange and unexpected it defies comparison even among the millions of species alive today.



The study is published in the journal <a href="https://bmcbiol.biomedcentral.com/articles/10.1186/s12915-025-02190-2" target="_blank" rel="noreferrer noopener">BMC Biology</a>.



Image Credit: Qiong Wu



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Parasitic wasp had a 'flytrap' for snatching its victims

A newly discovered species of parasitic wasp that lived alongside...

Regardless of how far apart we sit on branches of the evolutionary tree, human faces are very different from those of our ancestors. Modern humans can be recognized by their smaller facial structure when compared with Neanderthals and other hominin ancestors.



Anthropologists have long wondered why this difference exists and what kind of developmental changes in our facial bones led our species toward this slimmer appearance.



This difference is particularly noticeable when modern humans are lined up alongside the fossils of bigger-boned <a href="https://www.earth.com/news/tinshemet-cave-discovery-neanderthals-early-humans-sharing-and-complex-interactions/" target="_blank" rel="noreferrer noopener">ancestors</a> from distant eras.



<a href="https://www.sciencedirect.com/science/article/pii/S004724842500020X?via%3Dihub" target="_blank" rel="noreferrer noopener">Researchers</a> recently compared the evidence of facial bone growth in humans, Neanderthal remains, and chimpanzee skeletons.



One of the lead investigators, <a href="https://www.eva.mpg.de/human-origins/staff/alexandra-schuh/" target="_blank" rel="noreferrer noopener">Alexandra Schuh</a> from the Max Planck Institute for <a href="https://www.eva.mpg.de/index/" target="_blank" rel="noreferrer noopener">Evolutionary Anthropology</a>, found that variations in the pace of bone growth may offer a core explanation for how our faces became more refined.



<h2 class="wp-block-heading" id="h-human-vs-neanderthal-faces">Human vs. Neanderthal faces</h2>



Studying different groups side by side helps scientists pinpoint which growth patterns set each group apart. 



By measuring bone sizes at various life stages, experts see how the developing face changes over time. 



This reveals important clues about broader evolutionary shifts that shaped our modern appearance and separated us from our <a href="https://www.earth.com/news/neanderthal-fossils-reveal-signs-of-a-population-collapse/" target="_blank" rel="noreferrer noopener">extinct predecessors</a>.



This comparative approach also pulls in data from surviving primate relatives like chimpanzees, which share many features but do not have the same facial proportions as seen in humans.



By including such living primates, scientists build a clearer timeline of how certain traits might have deep roots that stretch back millions of years.



<h2 class="wp-block-heading" id="h-growth-pattern-of-human-faces">Growth pattern of human faces</h2>



One key discovery is that our faces stop expanding earlier than those of other large-faced primates and extinct hominin groups.



A shorter growth window makes a difference in the final adult profile, since less time for bone growth means a smaller overall structure. 



This sets modern humans apart from their hefty-boned <a href="https://www.earth.com/news/neanderthal-evolution-was-more-complex-than-previously-thought/" target="_blank" rel="noreferrer noopener">relatives</a> that are seen in archaeological finds.



Scientists observed that Neanderthal faces, for instance, keep growing for longer, allowing for a robust jaw and broader midface to develop. 



This pattern contrasts with ours, where growth slows around adolescence and locks in a leaner form, perhaps hinting at an evolutionary tweak that conserves energy while still supporting vital functions like chewing.



“Our findings reveal that a change in development - particularly during late growth stages - led to smaller faces. Compared to Neanderthals and chimpanzees who continue growing longer, human facial growth stops earlier, around adolescence, resulting in a smaller adult face,” said Schuh.



<h2 class="wp-block-heading" id="h-inside-the-face-structure">Inside the face structure</h2>



Shifts in bone activities, including when cells deposit new layers or break down older layers, appear to guide this reduced growth. 



If the process winds down sooner, the upper jaw - called the <a href="https://www.kenhub.com/en/library/anatomy/the-maxilla" target="_blank" rel="noreferrer noopener">maxilla</a> - does not project forward as much, leading to a face that is more compact and less imposing than that of a <a href="https://www.earth.com/news/dna-analysis-reveals-most-recent-modern-human-to-interbreed-with-neanderthals/" target="_blank" rel="noreferrer noopener">Neanderthal</a>.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/04/neanderthal-skull_compared_human-skull_Philipp-Gunz_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/04/neanderthal-skull_compared_human-skull_Philipp-Gunz_1s.webp" alt="Left: computed tomographic (CT) scan of a Neanderthal fossil (La Ferrassie 1). Right: CT scan of a modern human. Credit: Philipp Gunz" class="wp-image-1964150"/></a><figcaption class="wp-element-caption">Left: computed tomographic (CT) scan of a Neanderthal fossil (La Ferrassie 1). Right: CT scan of a modern human. Click to enlarge. Credit: Philipp Gunz</figcaption></figure>



In larger-faced species, these bone activities remain more intense for a longer period, boosting the formation of thicker and more protruding features. 



This ongoing bone growth helps explain why some ancient skulls are strikingly big, and it shows that timing has a powerful role in setting each group’s appearance.



<h2 class="wp-block-heading" id="h-faces-grow-less-as-we-age">Faces grow less as we age</h2>



Even though certain facial traits appear early in life, a major distinction between <a href="https://www.earth.com/news/neanderthal-behavior-provides-clues-about-their-extinction/" target="_blank" rel="noreferrer noopener">species</a> emerges in those final developmental years before adulthood. 



“Identifying key developmental changes allows us to understand how species-specific traits emerged throughout human evolution,” said Schuh.



Researchers note that humans have a relatively extended childhood, yet our facial structures do not keep scaling up throughout that entire stage.



<h2 class="wp-block-heading" id="h-environmental-or-genetic-influences">Environmental or genetic influences</h2>



Some <a href="https://www.hup.harvard.edu/catalog.php?isbn=9780674046368" target="_blank" rel="noreferrer noopener">experts</a> argue that better food processing and cooking might reduce strain on our jaw, but this alone seems insufficient to explain every detail. 



Others point to social or behavioral factors, suggesting that selective pressures may subtly shape how the face grows over time.



Biological data indicate that genetic mechanisms controlling bone growth may strongly steer the pace at which the face expands. 



Hormonal changes during adolescence could further speed up or slow down these processes, but researchers caution that the full story likely involves an interplay of genes, environment, and daily habits.



<h2 class="wp-block-heading" id="h-connecting-human-and-neanderthal-faces">Connecting human and Neanderthal faces</h2>



Building on these findings, scientists plan to examine more fossils from different time periods to see if other ancient human groups followed a similar pattern. 



They hope to trace shifts in facial growth rates across regions, comparing how different populations balanced the demands of survival with changes in jaw development.



By mapping these variations, experts hope to gain insight into which traits are universal and which might be unique offshoots of specific environments. 



This sort of detective work across the <a href="https://www.britannica.com/science/fossil-record" target="_blank" rel="noreferrer noopener">fossil record</a> pulls together biology, culture, and history, giving us a broader grasp of what shaped our defining look.



Clues also emerge about social evolution, given that facial expression and recognition might factor into how communities function. 



A smaller face could offer advantages in communication or other areas, though pinning down a direct link calls for deeper investigation into prehistoric behavior and ecological pressures.



<h2 class="wp-block-heading" id="h-what-did-we-learn">What did we learn?</h2>



Scientists agree that the timeline of facial growth stands out as a key to understanding why we appear different from <a href="https://www.britannica.com/list/human-ancestors" target="_blank" rel="noreferrer noopener">ancestral humans</a>. 



Once that window shuts, the face remains smaller and less projected, a shift that may have opened doors to new adaptations while still meeting our species’ unique developmental needs.



These insights show that it is not only the shape of our face that changed, but also the time it took to get there. 



As research continues, discoveries about early growth may help us see that each subtle change in our bones has powerful consequences for our evolutionary course.



The study is published in the <a href="https://www.sciencedirect.com/science/article/pii/S004724842500020X" target="_blank" rel="noreferrer noopener">Journal of Human Evolution</a>.



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Did early humans and Neanderthals know they were different species? Perhaps, here's how

Regardless of how far apart we sit on branches of...

Fingerprint analysis has been a dependable tool in crime-solving for more than a century. Investigators lean on fingerprint evidence to identify suspects or connect them to specific crime scenes, believing that every print offers a distinctive code.



Yet, a team of researchers has found that prints from different fingers of the same person can sometimes appear more alike. 



This insight came from an <a href="https://www.earth.com/news/ai-will-outsmart-humans-when-we-crack-the-neural-code/" target="_blank" rel="noreferrer noopener">artificial intelligence</a> model that revealed surprising connections between prints. 



Hod Lipson, from Columbia Engineering, stands out in this effort to question widely accepted forensic norms, in collaboration with Wenyao Xu from the <a href="https://www.buffalo.edu/" target="_blank" rel="noreferrer noopener">University at Buffalo</a>.



<h2 class="wp-block-heading" id="h-ai-takes-on-fingerprints">AI takes on fingerprints</h2>



For decades, it has been taken for granted that fingerprints from different fingers of one individual do not match. Much of this belief stems from the assumption that each finger displays completely separate ridges, loops, and swirls. 



One anonymous reviewer even stated, “It is well known that <a href="https://www.earth.com/news/human-microbiome-trillions-of-bacteria-unique-like-fingerprints/" target="_blank" rel="noreferrer noopener">every fingerprint is unique</a>,” when confronted with the researchers’ work. 



Despite such resistance, an undergraduate senior at <a href="https://www.engineering.columbia.edu/" target="_blank" rel="noreferrer noopener">Columbia Engineering</a> named Gabe Guo spearheaded a study that contradicts this long-standing assumption.



By using a public U.S. government database with roughly 60,000 prints, Guo fed pairs of fingerprints into a deep contrastive network. Some pairs belonged to the same person, while others came from different people. 



The artificial intelligence system became adept at telling when prints that looked different were actually from one individual, reaching an accuracy of 77% for single pairs. 



In cases where multiple samples were grouped together, the accuracy soared, offering the possibility of boosting existing forensic methods by more than tenfold.



<h2 class="wp-block-heading" id="h-researchers-rocking-the-boat">Researchers rocking the boat</h2>



Although these findings promised fresh possibilities for connecting crime scenes, the researchers faced an uphill battle during peer review. 



The project was rejected by a well-established forensics journal that did not accept the suggestion that different fingers might produce prints with <a href="https://www.earth.com/news/molecular-fingerprints-could-be-key-to-early-cancer-detection/" target="_blank" rel="noreferrer noopener">shared characteristics</a>. 



Undeterred, the group sought out a broader readership. The paper was turned away once again, prompting Lipson to challenge the decision.



“If this information tips the balance, then I imagine that cold cases could be revived, and even that innocent people could be acquitted," noted Lipson, who co-directs the <a href="https://make.columbia.edu/" target="_blank" rel="noreferrer noopener">Makerspace Facility</a> at Columbia.



Determined not to back away from a challenge, even if it meant disrupting over 100 years of accepted practice, the team kept refining their work. 



Finally, their persistence paid off as their study was finally recognized and published in the peer-reviewed journal, Science Advances.



<h2 class="wp-block-heading" id="h-ai-gives-new-clues-in-fingerprint-analysis">AI gives new clues in fingerprint analysis</h2>



Traditional methods rely on minutiae, which refer to branching patterns and endpoints in the ridges. 



“The AI was not using ‘minutiae,’ which are the branchings and endpoints in fingerprint ridges - the patterns used in traditional fingerprint comparison," Guo explained. 



"Instead, it was using something else, related to the angles and curvatures of the swirls and loops in the center of the fingerprint.” 



His findings suggest that experts may have overlooked important visual cues.



The collaboration included Columbia Engineering graduate Aniv Ray and PhD student Judah Goldfeder, both of whom indicated that the project’s early success could grow stronger with bigger datasets. 



“Just imagine how well this will perform once it’s trained on millions, instead of thousands of fingerprints,” Ray remarked, hinting that this approach could eventually refine how investigators hunt for clues across multiple crime scenes.



<h2 class="wp-block-heading" id="h-potential-bias-and-next-steps">Potential bias and next steps</h2>



The researchers are alert to possible data gaps. They noted that their system showed similar performance across various demographics but emphasized the need for larger, more diverse fingerprint collections. 



They hope that thorough validation will address any concerns about bias before anyone adopts this technique in actual investigations. 



The long-term goal is to offer law enforcement a supplementary tool that improves efficiency when cases seem tangled.



While the AI cannot officially conclude a legal matter, it can help narrow the field of suspects or connect distinct crime scenes based on partial matches. 



“Many people think that AI cannot really make new discoveries - that it just regurgitates knowledge," Lipson elaborated, pointing to a broader shift in how AI might support investigative work.



"But this research is an example of how even a <a href="https://www.earth.com/news/new-era-in-forecasting-ai-will-improve-extreme-weather-warnings/" target="_blank" rel="noreferrer noopener">fairly simple AI</a>, given a fairly plain dataset that the research community has had lying around for years, can provide insights that have eluded experts for decades."



<h2 class="wp-block-heading" id="h-ai-fingerprints-and-law-enforcement">AI, fingerprints, and law enforcement</h2>



This study demonstrates that <a href="https://www.earth.com/news/could-generative-ai-go-mad-and-wreck-internet-data/" target="_blank" rel="noreferrer noopener">artificial intelligence</a> can spot patterns that traditional analysis methods might miss. It also highlights the value of open datasets that have been underutilized in many areas of research. 



The findings may prompt forensic experts to rethink certain procedures, especially when multiple prints from the same suspect turn up at different locations.



Lipson sees a future where unexpected breakthroughs can come from fresh perspectives. 



“Even more exciting is the fact that an undergraduate student, with no background in forensics whatsoever, can use AI to successfully challenge a widely held belief of an entire field," Lipson concluded. 



"We are about to experience an explosion of AI-led scientific discovery by non-experts, and the expert community, including academia, needs to get ready.”



The full study was published in the journal <a href="https://www.science.org/doi/10.1126/sciadv.adi0329" target="_blank" rel="noreferrer noopener">Science Advances</a>.



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AI proves that human fingerprints are not unique, upending 100 years of law enforcement

Fingerprint analysis has been a dependable tool in crime-solving for...

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



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



<figure class="wp-block-embed aligncenter is-type-video is-provider-youtube wp-block-embed-youtube wp-embed-aspect-16-9 wp-has-aspect-ratio"><div class="wp-block-embed__wrapper">
https://youtu.be/Ug657J67iEo?si=w96YjGMsg939LD_3
</div></figure>



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



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



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



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



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



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



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



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

Is chocolate the next nutritional powerhouse?

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

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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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

Flu viruses are more flexible than expected

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



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



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



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



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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

Detecting mercury contamination with the tap of a finger

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



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



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



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



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



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



Video/ Image Credit: European Space Agency&nbsp;



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



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

Kainji Lake in north central Nigeria

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This South Asian bird has a metallic blue crown and iridescent blue-green feathers with brilliantly colored eyespots. During courtship, the vibrant feathers are raised into a fan and put on display. Surprisingly, these extravagant feathers can also be used for flight.

Indian Peacock

The bright colors of the poison dart frog signal a warning to predators of the frog’s toxicity, also known as aposematic coloration. These frogs stand out even in the tropical forests of Costa Rica and Brazil, with some of the brightest shades of yellow, copper, red, green, and blue on the planet.

Indian Peacock

News coming your way