Today's Image of the Day from the European Space Agency features the vibrant colors of the Mawrth Vallis region of Mars. The image reveals a landscape abundant in iron, magnesium, and aluminum.&nbsp;



Mawrth Vallis lies just south of the dichotomy boundary, a ridge marking the divide between Mars' southern highlands and northern lowlands. Layered, clay-rich deposits found in this valley indicate prolonged interactions with water. 



Mawrth Vallis is considered a prime candidate for studying past habitability and the potential for preserved biosignatures. The region continues to captivate scientists due to its geological complexity and history of <a href="https://www.earth.com/news/mars-has-a-water-reservoir-two-miles-deep-enough-to-fill-earths-red-sea/" target="_blank" rel="noreferrer noopener">liquid water</a> flow. 



<h2 class="wp-block-heading" id="h-the-colors-of-mars">The colors of Mars</h2>



<a href="https://www.earth.com/news/air-samples-from-mars-could-reveal-fascinating-secrets/" target="_blank" rel="noreferrer noopener">Mars</a> gets its distinctive red color from iron oxides, or rust, on its surface. The Martian soil and dust are rich in iron minerals, which oxidize when exposed to the small amounts of oxygen present in the Martian atmosphere.&nbsp;



This oxidation process gives the planet its reddish hue, similar to how iron objects on Earth develop rust. 



The scattering of sunlight by these iron oxide particles further enhances the reddish appearance when viewed from a distance. However, the human eye can only perceive a fraction of Mars' <a href="https://www.earth.com/news/mars-captured-in-true-color-like-youve-never-seen-the-red-planet-before/" target="_blank" rel="noreferrer noopener">true color</a> palette.&nbsp;



<h2 class="wp-block-heading" id="h-striking-colors-revealed">Striking colors revealed</h2>



The European Colour and Stereo Surface Imaging System (CaSSIS) aboard the ExoMars Trace Gas Orbiter (TGO) offers a more detailed view, showcasing a striking diversity of colors.&nbsp;



This CaSSIS <a href="https://www.esa.int/ESA_Multimedia/Images/2024/06/Metallic_Mars_landscape" target="_blank" rel="noreferrer noopener">image</a> reveals yellow layers rich in iron and magnesium clays, overlain by white and blue layers abundant in aluminum.&nbsp;



The area is draped by a dark, heavily eroded layer, illustrating a vibrant, metallic landscape formed around 3.6 billion years ago.



<h2 class="wp-block-heading" id="h-upcoming-rosalind-franklin-mission">Upcoming Rosalind Franklin mission</h2>



The Rosalind Franklin mission is a joint mission by the European Space Agency (ESA) and Roscosmos aimed at exploring the surface of Mars to search for signs of past or present life. 



The mission is named after Rosalind Franklin, the pioneering British scientist whose work was crucial in the discovery of DNA's structure.



The rover is designed to drill up to two meters below the Martian surface, where it is believed any signs of life may be better preserved, away from the harsh surface radiation. 



The Rosalind Franklin rover was originally scheduled to launch in 2020, but technical delays and the COVID-19 pandemic pushed the launch window to 2028. 



Once on Mars, the rover will collaborate with other missions like NASA's Perseverance and Curiosity rovers to advance our understanding of the Red Planet's habitability and history.



<h2 class="wp-block-heading" id="h-studying-mars-ancient-past">Studying Mars’ ancient past</h2>



While Rosalind Franklin prepares for its mission, the TGO remains in orbit, conducting crucial research to unravel Mars' ancient past and assess its potential <a href="https://www.earth.com/news/secrets-of-mars-seismic-discoveries-and-the-quest-for-past-life/" target="_blank" rel="noreferrer noopener">habitability</a>.&nbsp;



Since beginning its full science mission in 2018, TGO has not only captured stunning images but also provided a comprehensive inventory of Mars' atmospheric gases and mapped water-rich locations on the planet's surface.



For six years, CaSSIS has delivered breathtaking views of Mars in vivid color, documenting features ranging from volcanic landscapes to active dust devils and immense sand dunes.&nbsp;



Understanding Mars' water history and its implications for past <a href="https://www.earth.com/news/mars-is-letting-out-mysterious-methane-burps-but-why/" target="_blank" rel="noreferrer noopener">life</a> remains a core focus of ESA’s ExoMars missions.



<h2 class="wp-block-heading" id="h-metals-on-mars">Metals on Mars</h2>



Mars is rich in various metals that contribute to its geological and mineralogical diversity. 



While iron is the most prominent, magnesium is also abundant. It is often found in the form of clays, contributing to the planet's diverse mineral composition. 



Aluminum is another significant metal present on Mars, commonly found in layered deposits and sediments. 



<h2 class="wp-block-heading" id="h-major-changes-over-time">Major changes over time</h2>



The metals are not evenly distributed but are found in various concentrations across the Martian surface. 



For instance, regions like Mawrth Vallis exhibit a complex layering of different metal-rich minerals, including iron and magnesium-rich clays overlain by aluminium-rich layers.&nbsp;



This diversity indicates a rich geological history involving water activity, volcanic processes, and sedimentary deposition.



The presence of these metals suggests that Mars has undergone significant chemical and physical processes over billions of years, shaping its current landscape.&nbsp;



Understanding the distribution and composition of metals on Mars helps scientists piece together the planet's history and assess its past potential for habitability.



Image Credit: ESA/TGO/CaSSIS



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Metallic Mars: The diverse colors of the Red Planet

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

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA/Hubble &amp; NASA



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Violent clash of the Antennae Galaxies  

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Hubble spotlights galaxies in the constellation Virgo

Today's Image of the Day from the European Space Agency features the galaxy ESO 300-16, which is located 28.7 million light-years from Earth in the constellation Eridanus. 



The galaxy is part of the ESO (European Southern Observatory) catalog, which includes a vast collection of galaxies observed in the southern hemisphere.



ESO 300-16 is notable for its chaotic structure, lacking the well-defined <a href="https://www.earth.com/image/hubble-captures-a-collection-of-spiral-galaxies/" target="_blank" rel="noreferrer noopener">spiral arms</a> or elliptical shape seen in many other galaxies.



<h2 class="wp-block-heading" id="h-ghostly-assemblage-of-stars">Ghostly assemblage of stars</h2>



According to <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>, ESO 300-16 is a ghostly assemblage of stars which resembles a sparkling cloud.&nbsp;



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



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



<h2 class="wp-block-heading" id="h-irregular-galaxy-structure">Irregular galaxy structure </h2>



ESO 300-16 lies at a relatively close distance to Earth compared to many other extragalactic objects, making it an interesting target for studies on galaxy formation and <a href="https://www.earth.com/news/massive-galactic-explosion-provides-clues-about-galaxy-evolution/" target="_blank" rel="noreferrer noopener">evolution</a>. 



The galaxy's irregular structure suggests that it may have undergone past interactions with other galaxies or is in a stage of dynamic evolution.



One of the most striking features of ESO 300-16 is its wispy, diffuse appearance, with scattered patches of bright star-forming regions embedded within a fainter background. This indicates ongoing star formation, which is a common characteristic of irregular galaxies. 



Unlike large <a href="https://www.earth.com/news/the-mesmerizing-beauty-of-spiral-galaxies/" target="_blank" rel="noreferrer noopener">spiral galaxies</a>, where star formation is often concentrated in well-organized arms, ESO 300-16's active regions are more randomly distributed.



<h2 class="wp-block-heading" id="h-raw-material-for-star-formation">Raw material for star formation</h2>



Due to its irregular nature, the galaxy does not have a well-defined nucleus. Instead, it appears as a loose collection of stars, gas, and dust, which astronomers can study to understand the processes shaping such galaxies. 



Irregular galaxies like ESO 300-16 are often rich in gas and dust, providing the raw material for new stars to form. 



Observations in different wavelengths, such as infrared and ultraviolet, can help reveal the presence of young, hot stars and cooler dust clouds that might be sites of future <a href="https://www.earth.com/news/star-formation-reignited-in-the-galaxy-leo-p-after-billions-of-years/" target="_blank" rel="noreferrer noopener">star formation</a>.



<h2 class="wp-block-heading" id="h-studying-the-evolution-of-galaxies">Studying the evolution of galaxies </h2>



Hubble observations of ESO 300-16 provide insight into the structure and stellar populations of the galaxy, helping astronomers piece together its history and evolutionary path. 



The study of galaxies like ESO 300-16 contributes to our broader understanding of how galaxies form and evolve, especially those that do not fit into the traditional classifications of spirals and ellipticals.



Because irregular galaxies are often shaped by gravitational interactions or past mergers, ESO 300-16 may have had a turbulent past. 



It could have once been part of a larger system before being disrupted, or it might have formed in an environment where gravitational influences from nearby galaxies prevented it from developing a more regular shape. 



Studying its motion and the distribution of its stars can provide clues about any past interactions it may have experienced.



<h2 class="wp-block-heading" id="h-a-glimpse-into-the-early-universe">A glimpse into the early universe </h2>



ESO 300-16 also provides a glimpse into what some galaxies in the early <a href="https://www.earth.com/news/universe-is-expanding-faster-than-science-can-explain-hubble-tension-physics-crisis/" target="_blank" rel="noreferrer noopener">universe</a> might have looked like. 



Many early galaxies were irregular in shape before evolving into more structured forms over time. As a result, studying nearby irregular galaxies like ESO 300-16 can offer valuable analogs for understanding galaxy formation in the distant past.



Although ESO 300-16 is not one of the most famous galaxies, it remains an important object for astronomers studying irregular galaxies, star formation, and the role of interactions in shaping galactic structures. 



Image Credit: ESA



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Ghostly galaxy in the constellation Eridanus

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



The Rosetta Nebula is a vast cloud of gas and dust located in the constellation Monoceros, also known as the Unicorn. Shaped like a blooming rose in deep space, it lies about 5,200 light-years from Earth and spans roughly 100 light-years in diameter.&nbsp;



<h2 class="wp-block-heading" id="h-image-of-the-rosetta-nebula-nbsp">Image of the Rosetta Nebula&nbsp;</h2>



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



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



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



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



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



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



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



<h2 class="wp-block-heading" id="h-nebulae-that-are-similar-to-rosetta-nbsp">Nebulae that are similar to Rosetta&nbsp;</h2>



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



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



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



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



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



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



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



<h2 class="wp-block-heading" id="h-history-of-the-rosetta-nebula-nbsp">History of the Rosetta Nebula&nbsp;</h2>



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



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



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



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



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



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



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



Image Credit: ESA



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Rosetta Nebula: Sculpted by starlight over millions of years

Today's Image of the Day from the European Space Agency features the spiral galaxy NGC 5643, which is located roughly 40 million light-years away in the constellation Lupus.&nbsp;



NGC 5643 belongs to the Hubble classification SBc, indicating that it is a barred spiral galaxy with loosely wound arms.&nbsp;



Its orientation, nearly face-on to Earth, provides astronomers with an exceptional view of its detailed spiral structure and central bar.



<h2 class="wp-block-heading" id="h-ngc-5643-a-grand-design-spiral-nbsp">NGC 5643: A grand design spiral&nbsp;</h2>



“NGC 5643 is what’s known as a grand design spiral, referring to how the galaxy’s two large, winding spiral arms are clear to see,” noted <a href="https://www.esa.int/ESA_Multimedia/Images">ESA</a>. “The spiral arms are defined by bright blue stars, lacy reddish-brown dust clouds and pink star-forming regions.”



“As fascinating as the galaxy appears at visible wavelengths, some of NGC 5643’s most interesting features are invisible to the human eye.”&nbsp;



<h2 class="wp-block-heading" id="h-intense-activity-in-ngc-5643">Intense activity in NGC 5643</h2>



This galaxy is notable for its Seyfert 2 nucleus, a type of active galactic nucleus (AGN). The intense activity in its core is powered by a supermassive <a href="https://www.earth.com/news/awakening-of-a-black-hole-witnessed-for-the-first-time/">black hole</a> that accretes surrounding material, emitting energy across a wide range of wavelengths.&nbsp;



“When a supermassive black hole ensnares gas from its surroundings, the gas collects in a disc that heats up to hundreds of thousands of degrees. The superheated gas shines brightly across the electromagnetic spectrum, but especially at X-ray wavelengths,” said ESA.



Observations have revealed jets and outflows of material emanating from the nucleus, likely driven by the black hole’s activity.&nbsp;



NGC 5643’s AGN has been studied extensively for its role in galactic evolution, particularly in how its energetic processes interact with the galaxy’s interstellar medium.



<h2 class="wp-block-heading" id="h-the-mystery-of-ngc-5643-x-1">The mystery of NGC 5643 X-1</h2>



ESA pointed out that NGC 5643’s active galactic nucleus isn’t the brightest source of X-rays in the galaxy. 



“Researchers using ESA’s XMM-Newton discovered an even brighter X-ray-emitting object, called NGC 5643 X-1, on the galaxy’s outskirts. What could be a more powerful source of X-rays than a <a href="https://www.earth.com/news/how-do-black-holes-become-supermassive/">supermassive black hole</a>?”&nbsp;



“Surprisingly, the answer appears to be a much smaller black hole! While the exact identity of NGC 5643 X-1 is not yet known, evidence points to a black hole that is about 30 times more massive than the Sun.”&nbsp;



“Locked in an orbital dance with a companion star, the black hole ensnares gas from its stellar companion, creating a superheated disc that outshines the galactic center,” said ESA.



<h2 class="wp-block-heading" id="h-star-formation-in-ngc-5643">Star formation in NGC 5643</h2>



NGC 5643 also exhibits prominent regions of <a href="https://www.earth.com/news/six-rogue-worlds-discovered-inside-a-young-star-forming-nebula/">star formation</a> within its spiral arms. These areas are rich in gas and dust - the raw materials for birthing new stars - and glow brightly in ultraviolet and infrared light.&nbsp;



Observations from the Hubble Space Telescope and the Very Large Telescope (VLT) have helped uncover the complex interplay between star formation and the galaxy's central activity.



<h2 class="wp-block-heading" id="h-extended-ionized-gas-regions-nbsp">Extended ionized gas regions&nbsp;</h2>



A defining feature of NGC 5643 is the presence of its extended ionized gas regions, which are shaped by the galaxy's AGN activity and star-forming regions.&nbsp;



These structures have been mapped through optical spectroscopy, revealing intricate patterns that help astronomers understand the physical conditions of the gas, such as density, temperature, and composition.



The galaxy also has a dust lane that crosses its nucleus, partially obscuring direct observations of the central region in visible light.&nbsp;



Overall, NGC 5643 offers a fascinating glimpse into the dynamics of barred <a href="https://www.earth.com/news/the-mesmerizing-beauty-of-spiral-galaxies/">spiral galaxies</a> with active nuclei, serving as a valuable resource for studying the interactions between supermassive black holes, star formation, and galactic evolution.



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



Lupus is a constellation located in the southern sky, its name meaning "wolf" in Latin. It has been known since antiquity and was cataloged by the Greek astronomer Ptolemy.&nbsp;



Once part of the larger constellation Centaurus, Lupus was later recognized as a distinct constellation. It is relatively faint but holds historical significance in mythology, often associated with a sacrificial wolf in ancient stories.



Lupus is bordered by other constellations like Scorpius, Centaurus, and Libra. Its stars do not form a particularly striking pattern, but it contains a variety of interesting astronomical features. Among them are numerous double stars, globular clusters, and other deep-sky objects, visible through telescopes.&nbsp;



For observers in the Southern Hemisphere, Lupus is best seen in the winter and spring months, while it appears closer to the horizon for those in northern latitudes.



This constellation also lies along the <a href="https://www.earth.com/news/stars-at-the-edge-of-our-milky-way-galaxy-travel-more-slowly/">Milky Way</a>, offering a rich field of stars and nebulae for stargazers. Despite its modest brightness, Lupus holds a special place in the science of astronomy.



Image Credit: NASA/ESA Hubble Space Telescope



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Secrets of a spiraling galactic powerhouse

Fossil footprints from the ancient Carboniferous Period have caused a stir among paleontologists worldwide. These tracks suggest reptiles roamed Earth far earlier than anyone suspected. 



Researchers uncovered <a href="https://www.earth.com/news/fossil-discovery-pushes-back-reptile-evolution-by-40-million-years/" target="_blank" rel="noreferrer noopener">reptile</a>-like footprints in northern Victoria, Australia, and matched them to the era that started around 359 million years ago.



According to Professor John Long from <a href="https://www.flinders.edu.au" target="_blank" rel="noreferrer noopener">Flinders University</a>, these imprints challenge the traditional view of reptile evolution.



<h2 class="wp-block-heading" id="h-footprints-of-reptile-ancestors">Footprints of reptile ancestors</h2>



According to the experts, the tracks suggest that these <a href="https://www.earth.com/news/why-reptiles-are-more-colorful-in-open-habitats/" target="_blank" rel="noreferrer noopener">animals</a> may have appeared roughly 350 million years ago. That date pushes them back to 40 million years earlier than what was previously recorded.



One set of partial prints had distinct claw marks, hinting that these creatures were true reptiles rather than amphibians. Another set showed a smaller front foot and a larger hind foot, which is typical of land-walking vertebrates.



<h2 class="wp-block-heading" id="h-reptile-origins-in-gondwana">Reptile origins in Gondwana</h2>



Scientists have long studied the southern supercontinent <a href="https://academic.oup.com/book/41714/chapter-abstract/353976691?redirectedFrom=fulltext" target="_blank" rel="noreferrer noopener">Gondwana</a>, where many early tetrapods left behind their skeletons and <a href="https://www.earth.com/news/reptiles-provide-new-clues-about-the-diets-of-extinct-animals/" target="_blank" rel="noreferrer noopener">tracks</a>. This find in Victoria adds weight to the idea that pivotal evolutionary steps began in these territories.



At the time, Australia formed a central piece of this landmass. Warmer climates may have played a role in encouraging new adaptations among reptile forerunners.



<h2 class="wp-block-heading" id="h-new-timeline-of-reptile-evolution">New timeline of reptile evolution</h2>



Paleontologists analyze footprints to piece together how ancient <a href="https://www.earth.com/news/largest-ever-marine-reptile-ichthyotitan-severnensis-discovered-by-11-year-old-girl/" target="_blank" rel="noreferrer noopener">animals</a> moved. A set of clawed toes can reveal whether a creature was an amphibian or a reptile.



“This pushes back the likely origin of crown-group amniotes by at least 35-40 million years,” said Professor John Long. The research highlights how vital footprints can be for revealing new timelines.



Reptiles are part of the <a href="https://ucmp.berkeley.edu/vertebrates/tetrapods/amniota.html" target="_blank" rel="noreferrer noopener">amniote</a> group, which includes birds and mammals. The discovery of claw marks in these fossil tracks implies full independence from watery environments, which is a characteristic of reptiles.



Many scientists once assumed that amniotes emerged in the Northern Hemisphere. These footprints raise questions about when and where some of the earliest reptiles spread across ancient landscapes.



<h2 class="wp-block-heading" id="h-shifting-landscapes-and-animal-diversity">Shifting landscapes and animal diversity</h2>



Researchers plan to explore other parts of Victoria for more trace fossils that could fill gaps in the record. They hope future finds will clarify how these animals became adapted for dry land.



Unearthing additional trackways may add to our understanding of how reptiles branched off from amphibians. Each new print can reveal details about posture, movement, and survival tactics.



The Carboniferous Period stretched from about 359 million to 299 million years ago. It featured vast swampy forests, giant insects, and a rise in atmospheric oxygen levels.



Land masses were arranged differently than they are today. Some scientists believe shifting coastlines created niches that spurred new adaptations.



<h2 class="wp-block-heading" id="h-habitats-of-reptile-ancestors">Habitats of reptile ancestors</h2>



Some reptile ancestors likely ventured onto stable ground while others stayed near water. Traces of this transition remain scarce, so every fossil footprint matters.



Even a single impression can show scientists how early amniotes balanced their weight or held their tails. The shape, depth, and spacing can reveal clues about speed or range of motion.



A single fossil slab from Victoria has opened up this debate about reptile origins. Researchers suggest it is significant to re-check older formations in case more reptile evidence has been overlooked.



Professor Long and his team emphasize the need for more fieldwork to confirm whether reptiles appeared across multiple regions at around the same time. They believe this discovery highlights how a single trackway can reshape our ideas about early amniotes.



<h2 class="wp-block-heading" id="h-seeking-more-reptile-footprints">Seeking more reptile footprints</h2>



Future excavations may uncover more footprints from the early stages of reptile evolution. That could bring clarity to how quickly these animals adapted to life away from water.



Technological advancements like high-resolution scans can make it easier to analyze the details of each print. Insights like these help paleontologists reconstruct entire ecosystems from a few traces left in stone.



Footprint analysis often involves laser scanning to capture 3D shapes. These scans can highlight fine ridges that point to muscle strength or toe flexibility.



Traces of skin patterns, though rare, can also indicate the texture of scales. Each layer of mud or sand holds hints about local conditions.



<h2 class="wp-block-heading" id="h-early-land-adaptation-of-reptiles">Early land adaptation of reptiles </h2>



Before amniotes, vertebrates such as fish and amphibians still needed water for reproduction. Over time, eggs with protective membranes evolved and these allowed animals such as reptiles to venture inland.



That transition set the stage for reptiles, birds, and mammals to diversify into countless forms. These footprints mark a link in that long chain.



Researchers compare new prints to known trackways from synapsids and early amphibians. Key distinctions include toe curvature and the presence of claws.



Synapsids, which later led to mammals, often left broader footprints with different digit spacing. Reptile-like tracks, on the other hand, typically show sharper claw impressions.



<h2 class="wp-block-heading" id="h-ancient-footprints-of-reptile-ancestors">Ancient footprints of reptile ancestors</h2>



These ancient footprints connect modern wildlife to ancestors that once explored muddy banks. Each imprint brings a sense of wonder about how life took shape on land.



Understanding those steps may also shed light on broader evolutionary processes. After all, reptile success paved the way for the future rise of dinosaurs and beyond.



Scientists emphasize that no single discovery stands alone. Footprints, bones, and environmental data must all be pieced together to form a coherent story.



Though incomplete, this record keeps expanding thanks to fresh finds in unexpected places. Each new track offers a glimpse into a time of rapid evolutionary change.



The study is published in the journal <a href="https://www.nature.com/articles/s41586-025-08884-5" target="_blank" rel="noreferrer noopener">Nature</a>.



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Reptile ancestors appeared 40 million years earlier than we thought

Fossil footprints from the ancient Carboniferous Period have caused a...

What makes one child genetically different from another? In a recent study, experts examined how ancestry, genetic makeup, and lifestyle choices like smoking influence the rate of new genetic mutations in children.



The team analyzed over 10,000 parent-child trios, using data from the <a href="https://www.genomicsengland.co.uk/initiatives/100000-genomes-project" target="_blank" rel="noreferrer noopener">100,000 Genomes Project</a>. The researchers aimed to uncover how new genetic <a href="https://www.earth.com/news/luca-last-universal-common-ancestor-progenitor-all-life-on-earth/" target="_blank" rel="noreferrer noopener">changes</a> - also known as de novo mutations (DNMs) - form in sperm and egg cells and pass down to offspring.



<h2 class="wp-block-heading" id="h-how-do-new-genetic-mutations-form">How do new genetic mutations form?</h2>



DNMs are not present in the DNA of either parent and are not inherited. They are fresh mutations that arise in the reproductive cells of parents (sperm and eggs) and get passed on to children. 



Sometimes, these changes have no <a href="https://www.earth.com/news/worlds-first-gene-edited-spiders-spin-red-silk/" target="_blank" rel="noreferrer noopener">impact</a>. Other times, they can lead to severe genetic disorders.



Parental age, especially the father's, plays a role in increasing DNMs. Each year that a father ages adds around 1.5 mutations to his child’s genetic makeup. 



A mother’s aging adds about 0.4 mutations. But is that all? What else could be stirring the genetic pot?



<h2 class="wp-block-heading" id="h-subtle-ancestry-differences-in-mutations">Subtle ancestry differences in mutations</h2>



To find out, the researchers scoured genetic data from 10,557 parent-child trios. They looked for genetic variants present in the child but absent in both parents. This approach allowed them to map nearly 689,000 DNMs. It’s the biggest DNM catalog ever created.



But the sheer size of the dataset wasn’t the only notable feature. The researchers explored a diverse range of ancestries, including European, African, South Asian, and American groups. This diversity helped them detect subtle differences in mutation rates linked to <a href="https://www.earth.com/news/dna-changes-supercharged-the-human-brain-but-at-a-cost/" target="_blank" rel="noreferrer noopener">ancestry</a>.



<h2 class="wp-block-heading" id="h-does-ancestry-matter">Does ancestry matter?</h2>



It turns out, ancestry does matter. African ancestry groups exhibited slightly higher DNM rates than other populations. 



On average, children of African ancestry inherited about 67 new DNMs per generation. European, South Asian, and American groups inherited about 64 DNMs.



The gap seems minor, but it is statistically significant. The researchers suggest that genetic and environmental factors tied to ancestry may be at play.



Still, age had a far more pronounced effect than ancestry. A two-year <a href="https://www.earth.com/news/gene-regulation-controlling-cells-to-improve-medical-treatments/" target="_blank" rel="noreferrer noopener">difference</a> in a father’s age at the conception of his child could offset the ancestral differences in DNM rates.



<h2 class="wp-block-heading" id="h-genetic-variants-don-t-explain-mutation">Genetic variants don’t explain mutation</h2>



Genetic variations within populations could theoretically affect DNM rates. To investigate, the researchers zoomed in on European-ancestry trios. They searched for single nucleotide polymorphisms (SNPs), which are small genetic changes that might influence mutation rates.



The experts found nothing conclusive. No common genetic variants appeared to affect DNM rates significantly.



"The sheer scale of the 100,000 Genomes Project presented a great opportunity to look into the effects and exposures that explain rates and patterns of DNA changes," said Dr. Aylwyn Scally from the <a href="https://www.cam.ac.uk" target="_blank" rel="noreferrer noopener">University of Cambridge</a>.



<h2 class="wp-block-heading" id="h-smoking-affects-genetic-mutation-rates">Smoking affects genetic mutation rates</h2>



Does smoking alter the genetic blueprint passed to children? Yes, but the effect is small. The researchers found a slight increase in DNMs among children of parents who smoked.



On average, the increase was about 2% - less than one extra DNM over a parent’s reproductive <a href="https://www.earth.com/news/most-detailed-map-of-human-genetic-mutations-unveiled/" target="_blank" rel="noreferrer noopener">life</a>.



Still, this slight increase caught the researchers’ attention. They noted that while the effect size was small, it was statistically significant. 



"While evolution has done its best to develop mechanisms to protect the DNA we pass on to our offspring, our study has shown that it's not fully protected from certain exposures," said Dr. Raheleh Rahbari from the Wellcome Sanger Institute.



<h2 class="wp-block-heading" id="h-implications-for-genetic-studies">Implications for genetic studies</h2>



The findings matter for genetic research. Current models assume that mutation rates are the same across populations. But what if they aren’t? What if ancestry subtly shapes mutation rates, as this study suggests?



Adjusting genetic models to account for ancestry and lifestyle factors could refine predictions about rare genetic disorders. It could also help scientists pinpoint mutations that are linked to diseases, leading to more accurate diagnoses.



<h2 class="wp-block-heading" id="h-reproductive-health-and-genetic-mutations">Reproductive health and genetic mutations</h2>



Germ cells - sperm and eggs - guard genetic information. Their mutation rates stay low and minimize the risk of transmitting harmful changes. But factors like age, ancestry, and smoking can still nudge those rates higher.



"Ancestry and lifestyle choices like smoking are associated with the number of new DNA changes that arise in the genome," stated Dr. Hilary Martin from the <a href="https://www.sanger.ac.uk" target="_blank" rel="noreferrer noopener">Wellcome Sanger Institute</a>.



"The effects are small, but they deepen our understanding of genetic variation."



<h2 class="wp-block-heading" id="h-further-research-is-needed">Further research is needed</h2>



Despite its scale, the study had limits. The number of participants from certain ancestry groups was relatively small. And while the researchers examined smoking, they did not explore other potential environmental factors, such as alcohol use or pollutants.



Future studies with larger, more diverse datasets could reveal additional influences on mutation rates. As genetic sequencing becomes cheaper and faster, the ability to track DNMs across generations will most certainly improve.



The study is published in the journal <a href="https://www.nature.com/articles/s41467-025-59750-x" target="_blank" rel="noreferrer noopener">Nature Communications</a>.



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What causes genetic mutations in children? New factors have been identified

What makes one child genetically different from another? In a...

A rare, bright-blue amphibian has been identified in the western Amazon. This small creature, which belongs to the poison dart frog family, stands out with unusual copper accents on its limbs and an overall eye-catching look.



Dr. Evan D. Koch, a researcher at the <a href="https://www.nm.cz/en" target="_blank" rel="noreferrer noopener">National Museum of the Czech Republic</a>, helped document the new species in an underexplored region near the Juruá River.



The team first encountered the frog in March 2023, although its official recognition as a new <a href="https://www.earth.com/news/fossil-discovery-pushes-tree-frog-origins-back-55-million-years/" target="_blank" rel="noreferrer noopener">species</a> was only documented on May 14, 2025.



<h2 class="wp-block-heading" id="h-striking-blue-poison-dart-frog">Striking blue poison dart frog</h2>



The new species of frog bears light blue stripes set against a darker upper body. Its metallic-hued legs are patterned with irregular brown spots, making the species a definite standout. 



Experts have formally named it <a href="https://journals.plos.org/plosone/article/figures?id=10.1371/journal.pone.0321748" target="_blank" rel="noreferrer noopener">Ranitomeya aetherea</a>, referencing its sky-like tones that bring to mind something almost beyond this world.



Early observations suggest it inhabits lowland Amazonian forests, roughly 443 ft (135 meters) above sea level. Individuals often perch on broad-leafed plants within these humid, palm-rich <a href="https://www.earth.com/news/world-frog-day-2025-protecting-natures-tiny-guardians/" target="_blank" rel="noreferrer noopener">habitats</a>.



<h2 class="wp-block-heading" id="h-unusual-colors-and-potential-toxicity">Unusual colors and potential toxicity</h2>



Members of the broader family, Dendrobatidae, are well known for their potent <a href="https://www.sciencedirect.com/topics/medicine-and-dentistry/neurotoxin" target="_blank" rel="noreferrer noopener">neurotoxins</a>, though each species has its own chemical profile.



Many rely on <a href="https://www.pnas.org/doi/10.1073/pnas.2133521100" target="_blank" rel="noreferrer noopener">aposematic coloration</a> to warn potential predators that making a meal of it would be a bad idea. Even though researchers have only examined a handful of R. aetherea specimens, they suspect that the frog’s bright patches hint at toxic defenses, much like in its colorful cousins.



For locals, the presence of vibrant frogs is nothing new, but the copper and pale stripes on this one are not something they typically see. Field teams were quick to note that the frog’s underside shares this light-blue tone, and is spotted with dark blotches.



<h2 class="wp-block-heading" id="h-characteristics-of-the-blue-frog">Characteristics of the blue frog</h2>



Study participants noted that these frogs stay near water-filled compartments in certain broad-leaf flora. The watery pockets, known as <a href="https://www.sciencedirect.com/topics/agricultural-and-biological-sciences/phytotelmata" target="_blank" rel="noreferrer noopener">phytotelmata</a>, cradle single R. aetherea tadpoles at various stages of development.



Each juvenile has a tinted tail and a small oval mouth. Once they reach more advanced stages, faint stripes start to appear on the tiny bodies.



According to field notes, adults seem most active in the early morning or late afternoon. Males will climb small plants, typically a few feet off the ground, to call out in a series of fast, chirping notes. 



Observers say that solitary males can gather within the same area without obvious conflict, though they appear to react strongly to call playbacks.



<h2 class="wp-block-heading" id="h-unique-vocal-patterns">Unique vocal patterns </h2>



Calling sessions last under a second and carry a quick flurry of distinct, tonal notes. That pattern sets it apart from a few other relatives whose calls have fewer notes or run at a different pitch. 



In one instance, a male produced a longer series when a female approached, suggesting there may be a special “courtship call.”



That same male was spotted leading the curious female toward a hidden leaf base with water trapped inside. This behavior offers a peek into how they might bond or share parental tasks. 



Previous <a href="https://www.journals.uchicago.edu/doi/10.1086/650727" target="_blank" rel="noreferrer noopener">studies</a> on other species in this group have documented complex childrearing steps, and the research team suspects that R. aetherea may have similar habits.



<h2 class="wp-block-heading" id="h-strict-habitat-requirements">Strict habitat requirements </h2>



Across South America, frogs of the genus Ranitomeya often occupy extremely specific habitats. It has been over ten years since a new species in this genus was named, which makes this a significant find for biologists who are keen on amphibian diversity.



Some of its relatives, like Ranitomeya imitator, feature more greens and spots, while others go for bolder oranges or reds. R. aetherea’s softly tinted copper legs represent a separate thread in the group’s evolutionary tree.



Further genetic work suggests it clusters close to other species from the southwestern Amazon, yet it holds its own distinct lineage.



Investigators suspect that these frogs may have strict habitat requirements and boundaries around their living space, which means they may potentially have very limited range sizes.



Such a focus on exact territory often makes each species vulnerable to land-use changes or deforestation.



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



Local communities were aware of various frogs in their forest, but the scientific world had no formal record of frogs with this patterning until now.



Its presence highlights that the southwestern Amazon, with patches that are still difficult to reach, can house animal groups that slip under the radar. Additional exploration may uncover other new amphibians, especially within pockets that share similar vegetation or water sources.



Researchers plan to keep monitoring these populations over the coming years. This effort is essential for tracking any environmental threats that could place these frogs at risk. 



Given the increasing human activities in this region, timely observation may help shape protective measures in the near future.



The study is published in the journal <a href="https://journals.plos.org/plosone/article?id=10.1371/journal.pone.0321748" target="_blank" rel="noreferrer noopener">PLOS ONE</a>.



Image Credit: Koch et al., 2025, PLOS One, CC-BY 4.0



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Blue frog with copper legs discovered in the Amazon rainforest

A rare, bright-blue amphibian has been identified in the western...

The central California coast hides a dimpled and pockmarked seafloor region that is roughly the size of Los Angeles - five hundred square miles of soft‑edged pits stretching from Big Sur to Morro Bay. 



For decades ocean scientists assumed these round depressions - a whopping six‑football‑field stretch from rim to rim and about 16 feet deep - were scars left by bubbles of methane burping up through the mud. 



That tidy explanation raised eyebrows once plans for an <a href="https://www.earth.com/news/offshore-wind-farms-are-now-habitats-for-sharks-and-rays/" target="_blank" rel="noreferrer noopener">offshore wind farm</a> landed on the same patch of continental slope between 1,600 and 5,200 feet below the waves. If methane were still leaking, could turbine anchors stay put?



Curiosity turned urgent when more than 5,200 of the formations, known as pockmarks, appeared to be distributed with "eerie regularity."



The pattern suggested an active force was sculpting and preserving the craters even today. 



To settle the debate, a research team rolled out a fleet of high‑tech robots and a mountain of sensors - and overturned a favorite myth about <a href="https://www.earth.com/news/only-001-percent-of-earths-deep-seafloor-has-ever-been-directly-observed/" target="_blank" rel="noreferrer noopener">how the seafloor breathes</a>.



<h2 class="wp-block-heading" id="h-seafloor-full-of-large-pockmarks">Seafloor full of large pockmarks</h2>



Autonomous underwater vehicles zipped barely yards above the bottom, beaming back sonar so sharp it mapped individual ripples of sand. 



The survey refined ship‑based maps and revealed that most pockmarks sit almost perfectly spaced apart, each nearly circular and averaging 656 feet across. 



Back at mission control aboard the research vessel, experts from the Monterey Bay Aquarium Research Institute (<a href="https://www.mbari.org/" target="_blank" rel="noreferrer noopener">MBARI</a>), the U.S. Geological Survey (<a href="https://www.usgs.gov" target="_blank" rel="noreferrer noopener">USGS</a>), and <a href="https://www.stanford.edu" target="_blank" rel="noreferrer noopener">Stanford University</a> watched the topography scroll across their monitors at one‑foot resolution.



The robots also carried a <a href="https://www2.whoi.edu/site/coastalgroup/about/how-we-work/field-methods/chirp-sub-bottom-profiler/" target="_blank" rel="noreferrer noopener">CHIRP sub‑bottom profiler</a>, a sound cannon that peeks some 25 feet beneath the mud. 



Instead of pockets of gas, profiles showed neat layers: thin bands of fine silt interrupted by coarser sand sheets. Those buried sand sheets hinted at something far more dramatic than gentle gas seepage.



<h2 class="wp-block-heading" id="h-sending-in-the-robots">Sending in the robots</h2>



Guided by the maps, MBARI’s remotely operated vehicle <a href="https://www.mbari.org/technology/rov-doc-ricketts/" target="_blank" rel="noreferrer noopener">Doc Ricketts</a> descended for 30 dives, clocking 185 hours of video and punching 107 vibracores and 433 shallow pushcores into the pockmark floors. 



An additional cruise brought up piston cores nearly 25 feet long for comparison outside the craters. Not a whiff - chemical or acoustic - of methane turned up in any sample.



“There are many unanswered questions about the seafloor and its processes,” said MBARI Senior Research Technician Eve Lundsten. 



“This research provides important <a href="https://www.earth.com/news/seafloor-relic-uncovers-earths-ancient-mysteries/" target="_blank" rel="noreferrer noopener">data about the seafloor</a> for resource managers and others considering potential offshore sites for underwater infrastructure to guide their decision‑making.”



<h2 class="wp-block-heading" id="h-seafloor-avalanches-and-pockmarks">Seafloor avalanches and pockmarks</h2>



Each core carried a timeline of turmoil. Fine mud settled quietly for millennia, then a blanket of gritty sand crashed in, marking a colossal underwater avalanche called a sediment gravity flow. 



The team counted turbidite layers back at least 280,000 years, with the most recent flow sweeping through roughly 14,000 years ago. 



When such a slurry roars downslope, it scours the center of every pockmark in its path and drops a fresh sand layer across the field in one go - resetting the craters like simultaneous footprints.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/05/pockmark-chains_seafloor-holes_distribution-map_MBARI_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/05/pockmark-chains_seafloor-holes_distribution-map_MBARI_1s.webp" alt="Location Map showing the Sur Pockmark Field outlined in green, individual pockmarks are shown as small red dots. This study focuses on the largest section of the pockmark field, from the Lucia Chica Channel down to the San Simeon Channel. Red stars show the location of AUV-collected Chirp data from beneath pockmarks in Figure 3. Inset maps contain AUV-collected bathymetry showing pockmarks in detail with 5 meter contours. Credit: MBARI" class="wp-image-1969422"/></a><figcaption class="wp-element-caption">Location Map showing the Sur Pockmark Field outlined in green, individual pockmarks are shown as small red dots. This study focuses on the largest section of the pockmark field, from the Lucia Chica Channel down to the San Simeon Channel. Red stars show the location of AUV-collected Chirp data from beneath pockmarks in Figure 3. Inset maps contain AUV-collected bathymetry showing pockmarks in detail with 5 meter contours. Click image to enlarge. Credit: MBARI</figcaption></figure>



“We collected a massive amount of data, allowing us to make a surprising link between pockmarks and sediment gravity flows," Lundsten explained.



"We were unable to determine exactly how these pockmarks were initially formed, but with MBARI's advanced underwater technology, we've gained new insight into how and why these features have persisted on the seafloor for hundreds of thousands of years."



<h2 class="wp-block-heading" id="h-clean-energy-from-seafloor-pockmarks">Clean energy from seafloor pockmarks</h2>



Undersea avalanches strike tens of thousands of years apart, yet their legacy shapes today’s renewable energy blueprint. 



<a href="https://www.earth.com/news/how-do-wind-turbines-impact-property-values-in-the-us/" target="_blank" rel="noreferrer noopener">Turbine foundations</a> must grip rock‑steady ground for decades; a bubbling gas pocket could undermine that. The new findings relieve a major worry. 



Instead of methane, the main architect here is long‑dormant sediment flow, meaning the crust has remained effectively quiet since well before humans started farming California’s Central Valley.



“Expanding renewable energy is critical to achieving the dramatic cuts in carbon dioxide emissions needed to prevent further irreversible climate change," noted MBARI President and CEO Chris Scholin.



"However, there are still many unanswered questions about the possible environmental impacts of <a href="https://www.earth.com/news/offshore-wind-farms-threaten-marine-life-hotspots/" target="_blank" rel="noreferrer noopener">offshore wind energy development</a>,” 



<h2 class="wp-block-heading" id="h-many-questions-still-need-answers">Many questions still need answers</h2>



Although the study pinned down how the craters stay fresh, their birth story remains elusive. 



Did an ancient mega‑flow carve the first depressions, or did subtle currents gradually nudge sediment aside until a small hollow invited bigger scours? 



Computer models will test whether an unconfined flow racing over the dimpled plain can muster enough force to keep those bowls tidy without help from escaping gas.



Future research will also track how water and sediment swirl through the neighboring Lucia Chica and San Simeon Channels - twin conduits that may funnel slurries into the field. 



For now, the Sur Pockmark Field stands as the best‑charted seafloor province on North America’s west coast, a natural laboratory where wind‑farm planners, geologists, and marine ecologists share common ground.



What they'll find next is anyone's guess.



The full study was published in the <a href="https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2023JF007374" target="_blank" rel="noreferrer noopener">Journal of Geophysical Research Earth Surface</a>.



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Thousands of enormous holes discovered on the seafloor, evenly-spaced with "eerie regularity"

The central California coast hides a dimpled and pockmarked seafloor...

Every seed begins life with a simple aim: to reach water, collect nutrients, and stay upright. Beneath the surface, root tips probe the soil and spread into branches that keep the plant alive.



Getting those branches to appear at just the right spot and moment matters even more now that weather swings between long dry spells and sudden cloudbursts.



Researchers have traced that timing to autophagy, the recycling pathway many people associate with health benefits from fasting.



By following a shape‑shifting protein through Arabidopsis roots, the team uncovered how brief clean‑up pulses let new branches form and <a href="https://www.earth.com/news/symbiotic-relationship-plant-roots-underground-mycorrhizal-fungi/" target="_blank" rel="noreferrer noopener">help crops cope</a> with tougher conditions.



<h2 class="wp-block-heading" id="h-plant-roots-cellular-clean-up-crew">Plant roots' cellular clean‑up crew</h2>



Scientists at the <a href="https://www.ku.dk/en" target="_blank" rel="noreferrer noopener">University of Copenhagen</a> mapped the pathway in living seedlings. They watched the transcription factor ARF7 vanish and return in predictable waves, each tied to a jump in the growth hormone auxin. 



“Fasting has become popular as it seems to have a range of health‑promoting effects in humans, as periods without food cause the body to activate clean‑up processes to dispose of various waste products in cells," explains Assistant Professor Eleazar Rodriguez from the Department of Biology, who led the study.



"We have proven that the same mechanism, which also exists in the plant kingdom, plays a vital role in the ability of <a href="https://www.earth.com/news/measuring-plant-root-health-scanning-leaves-xray-device/" target="_blank" rel="noreferrer noopener">plant roots to grow</a> and absorb water and nutrients for the rest of the plant.” 



The process relies on NBR1, a tag that guides used proteins toward a vacuole for breakdown. Each removal of ARF7 resets the signaling circuit so it can fire again a few hours later. 



When autophagy slows, ARF7 accumulates, messages run long, and the root loses its usual rhythm.



<h2 class="wp-block-heading" id="h-autophagy-and-auxin">Autophagy and auxin</h2>



Side branches normally form with steady precision. Roughly every four to six hours, auxin peaks at the root tip and switches on genes that mark a patch of tissue for future branching. 



“The <a href="https://www.earth.com/news/maize-plant-genetics-shape-root-health-and-growth/" target="_blank" rel="noreferrer noopener">movement of a root</a> is almost like watching a snake slithering forward in search of water and nourishment in the soil. And we can see that the heartbeat is strongest every time the root meanders forth,” says Rodriguez.



Using a luminescent reporter, the team confirmed that ARF7 cycles in step with those hormone pulses. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/05/autophagy_Arabidopsis-plant_ezyme-study_credit-UCopenhagen_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/05/autophagy_Arabidopsis-plant_ezyme-study_credit-UCopenhagen_1s.jpg" alt="To investigate the significance of autophagy, the researchers developed a mutant Arabidopsis (thale cress) plant in which its autophagy was disabled which is shown on the right. With an enzyme from fire flies the researchers made it possible to distinguish the normal plant from the plant with its autophagy function disabled. The plant to the right has fewer light areas and thereby fewer potential places to grow new roots with it's autophagy function turned off. Credit: Eleazar Rodriguez, Department of Biology, University of Copenhagen." class="wp-image-1969564"/></a><figcaption class="wp-element-caption">To investigate the significance of autophagy, the researchers developed a mutant Arabidopsis (thale cress) plant in which its autophagy was disabled which is shown on the right. With an enzyme from fire flies the researchers made it possible to distinguish the normal plant from the plant with its autophagy function disabled. The plant to the right has fewer light areas and thereby fewer potential places to grow new roots with it's autophagy function turned off. Click image to enlarge. Credit: Eleazar Rodriguez, Department of Biology, University of Copenhagen. </figcaption></figure>



The pattern resembles the circadian rhythms that guide leaf opening, yet it runs on its own schedule and focuses solely on building the hidden half of the plant.



<h2 class="wp-block-heading" id="h-when-autophagy-stalls">When autophagy stalls</h2>



The group then disabled key autophagy genes to <a href="https://www.earth.com/news/plants-change-their-roots-to-survive-harsh-conditions/" target="_blank" rel="noreferrer noopener">test the pathway’s limits</a>. Mutant seedlings produced fewer lateral roots and soaked up less water. 



“When we disrupted the plant's autophagy, there was waste everywhere, and we were able to detect the ARF7 protein among the waste,” says Rodriguez.



Microscopy revealed swollen vacuoles packed with debris. Growth zones that once cleared their protein stockpile before each auxin wave now stayed loaded, leaving no room for a fresh signal. The result was a sparse, inefficient root system.



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



Because the recycling toolkit is shared across flowering plants, the findings open new options for breeders and for companies developing microbial soil additives. 



Numerous methods to change the <a href="https://www.earth.com/news/tomato-plants-use-their-roots-to-ration-water-during-drought/" target="_blank" rel="noreferrer noopener">genetic characteristics of plants</a> are available today. These can be used to get plants to develop longer roots, faster, and in doing so, become more resistant to droughts or floods. 



"One of the methods enlists the help of bacteria that live in symbiosis with the plant and can cause the plant to change its growth pattern. Several companies in Denmark are working on this right now,” explains Ph.D. student Jeppe Ansbøl, who co‑authored the study.



Tuning autophagy or adjusting NBR1 tags could let roots chase moisture deeper in the soil and capture stray fertilizer before it washes away, improving harvests without extra inputs.



<h2 class="wp-block-heading" id="h-autophagy-makes-stronger-roots">Autophagy makes stronger roots</h2>



“The more roots the plants have, the more water and nutrients they can take up, so the <a href="https://www.earth.com/news/good-microbes-in-tea-roots-grow-tastier-healthier-plants/" target="_blank" rel="noreferrer noopener">plants grow better, faster</a>," Rodriquez summarized.



"We're heavily dependent on plants because they feed us, extract CO2 from the atmosphere and produce the oxygen we breathe. As such, it is extremely important to understand them fully, to which end we have just taken a big step forward."



Pilot plots in Denmark are already testing these ideas under shifting rain patterns. Early observations hint that crops with tweaked recycling bounce back more quickly after both saturation and dry spells.



<h2 class="wp-block-heading" id="h-what-next-for-crops-and-autophagy">What next for crops and autophagy?</h2>



Upcoming work will examine whether other auxin response factors move through the same recycling pathway and how changes in light, temperature, or soil chemistry adjust the schedule. 



Studies in mosses and liverworts, which split from flowering plants roughly 400 million years ago, may reveal how old the link between autophagy and development really is.



For farmers, a timely cellular tidy‑up could translate into sturdier yields. By keeping root cells clear of clutter, plants gain the freedom to build the networks they need to thrive in a climate that rarely sits still.



The full study was published in the journal <a href="https://www.embopress.org/doi/full/10.1038/s44319-024-00142-5" target="_blank" rel="noreferrer noopener">EMBO Reports</a>.



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Scientists finally learn what makes plants grow faster and stronger

Every seed begins life with a simple aim: to reach...

Time often influences how we feel physically, affecting muscle function, whether it’s waking up with a jolt or unwinding at the end of a long day. Researchers studying the body’s natural cycles have begun to link disruptions in our sleep schedules to accelerated muscle aging.



The focus is on circadian rhythms and how they affect muscle <a href="https://www.earth.com/news/ripening-tomatoes-may-hold-clues-to-delay-human-aging/" target="_blank" rel="noreferrer noopener">health</a>. This direction comes from work involving lead author Dr. Jeffrey Kelu, a research associate at <a href="https://www.kcl.ac.uk/" target="_blank" rel="noreferrer noopener">King’s College London</a>. 



Dr. Kelu's team explored the idea that internal muscle clocks might explain why irregular routines hasten the signs of getting older.



<h2 class="wp-block-heading" id="h-how-muscle-clocks-affect-aging">How muscle clocks affect aging </h2>



Circadian rhythms rely on biological “timekeepers” in different parts of the body. Scientists have long known that the brain and other organs use these clocks to regulate temperature, hormones, and digestion.



Research now suggests muscle cells run on their own schedule. When these cycles are interrupted, the aging process can ramp up, also known as <a href="https://my.clevelandclinic.org/health/diseases/23167-sarcopenia" target="_blank" rel="noreferrer noopener">sarcopenia</a>, which is the gradual decline in muscle mass.



<h2 class="wp-block-heading" id="h-muscle-aging-patterns-in-fish">Muscle aging patterns in fish</h2>



“We then monitored the fish for two years, comparing them to healthy controls. While no significant differences were seen at younger ages, fish lacking a functional muscle clock eventually showed clear signs of premature <a href="https://www.earth.com/wp-admin/post.php?post=1970116&amp;action=edit" target="_blank" rel="noreferrer noopener">aging</a>,” said Dr. Kelu. 



The team ran experiments on <a href="https://www.genome.gov/genetics-glossary/Zebrafish" target="_blank" rel="noreferrer noopener">zebrafish</a>, small aquarium fish that share many genes with humans.&nbsp;



Scientists picked zebrafish partly because their transparent features make muscle changes easier to observe. These characteristics save valuable time and resources before trying similar work in larger animals or humans.



<h2 class="wp-block-heading" id="h-observing-long-term-health-impacts">Observing long-term health impacts</h2>



Zebrafish aren’t just chosen for convenience. Their muscle structure and cellular processes are surprisingly similar to those in humans, which makes them a reliable model for studying complex <a href="https://www.earth.com/news/ai-tool-analyzes-face-age-to-predict-cancer-risk/" target="_blank" rel="noreferrer noopener">biological systems</a> like circadian rhythms and protein turnover.



Zebrafish also reproduce quickly and develop rapidly, which helps researchers observe long-term effects like aging within a much shorter period. 



Because their bodies are transparent at early stages, scientists can watch what’s happening in real time, instead of relying solely on post-mortem tissue samples.



<h2 class="wp-block-heading" id="h-sleep-patterns-and-muscle-aging">Sleep patterns and muscle aging</h2>



“In the UK, approximately four million shift workers play a vital role in keeping businesses and emergency services operational around the clock," said Dr. Kelu.



"Our study provides further evidence that the disruption of circadian rhythms in shift workers compromises multiple aspects of <a href="https://www.earth.com/news/klotho-s-kl-protein-discovered-boosts-lifespan-muscle-brain-power-with-one-dose/" target="_blank" rel="noreferrer noopener">health</a>."



Muscle decline in later years appears to be only one piece of the puzzle. Experts <a href="https://pubmed.ncbi.nlm.nih.gov/21355031/" target="_blank" rel="noreferrer noopener">note</a> that shift schedules disturb normal sleep-wake cycles and hamper body clocks for years. 



This misalignment seems to speed up the same muscle wear-and-tear that shows up with age, leaving people more at risk of mobility issues.



<h2 class="wp-block-heading" id="h-what-this-means-for-everyday-routines">What this means for everyday routines</h2>



These findings don’t just affect night-shift workers. People with irregular sleep patterns, long-haul travelers, or anyone who regularly stays up late may also experience similar disruptions to their internal clocks. 



The disruptions can add up over time, even if obvious signs do not emerge right away. This raises questions about how much recovery the body truly gets when sleep schedules constantly change. 



Sticking to a consistent bedtime and allowing for deeper rest at night may help the body carry out its normal muscle maintenance routines more effectively.



<h2 class="wp-block-heading" id="h-muscle-aging-in-men-and-women">Muscle aging in men and women</h2>



Although the study used zebrafish, similar <a href="https://genomebiology.biomedcentral.com/articles/10.1186/gb-2003-4-10-r61" target="_blank" rel="noreferrer noopener">patterns</a> have been seen in humans, especially when it comes to how muscle mass declines with age. 



Recent population data suggests that men may experience sharper drops in muscle strength over time, which lines up with what was observed in male zebrafish. 



This difference might come from how circadian rhythms interact with hormones and metabolic changes across the lifespan. 



Further research is needed to investigate whether men and women need different strategies to protect muscle health as they get older.



<h2 class="wp-block-heading" id="h-sleep-s-influence-on-muscle-aging">Sleep's influence on muscle aging</h2>



Healthy muscles go through daily cleanup. Faulty proteins gather during active periods and are cleared at night so muscles can recover.



Scientists discovered that circadian rhythms direct this cleanup. When these rhythms break, damaged proteins build up, making muscle tissue weaker over time.



New possibilities are emerging. Certain treatments that target internal clocks may help prevent the early muscle loss reported in night workers, though more trials are needed.



“This work shows how studying something as complicated as muscle growth in a simple system, like little fish larva, can really teach us something,” said Professor Simon Hughes, from King’s College London. Therapies that stabilize muscle clocks might keep cells healthier for longer.



<h2 class="wp-block-heading" id="h-future-of-muscle-aging-treatments">Future of muscle aging treatments</h2>



Early-stage research is already testing drugs that target clock-related proteins like <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC4865262/" target="_blank" rel="noreferrer noopener">Rev-erb and Ror</a>, which play a role in regulating nighttime muscle cleanup. 



If these treatments prove safe and effective, they could become part of new therapies designed to slow or prevent sarcopenia in at-risk groups.



There’s also growing interest in <a href="https://pubmed.ncbi.nlm.nih.gov/22936255/" target="_blank" rel="noreferrer noopener">chronomedicine</a>, timing treatments to match the body’s natural rhythms. For muscle health, this might mean taking medications or scheduling physical therapy at specific times of day to get the best results.



The study is published in <a href="https://www.pnas.org/doi/10.1073/pnas.2422446122" target="_blank" rel="noreferrer noopener">Proceedings of the National Academy of Sciences</a>.



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Irregular sleep may cause premature muscle aging

Time often influences how we feel physically, affecting muscle function,...

Light is often associated with life, whether through the warm glow of a campfire or the brilliance of the sun. Yet, there is another kind of light - one that is nearly imperceptible but ever-present in living organisms.



This subtle illumination, known as ultraweak photon emission (UPE), is not visible to the naked eye but is a natural byproduct of metabolic processes.



Researchers at the <a href="https://www.ucalgary.ca" target="_blank" rel="noreferrer noopener">University of Calgary</a> recently explored UPE in a study that delved into its biological significance. Unlike bioluminescence, which produces visible light, UPE emits extremely low-intensity light that falls within the spectral range of 200–1,000 nm.



This phenomenon is observed in a wide range of <a href="https://www.earth.com/news/earth-day-2025-what-were-really-fighting-for/" target="_blank" rel="noreferrer noopener">life forms</a>, from bacteria and plants to animals and humans.



<h2 class="wp-block-heading" id="h-lighting-up-in-life-and-death">Lighting up in life and death</h2>



In mice, UPE might signal vitality. The researchers compared living and recently deceased mice, capturing UPE with high-sensitivity imaging equipment. 



The living mice shone brighter, while the recently deceased emitted barely any light. Both groups were kept at the same temperature of 37°C (98.6°F), but the difference in UPE was unmistakable.



This faint light might not look like much, but it could indicate life’s internal rhythm. The study suggests that UPE isn’t just random; it might be tied to fundamental biological <a href="https://www.earth.com/news/climate-wins-in-2025-came-from-unexpected-places/" target="_blank" rel="noreferrer noopener">processes</a> that continue as long as life does.



<h2 class="wp-block-heading" id="h-plant-responses-light-as-a-signal">Plant responses: Light as a signal</h2>



Plants emit UPE too, but in them, it responds to stress. The researchers exposed plant tissues to temperature changes, injuries, and chemicals. Injured areas glowed more intensely, and the brightness increased after chemical treatments.



Why the extra light? When plants experience stress, they ramp up chemical <a href="https://www.earth.com/news/global-warming-is-accelerating-beyond-control-as-co2-levels-rise/" target="_blank" rel="noreferrer noopener">reactions</a> that produce reactive oxygen species (ROS). These molecules are like cellular alarm bells. In their rush to signal damage, they produce tiny sparks of light, visible only through advanced imaging.



<h2 class="wp-block-heading" id="h-living-cells-flash-bursts-of-light">Living cells flash bursts of light</h2>



Think of living organisms as busy chemical labs. Cells carry out countless reactions to sustain life, and some reactions generate ROS. These molecules play dual roles - they’re essential for cell signaling but can become harmful when levels spike.



During stress, ROS levels surge, and oxidative stress kicks in. This imbalance excites electrons, creating conditions for UPE. It’s not a glow in the dark - it’s a faint, silent burst of photons, unnoticed by the human eye.



<h2 class="wp-block-heading" id="h-invisible-light-from-living-cells">Invisible light from living cells</h2>



Capturing UPE requires ultradark enclosures and specialized cameras. The researchers used Electron-Multiplying Charge-Coupled Device (EMCCD) cameras for plants and Charge-Coupled Device (CCD) cameras for mice. These devices can detect UPE in controlled, dark settings, minimizing background noise.



The images revealed more than just faint glows. They showed how UPE changes with temperature, stress, and injury. In mice, the light vanished after death. In plants, chemical treatments and injuries made specific regions flare up, marking them as sites of stress or damage.



<h2 class="wp-block-heading" id="h-a-potential-diagnostic-tool">A potential diagnostic tool</h2>



What if doctors could detect stress and disease just by measuring UPE? The study hints that UPE could serve as a non-invasive diagnostic tool. 



In mice, the difference between <a href="https://www.earth.com/news/climate-extremes-in-2024-what-have-we-learned/" target="_blank" rel="noreferrer noopener">life</a> and death appeared in the intensity of UPE. In plants, stress-induced light bursts pinpointed areas of damage.



If scientists can decode UPE patterns, they might develop ways to detect diseases earlier. Monitoring UPE could reveal cellular stress before symptoms become obvious, offering a glimpse into the body’s hidden struggles.



<h2 class="wp-block-heading" id="h-light-emissions-and-life-processes">Light emissions and life processes</h2>



UPE blurs the line between physics and biology. It’s not just a quirk of cellular chemistry; it’s a signal, a pulse, a silent language of life. 



The researchers suggest that understanding UPE could open doors to new diagnostic techniques and research avenues.



But much remains unknown. Why do some stressed cells emit more light than others? How do specific injuries alter UPE patterns? And could UPE one day serve as a life indicator, a subtle sign of biological activity in tissues?



<h2 class="wp-block-heading" id="h-the-secrets-of-invisible-light">The secrets of invisible light</h2>



The study from the University of Calgary raises more questions than it answers. 



What exactly triggers UPE in stressed plants? How does cellular metabolism fuel these faint flashes of light? And could these light signals one day serve as early warning signs of disease?



For now, UPE remains a silent, invisible light - a flicker of living cells that scientists are only beginning to understand. But as researchers dig deeper, they may find that even the faintest light reveals vital clues to what it means to be living.



The study is published in <a href="https://pubs.acs.org/doi/10.1021/acs.jpclett.4c03546" target="_blank" rel="noreferrer noopener">The Journal of Physical Chemistry Letters</a>. 



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All living beings emit a subtle light that fades after death

Light is often associated with life, whether through the warm...

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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Thomas has become dedicated to protecting​ all the citizens of Carroll, New Hampshire. But he has made sure to include all residents in his efforts, including those who walk on four legs!

Protecting All Animals

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