Because David was frightened of the bear&#8217;s erratic behavior, he humanely put down the creature. He brought the bear, who still mystified him, to a local government officer who was just as puzzled. Photo Credit: brytta / Getty Images

Erratic Behavior

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Spiral galaxy glows with young stars and interstellar dust

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

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA



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Cosmic eye in the Puppis constellation

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

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Dwarf galaxy provides a window into the early universe

Today's Image of the Day from the European Space Agency features 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 the galaxy NGC 2090, located approximately 40 million light-years away in the constellation Columba.



NGC 2090 is a stunning spiral galaxy that is notable for its well-defined structure, featuring a bright central core surrounded by tightly wound spiral arms.&nbsp;



These arms are filled with young, hot stars and interstellar gas, indicating active star formation.&nbsp;



Captured by the Webb Telescope’s MIRI and NIRCam instruments, the image reveals the galaxy's winding spiral arms and the swirling gas and dust of its disc in magnificent and unique detail, noted <a href="https://www.esa.int/ESA_Multimedia/Images" target="_blank" rel="noreferrer noopener">ESA</a>. 



<h2 class="wp-block-heading" id="h-observations-of-ngc-2090">Observations of NGC 2090</h2>



The galaxy’s spiral pattern is relatively symmetrical, making it a fascinating object of study for astronomers interested in galactic evolution and dynamics.&nbsp;



Observations of NGC 2090, including those conducted by the <a href="https://www.earth.com/news/hubble-helps-solve-the-mystery-of-a-young-eruptive-star/" target="_blank" rel="noreferrer noopener">Hubble</a> Space Telescope, have provided valuable insights into the properties of its stellar populations, gas content, and the nature of its spiral structure.



“NGC 2090 was one of many galaxies studied by the NASA/ESA Hubble Space Telescope to refine the measurement of the Universe’s expansion rate, or ‘Hubble constant,’” said ESA.&nbsp;



“This can be done by observing a special type of variable stars named ‘Cepheids’ in relatively nearby galaxies.”



<h2 class="wp-block-heading" id="h-new-insights-into-ngc-2090">New insights into NGC 2090</h2>



A Cepheid-based measurement from 1998 indicated that NGC 2090 is 37 million light-years away from Earth. However, the latest measurements suggest that the galaxy is 40 million light-years away.



“Already before that Hubble project in 1998, NGC 2090 had been well studied as a very prominent nearby example of star formation,” noted ESA.&nbsp;



“Described as a ‘flocculent’ spiral, this galaxy has a patchy, dusty disc and arms that are flaky or not visible at all. We can see those patterns well in Hubble's visible-light images. However, Webb’s NIRCam near-infrared data reveal the spiral arms with remarkable clarity.”&nbsp;



<h2 class="wp-block-heading" id="h-what-are-spiral-galaxies">What are spiral galaxies?</h2>



<a href="https://www.earth.com/news/the-mesmerizing-beauty-of-spiral-galaxies/" target="_blank" rel="noreferrer noopener">Spiral galaxies</a> are among the most common and visually striking types of galaxies in the universe.&nbsp;



They are characterized by their flat, disk-like shape with a bright central bulge surrounded by sweeping spiral arms.&nbsp;



<h3 class="wp-block-heading" id="h-spiral-arms-and-central-bulge-nbsp">Spiral arms and central bulge&nbsp;</h3>



The arms of a spiral galaxy are regions where stars, gas, and dust are concentrated, often glowing brightly with the light of young, hot stars that form within them.&nbsp;



The central bulge typically contains older stars and can host a supermassive black hole at its core.&nbsp;



<h3 class="wp-block-heading" id="h-types-of-spiral-galaxies-nbsp">Types of spiral galaxies&nbsp;</h3>



Spiral galaxies are classified into different types based on how tightly their arms are wound and the size of their central bulge, ranging from tightly wound "Sa" galaxies to loosely wound "Sc" types.



<h3 class="wp-block-heading" id="h-star-formation-nbsp">Star formation&nbsp;</h3>



The structure of spiral galaxies is maintained by the interplay of gravity and angular momentum, with a rotating disk of stars and gas giving rise to their iconic shape.&nbsp;



They are active sites of <a href="https://www.earth.com/news/massive-star-redefines-our-understanding-of-stellar-evolution/" target="_blank" rel="noreferrer noopener">star formation</a> due to the abundance of gas in their arms.&nbsp;



Spiral galaxies often have a halo of older stars and globular clusters surrounding their disks, which provides clues about their formation and evolution.&nbsp;



<h3 class="wp-block-heading" id="h-barred-spiral-galaxy">Barred spiral galaxy</h3>



The <a href="https://www.earth.com/news/milky-way-galaxy-is-surrounded-by-massive-magnetic-fields/" target="_blank" rel="noreferrer noopener">Milky Way</a>, the galaxy that contains our Solar System, is a prime example of a barred spiral galaxy, a subtype where a bar-shaped structure of stars extends from the central bulge.&nbsp;



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



Columba is a small and relatively faint constellation in the southern sky, whose name means "dove" in Latin. It was introduced in the late 16th century by the Dutch astronomer Petrus Plancius and first appeared in a celestial atlas by Johann Bayer in 1603.&nbsp;



The <a href="https://www.earth.com/news/super-jupiter-discovered-in-the-great-bear-constellation/" target="_blank" rel="noreferrer noopener">constellation</a> is said to represent the dove sent out by Noah during the biblical flood, tying it to themes of hope and peace.



Columba lies near the larger constellation Canis Major and is bordered by others such as Lepus and Puppis.&nbsp;



Although it lacks particularly bright stars, its most notable star, Alpha Columbae (also called Phact), shines at a magnitude of approximately 2.6 and is a hot blue-white star. Beta Columbae, another prominent star in the constellation, is a slightly cooler, yellow-white star.



The constellation is best viewed from the Southern Hemisphere during the summer months, though it can also be seen from lower latitudes in the Northern Hemisphere.&nbsp;



Image Credit: NASA/ESA/CSA James Webb Space Telescope&nbsp;



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Webb unveils a spiral galaxy in magnificent detail

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Young stars illuminate a spiral galaxy in the constellation Pavo

Today's Image of the Day from the European Space Agency features the Columbia Glacier, a tidewater glacier located in Prince William Sound on the south coast of Alaska.



The Columba Glacier is one of the most rapidly changing <a href="https://www.earth.com/news/melting-glaciers-pose-great-threat-to-biodiversity-in-mountain-ranges/" target="_blank" rel="noreferrer noopener">glaciers</a> in the world and has been closely studied for the insights it provides into glacial mechanics and climate change impacts. 



"Since the early 1980s, the Columbia Glacier has retreated more than 20 km and lost about half of its total volume. This one glacier accounts for nearly half of the ice lost in the Chugach Mountains," noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"The changing climate is thought to have caused its retreat. Until 1980, when its rapid and constant retreat began, the glacier’s terminus was observed at the northern edge of Heather Island, which lies near the end of Columbia Bay, the inlet into which the glacier currently flows before draining into Prince William Sound."



ESA noted that this satellite image, captured in September of 2023, reveals a mostly ice-free Columbia Bay dotted with numerous icebergs and fragmented sea-ice.



<h2 class="wp-block-heading" id="h-dramatic-calving-events">Dramatic calving events</h2>



The Columbia Glacier is known for its dramatic calving events, where large chunks of ice break off from the glacier's terminus and fall into the sea, becoming icebergs.



This process has been particularly active as the glacier has retreated, contributing to hazards for shipping in Prince William Sound.



The glacier has been the focus of extensive scientific research, serving as a case study for understanding the dynamics of tidewater glaciers and their responses to <a href="https://www.earth.com/news/preparing-for-ocean-acidification-a-silent-killer-of-climate-change/" target="_blank" rel="noreferrer noopener">climate change</a>. Studies have used satellite imagery, field observations, and modeling to track its changes over time.



<h2 class="wp-block-heading" id="h-climate-impacts-on-the-columbia-glacier">Climate impacts on the Columbia Glacier</h2>



"Columbia is just one of the many glaciers suffering from the effects of climate change. Most of the glaciers around the world are losing mass," said ESA.



"However, before the advent of satellites, measuring their retreat and studying their vulnerability to climate change was difficult considering their size, remoteness and rugged terrain they occupy."



Now, noted ESA, different satellite instruments are available to gather information systematically and over large areas, providing an effective means to monitor change, keep track of all calving stages, and quantify the melting rate.



<h2 class="wp-block-heading" id="h-climate-change-and-columbia-s-retreat-nbsp">Climate change and Columbia's retreat&nbsp;</h2>



Columbia Glacier flows from the Chugach Mountains into Columbia Bay. It was once one of the largest contributors to <a href="https://www.earth.com/news/sea-level-rise-will-cost-coastal-cities-over-1-trillion-in-damages/" target="_blank" rel="noreferrer noopener">sea level rise</a> due to its significant ice loss.&nbsp;



The glacier's dynamics are influenced by its interaction with water, where the terminus meets the ocean. As the glacier flows into the sea, large chunks of ice calve off the front, leading to dramatic scenes of ice crashing into the <a href="https://www.earth.com/news/shelf-sediment-ocean-composition/" target="_blank" rel="noreferrer noopener">ocean</a>. 



This process has been intensifying due to warmer temperatures and changes in water circulation, which undermine the ice from below.



Columbia Glacier's retreat has significant implications for marine navigation and local ecosystems. The increase in icebergs calving into the bay poses hazards to ships, while the fresh meltwater impacts local water temperatures and salinity, affecting the habitat of fish and other marine life.



<h2 class="wp-block-heading" id="h-melting-glaciers-in-a-warming-climate">Melting glaciers in a warming climate </h2>



Glaciers, which are large masses of accumulated snow and ice, store about 69 percent of the world's freshwater. As the climate warms, these glaciers increasingly melt and release freshwater into nearby seas and the ocean at large.



<h3 class="wp-block-heading" id="h-influx-of-freshwater">Influx of freshwater</h3>



The influx of freshwater from <a href="https://www.earth.com/news/melting-glaciers-pose-great-threat-to-biodiversity-in-mountain-ranges/" target="_blank" rel="noreferrer noopener">melting glaciers</a> alters the salinity (salt concentration) of the ocean water. Since freshwater is less dense than saltwater, its addition can lead to stratification in which lighter, less salty water layers on top of denser, saltier water.&nbsp;



Stratification can disrupt ocean currents, which are driven in part by differences in water density and temperature. These currents are crucial for regulating global climate by distributing heat and nutrients around the planet.



<h3 class="wp-block-heading" id="h-changes-in-salinity-nbsp">Changes in salinity&nbsp;</h3>



Furthermore, changes in <a href="https://www.earth.com/news/human-induced-changes-in-ocean-salinity-threaten-biodiversity-and-marine-ecosystems/" target="_blank" rel="noreferrer noopener">salinity</a> can affect marine life, which often has narrow salinity tolerance ranges. For example, shifts in salinity can impact breeding cycles, migration patterns, and the availability of nutrients.&nbsp;



<h3 class="wp-block-heading" id="h-global-carbon-cycle">Global carbon cycle</h3>



As the ocean's composition changes, its capacity to absorb carbon dioxide from the atmosphere could also be altered, affecting the global carbon cycle and, by extension, climate change feedback mechanisms.



The melting of glaciers contributes to more pronounced changes in ocean conditions, impacting everything from global climate systems to local ecosystems in marine environments.



Image Credit: ESA&nbsp;



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Columbia Glacier on the south coast of Alaska

The MODIS instrument, short for Moderate Resolution Imaging Spectroradiometer, is a key instrument aboard the Terra and Aqua satellites. MODIS is playing a vital role in the development of Earth ecosystem models, able to predict global changes, which then assist policy makers in making informed decisions about the protection of the global environment.

Heavy snow and cloud cover in the Alps are seen in this Image of the day&nbsp;from the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look at heavy snow and low clouds in the Alps. Wildlife such as ibex live in the higher peaks to elevations of 3,400 m (11,155 ft), and plants such as Edelweiss grow in rocky areas in lower elevations as well as in higher elevations.

Heavy snow and cloud cover in the Alps

Monitoring Earth Changes with MODIS

Aqua is a NASA scientific research satellite that studies precipitation, evaporation, and water cycles. Terra and Aura make up the Earth Observing System. It's the second component of the system.

A frozen Lake Erie in February Today’s Image of the Day comes from the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look at a frozen <a href="https://www.earth.com/image/icy-lake-erie/">Lake Erie</a>, which is currently 93.3 percent iced over. A frozen Lake Erie in February
This false-color image was created using data from the Moderate Resolution Imaging Spectroradiometer (MODIS) on board the Aqua satellite to differentiate between snow, ice, and clouds.
Lake Erie /ˈɪəri/ (French: Lac Érié) is the fourth-largest lake (by surface area) of the five Great Lakes in North America, and the eleventh-largest globally if measured in terms of surface area.It is the southernmost, shallowest, and smallest by volume of the Great Lakes and therefore also has the shortest average water residence time. At its deepest point Lake Erie is 210 feet (64 metres) deep. 
Situated on the International Boundary between Canada and the United States, Lake Erie&#8217;s northern shore is the Canadian province of Ontario, specifically the Ontario Peninsula, with the U.S. states of Michigan, Ohio, Pennsylvania, and New York on its western, southern, and eastern shores. These jurisdictions divide the surface area of the lake with water boundaries. 
The lake was named by the Erie people, a Native American people who lived along its southern shore. The tribal name &#8220;erie&#8221; is a shortened form of the Iroquoian word erielhonan, meaning long tail
&#8212;
By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="https://www.earth.com/staff">Earth.com</a> Staff Writer
Image Credit: <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a>

A frozen Lake Erie in February

Aqua Earth Observing Satellite

This beautiful photo gallery contains 50 incredible images of Earth from Space. These images were taken by astronauts onboard the International Space Station, as well as by a multitude of NASA satellites orbiting the earth.

Today’s Image of the Day comes thanks to the <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=90654&amp;eocn=home&amp;eoci=iotd_readmore">NASA Earth Observatory</a> and features a look at Super Typhoon Noru in the Pacific Ocean just south of <a href="https://www.earth.com/news/first-blue-chrysanthemums-created/">Japan</a>.
This image was captured by the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua satellite on July 31, 2017. 
At the time the photo was taken, Typhoon Noru was located just 250 kilometers south of Iwo Jima. Maximum sustained winds hit 150 miles per hour.
The storm briefly became a category 5 on July 30, before being downgraded to a category 4 one day later.
&#8211;
By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="https://www.earth.com/staff">Earth.com</a> Staff Writer
Source: <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=90654&amp;eocn=home&amp;eoci=iotd_readmore">NASA Earth Observatory</a>

Super Typhoon Noru in the Pacific Ocean

Incredible Images of Earth from Space

Photos from the International Space Station are found in this awesome Earth.com image gallery. Flat-earthers won't agree, but these incredible photos of the Earth were taken by astronauts onboard the International Space Station. The International Space Station is a modular space station in low Earth orbit.

Northern Italy from the space station is seen here in this Image of the Day from the <a href="http://www.esa.int/">European Space Agency</a> (ESA). The view includes the top half of the Italian Peninsula, along with <a href="https://www.earth.com/image/wildfires-burn-northern-corsica/">Corsica</a> and Sardinia off the coast. This image was captured by ESA astronaut Paolo Nespoli on his third and final mission to the Space Station.

Northern Italy from the Space Station

Photos from the International Space Station

An enormous hydrogen-rich molecular cloud has been faintly glowing near our solar system - escaping detection until now.



This newly discovered cloud is one of the largest single structures in the sky and among the closest to Earth ever detected. 



It’s called Eos, named after the Greek goddess of dawn. And it may even hold answers to some of the biggest questions in astronomy - like how stars are born.



Eos was discovered by scientists from <a href="https://newbrunswick.rutgers.edu/" target="_blank" rel="noreferrer noopener">Rutgers University–New Brunswick</a>, and their research marks the first time a molecular cloud has been detected using far-ultraviolet light. This discovery could change how scientists search for <a href="https://www.earth.com/news/our-solar-system-once-drifted-through-orions-star-forming-region/" target="_blank" rel="noreferrer noopener">star-forming regions</a> in the universe.



<blockquote class="wp-block-quote">
“This opens up new possibilities for studying the molecular universe,” said Blakesley Burkhart, an associate professor in the Department of Physics and Astronomy at Rutgers University and a research scientist at the Center for Computational Astrophysics at the <a href="https://www.simonsfoundation.org/flatiron/" target="_blank" rel="noreferrer noopener">Flatiron Institute</a> in New York.
</blockquote>



<h2 class="wp-block-heading" id="h-spotting-hidden-hydrogen-clouds">Spotting hidden hydrogen clouds</h2>



Gas and dust form <a href="https://www.earth.com/news/fluffy-molecular-clouds-may-change-our-understanding-of-star-formation/" target="_blank" rel="noreferrer noopener">molecular clouds</a>. They contain mostly hydrogen, along with other molecules like carbon monoxide. These clouds are where stars and planets begin to form.



Until now, astronomers mainly used radio and infrared signals to detect carbon monoxide in these clouds. That’s because molecular hydrogen - though more abundant - is hard to observe directly. This discovery changed that.



<blockquote class="wp-block-quote">
“This is the first-ever molecular cloud discovered by looking for far ultraviolet emission of molecular hydrogen directly,” Burkhart enthused. 



“The data showed glowing hydrogen molecules detected via fluorescence in the far ultraviolet. This cloud is literally glowing in the dark.”
</blockquote>



<h2 class="wp-block-heading" id="h-what-makes-eos-so-special">What makes Eos so special?</h2>



Eos is a crescent-shaped gas cloud about 300 light-years from Earth. It lies near the edge of a region of space called the Local Bubble - a cavity filled with gas that surrounds our <a href="https://www.earth.com/news/study-reveals-the-delicate-balance-of-our-solar-system/" target="_blank" rel="noreferrer noopener">solar system</a>.



In size, Eos covers an area in the sky equivalent to 40 full moons. It has a mass around 3,400 times that of the sun. According to models, the cloud will evaporate in about 6 million years. Though it’s nearby, Eos poses no danger to Earth.



What it offers is a rare chance to study how molecular clouds behave in our part of the galaxy.



<blockquote class="wp-block-quote">
“When we look through our telescopes, we catch whole solar systems in the act of forming, but we don’t know in detail how that happens,” Burkhart noted.



“Our discovery of Eos is exciting because we can now directly measure how molecular clouds are forming and dissociating - and how a galaxy begins to transform interstellar gas and dust into stars and planets.”
</blockquote>



<h2 class="wp-block-heading" id="h-peering-into-the-cosmic-dawn">Peering into the cosmic dawn</h2>



The team detected Eos using an instrument called FIMS-SPEAR - a far-ultraviolet spectrograph aboard the Korean satellite STSAT-1. 



This device breaks ultraviolet light into its components, much like a prism splits visible light, letting scientists examine the details of the radiation.



When Burkhart found the data in 2023, it had just been released to the public. “It was kind of like just waiting to be explored,” she said.



The use of this technique could dramatically shift how scientists study the space between stars.



<blockquote class="wp-block-quote">
“The use of the far-ultraviolet fluorescence emission technique could rewrite our understanding of the interstellar medium, uncovering hidden clouds across the galaxy and even out to the furthest detectable limits of cosmic dawn,” said Thavisha Dharmawardena, a <a href="https://www.nasa.gov" target="_blank" rel="noreferrer noopener">NASA</a> Hubble Fellow at <a href="https://www.nyu.edu/" target="_blank" rel="noreferrer noopener">New York University</a> and a co-first author of the study.
</blockquote>



<h2 class="wp-block-heading" id="h-why-eos-was-hidden">Why Eos was hidden</h2>



Hydrogen makes up almost all of Eos, but it contains little carbon monoxide. That makes it nearly invisible to conventional detection methods.



<blockquote class="wp-block-quote">
“The story of the cosmos is a story of the rearrangement of atoms over billions of years,” Burkhart explained. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/04/eos-molecular-cloud_visible-light_new-skyline-1_credit-Rutgers_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/04/eos-molecular-cloud_visible-light_new-skyline-1_credit-Rutgers_1s.webp" alt="Artist's conception of what the Eos molecular cloud would look like in the sky if it were visible to the naked eye. Credit: NatureLifePhoto/Flickr (New York City Skyline), Burkhart et al. 2025" class="wp-image-1967888"/></a><figcaption class="wp-element-caption">Artist's conception of what the Eos molecular cloud would look like in the sky if it were visible to the naked eye. Click image to enlarge. Credit: NatureLifePhoto/Flickr (New York City Skyline), Burkhart et al. 2025</figcaption></figure>



“The hydrogen that is currently in the Eos cloud existed at the time of the <a href="https://www.earth.com/news/if-the-big-bang-theory-is-correct-what-exactly-happened/" target="_blank" rel="noreferrer noopener">Big Bang</a> and eventually fell onto our galaxy and coalesced nearby the sun. So, it’s been a long journey of 13.6 billion years for these hydrogen atoms.”
</blockquote>



For many scientists, the discovery came as a surprise. "When I was in graduate school, we were told that you can’t easily directly observe <a href="https://www.earth.com/news/seeking-the-origins-of-the-molecule-that-made-the-universe/" target="_blank" rel="noreferrer noopener">molecular hydrogen</a>,” said Dharmawardena. “It’s kind of wild that we can see this cloud in data that we didn’t think we would see.”



<h2 class="wp-block-heading" id="h-future-of-far-uv-science">Future of far-UV science</h2>



The discovery of Eos is not the end of the story - it’s just the beginning. Burkhart and her team are supporting a proposed NASA mission also named Eos. Its goal is to extend this detection method across wider regions of the galaxy.



The team is already using the James Webb Space Telescope (<a href="https://science.nasa.gov/mission/webb/" target="_blank" rel="noreferrer noopener">JWST</a>) to look for more hydrogen clouds. Early results suggest they’ve identified the most distant molecular gas ever observed.



<blockquote class="wp-block-quote">
“Using JWST, we may have found the very furthest hydrogen molecules from the sun,” Burkhart said. “So, we have found both some of the closest and farthest using far-ultraviolet emission.”
</blockquote>



Eos has revealed that some of the most important structures in the galaxy might still be hiding in plain sight - waiting for someone to look at them the right way.



The full study was published in the journal <a href="https://www.nature.com/articles/s41550-025-02541-7" target="_blank" rel="noreferrer noopener">Nature Astronomy</a>.



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Massive star-forming cloud discovered surprisingly close to Earth

An enormous hydrogen-rich molecular cloud has been faintly glowing near...

Scientists have long puzzled over a curious geological mystery in the Pacific Ocean: could one deep-sea hotspot be responsible for both a sprawling underwater volcano chain and the largest volcanic plateau on Earth? 



After years of uncertainty, a new study connects these distant features, revealing a much clearer picture of how the Pacific Ocean floor has shifted and evolved.



The research, led by geologists from the <a href="https://umd.edu/" target="_blank" rel="noreferrer noopener">University of Maryland</a> and the University of Hawaiʻi, points to the Louisville hotspot as the common source of both the Louisville Ridge - a chain of underwater volcanoes - and the vast Ontong Java Plateau.



Their findings, published in the journal Nature, are helping to rewrite the volcanic history of the Pacific Ocean.



<h2 class="wp-block-heading" id="h-volcanoes-share-hidden-origin">Volcanoes share hidden origin</h2>



“Up until now, we’ve had this extremely disconnected picture of the <a href="https://www.earth.com/news/sunken-worlds-discovered-under-the-pacific-ocean-in-earths-mantle/" target="_blank" rel="noreferrer noopener">Pacific</a> and its volcanoes,” said Val Finlayson, the study’s lead author. 



“But for the first time, we’re able to make a clear connection between the younger southern and older western Pacific <a href="https://www.earth.com/news/new-camera-helps-scientists-forecast-volcanic-eruptions/" target="_blank" rel="noreferrer noopener">volcanic systems</a>. It’s a discovery that gives us a more complete history of how the Pacific Ocean basin has evolved over millions of years to become what it is today.”



The Ontong Java Plateau, located north of the Solomon Islands, is a massive submerged volcanic platform. It’s about 120 million years old and has puzzled researchers due to its size and unclear origins.



Meanwhile, the Louisville hotspot, located in the southern Pacific Ocean, has long been known to generate a line of underwater volcanoes. Scientists had suspected the two might be linked, but no one could prove it - until now.



<h2 class="wp-block-heading" id="h-volcanic-clues-beneath-the-crust">Volcanic clues beneath the crust</h2>



Part of the difficulty in confirming the connection came from the disappearance of key evidence. Over time, portions of the Louisville hotspot track were pushed beneath the Earth’s crust through subduction, making direct study impossible.



“Much of the physical evidence for a connection between Louisville and Ontong Java has disappeared because part of the Louisville hotspot track was subducted, or pushed, under <a href="https://www.earth.com/news/the-roughness-of-tectonic-plates-may-predict-earthquake-magnitude/" target="_blank" rel="noreferrer noopener">tectonic plates</a> in the Pacific region,” Finlayson explained.



“We had to sample deeply <a href="https://www.earth.com/news/underwater-volcanic-eruptions-are-more-harmful-than-previously-believed/" target="_blank" rel="noreferrer noopener">submerged volcanoes</a> from a different long-lived hotspot track to find evidence from tens of millions of years ago that suggested our models for the Pacific plate needed revision.”



<h2 class="wp-block-heading" id="h-footprints-of-a-hidden-past">Footprints of a hidden past</h2>



The breakthrough came when the team explored <a href="https://www.earth.com/news/alien-like-marine-life-found-on-underwater-mountains-includes-100-new-species/" target="_blank" rel="noreferrer noopener">underwater mountains</a> near Samoa. They expected to find relatively young volcanic structures. Instead, the researchers uncovered mountains far older than anticipated. Using rock samples, they analyzed both the age and chemical composition of the formations.



The data told a surprising story: the mountains were part of an ancient segment of the Louisville volcanic track. These volcanoes, formed by the same hotspot, left behind what the team likened to a trail of “footprints.”



“We can track these ‘footprints’ across time and space,” Finlayson said. “The footprints get progressively older as you move away from an active hot spot, similar to how your own footprints will fade away in the sand as you walk."



"But you can still tell that these prints belong to the same source. Thanks to this new evidence, we were able to revise current models of Pacific plate motion and gain a better understanding of how the seafloor has moved over millions of years.”



<h2 class="wp-block-heading" id="h-rewriting-volcanic-history">Rewriting volcanic history</h2>



This improved understanding of Pacific plate movement doesn't just fill in a missing chapter of geological history - it could help with future studies of volcanoes across the world.



Many Pacific islands are built on volcanic foundations, and a better grasp of how those formations developed could be useful for both researchers and local communities.



The research team now plans to apply these updated models to other mysterious volcanic features, both below the ocean surface and above it.



“We’ve solved one mystery, but there are countless more waiting to be unraveled. This finding offers us a more accurate history of the Pacific and its volcanic activity and helps us understand more about the dynamics and style of volcanism that occurs there,” Finlayson said. 



“Everything new we learn about the Earth’s tumultuous past helps us better understand the dynamic planet we live on today.”



The full study was published in the journal <a href="https://dx.doi.org/10.1038/s41586-025-08889-0" target="_blank" rel="noreferrer noopener">Nature</a>.



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Hidden connection unites the largest volcanoes in the Pacific

Scientists have long puzzled over a curious geological mystery in...

When naturalists tally the frogs in a farm pond or the orchids in a mountain meadow they always encounter the same rule of thumb: when you survey a larger range, the more species you find. The relationship seems simple, yet ecologists have puzzled over an odd signature hidden in species distribution data for nearly a century.



As one zooms out from local plots to regional landscapes. the tally of new species first soars. Then, it plateaus, taking off again at continental and global scales. That curious “S-shaped” curve is technically, the three-phase species–area relationship. 



It has appeared in everything from beetles to <a href="https://www.earth.com/news/bird-wings-have-a-surprising-effect-on-island-biodiversity/" target="_blank" rel="noreferrer noopener">birds</a> and from coral reefs to desert shrubs. Until now, no single mathematical framework explained why the curve changes its slope where it does.



<h2 class="wp-block-heading" id="h-predicting-species-distributions">Predicting species distributions </h2>



A collaboration of researchers spanning Portugal, Germany, the United States and South Africa has now filled that theoretical gap. 



The experts combined basic geometry with giant <a href="https://www.earth.com/news/what-are-the-biggest-drivers-of-biodiversity-loss/" target="_blank" rel="noreferrer noopener">biodiversity</a> datasets to show that the three phases arise inevitably from the way individual species spread their geographic ranges across Earth’s surface.



The team's model not only reproduces the classic patterns, it also generates equations that predict how many species should occur at the precise break points between phases - a feat with direct relevance for conservation planners who must estimate extinctions as habitats are lost.



<h2 class="wp-block-heading" id="h-range-size-affects-species-distributions">Range size affects species distributions</h2>



Ecologists formalized the species-area relationship (SAR) in the early twentieth century, discovering that a log-log plot of cumulative species versus area usually forms a straight line. Yet when studies started to cover larger domains, investigators found the line was actually composed of three segments.



In the first segment, from local quadrants to perhaps a few hundred square kilometers, adding more land brings a flood of new species because each little patch contains slightly different microhabitats. In the middle segment, spanning thousands of square kilometers, the pace slackens; the same bird species, for instance, occupy most forests inside a biogeographic region. 



Beyond that, when continents are added, evolutionary history enters the picture and the slope shoots up again as entirely different faunas come into view. Empirically describing those bends was straightforward; explaining them from first principles proved harder. 



<h2 class="wp-block-heading" id="h-individual-ranges-of-species">Individual ranges of species</h2>



“We demonstrated that the individual geographical ranges of all species within the studied areas shape the typical species distribution patterns we observe across the globe,” said lead author Luís Borda-de-Água of <a href="https://www.cibio.up.pt/en/" target="_blank" rel="noreferrer noopener">CIBIO</a> in Portugal.



By mathematically stacking these ranges like overlapping tiles on a floor plan, the team showed that the SAR’s inflection points fall where the average range size of <a href="https://www.earth.com/news/how-do-temperature-extremes-change-the-distribution-of-species/" target="_blank" rel="noreferrer noopener">resident species</a> equals the sampling area. At small scales most ranges eclipse the plot, so each extra hectare introduces new species.



At intermediate scales the plot begins to rival range size, so fewer novelties appear. At the largest scales even the widest-ranging species occupy only one continent, restoring the steep climb.



<h2 class="wp-block-heading" id="h-testing-patterns-and-crunching-records">Testing patterns and crunching records</h2>



To test the idea the researchers turned to the <a href="https://www.gbif.org/" target="_blank" rel="noreferrer noopener">Global Biodiversity Information Facility</a>, a compendium of citizen-science sightings and museum records. They extracted roughly 700 million geo-referenced observations spanning birds, <a href="https://www.earth.com/news/over-40-of-amphibians-face-extinction-due-to-escalating-climate-threats/" target="_blank" rel="noreferrer noopener">amphibians</a>, mammals and vascular plants.



For each taxonomic group they generated empirical SARs and compared them with the theoretical predictions. The correspondence was striking: predicted transition points - where the slope of the SAR changes - matched the observed curves within confidence bounds for all groups.



Borda-de-Água noted that this is a major step forward in ecology because it links a macroecological pattern to a simple, measurable property - range size - without invoking mysterious external factors. 



Senior author Henrique Pereira is a research professor at the German Center for Integrative Biodiversity Research <a href="https://www.idiv.de/" target="_blank" rel="noreferrer noopener">(iDiv</a>) and Martin Luther University Halle-Wittenberg. 



Pereira emphasized the significance of the research. “Discovering fundamental principles in ecology is just as thrilling as breakthroughs in physics.”



<h2 class="wp-block-heading" id="h-practical-stakes-for-a-shrinking-planet"><a></a>Practical stakes for a shrinking planet</h2>



Beyond intellectual satisfaction the model carries weighty consequences for biodiversity assessments. International panels such as IPBES rely on SARs to translate lost habitat into predicted extinctions. 



If analysts know where a landscape sits on the three-phase curve they can apply the correct slope and avoid over- or under-estimating risk. The new equations provide exactly that guidance. 



Suppose a logged forest fragment still covers more area than the average range of its endemic beetles; species losses may be modest. But once destruction pushes the fragment below the first transition threshold, disappearing hectares cause a much steeper decline in species count.



Because the theory is scale-free it can also help conservationists decide whether sampling has been adequate. If observed species richness does not yet reach the slowdown phase, additional survey work is warranted before managers proclaim an inventory complete.



<h2 class="wp-block-heading" id="h-shifting-species-distributions">Shifting species distributions </h2>



The authors acknowledge that species’ ranges are not static. <a href="https://www.earth.com/news/climate-action-and-biodiversity-striking-the-right-balance/" target="_blank" rel="noreferrer noopener">Climate change</a>, invasive species, and land-use shifts continually redraw distribution maps. 



Incorporating dynamic range models into the three-phase framework will be a priority, as will extending tests to marine organisms and microbes, whose ranges are harder to delineate.



Still, the study offers a rare optimism amid grim extinction headlines. By revealing the geometry behind one of ecology’s most robust laws, scientists gain a clearer lens through which to view and perhaps mitigate humanity’s impact on life’s diversity.



As Pereira puts it, advances like these “unveil hidden patterns that have been shaping life on Earth for millions of years,” providing the knowledge base needed to steer those patterns, responsibly, into the future.



The study is published in the journal <a href="https://www.nature.com/articles/s41467-025-59239-7" target="_blank" rel="noreferrer noopener">Nature Communications</a>.



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Saving biodiversity: Scientists discover hidden pattern guiding species distributions

When naturalists tally the frogs in a farm pond or...

Nicotine pouches - small, flavored packets placed between the gum and lip - have become a fast-growing trend among teenagers. A new study shows that the use of these pouches by high school students in the U.S. nearly doubled between 2023 and 2024.



The research was conducted by scientists at the <a href="https://keck.usc.edu/" target="_blank" rel="noreferrer noopener">Keck School of Medicine of the University of Southern California</a>. The team surveyed more than 10,000 high school students across the country to understand their use of nicotine pouches and other <a href="https://www.earth.com/news/tobacco-bans-could-help-prevent-1-2-million-lung-cancer-deaths/" target="_blank" rel="noreferrer noopener">tobacco</a> products.



<h2 class="wp-block-heading" id="h-teen-nicotine-pouch-use-soars">Teen nicotine pouch use soars</h2>



The data highlights a worrying trend. In 2023, just 3% of 10th and 12th graders reported using nicotine pouches. By 2024, that number had jumped to 5.4 percent. More teens said they had used the pouches in the past month and past year, and the number who used both <a href="https://www.earth.com/news/cannabis-and-nicotine-use-during-pregnancy-linked-to-infant-mortality/" target="_blank" rel="noreferrer noopener">nicotine</a> pouches and e-cigarettes also increased during that period.



Interestingly, while pouch use went up, the number of teens who reported vaping declined slightly - from 20% in 2023 to 17.6% in 2024. 



But dual use rose, with 3.6% of teens saying they had used both products in the past year, up from 2.1% the previous year.



“This growing public health issue needs more attention," said Dae-Hee Han, PhD, the study's lead author. "Like flavored <a href="https://www.earth.com/news/e-cigarettes-linked-to-increased-risk-of-heart-failure/" target="_blank" rel="noreferrer noopener">e-cigarettes</a> when they first emerged, use of this new oral nicotine product is becoming more widespread, particularly among adolescents.” 



<h2 class="wp-block-heading" id="h-teens-most-at-risk">Teens most at risk</h2>



Some teens are more likely to use nicotine pouches than others. Boys, non-Hispanic white teens, and students in rural areas showed higher rates of use. These groups mirror the typical profile of smokeless tobacco users, like those who chew tobacco, according to the researchers.



“We’re finding that the risk profile differs quite a bit between nicotine pouches and e-cigarettes, which means we need prevention approaches that are targeted for each,” Han said.



The health risks of nicotine pouches are still unclear, but there are known concerns. Some users have reported mouth sores and gum irritation. And nicotine addiction itself is a real issue, especially for teens. 



Studies suggest that nicotine exposure during adolescence can hurt brain development and affect memory, attention, and learning.



<h2 class="wp-block-heading" id="h-influencers-and-fda-approval">Influencers and FDA approval</h2>



Part of the pouch popularity seems to be driven by social media. A wave of “Zynfluencers” - influencers promoting the Zyn brand - has helped tie pouch use to ideas of confidence, masculinity, and mental focus.



In January, the U.S. Food and Drug Administration (FDA) gave Zyn permission to market flavored pouches to adults aged 21 and older. The decision was based on the idea that these products might be less harmful than <a href="https://www.earth.com/news/does-vaping-help-people-quit-smoking-cigarettes-new-study-breaks-it-down/" target="_blank" rel="noreferrer noopener">cigarettes</a> for adults trying to quit. But unlike nicotine gum or patches, pouches are not approved as tools to stop <a href="https://www.earth.com/news/smoking-cigarettes-accelerates-aging/" target="_blank" rel="noreferrer noopener">smoking</a>.



The same university behind the teen survey also found in a separate study that fewer than 1% of adults were actually using nicotine pouches. That raises a big question: Who is really buying them? 



“Parents, teachers, and pediatricians should be aware that teen nicotine pouch use is increasing across the nation,” said senior author Adam Leventhal, PhD.



“To reverse this trend, we need to heighten public awareness about pouches and educate youth about them. Policymakers might also consider ramping up regulation of the booming pouch market - including cinnamon, fruit, and other attractive flavors - to protect youth.”



<h2 class="wp-block-heading" id="h-monitoring-nicotine-pouch-use-among-teens">Monitoring nicotine pouch use among teens</h2>



The FDA’s decision relied partly on results from a different national survey, the National Youth Tobacco Survey (NYTS). That survey did not find a statistically significant rise in monthly teen use of pouches. However, like the USC-led study, the NYTS did find a big increase in lifetime use among teens.



The FDA didn’t mention that rise in its decision, but researchers say it matters. Tracking lifetime and yearly use helps identify when teens are experimenting with substances, even if they aren’t using them often.



Monitoring pouch use again in 2025 will be key to understanding how the FDA’s authorization is affecting behavior. Future research should also track long-term use, when teens first start using pouches, how strong the nicotine is, and what health problems may follow.



Researchers say more attention is needed to see whether new policies and prevention programs are working - especially for groups at higher risk, like teens in rural areas or those using both pouches and e-cigarettes.



“Nicotine pouches are relatively new, so we need time to collect data on prevalence, policy, and prevention,” Han said.



The full study was published in the journal JAMA Network Open.



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Nicotine pouches are a dangerous new trend among teens

Nicotine pouches - small, flavored packets placed between the gum...

Researchers have identified a hidden defensive structure deep in the forests of Neamț County, Romania. They used drones equipped with <a href="https://www.usgs.gov/faqs/what-lidar-data-and-where-can-i-download-it" target="_blank" rel="noreferrer noopener">LiDAR</a> (light detection and ranging) technology to map the terrain through dense foliage, and revealed evidence of an elaborate feature from around 5,000 years ago.



This discovery might date back to the late <a href="https://www.history.com/articles/neolithic-revolution" target="_blank" rel="noreferrer noopener">Neolithic</a>, a stage of prehistory that stretched from about 8,000 B.C. to 3,000 B.C., and it shows how early societies managed to build strong barriers in tricky places. 



Experts believe the structure had protective functions during a time of social shifts that occurred before the start of the Bronze Age - which began around 3,000 B.C.



The project was supervised by archaeologist <a href="https://www.researchgate.net/profile/Vasile-Diaconu" target="_blank" rel="noreferrer noopener">Vasile Diaconu</a>, who is affiliated with the Neamț County Museum Complex. 



<h2 class="wp-block-heading" id="h-finding-hidden-structures-with-lidar">Finding hidden structures with LIDAR</h2>



<a href="https://www.earth.com/news/complex-canopies-help-forests-recover-from-disturbances/" target="_blank" rel="noreferrer noopener">LiDAR</a> has proven valuable in many archaeological projects, from spotting hidden Mayan roads in Central America to mapping temple complexes in Southeast Asia. 



Researchers depend on these laser-based surveys to penetrate thick vegetation and capture precise ground elevations.



“LiDAR coverage provides the means to detect subtle anthropogenic features beneath a dense tropical forest canopy,” stated <a href="https://www.researchgate.net/profile/Arlen-Chase" target="_blank" rel="noreferrer noopener">Arlen F. Chase</a>, from the University of Nevada, Las Vegas (<a href="https://www.unlv.edu/" target="_blank" rel="noreferrer noopener">UNLV</a>). 



This method also limits the need for extensive on-site clearing, which saves time and preserves delicate ecosystems.



<h2 class="wp-block-heading" id="h-window-into-ancient-societies">Window into ancient societies</h2>



Many historians associate the <a href="https://www.earth.com/news/new-study-sheds-light-on-neolithic-rituals-involving-human-bones/" target="_blank" rel="noreferrer noopener">late Neolithic</a> with innovations in agriculture and early social organization. Creating a fortified area in rugged terrain reflects strategic thinking that goes beyond the needs of basic survival.



Differences in pottery styles, burial practices, and settlement layouts from this era shed light on gradual transitions that laid the groundwork for the Bronze Age. 



The structure in Neamț County might have served as a hub for trade or a refuge during regional tensions.



“LiDAR scans showed that most of the fortified sites were located in high areas, which had good visibility and were reinforced by ditches and even earthen mounds in order to increase their defensive capacity,” Diaconu said. 



“Field measurements indicated that some of these ditches had impressive dimensions with lengths of several hundred meters, which required considerable human effort in the construction.”



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



Modern archaeological ventures often rely on partnerships between traditional researchers and specialists in surveying or remote sensing. 



This project succeeded because a former student - Vlad Dulgheriu - brought drone expertise to an established excavation team. 



“Thanks to current technology and using LiDAR scans I was able to obtain a faithful image of an almost 5000-year-old fortification,” said Diaconu. He believes such measures reveal structures that have stayed hidden for centuries.



This fortification is evidence of the complexity of communities that existed long before metal tools became widespread. 



In some cases, even basic wooden defenses or earthworks required sophisticated planning and labor coordination.



Uncovering these features shows the value of integrating new approaches with classic archaeological methods. It also opens more ways to protect cultural heritage sites from vandalism or climate-related threats.



<h2 class="wp-block-heading" id="h-challenges-of-lidar-and-hidden-sites">Challenges of LIDAR and hidden sites</h2>



<a href="https://www.earth.com/news/forest-space-age-satellites-can-track-canopies-and-carbon-storage/" target="_blank" rel="noreferrer noopener">Surveying thick forests</a> comes with problems like poor visibility and limited access to remote areas. LiDAR cuts through these barriers, but analyzing data demands specialized skills and advanced software.



Drone-based work can also be sensitive in regions with protected wildlife or historical landmarks, requiring special permits. Once that is sorted out, researchers can process the data to outline potential structures more accurately.



By around 3,000 B.C., societies in various parts of the world were experimenting with <a href="https://www.earth.com/news/discovery-of-ancient-cymbals-suggests-that-music-connected-arabian-cultures/" target="_blank" rel="noreferrer noopener">copper alloy tools</a> and different forms of governance. 



This shift shows how groups often adjusted their lifestyles to local challenges, such as building enclosures or reorganizing their communities.



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



Neamț County has a reputation for cultural treasures that span from medieval monasteries to centuries-old rural settlements. 



This newly revealed fortification could add another layer to local identity, highlighting how human activity shaped these forests long ago.



Any site that merges natural features with strategic design hints at the resourcefulness of its builders. Over time, local communities may explore ways to protect it while promoting thoughtful tourism.



<h2 class="wp-block-heading" id="h-preserving-ancient-knowledge">Preserving ancient knowledge</h2>



Archaeological archives are full of examples where sites were lost because people lacked the tools to identify them. In today’s world, technology can salvage fragile remnants of <a href="https://www.earth.com/news/mayan-civilization-may-have-been-shaped-by-ingenious-fisheries/" target="_blank" rel="noreferrer noopener">earlier civilizations</a> without major disruptions.



Experts also stress ethical responsibilities when revealing newly identified places with significant heritage value. Protective measures must be balanced with the public’s interest in learning about the past.



<h2 class="wp-block-heading" id="h-continued-lidar-hidden-exploration">Continued LIDAR hidden exploration</h2>



Scholars anticipate more hidden sites will emerge as scanning tools improve and costs become more manageable. 



Each uncovered location can broaden our perspective on how people thrived in challenging climates or landscapes.



Research teams may also turn to other remote sensing methods, such as thermal imaging, to complement LiDAR. That way, various layers of data can combine to form a cohesive record of vanished structures.



As technology evolves, archaeology may make connections between previously unrelated findings. This can enrich discussions about the origins of social hierarchies, trade networks, and cultural practices. 



Local institutions might explore new avenues for research and tourism that rely on scanning technologies. This approach will highlight the resilience of ancient populations.



The findings were presented at the <a href="https://www.researchgate.net/publication/385377876_Let's_make_the_invisible_visible_LiDAR_investigations_and_archaeological_data_from_fortified_sites_attributed_to_the_Bronze_Age_in_Eastern_Romania" target="_blank" rel="noreferrer noopener">Landscape Archaeology Conference</a> in Spain, 2024.



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5,000-year-old fort hidden in the jungle confirms sophistication of ancient societies

Researchers have identified a hidden defensive structure deep in the...

The tiny tardigrade is often praised for its unmatched durability. Scientists have tested these microscopic animals in punishing conditions, and some have lived to tell the tale.



Tardigrades measure just around 0.02 inches, yet appear to shrug off extreme cold, radiation, and weeks without moisture. 



Observers are now stunned to see new <a href="https://pubs.acs.org/doi/10.1021/acs.nanolett.5c00378" target="_blank" rel="noreferrer noopener">experiments</a> that place micro designs on their bodies through a specialized electron beam approach.



Ding Zhao from <a href="https://www.zju.edu.cn/english/" target="_blank" rel="noreferrer noopener">Zhejiang University</a>, along with fellow researchers, has introduced a way to etch micro tracings onto tardigrade exteriors without hindering their natural <a href="https://www.earth.com/news/water-bear-tardigrade-fossils-reveal-how-they-survived-several-mass-extinction-events/" target="_blank" rel="noreferrer noopener">behaviors</a>.



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



Tardigrades, also called water bears or moss piglets, are tiny creatures that punch way above their weight. These microscopic animals lumber around on stubby legs, often in damp environments like moss, soil, or lichen. 



Despite their cuddly nickname, they’re some of the toughest life forms on Earth. They can survive boiling heat, freezing cold, crushing pressure, radiation, and even the vacuum of space. 



When things get rough, they curl up into a dry, shriveled ball called a “tun,” hit pause on life, and wait it out - sometimes for decades.



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



The term <a href="https://monroeengineering.com/blog/what-is-microfabrication/" target="_blank" rel="noreferrer noopener">microfabrication</a> describes a set of processes for building incredibly small devices. Researchers have used these methods to create sensors, circuit boards, and other intricate <a href="https://www.earth.com/news/robots-can-now-learn-from-humans-by-watching-how-to-videos/" target="_blank" rel="noreferrer noopener">tools</a>.



Achieving compatibility with delicate organisms has remained a sticking point. Old methods risk harming living cells with toxic chemicals or destructive radiation.



<h2 class="wp-block-heading" id="h-tattooing-tardigrades-without-harm">Tattooing tardigrades without harm</h2>



The experts used an electron beam to form patterns on a tardigrade’s outer layer. Some portions of the animals withstood the process and resumed normal movement soon after.



“Through this technology, we’re not just creating micro-<a href="https://www.earth.com/news/tattoo-ink-travels-through-the-body-and-may-cause-long-term-risks/" target="_blank" rel="noreferrer noopener">tattoos</a> on tardigrades - we’re extending this capability to various living organisms, including bacteria,” explained Ding Zhao.



This statement highlights how advanced microfabrication might find uses across a wide range of living systems.



<h2 class="wp-block-heading" id="h-why-tardigrades-survive-extreme-conditions">Why tardigrades survive extreme conditions</h2>



Scientists are still uncovering the factors behind these creatures’ legendary <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC5492148/" target="_blank" rel="noreferrer noopener">toughness</a>. Research has shown that certain species can return to life after losing nearly all their water content, which is a remarkable example of endurance.



This survival strategy makes them ideal test subjects for new fabrication ideas that require harsh steps like exposure to vacuum or cold. Their bodies recover in ways that few other animals can match.



<h2 class="wp-block-heading" id="h-tiny-implants-could-help-future-medicine">Tiny implants could help future medicine</h2>



Biomedicine may benefit from micro-scale implants or sensors that merge seamlessly with living <a href="https://www.earth.com/news/tattoos-and-body-art-found-on-1200-year-old-peruvian-mummies/" target="_blank" rel="noreferrer noopener">tissues</a>. Some experts foresee devices that collect data inside the human body without major surgical steps.



“It is challenging to pattern living matter, and this advance portends a new generation of biomaterial devices and biophysical sensors that were previously only present in science fiction,” noted Gavin King, who invented the underlying ice lithography technique but was not involved in this study.



<h2 class="wp-block-heading" id="h-next-steps-for-using-micro-tattoos">Next steps for using micro-tattoos</h2>



The researchers hope to expand these methods to other resilient microorganisms. New forms of <a href="https://pubchem.ncbi.nlm.nih.gov/compound/Anisole" target="_blank" rel="noreferrer noopener">anisole</a> or related compounds might open doors to printed electronics that stick firmly on biological surfaces.



Specialized micro-sensors could someday track health markers in real time and transmit signals externally. This might transform disease monitoring and personalized care options.



<h2 class="wp-block-heading" id="h-can-micro-tattoos-harm-tardigrades">Can micro-tattoos harm tardigrades?</h2>



There are still questions about long-term impacts on each test subject’s health and lifespan. Further studies will examine whether repeated procedures cause hidden issues inside their cells.



Refinements in cooling, beam intensity, and chemical agents are likely to minimize harm. Some scientists see this as a path to safer, more precise methods that respect an organism’s integrity.



<h2 class="wp-block-heading" id="h-discovery-of-tough-tardigrades">Discovery of tough tardigrades</h2>



Tardigrades belong to a distinct group called Phylum Tardigrada. They were first documented in the late 18th century by naturalists who studied water samples.



Early observations noted their curious shape and lumbering walk, prompting the nickname water bear. Centuries later, advanced labs continue to explore new features of their biology.



<h2 class="wp-block-heading" id="h-how-micro-tattoos-could-help-robotics">How micro-tattoos could help robotics</h2>



Scientists speculate that flexible circuits could coat the surfaces of living microbes to monitor chemical changes in high-risk environments. This might lead to real-time alerts about contamination or hidden toxins.



Similar concepts might appear in robotics, where living cells combine with manufactured parts to form hybrid machines. Supporters envision a time when microbes and human-made systems work in unison without harming each other.



<h2 class="wp-block-heading" id="h-future-research-directions">Future research directions </h2>



Teams worldwide exchange notes to refine micro-scale engineering on living hosts. This collaboration crosses disciplines, tying biology, physics, and chemistry into one puzzle.



Continual improvements in electron beam control allow for finer detail with fewer side effects. Leading laboratories consider tardigrades a stepping stone to more fragile organisms.



Enthusiasts believe new micro-designs on these creatures will spark ideas for advanced drug delivery and personalized treatments. Tiny adhesives may cling to tissues and guide medication where it is needed most.



Engineers and biologists see common ground in these experiments. The combination of precise patterns and natural resilience points to methods that could redefine how we use biological surfaces in tech.



The study is published in the journal <a href="https://pubs.acs.org/doi/10.1021/acs.nanolett.5c00378" target="_blank" rel="noreferrer noopener">Nano Letters</a>.



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Scientists found a way to put tattoos on the smallest, toughest creatures on Earth

The tiny tardigrade is often praised for its unmatched durability....

The sun-baked flats of southern Peru hold a secret bigger than any signpost. From a low ridge, the landscape looks plain enough - just ocher earth and scattered stones. Yet from the air, pale etchings known as Nazca geoglyphs spread out across thirty-one miles of desert like pages in an ancient picture book.



Scholars have long marveled at these Nazca geoglyphs: animals, people, and patterns scraped into the soil roughly two thousand years ago. 



Their purpose has never been obvious, and for decades each new survey has offered more puzzles than answers.



<h2 class="wp-block-heading" id="h-nazca-geoglyphs-carved-on-desert-canvas">Nazca geoglyphs carved on desert canvas</h2>



Masato Sakai of Japan’s <a href="https://www.yamagata-u.ac.jp/en/" target="_blank" rel="noreferrer noopener">Yamagata University</a> has spent two decades walking the Nazca Pampa, a dry plateau that sits about 1,640 feet above sea level. 



The lack of rain and the region’s remoteness have sheltered the drawings from erosion and farming. 



Two main styles dominate the site. Giant “line-type” designs - think the famous hummingbird - stretch for hundreds of feet. 



Smaller “surface-type” figures appear where workers once brushed away dark stones to expose lighter sand.



Early mapping relied on planes and satellite photos. Even then, the sharpest images missed many faint or partial motifs. 



Relief-type figures, often no larger than a city bus, hug age-old footpaths and easily hide in the dusty palette.



<h2 class="wp-block-heading" id="h-ai-scans-the-peruvian-sands">AI scans the Peruvian sands</h2>



Enter a collaboration with IBM Research. Between September 2022 and February 2023, Sakai’s team fed an artificial-intelligence model examples of known glyphs, then set it loose on high-resolution photos of the entire plateau. 



In six months, the system flagged 303 new surface-type drawings - almost doubling the catalog built up since the early twentieth century. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2024/09/Nazca-lines_petroglyphs_AI-analysis_credit-Yamagata-University_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2024/09/Nazca-lines_petroglyphs_AI-analysis_credit-Yamagata-University_1s.webp" alt="Fifteen of a total of 303 newly discovered relief-type figurative geoglyphs from the AI-assisted survey. Drone images taken during the field survey that confirmed the geoglyphs as authentic. The scale bars are 5 m. Outlines have been added as a guide to the eye. Versions of the images without the outlines and archaeological interpretations of the relief can be found in SI Appendix, Fig. S1. The figurative geoglyphs depict humanoids, head, domesticated animal (camelid), killer whales, birds, feline, ceremonial scene, and human/animal interaction. Credit: Yamagata University" class="wp-image-1967878"/></a><figcaption class="wp-element-caption">Fifteen of a total of 303 newly discovered relief-type figurative geoglyphs from the AI-assisted survey. Drone images taken during the field survey that confirmed the geoglyphs as authentic. The scale bars are 5 m. Outlines have been added as a guide to the eye. Versions of the images without the outlines and archaeological interpretations of the relief can be found in SI Appendix, Fig. S1. The figurative geoglyphs depict humanoids, head, domesticated animal (camelid), killer whales, birds, feline, ceremonial scene, and human/animal interaction. Click image to enlarge. Credit: Yamagata University</figcaption></figure>



That fresh haul pushes the confirmed total to 430 pieces, 318 of which Yamagata University has logged since it began work in 2004.



Instead of boxing objects the usual way, the model treated the desert as a grid of tiny image tiles and scored each one for geoglyph likelihood. 



The researchers split every confirmed figure into smaller patches to give the algorithm extra training material, a trick that compensated for the limited dataset.



<h2 class="wp-block-heading" id="h-what-are-the-nazca-geoglyphs-telling-us">What are the Nazca geoglyphs telling us?</h2>



Many newly spotted icons cluster within 141 feet of ancient trails. They show human torsos, stylized livestock, and eerie isolated heads. 



“The human heads depict human sacrifices to the gods,” Sakai explained. The pathway setting hints that small groups used these pictures as teaching aids or spiritual prompts during routine travel.



Pottery shards nearby suggest such relief-type figures may predate the grander line drawings. Their subjects lean toward domestic life, a contrast to the wild creatures often celebrated in the larger images.



<h2 class="wp-block-heading" id="h-ritual-routes-and-roadside-lessons">Ritual routes and roadside lessons</h2>



Line-type glyphs anchor the start and finish of broader pilgrimage routes, typically lying about 112 feet from ceremonial lines scored into the ground. 



Archaeologists think processions moved along these corridors, stopping at the vast bird, monkey, or whale outlines for communal rites. 



“At that time, there was no written language. People learned about the roles of humans and animals by looking at pictures and used them as places for rituals,” he said.



That spoken insight, paired with the spatial data, supports the idea that the Nazca culture wove its belief system straight into the landscape. 



Travelers likely rehearsed myths, seasonal duties, or social roles by pacing past images tailored to each lesson.



<h2 class="wp-block-heading" id="h-behind-the-numbers">Behind the numbers</h2>



The 303 fresh finds are all surface-type, yet they vary in design and age. Roughly half depict human or animal heads, many with eyes or mouths exaggerated for emphasis. 



The rest show full figures, including camelids and felines that were vital to everyday survival. Their average length is about 20 yards. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2024/09/nazca-lines_location-map_credit-University-of-Michigan_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2024/09/nazca-lines_location-map_credit-University-of-Michigan_1s.webp" alt="Field survey confirms 303 new relief-type figurative Nazca geoglyphs. Map of 303 newly confirmed and 380 previously known (black) figurative relief-type geoglyphs. Newly confirmed geoglyphs are individually AI predicted (yellow), part of an AI-predicted geoglyph group (rose), or identified in the field survey without AI predicting that location (green). Inset: Histogram of ranked AI candidates (blue), visited AI candidates (red), new geoglyphs in AI groups (rose), individually confirmed AI geoglyphs (yellow), and extrapolated new geoglyphs (light yellow) as a function of rank. Credit: University of Michigan" class="wp-image-1967876"/></a><figcaption class="wp-element-caption">Field survey confirms 303 new relief-type figurative Nazca geoglyphs. Map of 303 newly confirmed and 380 previously known (black) figurative relief-type geoglyphs. Newly confirmed geoglyphs are individually AI predicted (yellow), part of an AI-predicted geoglyph group (rose), or identified in the field survey without AI predicting that location (green). Inset: Histogram of ranked AI candidates (blue), visited AI candidates (red), new geoglyphs in AI groups (rose), individually confirmed AI geoglyphs (yellow), and extrapolated new geoglyphs (light yellow) as a function of rank. Click image to enlarge. Credit: University of Michigan</figcaption></figure>



The AI’s accuracy jumped once researchers applied transfer learning - starting with a vision model trained on everyday photographs before fine-tuning it for desert imagery.



Such efficiency matters because the Nazca Pampa spans more than 190 square miles. Manual surveys would take years, but AI can flag probable sites in days, letting field crews focus on verification and conservation.



<h2 class="wp-block-heading" id="h-ai-and-the-future-of-archaeology">AI and the future of archaeology</h2>



The success in Peru demonstrates how machine learning can spotlight hidden heritage without disturbing the ground. 



Similar techniques already aid shipwreck hunts in the Mediterranean and temple searches in Cambodia’s jungles. As satellite coverage improves, smaller teams will parse vast regions for subtle traces of ancient life.



For the Nazca Lines, the next step is protection. Mining, unregulated tourism, and modern roads nibble at the fragile crust. 



Digital maps built from AI detections give local authorities a clearer picture of what needs fencing, signage, or rerouting. 



Sharing these maps online also invites global scholars to test fresh hypotheses about how the drawings fit with climate shifts, trade, and social change over fifteen centuries.



<h2 class="wp-block-heading" id="h-what-s-next-for-the-nazca-geoglyphs">What's next for the Nazca geoglyphs?</h2>



What began as a curiosity spotted by pilot Toribio Mejía Xesspe in 1927 now stands as proof - yes, proof - of cooperation between traditional fieldwork and cutting-edge tech. 



The Nazca people left no written chronicles, but they etched stories big enough to survive millennia of wind and sun. 



With new eyes in the sky and smarter algorithms on the ground, today’s researchers are finally starting to read those stories in full.



The full study was published in the journal <a href="https://www.pnas.org/doi/full/10.1073/pnas.2407652121" target="_blank" rel="noreferrer noopener">Proceedings of the National Academy of Sciences</a>.



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One of Earth's greatest mysteries is partially solved by Artificial Intelligence

The sun-baked flats of southern Peru hold a secret bigger...

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

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

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



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



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



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



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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

Detecting mercury contamination with the tap of a finger

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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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