Today's Image of the Day from the European Space Agency features the Eagle Nebula, also known as Messier 16, which is located about 7,000 light-years away in the constellation Serpens.



The Eagle Nebula is one of the most iconic star-forming regions in our galaxy. It’s a vast cloud of gas and dust stretching roughly 70 light-years across. 



<h2 class="wp-block-heading" id="h-pillars-of-creation-nbsp">Pillars of Creation&nbsp;</h2>



What makes it especially famous is a portion of the <a href="https://www.earth.com/news/six-rogue-worlds-discovered-inside-a-young-star-forming-nebula/">nebula</a> captured by the Hubble Space Telescope in 1995 - an area called the "Pillars of Creation."&nbsp;



Some of these towering columns of gas are several light-years tall. The towers resemble sculpted fingers reaching out into space. Inside these pillars, new <a href="https://www.earth.com/news/serpens-nebula-image-reveals-how-stars-are-born/">stars</a> are being born as gravity pulls material together into dense cores that eventually ignite nuclear fusion.



The Pillars of Creation are often cited as a poetic example of the cosmic cycle of birth and destruction - where new stars are born even as the surrounding material is slowly destroyed by radiation.



<h2 class="wp-block-heading" id="h-hubble-image-of-the-eagle-nebula-nbsp">Hubble image of the Eagle Nebula&nbsp;</h2>



“This towering structure of billowing gas and dark, obscuring dust might only be a small portion of the Eagle Nebula, but it is no less majestic in appearance for it,” said <a href="https://esahubble.org/images/heic2507a/">ESA</a>.



“The new Hubble image is part of ESA/Hubble’s 35th anniversary celebrations. The cosmic cloud shown here is made of cold hydrogen gas, like the rest of the Eagle Nebula. In such regions of space new stars are born among the collapsing clouds.”&nbsp;



The hot, energetic stars emit intense ultraviolet light and powerful stellar winds that erode and sculpt the surrounding gas. The result is the creation of fantastical structures - like the narrow pillar with a blossoming head featured in the new image.



<h2 class="wp-block-heading" id="h-light-and-shadow-in-the-eagle-nebula">Light and shadow in the Eagle Nebula</h2>



The thick material in the pillar blocks most light, appearing dark and heavy against the backdrop. However, its edges glow where light from the more distant nebula shines through.&nbsp;



The striking colors reflect the chemistry and physics at play: blues signal ionized oxygen, reds indicate glowing hydrogen, and orange shows where starlight has managed to pierce the dust.



<h2 class="wp-block-heading" id="h-a-structure-under-siege">A structure under siege</h2>



Just out of frame lie the very stars responsible for shaping this dramatic pillar. Their radiation and winds continue to batter the cloud, compressing the gas and potentially triggering the birth of even more stars within.



For now, the pillar holds firm, but this stability is temporary. Over time, the relentless energy from newly formed <a href="https://www.earth.com/news/fluffy-molecular-clouds-may-change-our-understanding-of-star-formation/">stars</a> will eventually erode the entire structure.



“While the starry pillar has withstood these forces well so far, cutting an impressive shape against the background, eventually it will be totally eroded by the multitude of new stars that form in the Eagle Nebula,” explained ESA.



<h2 class="wp-block-heading" id="h-life-cycle-of-the-milky-way">Life cycle of the Milky Way</h2>



The nebula’s location in the Sagittarius Arm - one of the Milky Way’s major spiral arms - places it in a zone bustling with similar star-forming regions. This highlights the role of the Eagle Nebula in shaping the structure and the future of our galaxy.



Studies of the Eagle Nebula have revealed that the region is rich in young, hot stars - some of which are only a few million years old. These stars are in various stages of development, providing a natural laboratory for astronomers to study stellar life cycles.&nbsp;



<h2 class="wp-block-heading" id="h-evolution-of-the-eagle-nebula-nbsp">Evolution of the Eagle Nebula&nbsp;</h2>



Within the Eagle Nebula, there is a variety of stellar processes occurring in close proximity. Some stars are still forming within dense clouds of gas, while others have already matured and begun to emit powerful ultraviolet radiation.&nbsp;



The ongoing interaction between <a href="https://www.earth.com/news/star-formation-reignited-in-the-galaxy-leo-p-after-billions-of-years/">young stars</a> and their environment drives the evolution of the nebula itself.&nbsp;



As newly formed stars heat and disperse the gas and dust around them, they trigger further waves of star formation - or in some cases, halt it altogether.&nbsp;



This feedback loop not only influences the pace of star birth in the Eagle Nebula but also contributes to the broader life cycle of matter within the <a href="https://www.earth.com/news/milky-way-collision-may-change-everything-we-know-about-our-galaxy/">Milky Way</a>, enriching the galaxy with heavier elements forged in stellar cores.



Image Credit: ESA/Hubble &amp; NASA, K. Noll



-----



Like what you read? <a href="https://www.earth.com/subscribe/">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



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



-----

Eagle Nebula: Carving light from darkness

Today's Image of the Day from the European Space Agency features the Eagle Nebula, also known as Messier 16, which is located about 7,000 light-years away in the constellation Serpens. The Eagle Nebula is one of the most iconic star-forming regions in our galaxy. It’s a vast cloud of gas and dust stretching roughly 70 light-years across.  Pillars of Creation&nbsp; What makes it especially famous is a portion of the nebula captured by the Hubble Space Telescope in 1995 - an area called the...

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



The Rosette 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-rosette-nebula">Image of the Rosette Nebula </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-rosette">Distinct appearance of Rosette</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 Rosette Nebula is often studied to understand the life cycle of stars and the complex interactions between radiation and interstellar material. 



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-rosette">Nebulae that are similar to Rosette</h2>



Compared to other famous nebulae, the Rosette 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. 



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 Rosette 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 Rosette 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 Rosette 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. 



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-rosette-nebula">History of the Rosette Nebula </h2>



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



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 Rosette 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



-----



Like what you read? <a href="https://www.earth.com/subscribe/" target="_blank" rel="noreferrer noopener">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



Check us out on <a href="https://www.earth.com/earthsnap/" target="_blank" rel="noreferrer noopener">EarthSnap</a>, a free app brought to you by <a href="https://www.linkedin.com/in/eric-ralls/" target="_blank" rel="noreferrer noopener">Eric Ralls</a> and Earth.com.



-----

Rosette Nebula: A flower blooming in deep space

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

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;



-----



Like what you read? <a href="https://www.earth.com/subscribe/" target="_blank" rel="noreferrer noopener">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



Check us out on <a href="https://www.earth.com/earthsnap/" target="_blank" rel="noreferrer noopener">EarthSnap</a>, a free app brought to you by <a href="https://www.linkedin.com/in/eric-ralls/" target="_blank" rel="noreferrer noopener">Eric Ralls</a> and Earth.com.



-----

Webb unveils a spiral galaxy in magnificent detail

Today's Image of the Day from NASA Earth Observatory features active wildfires and scorched landscapes in New Mexico, where the Trout and Buck fires continue to burn across the Gila National Forest and nearby counties.



“As extreme <a href="https://www.earth.com/news/global-drought-has-caused-crisis-levels-of-food-and-water-scarcity/">drought</a> gripped parts of New Mexico in June 2025, firefighters battled large wildland fires in the southwestern part of the state,” noted <a href="https://earthobservatory.nasa.gov/images/154454/new-mexico-battles-wildfires">NASA</a>.



“The two largest were the Buck and Trout fires, which, as of June 18, had together burned more than 80,000 acres since igniting on June 11 and 12, respectively. High winds, low humidity, and dry tinder - grass, brush, and timber - have fueled their rapid spread.”



<h2 class="wp-block-heading" id="h-fires-captured-from-space">Fires captured from space</h2>



The image was captured on June 14, 2025 by the Operational Land Imager (OLI) on Landsat 8. It is a false-color image, which shows shortwave infrared, near-infrared, and visible light.



According to NASA, this band combination makes it easier to identify unburned vegetated areas (green) and the recently burned landscape (brown).&nbsp;



“Bright orange indicates the infrared signature of actively burning fires,” noted NASA.



<h2 class="wp-block-heading" id="h-progression-of-new-mexico-s-fires">Progression of New Mexico's fires</h2>



NASA’s <a href="https://www.earth.com/news/wildfire-seasons-are-now-overlapping-worldwide/">fire monitoring</a> tools revealed that the Trout Fire expanded rapidly in the days following the Landsat satellite imagery.&nbsp;



By June 18, the blaze had reached the edge of Lake Roberts and was threatening communities along Sapillo Creek. News reports indicated that evacuation orders had been issued for around 2,000 homes in the affected zones.&nbsp;



In contrast, the Buck Fire showed less growth and was reported to be 25 percent contained as of June 18.



<h2 class="wp-block-heading" id="h-emergency-fire-declaration-in-new-mexico">Emergency fire declaration in New Mexico</h2>



“On June 17, New Mexico's governor issued an emergency declaration in response to the Trout fire, which allowed emergency responders to request additional support from federal or other entities,” said NASA.



“More than 875 firefighting personnel were responding to the fire on June 18, including hotshot crews, hand crews, dozers, helicopters, and fixed-wing aircraft, according to InciWeb.”&nbsp;



“As of that date, the blaze was zero percent contained, though no infrastructure had been reported as damaged or destroyed. Several communities downwind of the Trout fire faced hazardous air quality.”



<h2 class="wp-block-heading" id="h-extreme-drought-in-new-mexico-nbsp">Extreme drought in New Mexico&nbsp;</h2>



New Mexico is facing an exceptionally severe drought in 2025 that is ranked among the worst in recent decades.&nbsp;



According to the U.S. Drought Monitor in mid-May, roughly 84 percent of the state was experiencing moderate to exceptional drought, with southern and central New Mexico hit the hardest.



This drought has the fingerprints of a warm, dry spring. <a href="https://www.earth.com/news/human-driven-climate-change-is-to-blame-for-sharp-snowpack-declines-since-1980/">Snowpacks</a> melted early and fast across mountain basins, pushing streamflows and reservoir levels far below average.&nbsp;



For instance, the Elephant Butte Reservoir sank to just 13 percent of its capacity, while many key watersheds recorded only 25 to 50 percent of median snow water equivalent.&nbsp;



Forecasts warn that flows in southern New Mexico river systems could fall to less than 25 percent of normal through the summer



<h2 class="wp-block-heading" id="h-elevated-fire-risks-and-other-hazards-nbsp">Elevated fire risks and other hazards&nbsp;</h2>



The repercussions are widespread: from parched reservoir and stream networks to stressed agricultural and ranching sectors.&nbsp;



Farms and livestock operations now face growing water shortages, and ranchers are already being urged to ration water and reduce herd sizes.



The dry, warm conditions have also created tinderbox-like environments. This year’s drought is fueling an elevated wildfire risk with active burn restrictions and existing large fires already stressing firefighting resources.



Meteorologists warn these drought conditions are unlikely to ease before the summer monsoon arrives (typically July), so residents and local authorities are bracing for months of heightened water scarcity and <a href="https://www.earth.com/news/fast-wildfires-are-gaining-even-more-speed/">fire danger</a>.



The Hermits Peak–Calf Canyon Fire of 2022 remains New Mexico’s largest recorded wildfire. The devastating fire, which burned from April into late June 2022, scorched approximately 341,000 acres, destroyed over 900 structures, and ranked as the most destructive fire in the state's history.



Image Credit: NASA Earth Observatory&nbsp;



-----



Like what you read? <a href="https://www.earth.com/subscribe/">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



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



-----

Fires spread in New Mexico amid extreme drought

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

Today's Image of the Day from the European Space Agency features Abell S1063, a massive galaxy cluster located about 4.5 billion light-years from Earth. The galaxy cluster was captured by the Webb telescope in stunning detail.



According to <a href="https://www.esa.int/ESA_Multimedia/Images/2025/05/Webb_glimpses_the_distant_past" target="_blank" rel="noreferrer noopener">ESA</a>, the image is what’s known as a deep field - a long exposure of a single area of the sky, collecting as much light as possible to draw out the most faint and distant galaxies that don’t appear in ordinary images.&nbsp;



<h2 class="wp-block-heading" id="h-galaxies-of-the-early-universe">Galaxies of the early universe </h2>



Composed of nine separate snapshots taken at different near-infrared wavelengths over roughly 120 hours, this image represents Webb’s most detailed and deepest view of a single target so far.&nbsp;



Thanks to the gravitational lensing effect of Abell S1063, astronomers can peer deeper into the past than ever before - possibly viewing some of the universe’s very <a href="https://www.earth.com/news/ancient-galaxies-formed-from-the-earliest-elements-in-the-universe/" target="_blank" rel="noreferrer noopener">first galaxies</a>.



“The eye is first drawn, in this new NASA/ESA/CSA James Webb Space Telescope Picture of the Month, to the central mega-monster that is galaxy cluster Abell S1063. This behemoth collection of galaxies, lying 4.5 billion light-years from Earth in the constellation Grus (the Crane), dominates the scene,” noted ESA.



“Looking more closely, this dense collection of heavy galaxies is surrounded by glowing streaks of light, and these warped arcs are the true object of scientists’ interest: faint galaxies from the universe’s distant past.”



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



Galaxy clusters are the largest known gravitationally bound systems and include not just galaxies, but also vast amounts of hot, X-ray-emitting gas and <a href="https://www.earth.com/news/the-true-nature-of-dark-matter-may-be-revealed-in-a-supernova/" target="_blank" rel="noreferrer noopener">dark matter</a>.&nbsp;



The galaxies within a cluster move through this hot intracluster medium, and their interactions can lead to phenomena like galaxy mergers or the stripping of gas from galaxies.&nbsp;



Galaxy clusters are important for studying the large-scale structure of the universe, the behavior of dark matter, and the evolution of galaxies over cosmic time.



<h2 class="wp-block-heading" id="h-hundreds-of-galaxies-bound-together-nbsp">Hundreds of galaxies bound together&nbsp;</h2>



As one of the most densely populated clusters known, Abell S1063 contains hundreds of galaxies bound together by gravity.&nbsp;



Its immense mass makes it an excellent example of a gravitational lens - a cosmic phenomenon where the cluster’s gravity bends and magnifies the light from galaxies far behind it.&nbsp;



This effect allows astronomers to observe incredibly faint and distant <a href="https://www.earth.com/news/milky-way-like-galaxies-were-present-in-the-early-universe/" target="_blank" rel="noreferrer noopener">galaxies</a> that would otherwise be beyond our detection limits.



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



The cluster has been the focus of several major observational campaigns. It was prominently featured in the Hubble Space Telescope’s Frontier Fields program, which used its gravitational lensing power to study the early universe.&nbsp;



“The new imagery from Webb’s Near-Infrared Camera (NIRCam) takes this quest even further back in time,” said ESA.



“This image showcases an incredible forest of lensing arcs around Abell S1063, which reveal distorted background galaxies at a range of cosmic distances, along with a multitude of faint galaxies and previously unseen features.”



These observations are helping scientists probe the Cosmic Dawn era - the period shortly after the Big Bang.



<h2 class="wp-block-heading" id="h-exploring-the-cosmic-dawn-nbsp">Exploring the Cosmic Dawn&nbsp;</h2>



The Cosmic Dawn refers to a time in the history of the universe when the first stars and galaxies began to form and shine. This pivotal era occurred roughly between 100 million and 1 billion years after the Big Bang.&nbsp;



During the Dark Ages, the <a href="https://www.earth.com/news/fastest-feeding-black-hole-found-in-the-early-universe/" target="_blank" rel="noreferrer noopener">universe</a> had cooled enough for neutral hydrogen to form, but no luminous objects yet existed to light it up.&nbsp;



The birth of the first stars - often massive and short-lived - marked the beginning of the Cosmic Dawn. These stars emitted intense ultraviolet radiation, which gradually ionized the surrounding hydrogen gas in a process known as reionization.&nbsp;



This transformed the universe from a cold, opaque environment into one that was transparent to light, enabling the large-scale structure of the cosmos to take shape.



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



Grus is a <a href="https://www.earth.com/news/super-jupiter-discovered-in-the-great-bear-constellation/" target="_blank" rel="noreferrer noopener">constellation</a> in the southern sky, its name derived from the Latin word for "crane," a type of large, graceful bird.&nbsp;



It was introduced in the late 16th century by the Dutch navigators Pieter Dirkszoon Keyser and Frederick de Houtman, during an era of celestial charting tied to European exploration of the southern hemisphere.&nbsp;



Grus is part of a group of constellations known as the "Southern Birds," which also includes Phoenix, Tucana, and Pavo.



This constellation lies near the celestial south pole and is best seen from the Southern Hemisphere during the months of August through October.&nbsp;



Image Credit: ESA/Webb, NASA &amp; CSA, H. Atek, M. Zamani



-----



Like what you read? <a href="https://www.earth.com/subscribe/" target="_blank" rel="noreferrer noopener">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



Check us out on <a href="https://www.earth.com/earthsnap/" target="_blank" rel="noreferrer noopener">EarthSnap</a>, a free app brought to you by <a href="https://www.linkedin.com/in/eric-ralls/" target="_blank" rel="noreferrer noopener">Eric Ralls</a> and Earth.com.



-----

Hundreds of galaxies illuminate the early universe 

Today's Image of the Day from the <a href="https://www.eso.org/public/">European Southern Observatory</a> (ESO) features a stunning view of the Sculptor Galaxy, one of the brightest spiral galaxies visible from Earth.



The ultra-detailed image, which was captured using ESO’s Very Large Telescope, reveals features in the Sculptor Galaxy that have never been seen before.&nbsp;



ESO researcher Enrico Congiu led a new study on the Sculptor Galaxy that is published in the journal Astronomy &amp; Astrophysics.&nbsp;



<h2 class="wp-block-heading" id="h-a-galaxy-wide-view-of-sculptor-nbsp">A galaxy-wide view of Sculptor&nbsp;</h2>



The team observed the galaxy in thousands of wavelengths at once, collecting an immense amount of data from every point across its structure. This allowed them to build a comprehensive, galaxy-wide view of how <a href="https://www.earth.com/news/white-dwarf-stars-may-be-billions-of-years-older-than-estimated/">stars</a> live and evolve within Sculptor.



"Galaxies are incredibly complex systems that we are still struggling to understand," said Congiu.



“The Sculptor Galaxy is in a sweet spot. It is close enough that we can resolve its internal structure and study its building blocks with incredible detail, but at the same time, big enough that we can still see it as a whole system.”



<h2 class="wp-block-heading" id="h-thousands-of-distinct-colors-nbsp">Thousands of distinct colors&nbsp;</h2>



<a href="https://www.earth.com/news/oxygen-detected-in-the-most-distant-and-primitive-galaxy-ever-analyzed/">Galaxies</a> span hundreds of thousands of light-years, yet their evolution is shaped by processes unfolding on much smaller scales.&nbsp;



The fundamental components of a galaxy - stars, gas, and dust - each emit light in distinct colors. The more shades of color captured in an image, the deeper the insight into a galaxy’s internal structure.&nbsp;



Traditional images typically contain only a few colors, but the new map of the Sculptor Galaxy includes thousands.&nbsp;



This rich spectrum provides astronomers with detailed information about the galaxy’s stars, gas, and dust - from their ages and chemical makeup to how they’re moving through space.



<h2 class="wp-block-heading" id="h-mapping-the-sculptor-galaxy-nbsp">Mapping the Sculptor Galaxy&nbsp;</h2>



The research team spent more than 50 hours observing the Sculptor Galaxy using the Multi Unit Spectroscopic Explorer (MUSE) on the Very Large Telescope.&nbsp;



To capture the full view - spanning roughly 65,000 light-years - they combined over 100 separate exposures into a single, detailed mosaic.&nbsp;



According to study co-author Kathryn Kreckel from Heidelberg University, Germany, this makes the map a potent tool.&nbsp;



“We can zoom in to study individual regions where stars form at nearly the scale of individual stars, but we can also zoom out to study the galaxy as a whole,” said Kreckel.&nbsp;



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



In their initial analysis of the data, the team identified around 500 planetary <a href="https://www.earth.com/news/orion-nebula-destroys-an-oceans-worth-of-water-every-month/">nebulae</a> scattered throughout the Sculptor Galaxy.



Study co-author Fabian Scheuermann, a doctoral student at Heidelberg University, emphasized the significance of the discovery.&nbsp;



Scheuermann noted that when astronomers study galaxies outside of our own cosmic neighborhood, they normally detect fewer than 100 planetary nebulae in each one.&nbsp;



<h2 class="wp-block-heading" id="h-a-galaxy-of-extremes">A galaxy of extremes</h2>



The Sculptor Galaxy, also known as NGC 253, is located about 11.4 million light-years away in the constellation Sculptor. It’s classified as a starburst galaxy, meaning it’s undergoing an exceptionally high rate of <a href="https://www.earth.com/news/fluffy-molecular-clouds-may-change-our-understanding-of-star-formation/">star formation</a>.&nbsp;



This vigorous star-making activity is especially intense in its central regions, where dense clouds of gas and dust feed the birth of new stars.&nbsp;



The galaxy is tilted at a steep angle from our perspective, which gives it a striking, elongated appearance when viewed through telescopes.



<h2 class="wp-block-heading" id="h-notable-features-of-the-sculptor-galaxy-nbsp">Notable features of the Sculptor Galaxy&nbsp;</h2>



Discovered in 1783 by Caroline Herschel, the Sculptor Galaxy has become a popular target for both professional astronomers and amateur skywatchers due to its brightness and relative proximity.&nbsp;



It’s part of the Sculptor Group, one of the nearest groups of galaxies to our Local Group. Despite being rich in star-forming regions, much of its inner structure is veiled by thick dust lanes.&nbsp;



However, infrared and X-ray observations have helped scientists peer through the obscuring material to study the galaxy’s core, revealing a wealth of activity including supernova remnants and a possible central <a href="https://www.earth.com/news/largest-ultramassive-black-hole-ever-seen-cosmic-horseshoe-lrg-3-757/">black hole</a>.



The Sculptor Galaxy is also notable for its extended halo of stars and gas, which suggests past interactions or mergers with smaller galaxies.&nbsp;



This halo, along with its active central region, makes NGC 253 a valuable subject for understanding how galaxies evolve, form stars, and recycle gas over time. Its combination of beauty and scientific richness continues to make it a focus of galactic studies.



Image Credit: European Southern Observatory&nbsp;



-----



Like what you read? <a href="https://www.earth.com/subscribe/">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



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



-----

Thousands of colors in the Sculptor Galaxy

Today's Image of the Day from the European Southern Observatory...

Today's Image of the Day from the European Space Agency features Messier 82, a starburst galaxy located in the constellation Ursa Major. This galaxy is actively forming new stars at a rate ten times that of the Milky Way.



In a study using the <a href="https://webb.nasa.gov/" target="_blank" rel="noreferrer noopener">James Webb Space Telescope</a> (JWST), an international team of astronomers has taken an unprecedented look at Messier 82 (M82), revealing intricate details about its frenzied star formation.&nbsp;



<h2 class="wp-block-heading" id="h-the-power-of-nircam">The power of NIRCam</h2>



The study, led by Alberto Bolatto, utilized Webb’s Near-Infrared Camera (NIRCam) to penetrate the thick dust and gas covering the galaxy's core, a region critical to understanding <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>.&nbsp;



"M82 has garnered a variety of observations over the years because it can be considered as the prototypical starburst galaxy," noted Bolatto. “With Webb’s size and resolution, we can look at this star-forming galaxy and see all of this beautiful new detail.”



Webb's NIRCam has proven crucial for observing areas like M82’s center, where layers of dust typically obscure the view in other wavelengths. The camera's ability to capture infrared light allows it to reveal the galaxy's core and its dynamic processes.&nbsp;



<h2 class="wp-block-heading" id="h-messier-82-image">Messier 82 image </h2>



“This image shows the power of Webb. Every single white dot in this image is either a star or a star cluster. We can start to distinguish all of these tiny point sources, which enables us to acquire an accurate count of all the star clusters in this galaxy,” noted study co-author Rebecca Levy from the University of Arizona.



One of the NIRCam's innovative features is its mode that prevents bright sources from overwhelming the detector, which was particularly useful in studying the intensely active center of Messier 82.&nbsp;



In the image, dark brown tendrils of dust weave through the galaxy's glowing white core, interspersed with small green specks that represent concentrated areas of iron from <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernova</a> remnants. Red patches highlight regions where molecular hydrogen is illuminated by the radiation from nearby young stars.



<h2 class="wp-block-heading" id="h-insights-into-galactic-winds">Insights into galactic winds</h2>



The study also focused on understanding how <a href="https://www.earth.com/news/spin-of-a-new-black-hole-is-unlocking-galactic-mysteries/" target="_blank" rel="noreferrer noopener">galactic wind</a>, driven by the rapid rate of star formation and subsequent supernovae, influences M82’s environment. 



The NIRCam images showed clumpy streams of gas, appearing in red, which extend above and below the galaxy's plane, marking the path of this wind rushing out from the starburst's core.



A key revelation came from the NIRCam’s tracing of polycyclic aromatic hydrocarbons (PAHs), sooty chemical molecules that map out the structure of the galactic wind. 



To the surprise of researchers, the PAH emissions closely resembled the patterns of the hot, ionized gas, suggesting a more complex interaction within the wind than previously understood. 



"It was unexpected to see the PAH emission resemble ionised gas," said Bolatto. "PAHs are not supposed to live very long when exposed to such a strong radiation field, so perhaps they are being replenished all the time. It challenges our theories and shows us that further investigation is required."



<h2 class="wp-block-heading" id="h-future-observations-of-messier-82">Future observations of Messier 82</h2>



The findings from Webb are just the beginning. The team plans to further analyze Messier 82 with additional data, including spectroscopic observations, to determine the ages of the <a href="https://www.earth.com/news/galaxy-collisions-hubble-spots-a-string-of-pearls-star-cluster/" target="_blank" rel="noreferrer noopener">star clusters</a> and the duration of each star formation phase within the starburst environment.&nbsp;



These observations will also assist in a broader understanding of similar processes in early <a href="https://www.earth.com/news/ceers-2112-ancient-galaxy-looks-strikingly-similar-to-ours/" target="_blank" rel="noreferrer noopener">galaxies</a>, which were common in the young universe.



<h2 class="wp-block-heading" id="h-broader-implications-of-the-study">Broader implications of the study</h2>



Study co-author Torsten Böker of the <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">European Space Agency</a> emphasized the broader implications of these findings.&nbsp;



“With these amazing Webb images, and our upcoming spectra, we can study how exactly the strong winds and shock fronts from young stars and supernovae can remove the very gas and dust from which new stars are forming,” explained Böker.&nbsp;



“A detailed understanding of this ‘feedback’ cycle is important for theories of how the early universe evolved, because compact starbursts such as the one in M82 were very common at high redshift.”



Image Credit: ESA/Webb, NASA &amp; CSA



-----



Like what you read? <a href="https://www.earth.com/subscribe/" target="_blank" rel="noreferrer noopener">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



Check us out on <a href="https://www.earth.com/earthsnap/" target="_blank" rel="noreferrer noopener">EarthSnap</a>, a free app brought to you by <a href="https://www.linkedin.com/in/eric-ralls/" target="_blank" rel="noreferrer noopener">Eric Ralls</a> and Earth.com.



-----

Messier 82: Unlocking the mysteries of star formation

Today's Image of the Day from NASA Earth Observatory features a blanket of dust over the Tarim Basin - a vast, arid region in northwestern China. 



Mountain peaks are visible through a break in the dust. These peaks are part of Tekilik Shan, a subrange of the Kunlun Mountains.



Though not as widely known as some other mountain ranges in the area, Tekilik Shan plays a significant role in shaping local <a href="https://www.earth.com/news/extreme-weather-is-pushing-nature-toward-a-breaking-point/" target="_blank" rel="noreferrer noopener">weather</a> patterns and geography.



Its snow-covered peaks can rise above 13,000 feet, contributing to the dramatic elevation differences that define the basin’s borders.



<h2 class="wp-block-heading" id="h-dust-storms-in-the-tarim-basin-nbsp">Dust storms in the Tarim Basin&nbsp;</h2>



Spring marks the height of <a href="https://www.earth.com/news/sahara-desert-dust-storms-carry-harmful-bacteria-and-fungi-around-the-globe/" target="_blank" rel="noreferrer noopener">dust storm</a> activity in the Tarim Basin, particularly in its southern region.&nbsp;



“It’s a time of year when regional wind patterns shift in ways that cause winds and storm systems to sweep in from the northwest,” noted <a href="https://earthobservatory.nasa.gov/images/154126/a-curtain-of-dust-over-the-tarim-basin" target="_blank" rel="noreferrer noopener">NASA</a>.



“In early spring, when landscapes in this region are especially dry and have minimal vegetation, land surfaces warm rapidly under the Sun’s heat every morning, fueling convection that can help loft dust upward by the afternoon.”



<h2 class="wp-block-heading" id="h-fingerlike-dust-formations-nbsp">Fingerlike dust formations&nbsp;</h2>



Satellite images revealed dust formations with fingerlike shapes that mirrored the landscape below. These projections aligned with valleys, which channeled and directed the airborne dust.&nbsp;



Ralph Kahn is an atmospheric scientist at the Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder and scientist emeritus at NASA’s Goddard Space Flight Center.



According to Kahn, the dust may have been “self-lofting.” In this process, sunlight heats recently stirred-up surface dust, creating pockets of convection that lift it even higher into the air.



This interpretation is supported by hourly observations from Japan’s Himawari-9 geostationary satellite, which showed dust gradually rising into the Tekilik Shan throughout the day. By late afternoon, the storm had grown dense enough to obscure the mountains.&nbsp;



<h2 class="wp-block-heading" id="h-decline-in-atmospheric-dust">Decline in atmospheric dust</h2>



Long-term satellite data from MODIS suggest that <a href="https://www.earth.com/news/dust-storms-in-the-gulf-of-alaska-help-shape-the-global-climate/" target="_blank" rel="noreferrer noopener">atmospheric dust</a> levels in this region have declined by about 1.5 percent each year since the early 2000s.&nbsp;



NASA researcher Hongbin Yu attributes this trend mainly to springtime changes - such as altered wind speeds, <a href="https://www.earth.com/news/how-soil-moisture-can-predict-severe-storms/" target="_blank" rel="noreferrer noopener">soil moisture</a>, or vegetation cover - rather than shifts in other seasons.



<h2 class="wp-block-heading" id="h-rainfall-in-the-tarim-basin-nbsp">Rainfall in the Tarim Basin&nbsp;</h2>



“The <a href="https://www.britannica.com/place/Takla-Makan-Desert" target="_blank" rel="noreferrer noopener">Takla Makan Desert</a> is one of the driest, most barren expanses on Earth. Flanked by mountain ranges on three sides and parched by the resulting <a href="https://glossary.ametsoc.org/wiki/Rain_shadow" target="_blank" rel="noreferrer noopener">rain shadow</a>, parts of the Tarim Basin receive no more than 10 millimeters (0.4 inches) of rain per year,” noted NASA.



“Dust storms can lead to public health problems in populated areas downwind by transporting small particles, bacteria, and viruses that infiltrate human respiratory systems.”&nbsp;



NASA added that dust storms can also affect Earth’s climate by scattering and absorbing incoming solar radiation and changing the properties of clouds.



<h2 class="wp-block-heading" id="h-landscape-of-the-tarim-basin-nbsp">Landscape of the Tarim Basin&nbsp;</h2>



The Tarim Basin is one of the largest endorheic basins in the world, meaning that its rivers do not drain into the sea but instead flow into interior lakes or evaporate.&nbsp;



The basin is encircled by three mountain ranges: the Tien Shan to the north, the Kunlun Mountains to the south, and the Pamirs to the west. These ranges create a powerful rain shadow effect, making the region exceptionally dry.



At the heart of the Tarim Basin lies the Taklamakan Desert, one of the most extreme deserts on Earth. The desert is known for its high dunes, intense temperature swings, and minimal <a href="https://www.earth.com/news/extreme-rainfall-will-wreak-havoc-on-mountain-ranges-as-warming-climate-turns-snow-to-rain/" target="_blank" rel="noreferrer noopener">rainfall</a>.



<h2 class="wp-block-heading" id="h-history-and-geology">History and geology</h2>



Despite its harsh environment, the basin has been historically significant. It was a key section of the ancient Silk Road, with several oases such as Kashgar, Khotan, and Loulan serving as vital trading and cultural centers for centuries.



Geologically, the basin is rich in natural resources, particularly oil and natural gas, and has become a focal point for China's energy exploration and development.&nbsp;



The region’s challenging climate and remote location, however, make infrastructure development and human habitation difficult.&nbsp;



The image was captured on March 27, 2025 by the Operational Land Imager instrument on Landsat 8.



-----



Like what you read? <a href="https://www.earth.com/subscribe/" target="_blank" rel="noreferrer noopener">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



Check us out on <a href="https://www.earth.com/earthsnap/" target="_blank" rel="noreferrer noopener">EarthSnap</a>, a free app brought to you by <a href="https://www.linkedin.com/in/eric-ralls/" target="_blank" rel="noreferrer noopener">Eric Ralls</a> and Earth.com.



-----

Blanket of dust covers China’s Tarim Basin

Today's Image of the Day from the European Space Agency features Messier 78 (M78), a reflection nebula located in the constellation Orion about 1,350 light-years away from Earth.&nbsp;



This image was released as part of the initial series of observations from ESA's <a href="https://www.esa.int/Science_Exploration/Space_Science/Euclid" target="_blank" rel="noreferrer noopener">Euclid space mission</a>.&nbsp;



All data collected during these early observations, including a series of incredible <a href="https://www.esa.int/Science_Exploration/Space_Science/Euclid/Euclid_s_first_images_the_dazzling_edge_of_darkness" target="_blank" rel="noreferrer noopener">new views</a> of the nearby universe, is available to the public.&nbsp;



<h2 class="wp-block-heading" id="h-image-of-messier-78">Image of Messier 78</h2>



Messier 78 is a dynamic region of star formation that is obscured by cosmic dust in this high-resolution image captured by the Euclid space telescope.



This specific view highlights how young stars generate winds of charged particles, carving out “cavities” in the molecular clouds around them.&nbsp;



The blue hues in the image represent ionized atomic hydrogen, which is a primary component of the cloud, while the red indicates the absorption and scattering of light by dust particles.



The image captures hundreds of stars varying in brightness, illuminating their nebulous, purple surroundings. A dark, arch-like structure stretches from the upper left to the bottom right of the frame, merging into the densest, darkest clouds at the image’s base.



<h2 class="wp-block-heading" id="h-active-site-of-star-formation-nbsp">Active site of star formation&nbsp;</h2>



Messier 78 is not just a single nebula but part of a larger complex of stars and nebulous regions in <a href="https://www.earth.com/news/orion-nebula-destroys-an-oceans-worth-of-water-every-month/" target="_blank" rel="noreferrer noopener">Orion</a>, which includes various other objects like dark nebulae that are visible as patches blocking light from behind.



This region is an active site of star formation, featuring many young stars and protostars, which are stars in the early stages of formation.&nbsp;



<h2 class="wp-block-heading" id="h-viewing-messier-78">Viewing Messier 78</h2>



M78 is easily observable with small telescopes, and it appears as a hazy patch of light with two prominent stars near its center, which illuminate the surrounding dust.&nbsp;



The nebula is also a favorite among amateur astronomers for its beauty and relatively bright appearance.



<h2 class="wp-block-heading" id="h-subject-of-scientific-interest-nbsp">Subject of scientific interest&nbsp;</h2>



Messier 78 is fascinating not only for its visual beauty but also for its scientific interest, particularly in the study of <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> and interstellar matter.&nbsp;



The nebula consists of dense, cold gas and dust, which are essential ingredients for the birth of new stars.&nbsp;



The intense blue light that characterizes M78 is due to the reflection of starlight off these dust particles - a process known as scattering.



<h2 class="wp-block-heading" id="h-region-surrounding-messier-78-nbsp">Region surrounding Messier 78&nbsp;</h2>



The region surrounding M78 includes several other interesting features. For instance, there are Herbig-Haro objects within it, which are small patches of nebulosity associated with <a href="https://www.earth.com/news/new-molecule-detected-in-space-where-stars-are-born/" target="_blank" rel="noreferrer noopener">newly born stars</a>.&nbsp;



These objects are formed when gas ejected by young stars collides with clouds of gas and dust at high speeds, creating shock waves that glow brightly.



<h2 class="wp-block-heading" id="h-earliest-stages-of-star-development-nbsp">Earliest stages of star development&nbsp;</h2>



Additionally, infrared observations of M78 have revealed much about the dust and colder objects in the area, which are not visible in optical light.&nbsp;



The observations have helped astronomers identify numerous young stars and brown dwarfs (objects that are too large to be planets and too small to be stars) within the nebula.&nbsp;



This makes M78 a critical area for studying the earliest stages of star development and the properties of the interstellar medium.



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



The <a href="https://www.earth.com/news/new-batch-of-brilliant-images-from-the-euclid-mission-live-up-to-the-hype/" target="_blank" rel="noreferrer noopener">Euclid space mission</a> is designed to study the dark universe, particularly focusing on dark energy and dark matter. These components are believed to drive the accelerating expansion of the universe and shape its large-scale structure. 



The mission aims to map the geometry of the dark universe and better understand the physics of the cosmos.



<h3 class="wp-block-heading" id="h-observing-billions-of-galaxies-nbsp">Observing billions of galaxies&nbsp;</h3>



Euclid uses two primary scientific instruments: a visible light camera (VIS) and a near-infrared spectrometer and photometer (NISP).&nbsp;



These instruments will allow Euclid to measure the shapes and redshifts of galaxies at distances of up to 10 billion light-years. By surveying more than a third of the sky, the mission is expected to observe several billion galaxies.



<h3 class="wp-block-heading" id="h-studying-the-dark-universe-nbsp">Studying the dark universe&nbsp;</h3>



The data collected will help astronomers in studying the effects of dark matter and dark energy in depth, testing cosmological models, and exploring new theories about the nature of the universe.&nbsp;



The mission, named after the ancient Greek mathematician Euclid, seeks to address key questions related to the structure of the universe and the fundamental laws of physics governing its evolution and expansion.



Image Credit: European Space Agency&nbsp;



-----



Like what you read? <a href="https://www.earth.com/subscribe/" target="_blank" rel="noreferrer noopener">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



Check us out on <a href="https://www.earth.com/earthsnap/" target="_blank" rel="noreferrer noopener">EarthSnap</a>, a free app brought to you by <a href="https://www.linkedin.com/in/eric-ralls/" target="_blank" rel="noreferrer noopener">Eric Ralls</a> and Earth.com.



-----

Young stars shine through dense dust

Today's Image of the Day from the European Space Agency features the star-forming region NGC 604. The nebula is located 2.73 million light-years away from Earth in the Triangulum Galaxy (M33). 



By studying regions like NGC 604, astronomers can gain insights into the complex interactions between stars and the interstellar medium, as well as the conditions that lead to the birth of stars. This, in turn, helps in understanding the evolution of <a href="https://www.earth.com/news/galaxies-like-our-own-milky-way-are-not-unique/" target="_blank" rel="noreferrer noopener">galaxies</a> and the universe as a whole.



<h2 class="wp-block-heading" id="h-massive-stars-of-ngc-604">Massive stars of NGC 604</h2>



"Sheltered among NGC 604’s dusty envelopes of gas are more than 200 of the hottest, most massive kinds of stars, all in the early stages of their lives," said <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"These types of stars are known as B-types and O-types, the latter of which can be more than 100 times the mass of our own Sun. It’s quite rare to find this concentration of them in the nearby universe. In fact, there’s no similar region within our own Milky Way galaxy."



According to ESA, this concentration of massive stars, combined with its relatively close distance, means that NGC 604 gives astronomers an opportunity to study these objects at a fascinating time early in their life.



<h2 class="wp-block-heading" id="h-gigantic-region-of-ionized-hydrogen">Gigantic region of ionized hydrogen</h2>



NGC 604 is one of the largest known regions of ionized hydrogen, also known as an H II region. This nebula is significantly larger than the Orion Nebula, which is one of the most well-known H II regions in our own <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 galaxy</a>.&nbsp;



NGC 604 spans about 1,500 light-years across, making it one of the largest H II regions in the Local Group of galaxies. This group includes the Milky Way, the Andromeda Galaxy, and about 54 other smaller galaxies.&nbsp;



<h2 class="wp-block-heading" id="h-ngc-604-starburst-phenomenon">NGC 604 starburst phenomenon </h2>



Within NGC 604, there are hundreds of young, hot, massive <a href="https://www.earth.com/news/stars-at-the-edge-of-our-milky-way-galaxy-travel-more-slowly/" target="_blank" rel="noreferrer noopener">stars</a>. These stars have ionized the surrounding gas, causing it to glow and creating the nebula. The region is a prime example of a starburst phenomenon, where stars form at a much higher rate than in typical galactic conditions.



“The bright orange streaks in this image signify the presence of carbon-based molecules known as polycyclic aromatic hydrocarbons, or PAHs," explained ESA.



"As you travel further from the immediate cavities of dust where the star is forming, the deeper red signifies molecular hydrogen. This cooler gas is a prime environment for star formation. Ionized hydrogen from ultraviolet radiation appears as a white and blue ghostly glow."



<h2 class="wp-block-heading" id="h-more-about-star-formation">More about star formation </h2>



Star formation is crucial for the evolution of galaxies and the synthesis of heavy elements. In the cores of stars, elements heavier than helium are created.



The elements are spread throughout the <a href="https://www.earth.com/news/ancient-stars-shakti-shiva-shaped-milky-way-galaxy/" target="_blank" rel="noreferrer noopener">galaxy</a> when stars reach the end of their lives and expel their material - either gently through winds or violently via supernova explosions. 



This enriching process allows for the formation of new stars and planets, and ultimately, the potential for life.



<h3 class="wp-block-heading">Cloud collapse</h3>



The process begins when part of a molecular cloud becomes unstable and starts to collapse under its own gravity. This can be triggered by events like shock waves from nearby <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernovae</a>, galactic collisions, or the influence of other massive stars.



<h3 class="wp-block-heading">Formation of a protostar</h3>



As the cloud collapses, it fragments into smaller clumps. Each clump will eventually form one or more stars. 



The material within these clumps continues to fall inward, heating up as it does so, eventually forming a warm core called a protostar. At this stage, the protostar is not yet hot enough for nuclear fusion (the process that powers stars) to occur.



<h3 class="wp-block-heading">Accretion disk</h3>



Around the protostar, material from the surrounding cloud continues to fall inward, forming a rotating disk. This material slowly accretes onto the protostar, increasing its mass.



<h3 class="wp-block-heading">Nuclear fusion begins</h3>



Once the core of the protostar reaches a high enough temperature and pressure, hydrogen atoms begin to fuse into helium, releasing energy in the process. This marks the transition from a protostar to a main sequence star, like our sun.



<h3 class="wp-block-heading">Main sequence and beyond</h3>



The star will spend the majority of its life in the main sequence stage, where it balances the gravitational forces trying to collapse it and the outward pressure from nuclear fusion. 



Eventually, the star will exhaust its hydrogen fuel. Its subsequent evolution will depend on its initial mass, leading to various end stages such as red giants, supernovae, neutron stars, or black holes.



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



-----



Like what you read? <a href="https://www.earth.com/subscribe/" target="_blank" rel="noreferrer noopener">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



Check us out on <a href="https://www.earth.com/earthsnap/" target="_blank" rel="noreferrer noopener">EarthSnap</a>, a free app brought to you by <a href="https://www.linkedin.com/in/eric-ralls/" target="_blank" rel="noreferrer noopener">Eric Ralls</a> and Earth.com.



-----

Young, massive stars in the Triangulum Galaxy

Flour,Chickpeas,In,Spoonful,,Chick-peas,In,A,Sack,And,Fresh

For decades, studies on mice, monkeys, and even roundworms have pointed to calorie restriction as a ticket to longevity. Trouble is, perpetual hunger does not rank high on most bucket lists, and adherence to such strict diets tends to plummet once real life barges in with birthdays and barbecues.



By the time researchers at the <a href="https://www.wisc.edu/" target="_blank" rel="noreferrer noopener">University of Wisconsin</a> put calorie-cutting under the microscope, they noticed a pattern: eating less helped animals live longer, but the menu’s makeup mattered just as much. 



That discovery widened the spotlight to proteins, the nutrients stitched together from 20 common <a href="https://www.sciencedirect.com/topics/biochemistry-genetics-and-molecular-biology/amino-acids" target="_blank" rel="noreferrer noopener">amino acids</a>. Nine of those are “essential,” meaning the body cannot manufacture them.



Early work hinted that dialing down total protein might mirror the benefits of calorie restriction without the gnawing hunger. 



Mice fed modest protein saw improved <a href="https://www.earth.com/news/drinking-this-amount-of-water-per-day-helps-control-blood-sugar-levels-in-people-with-diabetes/">blood sugar</a> control and trimmer waistlines, yet blanket reductions risked muscle loss, especially in older animals. Something more surgical was needed.



<h2 class="wp-block-heading" id="h-protein-quality-over-quantity">Protein quality over quantity</h2>



Metabolism researcher <a href="https://www.medicine.wisc.edu/directory/lamming_dudley" target="_blank" rel="noreferrer noopener">Dudley Lamming</a> stepped into that gap with a question few had asked: what if the magic hides in specific amino acids rather than protein as a whole? 



“We like to say a calorie is not just a calorie,” he says. “Different components of your diet have value and impact beyond their function as a calorie, and we’ve been digging in on one component that many people may be eating too much of.”



His team homed in on the branched-chain amino acids - <a href="https://www.earth.com/news/eating-too-much-protein-greatly-increases-heart-disease-risk/">leucine</a>, isoleucine, and <a href="https://www.earth.com/news/plants-use-dna-duplication-to-increase-their-resilience/">valine</a> - popular in sports supplements for their muscle-building buzz. Instead of treating them as a block, the researchers isolated each one. Isoleucine quickly took center stage.



<h2 class="wp-block-heading" id="h-cutting-back-on-isoleucine">Cutting back on isoleucine</h2>



When mice at the equivalent of 30 human years were fed chow that cut isoleucine by about two-thirds, their bodies shed fat quickly. 



“Very quickly, we saw the mice on the reduced-isoleucine diet lose adiposity - their bodies got leaner, they lost fat,” says Lamming. 



<a href="https://www.earth.com/news/spicy-foods-can-slow-down-eating-and-cut-calorie-intake/">Calorie intake</a> actually climbed; the animals nibbled more in an apparent effort to find the missing amino acid, yet their metabolisms revved high enough to keep weight off.



Over time, male mice lived about 33 percent longer, and females about 7 percent. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/06/isoleucine_amino-acid_diet-restriction_lifespan-increase_credit-Cell-Metabolism_1m.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/06/isoleucine_amino-acid_diet-restriction_lifespan-increase_credit-Cell-Metabolism_1s.webp" alt="This graphic illustration shows the impact that reduced isoleucine diet had on mice longevity. Credit: Cell Metabolism" class="wp-image-1975852"/></a><figcaption class="wp-element-caption">This graphic illustration shows the impact that reduced isoleucine diet had on mice longevity. Click image to enlarge. Credit: Cell Metabolism</figcaption></figure>



That extra runway arrived with smoother blood sugar curves, sturdier muscles, and fewer signs of frailty across 26 health checks - from grip strength to coat condition. 



Cancer, the usual culprit in an aging mouse colony, struck less often in males on the low-isoleucine diet, and prostate enlargement eased.



<h2 class="wp-block-heading" id="h-how-isoleucine-shapes-lifespan">How isoleucine shapes lifespan</h2>



Most roads in the aging field eventually intersect with <a href="https://www.nature.com/articles/s41392-023-01608-z" target="_blank" rel="noreferrer noopener">mTOR</a>, a cellular sensor finely tuned to amino acid levels. 



Drop isoleucine, and mTOR quiets down, dialing back growth signals that drive both tumor formation and the wear-and-tear of aging. 



The diet also boosts a hormone that helps the body cope with cold and is being studied as a potential diabetes therapy. 



The interplay of these pathways - not yet fully mapped - likely explains why trimming one nutrient outperforms broader protein cuts in middle-aged mice.



“Previous research has shown lifespan increase with low-calorie and low-protein or low-amino-acid diets starting in very young mice,” Lamming explains.



“We started with mice that were already getting older. It’s interesting and encouraging to think a dietary change could still make such a big difference in lifespan and what we call ‘healthspan,’ even when it started closer to mid-life.”



<h2 class="wp-block-heading" id="h-isoleucine-and-human-health">Isoleucine and human health</h2>



Humans need isoleucine for everything from <a href="https://www.earth.com/news/tibetan-women-have-quickly-evolved-to-thrive-in-low-oxygen-and-high-altitudes/">hemoglobin production</a> to immune defense, so eliminating it is off the table. 



The wrinkle is that many Western diets supply far more than the daily requirement, thanks to eggs, cheese, soy isolates, chicken, and beef featuring heavily on menus. 



Surveys from Wisconsin echo national data: people with higher body-mass indexes often report higher isoleucine intake.



“We can’t just switch everyone to a low-isoleucine diet,” Lamming continued. “But narrowing these benefits down to a single amino acid gets us closer to understanding the biological processes and maybe potential interventions for humans, like an isoleucine-blocking drug.”



The team’s nutritional modeling suggests that choosing more fruits, vegetables, and modest portions of animal protein can shave isoleucine totals without complicated meal plans.



<h2 class="wp-block-heading" id="h-human-trials-come-next">Human trials come next</h2>



Because the study relied on a genetically diverse strain of mice - much closer to human variety than lab inbreds - confidence is higher that the findings translate. 



Yet controlled human trials are still required. Researchers are now exploring whether temporary isoleucine dips, similar to the popular five-day <a href="https://www.earth.com/news/alternate-day-fasting-might-be-worth-trying-for-weight-loss/">fasting-mimicking diet</a>, can trigger the same metabolic perks without long-term restriction.



“It could be that by choosing healthier foods and healthier eating in general, we might be able to lower isoleucine enough to make a difference,” Lamming surmised.



While clinicians wait for definitive guidance, nutritionists already recommend leaning on <a href="https://www.earth.com/news/mixed-cover-crops-may-be-the-future-of-sustainable-farming/">legumes, whole grains, and vegetables</a>, which naturally carry less isoleucine than dairy or red meat. That shift dovetails with broader public-health advice to curb chronic disease risk.



<h2 class="wp-block-heading" id="h-eat-right-feel-good-live-longer">Eat right, feel good, live longer</h2>



To sum it all up, living longer has always hinged on a balance between what bodies need and what wears them out. 



The latest evidence suggests that tipping the scales away from a single amino acid might buy extra years without sacrificing satisfaction at the table. 



Turning lab findings into dinner-plate habits won’t happen overnight, but the path is far clearer now than when the conversation started with simply “eat less.”



These full studies were published in the journals <a href="https://www.cell.com/cell-metabolism/fulltext/S1550-4131(23)00374-1" target="_blank" rel="noreferrer noopener">Cell Metabolism</a> and <a href="https://www.nature.com/articles/s43587-024-00744-7" target="_blank" rel="noreferrer noopener">Nature Aging</a>.



-----



Like what you read? <a href="https://www.earth.com/subscribe/" target="_blank" rel="noreferrer noopener">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



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



-----

Removing this one thing from your diet could dramatically increase lifespan

For decades, studies on mice, monkeys, and even roundworms have...

In a fascinating new study, scientists documented 34 attempts by wild killer whales to give food to humans. These rare cases spanned four oceans and 20 years. Some happened near boats, others in open water or even from the shore. 



The events highlight the <a href="https://www.earth.com/news/killer-whales-use-kelp-to-massage-and-groom-each-other/">orcas</a>’ possible interest in humans and raise important questions about whale intelligence, communication, and social behavior.



“Orcas often share food with each other - it’s a prosocial activity and a way that they build relationships with each other,” said study lead author Jared Towers, of <a href="https://baycetology.org" target="_blank" rel="noreferrer noopener">Bay Cetology</a> in British Columbia, Canada. “That they also share with humans may show their interest in relating to us as well.”



<h2 class="wp-block-heading" id="h-social-lives-of-killer-whales">Social lives of killer whales</h2>



Orcas live some of the most complex social lives in the animal kingdom. They stick together in tight-knit family groups called pods, usually led by an older matriarch. 



These family units aren’t just casual gatherings - they’re lifelong bonds. Calves stay with their mothers for life, swimming, hunting, and <a href="https://www.earth.com/news/photographer-captures-killer-whales-wearing-fish-hats/">playing together</a>. 



In some regions, pods form larger communities or clans that share unique vocal dialects, kind of like cultural accents passed down through generations. This tight social structure helps them coordinate during hunts and <a href="https://www.earth.com/news/killer-whales-use-kelp-to-massage-and-groom-each-other/">protect each other</a> from threats.



But it’s not all business. Orcas socialize for the joy of it too. They engage in what clearly looks like play - tossing kelp, breaching dramatically, or nudging one another during underwater games. 



They form friendships beyond their pods and even flirt, showing preferences and personalities. These interactions suggest that orcas have emotional lives and a sense of identity.



<h2 class="wp-block-heading" id="h-what-orcas-gave-humans">What orcas gave humans</h2>



The 34 incidents involved six distinct populations of killer <a href="https://www.earth.com/news/ai-helps-humans-have-20-minute-conversation-with-humpback-whale-named-twain/">whales</a>. They offered humans a total of 18 species: six fish, five mammals, three invertebrates, two birds, one reptile, and even one piece of seaweed.



In 97 percent of these cases, the orcas waited for a human response. Some hovered for several minutes. 



On several occasions, they tried again when the humans ignored or returned the offering. In two especially curious cases, whales retrieved birds after humans returned them, only to offer them again.



This behavior could be a form of interspecies curiosity, communication, or even social learning. As the authors suggest, these events might represent "generalized altruism" - an advanced trait observed in only a few social animals.



<h2 class="wp-block-heading" id="h-exploration-more-than-play">Exploration more than play</h2>



Though play was observed in 38 percent of the interactions, the researchers argue most cases were not playful. The age of the whales varied widely, and many offered whole, fresh prey. 



In over 75 percent of ignored cases, the whales later used the prey for themselves or their group. This suggests the offerings had purpose and value, not just entertainment.



Curiosity-driven behavior, distinct from play, seemed a stronger motivator. As the study explains, animals often explore to reduce uncertainty. 



Offering food to humans might help orcas learn how we respond, just as they would with unfamiliar members of their own <a href="https://www.earth.com/news/whales-blow-bubble-smoke-rings-near-humans-to-communicate/">species</a>.



<h2 class="wp-block-heading" id="h-deep-social-intelligence-at-work">Deep social intelligence at work</h2>



Some whales returned the same item to humans multiple times. Others acted in pairs or small groups. 



Most of the 34 events involved a single whale separating from a larger group. This suggests the act was not for show. Rather, it might reflect the whale's individual decision to interact.



Interestingly, killer <a href="https://www.earth.com/news/how-dolphin-brains-evolved-to-see-underwater-by-using-sound-echolocation/">whales</a> have also been documented cooperating with human fishers in places like Australia and Russia. The authors noted that this history could influence modern interactions, especially as human activity increases near their habitats.



<h2 class="wp-block-heading" id="h-whales-may-view-humans-as-companions">Whales may view humans as companions</h2>



Killer whales rank second only to humans in brain-to-body ratio. They also show advanced emotional and social behavior. 



These traits support complex social learning, reciprocal behavior, and possibly even empathy.



“Offering items to humans could simultaneously include opportunities for killer whales to practice learned cultural behavior, explore or play and in so doing learn about, manipulate or develop relationships with us,” the researchers wrote.



<h2 class="wp-block-heading" id="h-humans-should-not-approach-whales">Humans should not approach whales</h2>



Despite the remarkable nature of these encounters, the researchers urge caution. Orcas can show complex and sometimes unpredictable behavior. 



While no wild killer whale has killed a person, some interactions have been intense. They warn against seeking out such encounters or encouraging the behavior without proper permissions.



Most of these whales belonged to populations that hunt near the surface and share prey frequently. 



No deep-water, fish-only populations were involved. This suggests that cooperative surface hunting may lead to more frequent and visible interspecies interactions.



<h2 class="wp-block-heading" id="h-complex-minds-of-whales-and-humans">Complex minds of whales and humans</h2>



The findings challenge our assumptions about human-animal relationships. If orcas are experimenting with ways to relate to us, it means they recognize us not as threats, but as potential social partners.



These whales are not just predators. They are thinkers, observers, and maybe, in some way, explorers of culture, curiosity, memory, learning, and emotion. 



Their actions suggest complex minds in both whales and humans, capable of choice, empathy, and communication.



The study is published in the <a href="https://psycnet.apa.org/fulltext/2026-29805-001.html" target="_blank" rel="noreferrer noopener">Journal of Comparative Psychology</a>. 



-----



Like what you read? <a href="https://www.earth.com/subscribe/">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.&nbsp;



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



-----

Killer whales are attempting to bond with humans, according to many observations

In a fascinating new study, scientists documented 34 attempts by...

Underwater volcanoes, in the area that is now South Africa, vented roughly 20,500 gigatons of carbon dioxide into the ocean-atmosphere system roughly 183 million years ago, crippling the oxygen cycle. 



Human activity between 1850 and 2019 has already pumped out about 2,390 gigatons of the gas. That’s 12 percent of the Jurassic total in less than two centuries.



<a href="https://www.gps.caltech.edu/people/francois-tissot" target="_blank" rel="noreferrer noopener">Professor François Tissot</a> of the California Institute of Technology studies what came next for the Jurassic seas and what it might tell us about the fate of today’s oceans.



<h2 class="wp-block-heading" id="h-sudden-loss-of-ocean-oxygen">Sudden loss of ocean oxygen</h2>



Bands of limestone from southern Italy record the <a href="https://www.sciencedirect.com/science/article/abs/pii/S0012825223003252" target="_blank" rel="noreferrer noopener">Toarcian Oceanic Anoxic Event</a> (T-OAE), a span when oxygen vanished from vast tracts of seawater and many marine species disappeared. 



During the event, only 6 to 8 percent of the seafloor lay under dead, oxygen-starved water. Yet that area was 28 to 38 times larger than today’s anoxic patches. 



“You can see lots of fossils within ocean sediments before the T‑OAE, and then suddenly they disappear,” said Tissot.



The <a href="https://www.sciencedirect.com/science/article/abs/pii/S0009254116305393" target="_blank" rel="noreferrer noopener">Karoo‑Ferrar</a> large igneous province triggered the event by pouring out vast amounts of carbon. It heated the planet, slowed ocean mixing, and altered chemistry enough to pull oxygen from the water.



The anoxic spell lasted roughly 300,000 to 500,000 years, eventually easing as volcanic pulses waned and natural feedbacks rebalanced carbon and <a href="https://www.earth.com/news/earths-oxygen-supply-may-have-been-kick-started-by-volcanoes/">oxygen cycles</a>.



<h2 class="wp-block-heading" id="h-carbon-disrupted-ocean-life">Carbon disrupted ocean life</h2>



Surging greenhouse gases warmed surface waters, strengthened stratification, and blocked the downward draw of fresh <a href="https://www.earth.com/news/dark-oxygen-discovery-deep-ocean-rocks-upends-centuries-of-scientific-beliefs/">oxygen</a>. 



Warmer water also holds less dissolved gas, so every degree of heating squeezed oxygen concentrations further.



Nutrient runoff from newly exposed volcanic ash likely spurred <a href="https://www.earth.com/news/green-algae-in-lake-erie-may-be-hiding-toxic-deadly-compounds/">algal blooms</a>. When that organic matter sank and decayed, it consumed even more oxygen in deeper layers.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/07/limestone-quarry_ancient-seabed_T-OAE-Map_credit-Tissot_1m.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/07/limestone-quarry_ancient-seabed_T-OAE-Map_credit-Tissot_1s.webp" alt="Map of localities in which the T-OAE was previously recognized, along with our study site. Local anoxia refers to sites where redox proxy data reveal locally dysoxic to anoxic conditions. The site of the MSS is shown by the star in the Inset. KFCA-LIP: Karoo–Ferrar–Chon Aike Large Igneous Province. Credit: Tissot" class="wp-image-1976065"/></a><figcaption class="wp-element-caption">Map of localities in which the T-OAE was previously recognized, along with our study site. Local anoxia refers to sites where redox proxy data reveal locally dysoxic to anoxic conditions. The site of the MSS is shown by the star in the Inset. KFCA-LIP: Karoo–Ferrar–Chon Aike Large Igneous Province. Click image to enlarge. Credit: Tissot</figcaption></figure>



The result was anoxia, a chemically reduced state that favors the precipitation of once‑soluble uranium isotopes into sediments, leaving a measurable fingerprint for modern geochemists.



Scientists use those isotopes, preserved in carbonate grains, to reconstruct ocean redox conditions long after the water is gone.



<h2 class="wp-block-heading" id="h-tracing-ancient-ocean-oxygen-change">Tracing ancient ocean oxygen change</h2>



Tissot’s team combined 30 limestone samples with a <a href="https://www.publichealth.columbia.edu/news/what-bayesian-modeling" target="_blank" rel="noreferrer noopener">Bayesian model</a> built by <a href="https://www.gmu.edu/" target="_blank" rel="noreferrer noopener">George Mason University</a> researcher <a href="https://www.researchgate.net/scientific-contributions/Michael-A-Kipp-2118354679" target="_blank" rel="noreferrer noopener">Michael Kipp</a> to convert uranium data into the size of past anoxic zones. 



The model showed oxygen loss peaking just after the first volcanic pulse, then gradually recovering as emissions slowed.



Because uranium mixes uniformly in seawater, its isotopic shift offers a global view rather than a local snapshot, sidestepping problems that plague black shale studies in restricted basins. 



Independent work on molybdenum and thallium isotopes points to the same magnitude of <a href="https://www.earth.com/news/jurassic-extinction-may-hold-clues-about-our-oceans-future/">Jurassic</a> deoxygenation, reinforcing confidence in the carbonate method. Multiple tracers show how fast oceans can suffocate when carbon overwhelms natural buffers.



<h2 class="wp-block-heading" id="h-rock-preserved-ocean-memory">Rock preserved ocean memory</h2>



The limestones sampled from Mercato San Severino in Italy belong to a 5,000-foot-thick sequence of shallow-water carbonates. These were laid down on the southern edge of the ancient <a href="https://www.sciencedirect.com/science/article/pii/S0012825223002830" target="_blank" rel="noreferrer noopener">Tethys Ocean</a>. 



These deposits are ideal for capturing uranium isotope signals because they formed under well-oxygenated conditions and remained chemically stable over time.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/07/limestone-quarry_ancient-seabed_Mercato-San-Severino_credit-Tissot_1m.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/07/limestone-quarry_ancient-seabed_Mercato-San-Severino_credit-Tissot_1s.webp" alt="A quarry illustrating bands of stratified limestone from the ancient seafloor in what is now Mercato San Severino in Italy. Credit: F. Tissot" class="wp-image-1976063"/></a><figcaption class="wp-element-caption">A quarry illustrating bands of stratified limestone from the ancient seafloor in what is now Mercato San Severino in Italy. Click image to enlarge. Credit: F. Tissot</figcaption></figure>



Geochemical screening confirmed the rocks remained largely unaltered after burial. Isotope ratios, trace elements, and sediment structure all supported the conclusion that these limestones faithfully recorded seawater chemistry from the time of deposition.



<h2 class="wp-block-heading" id="h-today-s-waters-mirror-the-past">Today's waters mirror the past</h2>



Modern measurements show that only about 0.2 percent of the seafloor is overlain by permanently anoxic water, mostly in marginal seas like the Black Sea. 



Yet the global inventory of dissolved oxygen has already fallen by roughly 2 percent since 1960. “Oxygen concentrations in both the open ocean and coastal waters have been declining since at least the middle of the 20th century,” said marine ecologist <a href="https://serc.si.edu/staff/denise-breitburg/breitburgd9302003?sort_bef_combine=field_pub_date_value%20ASC&amp;page=3" target="_blank" rel="noreferrer noopener">Denise Breitburg</a>.



A 2024 <a href="https://www.nature.com/articles/s41467-024-52197-6">study</a> warned that deoxygenation will accelerate this century as warming and stratification intensify. If emissions rise, mid-depth zones could lose 20 percent of oxygen by 2100, exceeding many species’ physiological limits.



Dead zones already plague more than 400 estuaries worldwide, harming fisheries and coastal economies and hinting at larger changes offshore.



<h2 class="wp-block-heading" id="h-action-needed-before-oceans-suffocate">Action needed before oceans suffocate </h2>



Past events show that once widespread anoxia takes hold, recovery can take tens of thousands of years even after carbon input stops. 



Unlike volcanic outbursts, human emissions are continuous and tightly linked to energy and food systems, making a quick cutoff challenging. 



Cutting fossil fuel use, protecting carbon‑storing ecosystems, and curbing nutrient runoff can slow oxygen loss before feedback amplifies the trend.



Satellites, autonomous floats, and seafloor sensors now track oxygen in near real time. This gives policymakers a chance to act before thresholds comparable to the <a href="https://www.earth.com/news/jurassic-rocks-reveal-new-details-about-earths-climate-system/">Jurassic</a> pulse are crossed.



Tissot’s limestone cores remind us that the ocean’s memory is long and its tolerance finite.



The study is published in <a href="https://www.pnas.org/doi/10.1073/pnas.2406032121" target="_blank" rel="noreferrer noopener">Proceedings of the National Academy of Sciences</a>.



-----



Like what you read?<a href="https://www.earth.com/subscribe/"> Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.&nbsp;



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



-----

What happened in the ocean millions of years ago could happen again today

Underwater volcanoes, in the area that is now South Africa,...

Cell biology is a world of constant motion and hidden structures. Much of what we know about cells comes from decades of research using microscopes, stains, and models. Yet, even in this well-charted territory, surprises still emerge - enter the "hemifusome."



This previously unknown organelle may help explain how cells sort, recycle, and discard their internal cargo. This function is vital to life and is often disrupted in instances of genetic disease.



The discovery of this organelle, which was made by scientists at the <a href="https://www.virginia.edu" target="_blank" rel="noreferrer noopener">University of Virginia</a> and the National Institutes of Health (<a href="https://www.nih.gov" target="_blank" rel="noreferrer noopener">NIH</a>), offers a new lens through which to study the inner workings of the cell. 



It also presents a possible turning point for understanding diseases where cellular housekeeping breaks down. Using cutting-edge imaging tools, researchers have caught this <a href="https://www.earth.com/news/cambrian-explosion-fossils-push-back-the-rise-of-complex-life/">organelle</a> in action and outlined its potential impact on health and medicine.



<h2 class="wp-block-heading" id="h-introducing-the-hemifusome">Introducing the hemifusome</h2>



The hemifusome is not a static component but a temporary structure that appears and disappears depending on the cell’s needs. 



It consists of two vesicles joined together by a partial membrane connection called a hemifusion diaphragm.



In this configuration, the vesicles do not fully merge but maintain a shared boundary that allows them to interact without blending entirely.



"This is like discovering a new recycling center inside the cell," said researcher Seham Ebrahim, Ph.D., of UVA's Department of Molecular Physiology and Biological Physics. 



"We think the hemifusome helps manage how <a href="https://www.earth.com/news/third-state-of-existence-beyond-life-and-death-confirmed-by-scientists/">cells</a> package and process material, and when this goes wrong, it may contribute to diseases that affect many systems in the body."



These hemifused vesicles appear in two configurations. In the direct form, a smaller vesicle is attached to the outer side of a larger one, whereas in the flipped version, the smaller vesicle is embedded on the inner, or luminal, side. 



In both cases, a dense particle called a proteolipid nanodroplet anchors the structure at the junction, possibly guiding its formation and stability.



<h2 class="wp-block-heading" id="h-how-the-hemifusome-appears">How the hemifusome appears</h2>



To study hemifusomes, researchers turned to cryo-electron tomography (cryo-ET). This imaging method freezes cells rapidly, preserving them close to their natural state. 



Unlike traditional <a href="https://www.earth.com/news/watching-electrons-move-1-quintillionth-of-second-attoseconds-attomicroscopy/">electron microscopy</a>, which can distort or destroy delicate structures, cryo-ET allows scientists to see cellular architecture as it truly exists.



By scanning the outer edges of four mammalian cell types, COS-7, HeLa, RAT-1, and NIH/3T3, the team identified hundreds of hemifusomes. These organelles made up nearly 10 percent of all membrane-bound vesicles in those regions. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/07/hemifused-vesicles_cryo-electron-tomography_Nature-Communications_1m.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/07/hemifused-vesicles_cryo-electron-tomography_Nature-Communications_1s.webp" alt="Cryo-electron tomography observation of hemifused vesicles at the leading edge of cultured cells. Credit: Nature Communications (2025)" class="wp-image-1976051"/></a><figcaption class="wp-element-caption">Cryo-electron tomography observation of hemifused vesicles at the leading edge of cultured cells. Click image to enlarge. Credit: Nature Communications (2025)</figcaption></figure>



Their consistency across <a href="https://www.earth.com/news/why-millions-of-fungal-species-still-remain-unknown/">cell</a> types suggests they are not rare anomalies but common cellular components.



"You can think of vesicles like little delivery trucks inside the cell," said Ebrahim, of UVA's Center for Membrane and Cell Physiology. "The hemifusome is like a loading dock where they connect and transfer cargo. It's a step in the process we didn't know existed."



<h2 class="wp-block-heading" id="h-what-makes-the-hemifusome-unique">What makes the hemifusome unique</h2>



Hemifusomes stand out not just for their shape, but for what’s inside them. The larger vesicle usually contains granular material, similar to what is seen in <a href="https://www.earth.com/news/mitochondria-cells-batteries-leaking-causes-inflammation-diseases/">endosomes</a> and ribosome-associated vesicles.



But the smaller vesicle shows a smooth, translucent interior. This likely reflects a protein-free or dilute aqueous solution, setting it apart from other vesicles in the cell.



The hemifusion diaphragm itself is unusually large, about 160 nanometers in diameter, far bigger than the 10 nanometer diaphragms seen in standard vesicle fusion <a href="https://www.earth.com/news/gold-eating-fungus-discovery-could-revolutionize-the-search-for-metals-and-minerals-on-earth-asteroids-and-other-planets/">events</a>. These extended diaphragms appear stable, not fleeting, suggesting they may be designed to last. 



In some cases, the diaphragm grows large enough to engulf the entire smaller vesicle into the larger one’s bilayer, creating a lens-like shape known in simulations as dead-end hemifusion. Seeing this in actual cells challenges the idea that such formations are purely theoretical.



<h2 class="wp-block-heading" id="h-anchors-and-architects-of-the-organelle">Anchors and architects of the organelle</h2>



One consistent feature at the heart of hemifusomes is the dense proteolipid nanodroplet, or PND. About 42 nanometers in diameter, these droplets are lodged at the rim of the hemifusion site. 



Their content, lipids and proteins, suggests they may help build or stabilize the hemifused structure.



These PNDs have never been observed in such a role before. Some appear free in the cytoplasm, others are embedded in membranes. Researchers propose that PNDs may serve as scaffolds for assembling new vesicles. 



As the PND integrates into a membrane, it may kickstart the formation of the smaller vesicle seen in hemifusomes.



This process, described as <a href="https://www.sciencedirect.com/topics/neuroscience/vasculogenesis" target="_blank" rel="noreferrer noopener">de novo vesiculogenesis</a>, stands apart from classical vesicle fusion. The presence of a unique, translucent vesicle and the absence of known docking steps indicate the hemifusome may follow its own assembly path.



<h2 class="wp-block-heading" id="h-are-hemifusomes-related-to-endosomes">Are hemifusomes related to endosomes?</h2>



Given their location and size, hemifusomes resemble some endosomal structures. To investigate this further, the researchers traced the journey of gold nanoparticles, common markers used to map endocytic activity. 



The particles entered known endosomes and <a href="https://www.earth.com/news/tricking-cells-into-thinking-they-ate-less-food-can-slow-aging-process/">lysosomes</a> but never appeared inside hemifusomes. This absence suggests that hemifusomes do not belong to the classical endocytic pathway.



Instead, they may represent a separate system operating independently of the cargo sorting carried out by proteins like ESCRT. This distinction may have wide implications for how we understand vesicle traffic inside cells.



<h2 class="wp-block-heading" id="h-multivesicular-bodies-and-disease">Multivesicular bodies and disease</h2>



Some hemifusomes evolve into more complex structures. The study observed compound hemifusomes that contained multiple vesicles, all partially fused. 



These could be early versions of <a href="https://www.sciencedirect.com/topics/medicine-and-dentistry/multivesicular-body" target="_blank" rel="noreferrer noopener">multivesicular bodies</a> (MVBs), which cells use to break down and recycle internal material.



In the canonical model, ESCRT proteins form inward buds that eventually pinch off inside a larger vesicle. But in hemifusomes, vesicles grow inward through hemifusion and expand with the help of PNDs. 



This alternative route might explain how MVBs form in ways not covered by traditional theories.



One such condition affected by these pathways is Hermansky-Pudlak syndrome. It is a genetic disorder marked by defects in pigmentation, lung function, vision, and bleeding. <a href="https://www.earth.com/news/damaged-mitochondria-recycled/">Cellular recycling</a> issues are central to the disease.



Understanding the hemifusome may help explain these disruptions and lead to future treatments.



<h2 class="wp-block-heading" id="h-a-new-model-for-vesicle-formation">A new model for vesicle formation</h2>



The study proposes a full model where PNDs trigger the formation of translucent vesicles that partially fuse with larger ones, forming hemifusomes. 



These structures may then bud inward, transforming into flipped hemifusomes. Over time, they could scission off as free vesicles inside MVBs.



In contrast to the ESCRT system, which requires tight protein coordination, this mechanism relies on structural and biophysical cues. 



It also sidesteps the need for large lipid donations from other organelles, solving a long-standing puzzle in vesicle formation research.



"This is just the beginning," Ebrahim said. "Now that we know hemifusomes exist, we can start asking how they behave in healthy cells and what happens when things go wrong. That could lead us to new strategies for treating complex genetic diseases."



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



The implications of this discovery stretch far beyond cell biology. By offering a new pathway for how cells build and manage internal compartments, the hemifusome challenges decades of assumptions. 



It also invites new thinking about disease, especially conditions where cells fail to manage their waste.



Future research will focus on identifying what proteins guide hemifusome formation and how PNDs are created. 



Scientists also want to know if these structures exist in other parts of the cell, not just at the periphery. Advanced imaging tools and genetic models will be key to answering these questions.



In a field where many believed the major organelles were already mapped, the hemifusome serves as a reminder. The cell still holds secrets. And some of them could lead to cures.



The study is published in the journal <a href="https://www.nature.com/articles/s41467-025-59887-9" target="_blank" rel="noreferrer noopener">Nature Communications</a>.



-----



Like what you read? <a href="https://www.earth.com/subscribe/">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.&nbsp;



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



-----

Scientists discover a new organelle inside human cells with huge potential impact on health

Cell biology is a world of constant motion and hidden...

A fresh set of numbers is changing what scientists thought happens when a city‑sized slab of ice dissolves into the sea. The target was <a href="https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2023GL104028">mega‑iceberg</a> A‑68A, a floating platform roughly twice the area of Delaware that drifted toward South Georgia in early 2021.



“We think this is the first time measurements have been made so close to an iceberg,” said <a href="https://www.bas.ac.uk/profile/nacas/" target="_blank" rel="noreferrer noopener">Natasha Lucas of the British Antarctic Survey</a>, lead author of the new study. 



For the first time, researchers steered robotic vehicles to within 14 mi of such a iceberg and kept them there long enough to watch meltwater, temperature, and life interact in real time.&nbsp;



<h2 class="wp-block-heading" id="h-tracking-the-a-68a-iceberg">Tracking the A-68A iceberg</h2>



A‑68A calved from the Larsen C Ice Shelf <a href="https://www.earth.com/news/iceberg-larsen-c-antarctica/">back in 2017</a>, then rode the currents of the <a href="https://www.asoc.org/learn/welcome-to-the-southern-ocean/" target="_blank" rel="noreferrer noopener">Southern Ocean</a> on a five‑year tour that ended near South Georgia. 



<a href="https://www.earth.com/news/small-satellites-are-monitoring-ocean-conditions-from-space/">Satellites</a> could trace its general route, but ships kept their distance because the iceberg’s smaller rifts and spins defied prediction.



That standoff ended when a six‑foot‑long glider slipped off the deck of the <a href="https://noc.ac.uk/facilities/ships/rrs-james-cook" target="_blank" rel="noreferrer noopener">research vessel RRS James Cook</a> and began diving and climbing through a 0.6‑mile‑deep column of water. 



Over 49 days it logged 265 vertical profiles, sending each packet of data to scientists piloting the craft from home offices locked down by COVID‑19 restrictions.



The adventure was not entirely smooth. One glider vanished in the melee of drifting growlers, and another spent 17 days wedged beneath the berg before currents spat it out, battery blinking but sensors intact. 



Still, the mission mapped a zone of ocean that had never been observed so closely or for so long.



<h2 class="wp-block-heading" id="h-sensors-beneath-a-68a">Sensors beneath A-68A</h2>



The glider recorded a frosty cap of freshwater spreading across the top 30 ft of the sea. Right below, the instruments found a band of cold winter water that had lost its usual punch, a sign that melt‑driven turbulence had chewed away the seasonal layer separating surface and depth.



As that barrier thinned, nutrient‑rich deep water began sliding upward, carrying iron and silica shaved from the iceberg’s base. 



The upheaval altered local stratification, flipping the normal stack of density and temperature that keeps layers neatly in place during the Antarctic summer.



Salinity told the same story. At barely two miles from A‑68A, the profiles showed tongue‑shaped intrusions of water warmer and saltier than their neighbors, hallmarks of <a href="https://www.earth.com/news/life-survived-when-earth-was-covered-in-ice-but-how/">meltwater</a> plumes that had raced up the iceberg’s base before fanning out sideways.



<h2 class="wp-block-heading" id="h-a-68a-fuels-ocean-life">A‑68A fuels ocean life</h2>



Plankton reacted almost immediately. Near the ice wall, the glider’s fluorometer logged low <a href="https://oceantracks.org/library/oceanographic-factors/chlorophyll" target="_blank" rel="noreferrer noopener">chlorophyll</a> and high backscatter, evidence that meltwater diluted existing blooms while also dumping silt that clouded the light.



Farther away, a spike in <a href="https://www.earth.com/news/shifting-ocean-color-is-pushing-marine-life-toward-the-poles/">chlorophyll</a> flared about 36 hours after the iceberg’s passage, matching lab‑measured growth rates for the local phytoplankton community.



The burst hints that the same plume which first thinned the bloom later primed the water with micronutrients, a one‑two punch that temporarily shuffled who eats whom in the surface ocean.



Because upwelling also lifts dissolved carbon and heat, even short‑lived events like this matter to krill, fur seals, and the economy of South Georgia’s fisheries.



<h2 class="wp-block-heading" id="h-carbon-questions-on-a-cold-frontier">Carbon questions on a cold frontier</h2>



The carbon sink south of 35° S absorbs roughly 40 percent of humanity’s <a href="https://www.earth.com/news/creating-forests-cant-realistically-cancel-out-fossil-fuel-emissions/">fossil‑fuel emissions</a>. How that service will fare as calving accelerates remains uncertain.



The new findings show giant bergs can raise near‑surface stratification yet also stir the mid‑depths, two adjustments that tug carbon uptake in opposite directions. 



Recent model work argues current estimates may already overshoot Southern Ocean uptake by up to 0.4 Pg C yr‑1. Field evidence like the A‑68A data set will help sort winners from losers in that accounting.



<h2 class="wp-block-heading" id="h-risk-reward-and-remote-control">Risk, reward, and remote control</h2>



Flying a glider next to a iceberg the size of Los Angeles is an exercise in calculated gamble. Lucas and colleagues guided their craft from desks more than 7,500 miles away, relying on patchy satellite snapshots to dodge smaller ice.



When the glider went missing under the berg, frustration turned to nervous excitement, then relief as it resurfaced with a <a href="https://www.earth.com/news/supergiant-gold-deposit-find-claims-to-be-the-worlds-largest-discovery-ever/">gold mine</a> of temperature and salinity profiles. 



That trove fixed the first real numbers on basal melt rate, pegging it at roughly 6.9 × 10^8 m³ per day, an estimate within a factor of two of satellite calculations derived from changes in the iceberg’s freeboard height.



<h2 class="wp-block-heading" id="h-icebergs-preview-ocean-changes">Icebergs preview ocean changes</h2>



A‑68A is gone now, splintered into shards tracked only by radar, but younger cousins are lining up. The trillion‑ton A‑23A grounded off South Georgia this <a href="https://earthobservatory.nasa.gov/images/154022/iceberg-grinds-to-a-stop-off-south-georgia-island" target="_blank" rel="noreferrer noopener">March</a>, parking just 43 miles from the shore.



Researchers expect more deep‑drafted icebergs to exit West Antarctica as warming currents nibble ice shelves. 



Each one represents a floating lab, a hazard to shipping, and an agent of surprise for ecosystems that evolved around predictable cycles of light and nutrients.



The new study proves those labs are accessible with today’s tools. It also shows that a single iceberg can redraw local physics and biology in days, a reminder that climate change sends ripple effects far beyond melting ice.



The study is published in <a href="https://www.nature.com/articles/s41561-025-01659-7" target="_blank" rel="noreferrer noopener">Nature Geoscience</a>.



-----



Like what you read?<a href="https://www.earth.com/subscribe/"> Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.&nbsp;



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



-----

Scientists measure marine environment near melting mega-iceberg for first time

A fresh set of numbers is changing what scientists thought...

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...

<div class="wp-block-sendtonews-playerselector">[sendtonews key="0ynNMYkMKa-2340414-12187" type="single"]</div>



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



---



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

[sendtonews key="0ynNMYkMKa-2340414-12187" type="single"] Today’s Video of the Day from the...

<div class="wp-block-sendtonews-playerselector">[sendtonews key="G9bUoxcjr4-2511624-12187" type="single"]</div>



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;



---



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...

Eagle Nebula: Carving light from darkness

News coming your way