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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA



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Ghostly galaxy in the constellation Eridanus

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

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA



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Rosetta Nebula: Sculpted by starlight over millions of years

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA/ESA Hubble Space Telescope



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Secrets of a spiraling galactic powerhouse

Today's Image of the Day from the European Space Agency features NGC 1333, a reflection nebula located in the Perseus molecular cloud about 960 light-years away from Earth. The photo is a mosaic of images captured by the James Webb Space Telescope.



“Webb’s superb sensitivity allows astronomers to investigate young objects with extremely low masses. Some of the faintest ‘stars’ in the picture are in fact newly born free-floating brown dwarfs with masses comparable to those of giant planets,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



The same cluster was featured in the 33rd anniversary image of the Hubble Space Telescope in April 2023. 



According to ESA, Hubble’s image just scratched the surface of this region, because clouds of dust obscure much of the star formation process. 



"Observing with larger aperture and in the infrared part of the spectrum, Webb is capable of peering through the dusty veil to reveal newborn stars, brown dwarfs and planetary mass objects."



<h2 class="wp-block-heading" id="h-webb-s-view-of-ngc-1333">Webb’s view of NGC 1333</h2>



ESA noted that the center of the image presents a deep peek into the heart of the NGC 1333 cloud.&nbsp;



“Across the image we see large patches of orange, which represent gas glowing in the infrared. These so-called Herbig-Haro objects form when ionized material ejected from young stars collides with the surrounding cloud. They are hallmarks of a very active site of star formation."



The disks of gas and dust that surround the <a href="https://www.earth.com/news/newly-discovered-stars-milky-way-are-old-as-universe/" target="_blank" rel="noreferrer noopener">stars</a> in this image may eventually produce planetary systems.&nbsp;



<h2 class="wp-block-heading" id="h-stars-in-the-sun-s-birth-cluster">Stars in the Sun's birth cluster</h2>



“Similar to the young stars in this mosaic, our own Sun and planets formed inside a dusty molecular cloud, 4.6 billion years ago. Our Sun did not form in isolation but as part of a cluster, which was perhaps even more massive than NGC 1333,” explained ESA.



Over time, the stars in the Sun's birth cluster would have drifted apart due to gravitational interactions and the dispersion of gas in the region.



Astronomers have been studying certain clues, such as isotopic signatures in meteorites, that hint the Sun may have formed near massive stars. These stars likely produced supernovae, which could have influenced the early <a href="https://www.earth.com/news/mysterious-objects-spotted-in-the-outer-solar-system-beyond-pluto/" target="_blank" rel="noreferrer noopener">solar system</a> by injecting heavy elements like iron-60.



<h2 class="wp-block-heading" id="h-star-formation-in-ngc-1333">Star formation in NGC 1333</h2>



NGC 1333 is a vibrant example of a stellar nursery, where active <a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">star formation</a> is ongoing. It is known for its chaotic appearance, shaped by the interactions between newborn stars and the surrounding material.



Within NGC 1333, astronomers have observed a high level of turbulence, which makes the region dynamic and complex. 



These disturbances are caused by the outflows of young stars as they eject material into their surroundings, creating shock waves and influencing further star formation.&nbsp;



These outflows are often seen as jets, which are visible in multiple wavelengths of light, especially infrared, as the surrounding dust absorbs visible light.



<h2 class="wp-block-heading" id="h-early-stages-of-planet-formation">Early stages of planet formation </h2>



NGC 1333 is also an area of interest for studying the early stages of star and <a href="https://www.earth.com/news/planet-formation-new-insights-mechanics-physics/" target="_blank" rel="noreferrer noopener">planet formation</a>, as many of the stars within the cluster are in their infancy.



These stars are still in the process of gathering material and developing protoplanetary disks. 



In images, NGC 1333 is marked by bright patches of blue and red, representing reflection <a href="https://www.earth.com/news/six-rogue-worlds-discovered-inside-a-young-star-forming-nebula/" target="_blank" rel="noreferrer noopener">nebulae</a> and the ionized gas created by energetic young stars.&nbsp;



<h2 class="wp-block-heading" id="h-the-perseus-molecular-cloud-nbsp">The Perseus molecular cloud&nbsp;</h2>



The Perseus molecular cloud is a vast region of cold gas and dust located about 600 light-years away from Earth in the constellation <a href="https://www.earth.com/news/1500-billion-orphan-stars-discovered-in-the-perseus-galaxy-cluster/" target="_blank" rel="noreferrer noopener">Perseus</a>.&nbsp;



It is one of the most studied star-forming regions in our galaxy due to its relative proximity and the diversity of its young stellar objects. This cloud spans several hundred light-years and contains dense pockets of gas where new stars are actively forming.&nbsp;



These areas are often enshrouded in thick dust, which obscures them in visible light but allows astronomers to study them using infrared and radio wavelengths.



The Perseus molecular cloud is particularly interesting because of the chemistry taking place within it, including the formation of complex organic molecules that could be precursors to life.&nbsp;



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



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Stellar nursery shines in the Perseus cloud

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



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Young, massive stars in the Triangulum Galaxy

Today's Image of the Day from NASA Earth Observatory features an astronaut view of Mount Nemrut, a volcano located in eastern Turkey near Lake Van.



Mount Nemrut is notable for its immense caldera, which was formed through a series of <a href="https://www.earth.com/news/volcanic-eruptions-play-an-overlooked-role-in-earths-climate/" target="_blank" rel="noreferrer noopener">eruptions</a>. The caldera, one of the largest in the world, now contains several lakes such as Lake Nemrut.&nbsp;



"The eastern half of the caldera is partially filled by solidified lava flows from past eruptions. Snow cover present at the time of this photo accentuates pressure ridges that formed as the lava was flowing and cooling," noted <a href="https://earthobservatory.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA</a>.



"These pressure ridges vary in size, thickness, and orientation due to the varying viscosity and flow direction of the lavas during eruptions."



<h2 class="wp-block-heading" id="h-formation-of-lake-nemrut">Formation of Lake Nemrut</h2>



"Lake Nemrut (Nemrut Gölü) occupies the western half of the caldera, creating a rough crescent shape that partially submerges the old lava flows," said NASA.



"This freshwater lake, reaching up to 176 meters deep, is accompanied by a smaller lake at the upper-center of the caldera."



The lake was formed after the collapse of the Nemrut volcano's summit. This collapse created a massive crater, which gradually filled with water over time, forming the <a href="https://www.earth.com/news/alarming-study-most-of-the-worlds-largest-lakes-are-quickly-losing-water/" target="_blank" rel="noreferrer noopener">lake</a>.



<h2 class="wp-block-heading" id="h-unesco-world-heritage-site">UNESCO World Heritage Site </h2>



Mount Nemrut and its surroundings are part of a protected UNESCO World Heritage Site due to their ecological and geological significance.



The site is home to diverse wildlife, including various bird species that use the lake as a stopover during migration. The caldera also contains smaller lakes and wetlands, adding to the area's biodiversity.



Lake Nemrut is a popular destination for tourists, hikers, and nature enthusiasts, offering stunning views of the volcanic landscape.



Despite its popularity, the lake remains relatively remote and unspoiled, contributing to its appeal as a natural wonder.



<h2 class="wp-block-heading" id="h-mount-nemrut-has-shaped-the-landscape">Mount Nemrut has shaped the landscape</h2>



Geologically, Mount Nemrut is interesting because its <a href="https://www.earth.com/news/new-research-enhances-predictions-on-volcanic-eruptions/" target="_blank" rel="noreferrer noopener">eruptions</a> have played a key role in shaping the local landscape. 



Its last major eruption occurred around 1441 AD, which indicates that it's not currently active.



The area around Nemrut is known for its geothermal activity, including hot springs and fumaroles, suggesting that there is still significant heat beneath the surface.



<h2 class="wp-block-heading" id="h-tribute-to-a-king">Tribute to a king</h2>



Over thousands of years, various civilizations have inhabited the region around Nemrut, leaving behind a wealth of archaeological sites.



The summit of Mount Nemrut is dominated by a vast funerary mound constructed by King Antiochus I Theos, who ruled the Kingdom of Commagene in the 1st century BCE. 



The site was intended to serve as his tomb sanctuary and a place to commemorate the king's vision of divine kingship and unity between Eastern and Western cultures.



The mound, made of loose crushed stones, measures about 50 meters (164 feet) in height and spans a diameter of 150 meters (492 feet), creating an imposing feature visible from afar.



Surrounding the mound are terraces on the eastern, western, and northern sides, each adorned with colossal statues and reliefs. The statues, ranging in height from 8 to 10 meters (26 to 33 feet), represent various deities, including Zeus, Apollo, Hercules, and the goddess Tyche, alongside King Antiochus himself. 



The heads of the statues, many of which have toppled over due to <a href="https://www.earth.com/news/new-map-shows-75-percent-of-the-u-s-at-risk-of-damaging-earthquakes/" target="_blank" rel="noreferrer noopener">earthquakes</a> and erosion, lie scattered around the site.



<h2 class="wp-block-heading" id="h-spiritual-and-religious-practices">Spiritual and religious practices</h2>



In addition to the statues, inscriptions at Mount Nemrut provide valuable historical information about the kingdom, the king's lineage, and the religious practices of the time.



The site is not only a marvel of ancient engineering but also a spiritual and astronomical center. Scholars believe the terraces were aligned with celestial events, serving as an observatory for solstices and equinoxes.



In addition to its natural and historical significance, the Nemrut volcano has been the subject of scientific study, as researchers aim to understand more about <a href="https://www.earth.com/news/volcanic-eruptions-play-an-overlooked-role-in-earths-climate/" target="_blank" rel="noreferrer noopener">volcanic activity</a> in the region, the history of its eruptions, and the potential risks it may pose in the future.



Image Credit: NASA Earth Observatory



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Mount Nemrut: Ancient mysteries and natural marvels 

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

A new phenomenon dubbed "ice piracy" is unfolding in the frigid wilderness of West Antarctica, where one glacier appears to be stealing ice from its neighbor. 



This unusual behavior - once believed to take hundreds or even thousands of years - has now been recorded happening in under two decades.



Scientists from the University of Leeds, working with international collaborators, have used high-resolution satellite data to reveal that a fast-moving glacier is redirecting ice flow away from its slower neighbor.



This surprising event is changing how scientists understand the dynamics of glaciers - and how such shifts may contribute to future sea-level rise. Their findings, now published in The Cryosphere, provide rare insight into these rapid changes.



<h2 class="wp-block-heading" id="h-fast-paced-shift-in-the-ice">Fast-paced shift in the ice</h2>



Between 2005 and 2022, researchers observed that seven <a href="https://www.earth.com/news/ice-streams-move-unpredictably-due-to-hidden-quakes/" target="_blank" rel="noreferrer noopener">ice streams</a> in the Pope, Smith, and Kohler (PSK) region of West Antarctica sped up significantly. 



One glacier nearly doubled its speed - an 87% increase - at the point where it meets the ocean. 



Three other glaciers accelerated by 60% to 84%. By 2022, six of these streams were moving at more than 700 meters (0.4 miles) per year. That’s the equivalent of covering just over seven football fields in just one year.



This kind of acceleration, especially so close to the grounding line - the point where a glacier starts to float - is a warning sign. 



Grounding lines help track the stability of ice sheets. Changes in their position or speed suggest the system is out of balance and can influence how ice flows inland.



<h2 class="wp-block-heading" id="h-slowing-glaciers-leads-to-ice-piracy">Slowing glaciers leads to ice piracy</h2>



But not every glacier followed the same pattern. The Kohler West glacier actually slowed down by 10% during the same time period. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/05/Antarctica_ice-piracy_Glacier-velocity-change_2005-2022_ESA_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/05/Antarctica_ice-piracy_Glacier-velocity-change_2005-2022_ESA_1s.webp" alt="The image depicts the average change in velocity of multiple glaciers flowing into the Crosson and Dotson Ice Shelves in West Antarctica from 2005 to 2022. Credit: ESA" class="wp-image-1969732"/></a><figcaption class="wp-element-caption">The image depicts the average change in velocity of multiple glaciers flowing into the Crosson and Dotson Ice Shelves in West Antarctica from 2005 to 2022. Click image to enlarge. Credit: ESA</figcaption></figure>



This stood in stark contrast to nearby glaciers like Kohler East and Smith West, which sped up dramatically - by about 560 meters per year.



The slowdown puzzled scientists, until they looked at the ice flow patterns.



<h2 class="wp-block-heading" id="h-kohler-west-and-kohler-east">Kohler West and Kohler East</h2>



“We think that the observed slowdown on Kohler West Glacier is due to the redirection of ice flow towards its neighbor - Kohler East," explained lead author Dr. Heather L. Selley from the <a href="https://www.leeds.ac.uk/" target="_blank" rel="noreferrer noopener">University of Leeds</a>.



"This is due to the large change in Kohler West’s surface slope, likely caused by the vastly different thinning rates on its neighboring <a href="https://www.earth.com/news/antarctic-glaciers-flow-faster-during-the-summer-time/" target="_blank" rel="noreferrer noopener">glaciers</a>.” 



She added that because Kohler East’s ice stream is flowing and thinning faster as it travels, it absorbs, or ‘steals’ ice from Kohler West. 



"This is effectively an act of ‘ice piracy’, where ice flow is redirected from one glacier to another, and the accelerating glacier is essentially ‘thieving’ ice from its slowing neighbor,” explained Selley.



“We didn’t know ice streams could ‘steal’ ice from each over such a short period, so this is a fascinating discovery. It’s unprecedented as we're seeing this from satellite data and it’s happening at a rate of under 18 years, whereas we’ve always thought it was this extremely long, slow process,” she added.



<h2 class="wp-block-heading" id="h-watching-ice-piracy-from-space">Watching ice piracy from space</h2>



To track this shift, the research team used satellite images and a technique that follows the movement of surface features like crevasses and rifts. 



They also incorporated data on ice thinning from the European Space Agency’s <a href="https://www.esa.int/Applications/Observing_the_Earth/FutureEO/CryoSat" target="_blank" rel="noreferrer noopener">CryoSat mission</a>.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/05/Antarctica_ice-piracy_speed-direction_Crosson-Dotson-Ice-Shelves_2015-2022_ESA_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/05/Antarctica_ice-piracy_speed-direction_Crosson-Dotson-Ice-Shelves_2015-2022_ESA_1s.webp" alt="The image depicts the average speed and direction of multiple glaciers flowing into the Crosson and Dotson Ice Shelves in West Antarctica from 2015 to 2022. The arrows show change in direction of flow. Credit: ESA" class="wp-image-1969725"/></a><figcaption class="wp-element-caption">The image depicts the average speed and direction of multiple glaciers flowing into the Crosson and Dotson Ice Shelves in West Antarctica from 2015 to 2022. The arrows show change in direction of flow. Click image to enlarge. Credit: ESA</figcaption></figure>



Data was sourced from satellites operated by ESA, NASA, the Canadian Space Agency, and the Japan Aerospace Exploration Agency.



“This study provides an interesting demonstration of ice piracy, where flow into one glacier gradually switches to flow into another glacier, as the ocean melts the grounding zone and re-configures ice flow,” said Pierre Dutrieux, climate researcher at the <a href="https://www.bas.ac.uk/" target="_blank" rel="noreferrer noopener">British Antarctic Survey</a>.



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



The research team looked into several factors that influence ice flow, including <a href="https://www.earth.com/news/ocean-temperatures-are-rising-faster-than-expected-and-likely-to-accelerate/" target="_blank" rel="noreferrer noopener">ocean temperatures</a>, circulation changes, air temperature, and snowfall. 



They discovered that ice redirection is affecting the amount of ice reaching the floating ice shelves fed by these glaciers.



Two major ice shelves - the Crosson and <a href="https://www.earth.com/news/antarctica-ice-shapes-never-seen-by-humans-dotson-ice-shelf-ran-submersible/" target="_blank" rel="noreferrer noopener">Dotson</a> - are already among the fastest-changing outlets in West Antarctica. 



Crosson spans roughly 40 miles (60 kilometers), and Dotson stretches about 30 miles (48 kilometers). Both are thinning and retreating at their grounding lines.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/05/Antarctica_ice-piracy_Crosson-Dotson-Ice-Shelves_map_ESA_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/05/Antarctica_ice-piracy_Crosson-Dotson-Ice-Shelves_map_ESA_1s.webp" alt="The Crosson and Dotson Ice Shelves are situated in West Antarctica. These huge ice shelves are fed by numerous glaciers flowing towards the Amundsen Sea. Credit: ESA" class="wp-image-1969723"/></a><figcaption class="wp-element-caption">The Crosson and Dotson Ice Shelves are situated in West Antarctica. These huge ice shelves are fed by numerous glaciers flowing towards the Amundsen Sea. Click image to enlarge. Credit: ESA</figcaption></figure>



“The changes in flow direction have substantially altered the ice mass flux into Dotson and Crosson Ice Shelves, likely playing an important role in maintaining Dotson and accelerating the deterioration of Crosson," explained Professor Anna Hogg, co-author and Professor of Earth Observation at the University of Leeds.



“This suggests that ice flow redirection is an important new process in contemporary <a href="https://www.earth.com/news/ice-sheet-fracture-sets-a-speed-record-in-antarctica/" target="_blank" rel="noreferrer noopener">ice sheet dynamics</a>, which is required to understand present-day structural change in glaciers and the future evolution of these systems.”



<h2 class="wp-block-heading" id="h-ice-piracy-rising-seas-global-impacts">Ice piracy, rising seas, global impacts</h2>



The stakes are high. Sea levels are already rising due to climate change, and over 410 million people could be affected by coastal flooding by the year 2100. <a href="https://www.earth.com/news/global-sea-levels-spiked-dramatically-in-2023/" target="_blank" rel="noreferrer noopener">Global sea levels</a> have increased by more than 10 centimeters over the past decade.



“This new study highlights the unique ability of satellites to provide both the temporal and spatial coverage required to assess change in the polar regions,” remarked Dr. Martin Wearing, ESA Digital Twin Earth Scientist and Polar Science Cluster Coordinator.



Using data from Copernicus Sentinel-1 and ESA's Earth Explorer CryoSat, the team has revealed the complex evolution of ice flow in part of West Antarctica over the past few decades. 



Understanding these changing dynamics and what drives them is crucial for improved projections of future ice-sheet change and contributions to sea-level rise.



<h2 class="wp-block-heading" id="h-what-does-it-all-mean">What does it all mean?</h2>



To sum it all up, the <a href="https://www.earth.com/news/antarctic-ice-sheet-past-present-and-future/" target="_blank" rel="noreferrer noopener">Antarctic ice sheet</a> - once thought to be sluggish and stable over millennia - is changing much faster than we realized, and in unexpected ways. 



This discovery of "ice piracy" shows that glaciers can dynamically interact, competing for ice and rerouting flow like rivers shifting course, which completely reshapes how we model future sea-level rise.



If one glacier can weaken another by stealing its ice, entire ice systems may destabilize quicker than predicted, feeding more ice into the ocean and raising sea levels. 



In plain terms: Antarctica isn’t just melting - it’s reorganizing itself in ways that could have big consequences for coastal cities around the world.



-----



The study brought together experts from the University of Leeds, the <a href="https://www.bas.ac.uk/" target="_blank" rel="noreferrer noopener">British Antarctic Survey</a>, and the UK Centre for Polar Observation and Modelling (<a href="https://cpom.org.uk/" target="_blank" rel="noreferrer noopener">CPOM</a>), which is led from <a href="https://www.northumbria.ac.uk/" target="_blank" rel="noreferrer noopener">Northumbria University</a>. 



The full study was published in the journal <a href="https://tc.copernicus.org/articles/19/1725/2025/" target="_blank" rel="noreferrer noopener">The Cryosphere</a>.



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Ice piracy: Antarctic glacier discovered "stealing" ice from a neighbor, and that's not good for sea level rise

A new phenomenon dubbed "ice piracy" is unfolding in the...

Scientists have identified a previously overlooked set of stem cells inside our hair follicles, and it could be a game-changer for people who feel anxious about thinning hair. 



Their work highlights an area higher up in each follicle that appears to control the biological switch between silent and active hair growth phases.



<a href="https://med.virginia.edu/dermatology/faculty/lu-q-le-md-phd/" target="_blank" rel="noreferrer noopener">Lu Q. Le</a>, MD, PhD, from UVA’s <a href="https://med.virginia.edu/" target="_blank" rel="noreferrer noopener">School of Medicine</a> and his colleagues conducted this investigation to learn how these forgotten cells might prompt new follicles to become active once again.



They believe this finding opens the door for new techniques to address hair loss, but they emphasize that ongoing analysis is needed before final treatments reach the public.



<h2 class="wp-block-heading" id="h-stem-cell-hair-growth-triggers">Stem cell hair growth triggers</h2>



This newly recognized cell group sits in the upper and middle <a href="https://www.earth.com/news/scientists-discover-a-hidden-way-that-humans-feel-and-sense-touch/" target="_blank" rel="noreferrer noopener">sections of the follicle</a>. Researchers say these cells can renew themselves and produce various specialized offspring that participate in building new hairs.



Some were skeptical about whether follicle activity hinged on lesser-known compartments, but the team reported strong evidence that this region holds untapped power to spark hair regrowth. 



They found that, in lab settings, depleting these cells disrupted the natural cycle of replacing older <a href="https://www.earth.com/news/daily-dose-finasteride-magic-pill-regrows-hair-heals-prostate-boosts-heart-health/">hairs</a> with fresh strands.



<h2 class="wp-block-heading" id="h-why-this-matters-for-everyone">Why this matters for everyone</h2>



Some people view <a href="https://www.earth.com/news/new-natural-cure-male-baldness-highly-effective-sugar-2-deoxy-d-ribose/" target="_blank" rel="noreferrer noopener">hair thinning</a> as an inevitable rite of passage. Researchers suggest the presence of unique cells, which may be more responsive to therapy, gives fresh reason to think differently.



“It is our hope that these stem cells could one day provide a novel therapy for treating hair loss in people,” said Le. 



That goal remains on the horizon, but the concept has stirred excitement among scientists who study the biology of skin.



<h2 class="wp-block-heading" id="h-challenges-with-existing-therapies">Challenges with existing therapies</h2>



Typical solutions, such as over-the-counter <a href="https://www.ncbi.nlm.nih.gov/books/NBK482378/" target="_blank" rel="noreferrer noopener">creams</a> or prescription <a href="https://www.ncbi.nlm.nih.gov/books/NBK513329/" target="_blank" rel="noreferrer noopener">medications</a>, may improve only certain types of hair shedding. Many users also struggle with results that come slowly or plateau.



These new insights, however, add another target for investigation. Experts think that directing medical treatments toward lesser-studied follicle zones could bring more consistent or sustainable outcomes.



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



The most compelling twist is that these cells are still present in bald areas, even after hair shafts are long gone. That means the problem might not be total cell loss - it could be a matter of reactivating what’s already there.



Le’s team found that the upper follicle stem cells were still intact in human scalp samples taken from bald patients. 



This raises the possibility that with the right signals or drugs, these dormant cells might be coaxed into restarting the <a href="https://www.earth.com/news/beethovens-dna-reveals-unanswered-questions-about-his-death/">hair</a> cycle from scratch.



<h2 class="wp-block-heading" id="h-a-few-surprising-details">A few surprising details</h2>



Some of the earliest <a href="https://www.jci.org/articles/view/46307" target="_blank" rel="noreferrer noopener">tests</a> on mice, documented in the Journal of Clinical Investigation, showed that once these high-placed cells were taken away, hair shafts were lost in parts of the skin.



The animals also displayed disorganized follicles, hinting at a broader role these cells may have in preserving a healthy hair structure.



An earlier <a href="https://pubmed.ncbi.nlm.nih.gov/2203463/" target="_blank" rel="noreferrer noopener">paper</a> on skin growth patterns pointed out that multiple factors interact to dictate why certain patches produce hair vigorously while others stay dormant. 



With this new clue, researchers can look more carefully at what signals these newly identified cells send to the surrounding layers.



<h2 class="wp-block-heading" id="h-hair-stem-cells-and-the-future">Hair, stem cells, and the future</h2>



Scientists believe that maintaining or boosting the activity of these mid-follicle populations might guard against baldness. 



They are especially intrigued by how these cells might react if transplanted into areas that have gone quiet.



“We plan to fully investigate the potential of these stem cells in human hair follicles,” Le said. 



To get there, the team is examining human samples to see how often these cells remain in bald regions and whether they can be awakened.&nbsp;



<h2 class="wp-block-heading" id="h-next-steps-in-the-lab">Next steps in the lab</h2>



To understand how these cells behave over time, researchers are experimenting with different ways to trace their movements inside hair follicles. 



They’ve used genetically marked cells in mice to watch how the upper follicle stem cells migrate and change during the hair cycle.



This tracking helped confirm that these cells not only exist but also actively repopulate lower regions of the follicle, especially the bulge. 



That behavior is key, because the bulge has long been viewed as the main source of <a href="https://www.earth.com/news/intermittent-fasting-can-slow-hair-growth-but-it-also-has-many-positive-health-benefits/">hair</a> growth, and it now seems these newly discovered cells are its upstream supply.



<h2 class="wp-block-heading" id="h-hope-for-stem-cells-and-hair-loss">Hope for stem cells and hair loss</h2>



Public health data suggest millions of adults feel uneasy about hair-related changes. Stress, genetics, and medical conditions can all play a role, so there is no single fix that works across the board.



Researchers say this discovery adds another set of possibilities to that conversation. They believe a refined understanding of these mid-follicle cells will guide specialists toward a more targeted approach in the years ahead.



These findings show promise for those who want a new strategy that tackles hair loss at its roots. They also raise interesting questions about how our bodies control tissue renewal.



The study is published in the <a href="https://www.jci.org/articles/view/180160" target="_blank" rel="noreferrer noopener">Journal of Clinical Investigation</a>.



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Scientists discover hidden stem cells that could reactivate hair growth

Scientists have identified a previously overlooked set of stem cells...

Around six hundred million years ago, our planet almost lost the invisible shield that keeps its surface hospitable. Earth's magnetic field, generated by whirling molten iron deep below our feet, faded until it was so weak it was barely detectable.



At the same moment, oxygen flooded the oceans and <a href="https://www.earth.com/news/nitrogen-was-plentiful-for-early-life-on-earth/" target="_blank" rel="noreferrer noopener">atmosphere</a>, and curious soft-bodied creatures began sliding across the seafloor. The coincidence has fascinated geologists and biologists for decades.



Fresh measurements from ancient crystals now reveal just how close Earth came to a magnetic stall. They also strengthen the suspicion that a waning field set the stage for the rise of complex life. 



The new data trace a dramatic drop in magnetic intensity and help explain why the field later rebounded, saving Earth from becoming a dry, radiation-blasted rock like Mars.



<h2 class="wp-block-heading" id="h-earth-s-ancient-magnetic-field">Earth's ancient magnetic field</h2>



To read the planet’s magnetic diary, researchers collected grains of <a href="https://www.earth.com/news/earths-mantle-may-contain-a-wealth-of-green-metals/" target="_blank" rel="noreferrer noopener">pyroxenite and gabbro</a> from South Africa, Brazil, and Canada.



Each mineral contains microscopic iron needles that froze in alignment with the ambient field when the rocks cooled. 



By reheating single crystals in a carefully shielded furnace, the team coaxed out tiny magnetic signals that record field strength at the time of eruption.



After analyzing hundreds of crystals, <a href="https://www.rochester.edu/" target="_blank" rel="noreferrer noopener">University of Rochester</a> geophysicist John Tarduno and colleagues saw a clear pattern. 



“In general, the field is protective. If we had not had a field early in Earth history, water would have been stripped from the planet by the <a href="https://www.earth.com/news/silent-storms-experts-identify-the-mysterious-source-of-solar-wind/" target="_blank" rel="noreferrer noopener">solar wind</a> (a stream of energized particles flowing from the Sun toward Earth),” Tarduno explained.



“But in the Ediacaran, we had a fascinating period in the development of the deep Earth when processes creating the magnetic field … had become so inefficient after billions of years that the field almost completely collapsed.”



<h2 class="wp-block-heading" id="h-very-weak-magnetic-field">Very weak magnetic field</h2>



Crystals dated to 591 million years ago indicate a magnetic field about 30 times weaker than today - the most feeble long-term value ever measured. 



Follow-up samples show the enfeebled state persisted for at least 26 million years.



Before and after that window, rocks more than 2 billion years old and younger than 565 million years record a field as sturdy as the modern one, revealing just how exceptional the <a href="https://www.earth.com/news/ecosystem-behavior-earth-first-sea-creatures-stirring-water-drove-evolution/" target="_blank" rel="noreferrer noopener">Ediacaran lull</a> was.



During the low-field stretch, solar wind could punch far deeper into the atmosphere. Charged particles stripped away lightweight hydrogen, a process that left relatively heavy oxygen behind. 



The timing lines up with multiple geochemical markers that show a sharp increase in oxygen levels, supporting the idea that the weakened shield helped push Earth past a threshold needed for the development of <a href="https://www.earth.com/news/fossils-capture-a-turning-point-in-the-evolution-of-life/" target="_blank" rel="noreferrer noopener">large, mobile animals</a>.



<h2 class="wp-block-heading" id="h-thinner-armor-richer-air">Thinner armor, richer air</h2>



The atmospheric link also finds support from geobiologist Shuhai Xiao of <a href="https://www.vt.edu/" target="_blank" rel="noreferrer noopener">Virginia Tech</a>. 



“The <a href="https://www.earth.com/earthpedia-articles/earths-magnetic-field-origin-structure-and-impact-on-humanity/" target="_blank" rel="noreferrer noopener">magnetosphere shields the Earth</a> from solar wind, thus holding the atmosphere to the Earth. Thus, a weaker magnetosphere means that lighter gases such as hydrogen would be lost from the Earth’s atmosphere,” Xiao explained to CNN.



As hydrogen escaped, oxygen concentrations rose, allowing metabolism-hungry organisms to branch out.



Tarduno agrees that other processes - such as <a href="https://www.earth.com/news/dark-oxygen-discovery-deep-ocean-no-photosynthesis-baffles-scientists/" target="_blank" rel="noreferrer noopener">photosynthetic microbes</a> - were certainly at work.



“We do not challenge that one or more of these processes were happening concurrently. But the weak field may have allowed oxygenation to cross a threshold, aiding animal radiation (evolution),” he said.



<h2 class="wp-block-heading" id="h-magnetic-field-and-earth-s-core">Magnetic field and Earth's core</h2>



Rock records also solve a puzzle about when <a href="https://www.earth.com/news/earths-inner-core-is-not-solid-it-is-shape-shifting-time-for-textbooks-to-be-rewritten/" target="_blank" rel="noreferrer noopener">Earth’s inner core</a> began to form. Once field strength hit its nadir, it bounced back quickly.



“The observations appear to support the claim that the inner core first nucleated soon after this time, pushing the geodynamo (the mechanism that creates the magnetic field) from a weak, unstable state into a strong, stable dipolar field,” noted Peter Driscoll of the <a href="https://carnegiescience.edu/" target="_blank" rel="noreferrer noopener">Carnegie Institution for Science</a>. 



A solid seed at the center released extra heat, turbocharging convection in the outer core and restoring the magnetic screen.



<h2 class="wp-block-heading" id="h-strange-seafloor-pioneers">Strange seafloor pioneers</h2>



While the field flickered, the <a href="https://www.earth.com/news/earths-first-animals-were-very-picky-about-where-they-lived/" target="_blank" rel="noreferrer noopener">Ediacaran seas</a> hosted life forms unlike anything alive today.



Disk-shaped <a href="https://www.earth.com/news/rewrite-the-textbooks-life-on-earth-did-not-arise-due-to-increased-oxygen-levels/" target="_blank" rel="noreferrer noopener">Dickinsonia</a> spread as wide as 4.6 feet (1.4 meters) across the mud; quilted fronds waved gently in the currents; and slug-like Kimberella scraped microbial mats for food.



These pioneers vanished before the Cambrian period began, around 539 million years ago, but their brief reign proved that multicellular bodies could flourish once oxygen climbed to breathable levels.



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



Not every expert is convinced the magnetic dip directly influenced the course of evolution.



“It is hard for me to evaluate the veracity of this claim because the influence that planetary magnetic fields might have on climate is not very well understood,” Driscoll cautioned. 



Untangling all the variables - solar activity, mantle chemistry, biological innovation - will take years of careful detective work.



For now, the crystal record points to a simple narrative: Earth’s shield weakened, gases escaped, oxygen levels increased, and life took a bold new turn.



By tracing that chain of events, scientists gain insight into how planets and biospheres interact, a lesson that will guide the search for living worlds far beyond our own.



The full study was published in the journal <a href="https://www.nature.com/articles/s43247-024-01360-4" target="_blank" rel="noreferrer noopener">Communications, Earth and Environment</a>.



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Complex life emerged on Earth 591 million years ago, now scientists think they figured out how it happened

Around six hundred million years ago, our planet almost lost...

Scientists have proposed a new explanation for dark matter and how the elusive substance that anchors galaxies might have taken shape in the newborn universe.



The scenario begins with weightless particles zipping through the cosmic furnace and ends with a chill population of massive pairs that could still be drifting through space today.



The work - carried out by physicists at <a href="https://home.dartmouth.edu/" target="_blank" rel="noreferrer noopener">Dartmouth College</a> - offers predictions that astronomers can check against existing observations of the Cosmic Microwave Background, the after-glow of the <a href="https://www.earth.com/news/if-the-big-bang-theory-is-correct-what-exactly-happened/" target="_blank" rel="noreferrer noopener">Big Bang</a>.



<h2 class="wp-block-heading" id="h-particles-after-the-big-bang">Particles after the Big Bang </h2>



“Dark matter <a href="https://www.earth.com/news/existence-of-dark-matter-confirmed-by-new-study/" target="_blank" rel="noreferrer noopener">started its life</a> as near-massless relativistic particles, almost like light,” said Robert Caldwell, senior author of the study. “That’s totally antithetical to what dark matter is thought to be - it is cold lumps that give galaxies their mass.”



In the model designed by Caldwell and undergraduate researcher Guanming Liang, countless high-energy quanta filled the universe just after the Big Bang. These particles, similar to the photons that carry light, hurtled about at near-light speed.



Under certain conditions, two such quanta could lock together because their spins pointed in opposite directions, rather like the attraction between the north and south poles of tiny magnets. 



The moment they bonded, the new entity’s energy plummeted and its inertia skyrocketed. Within a flash it went from a racing ray to a hefty relic.



<h2 class="wp-block-heading" id="h-a-sudden-drop-in-energy"><a></a>A sudden drop in energy</h2>



“The most unexpected part of our mathematical model was the energy plummet that bridges the high-density energy and the lumpy low energy,” Liang explained.



The researchers liken the transformation to steam condensing into water - a hot, diffuse gas suddenly collapses into a cooler, denser phase.



“At that stage, it's like these pairs were getting ready to become dark matter,” Caldwell said. “This phase transition helps explain the abundance of dark matter we can detect today. It sprang from the high-density cluster of extremely energetic particles that was the <a href="https://www.earth.com/news/how-planets-formed-in-the-harsh-early-universe/" target="_blank" rel="noreferrer noopener">early universe</a>.”



<h2 class="wp-block-heading" id="h-cooper-pairs-as-a-clue"><a></a>Cooper pairs as a clue</h2>



The paper introduces a brand-new particle to trigger the shift, yet the authors argue that nature already provides a parallel. In certain superconducting metals, two <a href="https://www.earth.com/news/massless-dirac-electrons-seen-moving-in-four-dimensions/" target="_blank" rel="noreferrer noopener">electrons</a> with opposite spins form so-called Cooper pairs that glide without electrical resistance.



“We looked toward superconductivity for clues as to whether a certain interaction could cause energy to drop so suddenly,” Caldwell noted. “Cooper pairs prove that the mechanism exists.”



If the analogy holds, the relic pairs born in the cosmic dawn would have cooled into a nearly pressure-free state - a key hallmark of the unseen matter whose <a href="https://www.earth.com/news/theory-gravity-exists-without-mass-so-dark-matter-does-not-exist/" target="_blank" rel="noreferrer noopener">gravity</a> sculpts galaxies.



<h2 class="wp-block-heading" id="h-a-simple-model-for-dark-matter">A simple model for dark matter</h2>



Dark matter accounts for roughly eighty-five percent of all mass, yet the universe’s overall energy density has fallen dramatically since its first moments.



Liang points out that the new theory addresses both facts at once: “Structures get their mass due to the density of cold dark matter, but there also has to be a mechanism wherein energy density drops to close to what we see today.”



The abrupt condensation of massless quanta into massive pairs drains energy from the radiation budget while boosting the matter budget, squaring theory with observation.



“The mathematical model of our theory is really beautiful because it's rather simplistic - you don't need to build a lot of things into the system for it to work,” said Liang. “It builds on concepts and timelines we know exist.”



<h2 class="wp-block-heading" id="h-a-signature-written-in-ancient-light">A signature written in ancient light</h2>



Because the transition would have left the paired particles almost motionless, the team predicts a distinctive imprint on the <a href="https://www.earth.com/news/universe-more-complicated-less-clumpy-than-it-should-be-cosmic-microwave-background-cmb/" target="_blank" rel="noreferrer noopener">cosmic microwave background</a>.



The CMB has already been mapped by satellites and ground-based projects, and more precise surveys are under way at the Simons Observatory in Chile and in planned CMB Stage-4 experiments.



“It's exciting,” Caldwell said. “We're presenting a new approach to thinking about and possibly identifying dark matter.”



The researchers emphasize that their proposal is testable: if future CMB data reveal the subtle pattern predicted by their equations, the case for heavy pairs born from light-like quanta will strengthen. If not, the idea will need revision or replacement - exactly how science should proceed.



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



For now the paper stakes out a middle ground between theoretical elegance and observational reach. 



Upcoming missions will either expose the predicted CMB trace or tighten the limits on how dark matter could have formed. Either outcome will refine our view of the invisible framework that holds the <a href="https://www.earth.com/news/more-than-one-big-bang-may-explain-cosmic-expansion-without-dark-matter/" target="_blank" rel="noreferrer noopener">cosmos</a> together.



Should the ancient sky bear the scar of those primordial pairings, physicists might finally glimpse how ghostly matter traded light speed for lasting weight - and reshaped the universe in the process.



The study is published in the journal <a href="http://dx.doi.org/10.1103/PhysRevLett.134.191004" target="_blank" rel="noreferrer noopener">Physical Review Letters</a>.



Image Credit: NASA, ESA and M. Montes (University of New South Wales)



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Where did dark matter come from? The answer may be surprisingly simple

Scientists have proposed a new explanation for dark matter and...

Nearly half a century after its launch, NASA’s Voyager 1 has pulled off another feat of longevity. 



A team of researchers has reawakened a quartet of roll thrusters that went silent in 2004, restoring a crucial backup system just months before the only Earth antenna capable of sending Voyager commands goes offline for major upgrades.



The rescue, led by the <a href="https://www.jpl.nasa.gov/" target="_blank" rel="noreferrer noopener">Jet Propulsion Laboratory</a> (JPL), required forensic electronics work, split-second timing, and a dash of nerve - but the payoff could keep humanity’s most distant spacecraft talking to Earth for years to come.



<h2 class="wp-block-heading" id="h-voyager-1-s-roll-thrusters">Voyager 1's roll thrusters</h2>



<a href="https://www.earth.com/news/voyager-1-resumes-sending-data-to-earth-from-interstellar-space/" target="_blank" rel="noreferrer noopener">Voyager 1</a>, launched in 1977 and now more than 15 billion miles away, relies on thrusters to nudge its 12-foot antenna toward our planet. Among them is a special subset that controls “roll” - the rotation you’d see if you spun the spacecraft the way a record turns on a turntable. 



Roll keeps Voyager’s star tracker locked on a guide star; without that pinpoint reference, communications falter. Each Voyager carries a set of primary roll <a href="https://www.earth.com/news/spaceship-thruster-technology-fueled-by-any-type-of-metal-could-fly-indefinitely/" target="_blank" rel="noreferrer noopener">thrusters</a> and an identical backup set. 



Voyager 1’s primaries stopped firing in 2004 when two tiny heater circuits lost power, preventing the hydrazine fuel from staying warm enough to ignite. Engineers wrote them off and switched to the backups, confident they would last the few remaining years they thought the mission had left.



“I think at that time, the team was OK with accepting that the primary roll thrusters didn’t work, because they had a perfectly good backup,” noted Kareem Badaruddin, Voyager mission manager at JPL. “And, frankly, they probably didn’t think the Voyagers were going to keep going for another 20 years.”



But time crawled on, and a new threat appeared: residual deposits in the hydrazine feed lines began clogging the backup thrusters. Left unchecked, the buildup could choke them as early as autumn 2025. The mission needed another option, and that meant revisiting the “dead” thrusters.



<h2 class="wp-block-heading" id="h-diagnosing-a-20-year-old-malfunction"><a></a>Diagnosing a 20-year-old malfunction</h2>



Over months, JPL engineers dug into telemetry archives and wiring diagrams. They now suspect the heaters themselves never failed; instead, a glitch in the power-distribution circuitry may have flipped an internal switch, cutting electricity to the units.



If the team could send a carefully crafted command sequence to reset that switch, the heaters - and the thrusters - might live again.



The maneuver carried risk: as soon as heaters came back, the onboard software could interpret the roll attitude as out of tolerance and trigger an immediate thruster pulse. If that happened before fuel lines warmed, a small explosion was possible.



Flight controllers therefore had to point the star tracker with razor-sharp precision, minimizing any need for instant firing during the warm-up.



<h2 class="wp-block-heading" id="h-communication-capacity-in-deep-space">Communication capacity in deep space </h2>



An additional deadline loomed. On May 4, 2025, NASA began a ten-month overhaul of Deep Space Station 43 (DSS-43), the 70-meter dish in Canberra, Australia. 



DSS-43 is the only antenna with enough transmitting power to communicate with the Voyagers; when it is mostly offline, mission ops must make do with short command windows in August and December.



Suzanne Dodd is the Voyager project manager and head of <a href="https://www.nasa.gov/communicating-with-missions/dsn/" target="_blank" rel="noreferrer noopener">NASA’s Interplanetary Network</a>.



“These antenna upgrades are important for future crewed lunar landings, and they also increase communications capacity for our science missions in deep space, some of which are building on the discoveries Voyager made," said Dodd.



Still, the downtime meant Voyager 1 had to regain its lost thrusters before May or risk flying blind until 2026.



<h2 class="wp-block-heading" id="h-twenty-three-hours-of-suspense"><a></a>Twenty-three hours of suspense</h2>



Commands left Earth on 19 March. They would need 23 hours to cross <a href="https://www.earth.com/news/threads-of-the-universe-cosmic-web-revealed-in-unprecedented-detail/" target="_blank" rel="noreferrer noopener">interstellar space</a> at light speed; Voyager’s response would require another 23 hours to get back. 



On 20 March, the operations room lit up as telemetry lines revived. Within minutes, engineers saw a temperature spike in the heater sensors - exactly what they had hoped for.



“It was such a glorious moment. Team morale was very high that day,” said Todd Barber, propulsion lead at JPL.



“These thrusters were considered dead. And that was a legitimate conclusion. It’s just that one of our engineers had this insight that maybe there was this other possible cause and it was fixable. It was yet another miracle save for Voyager.”



<h2 class="wp-block-heading" id="h-what-the-revival-means"><a></a>What the revival means</h2>



The restored primaries will not replace the partially clogged backups immediately; instead, they provide redundancy should the backups fail during the Canberra outage.



If both sets eventually succumb to clogging, Voyager can still use a third group - trajectory-correction thrusters last employed during its planetary flybys - but those cannot perform roll control. By reviving the original roll pair, the team retains every possible option.



Voyager 1 and its twin, <a href="https://www.earth.com/news/nasa-lost-contact-with-voyager-2-spacecraft-12-billion-miles-away/" target="_blank" rel="noreferrer noopener">Voyager 2</a>, continue to return data on <a href="https://www.earth.com/news/deep-space-cosmic-rays-from-supernova-sparked-rapid-earth-evolution/" target="_blank" rel="noreferrer noopener">cosmic rays</a>, magnetic fields, and plasma density at the frontier of interstellar space. 



Each byte depends on precise antenna pointing, itself dependent on thrusters designed a long time ago. That they still answer the call reflects not only durable engineering but also the determination of the people tending them.



<h2 class="wp-block-heading" id="h-perseverance-of-voyager-1-thrusters">Perseverance of Voyager 1 thrusters</h2>



With power dwindling and instruments shutting down one by one, both Voyagers are on borrowed time. Yet each time a new hurdle emerges - whether frozen hydrazine or a communications blackout - engineers find a workaround. 



Their latest triumph keeps an aging explorer alive and embodies the mission’s ethos: never assume a component is beyond saving until every possibility has been exhausted. 



As Voyager 1 presses onward, its revived thrusters stand as a reminder that in space exploration, small victories can yield vast horizons - sometimes 15 billion miles wide.



The research was published by <a href="https://www.jpl.nasa.gov/news/nasas-voyager-1-revives-backup-thrusters-before-command-pause/" target="_blank" rel="noreferrer noopener">NASA</a>.



Image credit: NASA/JPL-Caltech



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Voyager 1's thrusters brought back to life after 21 years

Nearly half a century after its launch, NASA’s Voyager 1...

In Uganda’s Budongo Forest, chimpanzees are doing more than just surviving. They’re treating their wounds with plants, cleaning each other’s injuries, and pulling snares off their companions’ limbs. 



These behaviors, documented in a new study, hint at something profound. Perhaps the roots of human medicine run deeper than we thought.



Elodie Freymann, a researcher from the <a href="https://www.ox.ac.uk" target="_blank" rel="noreferrer noopener">University of Oxford</a> and the study’s lead author, believes these findings offer a fresh perspective on how our ancestors might have first learned to care for wounds. 



“<a href="https://www.earth.com/news/chimpanzees-mix-vocal-calls-to-create-new-meanings-like-humans/" target="_blank" rel="noreferrer noopener">Animals</a> are helping each other out. They’re capable of identifying others in need and then addressing those specific needs,” Freymann said.



<h2 class="wp-block-heading" id="h-how-chimpanzees-treat-wounds">How chimpanzees treat wounds</h2>



For eight months, researchers watched two chimpanzee communities in Budongo - Sonso and Waibira. Injuries were common, from bites and scratches to deadly snares left by humans.



In Sonso alone, nearly 40% of the chimps bore snare scars. Freymann and her team saw twelve injuries in Sonso and five in Waibira during the study period. The injured chimps weren’t just tending to their own wounds. They were also helping each other.



A male chimp named KT managed to pull a nylon snare off his wrist. Another <a href="https://www.earth.com/news/chimpanzees-use-rhythmic-drumming-to-communicate-in-forests/" target="_blank" rel="noreferrer noopener">chimpanzee</a>, HW, licked the wound of a female after she had been attacked. 



In yet another case, a juvenile female chewed leaves, dabbed them onto her mother’s wounds, then licked her fingers and pressed them onto the injured area. This behavior wasn’t isolated to relatives. In four instances, chimps helped others unrelated to them.



<h2 class="wp-block-heading" id="h-chimpanzees-recognize-medicinal-plants">Chimpanzees recognize medicinal plants </h2>



<a href="https://www.earth.com/news/what-wild-chimpanzees-can-teach-us-about-parenting/" target="_blank" rel="noreferrer noopener">Chimpanzees</a> don’t just grab any leaf when they get hurt. They seem to know which plants help wounds heal. 



Freymann’s team documented several plant species used in wound care. Acalypha sp., for example, is known for its antimicrobial properties. Pseudospondias microcarpa has a reputation for soothing pain and reducing inflammation.



One chimp chewed Acalypha leaves, then pressed the pulp onto a cut. Another used Lasiodiscus pervillei leaves to wipe away dirt and blood. 



A juvenile male named KO even mashed the stem bark of Argomuellera macrophylla and rubbed it into a wound on his leg. The behavior mirrored traditional African medicine, where these plants treat everything from skin infections to digestive issues.



“It’s likely that our shared common ancestor also would have been capable of these care behaviors as well,” Freymann noted. If chimps know which plants heal wounds, maybe early humans learned from them.



<h2 class="wp-block-heading" id="h-the-social-side-of-care">The social side of care</h2>



Prosocial care - helping others - is rare among non-human <a href="https://www.earth.com/news/chimpanzees-share-alcoholic-fruit-to-increase-social-bonding/" target="_blank" rel="noreferrer noopener">animals</a>. But Budongo’s chimps are doing it. During the study, researchers documented seven cases of one chimp helping another. In three of these instances, the caregiver and the injured chimp were unrelated.



A male chimp named ZG licked the blood off a female’s wound after she was attacked by other chimps. In another case, NT, a juvenile female, watched her mother chew leaves and press them onto a wound. NT then did the same, imitating her mother’s technique.



Freymann sees this as evidence that chimps aren’t just mimicking; they’re actively learning. 



“Our research helps illuminate the evolutionary roots of human medicine and healthcare systems,” said Freymann. “By documenting how chimpanzees identify and utilize medicinal plants and provide care to others, we gain insight into the cognitive and social foundations of human healthcare behaviors.”



<h2 class="wp-block-heading" id="h-threats-to-chimpanzee-healthcare">Threats to chimpanzee healthcare</h2>



Chimpanzees in Budongo face a constant threat from human snares. Nearly 40% of the Sonso chimps bear scars from these traps. 



Freymann’s team observed multiple instances of snare removal, some self-directed and others involving help from group members. But the danger remains.



The findings also suggest that chimpanzees in Budongo, Gabon, and other regions might share similar care behaviors. This could mean that these practices are widespread, not isolated. But there’s still much to learn.



For Freymann, the implications extend beyond chimpanzees and their use of plants. Observing how these primates use plants for healing might provide clues for new medicinal compounds. 



“If we want to hone in on these amazing medicinal resources, watching and learning from the animals is an incredibly effective way to do it if it’s done ethically and responsibly,” she said.



<h2 class="wp-block-heading" id="h-learning-plant-medicine-from-chimpanzees">Learning plant medicine from chimpanzees</h2>



The study doesn’t just document chimpanzee healthcare. It challenges how we think about the origins of medicine. Watching chimps chew leaves and press them onto wounds, it’s easy to imagine early humans doing the same. Maybe they learned from the chimps. Maybe they figured it out together.



Budongo’s chimpanzees aren’t doctors, but they are healers. And in their actions, we might find the echoes of our own ancient medical traditions.



Freymann’s work reminds us that medicine is not just a human invention. It might be a shared legacy, passed down from ancestors who walked the forests long before us.



The study is published in the journal <a href="https://www.frontiersin.org/journals/ecology-and-evolution/articles/10.3389/fevo.2025.1540922/full" target="_blank" rel="noreferrer noopener">Frontiers in Evolution and Ecology</a>.



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Chimpanzees know which plants to use for healing wounds

In Uganda’s Budongo Forest, chimpanzees are doing more than just...

Scientists have detected oxygen in a galaxy so distant that its light traveled for 13.4 billion years to reach us. This discovery offers an exciting peek back into cosmic events that happened only a few hundred million years after everything got started.



The researchers say it is the most faraway system confirmed to show such atomic signals, highlighting the power of advanced telescopes that work together. They also identified intense star formation and a relatively low level of heavier elements.



<h2 class="wp-block-heading" id="h-scanning-the-galaxy-for-oxygen">Scanning the galaxy for oxygen</h2>



Jorge Zavala, an astronomer at the East Asian <a href="https://public.nrao.edu/telescopes/alma/" target="_blank" rel="noreferrer noopener">ALMA</a> Regional Center at the National Astronomical Observatory of Japan, played a key role in this effort.



“We pointed the more than forty 12-m antennas of the Atacama Large Millimeter/submillimeter Array (ALMA) and the 6.5-m James Webb Space Telescope (JWST) for several hours at a sky position that would appear totally empty to the naked human eye," said Zavala.



The goal was to catch a signal from one of the most distant astronomical objects known to date, he noted. 



The team successfully detected the emission from excited atoms of different elements such as hydrogen and oxygen. These emissions give scientists a clue about the materials that built the earliest stars.



<h2 class="wp-block-heading" id="h-unusual-conditions-for-a-galaxy">Unusual conditions for a galaxy</h2>



The galaxy, called <a href="https://arxiv.org/abs/2403.10238" target="_blank" rel="noreferrer noopener">GHZ2</a>, has a mass of a few hundred million times our Sun but appears to fit into a region only a few hundred light-years across. 



That density might resemble what is seen in tight star clusters, which sparks questions about how such crowded structures formed so early in the universe's history.



The metallicity - the portion of heavier elements - is around one-tenth of what we find in our Sun’s neighborhood. That is not surprising for something that appeared when the universe was still young; yet it shows that metals built up faster than initially expected.



<h2 class="wp-block-heading" id="h-bursts-of-star-formation">Bursts of star formation </h2>



Hot, short-lived stars dominate this object, which explains its brilliant shine and unusual energy signature. 



The radiation of the stars is strong enough to generate elements across the galaxy such as ionized oxygen and hydrogen. It shines in a way that intrigues astronomers who compare it to star <a href="http://earth.com/news/four-small-planets-discovered-orbiting-the-nearest-single-star-to-earth-barnards-star/" target="_blank" rel="noreferrer noopener">factories </a>in far more mature galaxies.



Observations indicate that star birth happens quickly in that environment, indicating a burst-like cycle rather than a slow pace. 



Many think these flurries of activity involving oxygen happened more frequently in the ancient universe, which possibly accounts for how certain galaxies grew so large, so rapidly.



<h2 class="wp-block-heading" id="h-possible-clues-to-star-clusters">Possible clues to star clusters</h2>



Studies suggest that GHZ2 might hold insights into the origin of <a href="https://esahubble.org/wordbank/globular-cluster/" target="_blank" rel="noreferrer noopener">globular clusters</a>, which are long-lived, tightly packed groups of stars. 



Some of these features, such as similar element patterns and high-density populations, echo what we see in those clusters inside 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>.



Researchers are still evaluating whether galaxies like GHZ2 might have seeded these ancient stellar gatherings. If so, it could fill a major gap in astrophysics by explaining how such clusters emerged.



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



Tom Bakx is an astronomer at <a href="https://www.chalmers.se/" target="_blank" rel="noreferrer noopener">Chalmers University</a> in Sweden, and former researcher at Nagoya University.



“This study is a crown on the multi-year endeavor to understand galaxies in the early Universe,” said Bakx. "Additional telescope time will be key to investigating how metals, star formation, and black holes evolved in the early universe."



The analysis of multiple emission lines enabled several key tests of galaxy <a href="https://www.earth.com/news/messier-33-m33-unusual-galaxy-without-central-black-hole/" target="_blank" rel="noreferrer noopener">properties</a>, and demonstrated the capabilities of ALMA through a synergy of telescopes like the JWST. 



The researchers explained that current results open the door to deeper inquiries into the dawn of galaxy <a href="https://www.earth.com/news/hidden-galaxies-discovery-would-upend-current-understanding-of-universe/" target="_blank" rel="noreferrer noopener">assembly</a>.&nbsp;



<h2 class="wp-block-heading" id="h-oxygen-detection-in-galaxies">Oxygen detection in galaxies</h2>



Experts also note that each new detection highlights the advantage of combining data from tools that specialize in imaging at different wavelengths. 



By merging radio and infrared observations, researchers can unravel the building blocks of galaxies that thrived only a few hundred million years after everything began.



Scientists have now turned their focus to capturing additional emission lines that could reveal the structure and chemistry of these distant systems. Those signals may shed light on black hole growth patterns, as well as the cosmic influences that shaped large-scale structures.



Eventually, a more complete picture of the early universe could clarify how stars and <a href="https://www.earth.com/news/runaway-star-may-be-dragging-a-planet-along-with-it/" target="_blank" rel="noreferrer noopener">clusters</a> formed under harsh conditions. Although it sounds challenging, every new breakthrough brings us closer to understanding how galaxies grew from humble beginnings.



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



GHZ2 stands out as a reminder that cosmic evolution took off at a swift pace. Researchers believe similar objects might still lie undiscovered, waiting to add new pieces to the puzzle.



This analysis signals a big leap in pinpointing when and how the earliest stellar communities arose. Scientists hope that follow-up observations will confirm details about the galaxy’s structure and oxygen's role in cosmic history.



The study is published in the journal <a href="https://www.nature.com/articles/s41550-024-02397-3" target="_blank" rel="noreferrer noopener">Nature Astronomy</a>.



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Oxygen detected in the most distant and primitive galaxy ever analyzed

Scientists have detected oxygen in a galaxy so distant that...

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.



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



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



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



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



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



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



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



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

Is chocolate the next nutritional powerhouse?

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

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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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

Flu viruses are more flexible than expected

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



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



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



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



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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

Detecting mercury contamination with the tap of a finger

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



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



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



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



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



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



Video/ Image Credit: European Space Agency&nbsp;



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



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

Kainji Lake in north central Nigeria

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