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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Hubble spotlights galaxies in the constellation Virgo

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

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA



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Ghostly galaxy in the constellation Eridanus

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA



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Rosetta Nebula: Sculpted by starlight over millions of years

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA/ESA Hubble Space Telescope



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Secrets of a spiraling galactic powerhouse

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

Headshot,Of,Ant,Orange,In,The,Argentine,Jungle.,(linepithema,Humile)

Ants march across sidewalks and kitchen counters as if they own the place. They cross oceans inside cargo ships, set up vast super-colonies, and push out native species on six continents. 



Once a <a href="https://www.earth.com/news/how-many-ants-live-on-earth-at-any-point-in-time-total-number-is-astounding/" target="_blank" rel="noreferrer noopener">nest of ants</a> settles in, homeowners and farmers often reach for poison baits, yet the insects lose interest before enough of them carry the toxic treat back home. 



A new study suggests that a tiny splash of caffeine could keep the party going - and give pest managers an edge.



The research shows that moderate doses of caffeine sharpen an ant’s memory for the bait’s location. Ants that sipped a caffeinated sugar drop found it again more quickly on later trips, leaving a stronger scent trail for nest-mates. 



The discovery points to a low-cost tweak that might finally turn the <a href="https://www.earth.com/news/ants-perform-life-saving-amputation-surgeries-on-injured-nest-mates/" target="_blank" rel="noreferrer noopener">invader’s own teamwork</a> against it.



<h2 class="wp-block-heading" id="h-tiny-ant-huge-impact">Tiny ant, huge impact</h2>



The Argentine ant (Linepithema humile) is only about one-tenth of an inch long, yet its cooperative spirit builds super-colonies stretching thousands of miles along the Mediterranean coast and the U.S. West Coast. 



Those armies displace local insects, rob hummingbird feeders, and even short-circuit electrical gear. 



Recent economic analyses peg the global cost of <a href="https://www.earth.com/news/ants-are-shifting-to-new-habitats-to-cope-with-climate-change/" target="_blank" rel="noreferrer noopener">invasive ants</a> - including crop losses and control bills - at billions of dollars each year. No wonder pest crews keep searching for smarter tactics.



<h2 class="wp-block-heading" id="h-giving-caffeine-to-ants">Giving caffeine to ants</h2>



To find out, researchers set up a miniature arena: a Lego drawbridge led each ant onto a letter-size acrylic platform where a single sugar drop waited. 



Some drops carried no additive, while others contained 25 parts per million (ppm), 250 ppm, or 2 000 ppm of caffeine. One hundred forty-two ants took part, and each explorer tackled the course four times.



“The idea with this project was to find some cognitive way of getting the ants to consume more of the poisonous baits we put in the field,” says the study’s first author Henrique Galante, a computational biologist at the <a href="https://www.uni-regensburg.de/en" target="_blank" rel="noreferrer noopener">University of Regensburg</a>. 



Automated cameras tracked every step, logging travel time and the straightness of each path. Without caffeine, the insects wandered, needing the same span to reach the treat on every attempt. Add a modest stimulant, and the story changed.



<h2 class="wp-block-heading" id="h-caffeine-gives-ant-focus-not-speed">Caffeine gives ant focus, not speed</h2>



“We found that intermediate <a href="https://www.earth.com/news/caffeine-evolution-in-plants-the-surprising-story-of-yerba-mate/" target="_blank" rel="noreferrer noopener">doses of caffeine</a> actually boost learning - when you give them a bit of caffeine, it pushes them into having straighter paths and being able to reach the reward faster," Galante explained.



In fact, ants that tasted 25 ppm caffeine shaved 28 percent off their foraging time on every return. Those on 250 ppm cut the clock by 38 percent. 



Picture an individual that spent 300 seconds during its first outing - it would need just 113 seconds after three more trips on the lower dose and 54 seconds on the medium dose.



<a href="https://www.earth.com/news/caffeine-consumption-may-lower-the-risk-of-dementia/" target="_blank" rel="noreferrer noopener">The stimulant</a> did not act like an energy drink. There was no uptick in raw speed. “What we see is that they're not moving faster, they're just being more focused on where they're going,” Galante noted. 



“This suggests that they know where they want to go, therefore, they have learned the locations of the reward.” 



Only path geometry tightened; pace stayed the same. At the heaviest 2 000 ppm dose - the level that kills half of honeybees in tests - the learning advantage disappeared.



<h2 class="wp-block-heading" id="h-sharper-trails-deadlier-bait">Sharper trails, deadlier bait</h2>



Argentine ants rely on <a href="https://www.earth.com/news/ants-are-now-using-cars-to-travel-spread-to-new-locations/" target="_blank" rel="noreferrer noopener">pheromone highways</a>. A worker that discovers food drags its stinger along the ground, laying a chemical breadcrumb trail that guides the next shift. Faster relearning multiplies that effect. 



“We're trying to make them better at finding these baits, because the faster they go and come back to them, the more pheromone trails they lay, the <a href="https://www.earth.com/news/evolutionary-deja-vu-the-symbiotic-relationships-of-trees-and-ants/" target="_blank" rel="noreferrer noopener">more ants will come</a>, and, therefore, the faster they will spread the poison in the colony before they realize it's poison,” Galante continued.



Adding caffeine could also slash the waste that now limits bait stations. In neighborhoods and orchards, technicians often replenish gels every few days because the first wave of foragers gives up. 



A caffeinated lure might stay attractive long enough for queens and larvae to receive a lethal serving.



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



The team is already field-testing the recipe at infested sites in Spain. They also plan to check whether caffeine interacts with common active ingredients such as hydramethylnon or spinosad. 



“The lowest dose we used is what you find in natural plants, the intermediate dose is similar to what you would find in some energy drinks, and the highest amount is set to be the LD50 of bees - where half the bees fed this dose die - so it's likely to be quite toxic for them,” Galante notes. 



Selecting a concentration that boosts memory without harming pollinators will be crucial.



Caffeine’s appeal extends beyond Argentine ants. Other <a href="https://www.earth.com/news/dirt-ants-were-once-masters-of-disguise-in-the-caribbean/" target="_blank" rel="noreferrer noopener">invasive species</a> - including fire ants and big-headed ants - share the same food-sharing habits that make baiting tricky. 



If the stimulant nudges their neural circuits in a similar way, managers could deploy a single additive across multiple pest fronts.



<h2 class="wp-block-heading" id="h-what-we-learned-about-ants-and-caffeine">What we learned about ants and caffeine</h2>



To sum it all up, caffeine improves ants' overall focus and learning without increasing speed, allowing them to navigate straighter paths and lay stronger pheromone trails. 



This effect boosts the effectiveness of bait traps, leading more ants to the poison and increasing the chances of it spreading through the colony. 



However, the benefit peaks at moderate doses - very high levels eliminate the learning advantage and can be toxic. So, overall, caffeine makes ants better at foraging and sharing, which ironically makes them more vulnerable to well-designed pest control strategies.



For now, the message is simple: a dash of coffee in the buffet may turn an army’s fabled navigation skills against itself. When the ants get better at remembering dessert, the colony’s days could finally be numbered.



The full study was published in the journal <a href="https://www.cell.com/iscience/fulltext/S2589-0042(24)01157-X" target="_blank" rel="noreferrer noopener">iScience</a>.



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When you give caffeine to ants, many interesting things happen

Ants march across sidewalks and kitchen counters as if they...

Orange cats are everywhere, from the iconic character Garfield to the independent tabby lounging in the sun. But what gives orange cats their signature color? For decades, the answer remained a mystery to scientists.



Now, researchers at <a href="https://www.med.stanford.edu" target="_blank" rel="noreferrer noopener">Stanford Medicine</a> and <a href="https://www.kyushu-u.ac.jp/en/" target="_blank" rel="noreferrer noopener">Kyushu University</a> have cracked the code. The answer lies in a gene called Arhgap36. This gene behaves strangely in orange cats, turning their fur a vivid shade of orange.



<h2 class="wp-block-heading" id="h-why-orange-cats-are-rare">Why orange cats are rare</h2>



Scientists have known for years that the orange trait in cats is linked to the X chromosome. Male cats, with their single X chromosome, only need one copy of the gene to flaunt their ginger fur. 



Females, however, require two copies to be completely orange. Otherwise, they become calicos or tortoiseshells, their fur a patchwork of orange, black, and white.



“In a number of <a href="https://www.earth.com/news/bengal-cats-wild-appearance-is-surprisingly-tied-to-domestic-cats/" target="_blank" rel="noreferrer noopener">species</a> that have yellow or orange pigment, those mutations almost exclusively occur in one of two genes, and neither of those genes are sex-linked,” explained Christopher Kaelin, a senior scientist in genetics and lead author of the study.



<h2 class="wp-block-heading" id="h-genetic-mystery-of-cat-colors">Genetic mystery of cat colors</h2>



Kaelin and his team had a hunch the answer was related to the X chromosome. But which gene? They collected DNA samples from spay and neuter clinics, comparing orange cats to non-orange cats. 



After analyzing the genomes, the researchers found 51 genetic variants that could explain the orange trait. They narrowed it down to three. 



One stood out: Arhgap36. A tiny deletion in this gene cranked up its activity in pigment cells. Normally, Arhgap36 keeps a low profile, mainly operating in nerve tissues and cancer cells. But in orange cats, it’s louder than a kitten demanding breakfast.



“Arhgap36 is not expressed in mouse pigment cells, in human pigment cells or in cat pigment cells from non-orange cats,” Kaelin said. 



“The mutation in orange cats seems to turn on Arhgap36 expression in a cell type, the pigment cell, where it’s not normally expressed.”



<h2 class="wp-block-heading" id="h-orange-cats-are-usually-male">Orange cats are usually male</h2>



Orange cats are predominantly male, and it all comes down to the X chromosome. Males have one X and one Y chromosome. If that X carries the orange gene, they’re entirely orange. 



Females, with two X chromosomes, need the orange <a href="https://www.earth.com/news/discovery-evolution-not-random-gene-families-pangenome-influence-called-revolutionary/" target="_blank" rel="noreferrer noopener">gene</a> on both to sport a solid ginger coat. If a female inherits only one copy, she becomes a mosaic of orange and black.



This randomness creates the striking tortoiseshell and calico patterns. Some cells activate the orange gene, while others activate the black gene. The result? A coat that’s as unpredictable as a cat’s mood.



<h2 class="wp-block-heading" id="h-a-shared-genetic-breakthrough">A shared genetic breakthrough</h2>



While Stanford scientists zeroed in on Arhgap36, researchers at Kyushu University pursued a parallel investigation. Professor Hiroyuki Sasaki and his team examined DNA from 18 cats including 10 that were orange. The findings matched those at Stanford.



“This was such strong evidence that even at this stage, we were confident that Arhgap36 was the orange gene,” said Sasaki.



The researchers expanded their study, analyzing <a href="https://www.earth.com/news/everyday-dna-damage-requires-constant-repair-by-cells-to-prevent-disease/" target="_blank" rel="noreferrer noopener">DNA</a> from 49 more cats, and the same pattern emerged. The Arhgap36 deletion consistently appeared in orange cats but not in others.



<h2 class="wp-block-heading" id="h-origins-of-orange-fur">Origins of orange fur</h2>



Where did this mutation come from? Kaelin believes it emerged early in domestication. Ancient paintings dating back to the 12th century depict calico cats, suggesting the mutation is centuries old.



“This is something that arose in the domestic cat, probably early on in the domestication process,” Kaelin said.



Sasaki wants to dig deeper. He plans to study ancient Egyptian cat mummies, searching for the orange gene. The goal? To pinpoint when and where the mutation first appeared.



<h2 class="wp-block-heading" id="h-looking-at-the-gene-beyond-fur">Looking at the gene beyond fur</h2>



Arhgap36 isn’t just about orange fur. In other animals, it’s linked to cancer and nerve development. Could it affect more than just a cat’s coat? Sasaki thinks so.



“For example, many cat owners swear by the idea that different coat colors and patterns are linked with different personalities,” he said. “There’s no scientific evidence for this yet, but it’s an intriguing idea and one I’d love to explore further.”



The gene could also impact brain and <a href="https://www.earth.com/news/oxytocin-holds-the-keys-to-both-your-heart-and-your-memory/" target="_blank" rel="noreferrer noopener">hormone</a> function. Sasaki’s team found the gene active in several tissues, not just skin cells. Whether this activity alters behavior or health is still a mystery.



The discovery of Arhgap36 as the orange gene is just the beginning. Sasaki and Kaelin plan to investigate how the gene influences pigment production. 



The experts are also exploring its role in cancer and skin conditions, hoping to uncover broader implications for both cats and humans.



<h2 class="wp-block-heading" id="h-orange-cat-mystery-solved">Orange cat mystery solved</h2>



For over a century, the orange gene remained a mystery, hiding in plain sight. Now, with the discovery of Arhgap36, scientists are one step closer to understanding how cats get their colors. But the story isn’t over.



Sasaki’s ultimate goal is to recreate the mutation in cat cell cultures, observing its effects in real time. Meanwhile, Kaelin wants to map out the entire molecular pathway, tracing how a simple gene deletion transforms a basic pigment cell into a beacon of orange fur.



From the dusty streets of ancient Egypt to the modern lab, orange cats have carried this genetic quirk for centuries. And as researchers continue to peel back the layers of DNA, the secrets of these fiery felines may prove to be more profound than anyone imagined.



The study is published in the journal <a href="https://www.cell.com/current-biology/fulltext/S0960-9822(25)00391-4" target="_blank" rel="noreferrer noopener">Current Biology</a>.



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Why are some cats orange? Scientists have finally found the answer

Orange cats are everywhere, from the iconic character Garfield to...

A colossal burst of solar radiation struck Earth 14,300 years ago, showering the planet with high-energy particles and leaving behind an unmistakable spike in radiocarbon. Until now, scientists could not gauge the true scale of that ancient storm.



A newly developed chemistry-climate model, SOCOL:14C-Ex, has changed that - showing the Ice-Age event to be the <a href="https://www.earth.com/news/strong-geomagnetic-solar-storm-alert-issued-auroras-expected-farther-south/" target="_blank" rel="noreferrer noopener">most intense</a> solar storm ever identified. It was 18 percent stronger than the famous AD 775 outburst and more than 500 times the power of any particle storm recorded by modern satellites.



<h2 class="wp-block-heading" id="h-hidden-signals-in-tree-rings">Hidden signals in tree rings</h2>



Researchers first noticed an abrupt jump in radiocarbon (14C) concentrations for the year 12350 BCE when they analyzed larch trunks preserved beneath Alpine glaciers. 



Such sharp rises, called Miyake events, occur when torrents of charged particles collide with the upper atmosphere, supercharging the natural production of cosmogenic isotopes.



Similar spikes near 775 CE and 994 CE have already revolutionized archaeological dating. The <a href="https://www.earth.com/news/ice-age-climate-shifts-changed-early-human-migration-patterns/" target="_blank" rel="noreferrer noopener">Ice-Age</a> signal, however, lay outside the warm-climate Holocene epoch, and existing models could not simulate isotope chemistry under glacial conditions.



That impasse motivated postdoctoral scientist Kseniia Golubenko and professor Ilya Usoskin at the <a href="https://www.oulu.fi/en" target="_blank" rel="noreferrer noopener">University of Oulu</a>, Finland, to create SOCOL:14C-Ex. 



The model couples atmospheric circulation, photochemistry, and radiocarbon pathways, then plugs in ancient ice-sheet boundaries, lower sea levels and a weaker geomagnetic field. Validated against the well-studied CE 775 event, the framework was ready for the Late-Glacial mystery.



<h2 class="wp-block-heading" id="h-quantifying-the-ice-age-blast">Quantifying the Ice Age blast</h2>



Running the 12350 BC data through SOCOL:14C-Ex revealed particle fluxes dwarfing anything in the satellite era.



“Compared to the largest event of the modern satellite era - the 2005 particle storm - the ancient 12350 BCE event was over 500 times more intense, according to our estimates,” Golubenko said. 



The model puts the radiation spike 18 percent above the CE 775 benchmark, establishing a new solar ceiling. Other intense solar storms are known - around 663 BCE, 5259 BCE and 7176 BCE - yet none match this Ice-Age titan.



“The ancient event in 12350 BCE is the only known extreme solar particle event outside of the Holocene epoch, the past ~12000 years of stable warm climate,” Golubenko stated. That fact alone widens the time frame scientists must consider when assessing solar variability.



<h2 class="wp-block-heading" id="h-a-tool-for-radiocarbon-dating">A tool for radiocarbon dating</h2>



Radiocarbon researchers often struggle to convert “floating” chronologies - relative sequences with no fixed calendar anchor - into absolute timelines. Sudden global 14C surges are perfect anchors.



“Miyake events allow us to pin down exact calendar years in floating archaeological chronologies,” Usoskin explained. 



The new Late-Glacial marker could help synchronize disparate records from the waning Ice Age: cave-paint dates, retreating ice margins, even megafaunal <a href="https://www.earth.com/news/at-least-two-of-earths-mass-extinctions-caused-by-massive-supernova-explosions/" target="_blank" rel="noreferrer noopener">extinctions</a>.



SOCOL:14C-Ex also frees scientists from the Holocene boundary, letting them mine older wood, peat, and stalagmite archives for yet-undetected spikes. The possibility of mapping a full 30,000-year record of solar storms has now moved within reach.



<h2 class="wp-block-heading" id="h-risks-of-intense-solar-storms">Risks of intense solar storms </h2>



Until this study, theorists debated whether the AD 775 storm represented a physical upper limit for solar particle acceleration. The Ice-Age event proves the Sun can exceed that benchmark.



“This event establishes a new worst-case scenario,” Golubenko noted. “Understanding its scale is critical for evaluating the risks posed by future solar storms to modern infrastructure like satellites, power grids, and communication systems.”



Modern civilization has never faced anything close to the Ice-Age blast. The 1989 Quebec blackout came from a geomagnetic storm far weaker; the Carrington flare of 1859, often cited as a dire warning, did not involve a massive particle shower. 



A repeat of the 12350 BCE storm today could cripple <a href="https://www.earth.com/news/burning-up-of-satellites-severely-harms-ozone-recovery/" target="_blank" rel="noreferrer noopener">satellite constellations</a>, corrupt navigation signals, and overload long-distance transmission lines.



<h2 class="wp-block-heading" id="h-a-collaborative-effort-across-disciplines"><a></a>A collaborative effort across disciplines</h2>



The study  brings together geophysicists, atmospheric chemists and dendrochronologists from Finland, France, and Switzerland under the leadership of Edouard Bard of the <a href="https://www.cerege.fr/en/" target="_blank" rel="noreferrer noopener">CEREGE</a>. 



The research blended laboratory isotope measurements, supercomputer modeling, and cross-checks against newly unearthed timber from the French Alps.



After confirming the Ice-Age spike’s magnitude, the team calculated its climatic footprint. Although the particle deluge doubled stratospheric ionization rates for months, temperature effects appear minimal, mirroring results from younger Miyake events. 



The principal legacy is the radiocarbon “barcode” now locked into prehistoric archives worldwide.



<h2 class="wp-block-heading" id="h-hunting-for-older-solar-storms">Hunting for older solar storms</h2>



With SOCOL:14C-Ex validated for glacial settings, Golubenko and colleagues plan to scan older growth rings and polar ice for further anomalies. Each discovery will refine models of solar dynamics and help planners gauge the rare but existential threat posed by extreme <a href="https://www.earth.com/news/space-weather-poses-significant-risks-to-railway-safety/" target="_blank" rel="noreferrer noopener">space weather</a>.



“Our new model lifts the existing limitation to the Holocene and extends our ability to analyze radiocarbon data even for glacial climate conditions.” 



Armed with that capability, scientists can now track the Sun’s wildest moods across multiple ice ages, offering both a clearer view of our star’s potential and a sterner test for the resilience of modern technology.



The study is published in the journal <a href="https://www.sciencedirect.com/science/article/pii/S0012821X25001827?via%3Dihub" target="_blank" rel="noreferrer noopener">Earth and Planetary Science Letters</a>.



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Most intense solar storm ever recorded hit Earth 14,300 years ago

A colossal burst of solar radiation struck Earth 14,300 years...

Rays,Of,Light,Passing,Through,Cyberspace.,Communication,Network,Concept.

At the scale of atoms and electrons, walls are not always walls. A particle that lacks the energy to climb a barrier can still appear on the far side, a curiosity known as “quantum tunneling.” 



In the heart of the Sun, this quirk lets hydrogen nuclei fuse quickly enough to keep daylight streaming toward Earth.



Physicists have puzzled over how long the hop through the barrier actually takes. Some experiments hinted that the leap happens so swiftly that it appears <a href="https://www.earth.com/news/dark-matter-may-consist-of-particles-that-travel-faster-than-light/" target="_blank" rel="noreferrer noopener">faster than light</a>, brushing against the limits set by Einstein’s special relativity. 



Others clocked a small but finite delay. The debate has rolled on because time, slippery even in classical physics, becomes downright elusive in the quantum world.



<h2 class="wp-block-heading" id="h-quantum-tunneling-defies-classical-limits">Quantum tunneling defies classical limits</h2>



Classical rules say a baseball that can’t clear a fence bounces back, end of story. In the <a href="https://www.earth.com/news/how-faster-than-light-tachyons-fit-into-the-special-theory-of-relativity/" target="_blank" rel="noreferrer noopener">quantum picture</a>, particles behave as waves that seep into and even through obstacles. 



A sliver of the wave survives inside the forbidden zone, giving the particle a genuine chance to show up on the other side. 



Engineers tap that chance in flash memory, Josephson junctions, and scanning tunneling microscopes that map surfaces atom by atom.



Because the <a href="https://www.earth.com/news/dark-photon-theory-casts-doubt-on-double-slit-experiment-quantum-light-interference-pattern/" target="_blank" rel="noreferrer noopener">wave spreads out</a>, deciding where to mark the particle’s position is tricky. 



Earlier timing experiments fixed on the crest of the outgoing wave and reported that the particle covered more ground than a free-flying counterpart in the same span, implying superluminal travel. 



Those results stirred excitement but also skepticism, as the crest is a moving pattern, not a point-like traveler.



<h2 class="wp-block-heading" id="h-trying-to-define-time">Trying to define "time"</h2>



Physicists Patrik Schach and Enno Giese of <a href="https://www.tu-darmstadt.de/index.en.jsp" target="_blank" rel="noreferrer noopener">TU Darmstadt</a> think the stopwatch itself was misread. “But the particle does not follow a path in the classical sense,” objects Giese. 



If you can’t pin down where the traveler is, measuring when it arrives gets murky. Instead of treating the atom as a marble darting through a tunnel, the pair propose using the atom as its own clock.



Their design, outlined in Science Advances, borrows a page from atomic timekeeping. They prepare each atom in a blend of two <a href="https://www.earth.com/news/quantum-oddity-points-to-new-class-of-subatomic-particles-fractional-charges-excitons/" target="_blank" rel="noreferrer noopener">internal energy states</a> and send it toward an optical barrier. 



With a technique akin to a Ramsey sequence, the two states tick against each other while the atom either tunnels or reflects. A reference atom that faces no barrier runs alongside, giving a direct comparison.



<h2 class="wp-block-heading" id="h-pocket-watches-and-quantum-tunnels">Pocket watches and quantum tunnels</h2>



“Time is what you read off a clock.” Einstein’s quip fits snugly here. The oscillation between the two energy levels works like a wristwatch small enough to ride the atom. 



If tunneling slows the tick, the phase between the levels shifts. Detecting that shift after a second laser pulse reveals how much time elapsed during the barrier encounter.



Calculations show the tunneled clock lags by about 10^-26 seconds - roughly a hundred septillionths of a second. That delay, though vanishingly small, is measurable with clouds of <a href="https://www.earth.com/news/edge-state-atoms-how-electrons-find-their-groove-in-frictionless-flow/" target="_blank" rel="noreferrer noopener">ultracold atoms</a> whose collective signal boosts sensitivity. 



The approach dodges the need to guess where the particle is at each instant and stays faithful to quantum principles.



<h2 class="wp-block-heading" id="h-building-a-fair-stopwatch">Building a fair stopwatch</h2>



A companion atom that never meets the barrier keeps regular time, letting researchers spot any lag or lead. “The tunneled clock is slightly older than the other,” says Schach. 



The outcome undercuts earlier claims of speeds beyond light and reframes the question: tunneling might feel instantaneous, yet its inner clock shows the journey costs a pinch of time.



Capturing such a slight slippage is no picnic. Lasers must maintain phase stability with dizzying precision, and stray magnetic fields must be kept in check. 



Using atom clouds spreads the work over many identically prepared clocks, and raising the transition frequency - much like switching from a wristwatch to an optical clock - amplifies the effect.



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



Sorting out tunneling time is more than settling an academic quarrel. Quantum engineers push devices toward ever <a href="https://www.earth.com/news/images-of-single-atoms-moving-freely-through-space-captured-for-the-first-time/" target="_blank" rel="noreferrer noopener">thinner barriers</a> in transistors and sensors, where picosecond wiggles can make or break performance. 



A crisp measure of tunneling time feeds directly into models that predict leakage currents, coherence losses, and heat budgets in next-generation chips and <a href="https://www.earth.com/news/ultra-cold-molecules-poised-to-revolutionize-quantum-computing/" target="_blank" rel="noreferrer noopener">quantum processors</a>.



On the fundamental side, timing the hop tests how quantum mechanics meshes with relativity. 



If the Darmstadt scheme proves that tunneling never outpaces light once the clock rides with the particle, one more apparent paradox evaporates, tightening the weave between the two towering theories of modern physics.



“We are currently discussing this idea with experimental colleagues and are in contact with our project partners,” adds Giese.



Laboratories already pushing atom interferometers to probe gravity or hunt dark matter may pivot to give the tunneling clock a spin. 



Success would not just timestamp a famous quantum trick; it would hand scientists a new metrological tool, ready to keep pace with particles that treat walls like suggestions rather than commands.



The full study was published in the journal <a href="https://www.science.org/doi/10.1126/sciadv.adl6078" target="_blank" rel="noreferrer noopener">Science Advances</a>.



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Breaking the light speed barrier with quantum tunneling – the debate gets heated

At the scale of atoms and electrons, walls are not...

Clos,Eup,Of,A,Woman,Wand,Touching,River,Water,In

Scientists have long mapped separate brain areas for sight, hearing, touch, taste, and smell. Yet new research reveals that when we focus sharply on any of those senses, signals converge on the same two structures buried deep in the brain - the midbrain reticular formation and the central thalamus.



This finding highlights a shared neural pathway that sustains <a href="https://www.earth.com/news/our-brain-stops-paying-attention-to-repeated-distractions/" target="_blank" rel="noreferrer noopener">attention</a> and wakefulness and could inspire therapies for coma, epilepsy, and attention-deficit disorders.



<h2 class="wp-block-heading" id="h-senses-in-a-single-brain-region">Senses in a single brain region</h2>



Research over the past century has shown that visual scenes activate the occipital cortex, melodies light up the temporal lobes, and so forth.



“We were expecting to find activity on shared networks, but when we saw all the <a href="https://www.earth.com/news/our-sense-of-smell-and-different-odors-can-influence-how-we-see-colors/" target="_blank" rel="noreferrer noopener">senses</a> light up the same central brain regions while a test subject was focusing, it was really astonishing,” said Aya Khalaf, a postdoctoral associate in neurology at <a href="https://medicine.yale.edu/" target="_blank" rel="noreferrer noopener">Yale School of Medicine</a> and lead author of the study.



Those two regions - the reticular formation, a mesh of neurons in the upper brainstem, and the intralaminar and mediodorsal nuclei of the thalamus - form part of the so-called subcortical arousal system, a set of circuits long suspected to regulate alertness and <a href="https://www.earth.com/news/consciousness-may-stem-from-unseen-dimensions-beyond-our-reality/" target="_blank" rel="noreferrer noopener">consciousness</a>.



Previous work had linked these hubs to vigilance by studying patients emerging from coma or experiencing absence seizures. But most of those experiments examined responses to a single type of stimulus, for example flashing lights or chirping sounds.



Khalaf and colleagues asked the broader question: do different senses share the same arousal circuitry when people deliberately pay attention?



<h2 class="wp-block-heading" id="h-a-massive-data-mine">A massive data mine</h2>



To answer that, the team turned to the publicly available <a href="https://www.humanconnectome.org/" target="_blank" rel="noreferrer noopener">Human Connectome Project</a> and other repositories, assembling functional MRI scans from 1,561 healthy adults.



Across 11 tasks, participants viewed moving shapes, listened to spoken stories, sampled liquid tastants, or felt puffs of air on their fingertips. Each task included abrupt cues that forced subjects to switch attention - for instance, a sudden change in picture orientation or a surprise tone embedded in white noise.



The investigators processed more than 500 hours of scan data through a pipeline that removed head motion and physiological noise, then aligned brain volumes to a common atlas.



In every sensory domain, when a cue demanded rapid attentional re-orientation, blood-oxygen signals spiked in the reticular formation and the central thalamus. The effect was absent or minimal during passive stimulation, underscoring the importance of active engagement.



<h2 class="wp-block-heading" id="h-consciousness-in-the-brain">Consciousness in the brain</h2>



Why would a taste test and a vision task end up at the same neural address? The authors propose that the midbrain reticular formation integrates sudden sensory changes and broadcasts a “wake-up” volley to the thalamus, which relays it to widespread cortical areas.



That burst synchronizes cortical rhythms, priming the brain to process incoming information. The scheme dovetails with classical animal studies showing that electrical stimulation of the reticular formation induces cortical desynchronization and behavioral arousal, while lesions produce stupor.



“It tells us how important this brain region is and what it could mean in efforts to restore consciousness,” Khalaf said.



“This has also given us insights into how things work normally in the brain. It’s really a step forward in our understanding of awareness and consciousness,” said senior author Hal Blumenfeld, a neurologist at Yale.



<h2 class="wp-block-heading" id="h-awakening-senses-in-the-brain">Awakening senses in the brain</h2>



Because the same deep-brain hubs fire regardless of which sense is active, treatments aimed at modulating those hubs could benefit diverse conditions.



Drugs that enhance thalamic neurotransmission, for instance, might improve focus in <a href="https://www.earth.com/news/autism-and-adhd-disorders-directly-linked-amount-of-time-kids-spend-on-screens/" target="_blank" rel="noreferrer noopener">attention deficit hyperactivity disorder</a>. Conversely, overactivity in the arousal circuit has been implicated in insomnia; dampening the circuitry could help induce sleep.



The results also support ongoing trials that deliver low-intensity ultrasound or deep-brain electrodes to the central thalamus in patients with disorders of consciousness. 



If attention triggers the thalamus to “switch on” the cortex, stimulating it directly might help rouse patients who are minimally conscious.



<h2 class="wp-block-heading" id="h-rethinking-sensory-rehabilitation"><a></a>Rethinking sensory rehabilitation</h2>



The discovery challenges sensory-specific training programs that ignore subcortical commonalities. 



For example, visual rehabilitation for <a href="https://www.earth.com/news/stroke-risk-is-elevated-by-air-pollution-and-traffic-noise/" target="_blank" rel="noreferrer noopener">stroke</a> survivors may benefit from pairing attentional cues with tactile or auditory tasks to engage the shared arousal pathway.



Likewise, virtual-reality therapies that bombard users with multi-sensory surprises might more effectively sharpen attentional control.



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



The Yale team plans to refine the timeline of activation using magnetoencephalography, which offers millisecond resolution. They also hope to dissect the frequency bands that link the thalamus to frontal and parietal cortices during attentional jumps. 



Such work could reveal whether gamma-band bursts or alpha-band suppression carry the critical “wake-up” message.



Another frontier involves patients. Investigators will compare responses in healthy volunteers with those in people who have attention deficits or who are emerging from anaesthesia. 



Identifying a lost or delayed thalamic spike could serve as a biomarker for impaired consciousness.



<h2 class="wp-block-heading" id="h-brain-regions-and-the-senses">Brain regions and the senses</h2>



For now, the study establishes the midbrain reticular formation and central thalamus as the universal relay through which sight, sound, taste, and touch gain conscious entry - at least when our minds snap to attention.



By showing that “all the senses light up the same central brain regions,” it confirms that consciousness depends not only on specialized cortical maps but also on a common deep-brain gatekeeper. 



Therapies that target this gatekeeper may eventually help restore awareness where it has dimmed and sharpen it where it wanders.



The study is published in the journal <a href="https://www.sciencedirect.com/science/article/pii/S1053811925002277?via%3Dihub" target="_blank" rel="noreferrer noopener">NeuroImage</a>.



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Scientists discover a brain region that connects all the senses

Scientists have long mapped separate brain areas for sight, hearing,...

An unprecedented survey of nearly 5,500 plant communities across 119 regions has uncovered a hidden ecological deficit: in landscapes with heavy human pressure, typical habitats contain barely one-fifth of the species they could support.



The international <a href="https://macroecology.ut.ee/en/darkdivnet/" target="_blank" rel="noreferrer noopener">DarkDivNet</a> consortium - whose members include the Biodiversity and Evolution Research Group at the <a href="https://www.ehu.eus/en/en-home" target="_blank" rel="noreferrer noopener">University of the Basque Country</a> (UPV/EHU) - reached this conclusion by analyzing “dark diversity,” the pool of <a href="https://www.earth.com/news/how-plant-diversity-can-help-combat-climate-change/%C3%B9" target="_blank" rel="noreferrer noopener">plant</a> species that should thrive in a site yet are absent.



<h2 class="wp-block-heading" id="h-measuring-human-pressure-on-plants">Measuring human pressure on plants</h2>



Conventional field studies tally the species that are present, but the DarkDivNet team flipped that approach. 



For every one-hectare plot, the researchers used climate, soil, and regional species pools to predict the full roster of plants likely to live there under natural conditions. They compared this “potential community” with the species that actually grew on the ground. 



Conventional approaches to measuring <a href="https://www.earth.com/news/feeding-the-world-without-harming-nature-the-complex-balance-of-farming/" target="_blank" rel="noreferrer noopener">biodiversity</a>, which focus solely on counting the species currently present and ignore those that could potentially inhabit an area, often downplay the full extent of human influence on ecosystems.



Because the technique captures loss before it becomes obvious, it serves as an early-warning system and a yard-stick for restoration goals.



<h2 class="wp-block-heading" id="h-from-pristine-reserves-to-patchy-farmlands"><a></a>From pristine reserves to patchy farmlands</h2>



The DarkDivNet project was conceived by Meelis Pärtel of the <a href="https://ut.ee/en" target="_blank" rel="noreferrer noopener">University of Tartu</a> and launched in 2018. Since then, research teams on every continent have followed a single protocol to ensure results are comparable.



One contribution came from lecturers Idoia Biurrun-Galarraga and Juan Antonio Campos-Prieto (UPV/EHU), who mapped 55 plots in Spain’s Gorbeia Nature Reserve, focusing on beech woods and upland heaths. 



Data gathering spanned five field seasons and navigated hurdles such as COVID-19 travel bans and political unrest affecting partner institutions.



To rate human pressure, the scientists turned to the <a href="https://hub.arcgis.com/maps/65518e782be04e7db31de65d53d591a9/about" target="_blank" rel="noreferrer noopener">Human Footprint Index</a>, a composite measure that integrates population density, <a href="https://www.earth.com/news/using-more-land-agricultural-expansion-will-harm-climate-and-biodiversity/" target="_blank" rel="noreferrer noopener">land-use</a> conversion, and infrastructure such as roads. Scores ranged from virtually undisturbed wilderness to intensively farmed or urbanized territory.



The resulting pattern was stark. Sites in low-footprint zones harbored about one-third of their potential species - already a significant shortfall caused mainly by natural dispersal limits. Where the footprint was high, realized diversity slumped to 20 percent.



<h2 class="wp-block-heading" id="h-human-pressure-beyond-plant-life">Human pressure beyond plant life</h2>



The deficit is not confined to places where bulldozers roar or fields extend to the horizon. Modelling showed that roads, <a href="https://www.earth.com/news/understanding-how-air-pollution-forms-may-help-us-prevent-it/" target="_blank" rel="noreferrer noopener">pollution</a>, and land-use change depress diversity hundreds of kilometers away, even inside protected areas.



According to the authors, the results “are alarming because they show that human disturbance exerts a much greater impact than initially thought, even reaching protected areas far from the source of human impact. 



Pollution, deforestation, overgrazing, and <a href="https://www.earth.com/news/fewer-forest-fires-happen-today-than-in-the-past-ironically-causes-bigger-issues/" target="_blank" rel="noreferrer noopener">forest fires</a> can exclude plant species from their natural habitats, preventing them from recolonizing.”



Yet the study did uncover a mitigating factor. Landscapes in which at least one-third of total area remains intact fare markedly better; species stranded in little-touched blocks can drift back into damaged patches.



“The negative influence of human activity was less pronounced when at least one third of a region's area remained well preserved, which supports the global goal of protecting 30% of the planet's surface,” the authors wrote. 



The finding lends empirical weight to the “30 by 30” conservation target adopted in the 2022 <a href="https://www.cbd.int/gbf" target="_blank" rel="noreferrer noopener">Kunming–Montreal Global Biodiversity Framework</a>.



<h2 class="wp-block-heading" id="h-dark-diversity-and-hidden-issues">Dark diversity and hidden issues</h2>



Identifying which species should be present but are missing allows land managers to diagnose underlying problems - be it altered fire regimes, livestock browsing, or lost <a href="https://www.earth.com/news/pollinators-face-extinction-risk-due-to-climate-change/" target="_blank" rel="noreferrer noopener">pollinators</a> - and to direct re-introductions where they stand a fighting chance. 



In restoration projects, the metric can reveal whether ecosystem recovery from human disturbance is on track long before plant counts return to pre-disturbance numbers.



Because the same protocol works in grasslands, forests, and wetlands, DarkDivNet data provide a common currency for comparing impacts and gauging trade-offs among land-use policies worldwide. 



The approach can also highlight priority corridors between intact refuges, where recolonization pressure is greatest.



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



The network plans to extend its reach to under-sampled biomes and to layer animal and fungal dark-diversity maps onto the botanical baseline, producing a multidimensional picture of ecological debt. 



Remote-sensing teams are testing whether patterns of missing species leave spectral fingerprints detectable by drones or satellites.



For now, the project delivers a sobering message: even where forests still stand tall and fields appear green, a silent erosion is under way.



By documenting both visible and invisible losses, dark-diversity analysis reveals the full scope of human influence - and spotlights how much of the living world can return if true refuges are safeguarded across at least 30 percent of every region.



The global tally of species we fail to see, in other words, may be the most important conservation number we need to track.



The study is published in the journal <a href="https://www.nature.com/articles/s41586-025-08814-5" target="_blank" rel="noreferrer noopener">Nature</a>.



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Human pressure has a hidden impact on plant diversity

An unprecedented survey of nearly 5,500 plant communities across 119...

Every third Friday of May, we pause to recognize the fragile existence of endangered species. We share the planet with countless animals, plants, and insects. Yet, many of them are vanishing right before our eyes. National Endangered Species Day urges us to take action before it’s too late.



The day was established in 2006 by the U.S. Congress to raise awareness about <a href="https://www.earth.com/news/world-wildlife-day-2025-a-global-call-to-protect-nature/" target="_blank" rel="noreferrer noopener">species</a> at risk of extinction. But the issue goes back decades. Laws to protect endangered species have been around for over 40 years.



Today, the urgency remains the same. Species are still disappearing, and their habitats are under threat.



<h2 class="wp-block-heading" id="h-what-makes-a-species-endangered">What makes a species endangered?</h2>



When the last of a <a href="https://www.earth.com/news/saving-earths-most-endangered-plants-from-extinction-proving-difficult-botanic-gardens/" target="_blank" rel="noreferrer noopener">species</a> vanishes, it’s gone forever. Endangered species hover dangerously close to that fate. Their numbers are so low that every birth counts, every death matters. Some hover in the thousands, others in the hundreds, and a few are down to mere tens.



Why do species disappear? The reasons are many. Habitat loss drives some to extinction. Climate change alters their environment, making it uninhabitable. Poaching and illegal trade push animals like rhinos and elephants to the brink.



Pollution seeps into ecosystems, poisoning marine life and birds. And sometimes, humans disrupt delicate ecosystems without realizing the consequences.



<h2 class="wp-block-heading" id="h-the-ripple-effect-of-extinction">The ripple effect of extinction</h2>



When a <a href="https://www.earth.com/news/most-endangered-primate-species-identified-in-new-report/" target="_blank" rel="noreferrer noopener">species</a> vanishes, it doesn’t go quietly. The loss ripples through ecosystems. A predator disappears, and prey populations explode. Plants die off, and animals lose their food source. The web of life is fragile, and every species has a role.



Take pollinators, for instance. Bees, butterflies, and bats help plants reproduce. If they disappear, crops fail, and food chains collapse. The same goes for apex predators. 



When wolves were reintroduced to Yellowstone, they restored balance by controlling deer populations. When keystone species vanish, chaos follows.



<h2 class="wp-block-heading" id="h-learning-from-the-past">Learning from the past</h2>



In the early 1970s, the Endangered Species Act set strict guidelines for protecting at-risk <a href="https://www.earth.com/news/climate-change-is-the-largest-threat-to-u-s-endangered-species/" target="_blank" rel="noreferrer noopener">species</a> in the United States. It prohibited activities that could harm these animals and their habitats. It also laid the groundwork for conservation efforts worldwide.



Since then, thousands of species have been added to endangered lists. Some, like the bald eagle, have made remarkable recoveries. Others, like the vaquita porpoise, remain on the brink.



Today, the International Union for Conservation of Nature (<a href="https://iucn.org" target="_blank" rel="noreferrer noopener">IUCN</a>) tracks endangered species globally. Its Red List reveals a grim reality. Over 41,000 species face extinction. That includes more than a quarter of all mammals, one in eight birds, and a staggering 40% of amphibians.



<h2 class="wp-block-heading" id="h-taking-action-on-endangered-species-day">Taking action on Endangered Species Day</h2>



National Endangered Species Day isn’t just about learning facts and figures. It’s about taking action. Conservation organizations host events, workshops, and fundraisers. Many zoos and nature centers offer guided tours, showing visitors how they care for endangered animals.



Some activities are simple yet impactful. Share photos of endangered species on social media. Spread the word about why these creatures matter. Support local conservation projects. 



Even small actions, like planting native flowers for bees or reducing plastic waste, can help protect fragile <a href="https://www.earth.com/news/earth-day-2025-what-were-really-fighting-for/" target="_blank" rel="noreferrer noopener">ecosystems</a>.



<h2 class="wp-block-heading" id="h-exploring-endangered-species-with-tech">Exploring endangered species with tech</h2>



Technology brings endangered species closer to home. Apps like <a href="https://www.earth.com/earthsnap/" target="_blank" rel="noreferrer noopener">EarthSnap</a> engage people in documenting local wildlife, creating snapshots of biodiversity in real time.



With EarthSnap, users can photograph plants and animals to identify species, contributing to a growing database of endangered life forms. This information becomes valuable data for conservationists tracking population changes and habitat loss. 



Meanwhile, virtual reality experiences transport people to remote habitats, offering immersive glimpses of endangered ecosystems. By bringing these distant worlds closer, technology fosters connection and urgency - reminding us of what’s at stake if species continue to vanish.



Online databases like the IUCN Red List provide up-to-date information on endangered species. They reveal how many individuals remain, what threats they face, and what’s being done to save them. The goal is to make people aware - and inspire them to act.



<h2 class="wp-block-heading" id="h-supporting-global-conservation-efforts">Supporting global conservation efforts</h2>



Conservation requires resources, time, and unwavering commitment. Organizations like the World Wildlife Federation and the <a href="https://janegoodall.org" target="_blank" rel="noreferrer noopener">Jane Goodall Institute</a> work tirelessly to protect endangered species. They fund anti-poaching efforts, rehabilitate injured animals, and restore habitats.



Individuals can help too. Donate to wildlife organizations. Volunteer at local conservation centers. Adopt sustainable habits such as using less plastic or buying sustainably sourced products. Every choice, no matter how small, can make a difference.



<h2 class="wp-block-heading" id="h-a-future-worth-protecting">A future worth protecting</h2>



National Endangered Species Day reminds us that time is running out for many species. The fate of these animals, plants, and insects isn’t set in stone. We have the power to change their stories.



Saving endangered species isn’t just about protecting animals. It’s about preserving ecosystems, supporting biodiversity, and ensuring a balanced, thriving planet for future generations. And that future starts with us.



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National Endangered Species Day: Protecting life on the brink

Every third Friday of May, we pause to recognize the...

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



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



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



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



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



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



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



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



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



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



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

Is chocolate the next nutritional powerhouse?

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

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



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



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



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



Video/ Image Credit: ESA



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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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Thankfully, the fishy siblings didn’t do the disturbing death-dance like the other fillet. She slid the knife along the belly and poked her fingers inside, hoping to feel something other than squishy guts.

Fingers Crossed

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