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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA/Hubble &amp; NASA



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Violent clash of the Antennae Galaxies  

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

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Hubble spotlights galaxies in the constellation Virgo

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA



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Ghostly galaxy in the constellation Eridanus

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA



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Rosetta Nebula: Sculpted by starlight over millions of years

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA/ESA Hubble Space Telescope



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Secrets of a spiraling galactic powerhouse

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

<h1>Peace Lily</h1>
Also recognized by NASA for the ability to remove volatile organic compounds (VOCs) from inside the home, peace lilies are beautiful and easy to care for. They simply require shade and weekly watering.

Peace Lily

Seagrass meadows are a hidden treasure of Florida’s coastal beauty, often overlooked in favor of beaches and mangroves. Yet beneath the surface, these underwater fields quietly support marine life, stabilize shores, and protect coastal communities. 



Along Florida’s Nature Coast, seagrass meadows are not just surviving - they’re thriving. A recent study reveals that seagrass ecosystems in this region have remained remarkably healthy and undisturbed for thousands of years - and this resilience is rare.



Globally, seagrass meadows are in trouble. Since 1879, nearly 30% have vanished. Between 1990 and 2009 alone, seagrass beds declined by an estimated 7% each year. Unlike many regions where seagrass meadow loss is the norm, Florida’s Nature Coast has become a rare refuge for these vital ecosystems.



<h2 class="wp-block-heading" id="h-lessons-from-past-seagrass-meadows">Lessons from past seagrass meadows</h2>



Researchers from the Florida Museum of Natural History at the <a href="https://www.ufl.edu/" target="_blank" rel="noreferrer noopener">University of Florida</a> set out to understand how these meadows have endured. The common problem they faced is that we don’t really know what an untouched ecosystem looks like anymore.



“Nothing is really pristine today, because humans have altered all of Earth’s environments, but this is about as good as it gets,” said Michal Kowalewski, senior author of the study.



One major hurdle is the lack of long-term environmental data. “Most of the contemporary biological data we have postdates the Industrial Revolution,” Kowalewski explained. 



“If you think about any type of real-time instrumentation that collects physical and chemical information about an environment, or if you think about the rigorous bio-inventory surveys, all of those things are from the last 50 to 100 years at most.”



<h2 class="wp-block-heading" id="h-fossil-clues-beneath-seagrass-meadows">Fossil clues beneath seagrass meadows</h2>



In other words, humanity has been altering nature far longer than we've been systematically observing it. Luckily, Earth itself keeps a record - in the form of fossils.



This is where conservation paleobiology steps in. Scientists use the recent fossil record to reconstruct past ecosystems. 



Seagrasses, unfortunately, don’t leave fossils. Their soft tissues decompose quickly. But the animals living in seagrass meadows - especially shell-bearing <a href="https://www.earth.com/news/mollusks-evolution-shishania-aculeata-spiny-armor-no-shells-500-million-years-ago/" target="_blank" rel="noreferrer noopener">mollusks</a> - do leave lasting traces.



Kowalewski and his team have shown that mollusk fossils are reliable indicators of <a href="https://www.earth.com/news/groundwater-plays-critical-role-ecosystem-health/" target="_blank" rel="noreferrer noopener">ecosystem health</a>. When mollusks thrive, it’s a good sign that the surrounding environment is in good shape, too.



<h2 class="wp-block-heading" id="h-studying-florida-s-nature-coast">Studying Florida's Nature Coast</h2>



For their study, the team sampled 21 sites across six estuaries along the Nature Coast. Using PVC hoses, they collected sediment from the seafloor, sifting through centuries of accumulated material.



“We collect sediment samples while scuba diving, and then we sieve those samples and extract all that we find in it,” Kowalewski said. “The samples are dominated by dead material, because it has accumulated there over many centuries. Typically, for every live bivalve or snail, we find thousands of <a href="https://www.earth.com/news/seagrass-meadows-are-very-reliable-fishing-grounds/" target="_blank" rel="noreferrer noopener">dead specimens</a>.”



Identifying and cataloging these specimens took years. But when the data was analyzed, the results were clear: mollusk diversity had barely changed in millennia. This suggests that the seagrass meadows they inhabit have remained stable, too.



“Only rarely do we find historical evidence that can make us optimistic about the current state of a local ecosystem,” Kowalewski said. 



“Most conservation paleobiology studies tell depressing stories about <a href="https://www.earth.com/news/rising-heat-shrinking-habitats-insects-face-hidden-threats/" target="_blank" rel="noreferrer noopener">shrinking habitats</a>, declining biodiversity and diminishing ecosystem services. For once, at least, this is not the case. What’s thrilling to me is we can show this system is still in very good condition, which makes it even more important to protect it.”



<h2 class="wp-block-heading" id="h-a-model-for-seagrass-restoration">A model for seagrass restoration</h2>



This discovery is more than just a pleasant surprise. It provides a valuable reference point for <a href="https://www.earth.com/news/without-tackling-climate-change-coral-restoration-efforts-are-insufficient/" target="_blank" rel="noreferrer noopener">restoration efforts</a> elsewhere. Healthy seagrass meadows are disappearing, but Florida's Nature Coast shows us what these ecosystems should look like.



Elsewhere in Florida, seagrass has not been so fortunate. In Tampa Bay, nearly half of the seagrass was lost between 1950 and 1980 due to urban growth and pollution. 



Although restoration efforts brought some recovery by 2018, recent declines have been noted again. On the state’s east coast, surveys show that up to 60% of seagrass has vanished in parts of the Indian River Lagoon.



<h2 class="wp-block-heading" id="h-hidden-nutrient-pollution">Hidden nutrient pollution</h2>



Most of these losses stem from nutrient pollution. Runoff from farms and cities feeds algae and bacteria, creating dense blooms that cloud the water. This “marine cloud” blocks sunlight from reaching the seagrass below, starving them of the light they need to survive.



The Nature Coast has so far escaped this fate. In 2020, it was designated an aquatic preserve, helping protect its relatively undeveloped watersheds.



Study co-author Thomas Frazer is a dean at the University of South Florida College of Marine Science.



“There’s not a lot of development in those watersheds, particularly from the area around Weeki Wachee all the way up into the Panhandle, so the effects of excess nutrient delivery are not as pronounced as is in other places that have suffered as a consequence,” said Frazer.



However, this does not mean the threat has passed. <a href="https://www.earth.com/wp-admin/post.php?post=1969992&amp;action=edit" target="_blank" rel="noreferrer noopener">Algal blooms</a> are now an annual event in many parts of Florida. Even Nature Coast seagrasses may be affected if water quality declines.



<h2 class="wp-block-heading" id="h-climate-change-and-moving-species">Climate change and moving species</h2>



Climate change adds another layer of complexity. <a href="https://www.earth.com/news/rising-temperatures-and-extreme-rainfall-study-reveals-a-missing-link/" target="_blank" rel="noreferrer noopener">Rising temperatures</a> are pushing temperate and subtropical species northward. Florida’s Gulf Coast, backed against the Panhandle, offers little room for further migration.



“There’s nowhere for them to go,” Frazer said. As marine life shifts, seagrass ecosystems may face new challenges. 



A single blade of seagrass is home to countless organisms - hydroids, bryozoans, sea squirts, bacteria, and algae. 



Normally, grazing fish and invertebrates keep these communities balanced. But if these grazers disappear or new species disrupt the balance, the health of the meadow could suffer.



“We’re already seeing range extensions of mobile fauna,” Frazer added. “A number of fishes, for example, are moving up north along the Gulf Coast, and they may either eat seagrass or consume grazers that help keep seagrasses clean of organisms that live on them.”



<h2 class="wp-block-heading" id="h-why-seagrasses-matter-so-much">Why seagrasses matter so much</h2>



Seagrasses are ancient. They’ve been around longer than the dinosaurs and their benefits to both marine and human life are immense. Rachel Carson captured their importance in her 1955 book The Edge of the Sea. 



“Thrusting their roots into the sand and shifting coral debris, the seagrasses achieve a firmer attachment than the rootless algae do; where they grow thickly, they help to secure the offshore sands against the currents, as on the land the dune grasses hold the dry sands against the winds," she wrote.



Seagrasses stabilize the seabed, prevent erosion, and are vital for marine biodiversity. Despite covering just 0.2% of the ocean floor, they are responsible for 50% of marine carbon burial. They provide food for sea turtles, manatees, and fish. For countless species, seagrass meadows are essential nurseries.



“They provide very important nursery habitat,” Frazer said. “In Florida alone, more than 80% of the fish caught by commercial fisherman and recreational anglers spend some part of their life history in those seagrass beds.”



<h2 class="wp-block-heading" id="h-protecting-seagrass-meadows">Protecting seagrass meadows</h2>



Frazer noted that seagrasses serve as a front line for storm protection. Their dense underwater meadows reduce wave energy by up to 40% in shallow waters, acting as natural storm barriers.



Florida’s Nature Coast now holds the largest seagrass meadows bed in the Gulf of Mexico. With careful management and ongoing conservation, it has the potential to stay that way.



While much of the world races to restore what’s been lost, the Nature Coast reminds us of a simple truth: sometimes, the best thing we can do is protect what we already have.



The full study was published in the journal <a href="https://www.int-res.com/abstracts/meps/v760/p71-86/" target="_blank" rel="noreferrer noopener">Marine Ecology Progress Series</a>.



Image Credit: Ben Jones / Ocean Image Bank



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Seagrass meadows still thrive on Florida's Nature Coast

Seagrass meadows are a hidden treasure of Florida’s coastal beauty,...

Healthy,Vegetarian,Dinner.,Woman,In,Jeans,And,Warm,Sweater,Holding

Aging can mean many things. It can mean slowing down, feeling less sharp, or facing more health issues. But it doesn’t have to. A new study suggests that what women eat in midlife could set the stage for how well they age. 



Published in JAMA Network Open, the study from <a href="https://www.tufts.edu" target="_blank" rel="noreferrer noopener">Tufts University</a> and <a href="https://hsph.harvard.edu" target="_blank" rel="noreferrer noopener">Harvard T.H. Chan School of Public Health</a> dives into the power of carbohydrates and fiber in shaping <a href="https://www.earth.com/news/organ-aging-can-predict-diseases-decades-in-advance/" target="_blank" rel="noreferrer noopener">health</a> decades later.



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



Not all carbs are equal. Some lift you up, while others drag you down.



“We’ve all heard that different carbohydrates can affect <a href="https://www.earth.com/news/how-old-are-you-really-new-tool-measures-aging-from-the-inside-out/" target="_blank" rel="noreferrer noopener">health</a> differently, whether for weight, energy, or blood sugar levels. But rather than just look at the immediate effects of these macronutrients, we wanted to understand what they might mean for good health 30 years later,” said lead author Andres Ardisson Korat.



The study zeroed in on 47,000 women, ages 70 to 93. The researchers looked at what these women ate over a span of three decades, starting in 1984. They tracked their intake of refined carbs, high-quality carbs, and fiber. They wanted to see who aged well - and who didn’t.



<h2 class="wp-block-heading" id="h-what-healthy-aging-looks-like">What healthy aging looks like</h2>



Living past 70 doesn’t mean you’re aging well. The researchers defined <a href="https://www.earth.com/news/curiosity-might-help-you-stay-sharp-as-you-age/" target="_blank" rel="noreferrer noopener">healthy</a> aging as reaching 70 without major chronic diseases, keeping a sharp mind, staying physically capable, and feeling good mentally. Out of 47,000 women, only 3,706 fit that bill.



What did those women have in common? A diet rich in high-quality carbs and fiber. The more they ate from whole grains, fruits, vegetables, and legumes, the better they aged.



<h2 class="wp-block-heading" id="h-high-quality-carbs-boost-aging">High-quality carbs boost aging</h2>



Eating more high-quality carbs wasn’t just good. It was transformative. Women who upped their intake of high-quality carbs by 10% had a 31% better chance of aging well. 



The same couldn’t be said for refined carbs. Sugary snacks and white bread were linked to a 13% drop in the odds of healthy <a href="https://www.earth.com/news/scientists-discover-a-protein-that-reverses-cellular-aging/" target="_blank" rel="noreferrer noopener">aging</a>. 



“Our results are consistent with other evidence linking consumption of fruits and vegetables, whole grains, and legumes with lower risks of chronic diseases, and now we see the association with physical and cognitive function outcomes,” said study senior author Qi Sun.



<h2 class="wp-block-heading" id="h-fiber-s-role-in-protecting-health">Fiber’s role in protecting health</h2>



Fiber doesn’t just keep things moving. It protects your mind. It shields your body. For every one-standard-deviation bump in fiber intake, the odds of healthy aging shot up by 17 percent.



Fruit fiber boosted odds by 14 percent. Vegetable fiber added 11 percent. Even cereal fiber, often overlooked, contributed a 7% increase.



The benefits of fiber went beyond disease prevention. Women with higher fiber intake had stronger memories, better physical function, and fewer mental health problems.



<h2 class="wp-block-heading" id="h-all-carbs-affect-aging-differently">All carbs affect aging differently</h2>



Glycemic index (GI) and glycemic load (GL) may sound like fancy terms, but they matter. Foods with a high GI hit blood sugar hard and fast. Not great for aging well.



High GL foods, on the other hand, had a surprising link to better mental health. But once the researchers factored in fiber intake, that connection weakened. The takeaway? Fiber might buffer some of the negative effects of high-GI foods.



<h2 class="wp-block-heading" id="h-replacing-refined-carbs">Replacing refined carbs</h2>



Imagine swapping out refined carbs for high-quality ones. What happens? Women who did had 8% to 16% better odds of aging well. That’s a big jump.



“Studies are starting to find an association between food choices in midlife and quality of life in later years. The more we can understand about healthy <a href="https://www.earth.com/news/human-bodies-begin-breaking-down-two-very-precise-ages/" target="_blank" rel="noreferrer noopener">aging</a>, the more science can help people live healthier for longer,” Korat said.



<h2 class="wp-block-heading" id="h-tracking-women-s-diets">Tracking women's diets</h2>



This study tracked women’s diets for over 30 years. It connected their midlife eating habits to their health in their 70s and 80s. The findings suggest that small, consistent changes matter more than drastic diets.



The researchers saw that women who ate more whole grains, fruits, and veggies over time aged better than those who filled up on white bread and sweets.



The study mostly included white, educated health professionals. Participants reported their own dietary habits, which might not be completely accurate. And after three decades, memories can get hazy.



Still, the findings were clear. Eating more high-quality carbs and fiber in midlife made a noticeable difference. It wasn’t just beneficial - it was transformative.



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



Aging well isn’t just about avoiding illness. It’s about staying mentally sharp, physically active, and feeling good. The study suggests that what women eat in their 40s and 50s can impact their health decades later.



But it’s not just about eating fewer carbs. It’s about eating the right ones. Whole grains, fruits, vegetables, and legumes gave women a better shot at aging well.



<h2 class="wp-block-heading" id="h-carbs-and-fiber-shape-aging">Carbs and fiber shape aging</h2>



The food choices women make in midlife are more than just meals. They’re investments. 



High-quality carbs and dietary fiber aren’t just good for digestion. They’re linked to lower risks of chronic diseases, sharper minds, and better physical health in old age.



Aging doesn’t have to mean decline, and it doesn’t have to mean slowing down. For the women in this study, eating well decades earlier paid off in a big way. The lesson? It’s never too early to think about the future. And it’s never too late to make better choices.



The study is published in the journal <a href="https://jamanetwork.com/journals/jamanetworkopen/fullarticle/2834202" target="_blank" rel="noreferrer noopener">JAMA Network Open</a>.



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High-quality carbs in midlife linked to healthier aging

Aging can mean many things. It can mean slowing down,...

In many places, men face a higher risk of disease but receive less timely care. These observations come from a broad international effort examining hypertension, diabetes, and HIV and aids.



Angela Chang from the <a href="https://www.sdu.dk/en" target="_blank" rel="noreferrer noopener">University of Southern Denmark</a> led a team that gathered worldwide information on who falls ill and who actually receives help. The analysis pointed to important differences by sex, affecting disease rates and overall health <a href="https://www.earth.com/news/organ-aging-can-predict-diseases-decades-in-advance/" target="_blank" rel="noreferrer noopener">outcomes</a>.



<h2 class="wp-block-heading" id="h-sex-differences-affect-health-outcomes">Sex differences affect health outcomes</h2>



Males have higher rates of smoking in most nations according to the <a href="https://apps.who.int/iris/handle/10665/343287" target="_blank" rel="noreferrer noopener">World Health Organization</a>. Smoking is a known factor for high blood pressure, making it a key contributor to heart problems. Females tend to lead in <a href="https://www.sciencedirect.com/science/article/pii/S2161831322010249" target="_blank" rel="noreferrer noopener">obesity</a> numbers in many regions, which can contribute to diabetes.



These diseases are not just about risk factors. The study shows that males often end up with higher mortality rates once they develop these <a href="https://www.earth.com/news/rats-are-spreading-a-deadly-disease-across-cities/" target="_blank" rel="noreferrer noopener">conditions</a>. 



Many men <a href="https://menandhiv.org/publication/the-mens-health-gap-men-must-be-included-in-the-global-health-equity-agenda/" target="_blank" rel="noreferrer noopener">fail to visit clinics</a> or hospitals as regularly as women, which could mean they don’t get diagnosed or treated when they need it.



<h2 class="wp-block-heading" id="h-disease-risks-and-care-gaps">Disease risks and care gaps </h2>



<a href="https://my.clevelandclinic.org/health/diseases/4314-hypertension-high-blood-pressure" target="_blank" rel="noreferrer noopener">Hypertension</a>, commonly called high blood pressure, is often undetected. Men skip checkups more frequently, so signs that might be obvious in a routine exam can slip under the radar. If left unaddressed, this condition can lead to complications like stroke and heart failure.



Diabetes also showed worrying trends. In around half of surveyed countries, men were more likely to die from this disease than women. In a few areas, women had a greater <a href="https://www.earth.com/news/heart-disease-remains-the-leading-cause-of-death-worldwide/" target="_blank" rel="noreferrer noopener">disease</a> burden, but men were still less likely to receive consistent care in those spots.



HIV and aids <a href="https://www.unaids.org/sites/default/files/media_asset/2020_global-aids-report_en.pdf" target="_blank" rel="noreferrer noopener">data</a> revealed that in most places where statistics were available, men’s prevalence and death rates outpaced those of women. The research suggested that men often lagged behind in testing, treatment, and adherence to medication schedules.



<h2 class="wp-block-heading" id="h-care-disparities-by-sex">Care disparities by sex</h2>



“Without sex-disaggregated cascade data, we’re flying blind - unable to detect who is falling through the cracks in prevention, diagnosis, and care,” said Angela Chang, senior author of the study.



The team emphasized that many health policies and programs do not consider these persistent differences in how men and women seek health support.



The researchers pointed out that risk factors aren’t only rooted in biology. Gender norms and expectations can increase or lower the likelihood that a person will smoke, receive checkups, or follow a treatment plan.



<h2 class="wp-block-heading" id="h-why-men-avoid-health-care">Why men avoid health care </h2>



Many men report that they avoid medical care unless absolutely necessary. In <a href="https://www.researchgate.net/publication/263198588_Men_and_primary_care_Improving_access_and_outcomes" target="_blank" rel="noreferrer noopener">surveys</a> across different countries, common reasons include fear of diagnosis, lack of time, or the belief that symptoms will go away on their own.



Some researchers suggest that social norms around masculinity encourage toughness and discourage vulnerability. This can stop men from seeking care early, which delays diagnosis and worsens outcomes.



<h2 class="wp-block-heading" id="h-men-s-health-care-disparities">Men’s health care disparities</h2>



“We have long advocated the benefits of publishing sex disaggregated data. Such data can reveal where the health journeys of men and women diverge, be it in relation to the risk factors they are exposed to, their health care seeking behaviors or their experiences in <a href="https://www.earth.com/news/fungal-diseases-that-infect-humans-are-becoming-more-common-in-warming-world/" target="_blank" rel="noreferrer noopener">health</a> care systems,” said Professors Kent Buse at Global 50/50. 



The experts emphasize that social constructs shape health as much as biology, suggesting that efforts to tackle these disparities should address cultural and systemic factors. The findings highlight the need for balanced health policies. 



Certain measures might need to target men more aggressively, aiming to increase early screening, boost clinic attendance, and raise awareness around symptoms that men are less likely to act on promptly.



<h2 class="wp-block-heading" id="h-gaps-in-men-s-health-care">Gaps in men's health care</h2>



Policymakers and health professionals may look at these gaps and explore fresh approaches to reach men. From workplace screening programs to flexible clinic hours, there are strategies that address the common reasons men often give for not seeking help.



Experts agree that looking at sex-disaggregated data is the first step toward making sure no one gets left behind. The focus is on gathering stronger, more detailed information. That way, actions can be tailored and effective, ensuring better health for all.



<h2 class="wp-block-heading" id="h-the-problem-with-missing-data">The problem with missing data</h2>



A major issue researchers faced was the lack of complete data for many countries. While the team found data on risk and death rates for over 200 countries, full care cascade data, especially broken down by sex, was often missing, particularly for diabetes and hiv and aids.



Without this information, it’s hard to see where and why people are dropping off the care pathway. This makes it more difficult to design effective solutions or understand how patterns differ across age, income, and region.



The study is published in the journal <a href="https://journals.plos.org/plosmedicine/article?id=10.1371/journal.pmed.1004592" target="_blank" rel="noreferrer noopener">PLOS Medicine</a>.



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Men die more from preventable health issues but seek less care

In many places, men face a higher risk of disease...

The Southern Ocean, vast and cold, swallows more carbon than its size suggests. It’s a carbon sink, a crucial one, pulling atmospheric carbon down into its icy depths. But what happens when the rules change?



New research from the University of East Anglia (<a href="https://www.uea.ac.uk" target="_blank" rel="noreferrer noopener">UEA</a>) takes a hard look at this question. The study warns that the ocean’s role in carbon absorption might weaken as greenhouse gas (GHG) emissions climb.



The old driver, the ozone hole, might be stepping back. In its place? Rising emissions, <a href="https://www.earth.com/news/carbon-crisis-what-if-the-ocean-lost-all-of-its-life/" target="_blank" rel="noreferrer noopener">warming waters</a>, and unpredictable winds.



<h2 class="wp-block-heading" id="h-ozone-depletion-s-reversible-impact">Ozone depletion’s reversible impact</h2>



Back in the 20th century, the ozone hole ruled the Southern Ocean’s winds. It churned up the waters, dragging carbon-heavy currents to the surface. The result? The ocean became less capable of soaking up more carbon.



But now, the ozone hole is healing. And as it recovers, its grip on the winds is slipping. That might sound like good news, but there’s a catch.



Dr. Tereza Jarníková of the Tyndall Cente for Climate Change Research at UEA is the lead author of the study.



“An interesting, and hopeful, highlight of this work is that the effects of human-caused ozone hole damage on the winds, circulation, and carbon uptake of the Southern Ocean are reversible, but only under a lower scenario of greenhouse gas emissions,” noted Dr. Jarníková.



<h2 class="wp-block-heading" id="h-wind-patterns-in-the-southern-ocean">Wind patterns in the Southern Ocean</h2>



In the 20th century, ozone depletion drove wind <a href="https://www.earth.com/news/how-the-ocean-holds-carbon-hidden-mechanisms-revealed/" target="_blank" rel="noreferrer noopener">patterns</a> in the Southern Ocean. The stronger winds pulled carbon-laden waters to the surface, reducing the ocean’s carbon sink potential.



Now, as the ozone hole mends, those winds are calming down. But will that last? The study suggests it won’t. 



Under a high-emission scenario, wind speeds could surge by 0.75 meters per second (2.46 feet per second) by the end of the century. In a low-emission world, the increase might hold at 0.35 meters per second (1.15 feet per second). In both cases, GHGs, not ozone, would be the dominant force behind the winds.



<h2 class="wp-block-heading" id="h-carbon-storage-in-the-southern-ocean">Carbon storage in the Southern Ocean</h2>



The ocean’s mixed-layer depth (MLD) tells a story of shifting currents. When the MLD deepens, carbon-rich waters rise to the surface, limiting how much more carbon the ocean can absorb.



Ozone depletion deepened the MLD in the past, slashing the Southern Ocean’s carbon sink capabilities. But as the ozone hole heals, the MLD could stabilize.



Still, there’s a new threat. Rising GHGs could keep pushing those waters up. In a high-emission scenario, MLD deepening could intensify, making it harder for the ocean to absorb atmospheric carbon.



<h2 class="wp-block-heading" id="h-ocean-currents-and-carbon-uptake">Ocean currents and carbon uptake</h2>



Meridional overturning circulation (MOC) acts like a conveyor belt, carrying nutrient-rich waters to the surface. This process fuels biological productivity, pulling carbon down into the deep <a href="https://www.earth.com/news/a-weaker-ocean-will-release-more-carbon-into-the-atmosphere/" target="_blank" rel="noreferrer noopener">ocean</a>.



But the study finds that the MOC’s influence on carbon uptake is waning. Why? Rising surface temperatures are flattening the carbon gradient between surface and deep waters. The result is that less carbon gets absorbed.



<h2 class="wp-block-heading" id="h-temperature-the-new-carbon-thief">Temperature: The new carbon thief</h2>



The Southern Ocean is warming. By 2100, surface temperatures could rise by 1.6°C under a high-emission scenario. Warm water holds less carbon, making it harder for the ocean to trap atmospheric CO2.



Even if winds intensify and the MLD deepens, the warming <a href="https://www.earth.com/news/seagrass-plays-a-major-role-in-global-carbon-storage/" target="_blank" rel="noreferrer noopener">waters</a> might still win. The ocean’s capacity to absorb carbon is shrinking, driven by temperature increases that are now outpacing other factors.



<h2 class="wp-block-heading" id="h-future-scenarios-a-tug-of-war">Future scenarios: A tug of war</h2>



The UEA team used the UK Earth System Model (UKESM1) to simulate three possible ozone futures. 



In the first scenario, the ozone hole never forms, maintaining stable winds and circulation. In the second, the hole forms but gradually recovers after the 1987 Montréal Protocol. The third scenario envisions the ozone hole persisting at its 1987 size, continuing to <a href="https://www.earth.com/news/carbon-storage-mystery-emerges-in-the-southern-ocean/" target="_blank" rel="noreferrer noopener">influence</a> wind patterns and circulation.



Layered over these scenarios are two GHG pathways: one with emissions peaking and then falling, and another where emissions keep climbing. The results reveal a tug of war between ozone recovery and GHG-driven warming. 



<h2 class="wp-block-heading" id="h-ocean-loses-its-grip-on-carbon">Ocean loses its grip on carbon</h2>



The Southern Ocean’s days as a reliable carbon sink may be numbered. The study suggests that by mid-century, GHG emissions will dominate wind patterns, mixed-layer depth, and overturning circulation.



In the past, ozone depletion drove the winds. It pushed carbon-rich waters to the surface, reducing the ocean’s capacity to absorb more carbon. 



But as the 21st century unfolds, GHGs will take the lead. Temperature changes, not wind shifts, will determine how much carbon the ocean can hold.



The research delivers a clear message and the findings serve as a stark reminder. The Southern Ocean's ability to absorb carbon depends on emissions, temperature, and circulation. 



The study was funded by the UK Natural Environment Research Council (<a href="https://www.ukri.org/councils/nerc/" target="_blank" rel="noreferrer noopener">NERC</a>) and the <a href="https://royalsociety.org" target="_blank" rel="noreferrer noopener">Royal Society</a>. The findings are published in the journal <a href="https://www.science.org/doi/10.1126/sciadv.adr3589" target="_blank" rel="noreferrer noopener">Science Advances</a>.



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Rising emissions weaken carbon storage in the Southern Ocean

The Southern Ocean, vast and cold, swallows more carbon than...

You grab a snack, tear open the package, and munch away. But have you ever wondered what might be slipping into your food? Synthetic chemicals sneak in through packaging, processing, and storage. You can’t see these chemicals, but they are there, and they’re raising serious health concerns.



A study published in the journal Nature Medicine dives into the hidden world of <a href="https://www.earth.com/news/many-people-are-willing-to-switch-to-plant-based-food-to-save-the-climate/" target="_blank" rel="noreferrer noopener">food</a> contaminants. 



The research was not just focused on preservatives and additives. The team studied chemicals that come from food packaging and contact materials - the plastics, metals, and papers that wrap, store, and process what we eat.



<h2 class="wp-block-heading" id="h-synthetic-chemicals-in-food">Synthetic chemicals in food</h2>



Synthetic chemicals are gatecrashers in our food <a href="https://www.earth.com/news/coal-emissions-threaten-indias-food-security/" target="_blank" rel="noreferrer noopener">system</a>. They don’t come from ingredients. They come from the packaging, the containers, and the processing equipment. 



Bisphenols, phthalates, PFAS - these chemicals don’t just sit there. They migrate, moving from plastic wrap into your sandwich, from the can lining into your soup.



It turns out, the more ultra-processed <a href="https://www.earth.com/news/earth-day-2025-what-were-really-fighting-for/" target="_blank" rel="noreferrer noopener">foods</a> you eat, the higher your exposure. These foods aren’t just packed with artificial flavors and preservatives. Ultra-processed foods are also packed in materials that leach synthetic chemicals.



<h2 class="wp-block-heading" id="h-chemicals-hidden-in-food-packaging">Chemicals hidden in food packaging </h2>



Your meal passes through four critical stages before landing on your plate. The first stage is transportation, where food sits in containers lined with synthetic materials, allowing chemicals to leach into it.



Next comes processing. Here, machines made from plastic and metal come into direct contact with the food, increasing the risk of contamination.



The third stage is packaging. Plastic wraps and aluminum cans may seem harmless, but they can act as chemical conduits, allowing synthetic substances to migrate into the food.



Finally, there is preparation. Heating a plastic-wrapped <a href="https://www.earth.com/news/vicious-cycle-food-systems-both-suffer-from-and-cause-emissions/" target="_blank" rel="noreferrer noopener">meal</a> in the microwave can exacerbate chemical leaching, effectively delivering those contaminants straight to your table.



<h2 class="wp-block-heading" id="h-synthetic-chemical-delivery-system">Synthetic chemical delivery system</h2>



Ultra-processed <a href="https://www.earth.com/news/food-waste-has-a-surprising-impact-on-climate-change/" target="_blank" rel="noreferrer noopener">foods</a> are engineered for taste and convenience, but they’re also perfect carriers for synthetic chemicals.



Foods that come in contact with synthetic materials during every stage of production are more likely to end up with higher chemical loads. And that’s not all. 



The study connects these contaminants to serious health issues - cancers, heart disease, metabolic disorders, and more.



<h2 class="wp-block-heading" id="h-public-health-blind-spot">Public health blind spot</h2>



Jane Muncke, the study’s lead author from <a href="https://foodpackagingforum.org" target="_blank" rel="noreferrer noopener">Food Packaging Forum</a> Foundation, said that the evidence is becoming more clear that today’s packaged ultra-processed foods contain many synthetic chemicals and microplastics from various sources.



The presence of these chemicals is well-documented, and their harmful effects are clear. Yet, regulatory frameworks remain inadequate, barely addressing the full scope of the problem.



<h2 class="wp-block-heading" id="h-outdated-testing-methods">Outdated testing methods </h2>



Testing for these chemicals isn’t as straightforward as it sounds. Most testing methods are outdated, designed for known contaminants. 



But what about the ones we haven’t identified yet? The study pushes for more advanced testing methods that can catch emerging chemicals and microplastics before they slip through regulatory cracks.



Packaging is supposed to protect food. But what if it’s doing the opposite? Plastic containers, metal cans, and even paper wrappers can all leach chemicals into food. 



Redesigning these materials for safety isn’t just a nice idea - it’s a necessity. The study urges policymakers to push for safer, more sustainable packaging alternatives.



<h2 class="wp-block-heading" id="h-rethinking-food-safety">Rethinking food safety</h2>



Muncke explained that there's a broader issue - one that extends beyond just individual chemicals. She noted that the health impacts of this type of food contamination are currently under-appreciated and under-studied. 



"The scientific evidence shows a need for adopting a holistic approach to policymaking, that integrates considerations of planetary and human health, including hazardous FCCs and their impacts on health," said Muncke.



"All food packaging, processing equipment, and other food contact materials need to be adequately tested for their safety with regard to migrating food contact chemicals and microplastics using modern testing methods."



<h2 class="wp-block-heading" id="h-where-do-we-go-from-here">Where do we go from here?</h2>



If we keep eating ultra-processed foods, we keep ingesting synthetic chemicals. The study lays it out clearly - we need safer packaging, stricter testing, and stronger regulations. But we also need to rethink what we eat. 



Ultra-processed foods might be convenient, but they come with invisible risks. Maybe it’s time to take a closer look at that snack in your hand and consider what may be hiding inside.



The study is published in the journal <a href="https://www.nature.com/articles/s41591-025-03697-5" target="_blank" rel="noreferrer noopener">Nature Medicine</a>.



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Food packaging is leaking harmful chemicals into meals

You grab a snack, tear open the package, and munch...

Climate change solutions might be closer than we think - not in labs or remote forests, but in the microbes living in our homes. James Henriksen, a microbiologist at <a href="https://www.colostate.edu" target="_blank" rel="noreferrer noopener">Colorado State University</a>, believes the secret to fighting climate change could be hiding in dishwashers, air conditioners, and water heaters.



Henriksen wants everyone to join the hunt for extremophiles - organisms that thrive in extreme <a href="https://www.earth.com/news/climate-wins-in-2025-came-from-unexpected-places/" target="_blank" rel="noreferrer noopener">conditions</a>. They’re tiny, they’re tough, and some might be surprisingly useful.



These microbes have adapted to harsh environments, evolving traits that could potentially absorb carbon dioxide or clean up pollutants.



<h2 class="wp-block-heading" id="h-home-microbes-fighting-climate-change">Home microbes fighting climate change</h2>



<a href="https://citsci.org/projects/the-extremophile-campaign-in-the-wild/" target="_blank" rel="noreferrer noopener">The Extremophile Campaign: In Your Home</a> is a new initiative from CitSci, the Two Frontiers Project, and SeedLabs. It kicked off in October, rallying citizen scientists to search for hidden organisms.



“We believe that we have found new organisms, and we know that they have unique characteristics purely from the fact that they're growing and thriving in some of these unusual environments,” Henriksen said. Already, the campaign has led to some intriguing <a href="https://www.earth.com/news/south-africas-land-is-continuously-rising-as-water-disappears-climate-change/" target="_blank" rel="noreferrer noopener">discoveries</a>.



<h2 class="wp-block-heading" id="h-a-microbe-with-a-big-appetite">A microbe with a big appetite</h2>



Deep in the volcanic ocean vents off the island of Vulcano, Henriksen and his team stumbled upon Chonkus. This cyanobacterium isn’t just any microbe. It devours carbon dioxide and then sinks, locking away CO2 in the ocean depths.



Unlike plants, Chonkus can absorb far more CO2, using photosynthesis to turn the gas into biomass. It’s a microscopic powerhouse that might one day help mitigate <a href="https://www.earth.com/news/todays-children-will-face-more-climate-extremes-than-ever-before/" target="_blank" rel="noreferrer noopener">climate</a> change.



Henriksen isn’t surprised. “Half the air you're breathing comes from microbes,” he said. “They play essential roles in carbon and nitrogen cycles.”



<h2 class="wp-block-heading" id="h-mapping-the-microbes">Mapping the microbes</h2>



Henriksen co-founded the Two Frontiers Project to hunt for microbes in extreme environments – from the depths of the ocean to outer space. But what about the extreme environments right under our noses?



“There’s not just unknown species,” he said. “It’s like there’s a rainforest everywhere you look, and we know almost nothing about the organisms there and what they can do.”



Our homes, it turns out, are teeming with unseen life - and Henriksen wants us to pay attention.



<h2 class="wp-block-heading" id="h-microbes-hidden-in-the-home">Microbes hidden in the home</h2>



If you’re feeling brave, take a closer look at your appliances. What’s lurking inside your dishwasher or around the base of your water heater? If it’s slimy, crusty, or gooey, Henriksen wants to hear about it.



Instead of scrubbing away the weird spots and unpleasant odors, you can help scientists by documenting them. That slimy film? It could be home to a whole community of extremophiles - microbes that might hold the key to <a href="https://www.earth.com/news/climate-change-is-now-impacting-earths-rotation/" target="_blank" rel="noreferrer noopener">climate solutions</a>.



Participating is easy. Snap a photo of your odd discovery. Fill out an online survey at <a href="https://citsci.org/" target="_blank" rel="noreferrer noopener">CitSci.org</a>. If researchers need more information, they’ll send a collection kit.



Henriksen’s team will then analyze the samples using metagenomic sequencing. Each microbe’s DNA will be studied, cataloged, and possibly saved for future research. Some samples might even lead to new scientific breakthroughs.



<h2 class="wp-block-heading" id="h-what-s-in-the-slime">What's in the slime?</h2>



Metagenomic sequencing sounds complex, but the goal is simple: figure out what’s living in that slimy mess. Henriksen and his team are looking for microbes that can absorb CO₂, degrade <a href="https://www.earth.com/news/pollutants-from-fossil-fuels-are-embedded-in-coral-skeletons/" target="_blank" rel="noreferrer noopener">pollutants</a>, or perform other useful tasks.



The DNA data will be stored for future study. Some organisms might be cultivated and tested further. Every sample holds the potential for new discoveries.



<h2 class="wp-block-heading" id="h-nature-s-hidden-survivors">Nature's hidden survivors </h2>



Beyond homes, the Extremophile Campaign: In the Wild asks people to keep an eye out for microbial hotspots in nature. Springs in places like Colorado and California often contain unusual chemistry - acidic water, carbonation, and, yes, slime.



"Life is surviving and thriving in this hot water, in water that is as carbonated as soda pop and as acidic as lemon juice,” Henriksen said. “Microbes are pulling high concentrations of CO₂ out of the water, out of the air, and they're building that slime or the green algae that you see.”&nbsp;



If you spot something slimy, crusty, or just plain weird, the researchers want to know.



<h2 class="wp-block-heading" id="h-a-platform-to-fight-climate-change-nbsp">A platform to fight climate change&nbsp;</h2>



Both extremophile campaigns run through CitSci.org, a platform that connects researchers with citizen scientists. The site was developed at Colorado State University’s Natural Resource Ecology Laboratory two decades ago and now hosts nearly 1,500 projects.



“CitSci has been an amazing partner in helping get this up and running,” Henriksen said. 



Through CitSci, Henriksen hopes to gather data from as many people and places as possible. With more eyes on the ground, the chances of finding new microbial allies in the climate fight increase.



<h2 class="wp-block-heading" id="h-your-gunk-might-save-the-planet">Your gunk might save the planet</h2>



Henriksen sees potential in every home. That gross gunk in your appliance? It might contain the next Chonkus – a microbe that could capture <a href="https://www.earth.com/news/mountains-both-carbon-sinks-and-carbon-sources/" target="_blank" rel="noreferrer noopener">carbon</a> or break down pollutants. All it takes is a photo, a survey, and a bit of curiosity.



“We believe that everybody can contribute and participate in science," Henriksen said. &nbsp;



From volcanic vents to kitchen sinks, the next big climate solution might be hiding in plain sight - and researchers want you to help find it.



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Slime found in home appliances could help fight climate change

Climate change solutions might be closer than we think -...

Language is often considered the hallmark of human intelligence, a complex system that enables us to share thoughts, express emotions, and convey intricate messages.



For years, scientists believed that recursion - the ability to nest phrases within phrases - was a defining characteristic of human language. However, new research challenges this view, suggesting that wild orangutans also use recursive communication.



This discovery offers a glimpse into the evolutionary origins of human language, potentially dating back millions of years. By studying Sumatran <a href="https://www.earth.com/news/orangutan-mothers-have-unique-parenting-styles-like-humans/" target="_blank" rel="noreferrer noopener">orangutans</a>, researchers have found evidence of structured vocal patterns previously thought to be exclusive to humans. 



This breakthrough not only reshapes our understanding of primate communication but also provides critical insights into how complex language structures may have developed.



<h2 class="wp-block-heading" id="h-the-roots-of-human-language">The roots of human language</h2>



Language thrives on repetition. Imagine a chain of events like this: “This is the house that Jack built, that sheltered the cat, that chased the mouse, that stole the cheese.”



Each segment builds on the one before, stacking phrases to form a layered, connected structure. This pattern is called recursion.



The pattern stacks phrases like Russian nesting dolls. Each layer connects to the next, creating a complex yet understandable message. Humans use it all the time, embedding clauses within sentences to convey rich and detailed thoughts.



<h2 class="wp-block-heading" id="h-orangutans-use-recursion-too">Orangutans use recursion too</h2>



For years, scientists believed that only humans could use such layered communication. But researchers from <a href="https://warwick.ac.uk" target="_blank" rel="noreferrer noopener">The University of Warwick</a> have uncovered a startling discovery. Sumatran orangutans, it turns out, use the same pattern.



“When analyzing the vocal data of alarm calls from female Sumatran <a href="https://www.earth.com/news/international-orangutan-day-2024-protecting-the-people-of-the-forest/" target="_blank" rel="noreferrer noopener">orangutans</a>, we found that the rhythmic structure of orangutans’ sounds made were self-embedded across three levels - an impressive third-order recursion,” noted Dr. Chiara De Gregorio, who led the study.



In other words, orangutans aren’t just making noise. They’re stacking vocal sounds, creating layers that echo the structure of human language.



<h2 class="wp-block-heading" id="h-language-patterns-in-orangutan-calls">Language patterns in orangutan calls</h2>



The <a href="https://www.earth.com/news/wild-orangutan-treats-his-facial-wound-with-a-healing-plant/" target="_blank" rel="noreferrer noopener">orangutans</a>’ calls didn’t follow a single, simple rhythm. Instead, they built three distinct layers. 



First, they strung together small sounds, forming short sequences. Next, they combined these sequences into longer, more complex bouts. Finally, they arranged those bouts into extended, rhythmic series.



Each level nested within the next, forming a layered structure. And it wasn’t random. The rhythm changed based on the type of threat the orangutans faced.



<h2 class="wp-block-heading" id="h-orangutans-use-rhythm-as-a-tool">Orangutans use rhythm as a tool</h2>



Picture a tiger lurking nearby. The orangutan’s calls grow rapid, urgent, and insistent. Now, imagine a less direct threat - a piece of cloth with bright spots. The calls slow down, becoming irregular, almost hesitant.



This adaptability is no accident. <a href="https://www.earth.com/news/most-endangered-primate-species-identified-in-new-report/" target="_blank" rel="noreferrer noopener">Orangutans</a> use rhythm as a tool, adjusting their vocal patterns to fit the situation. 



Dr. De Gregorio and her team noticed these shifts, hinting that orangutans are communicating specific information about their surroundings.



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



If recursion exists in orangutan calls, what does that mean for us? Dr. De Gregorio sees it as a glimpse into our evolutionary past.



“This discovery shows that the roots of one of the most distinctive features of human language - recursion - was already present in our evolutionary past,” she noted.



In other words, recursion might not be a human invention. It could be a skill we inherited from ancient ancestors - a skill that orangutans still use today.



<h2 class="wp-block-heading" id="h-orangutan-connection-to-human-language">Orangutan connection to human language</h2>



Language didn’t appear overnight. It evolved, layer by layer, like the vocal sequences of the orangutans. The researchers believe that studying these calls could help us understand how human language began.



Orangutans, with their recursive vocal structures, may hold clues to how our ancestors communicated. Perhaps they, too, stacked sounds, building rhythms to convey complex ideas. 



Over time, these rhythms could have evolved into more structured language systems.



<h2 class="wp-block-heading" id="h-the-bigger-picture">The bigger picture</h2>



Why does any of this matter? Because if recursion isn’t uniquely human, then neither is the complexity of thought it enables. 



Orangutans are showing us that the seeds of language run deeper than we thought, stretching back millions of years.



By preserving these animals and their habitats, we’re not just protecting a species. We are safeguarding a link to our own evolutionary history - a history told through layers of sound, rhythm, and meaning.



<h2 class="wp-block-heading" id="h-language-research-in-primates">Language research in primates</h2>



Dr. De Gregorio and her team have opened a door to new questions. How widespread is recursion among non-human primates? Do other species use similar vocal structures?



For now, the calls of Sumatran orangutans echo through the forest, carrying a message that’s both ancient and new. And in those layered rhythms, we might just hear the distant roots of our own language, reverberating through time.



The study is published in the journal <a href="https://nyaspubs.onlinelibrary.wiley.com/doi/abs/10.1111/nyas.15373" target="_blank" rel="noreferrer noopener">Annals of the New York Academy of Sciences</a>.



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Orangutans use complex vocal patterns found in human language

Language is often considered the hallmark of human intelligence, a...

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



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



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



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



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



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



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



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



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



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



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

Is chocolate the next nutritional powerhouse?

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

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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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

Flu viruses are more flexible than expected

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



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



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



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



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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

Detecting mercury contamination with the tap of a finger

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



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



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



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



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



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



Video/ Image Credit: European Space Agency&nbsp;



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



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

Kainji Lake in north central Nigeria

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<h1>Snake Plant</h1>
The snake plant is known as one of the best for filtering out formaldehyde, which is common in cleaning products. Low light and humidity are the ideal conditions for the snake plant.

Snake Plant

<h1>Aloe Vera </h1>
In addition to many natural health benefits such as healing wounds and easing sunburn, the aloe plant helps combat formaldehyde and benzene. Place it in a sunny window for best results.

Snake Plant

Snake Plant

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