Today's Image of the Day from the European Space Agency features a Copernicus map of scorching summer temperatures across southern Europe.



“A powerful heatwave has been gripping large parts of southern Europe and North Africa, pushing air temperatures beyond seasonal norms and triggering widespread health and wildfire alerts. Among the hardest-hit countries are Spain, France, Italy, Greece, Cyprus, and Algeria,” said <a href="https://www.esa.int/ESA_Multimedia/Images/2025/07/Southern_Europe_s_land_and_sea_sizzles">ESA</a>.



“This image, a mosaic from five overlapping orbital passes in the morning of 29 June 2025, was captured by the <a href="https://www.esa.int/Applications/Observing_the_Earth/Copernicus/Sentinel-3">Copernicus Sentinel-3</a> mission’s Sea and Land Surface Temperature Radiometer.”&nbsp;



<h2 class="wp-block-heading" id="h-tracking-land-surface-temperatures-nbsp">Tracking land surface temperatures&nbsp;</h2>



According to ESA, the image reveals the temperature of the land surface - not air temperature.



Tracking land surface temperature is essential for predicting weather and climate patterns, assessing wildfire risk, helping <a href="https://www.earth.com/news/rising-temperatures-threaten-the-future-of-banana-farming/">farmers</a> plan irrigation, and informing urban design strategies to reduce heat.



“Unlike measurements of air temperature, this satellite instrument measures the actual thermal energy emitted from Earth’s surface, which typically registers higher than air temperatures.”



<h2 class="wp-block-heading" id="h-heat-dome-over-western-europe-nbsp">Heat dome over Western Europe&nbsp;</h2>



The image includes information from the Copernicus Marine Service, which shows that <a href="https://www.earth.com/news/ocean-temperatures-are-rising-faster-than-expected-and-likely-to-accelerate/">surface temperatures</a> are also hot across the Mediterranean Sea.



The ongoing heatwave is fueled by a high-pressure system stalled over Western Europe, known as a “heat dome.” This system traps hot, dry air beneath it, causing temperatures to rise steadily.&nbsp;



As it moves eastward, the dome pulls in even more hot air from North Africa, intensifying the extreme heat across the region.



<h2 class="wp-block-heading" id="h-heat-dome-over-the-united-states-nbsp">Heat dome over the United States&nbsp;</h2>



In June 2025, a heat dome developed over the central and eastern United States. It began forming around June 20 and persisted through the week.



The heat dome covered a large part of the country - from the Great Plains through the Midwest, Upper Midwest, Ohio and Tennessee River Valleys - and extended into the Mid‑Atlantic and Northeast regions.



More than 280 daily high-temperature records were shattered across the U.S., affecting some 130 million people under <a href="https://www.earth.com/news/extreme-heat-impacts-our-daily-routines-and-transportation/">heat warnings</a> or advisories.&nbsp;



Cities like New York, Baltimore, Philadelphia, Boston, Newark, Providence, and Raleigh saw triple-digit highs - some reaching more than 105 degrees.



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



The heat dome not only caused dangerous daytime highs but also oppressive night-time warmth, with low temperatures often staying above 80 °F due to trapped heat. 



This persistent warmth strained power grids, led to emergency declarations, and triggered significant public health concerns.



Infrastructure suffered too: roads buckled in Missouri and softened asphalt sank vehicles in New York City, while a Baltimore Amtrak train stalled in a tunnel from the heat. 



Emergency measures included power reductions, heat shelters, and utility advisories in several states.



<h2 class="wp-block-heading" id="h-heat-domes-and-climate-change">Heat domes and climate change</h2>



Climate scientists emphasize that heat domes are fueled by anthropogenic <a href="https://www.earth.com/news/climate-change-earth-energy-imbalance-temperature-rise/">climate change</a>. These high-pressure patterns are occurring more frequently and enduring longer due to warming oceans, Arctic amplification, and altered jet stream behavior.&nbsp;



As global temperatures rise, the atmosphere can hold more moisture and energy, which intensifies heatwaves and makes them more persistent.&nbsp;



In particular, the weakened and meandering jet stream - a result of a warming Arctic - is allowing systems like heat domes to stall over regions for days or even weeks.



<h2 class="wp-block-heading" id="h-adapting-to-a-hotter-future">Adapting to a hotter future</h2>



Recent climate models show that events like the June 2025 heat dome (once considered rare), are becoming increasingly common.&nbsp;



What used to be a one-in-100-year heat event in many U.S. cities may now occur once a decade or even more often. This shift has serious implications not just for human health, but also for infrastructure, agriculture, and energy systems.&nbsp;



Power grids are pushed to their limits, roads and railways buckle under extreme heat, and crops suffer from both high temperatures and water stress.



Public health officials are especially concerned about the cumulative toll of prolonged <a href="https://www.earth.com/news/extreme-heat-is-pushing-parts-of-earth-beyond-human-survival/">extreme heat</a>. 



Nights that remain hot offer little relief and are particularly dangerous for vulnerable populations such as the elderly, young children, and people with chronic health conditions. 



Without sustained adaptation efforts - such as redesigning cities to reduce heat retention, expanding access to cooling centers, and modernizing energy infrastructure - the human and economic cost of extreme heat is expected to grow significantly in the coming decades.



Image Credit: ESA



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Heat dome scorches Southern Europe 

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

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Eagle Nebula: Carving light from darkness

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



The Rosette Nebula is a vast cloud of gas and dust located in the constellation Monoceros, also known as the Unicorn.



Shaped like a blooming rose in deep space, it lies about 5,200 light-years from Earth and spans roughly 100 light-years in diameter.&nbsp;



<h2 class="wp-block-heading" id="h-image-of-the-rosette-nebula">Image of the Rosette Nebula </h2>



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



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



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



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



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



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



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



<h2 class="wp-block-heading" id="h-nebulae-that-are-similar-to-rosette">Nebulae that are similar to Rosette</h2>



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



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



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



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



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



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



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



<h2 class="wp-block-heading" id="h-history-of-the-rosette-nebula">History of the Rosette Nebula </h2>



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



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



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



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



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



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



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



Image Credit: ESA



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Rosette Nebula: A flower blooming in deep space

Today's Image of the Day from the European Space Agency features UGC 5460, a spiral galaxy that is located about 60 million light-years away in the constellation Ursa Major.&nbsp;



“This image combines four different wavelengths of light to reveal UGC 5460’s central bar of stars, winding spiral arms and bright blue star clusters. Also captured in the upper left-hand corner of this image is a far closer object: a star just 577 light-years away in our own galaxy,” said <a href="https://www.esa.int/ESA_Multimedia/Images" target="_blank" rel="noreferrer noopener">ESA</a>.



“UGC 5460 has hosted two recent supernovae named SN 2011ht and SN 2015as. It’s because of these two stellar explosions that Hubble targeted this galaxy, collecting data for three observing programmes that aim to study various kinds of supernovae.”&nbsp;



<h2 class="wp-block-heading" id="h-a-core-collapse-supernova-nbsp">A core-collapse supernova&nbsp;</h2>



SN 2015as is an example of a core-collapse supernova. This type of <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernova</a> occurs when the core of a massive star - typically with more than 8 times the mass of the sun - can no longer support its own gravity after exhausting its nuclear fuel. 



This causes the core to collapse under its own weight, leading to an extremely violent explosion. The collapse triggers the release of an enormous amount of energy, expelling the outer layers of the star into space.



In the aftermath of the explosion, a dense <a href="https://www.earth.com/news/shockingly-bright-carbon-monoxide-detected-in-supernova-remnant/" target="_blank" rel="noreferrer noopener">remnant</a> is created. This is often a neutron star or black hole, depending on the mass of the original star. Core-collapse supernovae are some of the most powerful events in the universe.



According to ESA, Hubble observations of SN 2015as will help researchers understand what happens when the expanding shockwave of a <a href="https://www.earth.com/news/supernova-dandelion-year-1181-leaves-behind-zombie-star-defying-death/" target="_blank" rel="noreferrer noopener">supernova</a> collides with the gas that surrounds the exploded star.



<h2 class="wp-block-heading" id="h-rare-stars-with-large-eruptions-nbsp">Rare stars with large eruptions&nbsp;</h2>



“SN 2011ht might have been a core-collapse supernova as well, but it could also be an impostor called a luminous blue variable. Luminous blue variables are rare stars that experience eruptions so large that they can mimic supernovae,” noted ESA.



“Crucially, luminous blue variables emerge from these eruptions unscathed, while stars that go supernova do not. Hubble will search for a stellar survivor at SN 2011ht’s location, and the explosion’s identity may be revealed at last.”



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



Spiral galaxies are some of the most recognizable and beautiful structures in the universe. They are known for their distinctive arms that spiral outward from a central bulge.&nbsp;



These galaxies are typically composed of stars, gas, dust, and dark matter. The arms are often sites of intense <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>, where clouds of gas collapse to form new stars. 



In the center of a spiral galaxy lies a dense concentration of older stars and, often, a supermassive black hole.



<h2 class="wp-block-heading" id="h-structure-of-a-spiral-galaxy-nbsp">Structure of a spiral galaxy&nbsp;</h2>



The structure of a spiral galaxy is generally divided into three main components: the disk, the bulge, and the halo.&nbsp;



The disk is where the spiral arms are located and contains most of the galaxy's visible stars and interstellar medium.&nbsp;



The bulge is a tightly packed region of older stars at the core, and the halo consists of a sparse collection of stars and globular clusters that surround the galaxy.&nbsp;



Spiral galaxies can be classified into different types based on the tightness and number of their spiral arms, as well as the size of their central bulge.



<h2 class="wp-block-heading" id="h-the-milky-way-galaxy">The Milky Way galaxy</h2>



Our solar system is located within a large spiral galaxy known as the Milky Way. The name refers to its appearance as a dim, milky band of light stretching across the night sky.&nbsp;



The term "Milky Way" comes from ancient Greek mythology, where it was associated the goddess Hera's milk spilling into the sky. In Greek, it was called "Galaxias Kyklos," meaning "milky circle."&nbsp;



Spanning about 100,000 light-years in diameter, the Milky Way is composed of stars, gas, dust, and dark matter. The galaxy has a distinct disk shape with spiral arms that wind outward from a central bulge, which houses a supermassive <a href="https://www.earth.com/news/milky-ways-black-hole-unleashes-mysterious-flares/" target="_blank" rel="noreferrer noopener">black hole</a>. 



Our sun is located in one of the spiral arms - known as the Orion Arm - positioned roughly halfway from the center to the outer edge.&nbsp;



The Milky Way is part of a small group of galaxies called the Local Group, which includes the Andromeda Galaxy and several smaller galaxies.



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Hubble views a spiral galaxy with stellar explosions

Today's Image of the Day from NASA Earth Observatory features Lake Chad in central Africa. The photograph was taken by an astronaut aboard the International Space Station.



According to <a href="https://earthobservatory.nasa.gov/images/154407/lake-chads-water-wetlands-and-dunes" target="_blank" rel="noreferrer noopener">NASA</a>, Lake Chad once ranked among the largest natural lakes in the world. It was a critical resource for millions of people and animals, supporting agriculture and fishing across the region.&nbsp;



Lake Chad straddles the borders of Chad, Nigeria, Niger, and Cameroon. The shallow <a href="https://www.earth.com/news/lakes-are-warming-toward-the-point-of-no-return/" target="_blank" rel="noreferrer noopener">lake</a> is primarily fed by the Chari River, which brings water from the Central African Republic. 



The water levels are also influenced by seasonal rainfall. The rainfall patterns vary significantly across the basin but generally follow a wet-dry seasonal cycle.



<h2 class="wp-block-heading" id="h-environmental-decline-and-shrinkage-nbsp">Environmental decline and shrinkage&nbsp;</h2>



From the 1960s to the early 2000s, the lake lost more than 90 percent of its surface area. It transformed from a vast expanse of open water into a patchwork of wetlands, reed beds, and scattered pools.&nbsp;



This environmental decline has had severe consequences for local communities, leading to food and <a href="https://www.earth.com/news/global-water-security-relies-on-the-origins-of-rainfall/" target="_blank" rel="noreferrer noopener">water insecurity</a>, loss of livelihoods, and increasing competition over scarce resources.



“Ongoing droughts and the rising demand for fresh water have shrunk the lake to less than a tenth of the area it covered in the middle of the last century,” noted NASA.



“Although the lake has experienced dry and wet periods for thousands of years, there has been a significant decline in the amount of lake water available since the 1960s.”



<h2 class="wp-block-heading" id="h-conflict-culture-and-economy">Conflict, culture, and economy</h2>



Lake Chad is a geopolitical hotspot. The region has been affected by conflict, including the insurgency led by Boko Haram, which has displaced millions and further complicated efforts to manage and protect the lake’s fragile ecosystem.&nbsp;



Despite these challenges, regional governments and international organizations are working to restore and sustain the lake, including ambitious proposals to divert water from the Congo River basin.



Culturally and economically, Lake Chad remains vital. It is a hub for trade and social exchange among diverse ethnic groups and continues to provide fish and fertile land despite its reduced size.&nbsp;



The future of Lake Chad hinges on sustainable water management, <a href="https://www.earth.com/news/climate-extremes-alter-how-sunlight-travels-through-clear-lakes/" target="_blank" rel="noreferrer noopener">climate</a> resilience, and political cooperation across national boundaries.



<h2 class="wp-block-heading" id="h-evolution-of-lake-chad-nbsp">Evolution of Lake Chad&nbsp;</h2>



According to NASA, the evolution of Lake Chad has been documented by astronaut photography over the past 60 years.&nbsp;



“During the Apollo 7 mission in 1968, an astronaut acquired an oblique <a href="https://eol.jsc.nasa.gov/SearchPhotos/photo.pl?mission=AS07&amp;roll=8&amp;frame=1932" target="_blank" rel="noreferrer noopener">photograph</a> of the lake as one large body of water. In 1982, another <a href="https://eol.jsc.nasa.gov/SearchPhotos/photo.pl?mission=STS005&amp;roll=39&amp;frame=1022" target="_blank" rel="noreferrer noopener">photo</a> from the space shuttle mission STS-5 recorded receding water levels and encroaching sand dunes.”



“A <a href="https://eol.jsc.nasa.gov/SearchPhotos/photo.pl?mission=ISS042&amp;roll=E&amp;frame=244403" target="_blank" rel="noreferrer noopener">photo</a> taken in 2015 during space station Expedition 42 captured the lake’s remaining waters and wetlands in dark green, blue, and brown, contrasting with the sandy shades of the surrounding land.”&nbsp;



<h2 class="wp-block-heading" id="h-wildlife-of-lake-chad">Wildlife of Lake Chad</h2>



Lake Chad still supports wildlife, though species diversity and abundance have declined significantly due to ecosystem degradation



The lake and its surrounding wetlands are home to several species of fish, including tilapia, catfish, and Nile perch, which are important both ecologically and economically.&nbsp;



These fish support a major regional fishing industry, although overfishing and changes in water conditions have put pressure on fish populations.



Birds are another key component of the ecosystem. The lake serves as a crucial habitat and stopover point for <a href="https://www.earth.com/news/birds-may-be-using-quantum-physics-for-migration/" target="_blank" rel="noreferrer noopener">migratory birds</a> traveling along the African-Eurasian flyway. 



Species such as herons, storks, ducks, and geese can be found in the region, especially during the wet season when parts of the lake flood and create rich feeding grounds.



Mammals that depend on the surrounding floodplains and wetlands include hippos and various antelope species, yet their numbers have declined.&nbsp;



<h2 class="wp-block-heading" id="h-conservation-efforts-and-challenges">Conservation efforts and challenges</h2>



Reptiles like Nile crocodiles and turtles also inhabit the lake's waters and marshy areas. In the past, larger wildlife such as elephants and lions may have roamed the wider Lake Chad basin, but they are now mostly gone from the immediate lake area due to habitat loss and human activity.



Despite these challenges, Lake Chad remains an important, yet increasingly fragile, refuge for wildlife in a region where water and natural habitats are becoming more scarce.&nbsp;



Conservation efforts aim to balance the needs of people and <a href="https://www.earth.com/news/thousands-of-freshwater-species-are-threatened-with-extinction/" target="_blank" rel="noreferrer noopener">wildlife</a>, but the success of such efforts depends on managing the lake’s limited resources in the face of climate change, political instability, and population growth.



Image Credit: NASA Earth Observatory&nbsp;



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Lake Chad: A vanishing lifeline in Central Africa

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

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.&nbsp;



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.&nbsp;



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 the bar plays a crucial role in the dynamics and evolution of the Milky Way by funneling gas inward toward the galactic center. This can feed star formation and fuel the supermassive black hole at the core. 



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.&nbsp;



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.&nbsp;



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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Barred spiral galaxy glows in the constellation Virgo

The Slender Blind Snake, or <a href="https://en.wikipedia.org/wiki/Leptotyphlopidae">Leptotyphlopidae</a>, rarely exceeds 30 cm (just under 12 inches) in length. They are found in southwestern North America, Central and <a href="http://www.earth.com/news/south-american-monkeys-face-extinction/">South America</a>, Africa, Asia, in habitats that range from arid areas to rainforests.

Slender Blind Snake

Smiling,Mature,Mother,And,Adult,Daughter,On,Sofa,In,Living

Imagine chatting over coffee with your grandmother when she pauses mid-sentence and mutters, “Oh, what’s the word I’m looking for?” That familiar snag - scientists call it word-finding difficulty (WFD) - often arrives long before gray hair or reading glasses. It can feel trivial, yet it quietly hints at how the brain ages.



Those hesitations pop up everywhere, from grocery aisles to family reunions. They even slip into laboratory tasks designed to stress-test language. 



Far from mere annoyance, a faltering word can help clinicians spot trouble brewing in <a href="https://www.earth.com/news/pupil-size-during-sleep-decides-if-new-or-old-memories-are-replayed/">memory networks</a> years before other symptoms emerge.



<h2 class="wp-block-heading" id="h-word-finding-difficulty-wfd">Word-finding difficulty (WFD)</h2>



Early work at the <a href="https://www.utoronto.ca/" target="_blank" rel="noreferrer noopener">University of Toronto</a> and <a href="https://www.baycrest.org/" target="_blank" rel="noreferrer noopener">Baycrest Health Sciences</a> ties WFD to the same neural highways that falter in Alzheimer’s disease. 



Researchers note that slower speech, rather than the odd lapse, tracks most closely with overall cognitive health. 



Beyond disease, fresh evidence links verbal fluency to longevity; adults who keep words flowing live longer than peers whose speech grows hesitant.



Because everyday talk is complex, scientists break the puzzle into manageable pieces. 



Clues come from spontaneous pauses like “um,” “uh,” and from those frustrating “tip-of-the-tongue” moments when meaning is clear but the sound won’t surface. 



<h2 class="wp-block-heading" id="h-three-wfd-theories">Three WFD theories</h2>



One camp blames a global slowdown. The processing speed theory says an <a href="https://www.earth.com/news/aging-hotspot-found-in-the-brain-may-hold-the-key-to-longevity/">aging brain</a> resembles an old laptop that needs a beat to open each file. 



Neural transmissions still fire, just more leisurely, leading to extra silence before the right syllable appears.



Another view, the <a href="https://pubmed.ncbi.nlm.nih.gov/33934024/" target="_blank" rel="noreferrer noopener">inhibition deficit</a> hypothesis, argues that older adults struggle to hush irrelevant notions. Competing names or ideas intrude, and mental traffic control can’t wave them aside quickly. 



Yet real-world conversations rarely show a flood of wrong guesses, casting doubt on inhibition as the chief culprit.



A third explanation zooms straight into language. The <a href="https://www.researchgate.net/publication/319777924_Research_into_Tip_of_the_Tongue_State_Transmission_Deficit_Model_vs_Blocking_Hypothesis" target="_blank" rel="noreferrer noopener">transmission deficit</a> hypothesis pictures vocabulary as a layered web: concept at the top, word form in the middle, and sound at the bottom. 



Age loosens the link between the middle and bottom tiers, so the speaker knows the concept but can’t launch its sound. That fragile connection makes spoken naming harder than listening or reading, which rely on sturdier routes.



<h2 class="wp-block-heading" id="h-picture-word-game">Picture-word game</h2>



To probe these ideas, scientists use <a href="https://pubmed.ncbi.nlm.nih.gov/35389697/" target="_blank" rel="noreferrer noopener">picture-word interference</a> tasks. Volunteers see a picture - say, a dog - while a word flashes or plays. If that word is “cat,” its meaning overlaps and slows the answer. 



If it is “fog,” the shared consonant kick-starts articulation. This setup teases apart semantic and phonological forces without the messiness of free conversation.



Moving experiments online has boosted participation. Researchers turned the task into a fast-paced game, keeping attention high across all ages. 



Reaction times shrink into the millisecond range, revealing hiccups long before a listener hears any stumble.



<h2 class="wp-block-heading" id="h-what-125-volunteers-revealed">What 125 volunteers revealed</h2>



In one study, 125 adults aged 18 to 85 tackled the game, logged executive-function scores, and recorded natural chat for later analysis. 



Older participants slowed markedly when “cat” accompanied a dog image and enjoyed less help from a “fog” cue. Those patterns matched the weakened pathway predicted by the transmission deficit hypothesis.



Yet when daily speech samples were scored, neither semantic slowdown nor <a href="https://www.earth.com/news/speech-planning-how-our-brains-prepare-to-speak/">phonological</a> boost predicted real-life WFD. 



Instead, overall reaction time - the raw speed of pulling any word - stood out as the best indicator. The finding nudged attention back toward general <a href="https://www.earth.com/news/scientists-discover-the-speed-at-which-the-brain-processes-information/">processing speed</a>.



<h2 class="wp-block-heading" id="h-speed-outpaces-distraction">Speed outpaces distraction</h2>



Follow-up work confirmed that the cadence of ordinary talk mirrors cognitive vitality. The University of Toronto team found that people who spoke more slowly also scored lower on tasks requiring planning and focus, even when word-finding errors were rare. 



Crucially, pauses to chase a lost word did not track with decline; what mattered was how briskly sentences rolled once the right words appeared.



This distinction eases common worries. A brief hunt for a noun may simply reflect normal aging, whereas a gradual slowdown in fluent speech could wave a red flag earlier than memory tests. 



Clinicians now argue that talking speed belongs in standard cognitive checkups, alongside <a href="https://www.earth.com/news/how-you-position-your-arm-can-alter-blood-pressure-readings-according-to-scientists/">blood pressure</a> and reflex taps.



<h2 class="wp-block-heading" id="h-looking-ahead-to-early-detection">Looking ahead to early detection</h2>



The picture-word game offers a quick, engaging way to capture subtle shifts before they tip into impairment. Because it measures speed and accuracy together, it may outshine traditional naming lists for spotting risk early. 



<a href="https://www.earth.com/news/what-baby-talk-reveals-about-infant-learning/">Speech-analysis</a> software, already parsing recordings for millisecond pauses, could soon alert physicians when a patient’s verbal tempo drifts.



Meanwhile, everyday habits still matter. Conversational practice, storytelling, word games, and even learning new languages keep those neural pathways exercised. 



Just as daily walks support the heart, lively chatter supports the mind. And when a loved one stalls on a name, patience helps more than finishing the thought for them. 



Sometimes the right word arrives on its own schedule - one more reminder that brains, like conversations, thrive when given a little time to breathe.



The full study was published in the journal <a href="https://www.tandfonline.com/doi/full/10.1080/13825585.2024.2315774" target="_blank" rel="noreferrer noopener">Aging, Neuropsychology, and Cognition</a>.



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Scientists identify a speech pattern that is a clear indication of a person in cognitive decline

Imagine chatting over coffee with your grandmother when she pauses...

For nearly a century, brominated vegetable oil - better known as BVO - helped keep that sharp, zesty taste of citrus-flavored sodas evenly distributed from the first sip to the last. 



Most shoppers never noticed the name on ingredient lists, and few paused to wonder why a cooking oil had been blended with <a href="https://pubchem.ncbi.nlm.nih.gov/compound/Bromine" target="_blank" rel="noreferrer noopener">bromine</a>, a heavy chemical element more often associated with pool disinfectants than with beverages.



Over the past year, though, BVO has moved from obscurity into the spotlight. New toxicology studies forced the U.S. Food and Drug Administration (<a href="https://www.fda.gov/" target="_blank" rel="noreferrer noopener">FDA</a>) to take a hard second look at an additive it once allowed at up to 15 parts per million. 



The agency’s verdict set off a countdown: <a href="https://www.earth.com/news/soda-taxes-actually-work-improving-both-health-and-mindset/">all sodas</a> sold after August 2, 2025, must be BVO-free, shutting the door on a substance that first slipped into fizz back in the 1930s.



<h2 class="wp-block-heading" id="h-citrus-sodas-and-bvo">Citrus sodas and BVO</h2>



Public worries about <a href="https://cris.msu.edu/news/trending/trending-brominated-vegetable-oil-bvo/" target="_blank" rel="noreferrer noopener">brominated vegetable oil</a> started decades ago, when researchers spotted bromine accumulating in human tissue samples taken in the United Kingdom during the 1970s. Animal studies soon linked high BVO intakes with heart and behavioral problems. 



Even so, the FDA kept the ingredient on a short leash rather than banning it outright, capping concentrations and labeling it “interim” while scientists gathered more data. The arrangement limped along for half a century.



Fresh evidence tipped the scale. A 90-day study funded by the FDA and the National Institutes of Health (<a href="https://www.nih.gov/" target="_blank" rel="noreferrer noopener">NIH</a>) tracked rats fed diets ranging from zero to high levels of BVO. 



Bromine not only flooded their bloodstreams but also settled in the heart, liver, and body fat. Thyroid cells enlarged, thyroid-stimulating hormone climbed, and T4 hormone dipped, hinting at metabolic trouble ahead.



<h2 class="wp-block-heading" id="h-why-brominated-oils-raised-alarms">Why brominated oils raised alarms</h2>



<a href="https://www.earth.com/news/eating-seafood-helps-children-develop-better-social-behaviors/">Thyroid shifts</a> matter because that small gland choreographs energy levels, growth, and mood. When bromine crowds out iodine - its chemical cousin - hormone production stumbles. 



Researchers worry that even subtle, long-term interference could nudge people toward weight gain, sluggishness, and <a href="https://www.earth.com/news/unhealthy-diet-leaves-brain-feeling-foggy-frazzled-sad/">brain fog</a>. 



Because bromine accumulates rather than being flushed straight through, the risk grows the longer someone drinks BVO-laced sodas.



Most major brands ditched BVO years ago. PepsiCo pulled it from Gatorade in 2013 and from Mountain Dew soon after. Coca-Cola quietly reformulated Fanta and Powerade. 



Yet store-brand and regional citrus sodas sometimes clung to the old recipe. In mid-2024, Keurig Dr. Pepper still listed BVO in Sun Drop, though the company pledged to roll out a new formula before year’s end.



<h2 class="wp-block-heading" id="h-fda-ruling-s-impact-on-bvo-sodas">FDA ruling's impact on BVO sodas</h2>



<a href="https://foodsafety.gwu.edu/jim-jones">James Jones</a>, deputy commissioner for human foods, summed up the agency’s thinking: “The proposed action is an example of how the agency monitors emerging evidence and, as needed, conducts scientific research to investigate safety-related questions, and takes regulatory action when the science does not support the continued safe use of additives in foods.” 



The final rule arrived on July 3, 2024, and became effective a month later, with a one-year grace period to drain warehouses and reset production lines.



Between now and August 2, 2025, shoppers can still run into cans made before the deadline. 



The safest approach is old-fashioned label reading - look for “brominated vegetable oil” or “<a href="https://www.sciencedirect.com/science/article/abs/pii/0300483X76900512" target="_blank" rel="noreferrer noopener">brominated soybean oil</a>.” After that date, any product that still lists the additive will be pulled from shelves.



<h2 class="wp-block-heading" id="h-how-beverage-makers-responded">How beverage makers responded</h2>



For companies, swapping out BVO meant finding other ways to keep citrus oils suspended. Many turned to ingredients already common in European and Japanese drinks, where BVO has been banned for years. 



<a href="https://www.sciencedirect.com/science/article/abs/pii/S0278691597803055" target="_blank" rel="noreferrer noopener">Sucrose acetate isobutyrate</a> and glycerol ester of wood rosin (<a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC7009419/" target="_blank" rel="noreferrer noopener">GEWR</a>) emerged as the go-to solutions; both create a dense phase that marries well with fruit oils without relying on bromine. 



Because the substitutes have long safety records abroad, the transition proved smoother than earlier label rewrites involving artificial dyes.



Retailers responded in parallel. National grocery chains began flagging private-label SKUs that needed reformulation, giving suppliers early notice. 



Craft <a href="https://www.earth.com/news/ultra-processed-foods-like-soda-and-snacks-are-the-new-silent-killer/">soda makers</a>, eager to stand out in a crowded aisle, advertised “BVO-free” right on the front of the bottle, turning regulatory compliance into a selling point.



<h2 class="wp-block-heading" id="h-what-science-says-about-bvo">What science says about BVO</h2>



Several studies over the years had very similar results. Bromine lodged in organs after only three months, a blip compared with human drinking habits that can stretch across decades. 



The thyroid, sensitive to iodine balance, responded quickly. Researchers did not observe tumors or acute poisoning, but the hormonal disruptions alone convinced regulators that routine consumption no longer passed the sniff test.



Back in the 1950s, the FDA first labeled BVO “<a href="https://www.fda.gov/food/food-ingredients-packaging/generally-recognized-safe-gras" target="_blank" rel="noreferrer noopener">generally recognized as safe</a>,” largely because citrus sodas were already popular. 



By 1970, the agency had reversed its stance, restricting use to citrus drinks and setting the 15-parts-per-million ceiling. Subsequent studies, including one published on May 16, 2022, in Food and Chemical Toxicology, kept adding red flags. 



Taken together, the evidence portrays a slow-burn risk rather than an immediate hazard - yet that is exactly the kind of threat public health agencies try to prevent.



<h2 class="wp-block-heading" id="h-changes-in-the-u-s-food-code">Changes in the U.S. food code</h2>



The BVO saga hints at future shake-ups in the U.S. food code. The FDA is reassessing a roster of additives, with an eye toward automatic bans on <a href="https://www.earth.com/news/one-in-five-packaged-foods-in-the-u-s-contains-synthetic-dyes/">colorants that cause cancer</a> in animals. 



Speeding up that process would spare consumers from the long twilight period BVO endured. 



For beverage developers, the lesson is clear: lean on ingredients with global acceptance, and keep an eye on toxicology journals as closely as on flavor-trend reports.



By August 2025, American citrus sodas will taste the same to most palates, but the chemistry behind that flavor will have changed. 



With no more swimming pool disinfectants like bromine in your beverages, the drink industry inches toward simpler, more transparent labels - something shoppers have been thirsting for as much as the fizz itself.



The full study was published in the journal <a href="https://www.sciencedirect.com/science/article/abs/pii/S0278691522003350" target="_blank" rel="noreferrer noopener">Food and Chemical Toxicity</a>.



Read the <a href="https://www.fda.gov/food/food-additives-petitions/brominated-vegetable-oil-bvo" target="_blank" rel="noreferrer noopener">The U.S. FDA ruling on BVO</a>.



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Highly toxic soda ingredient, banned by the FDA in 2024, is still being used today

For nearly a century, brominated vegetable oil - better known...

Fish oil capsules have long been sold for heart and joint health, yet new evidence suggests they may also steady tempers and aggression.



A sweeping <a href="https://www.mdpi.com/2072-6643/13/7/2154" target="_blank" rel="noreferrer noopener">meta‑analysis</a> from the <a href="https://www.upenn.edu/" target="_blank" rel="noreferrer noopener">University of Pennsylvania</a> reports that a daily dose of omega‑3 fatty acids can shrink aggressive behavior by up to 28 percent. <a href="https://crim.sas.upenn.edu/people/adrian-raine" target="_blank" rel="noreferrer noopener">Adrian Raine</a>, a neurocriminologist at the university, led the study.



<h2 class="wp-block-heading" id="h-mood-memory-and-fish-oil">Mood, memory, and fish oil</h2>



Brains run on fat, and two key omega‑3 molecules, eicosapentaenoic acid (<a href="https://pubchem.ncbi.nlm.nih.gov/compound/Eicosapentaenoic-Acid" target="_blank" rel="noreferrer noopener">EPA</a>) and docosahexaenoic acid (<a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC10776907/" target="_blank" rel="noreferrer noopener">DHA</a>), slip into cell membranes, helping neurons fire smoothly.



Low tissue levels of these fats have been tied to mood swings and impulsive violence, while diets rich in cold‑water fish tend to show the opposite pattern.



Because the body converts plant‑based <a href="https://pubmed.ncbi.nlm.nih.gov/24898228/" target="_blank" rel="noreferrer noopener">alpha‑linolenic acid</a> to EPA and DHA inefficiently, researchers have wondered whether supplements could fill the gap. 



Small trials dating back to the 1990s hinted at behavioral benefits, but sample sizes were too thin to guide policy.



<h2 class="wp-block-heading" id="h-aggression-and-fish-oil">Aggression and fish oil</h2>



Raine’s team pored over 28 randomized controlled trials that enrolled 3,918 participates, from children to older adults. 



Across genders, diagnoses, dosages, and study lengths, the capsules produced a modest but reliable drop in both reactive and premeditated aggression.



“I think the time has come to implement omega‑3 supplementation to reduce aggression,” said Raine. 



The average effect size, about 0.22 on the standardized “g” scale, may sound small, yet public‑health experts note that even tiny behavioral shifts can matter when applied to millions.&nbsp;



<h2 class="wp-block-heading" id="h-the-chemistry-of-calm">The chemistry of calm</h2>



EPA and DHA dampen production of pro‑inflammatory molecules that sensitize the <a href="https://www.earth.com/news/how-your-brain-makes-a-decision-before-you-know-it/">brain</a>’s stress circuits. They also nudge serotonin and dopamine signaling toward a calmer set point, offering a biochemical explanation for the behavioral change.



Notably, the analysis found benefits at doses as low as 250 milligrams of combined EPA and DHA, an amount found in a single soft gel. 



Higher intakes did not guarantee bigger gains, hinting that individual genetics and baseline diet modulate the response.



<h2 class="wp-block-heading" id="h-the-omega-imbalance">The omega imbalance</h2>



Most Americans don’t get enough <a href="https://www.mdpi.com/2072-6643/13/7/2154" target="_blank" rel="noreferrer noopener">long-chain omega‑3s</a> from food alone. The average U.S. diet is heavy on <a href="https://www.mayoclinic.org/diseases-conditions/heart-disease/expert-answers/omega-6/faq-20058172" target="_blank" rel="noreferrer noopener">omega‑6 fatty acids</a> - often in a 10:1 ratio to omega‑3 - which may fuel inflammation and irritability.



Experts recommend at least two servings of fatty fish a week, such as salmon or sardines. 



For those who don’t eat seafood, even a basic supplement may close the gap and improve both physical and mental health.



<h2 class="wp-block-heading" id="h-supplements-that-calm-behavior">Supplements that calm behavior</h2>



One six‑month <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC4336833/" target="_blank" rel="noreferrer noopener">trial</a> in 8‑ to 16‑year‑olds reported a 59 percent drop in disruptive conduct that lasted half a year after the study ended. 



Similar shifts have shown up in adult parolees and nursing‑home residents, suggesting age is no barrier.



Public‑school cafeterias could offer <a href="https://www.earth.com/news/fish-like-rainbow-trout-suffer-extreme-pain-when-killed-by-air/">fish</a> twice a week, while correctional facilities might issue capsules at intake. Raine notes that such steps are “low cost, low risk,” especially compared with medications or restraint.



Beyond behavior, omega‑3s continue to earn cardiovascular praise. In the <a href="https://www.nejm.org/doi/full/10.1056/NEJMoa1812792" target="_blank" rel="noreferrer noopener">REDUCE‑IT trial</a>, 4 grams of purified EPA cut fatal heart attacks by 25 percent among statin users. 



A calmer mind and a stronger heart in the same pill has obvious appeal for clinicians.



<h2 class="wp-block-heading" id="h-fewer-risks-broad-access">Fewer risks, broad access</h2>



Compared to prescription medications for <a href="https://www.earth.com/news/dopamines-role-in-male-aggression-fades-with-fighting-experience/">aggression</a>, fish oil has fewer side effects and is easier to access. It doesn’t require a prescription, and many brands are available over the counter at grocery stores or online.



That said, fish oil should not replace professional treatment when serious behavioral issues are involved. It can be a helpful addition, but therapy, structured support, and in some cases medication are still essential tools.



<h2 class="wp-block-heading" id="h-room-to-refine-dosing">Room to refine dosing</h2>



Omega‑3 is “not a magic bullet,” Raine warned, stressing that therapy, education, and social support still matter. Most studies followed volunteers for four months; researchers need longer follow‑ups to see whether tempers stay cool.



Scientists also hope to learn why some volunteers improve more than others. 



<a href="https://www.earth.com/news/genetic-supergenes-power-explosive-evolution-in-some-fish/">Genetics</a> that alter fatty‑acid metabolism, baseline inflammation, and even gut microbiota may shape response. Tailored dosing could push the average benefit beyond today’s modest figures.



For now, experts say parents of an irritable child, or adults who catch themselves snapping, might consider swapping a sugary snack for <a href="https://www.earth.com/news/many-young-salmon-break-the-typical-migration-rules-boosting-survival-chances/">salmon</a>, or adding a budget fish‑oil capsule to breakfast. The risk is tiny, the price is low, and the evidence is getting harder to ignore.



<h2 class="wp-block-heading" id="h-who-needs-fish-oil-most">Who needs fish oil most?</h2>



Not everyone responds the same to omega‑3 fatty acids. Genetic differences, particularly in the <a href="https://www.ncbi.nlm.nih.gov/gene/3992" target="_blank" rel="noreferrer noopener">FADS gene</a>, can affect how well the body makes EPA and DHA from plant-based sources.



People of Amerindian or African ancestry may have variations that change their conversion efficiency. 



For some, this means supplements could be especially important to meet their brain’s needs and reduce inflammation-driven behaviors.



The study is published in <a href="https://pubmed.ncbi.nlm.nih.gov/38911617/" target="_blank" rel="noreferrer noopener">Aggression and Violent Behavior</a>.



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Fish oil supplements shown to control aggression in human studies

Fish oil capsules have long been sold for heart and...

The world’s seas have long acted as a planetary safety net, soaking up excess heat and roughly a quarter of all human-generated carbon dioxide. 



Yet this crucial buffer is anything but uniform. Some waters capture carbon, others release it, and the balance can swing in a matter of days.



Until now, most global maps blurred those variations into month-long snapshots at coarse, 100-kilometer grids. 



A new satellite-driven product called <a href="https://essd.copernicus.org/articles/13/777/2021/">OceanSODA-ETHZ</a> changes that picture, offering eight-day updates at 25-kilometer resolution and revealing the ocean <a href="https://www.earth.com/news/earths-carbon-sinks-are-being-pushed-to-their-limits/">carbon sink</a> in unprecedented detail.



<h2 class="wp-block-heading" id="h-satellites-fill-ocean-carbon-gaps">Satellites fill ocean carbon gaps</h2>



Direct readings of surface-water CO2 come from ships and buoys, leaving vast gaps in space and time.



“Increasing the resolution of these global datasets is challenging because the number of direct measurements of carbon dioxide at the ocean’s surface is rather sparse across all regions and times,” explained project co-leader Nicolas Gruber of ETH Zurich.



To fill those gaps, Gruber’s team paired the in situ data with a suite of Earth-observation satellites that sense <a href="https://www.earth.com/news/humans-are-substantially-changing-the-seasons-of-the-ocean/">sea-surface temperature</a>, color, wind, and more - variables tightly linked to how much CO2 water can hold.



Feeding that information into a cascade of machine-learning algorithms produced a fine-grained, eight-day global mosaic.



“This new version maps the parameters of the ocean carbon system every eight days at a resolution of about 25 by 25 kilometers, more than 30 times finer than previous products,” Gruber said.



“A critical part of the approach is the use of satellite data, which provides detailed information to interpolate the measurements in time and space.”



<h2 class="wp-block-heading" id="h-satellites-track-ocean-carbon-changes">Satellites track ocean carbon changes</h2>



Presented this week at <a href="https://lps25.esa.int/">ESA’s Living Planet Symposium</a>, the dataset already highlights dramatic short-term swings. 



An animation released by the team tracks the 2017 Atlantic <a href="https://www.earth.com/news/how-hurricanes-help-oceans-fight-climate-change/">hurricane</a> season, when storms such as Maria and Irma churned deep, carbon-rich waters to the surface.



<figure class="wp-block-embed 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/cEUvoY8krHM?si=cX1giVtLnycyFKqr
</div><figcaption class="wp-element-caption">Animation generated using the new OceanSODA-ETHZv2 product by Luke Gregor, Jamie Shutler and Nicolas Gruber</figcaption></figure>



In the visualization, red plumes - areas where the sea outgasses CO2 - flare beneath the swirling wind arrows, then fade as cooler, oxygen-laden surface layers return.



Jamie Shutler from the University of Exeter, while not involved in developing the product, is already using it for storm studies.



“Thanks to its fine detail, the dataset can help us separate and understand the influence of events like hurricanes - where deep water, often high in carbon, can be forced to rise to the surface - which can cause sudden spikes or changes in surface ocean carbon dioxide levels,” said Shutler.



<h2 class="wp-block-heading" id="h-a-new-view-of-ocean-acidification">A new view of ocean acidification</h2>



Every molecule of CO2 that the ocean absorbs reacts with seawater, lowering pH and shifting carbonate chemistry in ways that erode coral skeletons, thin oyster shells, and alter plankton communities.



Until now, researchers tracking this “other CO2 problem” relied on sparse records or coarse climatologies. 



OceanSODA-ETHZ delivers near-real-time fields of surface pH and carbonate ions, letting scientists watch <a href="https://www.earth.com/news/ocean-acidification-is-spreading-into-deeper-waters/">acidification</a> pulses unfold as upwelling, rainfall, or melting sea ice change local chemistry.



Because the product also extends back to 1985, analysts can mine four decades of fine-scale variability to see where buffers are weakening and hotspots are emerging. 



Those insights can feed into fisheries management, coastal planning, and global carbon-budget assessments.



<h2 class="wp-block-heading" id="h-esa-powers-new-ocean-maps">ESA powers new ocean maps</h2>



The dataset is the latest deliverable from <a href="https://eo4society.esa.int/">ESA’s FutureEO “Science for Society” program</a>, which funds innovative uses of satellite records.



“The fact that we can use this method to gain new insights into the exchange of carbon dioxide between the ocean and atmosphere - and on the ocean acidification altogether - is a great step forward in ocean science,” said Roberto Sabia, an ocean scientist at <a href="https://www.esa.int/Applications/Observing_the_Earth">ESA Earth-Observation</a>. 



Gruber and colleagues emphasize that OceanSODA-ETHZ is not a static atlas but a living product that can assimilate new ship measurements and leverage upcoming satellite missions.



Higher-resolution sensors such as <a href="https://pace.gsfc.nasa.gov/">NASA’s PACE</a> and <a href="https://www.esa.int/Applications/Observing_the_Earth/Copernicus/Copernicus_Sentinel_Expansion_missions">ESA’s Copernicus Expansion</a> promise even clearer views of <a href="https://www.earth.com/news/plankton-help-predict-ocean-biodiversity-losses/">plankton</a> blooms, sea-surface roughness, and dissolved organic matter - all factors that modulate carbon exchange.



<h2 class="wp-block-heading" id="h-forecasts-of-regional-carbon-uptake">Forecasts of regional carbon uptake</h2>



Ultimately, the goal is to couple these detailed maps with ocean-atmosphere models, yielding short-term forecasts of regional carbon uptake akin to daily weather predictions.



Such tools could alert coastal managers when acidification thresholds are likely to be breached or help negotiators refine national emissions budgets by tracking natural carbon sinks more precisely.



For now, the new product already reshapes our understanding of the ocean’s role in moderating climate. 



Where earlier charts smoothed over crucial dynamics, OceanSODA-ETHZ reveals a living, breathing carbon landscape - one where swirling eddies, roaring storms, and shifting <a href="https://www.earth.com/news/small-ocean-currents-play-a-huge-role-in-earths-climate/">currents</a> all leave their stamp on the planet’s most important carbon reservoir.



Image Credit: ESA



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Satellites reveal how oceans absorb carbon in unprecedented detail

The world’s seas have long acted as a planetary safety...

Fire has licked the planet’s surface for more than 400 million years, scorching forests, clearing grasslands, and lofting smoke into the upper air. Yet pinning down when people stopped fearing flames and started steering them has been surprisingly hard.



A fresh <a href="https://www.pnas.org/doi/10.1073/pnas.2500042122" target="_blank" rel="noreferrer noopener">analysis</a> of a 300,000‑year‑old sediment core pulled from the East China Sea finds a sharp surge in soot about 50,000 years ago, a signal that stands apart from normal climate‑driven wildfire patterns.



The work, led by Dr. Zhao Debo at the <a href="http://english.qdio.cas.cn/" target="_blank" rel="noreferrer noopener">Institute of Oceanology</a>, Chinese Academy of Sciences, together with partners in Germany and France, strings together chemical, archaeological, and climate evidence into one timeline.



“Our findings challenge the widely held belief that humans only began influencing the <a href="https://www.earth.com/news/ideas-traveled-farther-than-people-in-the-early-days-of-farming/">environment</a> with fire in the recent past, during the Holocene,” said Dr. Zhao Debo.



<h2 class="wp-block-heading" id="h-when-humans-began-using-fire">When humans began using fire</h2>



Researchers tracked <a href="https://www.nature.com/articles/s43247-024-01343-5" target="_blank" rel="noreferrer noopener">pyrogenic carbon</a>, the charred plant residue left when biomass burns incompletely, because rivers flush those tiny black flecks into coastal mud where they store a record of past fires.



Between 60,000 and 45,000 years ago that charcoal fraction doubled, then stayed high. The jump broke its long connection to East Asian monsoon strength, showing that weather alone could not explain the flames.



Parallel charcoal peaks in Europe, Southeast Asia, and the Papua New Guinea–Australia corridor line up with the same window, pointing to a continent‑scale shift rather than scattered lightning <a href="https://www.earth.com/news/birth-of-farming-driven-by-humans/">strikes</a>.



<h2 class="wp-block-heading" id="h-fire-use-spreads-across-continents">Fire use spreads across continents</h2>



Archaeological <a href="https://www.science.org/content/article/more-45000-years-ago-modern-humans-ventured-neanderthal-territory-here-s-what-happened" target="_blank" rel="noreferrer noopener">hearths</a> from Bulgaria’s <a href="https://visitbulgaria.com/bacho-kiro-cave/" target="_blank" rel="noreferrer noopener">Bacho Kiro Cave</a> to northern Australia’s <a href="https://www.britannica.com/place/Madjedbebe" target="_blank" rel="noreferrer noopener">Madjebebe</a> site cluster inside the same interval, confirming that <a href="https://www.science.org/content/article/more-45000-years-ago-modern-humans-ventured-neanderthal-territory-here-s-what-happened" target="_blank" rel="noreferrer noopener">campfires</a> had become routine parts of daily life.



Genetic <a href="https://www.nature.com/articles/s41586-025-09154-0" target="_blank" rel="noreferrer noopener">studies</a> trace almost all non‑African ancestry to a single successful wave of Homo sapiens that left Africa about 50,000 years ago, matching the charcoal timeline.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/07/humans_fire_early-homo-sapiens_map-sites_credit-IOCAS_1m.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/07/humans_fire_early-homo-sapiens_map-sites_credit-IOCAS_1s.webp" alt="Fire history of Europe, East Asia, Southeast Asia and Papua New Guinea–Australia and age distribution of archaeological sites since the last 300,000 years. Credit: IOCAS" class="wp-image-1976185"/></a><figcaption class="wp-element-caption">Fire history of Europe, East Asia, Southeast Asia and Papua New Guinea–Australia and age distribution of archaeological sites since the last 300,000 years. Click image to enlarge. Credit: IOCAS</figcaption></figure>



While earlier <a href="https://www.earth.com/news/evidence-of-ancient-plant-farming-found-in-east-africa/">humans</a> played with sparks, evidence for habitual fire stretches back at least 250,000 years in Europe, those earlier experiments were local and intermittent. The new record shows the first moment when fire use scales with population growth.



<h2 class="wp-block-heading" id="h-migration-cold-nights-and-campfires">Migration, cold nights, and campfires</h2>



The out‑of‑Africa travelers trekked into ice‑age Eurasia where nights dipped well below freezing. Fire kept predators away, cooked meat, dried hides, and allowed late‑night tool making.



“Even during the Last Glaciation, the use of fire had probably started to reshape ecosystems and carbon fluxes,” added <a href="http://english.qdio.cas.cn/people/jzg/202208/t20220803_310174.html" target="_blank" rel="noreferrer noopener">Professor Wan Shiming</a>, a co‑author on the study.



Controlled flame also opened new food groups. Roasting tubers breaks down starches, and heated stone cracks to yield sharper blades, advantages that likely boosted survival odds for the migrants.



<h2 class="wp-block-heading" id="h-burning-added-carbon-to-land-and-ocean">Burning added carbon to land and ocean</h2>



Modern wildfires already release between 116 and 385 teragrams of <a href="https://www.nature.com/articles/s41598-017-10455-2" target="_blank" rel="noreferrer noopener">pyrogenic carbon</a> to land and sea each year, a sizable slice of the global carbon ledger. 



When ancient people started burning wood on purpose, they nudged that ledger long before industrial smokestacks appeared.



Charcoal is stable. Some pieces survive for millennia in soils, some drift as <a href="https://www.pnas.org/doi/10.1073/pnas.2305030121" target="_blank" rel="noreferrer noopener">dissolved black carbon</a> into the deep ocean where currents can store it for thousands of years. 



By pushing extra charcoal into these sinks, early fire managers may have offset part of the carbon dioxide they released.



Climate models that begin counting human impacts only with <a href="https://www.earth.com/news/cave-discovery-of-ancient-avocados-could-rescue-a-global-crop/">farming</a> or factories might therefore miss a slow, earlier perturbation that started when nightly campfires became normal.



<h2 class="wp-block-heading" id="h-early-human-fire-use-shaped-climate">Early human fire use shaped climate</h2>



The <a href="https://www.sciencedirect.com/science/article/pii/S2212682112000261" target="_blank" rel="noreferrer noopener">East China Sea</a> record shows that environmental influence is not a recent human monopoly. Small groups with stone tools and wooden spears were already altering regional fire regimes and, in turn, the carbon cycle.



That insight reframes today’s policy debates. If early people changed atmospheric chemistry with nothing but sticks and sparks, eight billion of us wielding fossil fuels carry far more leverage, and responsibility, than any ancestral hunter‑gatherer could imagine.



Fire management still shapes global climate in modern times. Prescribed burns reduce fuel loads but also emit smoke; savanna fires in Africa and Australia pulse <a href="https://www.earth.com/news/worlds-first-greenhouse-gas-detecting-satellite-is-now-in-orbit/">greenhouse gases</a> each dry season; boreal megafires now send record carbon plumes aloft. 



Understanding the deep history of intentional burning helps calibrate those modern choices. Fifty thousand years later we still gather around flames, but the scale has ballooned from glowing embers to global power grids.



The study is published in <a href="https://www.pnas.org/doi/10.1073/pnas.2500042122" target="_blank" rel="noreferrer noopener">Proceedings of the National Academy of Sciences</a>.



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Humans learned to use and control fire much earlier than previously believed

Fire has licked the planet’s surface for more than 400 million...

The James Webb Space Telescope has delivered the clearest, deepest images yet of the Bullet Cluster, unveiling thousands of faint, distant galaxies and offering the most precise map of dark matter in this iconic colliding galaxy cluster.



“With <a href="https://www.earth.com/news/thousands-of-galaxies-revealed-in-a-single-webb-image/">Webb</a>’s observations, we carefully measured the mass of the Bullet Cluster with the largest lensing dataset to date, from the galaxy clusters’ cores all the way out to their outskirts,” said lead author Sangjun Cha, a PhD student at <a href="https://www.yonsei.ac.kr/en_sc/index.do">Yonsei University</a> in Seoul. 



Previous studies relied on less lensing data, leading to less precise estimates of the system’s mass.



“Webb’s images dramatically improve what we can measure in this scene -&nbsp; including pinpointing the position of invisible particles known as dark matter,” said co-author Kyle Finner, an assistant scientist at <a href="https://www.caltech.edu/">Caltech</a>. 



<h2 class="wp-block-heading" id="h-how-light-shows-the-dark">How light shows the dark</h2>



The Bullet Cluster is made of two massive galaxy clusters bound by <a href="https://www.earth.com/news/desi-gravity-study-new-discovery-proves-einstein-right-again/">gravity</a>. It acts as a natural gravitational lens that magnifies background galaxies.



James Jee, a professor at Yonsei University and research associate at UC Davis, is a co-author of the study. “Gravitational lensing allows us to infer the distribution of dark matter,” he said.



To visualize this effect, Jee compares it to ripples on a pond. You can't see the clear water unless there are ripples that distort the shapes of the pebbles below - just as dark matter distorts the light from galaxies behind it.



By measuring thousands of galaxies, the scientists used Webb’s images to weigh visible and invisible mass in the cluster. 



The team also mapped the faint glow of intracluster stars - those not bound to any single galaxy. These drifting stars may closely trace dark matter.



<h2 class="wp-block-heading" id="h-webb-s-dark-matter-reveal">Webb’s dark matter reveal</h2>



Webb’s observations produced a layered view, combining near-infrared data with X-ray imagery from <a href="https://www.nasa.gov/mission/chandra-x-ray-observatory/">NASA’s Chandra X-ray Observatory</a>, revealing hot gas in pink, the bullet shape in the cluster, and the newly refined dark matter distribution in blue.



“We confirmed the intracluster light can be a reliable tracer of dark matter, even in a highly dynamic environment like the Bullet Cluster,” Cha said. 



This strengthens the case that these unbound stars closely trace dark matter’s invisible scaffolding.



The new map reveals detailed structure, including an asymmetric mass region on the left side of the larger cluster. This feature indicates prior collisions that have left behind signatures in the distribution of matter.



<h2 class="wp-block-heading" id="h-mysterious-nature-of-dark-matter">Mysterious nature of dark matter </h2>



Dark matter does not emit, reflect, or absorb light, making it notoriously difficult to study. Yet the Bullet Cluster offers a rare laboratory, showing dark matter separated from hot gas during a cosmic collision while still aligning with the galaxies.



“As the <a href="https://www.earth.com/news/titanic-galaxy-cluster-collision-defies-all-current-understanding-of-the-universe/">galaxy clusters</a> collided, their gas was dragged out and left behind, which the X-rays confirm,” Finner explained. “Webb’s observations show that dark matter still lines up with the galaxies - and was not dragged away.”



The results set tighter constraints on the possibility of dark matter particles interacting with each other. They support theories that dark matter passes through itself without friction, consistent with its mysterious and ghostly nature.



<h2 class="wp-block-heading" id="h-clues-to-a-chaotic-past"><a></a>Clues to a chaotic past</h2>



The elongated mass and clumps in the new map hint at a more complex history for the Bullet Cluster, suggesting multiple collisions over billions of years.



“A more complicated scenario would lead to a huge asymmetric elongation like we see on the left,” Jee said.



The Bullet Cluster, located in the Carina <a href="https://www.earth.com/news/super-jupiter-discovered-in-the-great-bear-constellation/">constellation</a> 3.8 billion light-years from Earth, is so massive that even Webb’s powerful NIRCam could only capture part of it.



“It’s like looking at the head of a giant,” Jee explained. “Webb’s initial images allow us to extrapolate how heavy the whole 'giant' is, but we’ll need future observations of the giant’s whole 'body' for precise measurements.”



<h2 class="wp-block-heading" id="h-future-missions-deeper-maps">Future missions, deeper maps</h2>



NASA’s upcoming <a href="https://www.earth.com/news/nasas-roman-space-telescope-hopes-to-solve-the-dark-matter-mystery/">Nancy Grace Roman Space Telescope</a>, launching by May 2027, will complement Webb’s discoveries with wide-field near-infrared imaging. 



The Roman telescope will enable complete mass estimates of the Bullet Cluster and allow scientists to simulate its ancient collision in detail.



“With Roman, we will have complete mass estimates of the entire Bullet Cluster, which would allow us to recreate the actual collision on computers,” Finner said.



Through these detailed observations, Webb is enriching our understanding of dark matter. It’s also advancing knowledge of how massive structures form and evolve, offering a clearer view of the hidden forces shaping the cosmos.



The study is published in the <a href="https://iopscience.iop.org/article/10.3847/2041-8213/add2f0">Astrophysical Journal Letters</a>.



Image Credit: NASA, ESA, CSA, STScI, CXC



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Webb telescope uncovers secrets of dark matter in cosmic collision zone

The James Webb Space Telescope has delivered the clearest, deepest...

Coffee is prized for its taste and mental boost. A new study shows that caffeine may also fine‑tune the internal clock that makes cells grow old.



Researchers observed that yeast aged more slowly when caffeine altered the same energy pathways that help human cells <a href="https://www.earth.com/news/organ-aging-can-predict-diseases-decades-in-advance/">survive</a> under stress.



<h2 class="wp-block-heading" id="h-caffeine-slows-aging-in-yeast-cells">Caffeine slows aging in yeast cells</h2>



Dr. Charalampos (Babis) Rallis of <a href="https://www.qmul.ac.uk/">Queen Mary University of London</a> focused on the yeast species Schizosaccharomyces pombe because its DNA repair and growth controls echo our own. 



The team logged changes in <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC9139625/" target="_blank" rel="noreferrer noopener">chronological lifespan</a>, the length of time that non‑dividing cells stay viable, then mapped the molecular traffic that caffeine set in motion.



“This is our most exciting find to date,” said Dr. Rallis. The results point to a fuel‑sensing <a href="https://www.earth.com/news/healthy-aging-how-some-people-live-past-100-years/">pathway</a> that kicks in when nutrients dip, mirroring how people burn stored energy between meals.&nbsp;



<h2 class="wp-block-heading" id="h-yeast-helps-us-understand-aging">Yeast helps us understand aging</h2>



Fission yeast may seem worlds apart from humans, but it shares many core <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC4772020/" target="_blank" rel="noreferrer noopener">regulatory pathways</a> found in our cells. Systems like <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC2779044/" target="_blank" rel="noreferrer noopener">AMPK</a> and <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC3241408/" target="_blank" rel="noreferrer noopener">TOR</a> have been conserved over hundreds of millions of years because they work so well.



This makes yeast an ideal testing ground for decoding how compounds like caffeine affect <a href="https://www.earth.com/news/scientists-are-experimenting-with-new-approach-to-fight-and-stop-human-aging-necrosis/">lifespan</a> and stress response. What happens in a petri dish often sparks questions that ripple out to animal models and eventually to people.



<h2 class="wp-block-heading" id="h-how-caffeine-may-slow-aging">How caffeine may slow aging</h2>



The key player is AMPK, an enzyme that "notices" when the cell’s ATP (energy) balance tilts toward empty and then shifts metabolism to survival mode. 



“Caffeine helps flip that switch,” said <a href="https://scholar.google.com/citations?user=913OCBIAAAAJ&amp;hl=en" target="_blank" rel="noreferrer noopener">Dr. John‑Patrick Alao</a>, the postdoctoral scientist who ran the experiments.



Earlier <a href="https://pubmed.ncbi.nlm.nih.gov/23551936/" target="_blank" rel="noreferrer noopener">work</a> suggested caffeine blocked <a href="https://pubmed.ncbi.nlm.nih.gov/23551936/" target="_blank" rel="noreferrer noopener">TOR</a>, a growth promoter, but new data reveal the compound reaches TOR indirectly by first waking up AMPK. 



Cells then slow growth, patch damaged DNA, and boost antioxidant defenses, the very responses that lengthen life in many lab organisms.



<h2 class="wp-block-heading" id="h-caffeine-and-metformin-use-same-pathway">Caffeine and metformin use same pathway</h2>



<a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC6779524/" target="_blank" rel="noreferrer noopener">Metformin</a>, the common diabetes drug, also charges AMPK and is being tested as a geroprotector in humans. The overlap hints that coffee’s benefits may parallel those seen in metformin cohorts, though dosage and metabolism differ widely.



Both agents dial back inflammation, clear out faulty proteins through autophagy, and keep insulin signaling from running too hot. 



If future trials confirm safety, researchers may combine low‑dose caffeine with metformin analogs to see whether their effects stack without side effects.



<h2 class="wp-block-heading" id="h-caffeine-helps-manage-cell-stress">Caffeine helps manage cell stress</h2>



The AMPK pathway doesn’t just manage fuel, it also guides how cells respond to <a href="https://www.ncbi.nlm.nih.gov/medgen/222489" target="_blank" rel="noreferrer noopener">genotoxic stress</a>, such as radiation or chemicals that harm DNA. 



The yeast data showed caffeine increased sensitivity to DNA damage in some mutants, revealing AMPK's role in damage response.



This dual role, energy control and DNA repair, suggests that caffeine tunes both survival and quality control systems. 



It’s part of a wider stress adaptation strategy that has been conserved across <a href="https://www.earth.com/news/scientists-discover-a-protein-that-reverses-cellular-aging/">evolution</a>, and is now offering new angles for anti-aging research.



<h2 class="wp-block-heading" id="h-people-who-drink-coffee-may-live-longer">People who drink coffee may live longer</h2>



Observational work involving hundreds of thousands of adults links two to four cups of coffee daily with <a href="https://pubmed.ncbi.nlm.nih.gov/31055709/" target="_blank" rel="noreferrer noopener">lower all‑cause mortality</a>. 



Separate <a href="https://pubmed.ncbi.nlm.nih.gov/34468722/" target="_blank" rel="noreferrer noopener">analyses</a> in Asian populations find similar protection against heart disease and several cancers.



Because these studies track behavior, not biology, confounding factors like diet, exercise, and income can cloud cause and effect. 



The yeast data now give those population numbers a plausible mechanism anchored in cell chemistry, without the noise of other factors.



<h2 class="wp-block-heading" id="h-future-research-on-caffeine-and-aging">Future research on caffeine and aging</h2>



Yeast tolerate caffeine levels far above a latte, so dose matters when translating findings to people. 



Human AMPK is embedded in tissues that react differently, so benefits in muscle may come at a cost elsewhere if DNA repair stalls during caffeine peaks.



High caffeine can raise blood pressure, trigger anxiety, and interfere with sleep - processes that can speed cell aging if left unchecked. 



Clinical trials that track AMPK activation, cardiovascular markers, and cognitive scores together will be needed before doctors advise specific amounts.



<h2 class="wp-block-heading" id="h-the-role-of-diet-and-exercise">The role of diet and exercise </h2>



Exercise is one of the most well-known ways to activate AMPK in humans. When muscles burn through energy during physical activity, this pathway turns on to help cells adapt and recover.



Certain foods, including those high in polyphenols like berries and green tea, may also give AMPK a nudge. 



Understanding how diet and lifestyle naturally influence this system could lead to everyday habits that support healthy aging.



<h2 class="wp-block-heading" id="h-a-healthy-lifestyle-matters">A healthy lifestyle matters</h2>



For now, moderate coffee remains a safe pleasure that lines up with epidemiology and basic science. Sleepless nights and energy drinks loaded with sugar still pose risks that no enzyme tweak can erase.



Nutrient‑sensing pathways such as AMPK give researchers a roadmap for therapies, yet lifestyle, steady sleep, balanced diet, and movement, keep the road free of potholes. 



The next wave of studies may explore caffeine analogs that lock onto AMPK with precision, separating the perks from the jitters.



The study is published in <a href="https://microbialcell.com/researcharticles/2025a-alao-microbial-cell/" target="_blank" rel="noreferrer noopener">Microbial Cell</a>.



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Scientists learn that caffeine could slow cellular aging under the right conditions

Coffee is prized for its taste and mental boost. 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.



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



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



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



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



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



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



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



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

Is chocolate the next nutritional powerhouse?

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

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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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

Flu viruses are more flexible than expected

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



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



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



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



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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

Detecting mercury contamination with the tap of a finger

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



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



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



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



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



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



Video/ Image Credit: European Space Agency&nbsp;



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



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

Kainji Lake in north central Nigeria

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Bee Hummingbirds, native to Cuba, are known by the scientific name <a href="https://en.wikipedia.org/wiki/Bee_hummingbird">Mellisuga Helenae</a>. At 5.7 centimeters (2.24 inches) in length and 1.7 grams (0.06 ounces), the world’s smallest bird is hardly larger than a bee. While the Bee hummingbird flies from flower to flower, it transfers pollen, it feeds primarily on <a href="https://www.earth.com/news/bees-high-nectar-special-neurons/">nectar</a> and the the occasional spider or insect.

Bee Hummingbirds

The Etruscan Pygmy Shrew, or white-toothed pygmy shrew (<a href="https://en.wikipedia.org/wiki/Etruscan_shrew">Suncus etruscus</a>), weighs in at about 1.8 grams (0.063 ounces) and averages 4 centimeters (1.6 inches) in length excluding the tail. Known as the smallest mammal by mass, the pygmy shrew has an incredibly fast <a href="https://www.earth.com/news/age-related-changes-in-metabolism-dont-match-our-expectations/">metabolism</a> and eats 1.5 to 2 times its body weight each day.

Bee Hummingbirds

News coming your way