Greenhouses in the Cayambe Valley of Ecuador are seen here in today’s Image of the Day from the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> . This area has one of the highest densities of greenhouses for <a href="https://www.earth.com/news/roses-red-violets-blue/">rose</a> production in the world, according to Gregory Knapp, geographer from the <a href="https://www.utexas.edu/">University of Texas at Austin</a>.

Greenhouses in the Cayambe Valley of Ecuador

Today's Image of the Day from the European Space Agency features the barred spiral galaxy NGC 3783, which is located about 130 million light-years away in the constellation Centaurus. 



NGC 3783 is also the most prominent of a galaxy group (by the same name) that contains 47 galaxies.&nbsp;



<h2 class="wp-block-heading" id="h-what-are-galaxy-groups">What are galaxy groups?</h2>



“Like galaxy clusters, galaxy groups are aggregates of gravitationally bound galaxies. Galaxy groups, however, are less massive and contain fewer members than <a href="https://www.earth.com/news/titanic-galaxy-cluster-collision-defies-all-current-understanding-of-the-universe/" target="_blank" rel="noreferrer noopener">galaxy clusters</a> do: where galaxy clusters can contain hundreds or even thousands of constituent galaxies, galaxy groups do not typically include more than 50,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



“The Milky Way is actually part of a galaxy group, known as the Local Group, which contains two other large galaxies (Andromeda and the Triangulum galaxy), as well as several dozen satellite and dwarf galaxies.”



<h2 class="wp-block-heading" id="h-a-blue-giant-star">A blue giant star</h2>



The bright object that appears to the right of the galaxy is the star HD 101274. “The perspective in this image makes the star and the galaxy look like close companions, but this is an illusion. HD 101274 lies only about 1,530 light-years from Earth, meaning it is about 85 thousand times closer than NGC 3783,” explained ESA.&nbsp;



The star is part of the NGC 3766 cluster, sometimes referred to as the Pearl Cluster, which is known for its richness in bright stars and its relatively young age.



Characterized by its high temperature and luminosity, HD 101274 is categorized as a blue giant star.



<h2 class="wp-block-heading" id="h-significance-of-blue-giants">Significance of blue giants</h2>



Blue giants are massive stars that have left the main sequence phase of stellar evolution and are burning helium or heavier elements in their cores. These stars are known for their short lifespans relative to smaller stars due to their rapid consumption of nuclear fuel.



<a href="https://www.earth.com/news/dark-stars-scientists-discover-a-new-type-of-star-powered-by-dark-matter/" target="_blank" rel="noreferrer noopener">Stars</a> like HD 101274 are important for astronomers because they help in studying the properties of stellar populations in clusters and the dynamics of stellar evolution in different environments. 



Observations of blue giant stars can provide valuable insights into the characteristics of their atmospheres, internal structures, and the processes occurring within and around them.



<h2 class="wp-block-heading" id="h-active-galactic-nucleus-of-ngc-3783">Active galactic nucleus of NGC 3783</h2>



One of the most interesting aspects of NGC 3783 is that it harbors an active galactic nucleus. This means that its central region is exceptionally luminous, likely due to the presence of a supermassive black hole. 



The black hole is actively accreting material, which emits a substantial amount of radiation as it spirals inward and heats up.



The galaxy has been studied extensively in the ultraviolet and X-ray light spectra to understand better the properties of the accretion disk around the black hole and the complex dynamics of the material surrounding it. 



These studies are crucial for understanding the physics of active galactic nuclei and the role they play in <a href="https://www.earth.com/news/galaxies-like-our-own-milky-way-are-not-unique/" target="_blank" rel="noreferrer noopener">galaxy evolution</a>.



According to ESA, NGC 3783 is a&nbsp;Type I Seyfert galaxy. “In this image it is recorded by Hubble in incredible detail, from its glowing central bar to its narrow, winding arms and the dust threaded through them, thanks to five separate images taken in different wavelengths of light," noted ESA.



“In fact, the galactic center is bright enough to Hubble that it exhibits diffraction spikes, normally only seen on stars such as HD 101274.”



<h2 class="wp-block-heading" id="h-massive-collection-of-galaxy-clusters">Massive collection of galaxy clusters</h2>



The NGC 3783 group is part of the larger Hydra-Centaurus Supercluster, which itself is a massive collection of <a href="https://www.earth.com/news/shapes-of-one-million-galaxies-hint-at-the-universes-origins/" target="_blank" rel="noreferrer noopener">galaxies</a> and galaxy clusters located primarily in the constellations of Hydra and Centaurus.



The NGC 3783 group consists of several galaxies that are gravitationally bound and interact with each other. These interactions can influence the galaxies' evolution through mechanisms like tidal forces and merger events, which can trigger star formation, fuel central black holes, and reshape the galaxies' structures.



Studying the NGC 3783 group helps astronomers understand how <a href="https://www.earth.com/news/ceers-2112-ancient-galaxy-looks-strikingly-similar-to-ours/" target="_blank" rel="noreferrer noopener">galaxies</a> evolve together in a common gravitational environment, offering insights into the dynamics and evolution of structures on cosmic scales.



Image Credit: ESA/Hubble &amp; NASA



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Luminous spiral galaxy and a blue giant star

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

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



By studying regions like NGC 604, astronomers can gain insights into the complex interactions between stars and the interstellar medium, as well as the conditions that lead to the birth of stars. 



This, in turn, helps us understand the evolution of <a href="https://www.earth.com/news/galaxies-like-our-own-milky-way-are-not-unique/" target="_blank" rel="noreferrer noopener">galaxies</a> and the universe as a whole.



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



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



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



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



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



NGC 604 is one of the largest known regions of ionized hydrogen, also known as an H II region. This nebula is significantly larger than the Orion Nebula, which is one of the most well-known H II regions in our own <a href="https://www.earth.com/news/large-amount-of-dark-matter-may-be-missing-from-the-milky-way/" target="_blank" rel="noreferrer noopener">Milky Way galaxy</a>.&nbsp;



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



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



Within NGC 604, there are hundreds of young, hot, massive <a href="https://www.earth.com/news/stars-at-the-edge-of-our-milky-way-galaxy-travel-more-slowly/" target="_blank" rel="noreferrer noopener">stars</a>. These stars have ionized the surrounding gas, causing it to glow and creating the nebula. 



The region is a prime example of a starburst phenomenon, where stars form at a much higher rate than in typical galactic conditions.



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Young, massive stars in the Triangulum Galaxy

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Hundreds of galaxies illuminate the early universe 

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 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...

The MODIS instrument, short for Moderate Resolution Imaging Spectroradiometer, is a key instrument aboard the Terra and Aqua satellites. MODIS is playing a vital role in the development of Earth ecosystem models, able to predict global changes, which then assist policy makers in making informed decisions about the protection of the global environment.

Heavy snow and cloud cover in the Alps are seen in this Image of the day&nbsp;from the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look at heavy snow and low clouds in the Alps. Wildlife such as ibex live in the higher peaks to elevations of 3,400 m (11,155 ft), and plants such as Edelweiss grow in rocky areas in lower elevations as well as in higher elevations.

Heavy snow and cloud cover in the Alps

Monitoring Earth Changes with MODIS

Aqua is a NASA scientific research satellite that studies precipitation, evaporation, and water cycles. Terra and Aura make up the Earth Observing System. It's the second component of the system.

A frozen Lake Erie in February Today’s Image of the Day comes from the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look at a frozen <a href="https://www.earth.com/image/icy-lake-erie/">Lake Erie</a>, which is currently 93.3 percent iced over. A frozen Lake Erie in February
This false-color image was created using data from the Moderate Resolution Imaging Spectroradiometer (MODIS) on board the Aqua satellite to differentiate between snow, ice, and clouds.
Lake Erie /ˈɪəri/ (French: Lac Érié) is the fourth-largest lake (by surface area) of the five Great Lakes in North America, and the eleventh-largest globally if measured in terms of surface area.It is the southernmost, shallowest, and smallest by volume of the Great Lakes and therefore also has the shortest average water residence time. At its deepest point Lake Erie is 210 feet (64 metres) deep. 
Situated on the International Boundary between Canada and the United States, Lake Erie&#8217;s northern shore is the Canadian province of Ontario, specifically the Ontario Peninsula, with the U.S. states of Michigan, Ohio, Pennsylvania, and New York on its western, southern, and eastern shores. These jurisdictions divide the surface area of the lake with water boundaries. 
The lake was named by the Erie people, a Native American people who lived along its southern shore. The tribal name &#8220;erie&#8221; is a shortened form of the Iroquoian word erielhonan, meaning long tail
&#8212;
By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="https://www.earth.com/staff">Earth.com</a> Staff Writer
Image Credit: <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a>

A frozen Lake Erie in February

Aqua Earth Observing Satellite

This beautiful photo gallery contains 50 incredible images of Earth from Space. These images were taken by astronauts onboard the International Space Station, as well as by a multitude of NASA satellites orbiting the earth.

Today’s Image of the Day comes thanks to the <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=90654&amp;eocn=home&amp;eoci=iotd_readmore">NASA Earth Observatory</a> and features a look at Super Typhoon Noru in the Pacific Ocean just south of <a href="https://www.earth.com/news/first-blue-chrysanthemums-created/">Japan</a>.
This image was captured by the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua satellite on July 31, 2017. 
At the time the photo was taken, Typhoon Noru was located just 250 kilometers south of Iwo Jima. Maximum sustained winds hit 150 miles per hour.
The storm briefly became a category 5 on July 30, before being downgraded to a category 4 one day later.
&#8211;
By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="https://www.earth.com/staff">Earth.com</a> Staff Writer
Source: <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=90654&amp;eocn=home&amp;eoci=iotd_readmore">NASA Earth Observatory</a>

Super Typhoon Noru in the Pacific Ocean

Incredible Images of Earth from Space

Photos from the International Space Station are found in this awesome Earth.com image gallery. Flat-earthers won't agree, but these incredible photos of the Earth were taken by astronauts onboard the International Space Station. The International Space Station is a modular space station in low Earth orbit.

Northern Italy from the space station is seen here in this Image of the Day from the <a href="http://www.esa.int/">European Space Agency</a> (ESA). The view includes the top half of the Italian Peninsula, along with <a href="https://www.earth.com/image/wildfires-burn-northern-corsica/">Corsica</a> and Sardinia off the coast. This image was captured by ESA astronaut Paolo Nespoli on his third and final mission to the Space Station.

Northern Italy from the Space Station

Photos from the International Space Station

The Mediterranean has long been a crossroads of trade and tourism, yet its deepest pocket, the Calypso Deep, seemed beyond the reach of day-to-day pollution. 



That hope ended earlier this year when researchers reported plastic bags, glass shards, and crumpled cans resting 16,770 feet beneath the waves in the <a href="https://en.wikipedia.org/wiki/Ionian_Sea" target="_blank" rel="noreferrer noopener">Ionian Sea</a>.



Their survey logged 167 items on the trench floor - 148 confirmed pieces of marine litter and 19 more that almost certainly came from people. 



By any measure, it is one of the densest concentrations of trash ever recorded in the <a href="https://www.earth.com/news/deep-ocean-buffet-big-fish-are-surprisingly-reliant-on-the-twilight-zone/">dark zone</a> of the ocean.



The discovery arrives as global attention continues to focus on <a href="https://www.earth.com/news/surprise-study-some-scientists-call-for-halting-ocean-plastic-cleanup-efforts/">plastic waste</a>. 



Videos of snagged sea turtles and bottle-strewn beaches have already ignited public concern, but those images barely hint at what sinks far below the reach of sunlight.



Now evidence from Calypso Deep shows that even the <a href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/calypso" target="_blank" rel="noreferrer noopener">Mediterranean’s farthest recesses</a> are filling up.



<h2 class="wp-block-heading" id="h-calypso-deep-is-full-of-plastic-waste">Calypso Deep is full of plastic waste</h2>



The team used the submersible <a href="https://en.wikipedia.org/wiki/DSV_Limiting_Factor" target="_blank" rel="noreferrer noopener">Limiting Factor</a> to reach the bottom of a kidney-shaped trench roughly 12.4 miles long and 3.1 miles across. 



During a 43-minute trek near the seafloor of the Calypso Deep, cameras captured thousands of objects per square mile, mostly plastic waste discarded by humans.



A single straight-line pass of 2,130 feet was enough to confirm that human trash blankets large stretches of the basin. Most pieces were flexible plastics; glass, metal, and paper rounded out the list. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/marine-trash_Calypso-Deep-region_Mediterranean_study-map_UBarcelona_1m.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/03/marine-trash_Calypso-Deep-region_Mediterranean_study-map_UBarcelona_1s.webp" alt="(A) General location of the Calypso Deep (box) in the Ionian Sea. PP: Peloponnese Peninsula. (B) Close up and general bathymetry of Calypso Deep (box) and surrounding area. For depth ranges, see color scale. (C) Detailed bathymetry of Calypso Deep with depth contours in meters. The position of the deepest point is indicated by the white dot, while the dive area is indicated by the red dot. Credit: University of Barcelona" class="wp-image-1976573"/></a><figcaption class="wp-element-caption">(A) General location of the Calypso Deep (box) in the Ionian Sea. PP: Peloponnese Peninsula. (B) Close up and general bathymetry of Calypso Deep (box) and surrounding area. For depth ranges, see color scale. (C) Detailed bathymetry of Calypso Deep with depth contours in meters. The position of the deepest point is indicated by the white dot, while the dive area is indicated by the red dot. Click image to enlarge. Credit: University of Barcelona</figcaption></figure>



Even without animals caught on camera, the piles raise alarms because deep-sea communities recover slowly from disturbance.



Calypso Deep lies about 37 miles west of the Peloponnese coast inside the Hellenic Trench, a zone of steep, stepped walls prone to earthquakes. 



<h2 class="wp-block-heading" id="h-plastic-waste-rides-currents">Plastic waste rides currents</h2>



Weak currents, usually under 0.8 inches per second and rarely reaching 7 inches per second, let debris settle instead of sweeping it away.



“It comes from various sources, both terrestrial and marine. It could have arrived by various routes, including long-distance transport by ocean currents or direct dumping,” explains <a href="https://web.ub.edu/en/web/directori/?accio=SEL&amp;id=v759w8s35bo5v72r&amp;lang=ca" target="_blank" rel="noreferrer noopener">Miquel Canals</a>, professor at the Department of Earth and Ocean Dynamics at the University of Barcelona.



“Some light waste, such as plastics, comes from the coast and escapes to Calypso Deep, just about 37 miles away. Certain plastics, <a href="https://www.earth.com/news/plastic-bag-bans-have-drastically-reduced-ocean-pollution/">like bags</a>, drift just above the seabed until they are partially or completely buried or break down into smaller fragments," Canals continued.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/marine-trash_Calypso-Deep-region_Mediterranean_litter-photos_UBarcelona_1m.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/03/marine-trash_Calypso-Deep-region_Mediterranean_litter-photos_UBarcelona_1s.webp" alt="Examples of identified litter items with category attribution per material type (cf. Table 2). (A) Plastic bag, J3. (B) Plastic heavy-duty sack, J36. (C) Plastic sheet, J67. (D) Plastic food container made of hard plastic, J225. (E) Plastic heavy-duty sack, J36. (F) Plastic bag, J3 (G) Cups and lids of hard plastic, J227. (H) Plastic rope &gt; 1 cm in diameter, J49. (I) Paper cartons/Tetrapak (non-milk), J151. (J) Metal drink can, J175. (K) Glass bottle. Note sediment shadow with side scouring downwards of the bottle J200. (L) Plastic drink bottle. Credit: University of Barcelona" class="wp-image-1976569"/></a><figcaption class="wp-element-caption">Examples of identified litter items with category attribution per material type. (A) Plastic bag, J3. (B) Plastic heavy-duty sack, J36. (C) Plastic sheet, J67. (D) Plastic food container made of hard plastic, J225. (E) Plastic heavy-duty sack, J36. (F) Plastic bag, J3 (G) Cups and lids of hard plastic, J227. (H) Plastic rope > 1 cm in diameter, J49. (I) Paper cartons/Tetrapak (non-milk), J151. (J) Metal drink can, J175. (K) Glass bottle. Note sediment shadow with side scouring downwards of the bottle J200. (L) Plastic drink bottle. Click image to enlarge. Credit: University of Barcelona</figcaption></figure>



Rivers, wind, and ship traffic all feed the stream of refuse heading offshore. As algae and other organisms cling to floating polymers, the added weight turns buoyant scraps into sinking hazards. The trench’s closed shape then locks the pieces in place.



<h2 class="wp-block-heading" id="h-calypso-deep-as-a-plastic-graveyard">Calypso Deep as a plastic graveyard</h2>



Surface eddies often corral floating trash into the trench. When these eddies form over the Calypso Trench, some debris slowly falls to the bottom, aided by degradation and ballasting processes that increase its density. 



Surface currents can also carry debris northward from the Adriatic Sea through the Strait of Otranto and from waters off northwestern Greece. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/marine-trash_Calypso-Deep-region_Mediterranean_3D-model_UBarcelona_1m.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/03/marine-trash_Calypso-Deep-region_Mediterranean_3D-model_UBarcelona_1s.webp" alt="(A) 3D model generated from a subset of video frames by reference to a litter item of known size shown in B. The white dashed line in A represents the camera frames along the Deep Submergence Vehicle (DSV) Limiting Factor moving path, whereas the red dashed line represents the frames counted between two items identified on the seabed. (B) Accumulation of litter items in the inner Calypso Deep with a litter item of known size (12 cm) used as a reference for 3D model generation. Credit: University of Barcelona" class="wp-image-1976567"/></a><figcaption class="wp-element-caption">(A) 3D model generated from a subset of video frames by reference to a litter item of known size shown in B. The white dashed line in A represents the camera frames along the Deep Submergence Vehicle (DSV) Limiting Factor moving path, whereas the red dashed line represents the frames counted between two items identified on the seabed. (B) Accumulation of litter items in the inner Calypso Deep with a litter item of known size (12 cm) used as a reference for 3D model generation. Click image to enlarge. Credit: University of Barcelona</figcaption></figure>



The same circular flows that drive marine life cycles are now channeling waste into permanent graveyards at the very bottom of Earth's deepest bodies of water.



<a href="https://web.ub.edu/ca/web/actualitat/w/a-sea-of-rubbish-ocean-floor-landfills-?" target="_blank" rel="noreferrer noopener">Earlier work in 2021</a> showed the Strait of Messina carrying the world’s heaviest load of undersea garbage, confirming that the Mediterranean is especially at risk.



“We have also found evidence of boats dumping bags of rubbish, indicated by piles of assorted waste followed by an almost straight furrow," said Canals, expressing his frustration.



That is why the bottom of the Calypso Deep is littered with humans' plastic waste, and also why the problem will do nothing but continue to worsen.



"Unfortunately, when it comes to the Mediterranean, it is fair to say that ‘not a single inch of it is clean.’”



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



Unlike beaches and coastlines, the <a href="https://www.earth.com/news/99-percent-of-the-deep-ocean-floor-has-still-never-been-seen-by-humans/">ocean floor</a> remains largely out of sight, making it difficult to build social and political momentum for its conservation. 



Yet what settles at the bottom can influence marine life, food webs, fisheries, climate feedback loops, and even geological stability.



<a href="https://www.earth.com/news/the-mediterranean-nearly-lost-all-of-its-water-6-million-years-ago/">The Mediterranean</a> is an enclosed sea, surrounded by humanity, with intense maritime traffic and widespread fishing activity.



“Scientists, communicators, journalists, influencers - everyone with a platform - must work together. The problem is vast, even if it is not directly visible, and we cannot ignore it," Canals implored.



The trail of refuse from shorelines to Calypso Deep underlines a plain truth: plastics and other debris do not vanish once tossed aside. They ride currents, sink in stages, and ultimately collect in the planet’s most secluded hollows. 



The evidence provided by this research should galvanize global efforts - especially in the Mediterranean - to curb dumping, particularly of plastics, in line with the pending <a href="https://www.globalplasticlaws.org/un-global-plastics-treaty" target="_blank" rel="noreferrer noopener">UN Global Plastics Treaty</a>.



From the North Atlantic’s first recorded litter in 1975 to the record densities documented across the Mediterranean today, the pattern remains the same - human waste reaches everywhere water flows.



We must do more, we must do better, and we must do it now.



-----



Thanks to the leaders of this research team - Miquel Canals of the <a href="https://web.ub.edu/en/" target="_blank" rel="noreferrer noopener">University of Barcelona</a>, Georg Hanke of the European Commission’s <a href="https://commission.europa.eu/about/departments-and-executive-agencies/joint-research-centre_en" target="_blank" rel="noreferrer noopener">Joint Research Centre</a>, François Galgani of <a href="https://www.ifremer.fr/en" target="_blank" rel="noreferrer noopener">IFREMER</a>, and Victor Vescovo of <a href="https://caladanoceanic.com/" target="_blank" rel="noreferrer noopener">Caladan Oceanic</a>



The full study was published in the journal <a href="https://www.sciencedirect.com/science/article/pii/S0025326X25000852">Marine Pollution Bulletin</a>.



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Scientists make disturbing discovery on the deepest parts of the seafloor: 'Not a single inch of it is clean'

The Mediterranean has long been a crossroads of trade and...

For years, bacteria dominated gut health research. Now, the gut virome is gaining attention as a major player in health and disease. Bacteriophages, which are viruses that infect <a href="https://www.earth.com/news/scientists-think-they-found-two-key-bacteria-that-cause-multiple-sclerosis/">bacteria</a>, make up around 90% of the gut virome.



Though small in biomass, they outnumber bacteria by up to tenfold. These tiny viruses shape microbial communities, influence immunity, and affect gut health.



A landmark review published recently in Precision Clinical Medicine reveals how the gut virome links to diseases like inflammatory bowel disease (<a href="https://www.cdc.gov/inflammatory-bowel-disease/about/index.html" target="_blank" rel="noreferrer noopener">IBD</a>), <a href="https://www.earth.com/news/colonoscopy-vs-stool-tests-doctors-found-out-which-is-better-at-detecting-cancer/">colorectal cancer</a>, and Clostridium difficile infection (<a href="https://my.clevelandclinic.org/health/diseases/15548-c-diff-infection" target="_blank" rel="noreferrer noopener">CDI</a>).



<h2 class="wp-block-heading" id="h-gut-s-virome-changes-across-life-stages">Gut's virome changes across life stages</h2>



The gut virome changes constantly throughout life. Infants show high <a href="https://www.earth.com/news/bacteria-that-eat-forever-chemicals-discovered-in-contaminated-soil/">diversity</a> in gut bacteriophages (also called phages), which is shaped by birth method, diet, and antibiotic exposure.



As individuals grow, diet and hormones refine the virome. In adults, phages and bacteria form a stable, <a href="https://www.nature.com/articles/s41579-021-00536-5" target="_blank" rel="noreferrer noopener">balanced community</a>.



However, aging shifts this balance. Older adults show more lysogenic phages, which integrate into bacterial genomes and potentially alter metabolism and immune interactions.



<h2 class="wp-block-heading" id="h-diet-and-environment-shape-the-virome">Diet and environment shape the virome</h2>



Diet greatly <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC9455721/" target="_blank" rel="noreferrer noopener">influences</a> the virome. High-fiber diets support beneficial phages by encouraging helpful bacteria. Western diets, rich in fat and sugar, promote harmful <a href="https://www.earth.com/news/some-bacteria-breathe-by-creating-electricity/">phages</a>.



Urbanization reduces exposure to natural viruses. Studies show that rural diets which are rich in fiber boost gut virome diversity.



Host genetics and immunity also play roles. Genetic variants can affect viral detection and clearance. Immune defenses, like <a href="https://my.clevelandclinic.org/health/treatments/interferons" target="_blank" rel="noreferrer noopener">interferons</a> and <a href="https://www.immunology.org/public-information/bitesized-immunology/receptors-molecules/immunoglobulin-iga" target="_blank" rel="noreferrer noopener">IgA</a>, keep the virome balanced.



However, immune dysfunction can trigger viral imbalances, worsening conditions like HIV and gut inflammation.



<h2 class="wp-block-heading" id="h-viruses-and-bacteria-interacting">Viruses and bacteria interacting</h2>



Viruses, including phages, along with bacteria and fungi form a complex and dynamic ecosystem in the gut. The components interact in positive and negative ways, thus affecting host metabolism, immune regulation and resistance to disease. 



The gut virome plays a crucial regulatory role in these intricate interactions. Phages interact with bacteria through lytic, lysogenic, and budding cycles, which regulate bacterial populations and gene flow. 



In a form of microbial arms race, the bacteria defend against phages using <a href="https://www.earth.com/news/crispr-used-to-remove-extra-chromosomes-in-down-syndrome-and-restore-cell-function/">CRISPR systems</a> and the phages evolve escape mechanisms.



Some phages even boost bacterial metabolism and biofilm formation, affecting disease risk. For instance, phages can transfer genes that enhance bacterial survival in acidic conditions.



<h2 class="wp-block-heading" id="h-virome-s-influence-on-immunity">Virome’s influence on immunity</h2>



The virome affects gut immunity deeply. <a href="https://www.earth.com/news/when-bacteria-get-hungry-they-turn-on-each-other/">Phages</a> can anchor to gut mucus and form a protective barrier. They also shape our own <a href="https://www.ncbi.nlm.nih.gov/books/NBK459471/" target="_blank" rel="noreferrer noopener">T and B cell</a> activity and regulate macrophages. In addition, viruses that infect eukaryotic cells affect immune pathways and maintain gut balance.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/07/virome_microbiome_human-gut_graphic_credit-PCM_1m.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/07/virome_microbiome_human-gut_graphic_credit-PCM_1s.webp" alt="This infographic illustrates four major therapeutic approaches—fecal microbial transplantation (FMT), phage therapy, dietary interventions, and probiotics/prebiotics—that aim to restore gut health by modulating the microbiome and virome. Each strategy offers unique methods, benefits, and challenges in managing gastrointestinal disorders such as IBD, CRC, and CDI, highlighting the growing potential of virome-informed precision medicine. Credit: Precision Clinical Medicine" class="wp-image-1976450"/></a><figcaption class="wp-element-caption">This infographic illustrates four major therapeutic approaches—fecal microbial transplantation (FMT), phage therapy, dietary interventions, and probiotics/prebiotics—that aim to restore gut health by modulating the microbiome and virome. Each strategy offers unique methods, benefits, and challenges in managing gastrointestinal disorders such as IBD, CRC, and CDI, highlighting the growing potential of virome-informed precision medicine. Click image to enlarge. Credit: Precision Clinical Medicine</figcaption></figure>



However, infections and antibiotics can disrupt this harmony and lead to inflammation. Phages can trigger TLR9 pathways, causing excessive immune responses such as those linked to IBD.



<h2 class="wp-block-heading" id="h-virome-s-role-in-disease">Virome’s role in disease</h2>



Imbalances in the gut virome have been linked to several gut diseases. In IBD, specific phages become abundant and worsen inflammation.



Certain groups of phages (such as Caudovirales) amplify immune responses, while norovirus and rotavirus can damage the gut lining. Viral imbalances are also common in IBS and CDI.



In colorectal cancer, phages and eukaryotic viruses like HPV and JC virus (polyomavirus) appear more often. They may promote tumor growth by altering bacterial communities and gene expression.



Studies suggest that some phages directly influence cancer risk by promoting biofilms and transferring harmful genes.



<h2 class="wp-block-heading" id="h-virus-based-treatments">Virus-based treatments</h2>



Several therapies now explore the virome’s potential to treat certain diseases or conditions. Fecal microbiota transplantation (FMT) restores gut balance and reduces inflammation in IBD and CDI.



FMT works not only by shifting bacteria but also by transferring beneficial phages. Studies show that donor phages often align quickly with recipients and promote recovery.



Phage therapy, which uses viruses to kill specific bacteria, is another approach that is gaining traction. It can reduce harmful microbes while preserving beneficial ones.



Researchers have created phage cocktails that target specific gut pathogens like E. coli and Klebsiella pneumoniae, and this approach has had promising results in animal models.



<h2 class="wp-block-heading" id="h-diet-as-a-tool-to-reshape-the-virome">Diet as a tool to reshape the virome</h2>



Dietary strategies also reshape the virome. High-fiber diets boost beneficial phages and support bacterial diversity.



Whey protein has shown potential in managing Crohn’s disease by improving phage-bacteria interactions.



Other interventions, such as exclusive enteral nutrition and low-FODMAP diets, also show benefits in gut diseases.



<h2 class="wp-block-heading" id="h-probiotics-prebiotics-and-phages">Probiotics, prebiotics, and phages</h2>



Probiotics introduce beneficial bacteria, while prebiotics feed them. Combining them, known as symbiotics, shows promise for restoring and maintaining gut health.



Recent research suggests that adding phages can enhance these effects. Phage-based products, such as PreforPro, have already shown benefits in clinical trials.



These products can reduce populations of harmful bacteria and improve probiotic performance, thereby creating a more stable gut environment.



<h2 class="wp-block-heading" id="h-using-gut-viruses-to-detect-diseases-early">Using gut viruses to detect diseases early</h2>



The gut virome is now being studied as a diagnostic tool. Viral patterns are more stable than bacterial ones, making them reliable biomarkers.



Distinct virome signatures can predict IBD and colorectal cancer. Machine learning models already use virome data to detect these diseases early.



Virome profiling may also track treatment responses, such as FMT success in IBD and CDI.



<h2 class="wp-block-heading" id="h-challenges-and-future-prospects">Challenges and future prospects</h2>



Despite the excitement over potential new treatments, many hurdles remain. Current methods struggle to capture the full virome due to technical limits.



Many phages are still unculturable, and their roles remain unclear. Researchers are working to improve viral databases and develop targeted therapies. Once these gaps close, virome-based therapies could change how we treat gut diseases.



The study is published in the journal <a href="https://academic.oup.com/pcm/article/8/2/pbaf010/8152264" target="_blank" rel="noreferrer noopener">Precision Clinical Medicine</a>.



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Move over microbiome, it's time for the human gut's "virome" to shine

For years, bacteria dominated gut health research. Now, the gut...

People often clock thousands of steps a day yet still wonder why the scale or their blood pressure hardly budges. A simple twist on walking, first tested in Japan, may be the missing ingredient.



This "Japanese walking" exercise methodology, called interval walking training (<a href="https://cdnsciencepub.com/doi/10.1139/apnm-2023-0595" target="_blank" rel="noreferrer noopener">IWT</a>), swaps steady strolling for bursts of brisk movement, then recovery‑paced steps.



Cardiometabolic researcher <a href="https://researchprofiles.ku.dk/en/persons/kristian-karstoft" target="_blank" rel="noreferrer noopener">Kristian Karstoft</a> of the University of Copenhagen’s <a href="https://healthyaging.ku.dk/" target="_blank" rel="noreferrer noopener">Center for Healthy Aging</a> has spent more than a decade tracking its effects.



<h2 class="wp-block-heading" id="h-why-pace-changes-matter">Why pace changes matter</h2>



Most walkers cruise at one comfortable speed and never raise their heart rate high enough to stimulate deeper adaptations. 



Switching between fast and slow bouts nudges the body to use oxygen more efficiently, a trait measured by <a href="https://pubmed.ncbi.nlm.nih.gov/17605959/" target="_blank" rel="noreferrer noopener">VO2peak</a>.



That oxygen boost drives down resting blood pressure and encourages muscles to burn more sugar for fuel. It also keeps a session feeling manageable because the recovery intervals prevent the distress that can accompany continuous hard effort.



Regular shifts in speed even appear to sharpen insulin action, regulating blood sugar swings that set the stage for diabetes. 



Scientists call that improvement better <a href="https://www.sciencedirect.com/topics/medicine-and-dentistry/glycemic-control" target="_blank" rel="noreferrer noopener">glycemic control</a>, a term describing how tightly the body keeps glucose within a healthy range.



<h2 class="wp-block-heading" id="h-how-japanese-walking-works">How "Japanese walking" works</h2>



Japanese physiologists outline a straightforward walking recipe, alternating three minutes at roughly seventy percent of personal maximum effort with three minutes around forty percent. Completing five of these cycles takes about half an hour.



“Additionally, interval walking training is a great way to meet the recommended 150 minutes a week of moderate‑intensity aerobic activity,” noted <a href="https://www.massgeneral.org/doctors/23054/sarah-eby" target="_blank" rel="noreferrer noopener">Sarah F. Eby</a>, the sports medicine specialist at Mass <a href="https://www.massgeneral.org/" target="_blank" rel="noreferrer noopener">General Brigham</a> and assistant professor at <a href="https://connects.catalyst.harvard.edu/Profiles/display/Person/211149" target="_blank" rel="noreferrer noopener">Harvard Medical School</a>. 



That schedule, performed on at least five days each week, fits neatly into current public‑health advice to accumulate one hundred fifty minutes of moderate exercise.&nbsp;



A simple watch or phone app can cue the switches, though early Japanese volunteers used a waist‑worn beeper nicknamed <a href="https://www.pubcompare.ai/product/VyniCZIBPBHhf-iFORRd/" target="_blank" rel="noreferrer noopener">JD Mate</a>. Supportive shoes and a safe sidewalk are the only other requirements.



<h2 class="wp-block-heading" id="h-proof-in-older-adults">Proof in older adults</h2>



In a seminal five‑month experiment involving <a href="https://pubmed.ncbi.nlm.nih.gov/25539937/" target="_blank" rel="noreferrer noopener">adults averaging sixty‑three years old</a>, IWT raised VO2peak ten percent and drove <a href="https://www.heart.org/en/health-topics/high-blood-pressure/understanding-blood-pressure-readings" target="_blank" rel="noreferrer noopener">systolic pressure</a> down nine millimeters of mercury compared with either continuous walking or no exercise.



Knee strength climbed as much as seventeen percent, a critical buffer against falls. Body mass index dipped and fasting glucose improved within weeks, suggesting metabolic changes arrive quickly.



What surprised the investigators most was adherence. Ninety‑five percent of more than eight hundred participants kept the habit for the full study window.



Those who logged at least four sessions a week enjoyed the biggest gains, reinforcing the idea that consistency outranks intensity. 



The pattern held over nearly two years, although adherence slipped for volunteers starting with higher waistlines.



<h2 class="wp-block-heading" id="h-benefits-of-iwt-japanese-walking">Benefits of IWT Japanese walking</h2>



A Danish trial later pitted IWT against energy‑matched continuous <a href="https://www.earth.com/news/dog-walking-improves-mobility-and-prevents-falls-in-older-adults/">walking</a> in adults living with type 2 diabetes. 



Only the interval group shrank abdominal fat and cut twenty‑four‑hour glucose fluctuations, despite similar caloric burn.



“Compared to energy‑expenditure and time‑duration matched continuous walking training, IWT is superior for improving physical fitness, body composition, and glycemic control in individuals with type 2 diabetes,” stated Karstoft. 



Follow‑up mechanistic work pointed toward enhanced glucose effectiveness, meaning muscles absorbed sugar without extra insulin. 



<h2 class="wp-block-heading" id="h-safety-and-sticking-with-it">Safety and sticking with it</h2>



Because walking remains fully aerobic, lactate rarely spikes and the risk of cardiac complications stays low. No serious adverse events surfaced across dozens of trials, even among recent joint‑replacement patients cleared by their surgeons.



Digital prompts can help sustain motivation once novelty fades. Yet data from a Danish smartphone roll‑out show that unsupervised users averaged only nine minutes of fast <a href="https://www.earth.com/news/upright-walking-may-have-sparked-human-creativity-and-music/">walking</a> per week after a year, underscoring the value of social or clinical follow‑up.



Coaching, group strolls, or gamified leaderboards may lift engagement, particularly for people carrying extra weight. 



Researchers are testing whether regular phone calls paired with step‑count feedback can duplicate laboratory adherence in the real world.



<h2 class="wp-block-heading" id="h-getting-started-today">Getting started today</h2>



Consult your clinician if you have chronic conditions, then pick a flat route and set a timer for thirty minutes. Begin with one minute brisk, one minute relaxed for fifteen cycles, or even shorter bursts until comfort builds.



“Studies specifically looking at the benefits of interval <a href="https://www.earth.com/news/walking-can-counteract-the-health-risks-of-sitting/">walking training</a> have found improved physical fitness, muscle strength, and glycemic control,” said Eby. 



She advises ramping up gradually so each brisk interval still allows a short phrase before breath runs out.



Track sessions on a calendar; seeing streaks grow is strangely satisfying. Celebrate milestones such as a lower belt notch or an easier climb up the porch steps.



A final word for anyone who thinks walking is too gentle to matter, remember that pace, not mileage, drives adaptation. 



The Japanese approach proves that swapping a few calm blocks for a confident stride can steer health markers in the right direction long before you break into a jog.



The study is published in <a href="https://cdnsciencepub.com/doi/10.1139/apnm-2023-0595" target="_blank" rel="noreferrer noopener">Applied Physiology, Nutrition, and Metabolism</a>.



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This Japanese walking technique improves health and prevents disease

People often clock thousands of steps a day yet still...

Off the eastern tip of Java, dredging barges dragged up more than sand. They pulled a piece of the past: a submerged river valley under the Madura Strait packed with fossils that had slept under fifty feet of water since long before the last Ice Age melted away.



Among the finds were two skull fragments of Homo erectus, a <a href="https://www.earth.com/news/fossil-discovery-anadoluvius-turkae-suggests-humans-originated-in-europe-not-africa/">human ancestor</a> that roamed Asia until roughly 117,000 years ago, as well as more than 6,000 animal fossils that paint a vivid portrait of a lost ecosystem. <a href="https://www.universiteitleiden.nl/en/staffmembers/harry-berghuis" target="_blank" rel="noreferrer noopener">Harold Berghuis</a> of <a href="https://www.universiteitleiden.nl/en" target="_blank" rel="noreferrer noopener">Leiden University</a> leads the team studying the haul.



<h2 class="wp-block-heading" id="h-sundaland-rises-then-sinks">Sundaland rises then sinks</h2>



During colder glacial times, much of Southeast Asia’s continental shelf formed a single low‑lying continent known as <a href="https://www.cepf.net/our-work/biodiversity-hotspots/sundaland#:~:text=The%20Sundaland%20Biodiversity%20Hotspot%20covers,islands%20of%20Borneo%20and%20Sumatra." target="_blank" rel="noreferrer noopener">Sundaland</a>. 



Sea level then sat about 400 feet lower than it does today, exposing wide plains crisscrossed by rivers and grasslands.



When global ice melted between <a href="https://www.nature.com/articles/s42003-023-04510-0" target="_blank" rel="noreferrer noopener">22,000 and 6,000 years ago</a>, the ocean climbed roughly 443 feet, drowning half of that landmass. 



The rapid pulses of rise carved islands out of peninsulas and pushed coastlines hundreds of miles inland, isolating plants, animals, and the people who depended on them.



Geologists can still follow the drowned river channels with high‑resolution sonar. Each channel marks a corridor that once connected Borneo, Sumatra, and Java to the Asian mainland, providing migration routes for both megafauna and hominins.



<h2 class="wp-block-heading" id="h-river-fossils-under-the-madura-strait">River fossils under the Madura Strait</h2>



The valley now mapped under the Madura Strait was carved by the ancient Solo River. 



Optically Stimulated Luminescence dating (<a href="https://www.antarcticglaciers.org/glacial-geology/dating-glacial-sediments-2/optically-stimulated-luminescence/" target="_blank" rel="noreferrer noopener">OSL</a>) shows its sandy fill settled between 162,000 and 119,000 years ago, anchoring the new fossils to the late <a href="https://www.sciencedirect.com/science/article/pii/S295023652500012X" target="_blank" rel="noreferrer noopener">Pleistocene</a>.



OSL works because quartz grains store energy from cosmic rays like tiny batteries. When technicians shine a laser on a grain in the lab, it releases that stored charge as light, revealing the moment the grain last basked in sunlight.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/07/madura-strait_sunda-shelf_homo-erectus-remains_map_credit-ScienceDirect_1m.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/07/madura-strait_sunda-shelf_homo-erectus-remains_map_credit-ScienceDirect_1s.webp" alt="The Sunda Shelf of Southeast Asia, with the Indonesian archipelago. Box indicates the position of map B. B: Eastern Java, the Madura Strait, the Solo River, Ngandong, Sambungmacan, and other hominin sites. Box indicates the position of map C. C: The Madura Strait north of Surabaya, with the sand extraction area and the location of the BMS land-reclamation. Map data: GEBCO and ALOS" class="wp-image-1976530"/></a><figcaption class="wp-element-caption">The Sunda Shelf of Southeast Asia, with the Indonesian archipelago. Box indicates the position of map B. B: Eastern Java, the Madura Strait fossils location, the Solo River, Ngandong, Sambungmacan, and other hominin sites. Box indicates the position of map C. C: The Madura Strait north of Surabaya, with the sand extraction area and the location of the BMS land-reclamation. Click image to enlarge. Map data: GEBCO and ALOS</figcaption></figure>



The method is ideal for underwater sites where radiocarbon fails, yet it is rarely applied because retrieving uncontaminated samples from the seafloor is difficult. 



The Madura team’s success shows how pipeline spoil, often discarded as waste, can become forensic evidence on continental‑scale change.



<h2 class="wp-block-heading" id="h-madura-strait-reveals-fossil-menagerie">Madura Strait reveals fossil menagerie</h2>



The tally of species rivals a natural‑history museum catalog. There were buffalo, several kinds of deer, and <a href="https://nationalzoo.si.edu/animals/komodo-dragon" target="_blank" rel="noreferrer noopener">Komodo dragons</a> longer than a canoe.



The biggest draw, though, is <a href="https://eartharchives.org/articles/stegodon-the-elephant-with-sideways-trunk/index.html" target="_blank" rel="noreferrer noopener">Stegodon trigonocephalus</a>, an elephant‑like giant that could stand almost 13 feet at the shoulder. 



Its presence suggests tall grass and open water holes, conditions that match pollen studies from upland Java.



Fossil monitors link today’s dragon‑patrolled islands to their mainland roots; remains of <a href="https://ielc.libguides.com/sdzg/factsheets/komododragon" target="_blank" rel="noreferrer noopener">Varanus komodoensis</a> have turned up on nearby <a href="https://www.theextinctions.com/articles-1/lesser-sunda-islands-part-1-flores-and-sumba" target="_blank" rel="noreferrer noopener">Flores and Sumba</a>, confirming that the apex lizard once ranged far beyond its present refuges. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/07/maduro-strait_indonesia_homo-erectus_ancient-remains_credit-ScienceDirect_1m.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/07/maduro-strait_indonesia_homo-erectus_ancient-remains_credit-ScienceDirect_1s.webp" alt="Madura Strait 1 (MS1): Homo erectus frontal fragment with dextral supraorbital torus. A: Photographs. B: CT-based 3D surface rendered images. Note that the exact orientation of the fragment is unknown. For the anterior view, a slightly diagonal orientation has been assumed. C: CT-based 3D surface rendered image of MS1 in a more horizontal orientation, with anatomical indications. D: CT-slice. Credit: ScienceDirect" class="wp-image-1976532"/></a><figcaption class="wp-element-caption">Madura Strait 1 (MS1) fossils: Homo erectus frontal fragment with dextral supraorbital torus. A: Photographs. B: CT-based 3D surface rendered images. Note that the exact orientation of the fragment is unknown. For the anterior view, a slightly diagonal orientation has been assumed. C: CT-based 3D surface rendered image of MS1 in a more horizontal orientation, with anatomical indications. D: CT-slice. Click image to enlarge. Credit: ScienceDirect</figcaption></figure>



Carnivore teeth in the assemblage are scarce, hinting that reptiles, not big cats, topped the food chain.



Antelope‑like bovids and open‑country rodents round out the scene, pointing to savanna rather than rainforest. Together the bones sketch a community more East African than Indonesian.



<h2 class="wp-block-heading" id="h-humans-with-tools-and-strategy">Humans with tools and strategy</h2>



Researchers counted more than 300 bones marked by stone blades or flakes. Some show percussion scars where marrow was pounded out.



“The Sunda Shelf played an important role in the dispersal and evolution of hominin populations,” wrote Berghuis and colleagues in their 2025 report. Others bear parallel slices typical of tendon removal.&nbsp;



“Thus far, hominin <a href="https://www.earth.com/news/archaeopteryx-fossil-soft-tissue-flight-evolution-proves-darwin-right/">fossils</a> from submerged Sundaland were not available.” The Madura Strait fragments break that drought. Underscoring the novelty of the find.&nbsp;



Tool cut geometry matches <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC4920301/" target="_blank" rel="noreferrer noopener">Acheulean‑derived technologies</a> already known from Java’s terrestrial sites. That continuity supports the idea that people followed rivers seasonally, carrying simple gear that was easy to replace when tools were lost in mud or water.



<h2 class="wp-block-heading" id="h-what-the-skulls-add-to-the-story">What the skulls add to the story</h2>



Although each piece is only a few inches across, the brow ridge profile and bone thickness match late <a href="https://pubmed.ncbi.nlm.nih.gov/18479734/" target="_blank" rel="noreferrer noopener">Homo erectus skulls</a> dug from Ngandong and Sambungmacan farther up the Solo. 



That link pushes the species’ confirmed range hundreds of miles east, showing it followed river corridors onto the shelf when sea level was low.



One fragment comes from an adolescent, the other from a lightly built adult. Their presence alongside butchered game hints that family groups, not lone hunters, roamed the valley.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/07/maduro-strait_indonesia_homo-erectus_skull_credit-ScienceDirect_1.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/07/maduro-strait_indonesia_homo-erectus_skull_credit-ScienceDirect_1s.webp" alt="3D surface images of MS1 and Sambungmacan 3 (anterior view). This comparative skull has the closest metric and morphological match with MS1. Credit: ScienceDirect" class="wp-image-1976534"/></a><figcaption class="wp-element-caption">3D surface images of Madura Strait (MS1) and Sambungmacan 3 (anterior view) fossils. This comparative skull has the closest metric and morphological match with MS1. Click image to enlarge. Credit: ScienceDirect</figcaption></figure>



Because no fire traces were found, the visitors probably camped on higher terraces that are now long submerged. 



The bones they left behind washed into lower channels during seasonal floods and were sealed beneath overbank sand.



<h2 class="wp-block-heading" id="h-looking-for-cousins-beneath-the-waves">Looking for cousins beneath the waves</h2>



The Solo River was only one of many channels draining Sundaland. As survey vessels map more buried valleys, archaeologists expect to meet a wider cast: <a href="https://www.earth.com/news/mysterious-denisovan-species-humans-lived-undisturbed-tibetan-plateau-160000-years/">Denisovans</a>, perhaps, or even the diminutive <a href="https://australian.museum/learn/science/human-evolution/homo-floresiensis/" target="_blank" rel="noreferrer noopener">Homo floresiensis</a>.



Every bucket of dredged sand now promises not just minerals for construction but clues to human origins. 



Underwater archaeology once focused on shipwrecks; now it is turning to paleolandscapes that could double the search area for early humans in Southeast Asia.



The Indonesian government is drafting guidelines that will require sand‑mining companies to report <a href="https://www.earth.com/news/scientists-find-a-47-million-year-old-cicada-fossil-with-preserved-wing-details/">fossil</a> finds within 48 hours. 



Those rules could transform commercial dredges into accidental research partners, expanding the data set at a fraction of normal field costs.



For now the Madura Strait cache stands alone, yet it already stretches the timeline of underwater archaeology in Asia. 



Skulls, riverbeds, and giant beast bones, all locked together in a drowned landscape, remind us that today’s ocean floor was yesterday’s hunting ground.



The study is published in <a href="https://www.sciencedirect.com/science/article/pii/S295023652500012X?via%3Dihub" target="_blank" rel="noreferrer noopener">Quaternary Environments and Humans</a>.



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Archaeologists find 140,000-year-old human and animal remains at the bottom of the ocean

Off the eastern tip of Java, dredging barges dragged up...

In the United States, about 32 percent of adults now have at least one tattoo. Despite their widespread presence across all walks of life, tattoos still trigger snap judgments about an individual's personality, values, or lifestyle.



A new study from <a href="https://msu.edu/" target="_blank" rel="noreferrer noopener">Michigan State University</a> questions those snap judgments. The study revealed that observers frequently misinterpret personality traits based on tattoo content, style, and appearance



<h2 class="wp-block-heading" id="h-tattoos-are-common-but-still-judged">Tattoos are common but still judged</h2>



Ink has become a common part of daily life, from teachers' forearms to politicians' ankles. <a href="https://www.pewresearch.org/wp-content/uploads/2023/08/SR_23.08.15_Tattoos_topline.pdf" target="_blank" rel="noreferrer noopener">Eight in ten Americans</a> say their communities are now more accepting of body art compared to 20 years ago.



Even so, a deep undercurrent of <a href="https://pubmed.ncbi.nlm.nih.gov/28934022/" target="_blank" rel="noreferrer noopener">tattoo stigma</a> survives. Earlier research found that tattooed adults were viewed as more deviant, less conscientious, and more promiscuous than their un‑inked peers. 



Children as young as six linked tattoos to delinquent behavior in a classic 2000 <a href="https://bpspsychub.onlinelibrary.wiley.com/doi/abs/10.1348/135532500168065" target="_blank" rel="noreferrer noopener">study</a> by Durkin and Houghton.



Studies also show <a href="https://www.psychologytoday.com/ca/blog/head-games/201809/are-people-with-tattoos-stigmatized" target="_blank" rel="noreferrer noopener">gender effects</a>. Women with visible ink are often judged more harshly than men, especially in hospitality and healthcare settings.



Modern workplaces try to project inclusivity, yet hiring managers still admit that visible <a href="https://www.earth.com/news/wireless-e-tattoo-detects-when-your-brain-gets-overloaded/">ink</a> can hurt an applicant. Simmering bias fuels a market for makeup that covers sleeves during interviews.



<h2 class="wp-block-heading" id="h-tattoo-and-personality-links">Tattoo and personality links</h2>



William Chopik and Brooke Soulliere, both psychologists at Michigan State University, photographed 375 tattoos from 274 volunteers. The volunteers completed a full <a href="https://www.truity.com/test/big-five-personality-test" target="_blank" rel="noreferrer noopener">Big Five personality traits</a> inventory before rolling down their sleeves.



“We found that people did tend to rate the personalities of tattooed people consistently,” explained Chopik. 



A separate panel looked only at each image and guessed the wearer’s personality. Observers saw the ink but not the person’s face, clothing, or setting. That design isolated the tattoo as the single visible cue, mimicking quick judgments made on a sidewalk or social feed.



Soulliere added that the study covered 18 features, from size to color to placement. Testing each cue against personality scores allowed the team to see which visual <a href="https://www.earth.com/news/tattoos-increase-the-risk-of-developing-lymphoma/">hints</a>, if any, were worth trusting.



<h2 class="wp-block-heading" id="h-tattoos-rarely-show-true-personality">Tattoos rarely show true personality</h2>



The results showed agreement among raters, meaning most viewers made the same assumptions. Agreement, however, is not accuracy. 



Traits such as agreeableness, conscientiousness, extraversion, and neuroticism were wrongly assigned. The raters’ confidence did not rescue their guesses.



Psychologists describe this pattern with the <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC9103609/" target="_blank" rel="noreferrer noopener">lens model</a>, which says people read surface cues to infer hidden qualities. Tattoos act as one such lens, but the view they provide can be cloudy. Studies over the past decade linked skulls, guns, or prison motifs to criminal stereotypes among jurors.



Sticker‑covered <a href="https://www.sciencedirect.com/science/article/abs/pii/S0092656621001239" target="_blank" rel="noreferrer noopener">laptops</a> tell a parallel story. Raters accurately judged an <a href="https://www.earth.com/news/tattoo-ink-travels-through-the-body-and-may-cause-long-term-risks/">owner</a>’s openness and extraversion by glancing at personalized decals.



<h2 class="wp-block-heading" id="h-tattoo-meaning-and-personality-often-clash">Tattoo meaning and personality often clash</h2>



Getting tattooed often involves what psychologists call identity claims. A self‑directed claim might memorialize a child’s birthdate, while an other‑directed claim signals allegiance to a military unit or sports team. 



The problem arises when outsiders guess the message without context. A snake entwined with roses could honor recovery from illness, yet many will see danger or rebellion.



Anthropologists note that body art has held meaning across cultures for millennia, from Polynesian rite‑of‑passage marks to Japanese irezumi. Western viewers unfamiliar with these traditions may project their own narratives instead.



Social media accelerates the misreading. A single viral image can lock a stranger into a public persona built on nothing more than a wrist tattoo glimpsed under café lights.



<h2 class="wp-block-heading" id="h-tattoos-link-to-openness-only">Tattoos link to openness only</h2>



The Michigan State team uncovered one sliver of accuracy. Viewers who saw a tattoo described as quirky, goofy, or simply odd tended to peg the owner as high in openness to experience. 



“When people see a wacky or goofy tattoo, they assume that person is open to experience, and they’re correct about it,” noted Soulliere.



Openness tracks curiosity, creativity, and a hunger for novelty. A full sleeve of abstract color or a playful cartoon can hint at those traits more faithfully than a skull wrapped around a dagger. 



Many open‑minded folks choose minimalist ink, and some conventional thinkers pick bold designs on a dare.



Researchers suspect the accuracy stems from selection rather than signal. People high in openness may be drawn to unusual images, so the art style predicts the trait.



<h2 class="wp-block-heading" id="h-tattoo-and-personality-bias-affects-life">Tattoo and personality bias affects life</h2>



Snap judgments about tattoos happen in classrooms, clinics, courtrooms, and dating apps. Mistaking agreeableness or conscientiousness can nudge decisions on trust, hiring, or even sentencing. 



Bias also works inward. People who know the stereotypes may edit their ink choices to avoid certain images, limiting self‑expression in subtle ways.



Future research may test whether adding context - such as the story behind a tattoo - improves accuracy. For now, experts urge caution before reading too much into a rose, a dragon, or a pop‑culture tribute.



<h2 class="wp-block-heading" id="h-reducing-tattoo-and-personality-bias">Reducing tattoo and personality bias</h2>



The first step is awareness, and studies like this one give people an evidence‑based reason to pause before leaping to conclusions. 



Training programs in customer service and law enforcement already include modules on implicit bias, but tattoos rarely appear in those slides.



Organizations could add quick reminders that body art alone predicts little besides a taste for ink. A supervisor who knows that fact is less likely to equate a forearm phoenix with poor reliability. 



Small actions add up. Asking an employee about their new tattoo, rather than assuming its meaning, turns a potential bias trap into a conversation starter.



The study is published in the <a href="https://www.sciencedirect.com/science/article/abs/pii/S0092656625000613?via%3Dihub" target="_blank" rel="noreferrer noopener">Journal of Research in Personality</a>.



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Tattoos lead to mistaken assumptions about personality and values

In the United States, about 32 percent of adults now...

Tiny bits of plastic no wider than a human hair have turned up in some unexpected places, including the human bloodstream. 



Now, data presented at the European Society of Human Reproduction and Embryology meeting shows that these <a href="https://www.earth.com/news/microplastics-spread-deep-into-the-ocean-far-below-the-surface/">fragments</a> have breached the fluids that surround eggs and travel with sperm.



The research team led by Dr. Emilio Gómez‑Sánchez of Next Fertility Murcia in Spain scanned <a href="https://www.sciencedirect.com/topics/biochemistry-genetics-and-molecular-biology/follicular-fluid" target="_blank" rel="noreferrer noopener">follicular fluid</a> from 29 women and seminal fluid from 22 men.



The experts found microplastics in 69 percent of the women and 55 percent of the men they studied. According to Dr. Gómez‑Sánchez, the team was surprised to find that the particles were so widespread.



<h2 class="wp-block-heading" id="h-plastics-in-human-reproductive-fluids">Plastics in human reproductive fluids</h2>



The study detected polymers such as <a href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/polytetrafluoroethylene" target="_blank" rel="noreferrer noopener">polytetrafluoroethylene</a> and <a href="https://adrecoplastics.co.uk/polypropylene-uses/" target="_blank" rel="noreferrer noopener">polypropylene</a>, materials better known for slick frying pans and food packaging. Seeing them next to human eggs turns a theoretical hazard into a measurable one.



Back in 2021, Italian obstetricians spotted twelve plastic fragments in every placenta they examined, confirming that particles smaller than five millimeters can cross the <a href="https://pubmed.ncbi.nlm.nih.gov/33395930/" target="_blank" rel="noreferrer noopener">maternal‑fetal boundary</a>.



Similarly sized particles have been uncovered deep in <a href="https://pubmed.ncbi.nlm.nih.gov/35364151/" target="_blank" rel="noreferrer noopener">lung tissue</a> removed during surgery, proving that inhalation is a realistic delivery route for <a href="https://www.earth.com/news/simple-way-to-remove-microplastics-from-tap-water-home-faucet/">plastic</a> dust.



Researchers in the Netherlands have even measured plastic mass circulating in human blood samples, an <a href="https://pubmed.ncbi.nlm.nih.gov/35367073/" target="_blank" rel="noreferrer noopener">observation</a> that explains how fragments migrate to distant tissues.



<h2 class="wp-block-heading" id="h-how-plastics-enter-the-human-body">How plastics enter the human body</h2>



Most people take in <a href="https://www.earth.com/news/microplastics-in-human-brains-may-affect-mental-health/">plastic</a> flecks by eating, drinking, or breathing, because everyday products shed invisible dust whenever they are heated, abraded, or exposed to sunlight. 



Once swallowed or inhaled, particles small enough can slip through the gut wall or the thin air‑blood membrane in the lungs.



Animal studies suggest that fragments under one micrometer can enter cells directly, whereas larger shards get trapped in tissue and spark local irritation. Either way, they bypass the body’s usual waste filters.



Laboratory work on mice shows that digestive uptake rises when <a href="https://www.earth.com/news/airborne-microplastics-where-they-come-from-and-where-they-go/">microplastics</a> hitchhike on fats, a detail that matters for fertility research because reproductive hormones ride on similar lipid highways. 



The overlap raises worry that plastics may act as endocrine mimics or carriers for other chemicals.



Dr. Gómez‑Sánchez’s team avoided laboratory contamination by collecting every human sample in glass vials and verifying the absence of background plastic. This means the polymers they found were genuine residents, not stray lab dust.



<h2 class="wp-block-heading" id="h-plastic-harms-fertility">Plastic harms fertility</h2>



Mice exposed to polystyrene fragments shed sperm with damaged DNA and sluggish movement, effects traced to <a href="https://pubmed.ncbi.nlm.nih.gov/31896473/" target="_blank" rel="noreferrer noopener">oxidative stress</a> that overwhelms antioxidant defenses.



Separate <a href="https://pubmed.ncbi.nlm.nih.gov/36948006/" target="_blank" rel="noreferrer noopener">work</a> on rodent Leydig cells shows shriveled mitochondria after nanoplastic exposure, which throttles testosterone production and shrinks litter sizes.



Reviews published in 2024 concluded that microplastics can disrupt the <a href="https://pubmed.ncbi.nlm.nih.gov/38750730/" target="_blank" rel="noreferrer noopener">hypothalamic‑pituitary‑gonadal axis</a>, leading to hormonal imbalances and faulty egg maturation.



Because human oocytes develop over months, chronic exposure could matter more than a short spike. That makes the repeated detection of PTFE in both eggs and sperm especially noteworthy.



<h2 class="wp-block-heading" id="h-plastic-levels-in-eggs-and-sperm">Plastic levels in eggs and sperm</h2>



In the current data set, PTFE appeared in 31 percent of sampled egg fluid and 41 percent of semen. PP ranked second among women and <a href="https://www.chemicalsafetyfacts.org/chemicals/polystyrene/" target="_blank" rel="noreferrer noopener">polystyrene</a> second among men, with <a href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/polyethylene-terephthalate" target="_blank" rel="noreferrer noopener">polyethylene terephthalate</a> also present but in smaller numbers.



Annual plastic output has climbed from under two million tons in 1950 to about 460 million in 2019, a 230‑fold jump documented by the <a href="https://pubmed.ncbi.nlm.nih.gov/36969097/" target="_blank" rel="noreferrer noopener">Minderoo‑Monaco Commission on Plastics and Human Health</a>.



Each uptick in production increases litter, weathering, and fragment release, tightening the feedback loop between plastics and people. Reproductive cells, delicate by design, stand on the front line.



Gómez‑Sánchez reported that most reproductive samples contained only one or two plastic particles, amounts considered low compared with overall debris in the fluids. Yet fertility specialists note that even trace metals can derail embryo development, so particle counts alone may not predict risk.



<h2 class="wp-block-heading" id="h-human-fertility-research-must-include-plastics">Human fertility research must include plastics</h2>



“They should be considered an additional argument in favor of avoiding the generalized use of plastics in our daily lives,” said Professor Carlos Calhaz‑Jorge of the University of Lisbon. He also noted that further research is needed to prove causation.



The research team will now study hundreds of patients and link particle loads to embryo quality during <a href="https://my.clevelandclinic.org/health/treatments/22457-ivf" target="_blank" rel="noreferrer noopener">in vitro fertilization cycles</a>. Those correlations could supply the first direct human evidence beyond laboratory rodents.



They plan lifestyle questionnaires to test whether habits such as heavy bottled‑water use or microwaving food in plastic correlate with higher particle counts. The approach could convert abstract exposure theory into personal advice.



“Microplastics are just one variable in a complex equation,” said Dr. Gómez‑Sánchez. He urges moderation of plastic use rather than alarm. 



<h2 class="wp-block-heading" id="h-simple-habits-to-lower-exposure">Simple habits to lower exposure</h2>



Switching from plastic bottles to glass or stainless steel lowers ingestion because heat and time no longer leach particles from container walls. Replacing scratched nonstick pans can cut PTFE flakes in the diet.



Researchers advise skipping plastic cutting boards and using ceramic or bamboo instead, because knife action liberates shavings that cling to food. Letting take‑out cool before transferring it from polystyrene boxes also helps.



Air purifiers with HEPA filters capture airborne fibers shed by synthetic textiles, a step especially useful for nurseries. Regular vacuuming with a sealed system keeps particles from resuspending.



These tweaks are not foolproof, yet they come with side benefits like removing chemical additives that ride on plastic dust. They buy time while science sorts out the clinical stakes.



<h2 class="wp-block-heading" id="h-efforts-to-cut-human-plastics-pollution">Efforts to cut human plastics pollution</h2>



Public‑health researchers argue that personal choices alone cannot outrun a supply chain making more than a billion pounds of new plastic every day. 



Negotiators at the United Nations are hammering out a global treaty that could cap production and streamline recycling.



<a href="https://www.bc.edu/bc-web/schools/morrissey/departments/biology/people/faculty-directory/Phil-Landrigan.html" target="_blank" rel="noreferrer noopener">Dr. Philip Landrigan</a> of Boston College calls the treaty a once‑in‑a‑generation chance to protect human health, because curbing output remains the only sure way to slow microplastic fallout. He points to the emerging fertility data as evidence that time is short.



Whether lawmakers act or not, the science of sub‑visible plastic is moving fast thanks to sharper imaging tools and nanomechanical sensors. Studies that once took months now finish in days, filling the literature with fresh clues.



Every new dataset sharpens the same picture: plastics weather into dust, the dust goes everywhere, and living tissue keeps no closed doors. Eggs and sperm, it turns out, are no exception.



The study is published in the journal <a href="https://academic.oup.com/humrep#google_vignette" target="_blank" rel="noreferrer noopener">Human Reproduction</a>.



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Tiny plastic particles found in human egg and sperm fluids

Tiny bits of plastic no wider than a human hair...

The sea spider, those spindly marine oddities that seem composed almost entirely of legs and claws, just given up their genetic secrets.



An international effort led by the <a href="https://www.univie.ac.at/en/">University of Vienna</a> and the <a href="https://www.wisc.edu/">University of Wisconsin–Madison</a> has delivered the first chromosome-level genome for Pycnogonum litorale, a species common in North Atlantic tide pools.



Stretching across 57 pseudo-chromosomes and paired with extensive developmental transcriptomes, the assembly offers an unprecedented look at how an arthropod can evolve such an extreme body plan. This includes a nearly vanishing abdomen and internal organs that spill far into its limbs.



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



To achieve a genome this contiguous, the team combined long-read sequencing with Hi-C proximity data. Long reads captured tens of thousands of DNA bases at a stretch. This helped bridge the repetitive regions that routinely break short-read assemblies.



Hi-C, which measures how DNA folds inside the nucleus, then provided a “scaffolding” map that placed those long contigs into chromosomal order.



“The genomes of many non-canonical laboratory organisms are challenging to assemble, and Pycnogonum is no exception," said first author Nikolaos Papadopoulos, a zoologist at the University of Vienna. 



"Only the combination of modern high-throughput data sources made a high-quality genome possible. This can now serve as a stepping stone for further research.”



Because <a href="https://www.earth.com/news/surprising-breeding-behaviors-of-giant-sea-spiders-revealed/">sea spiders</a> are not standard lab animals, researchers collected specimens by hand, often prying them from kelp during low tide. They then rushed them back to the lab for nucleic acid extraction.



The payoff is a reference genome that joins spider, <a href="https://www.earth.com/news/fossil-reveals-the-first-ancestors-of-scorpions-and-spiders/">scorpion</a>, mite, and horseshoe crab assemblies on public databases. Yet it lacks the duplications that mark other arachnid genomes, making it a vital baseline for evolutionary comparisons.



<h2 class="wp-block-heading" id="h-vanished-gene-vanished-abdomen">Vanished gene, vanished abdomen</h2>



The analysis focused on Hox genes, key developmental regulators shared by animals from fruit flies to humans. One gene turned up missing: abdominal-A (abd-A).



In most arthropods, abd-A helps establish the rear-body segments that carry guts and reproductive organs. Sea spiders, with their virtually absent abdomens, appear to have dispensed with both the physical structure and its genetic architect.



“In arthropods, Hox genes play a central role in the correct specification of the different body segments, explained co-author Andreas Wanninger, who co-led the Vienna team. "In many other animal groups they are essential ‘master controllers’ during body plan development.” 



The disappearance of abd-A mirrors patterns seen in <a href="https://www.earth.com/news/how-mites-survived-without-sex-for-millions-of-years/">mites</a> and barnacles, two other arthropod groups that have independently shrunk or lost their hind segments.



<h2 class="wp-block-heading" id="h-sea-spiders-skipped-genome-doubling">Sea spiders skipped genome doubling</h2>



Spiders and scorpions carry extra copies of almost every gene, relics of an ancient whole-genome duplication that likely fueled innovations such as silk glands and complex venom cocktails.



P. litorale shows no sign of that event. Because sea spiders sit at the very base of the chelicerate lineage, the simplest explanation is that the duplication occurred later. It likely arose within the spider-scorpion branch, rather than in the common ancestor of all chelicerates.



That finding reshapes timelines for when gene families expanded and may help researchers pinpoint which duplications underlie spider-specific traits.



<h2 class="wp-block-heading" id="h-tools-for-growth-and-repair">Tools for growth and repair</h2>



Beyond raw sequence, the consortium generated RNA profiles from embryos and juveniles, capturing when each gene flicks on and off as new body segments form.



Those developmental datasets make the sea spider a promising model for studies of ancestral arthropod development, limb regeneration, and physiological resilience in cold, nutrient-poor seas.



Georg Brenneis, an expert in arthropod development at the University of Vienna, is a senior author of the study.



“From an evolutionary developmental perspective, sea spiders are very interesting: their mode of development may be ancestral for arthropods, but at the same time they boast multiple body plan innovations unique to themselves. Beyond this, they also possess remarkable regenerative abilities.” 



“Now that we have the genome and comprehensive datasets on gene activities during development, we can systematically study all of these aspects on the molecular level,” he said.



<h2 class="wp-block-heading" id="h-editing-limbs-and-trunk">Editing limbs and trunk</h2>



With <a href="https://www.earth.com/news/crispr-used-to-remove-extra-chromosomes-in-down-syndrome-and-restore-cell-function/">CRISPR</a> editing becoming feasible in marine invertebrates, investigators can now ask how the remaining sea spider Hox genes choreograph eight elongated walking legs and a tubular trunk. They can also explore how the animals quickly regrow lost appendages.



Comparative physiologists might search the genome for stress-response genes that let sea spiders thrive in icy fjords, while ecological genomics teams could examine how gene flow operates across their wide geographic ranges.



<h2 class="wp-block-heading" id="h-tracing-ancient-sea-spider-cousins">Tracing ancient sea spider cousins</h2>



Without the duplication, shared sea spider genes likely existed as single copies in the last common chelicerate ancestor.



Aligning those sequences will clarify where new venom toxins arose, when silk machinery evolved, and how immune genes diversified.



The genome also lets scientists investigate regulatory DNA - enhancers, promoters, and non-coding RNAs. These elements rewired a conventional arthropod blueprint into the minimalist sea spider form.



<h2 class="wp-block-heading" id="h-expanding-the-genomic-catalog">Expanding the genomic catalog</h2>



The authors envision expanding the catalog to additional sea spider species to test whether abd-A loss is universal. They also aim to map gains and losses of other developmental genes across the group’s 1,300 known species.



Such work could uncover genetic shortcuts to extreme morphological change - insights that extend far beyond any single marine arthropod.



For now, the P. litorale genome stands as a milestone: the first high-quality reference for the world’s most enigmatic chelicerates. It’s also a reminder that even life’s strangest branches follow molecular rules that genomics can finally reveal.



The study is published in the journal <a href="https://bmcbiol.biomedcentral.com/articles/10.1186/s12915-025-02276-x">BMC Biology</a>.



Image Credit: Richard Lord/ <a href="https://creativecommons.org/licenses/by-nc-sa/4.0/legalcode.en">CC BY-NC-SA 4.0</a>



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All legs, no guts: Sea spider genome stuns scientists

The sea spider, those spindly marine oddities that seem composed...

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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