Today's Image of the Day from the European Space Agency features Messier 78 (M78), a reflection nebula located in the constellation Orion about 1,350 light-years away from Earth.&nbsp;



This image was released as part of the initial series of observations from ESA's <a href="https://www.esa.int/Science_Exploration/Space_Science/Euclid" target="_blank" rel="noreferrer noopener">Euclid space mission</a>.&nbsp;



All data collected during these early observations, including a series of incredible <a href="https://www.esa.int/Science_Exploration/Space_Science/Euclid/Euclid_s_first_images_the_dazzling_edge_of_darkness" target="_blank" rel="noreferrer noopener">new views</a> of the nearby universe, is available to the public.&nbsp;



<h2 class="wp-block-heading" id="h-image-of-messier-78">Image of Messier 78</h2>



Messier 78 is a dynamic region of star formation that is obscured by cosmic dust in this high-resolution image captured by the Euclid space telescope.



This specific view highlights how young stars generate winds of charged particles, carving out “cavities” in the molecular clouds around them.&nbsp;



The blue hues in the image represent ionized atomic hydrogen, which is a primary component of the cloud, while the red indicates the absorption and scattering of light by dust particles.



The image captures hundreds of stars varying in brightness, illuminating their nebulous, purple surroundings. A dark, arch-like structure stretches from the upper left to the bottom right of the frame, merging into the densest, darkest clouds at the image’s base.



<h2 class="wp-block-heading" id="h-active-site-of-star-formation-nbsp">Active site of star formation&nbsp;</h2>



Messier 78 is not just a single nebula but part of a larger complex of stars and nebulous regions in <a href="https://www.earth.com/news/orion-nebula-destroys-an-oceans-worth-of-water-every-month/" target="_blank" rel="noreferrer noopener">Orion</a>, which includes various other objects like dark nebulae that are visible as patches blocking light from behind.



This region is an active site of star formation, featuring many young stars and protostars, which are stars in the early stages of formation.&nbsp;



<h2 class="wp-block-heading" id="h-viewing-messier-78">Viewing Messier 78</h2>



M78 is easily observable with small telescopes, and it appears as a hazy patch of light with two prominent stars near its center, which illuminate the surrounding dust.&nbsp;



The nebula is also a favorite among amateur astronomers for its beauty and relatively bright appearance.



<h2 class="wp-block-heading" id="h-subject-of-scientific-interest-nbsp">Subject of scientific interest&nbsp;</h2>



Messier 78 is fascinating not only for its visual beauty but also for its scientific interest, particularly in the study of <a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">star formation</a> and interstellar matter.&nbsp;



The nebula consists of dense, cold gas and dust, which are essential ingredients for the birth of new stars.&nbsp;



The intense blue light that characterizes M78 is due to the reflection of starlight off these dust particles - a process known as scattering.



<h2 class="wp-block-heading" id="h-region-surrounding-messier-78-nbsp">Region surrounding Messier 78&nbsp;</h2>



The region surrounding M78 includes several other interesting features. For instance, there are Herbig-Haro objects within it, which are small patches of nebulosity associated with <a href="https://www.earth.com/news/new-molecule-detected-in-space-where-stars-are-born/" target="_blank" rel="noreferrer noopener">newly born stars</a>.&nbsp;



These objects are formed when gas ejected by young stars collides with clouds of gas and dust at high speeds, creating shock waves that glow brightly.



<h2 class="wp-block-heading" id="h-earliest-stages-of-star-development-nbsp">Earliest stages of star development&nbsp;</h2>



Additionally, infrared observations of M78 have revealed much about the dust and colder objects in the area, which are not visible in optical light.&nbsp;



The observations have helped astronomers identify numerous young stars and brown dwarfs (objects that are too large to be planets and too small to be stars) within the nebula.&nbsp;



This makes M78 a critical area for studying the earliest stages of star development and the properties of the interstellar medium.



<h2 class="wp-block-heading" id="h-euclid-space-mission-nbsp">Euclid space mission&nbsp;</h2>



The <a href="https://www.earth.com/news/new-batch-of-brilliant-images-from-the-euclid-mission-live-up-to-the-hype/" target="_blank" rel="noreferrer noopener">Euclid space mission</a> is designed to study the dark universe, particularly focusing on dark energy and dark matter. These components are believed to drive the accelerating expansion of the universe and shape its large-scale structure. 



The mission aims to map the geometry of the dark universe and better understand the physics of the cosmos.



<h3 class="wp-block-heading" id="h-observing-billions-of-galaxies-nbsp">Observing billions of galaxies&nbsp;</h3>



Euclid uses two primary scientific instruments: a visible light camera (VIS) and a near-infrared spectrometer and photometer (NISP).&nbsp;



These instruments will allow Euclid to measure the shapes and redshifts of galaxies at distances of up to 10 billion light-years. By surveying more than a third of the sky, the mission is expected to observe several billion galaxies.



<h3 class="wp-block-heading" id="h-studying-the-dark-universe-nbsp">Studying the dark universe&nbsp;</h3>



The data collected will help astronomers in studying the effects of dark matter and dark energy in depth, testing cosmological models, and exploring new theories about the nature of the universe.&nbsp;



The mission, named after the ancient Greek mathematician Euclid, seeks to address key questions related to the structure of the universe and the fundamental laws of physics governing its evolution and expansion.



Image Credit: European Space Agency&nbsp;



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Messier 78: Young stars shine through dense dust

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

Today's Image of the Day from the European Space Agency showcases the striking beauty of the planetary nebula NGC 2899, which resembles a moth in flight. The photo was captured by the Hubble Space Telescope.



“The planetary nebula NGC 2899 is shaped like a single macaroni noodle, with its edges pointed up, but its edge-on central torus is semi-transparent in the middle,” noted <a href="https://www.esa.int/ESA_Multimedia/Images" target="_blank" rel="noreferrer noopener">ESA</a>.



“The top and bottom edges are thick and orange. The center is semi-transparent blue and green. The wider central region looks roughly like a moth, also filled with semi-transparent blue and green.”



<h2 class="wp-block-heading" id="h-defining-features-of-the-planetary-nebula">Defining features of the planetary nebula</h2>



The nebula features a bipolar, cylindrical outflow of gas extending diagonally, driven by intense radiation and stellar winds from a central <a href="https://www.earth.com/news/white-dwarf-planets-are-more-habitable-than-we-thought/" target="_blank" rel="noreferrer noopener">white dwarf</a> with a scorching temperature of nearly 22,000 degrees Celsius.&nbsp;



“In fact, there may be two companion stars that are interacting and sculpting the nebula, which is pinched in the middle by a fragmented ring or torus - looking like a half-eaten donut,” said ESA.



Streams of gaseous “pillars” extend outward, all pointing back toward the central source of energy. The vibrant colors in the image come from glowing hydrogen and oxygen gases.&nbsp;



<h2 class="wp-block-heading" id="h-discovery-and-significance-of-ngc-2899">Discovery and significance of NGC 2899</h2>



NGC 2899 was discovered by British astronomer John Herschel on March 2, 1835, during his survey of the southern skies from the Cape of Good Hope in South Africa. Herschel cataloged many deep-sky objects in the southern hemisphere, contributing significantly to the New General Catalogue (NGC) compiled later by John Louis Emil Dreyer.



NGC 2899 is located approximately 4,500 light-years from Earth in the southern constellation Vela, which is part of the larger Vela-Puppis-Carina region of the Milky Way known for its rich <a href="https://www.earth.com/news/fluffy-molecular-clouds-may-change-our-understanding-of-star-formation/" target="_blank" rel="noreferrer noopener">star-forming activity</a> and remnants of past stellar explosions.&nbsp;



Vela, whose name means "sails" in Latin, represents the sails of the ancient Greek mythological ship Argo Navis. This region of the sky is particularly abundant in nebulae, star clusters, and other deep-sky objects, making it a focal point for astronomical observations.&nbsp;



The nebula’s distance places it well within our galaxy, offering astronomers a valuable glimpse into the later stages of stellar evolution and the processes that sculpt and illuminate planetary nebulae.



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



Nebulae are vast clouds of gas and dust in space, often serving as the birthplaces or remnants of stars.&nbsp;



They come in various types, including emission nebulae that glow due to ionized gases energized by nearby stars, reflection nebulae that shine by scattering starlight, and dark nebulae that obscure light from background <a href="https://www.earth.com/news/runaway-star-may-be-dragging-a-planet-along-with-it/" target="_blank" rel="noreferrer noopener">stars</a>.&nbsp;



Planetary nebulae form when dying stars shed their outer layers, creating colorful, often symmetrical shapes. Nebulae can span light-years across and are key to understanding the life cycles of stars and the structure of galaxies.



<h2 class="wp-block-heading" id="h-the-fate-of-dying-stars">The fate of dying stars</h2>



Not all dying stars become planetary nebulae. In fact, stars much more massive than the Sun follow a very different and far more violent path.&nbsp;



These massive stars end their lives in dramatic supernova explosions, releasing tremendous energy and scattering heavy elements into space, which enriches the interstellar medium.&nbsp;



What remains after the explosion depends on the star’s mass. The collapsed core can form a neutron star - an incredibly dense object composed mostly of neutrons. Or, if the star was even more massive, it may create a <a href="https://www.earth.com/news/astronomers-confirm-lone-black-hole-wandering-through-our-galaxy/" target="_blank" rel="noreferrer noopener">black hole</a>, where gravity is so intense that not even light can escape.



<h2 class="wp-block-heading" id="h-examples-of-winged-nebulae-nbsp">Examples of “winged” nebulae&nbsp;</h2>



Several well-known nebulae are noted for their "winged" or symmetrical, wing-like appearances, often earning them evocative nicknames.&nbsp;



One of the most famous is the Butterfly Nebula, located in the constellation Scorpius. This planetary <a href="https://www.earth.com/news/dragons-egg-nebula-is-a-truly-stunning-sight-to-behold/" target="_blank" rel="noreferrer noopener">nebula</a> displays two expansive lobes that resemble butterfly wings, shaped by fast stellar winds from a dying star.



The Omega Nebula (also known as the Swan Nebula) in the constellation Sagittarius is a bright star-forming region that has been said to resemble a swan in flight. It has broad, glowing "wings" formed by clouds of ionized hydrogen gas. 



Similarly, the Eagle Nebula has an overall shape reminiscent of a bird with outstretched wings, which inspired its name. It is located in the constellation Serpens and home to the iconic "Pillars of Creation."



Image Credit: ESA



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Planetary nebula with ethereal wings captured by Hubble

Today's Image of the Day from the European Space Agency features the vibrant colors of the Mawrth Vallis region of Mars. The image reveals a landscape abundant in iron, magnesium, and aluminum.&nbsp;



Mawrth Vallis lies just south of the dichotomy boundary, a ridge marking the divide between Mars' southern highlands and northern lowlands. Layered, clay-rich deposits found in this valley indicate prolonged interactions with water. 



Mawrth Vallis is considered a prime candidate for studying past habitability and the potential for preserved biosignatures. The region continues to captivate scientists due to its geological complexity and history of <a href="https://www.earth.com/news/mars-has-a-water-reservoir-two-miles-deep-enough-to-fill-earths-red-sea/" target="_blank" rel="noreferrer noopener">liquid water</a> flow. 



<h2 class="wp-block-heading" id="h-the-colors-of-mars">The colors of Mars</h2>



<a href="https://www.earth.com/news/air-samples-from-mars-could-reveal-fascinating-secrets/" target="_blank" rel="noreferrer noopener">Mars</a> gets its distinctive red color from iron oxides, or rust, on its surface. The Martian soil and dust are rich in iron minerals, which oxidize when exposed to the small amounts of oxygen present in the Martian atmosphere.&nbsp;



This oxidation process gives the planet its reddish hue, similar to how iron objects on Earth develop rust. 



The scattering of sunlight by these iron oxide particles further enhances the reddish appearance when viewed from a distance. However, the human eye can only perceive a fraction of Mars' <a href="https://www.earth.com/news/mars-captured-in-true-color-like-youve-never-seen-the-red-planet-before/" target="_blank" rel="noreferrer noopener">true color</a> palette.&nbsp;



<h2 class="wp-block-heading" id="h-striking-colors-revealed">Striking colors revealed</h2>



The European Colour and Stereo Surface Imaging System (CaSSIS) aboard the ExoMars Trace Gas Orbiter (TGO) offers a more detailed view, showcasing a striking diversity of colors.&nbsp;



This CaSSIS <a href="https://www.esa.int/ESA_Multimedia/Images/2024/06/Metallic_Mars_landscape" target="_blank" rel="noreferrer noopener">image</a> reveals yellow layers rich in iron and magnesium clays, overlain by white and blue layers abundant in aluminum.&nbsp;



The area is draped by a dark, heavily eroded layer, illustrating a vibrant, metallic landscape formed around 3.6 billion years ago.



<h2 class="wp-block-heading" id="h-upcoming-rosalind-franklin-mission">Upcoming Rosalind Franklin mission</h2>



The Rosalind Franklin mission is a joint mission by the European Space Agency (ESA) and Roscosmos aimed at exploring the surface of Mars to search for signs of past or present life. 



The mission is named after Rosalind Franklin, the pioneering British scientist whose work was crucial in the discovery of DNA's structure.



The rover is designed to drill up to two meters below the Martian surface, where it is believed any signs of life may be better preserved, away from the harsh surface radiation. 



The Rosalind Franklin rover was originally scheduled to launch in 2020, but technical delays and the COVID-19 pandemic pushed the launch window to 2028. 



Once on Mars, the rover will collaborate with other missions like NASA's Perseverance and Curiosity rovers to advance our understanding of the Red Planet's habitability and history.



<h2 class="wp-block-heading" id="h-studying-mars-ancient-past">Studying Mars’ ancient past</h2>



While Rosalind Franklin prepares for its mission, the TGO remains in orbit, conducting crucial research to unravel Mars' ancient past and assess its potential <a href="https://www.earth.com/news/secrets-of-mars-seismic-discoveries-and-the-quest-for-past-life/" target="_blank" rel="noreferrer noopener">habitability</a>.&nbsp;



Since beginning its full science mission in 2018, TGO has not only captured stunning images but also provided a comprehensive inventory of Mars' atmospheric gases and mapped water-rich locations on the planet's surface.



For six years, CaSSIS has delivered breathtaking views of Mars in vivid color, documenting features ranging from volcanic landscapes to active dust devils and immense sand dunes.&nbsp;



Understanding Mars' water history and its implications for past <a href="https://www.earth.com/news/mars-is-letting-out-mysterious-methane-burps-but-why/" target="_blank" rel="noreferrer noopener">life</a> remains a core focus of ESA’s ExoMars missions.



<h2 class="wp-block-heading" id="h-metals-on-mars">Metals on Mars</h2>



Mars is rich in various metals that contribute to its geological and mineralogical diversity. 



While iron is the most prominent, magnesium is also abundant. It is often found in the form of clays, contributing to the planet's diverse mineral composition. 



Aluminum is another significant metal present on Mars, commonly found in layered deposits and sediments. 



<h2 class="wp-block-heading" id="h-major-changes-over-time">Major changes over time</h2>



The metals are not evenly distributed but are found in various concentrations across the Martian surface. 



For instance, regions like Mawrth Vallis exhibit a complex layering of different metal-rich minerals, including iron and magnesium-rich clays overlain by aluminium-rich layers.&nbsp;



This diversity indicates a rich geological history involving water activity, volcanic processes, and sedimentary deposition.



The presence of these metals suggests that Mars has undergone significant chemical and physical processes over billions of years, shaping its current landscape.&nbsp;



Understanding the distribution and composition of metals on Mars helps scientists piece together the planet's history and assess its past potential for habitability.



Image Credit: ESA/TGO/CaSSIS



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Metallic Mars: The diverse colors of the Red Planet

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA/Hubble &amp; NASA



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Violent clash of the Antennae Galaxies  

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Hubble spotlights galaxies in the constellation Virgo

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA



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Ghostly galaxy in the constellation Eridanus

Badlands National Park&nbsp;(Lakota:&nbsp;Makȟóšiča) is an American&nbsp;national park&nbsp;located in southwestern&nbsp;South Dakota. The park protects 242,756 acres (379.3&nbsp;sq&nbsp;mi; 982.4&nbsp;km2)&nbsp;of sharply&nbsp;eroded&nbsp;buttes&nbsp;and&nbsp;pinnacles, along with the largest undisturbed&nbsp;mixed grass prairie&nbsp;in the United States. The&nbsp;National Park Service&nbsp;manages the park, with the South Unit being co-managed with the&nbsp;Oglala Lakota&nbsp;tribe. The White River Badlands have developed an international reputation as a fossil-rich area. They contain the richest deposits of&nbsp;Oligocene&nbsp;mammals known, providing a glimpse of life in the area 33 million years ago.



For those interested in front-country camping, the park offers two official campgrounds. The&nbsp;Cedar Pass Campground&nbsp;is a paid campground with 96 sites total, some designated for RV camping with electric hookups. Sage Creek Campground&nbsp;is a free, first-come first-serve campground with 22 sites.&nbsp;Motor homes, pull behind trailers, and other recreational vehicles greater than 18 feet in length are prohibited.&nbsp; For those seeking a more rugged camping experience, back-country camping is also available in the park. Back-country camping is permitted anywhere in the park as long as it is 0.5 miles from a road or trail and is not visible from a trail or roadway.

Badlands National Park, South Dakota

Hydrogen is essential for fertilizer production and is increasingly promoted as a clean fuel for decarbonizing industry and shipping.



Yet almost all of today’s hydrogen - about 90 million metric tons a year - comes from reforming oil and gas, releasing roughly 2.4 percent of global CO2 emissions in the process. Blue and green hydrogen remain too expensive to scale rapidly, despite advances in carbon capture and clean electricity production.



A new review highlights a third option: tapping naturally occurring hydrogen produced by geological processes over millions of years. 



<h2 class="wp-block-heading" id="h-hunting-for-clean-hydrogen">Hunting for clean hydrogen</h2>



Researchers from the <a href="https://www.ox.ac.uk/">University of Oxford</a>, <a href="https://www.durham.ac.uk/">Durham University</a>, and the <a href="https://www.utoronto.ca/">University of Toronto</a> calculate that Earth’s continental <a href="https://www.earth.com/news/earths-first-crust-already-had-chemical-traits-of-modern-continents/">crust</a> has produced enough hydrogen over the past billion years to meet humanity’s projected needs for at least 170,000 years.



Microbes have consumed much of it, and some has leaked away, but the rest could still form recoverable accumulations. To find it, scientists say geologists must pursue hydrogen like helium or gas - though it diffuses and reacts more easily.



“We have successfully developed an exploration strategy for helium, and a similar ‘first principles’ approach can be taken for hydrogen,” said co-author Jon Gluyas, a professor at Durham University. 



The review outlines the critical elements of such a strategy and identifies where current knowledge is solid or still developing.



<h2 class="wp-block-heading" id="h-how-does-hydrogen-form">How does hydrogen form?</h2>



Hydrogen forms through several crustal reactions. One of the best known is serpentinization, where water reacts with iron-rich minerals underground, oxidizing iron and releasing molecular hydrogen. 



Other pathways include radiolysis - where decaying uranium splits water molecules - and organic shale maturation, which can generate hydrogen alongside hydrocarbons. 



Production rates vary widely by region, depending on temperature, pressure, rock type, and the availability of liquid water.



<h2 class="wp-block-heading" id="h-holding-hydrogen-underground">Holding hydrogen underground</h2>



After formation, hydrogen must migrate through fractures and porous rock layers until it meets a geological trap that prevents further escape.



Traditional seals like rock salt or claystone can work, but because hydrogen molecules are so small, maintaining containment over geological time may require exceptionally tight caps. Even a perfect seal is not enough if microbes lurk in the reservoir.



“We know, for example, that underground microbes readily feast on hydrogen," said co-author Barbara Sherwood Lollar of the University of Toronto. 



"Avoiding environments that bring them into contact with the hydrogen is important in preserving hydrogen in economic accumulations.” 



Sherwood noted that high temperatures, salty brines, or low nutrient levels can slow microbial consumption.



<h2 class="wp-block-heading" id="h-targeting-deposits-in-earth-s-crust">Targeting deposits in Earth's crust</h2>



The review challenges speculation that mantle-derived hydrogen, sometimes touted as limitless, could be a major target. Analyses of isotopic fingerprints and gas ratios show that most mature accumulations originate from crustal rocks, not from deep-Earth plumes.



The good news is that suitable crustal settings are common: ancient cratonic shields, younger rift basins, iron-rich volcanic belts, and faulted sedimentary basins all provide the right mix of source, pathways, and potential traps. 



Some systems are geologically young, forming hydrogen within the past few million years, while others date back hundreds of millions.



Scientists have found encouragement in real-world hints. A village water well in Bourakébougou, Mali, accidentally tapped a stream of 98 percent hydrogen in 2012. Similar incidents have been reported in Kansas, South Australia, and the Pyrenees.



Drilling for water, oil, or minerals has accidentally revealed many deposits - hinting that targeted exploration could find much more.



<h2 class="wp-block-heading" id="h-searching-for-accumulated-hydrogen">Searching for accumulated hydrogen</h2>



Turning theory into drill bits will require integrating geophysics, geochemistry, microbiology, and reservoir engineering.



Study lead author Chris Ballentine from the University of Oxford offered a culinary analogy. “Combining the ingredients to find accumulated hydrogen in any of these settings can be likened to cooking a soufflé - get any one of the ingredients, amounts, timing, or temperature wrong and you will be disappointed.”



“One successful exploration recipe that is repeatable will unlock a commercially competitive, low-carbon hydrogen source that would significantly contribute to the energy transition - we have the right experience to combine these ingredients and find that recipe.”



<h2 class="wp-block-heading" id="h-identifying-significant-hydrogen-fields">Identifying significant hydrogen fields</h2>



To pursue that recipe, the research team has launched <a href="https://www.snowfoxdiscovery.com/">Snowfox Discovery Ltd</a>., aiming to identify “societally significant” hydrogen fields.



Early priorities include mapping iron-rich rock belts intersected by deep <a href="https://www.earth.com/news/groundwater-plays-critical-role-ecosystem-health/">groundwater</a>, quantifying how fast different microbial communities devour hydrogen, and testing seal integrity for a highly diffusive gas.



Seismic imaging and magnetotelluric surveys could reveal subsurface alteration zones where hydrogen-generating reactions are ongoing. Meanwhile, isotopic tracers will help distinguish fresh hydrogen from ancient residues or from contamination by <a href="https://www.earth.com/news/rising-methane-emissions-threaten-earths-habitability/">methane</a>.



<h2 class="wp-block-heading" id="h-a-step-toward-greener-fuel">A step toward greener fuel</h2>



If abundant, natural hydrogen could bridge blue and green hydrogen as a low-carbon feedstock during infrastructure scale-up.



However, extraction must avoid repeating the environmental mistakes of fossil-fuel development. Regulators will need to set standards for monitoring leaks, safeguarding groundwater, and managing co-produced gases.



Even partial success would diversify the <a href="https://www.earth.com/news/clean-energy-biodiversity-wildlife-habitats-delicate-balancing-act/">clean energy</a> portfolio and relieve pressure on renewables to shoulder all hydrogen demand. 



With the window to limit global warming rapidly closing, exploring Earth’s hidden hydrogen could buy valuable time - and illuminate a new frontier where geology and the energy transition meet.



The study is published in the journal <a href="https://www.nature.com/articles/s43017-025-00670-1">Nature Reviews Earth &amp; Environment</a>.



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Clean hydrogen source could power Earth for 170,000 years

Hydrogen is essential for fertilizer production and is increasingly promoted...

Cancer is one of the many health risks linked to physical inactivity, and it has become a growing concern in today’s sedentary world.



Most of us know that we should move more. Yet, with modern life keeping us in chairs and behind screens, the cost of sitting too much is steep - about £7.4 billion a year in the U.K. alone. But beyond the financial toll, it’s our health that suffers most.



Now, fresh evidence suggests a simple habit could make a big difference: walking. New research from the <a href="https://www.ox.ac.uk/" target="_blank" rel="noreferrer noopener">University of Oxford</a> shows that taking more daily steps can lower your chances of developing certain cancers. 



The study followed over 85,000 U.K. adults and found a strong connection between <a href="https://www.earth.com/news/walking-can-drastically-improve-your-health-without-thousands-of-daily-steps/" target="_blank" rel="noreferrer noopener">walking</a> regularly and a reduced risk for 13 types of cancer.



<h2 class="wp-block-heading" id="h-understanding-the-step-cancer-connection">Understanding the step-cancer connection</h2>



Participants wore devices that tracked how much - and how intensely - they moved each day. On average, they were monitored for six years.



The researchers spotted a clear pattern: the more someone walked, the lower their cancer risk. This link held up no matter how fast or slowly those steps were taken.



In fact, the benefits started to appear around 5,000 steps per day. Below that, there wasn’t much effect. But once participants hit 7,000 steps, cancer risk dropped by 11%. At 9,000 steps, the risk fell by 16%. Beyond that, the advantage leveled off, with only small additional improvements.



These numbers back the common advice to walk <a href="https://www.earth.com/news/scientists-prove-how-many-daily-steps-you-should-take-to-avoid-early-death/" target="_blank" rel="noreferrer noopener">10,000 steps a day</a> - not just for heart health or fitness reasons, but as a way to lower cancer risk as well.



<h2 class="wp-block-heading" id="h-pace-doesn-t-matter-movement-does">Pace doesn’t matter; movement does</h2>



Researchers also looked at how fast people walked. While faster walking was initially linked to lower cancer risk, this difference disappeared when total movement was taken into account. It turns out that it’s the overall amount of activity that matters most - not how briskly you do it.



Swapping sitting time for either light or moderate activity reduced cancer risk. But trading light movement for more intense activity didn’t add extra benefits. The key message? Just move more, at any speed.



<h2 class="wp-block-heading" id="h-what-types-of-cancer-are-affected">What types of cancer are affected?</h2>



The experts looked at 13 cancers: esophageal, liver, lung, kidney, gastric, endometrial, myeloid leukemia, myeloma, colon, head and neck, rectal, bladder, and <a href="https://www.earth.com/news/plant-based-diet-improves-health-in-women-with-breast-cancer/" target="_blank" rel="noreferrer noopener">breast cancer</a>.



Over six years, about 3% of participants developed one of these cancers. For men, the most common were colon, rectal, and lung cancers. For women, breast, colon, endometrial, and lung cancers were most common.



Physical activity showed the strongest protection against six <a href="https://www.earth.com/news/obesity-is-linked-to-32-cancer-types-that-could-drive-40-of-cases/" target="_blank" rel="noreferrer noopener">cancer types</a>: gastric, bladder, liver, endometrial, lung, and head and neck cancers.



<h2 class="wp-block-heading" id="h-why-this-study-stands-out">Why this study stands out</h2>



Most earlier studies in this field have relied on people reporting their own activity levels. That method isn’t always reliable. People often forget or overestimate how much they move. This new study used wearable trackers, which gave a much clearer picture of actual daily movement.



It’s also different from research that focuses only on intense exercise. While hitting the gym can be helpful, not everyone is able or motivated to do that. The research suggests that even lighter movement, like walking, can reduce cancer risk.



<h2 class="wp-block-heading" id="h-small-changes-add-up">Small changes add up</h2>



You don’t have to walk miles at a time to see real health benefits. Just 4,000 steps a day - roughly equal to two miles (3.2 kilometers) or about 40 minutes of light walking - can help improve your long-term health.



The good news is that you don’t need to carve out a large chunk of time to make it happen. These steps can be spread throughout the day, making it easier to fit movement into your routine.



Consider small adjustments to your daily habits. Take the stairs instead of the lift whenever possible - it’s a simple way to get your heart rate up. During your lunch break, step outside for a short walk to clear your mind and add to your daily total. 



If you're often on phone calls, use that time to walk around instead of sitting still while you talk. Even parking a little farther away from your destination can give you those extra steps that make a difference.



Incorporating more movement into your day, especially during middle age, can be one of the easiest and most effective ways to reduce your risk of cancer over time. It doesn’t require a gym membership or special equipment - just a conscious decision to sit less and move more.



<h2 class="wp-block-heading" id="h-a-simple-way-to-lower-cancer-risk">A simple way to lower cancer risk</h2>



Of course, the connection between movement and cancer is complex. Scientists still have more to learn - especially about how different types of activity influence individual cancers over time.



But one thing is clear: sitting less and moving more really matters. You don’t have to run marathons. Just get up, take more steps, and you could be walking toward <a href="https://www.earth.com/news/intermittent-fasting-could-be-the-key-to-better-health/" target="_blank" rel="noreferrer noopener">better health</a> - one day at a time.



Details of the study are published in the <a style="font-style: italic;" href="https://bjsm.bmj.com/content/early/2025/03/14/bjsports-2024-109360">British Journal of Sports Medicine</a>.



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Walking each day at any speed lowers the risk of cancer

Cancer is one of the many health risks linked to...

Physicists have reached an unexpected breakthrough: they changed beams of light into a supersolid that flows without normal resistance. This marks a major milestone in condensed matter physics because it shows that light can adopt a structure resembling a <a href="https://www.nature.com/articles/d41586-025-00637-8">solid</a> while also moving around freely like a liquid.



“We actually made light into a solid. That’s pretty awesome,” said <a href="https://polaritonics.nanotec.cnr.it/people/dimitris-trypogeorgos/" target="_blank" rel="noreferrer noopener">Dimitrios Trypogeorgos</a> from Italy’s National Research Council (CNR). This is the first demonstration of this peculiar mix of solidity and fluidity using photons instead of atoms.



<h2 class="wp-block-heading" id="h-quantum-background">Quantum background</h2>



Most people see light as something that travels in waves, but in advanced research, it can also be treated as photons. These tiny bits of energy sometimes band together with matter to form quasiparticles that behave in ways not seen in everyday items.



<a href="https://www.nature.com/articles/141074a0" target="_blank" rel="noreferrer noopener">Quantum effects</a> often only show up when things are extremely cold, near minus 460oF (238oC). In those conditions, random motion slows to a crawl, and subtle interactions become easier to spot.



<h2 class="wp-block-heading" id="h-how-light-was-shaped">How light was shaped</h2>



The team used a semiconductor with specialized layers to control how photons interact with material. This setup allowed them to create a medium in which <a href="https://www.earth.com/news/new-quantum-device-uses-crystal-layers-to-generate-entangled-photons/">photons</a> combined with other particles to form a type of condensate that organized into a solid-like grid.



That structured grid didn’t stop these particles from flowing without friction, though. Previous supersolids were made from atomic gases, but using light and matter together is a new route to exploring these odd states.



<h2 class="wp-block-heading" id="h-insights-from-the-experiment">Insights from the experiment</h2>



Researchers found that the resulting formation showed properties of solids, yet it had <a href="https://knotphysics.net/superfluidity" target="_blank" rel="noreferrer noopener">zero viscosity</a>, which means it offered no internal friction. This dual identity made it a supersolid, and placed it in an unusual category of matter that many experts have wanted to study in detail.



“While the team has convincingly shown that they produced a supersolid, additional measurements and analyses are necessary to comprehend its properties fully,” said <a href="https://www.lkb.fr/quantumfluids/about-the-team/people/alberto-bramati/" target="_blank" rel="noreferrer noopener">Alberto Bramati</a> from Sorbonne University in France. He and others believe further tests might reveal even more surprises about the nature of quantum fluids.



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



When something lacks viscosity, it can flow in a nearly frictionless way. That suggests possibilities for applications that need smooth transport, such as superconductors, or for quantum computing systems that rely on minimal energy loss.



Scientists are intrigued by the chance to explore how a supersolid evolves under different conditions. These findings might help in designing new materials or devices that show stable performance while also harnessing quantum properties.



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



This experiment opens fresh avenues for studying <a href="https://www.earth.com/news/new-form-of-quantum-entanglement-discovered-will-transform-next-gen-technology/">quantum</a> particles that move as if they have no barriers. Researchers believe that having a supersolid based on light can simplify future work, since it may be easier to manipulate photons than to chill atoms to very low temperatures.



Experts are also hoping to watch how this supersolid responds to tweaks in temperature and external fields. Understanding those responses could drive progress in making specialized photonic systems that store and carry information with high efficiency.



<h2 class="wp-block-heading" id="h-practical-perspectives">Practical perspectives</h2>



Many quantum effects seem rarefied, yet the knowledge gained often leads to useful discoveries. Superfluids once looked like a curiosity, but they advanced cryogenics and found roles in sensors.



Supersolids made from light might do something similar, especially for systems that require precise control of energy. This achievement hints at a future where photonic supersolids serve as a platform for advanced devices.



<h2 class="wp-block-heading" id="h-possible-challenges">Possible challenges</h2>



Although the new setup shows promise, there could be technical hurdles. Maintaining the right conditions to keep <a href="https://www.earth.com/news/dark-photon-theory-casts-doubt-on-double-slit-experiment-quantum-light-interference-pattern/">photons</a> locked in a solid state might be tricky.



If scientists can stabilize these conditions over longer periods, they will be able to collect more detailed data. That could reveal how flexible the material is, or how it reacts when disturbed by external factors.



<h2 class="wp-block-heading" id="h-reaching-for-more-answers">Reaching for more answers</h2>



Trypogeorgos and his colleagues foresee plenty of questions to tackle. Are there new phases of matter waiting to emerge from similar setups?



Researchers might also look into mixing various types of particles with photons to craft specialized supersolids. Each twist could lead to new physics that changes our understanding of how matter and light behave.



<h2 class="wp-block-heading" id="h-a-wider-view">A wider view</h2>



Supersolidity is not just a scientific quirk. It brings attention to the ways quantum mechanics can reshape our view of nature by blending properties once thought to be totally separate.



Flowing like liquids yet forming solid grids, these newly created structures stand as an example of how <a href="https://www.earth.com/news/schrodingers-cat-put-into-silicon-chip-may-be-holy-grail-for-error-proof-quantum-computing/">quantum</a> rules can bend conventional wisdom. They showcase a unique overlap of order and freedom in a single material.



Physicists are still exploring what unexpected features might arise. Identifying potential uses for these odd states of light may take time, but the journey already looks rewarding.



The study is published in <a href="https://www.nature.com/articles/s41586-025-08616-9" target="_blank" rel="noreferrer noopener">Nature</a>.



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Physicists succeed in converting light into a supersolid that flows like a liquid

Physicists have reached an unexpected breakthrough: they changed beams of...

Imagine a world without apples, almonds, tomatoes, or coffee. It would not just be bland - it would be dangerously imbalanced. This isn’t fiction but a potential reality if pollinators like bees disappear. World Bee Day, observed on May 20, is a global call to remember, appreciate, and protect these essential creatures.



In 2025, under the theme&nbsp;"Bee inspired by nature to nourish us all,"&nbsp;the campaign goes beyond admiration. It urges action to support biodiversity, sustainable agriculture, and ecosystem resilience. 



Bees, alongside other <a href="https://www.earth.com/news/native-bee-species-face-extinction-due-to-honey-bee-competition/" target="_blank" rel="noreferrer noopener">pollinators</a>, not only fill our plates but also keep our planet’s life systems in balance. Their survival is tightly linked to our own.



<h2 class="wp-block-heading" id="h-pollinators-help-most-plants-grow">Pollinators help most plants grow</h2>



<a href="https://www.earth.com/news/bees-sleep-like-humans-with-similar-brain-patterns/" target="_blank" rel="noreferrer noopener">Bees</a> are important, but they’re not the only creatures that help plants grow. Butterflies, birds, bats, and even some animals like lemurs also move pollen from one flower to another. This process is called pollination. 



Without it, most plants can't make fruits or seeds. Together, all these pollinators help nearly 90 out of every 100 wild plants grow. They also help with growing more than three-quarters of the food crops we eat, like apples, almonds, onions, coffee, and avocados.



There are more than 20,000 kinds of bees in the world. Most of them live in the wild. We usually just take them for granted. But when they disappear, we feel the difference. 



Farmers lose money because crops don’t grow well. Food prices go up. The variety of fruits and vegetables drops. Our meals become less healthy.



<a href="https://www.earth.com/news/bee-survival-depends-on-more-than-just-pollen-abundance/" target="_blank" rel="noreferrer noopener">Pollinators</a> don’t just help plants grow. They make fruits bigger, tastier, and more colorful and work for free, every day, without anyone asking. But when nature is damaged, pollinators are usually the first to be affected. And when they vanish, we have a lot to lose.



<h2 class="wp-block-heading" id="h-world-bee-day-live-like-bees">World Bee Day: Live like bees</h2>



Bees live in a way that works well with <a href="https://www.earth.com/news/earth-day-2025-what-were-really-fighting-for/" target="_blank" rel="noreferrer noopener">nature</a>. They don’t destroy or waste anything. Instead, bees build hives, help flowers grow, and support many other plants and animals. Everything they do fits into the natural system. It’s smart, balanced, and helpful to the planet.



This year’s World Bee Day message means we should look at how bees live and learn from them. Bees work together, help each other and keep nature healthy without causing harm.



If we follow their example, we can grow food in better ways. We don’t need to clear forests or harm wild plants. We can farm without using harmful chemicals. Nature already knows the right way - bees are showing it to us. We just need to watch and do the same.



<h2 class="wp-block-heading" id="h-pollinators-are-in-trouble">Pollinators are in trouble</h2>



This isn’t just a story about bees dying. It’s about something much bigger. Nature is like a chain, and pollinators are one of its strong links. When that link breaks, the whole system starts to fall apart. Animals, plants, and people all feel the damage.



Pollinators like bees, butterflies, bats, and birds are disappearing much faster than they should - up to 1,000 times faster. Around 35 out of every 100 insect pollinators are in danger. For animals like birds and bats, 17 out of 100 are also at risk.



If this keeps happening, the way we eat will change. Fruits, nuts, seeds, and leafy vegetables may become rare. The bright, fresh foods we enjoy today might be replaced by plain, cheap ones like rice, wheat, and corn. That means less nutrition and more hunger.



Farmers will have a harder time growing crops. Prices in stores will go up. The poorest people, who already struggle, will suffer the most. No one wants that kind of future.



<h2 class="wp-block-heading" id="h-world-bee-day-and-pollinator-protection">World Bee Day and pollinator protection</h2>



In 2018, the United Nations officially started World Bee Day. They chose May 20 because it’s the birthday of Anton Janša. He lived in Slovenia in the 1700s and helped improve how people care for bees. He believed bees were special because they worked hard and didn’t need much in return.



Today, we still respect bees for the same reason. But respect is not enough anymore. Bees are in danger, and they need our help.



Yurdi Yasmi is the director of the Food and Agriculture Organization (FAO) Plant Production and Protection Division.



“This call is extended to all Member Nations, international and regional organizations, civil society, leaders of Indigenous Peoples, researchers, the private sector, everyone working in the sector and anyone with an interest in bees and other pollinators to get involved, share their experiences and show how important these pollinators are,” said Yasmi.



The <a href="https://www.fao.org/home/en" target="_blank" rel="noreferrer noopener">FAO</a> is not just spreading awareness. It’s also training beekeepers, supporting eco-friendly farms, and encouraging laws that protect pollinators. Their message is simple - if we protect pollinators, we protect our future too.



<h2 class="wp-block-heading" id="h-bee-projects-are-helping-people-and-nature">Bee projects are helping people and nature</h2>



In Samoa, bees do more than make honey. A project called “<a href="https://beeeducated.org" target="_blank" rel="noreferrer noopener">Bee Educated!</a>” trains women to care for hives. They learn, earn, and teach others. Bees bring money and confidence. They also bring balance to the land. It’s not just a project - it’s a movement.



In Yemen, beekeeping keeps going even through war. With support from the FAO and World Bank, farmers get better tools. They learn how to protect their bees and gather honey safely. Despite conflict and climate stress, the bees - and their keepers - persist.



These stories prove something important. When you help bees, you help people. You protect culture, jobs, and land. And you do it with nature, not against it.



<h2 class="wp-block-heading" id="h-participating-in-world-bee-day-2025">Participating in World Bee Day 2025</h2>



You don’t need to own a big farm to help bees and other pollinators. Small actions at home make a big difference. You can plant flowers that naturally grow in your area. These flowers give bees food. You can stop using harmful sprays in your garden. You can let wild bees build their nests safely.



Buying honey from nearby beekeepers also helps. So does telling your friends and family why bees matter. Even putting a shallow bowl of water with some stones outside gives bees a place to rest and drink.



Farmers can help too. They can grow many kinds of crops instead of just one. This gives pollinators more food. They can also reduce their use of pesticides and plant hedges and trees around fields to create safe spaces for bees.



Governments can support all these efforts. They can give money or rewards to farmers who protect pollinators. They can listen to Indigenous people, who have deep knowledge of nature and land. The more people who join in, the better it is for pollinators - and for us all.



<h2 class="wp-block-heading" id="h-we-can-still-protect-bees">We can still protect bees</h2>



Bees may be small, but their role in nature is huge. They help flowers, fruits, and vegetables grow by carrying pollen between plants. This links everything in the natural world - from the soil beneath our feet to the air we breathe.



Bees don’t just move pollen. They help life continue. They build hives from wax and turn flower nectar into honey which feeds people around the world.



Even though bees work quietly, their effect is powerful. Without them, many plants would stop growing. Our food system would weaken. Whole ecosystems would fall out of balance.



World Bee Day is not just a time to thank bees. It’s also a serious reminder. If we don’t act now, we could lose them. But it’s also a message of hope. We can still choose to protect bees and follow the example of nature.



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World Bee Day 2025: Protecting the pollinators that feed the world

Imagine a world without apples, almonds, tomatoes, or coffee. It...

Carbon credits have become a popular tool for offsetting the environmental impact of air travel. 



Every flight we take adds to the growing cloud of greenhouse gas emissions hovering over the planet. The aviation industry now emits more carbon dioxide than many individual nations. 



To soften the environmental blow, some airlines offer passengers the option to “offset” their emissions - usually by paying into forest protection schemes. 



The promise is simple: fund the preservation of trees, and they’ll absorb enough carbon to balance out your flight. But does it really work? A new study says not always.



<h2 class="wp-block-heading" id="h-concerns-about-carbon-credits">Concerns about carbon credits</h2>



Researchers from <a href="https://www.bu.edu/" target="_blank" rel="noreferrer noopener">Boston University</a> and the nonprofit Clean Air Task Force recently examined how forest carbon credit systems are run and regulated in North America. 



These programs are often part of the voluntary carbon market, where companies and individuals can buy credits to compensate for their emissions. But the study found that the protocols behind many of these credits are weak - and in some cases, entirely ineffective.



“There’s been a lot of appetite for these credits so corporations can meet their sustainability goals, but some of the credits that have been sold have been found to be dubious at best,” said Lucy Hutyra, a BU College of Arts &amp; Sciences Distinguished Professor, and chair of Earth and Environment.



“This paper is not about whether the system is broken, let’s just scrap it; it’s looking at what works well, what doesn’t, and how we can improve it.”



<h2 class="wp-block-heading" id="h-flaws-in-the-current-system">Flaws in the current system</h2>



<a href="https://www.earth.com/news/millions-of-carbon-credits-are-not-tied-to-forest-preservation-as-claimed/" target="_blank" rel="noreferrer noopener">Forest carbon credits</a> come in different forms. Some are part of mandatory systems; others are voluntary. At the cheaper end, they involve paying landowners to keep forests standing. 



On paper, each credit is a promise to absorb one ton of carbon dioxide somewhere to make up for one ton emitted elsewhere. But it’s not always that simple.



The researchers evaluated 20 forest carbon credit protocols and gave each one a score based on how effectively it guarantees climate benefits. Most didn’t score well. 



Only one protocol received a “satisfactory” rating - and it hasn’t even been used yet. None earned a “robust” rating or higher.



“Our results show that the protocols used to generate credits are a critical weak link in the forest carbon market system,” said BU alum Rebecca Sanders-DeMott, the Clean Air Task Force's director of ecosystem carbon science. 



“Without significant improvements, the integrity of the forest carbon market will remain at risk,” she stated.



<h2 class="wp-block-heading" id="h-essential-role-of-forests">Essential role of forests</h2>



Forests play an essential role in absorbing <a href="https://www.earth.com/news/atmospheric-co2-could-push-temperatures-much-higher-than-expected/" target="_blank" rel="noreferrer noopener">atmospheric carbon</a>. But depending on how a credit scheme is managed, the benefits may be overstated. 



One example is the use of “buffer zones,” which are extra preserved areas intended to act as insurance in case something happens to the main forest area, such as a wildfire or disease outbreak.



“In the current system, the buffer pool risks are very conservative, very low estimates of risk,” said Hutyra. “The <a href="https://www.earth.com/news/california-wildfire-season-is-longer-peaks-earlier/" target="_blank" rel="noreferrer noopener">wildfire</a> risk in one part of California could be really quite different than another part.”



They propose the establishment of larger buffer zones and detailed, location-specific risk maps to better reflect real-world threats.



<h2 class="wp-block-heading" id="h-carbon-credits-need-improvement">Carbon credits need improvement</h2>



In addition to managing risk better, the study highlights four other areas where the carbon market could improve. 



It lists 22 total recommendations - half are relatively simple to implement, like reassessing project risks every five years. The rest are more complex.



One major issue is something called “leakage.” If you protect one area of forest from development, but that simply pushes deforestation or construction to another location, you haven’t achieved a true reduction in emissions.



“The net effect is no actual change in the land <a href="https://www.earth.com/news/carbon-sinks-are-a-powerful-weapon-against-climate-change/" target="_blank" rel="noreferrer noopener">carbon sink</a>, in real emissions to the atmosphere,” Hutyra explained.



To fix this, they suggest national and global tracking of land use changes and stronger incentives to support truly climate-positive outcomes.



<h2 class="wp-block-heading" id="h-what-s-next-for-carbon-credits">What’s next for carbon credits </h2>



The research team is now focused on getting their recommendations into the hands of those who can make a difference. 



The Clean Air Task Force is preparing an easy-to-read version of the report, organizing webinars, and reaching out to groups who manage carbon credit protocols.



Even without strong federal interest in regulating these markets right now, the researchers are hopeful that their work will help steer voluntary efforts in a more effective direction.



“Global energy demand is rising and, while decarbonizing our energy systems is critical, it will take time - decades, in fact. Meanwhile, the impacts of climate change are already being felt and are accelerating. Forests, which have long served as vital <a href="https://www.earth.com/news/mixed-forests-with-many-tree-species-are-more-effective-at-carbon-storage/">carbon sinks</a>, are under increasing threat," said Sanders-DeMott.



"By taking these recommendations seriously, carbon market actors can help restore confidence in carbon markets and unlock the full potential of forests to mitigate the worst effects of climate change, buying us time as we scale the technologies we need to ensure a high-energy, zero-emissions future.”



The full study was published in the journal <a href="https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2024EF005414" target="_blank" rel="noreferrer noopener">Earth's Future</a>.



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Forest carbon credits are failing, so what needs to change?

Carbon credits have become a popular tool for offsetting the...

European honey bees, celebrated for their industrious nature, may be pushing Australia’s native bees to the brink. 



Research from <a href="https://www.curtin.edu.au" target="_blank" rel="noreferrer noopener">Curtin University</a> reveals how these introduced bees could be reducing the reproductive success of native cavity-nesting <a href="https://www.earth.com/news/bees-sleep-like-humans-with-similar-brain-patterns/" target="_blank" rel="noreferrer noopener">bees</a>. 



The findings hint at a deeper problem - one that could disrupt ecosystems and challenge biodiversity in ways that few expect.



<h2 class="wp-block-heading" id="h-native-bee-reproductive-struggles">Native bee reproductive struggles</h2>



Dr. Kit Prendergast, a researcher at Curtin’s School of Molecular and Life Sciences, didn't just set up bee hotels to provide shelter. She turned them into research stations. 



“Bee hotels are more than just a way to give <a href="https://www.earth.com/news/bee-survival-depends-on-more-than-just-pollen-abundance/" target="_blank" rel="noreferrer noopener">bees</a> a place to nest - they’re powerful research tools that let us measure how well native bees are surviving and reproducing in different environments,” Dr. Prendergast said.



For two spring-to-summer seasons, Dr. Prendergast and her team studied 1000 native bee nests in 14 urban bushland and garden sites. 



The findings? In areas swarming with honey <a href="https://www.earth.com/news/artificial-diet-offers-hope-for-saving-endangered-honey-bees/" target="_blank" rel="noreferrer noopener">bees</a>, native bees faced trouble. They produced fewer female offspring. Their offspring had higher mortality rates. And the males that survived were noticeably smaller.



<h2 class="wp-block-heading" id="h-honey-bees-outcompete-native-bees">Honey bees outcompete native bees </h2>



Honey <a href="https://www.earth.com/news/science-is-giving-beekeepers-a-better-way-to-fight-colony-collapse/" target="_blank" rel="noreferrer noopener">bees</a> collected pollen from many types of plants, including both local and non-native ones. Native bees, however, focused on a smaller number of specific plants. 



This difference in foraging behavior made it harder for native bees to find enough food, as honey bees took pollen from a wider range of sources.



During the first year, honey bees collected pollen from 10.3 different species on average, while native bees gathered from just 4.3. In the second year, honey bees still maintained their wide range, collecting from 8.1 species. Native bees, however, only managed 2.8.



That’s a lot of overlap. Too much. In areas with high pollen overlap, native bees provisioned fewer cells for their offspring. Less food meant fewer babies. And fewer babies meant a population under pressure.



<h2 class="wp-block-heading" id="h-urban-gardens-intensify-pollen-competition">Urban gardens intensify pollen competition</h2>



Gardens may look like paradises for <a href="https://www.earth.com/news/bees-wearing-tiny-qr-codes-reveal-foraging-secrets/" target="_blank" rel="noreferrer noopener">bees</a>, but they can also be battlegrounds. 



Honey bees, with their broad pollen preferences, took full advantage of exotic plants. They outcompeted native bees in residential gardens, where floral diversity was often lower and more fragmented.



Dr. Prendergast pointed out that in these urban gardens, the impact of honey bee densities became more pronounced. Parasitism rates among native bees increased, suggesting that honey bee competition might make them more vulnerable to parasites.



<h2 class="wp-block-heading" id="h-honey-bees-affect-native-bee-sex-ratios">Honey bees affect native bee sex ratios</h2>



Honey bees didn’t just take pollen. They also affected the sex ratio of native bees. Female bees need more resources to develop, and when those resources get scarce, fewer females emerge.



“In some conditions, greater overlap in pollen use was associated with lower offspring numbers in native bees,” Dr. Prendergast noted. 



And the offspring that did emerge? More males than females. This male-biased sex ratio could destabilize native bee populations over time, making it harder for them to recover.



<h2 class="wp-block-heading" id="h-competition-reduces-reproduction">Competition reduces reproduction</h2>



Pollen is essential for bees. They collect it, eat it, and use it to feed their young. The study found that honey bees gathered pollen from more plant types than native bees.



In the first year, honey bees collected pollen from 58 plant species, but native bees only collected from 41. The next year, honey bees still foraged from 41 species, while native bees dropped to 24.



This difference matters. When honey bees take pollen from many plants, they leave less for native bees. 



With less pollen available, native bees have less food to feed their young. This leads to fewer offspring, smaller young, and fewer females, which can weaken native bee populations over time.



<h2 class="wp-block-heading" id="h-the-urban-vs-bushland-divide">The urban vs. bushland divide</h2>



Urban gardens didn’t just have more honey bees. They had more floral competition and higher parasitism rates. 



Native bees in bushland remnants fared slightly better, surrounded by more native flora and fewer honey bees. But even in these relatively protected areas, the pressure was still on.



The competition in gardens was particularly intense, with honey bees exploiting exotic plants that native bees couldn’t use as effectively. As a result, native bees had to work harder, forage longer, and ultimately, face greater risks from parasites.



<h2 class="wp-block-heading" id="h-honey-bees-increase-native-bee-mortality">Honey bees increase native bee mortality </h2>



Mortality rates for native bee offspring spiked in the first year of the study. Urban gardens with high honey bee densities saw the most significant increases. Fewer provisioned cells. More dead larvae. And for the males that did survive? They were smaller than usual.



“This shows that honey bees are not as benign as some might think - they can negatively impact local ecosystems and potentially contribute to declines in native bee populations,” Dr. Prendergast explained. 



And those smaller males? They’re less likely to find mates, further straining the population.



<h2 class="wp-block-heading" id="h-honey-bees-collect-more-pollen">Honey bees collect more pollen</h2>



Pollen analysis revealed a stark picture. Honey bees collected over twice as many pollen species as native bees. They didn’t just stick to native plants - they also targeted exotics, increasing the overlap and making it harder for native bees to find enough food.



The most common pollen species for honey bees included Eucalyptus marginata, Corymbia calophylla, and Melaleuca sp. For native bees, it was the same lineup. 



This shared preference intensified the competition, with honey bees taking more than their share, leaving native bees with less.



<h2 class="wp-block-heading" id="h-strategies-to-protect-native-bees">Strategies to protect native bees</h2>



What can be done to protect native bees? Dr. Prendergast suggests increasing native plant diversity in urban areas. By planting more species that native bees prefer - and that honey bees don’t - we can reduce competition.



Managing honey bee populations in urban gardens could also help. Fewer managed hives, fewer feral colonies. But it’s not that simple. Honey bees are valuable pollinators, and their removal isn’t always practical.



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



Dr. Prendergast’s work is just the beginning. The study, funded by the City of Stirling, the <a href="https://www.aws.org.au/" target="_blank" rel="noreferrer noopener">Australian Wildlife Society</a>, Hesperia, and the <a class="" href="https://www.forrestresearch.org.au/">Forrest Research Foundation</a>, points to a need for more targeted research.



Future studies could focus on long-term monitoring, examining how native bee populations fare over several years in areas with varying honey bee densities.



Understanding how pollen overlap affects native bee fitness in different habitats could also provide clues for more effective conservation strategies. Because in this hidden battle, the stakes are high. 



For native bees, survival may depend on more than just flowers - it may depend on the flowers they can still call their own.



The study is published in the journal <a href="https://www.frontiersin.org/journals/bee-science/articles/10.3389/frbee.2025.1508958/full" target="_blank" rel="noreferrer noopener">Frontiers in Bee Science</a>.



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Native bee species face extinction due to honey bee competition

European honey bees, celebrated for their industrious nature, may be...

Nature’s seasonal cycle offers countless marvels, and the shape and descent of leaves are among them. The way <a href="https://www.earth.com/news/scientists-finally-learn-what-makes-plants-roots-grow-faster-and-stronger-autophagy/" target="_blank" rel="noreferrer noopener">leaves</a> flutter down might appear random, but new findings suggest a more structured pattern than previously thought.



Matthew Dominic Biviano and Kaare Hartvig Jensen from the <a href="https://www.dtu.dk/english/" target="_blank" rel="noreferrer noopener">Technical University of Denmark</a> set out to investigate whether leaf geometry somehow reduces the loss of valuable nutrients.



After examining this process in detail, the team discovered that shape plays a noticeable role. 



<h2 class="wp-block-heading" id="h-how-falling-leaves-deliver-nutrients">How falling leaves deliver nutrients</h2>



Leaves come in an impressive range of sizes and outlines. Some have smooth edges, others have deep lobes, but all serve as living solar panels through <a href="https://education.nationalgeographic.org/resource/photosynthesis/" target="_blank" rel="noreferrer noopener">photosynthesis</a>, which is the process by which plants use sunlight to convert water and carbon dioxide into sugars that fuel growth.



Beyond gathering sunlight, <a href="https://www.earth.com/news/how-trees-decide-between-growing-and-breathing/" target="_blank" rel="noreferrer noopener">leaves</a> also supply valuable carbon when they fall. <a href="https://www.nature.com/articles/s41467-021-27373-7" target="_blank" rel="noreferrer noopener">Studies</a> suggest that about 40% of a tree’s captured carbon is stored in leaves before they drop.



A leaf that falls straight down likely lands closer to the tree that produced it. This matters because decaying leaf litter sends carbon and minerals into the soil, which can then feed the parent plant and its surrounding community.



If a leaf drifts too far, however, that resource might not be returned to the same tree. Trees can end up missing out on a chunk of the nutrients they originally invested in <a href="https://www.earth.com/news/mountain-wetlands-are-turning-into-mercury-hotspots/" target="_blank" rel="noreferrer noopener">leaf</a> growth.



<h2 class="wp-block-heading" id="h-leaf-shape-and-descent-speed">Leaf shape and descent speed</h2>



The two physicists designed an apparatus to release 100 artificial <a href="https://www.earth.com/news/scientists-finally-understand-why-rose-petals-have-pointed-tips/" target="_blank" rel="noreferrer noopener">leaves</a> inside a tank of water. This slower water environment allowed them to observe how shape and symmetry affect sinking behavior without the rapid variables of air currents.



Through repeated trials, the team found patterns in how leaves fell. Some shapes plummeted down briskly, while others seemed to twist or spin, adding extra distance in their underwater journey.



Data from this experiment indicated that symmetrical forms dropped more swiftly. Leaves with simpler outlines moved less erratically, suggesting that these shapes limit how far they can drift.



Asymmetrical or heavily lobed leaves, on the other hand, displayed a slower descent. Their uneven outlines created more swirling movement in the water, a motion that may also occur in air and increase the travel distance.



<h2 class="wp-block-heading" id="h-leaf-shapes-and-nutrient-recycling">Leaf shapes and nutrient recycling</h2>



One interpretation of these findings is that certain trees evolved leaf shapes that descend faster, leading to less wandering. That means most nutrients stay within easy reach of the parent tree’s roots.



In contrast, leaves with dramatic lobes or irregular shapes might inadvertently end up far away. This could hold advantages in other contexts, but it may offer fewer benefits for reusing nutrients.



Scientists have long pondered the variety of leaf designs in nature. Many are symmetrical in a left-right sense, which might be due to simple genetic or developmental rules.



This study suggests a functional angle as well. A faster drop rate might be one reason so many trees produce leaves with balanced shapes and fewer pronounced lobes.



<h2 class="wp-block-heading" id="h-leaf-shape-affects-nutrient-spread">Leaf shape affects nutrient spread</h2>



Every leaf is a balancing act of multiple needs. Photosynthesis efficiency, water collection, temperature control, and aerodynamic or <a href="https://ugc.berkeley.edu/background-content/sedimentation/" target="_blank" rel="noreferrer noopener">sedimentation</a> behavior can all influence how leaves end up looking.



A species might sacrifice faster drop rates if a particular shape offers a better solution for life in its habitat. What works best in one environment may not work in another.



The distance leaves travel also shapes ecological interactions. Fallen leaves add vital nutrients for fungi, microbes, and insects in the soil, which support overall forest health.



If those resources end up scattered, they can still help neighboring plants, but the original tree may gain fewer rewards for its investment. The new insights from the water-tank trials could prompt deeper studies into how leaf forms differ across various climates.



<h2 class="wp-block-heading" id="h-how-falling-leaves-affect-forest-health">How falling leaves affect forest health</h2>



Some researchers aim to probe more tree types, possibly working in wind tunnels or actual forest settings. Others might apply these principles to other plant organs that detach and disperse.



By uncovering the role of leaf shape, scientists add a new twist to our understanding of forest cycles. The research highlights how small changes can ripple through the life of an ecosystem.



Walking through a forest, people often notice an abundance of fallen leaves close to the trunk. These findings add context to that sight, suggesting a quiet biological strategy at play.



When leaves don’t stray far, the tree’s nutrients remain close, fueling new growth in the seasons ahead. This hidden process may help ensure forests remain robust and self-sustaining.



<h2 class="wp-block-heading" id="h-observing-fallen-leaves-in-nature">Observing fallen leaves in nature</h2>



Not every tree follows the same patterns. Tropical species with huge leaves might face different conditions, while ornamental breeds in gardens could show unique traits.



Curious observers might find it interesting to look at fallen leaves and ponder their shape and destination on the ground. Sometimes, that simple act of watching can reveal how nature finds ways to keep cycles intact.



The research from Denmark connects a leaf’s geometry with its journey back to the soil beneath its parent tree. This link highlights nature’s subtle interdependencies and the practical ways that form relates to function.



The study is published in the <a href="https://royalsocietypublishing.org/doi/10.1098/rsif.2024.0654" target="_blank" rel="noreferrer noopener">Journal of The Royal Society Interface</a>.



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Leaf shape is a tree's secret weapon to reclaim nutrients

Nature’s seasonal cycle offers countless marvels, and the shape and...

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



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



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



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



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



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



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



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



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



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



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

Is chocolate the next nutritional powerhouse?

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

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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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

Flu viruses are more flexible than expected

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



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



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



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



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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

Detecting mercury contamination with the tap of a finger

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



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



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



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



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



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



Video/ Image Credit: European Space Agency&nbsp;



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



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

Kainji Lake in north central Nigeria

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Assateague Island is a 37-mile (60 km) long barrier island located off the eastern coast of the Delmarva Peninsula facing the Atlantic Ocean. The northern two-thirds of the island is in Maryland while the southern third is in Virginia. The <a href="https://www.earth.com/image/assateague-island-national-seashore-maryland-2/">Maryland</a> section contains the majority of Assateague Island National Seashore and Assateague State Park. The Virginia section contains Chincoteague National Wildlife Refuge and a one-mile stretch of land containing the lifeguarded recreational beach and interpretive facilities managed by the National Park Service (or NPS). It is best known for its herds of feral horses, pristine beaches and the Assateague Lighthouse. The island also contains numerous marshes, bays, and coves, including Toms Cove.



Camping is available only in the Maryland district of Assateague Island. Reservations are required from March 15 through November 15. Campsite reservations are available six months in advance.&nbsp; Oceanside Drive-in:&nbsp;Tents, trailers and recreational vehicles (no hookups). Sites have a picnic table and a fire ring.&nbsp;Oceanside Walk-in:&nbsp;Tent-only sites, located 100-200 feet from centralized parking areas. Sites have a picnic table and a fire ring. Walk-in sites are closed from November 16 through March 14. Bayside Drive-in:&nbsp;Tents, trailers and recreational vehicles (no hookups). Sites have a picnic table and a fire ring. A Drive-In "Generator-Free Zone" is located in Bayside B Loop. Horse Camp:&nbsp;There are 2 campsites for horse camping available October 16 through April 14. Each site accommodates up to 6 people and 6 horses.&nbsp;Assateague has two oceanside and four bayside camping areas in Maryland for visitors who wish to backpack or paddle the island.

Badlands National Park, South Dakota

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