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



By studying regions like NGC 604, astronomers can gain insights into the complex interactions between stars and the interstellar medium, as well as the conditions that lead to the birth of stars. This, in turn, helps in understanding the evolution of <a href="https://www.earth.com/news/galaxies-like-our-own-milky-way-are-not-unique/" target="_blank" rel="noreferrer noopener">galaxies</a> and the universe as a whole.



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



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



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



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



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



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



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



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



Within NGC 604, there are hundreds of young, hot, massive <a href="https://www.earth.com/news/stars-at-the-edge-of-our-milky-way-galaxy-travel-more-slowly/" target="_blank" rel="noreferrer noopener">stars</a>. These stars have ionized the surrounding gas, causing it to glow and creating the nebula. The region is a prime example of a starburst phenomenon, where stars form at a much higher rate than in typical galactic conditions.



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Young, massive stars in the Triangulum Galaxy

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

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA



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Ghostly galaxy in the constellation Eridanus

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA/ESA Hubble Space Telescope



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Secrets of a spiraling galactic powerhouse

Today's Image of the Day from the European Space Agency features a brilliant stellar nursery located about 163,000 light-years away.



According to ESA, the image is one of the most photogenic examples of the many stellar nurseries observed by the NASA/ESA Hubble Space Telescope during its 30-year lifetime. 



“The portrait features the giant nebula NGC 2014 and its neighbor NGC 2020 which together form part of a vast star-forming region in the Large Magellanic Cloud, a satellite galaxy of the Milky Way,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



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



Stellar nurseries are regions in space where new stars are <a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">born</a> - often within vast clouds of gas and dust called molecular clouds.&nbsp;



These areas are fascinating because they are cradles of stellar evolution, where gravity causes clumps of gas to collapse, eventually forming protostars.&nbsp;



Over time, the protostars will heat up and start the nuclear fusion process that powers a star.



One of the most well-known stellar nurseries is the Orion Nebula, which is visible to the naked eye and located about 1,350 light-years from Earth.&nbsp;



<h2 class="wp-block-heading" id="h-dynamic-nature-of-a-stellar-nursery-nbsp">Dynamic nature of a stellar nursery&nbsp;</h2>



Within these nurseries, the balance between gravity and pressure determines the types of stars that form, from massive, luminous stars to smaller, cooler ones like our Sun.&nbsp;



The environment is incredibly dynamic, with powerful winds from young stars shaping the clouds and triggering the birth of even more stars.



These regions are often illuminated by the light from massive newborn stars - creating stunning, colorful displays. The light reveals the intricate structure of the dust and gas, sculpted by the energy of young stars.&nbsp;



<h2 class="wp-block-heading" id="h-significance-of-stellar-nurseries-nbsp">Significance of stellar nurseries&nbsp;</h2>



Stellar nurseries are essential for understanding the early stages of planetary formation, as protoplanetary disks (the material from which <a href="https://www.earth.com/news/planet-formation-new-insights-mechanics-physics/" target="_blank" rel="noreferrer noopener">planets form</a>) are often found around young stars in these regions.



Stellar nurseries play a crucial role in the ongoing evolution of <a href="https://www.earth.com/news/black-hole-is-starving-its-host-galaxy-of-star-forming-fuel/" target="_blank" rel="noreferrer noopener">galaxies</a>. They are responsible for the continuous birth of new stars that enrich the interstellar medium with heavier elements. This constant recycling of material is key to the development of future generations of stars and planets.&nbsp;



Furthermore, the study of these regions helps astronomers understand the fundamental processes that govern the life cycles of stars and the overall dynamics of the universe.



<h2 class="wp-block-heading" id="h-the-local-group">The Local Group</h2>



The Local Group is a collection of over 80 galaxies that includes the Milky Way, the Andromeda Galaxy, and the Triangulum Galaxy, along with numerous smaller dwarf galaxies. These galaxies are bound together by gravity and span a region roughly 10 million light-years across.&nbsp;



The <a href="https://www.earth.com/news/milky-ways-thin-disk-is-billions-of-years-older-than-we-thought/" target="_blank" rel="noreferrer noopener">Milky Way</a> and Andromeda are the dominant members, with their respective satellite galaxies orbiting them.&nbsp;



The Local Group is part of a larger structure known as the Virgo Supercluster, and its galaxies are moving toward the gravitational center of the Local Group, contributing to its dynamic nature.&nbsp;



<h2 class="wp-block-heading" id="h-large-magellanic-cloud">Large Magellanic Cloud</h2>



The Large Magellanic Cloud (LMC) is the fourth largest galaxy in the Local Group and can be seen with the naked eye from the Southern Hemisphere.&nbsp;



This irregular dwarf galaxy is home to the Tarantula Nebula, one of the most active star-forming regions in our cosmic neighborhood.&nbsp;



The Large Magellanic Cloud played a key role in astronomical history, particularly when the supernova SN 1987A was observed, providing valuable insights into stellar evolution.&nbsp;



The LMC's interaction with the Milky Way, along with its own companion, the Small Magellanic Cloud, is believed to influence its shape and star formation activity. Its proximity and unique properties make it a crucial object of study for understanding <a href="https://www.earth.com/news/massive-galactic-explosion-provides-clues-about-galaxy-evolution/" target="_blank" rel="noreferrer noopener">galaxy evolution</a>, star formation, and the dynamics of interacting galaxies.



Image Credit: NASA, ESA, and STScI



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Hubble captures a stunning stellar nursery

Today's Image of the Day from the European Space Agency features the Little Dumbbell Nebula, also known as Messier 76. The nebula is located in the constellation Perseus 3,400 light-years away from Earth.



Astronomers captured this image of the Little Dumbbell Nebula to commemorate the 34th anniversary of the Hubble Space Telescope, a joint venture between NASA and the European Space Agency (<a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>).



The snapshot provides not only a breathtaking view, but also deep insights into the life cycle of <a href="https://www.earth.com/news/dark-stars-scientists-discover-a-new-type-of-star-powered-by-dark-matter/" target="_blank" rel="noreferrer noopener">stars</a> and the dynamic processes within nebulae.



<h2 class="wp-block-heading" id="h-understanding-messier-76">Understanding Messier 76</h2>



Messier 76 is categorized as a planetary nebula - a term which refers to its round, planet-like appearance when viewed through early, low-power telescopes. 



However, the term is somewhat misleading as planetary nebulae have no connection to actual <a href="https://www.earth.com/news/nasa-finds-17-exoplanets-that-have-oceans-and-possibly-alien-life/" target="_blank" rel="noreferrer noopener">planets</a>.&nbsp;



Instead, they represent an expansive shell of luminous gases expelled by a dying red giant star, which subsequently collapses into a dense, hot white dwarf. 



This transformation marks the late stages of stellar evolution for medium to low-mass stars.



<h2 class="wp-block-heading" id="h-structure-of-messier-76">Structure of Messier 76</h2>



The structure of Messier 76 is particularly notable. It includes a central ring, giving the appearance of a bar-like feature, with two distinct lobes emanating from either side. 



This formation is believed to be the result of materials ejected by the star during its red giant phase, possibly sculpted by interactions with a companion star.&nbsp;



Although this binary companion is not visible in current Hubble images, its presence is inferred from the thick disk of dust and gas aligned with its orbital plane. 



The phenomenon of the companion star potentially being absorbed by the primary star, a process akin to stellar cannibalism, is a captivating aspect of the nebula's history.



<h2 class="wp-block-heading" id="h-the-dynamic-environment-of-the-nebula">The dynamic environment of the nebula</h2>



At the core of the nebula, the primary star, now collapsing into a <a href="https://www.earth.com/news/white-dwarf-stars-may-be-billions-of-years-older-than-estimated/" target="_blank" rel="noreferrer noopener">white dwarf</a>, reaches extreme temperatures. This heat is estimated to be 120,000 degrees Celsius - about 24 times hotter than the surface of our Sun.&nbsp;



This intensely hot remnant is visible as a small, bright point at the center of the nebula. Directly below this, another star can be seen; however, it is merely aligned with the nebula by chance and is not a part of it.



<h2 class="wp-block-heading" id="h-powerful-glow-of-messier-76">Powerful glow of Messier 76</h2>



The dynamics within Messier 76 are driven by powerful forces. The central disk seems to constrict the material, creating two lobes of gas escaping along the rotational axis of the star, perpendicular to the disk.&nbsp;



The lobes are propelled outward by a potent stellar wind, moving at a staggering two million miles per hour. This rapid movement is sufficient to travel the distance from Earth to the <a href="https://www.earth.com/news/timeless-mystery-solved-scientists-uncover-what-is-inside-the-moons-core/" target="_blank" rel="noreferrer noopener">Moon</a> in just over seven minutes.&nbsp;



The collision of the fast-moving gas with older, slower-moving material ejected during the star’s red giant phase results in the stunning glowing effect seen in the nebula. 



The glow, ignited by the ultraviolet radiation from the white dwarf, is a spectacle of colors with red emanating from nitrogen and blue from oxygen.



<h2 class="wp-block-heading" id="h-a-cosmic-moment-in-time">A cosmic moment in time</h2>



Despite its current brilliance, the existence of the Little Dumbbell Nebula is fleeting on a cosmological scale. It is expected to last only about 15,000 years - a mere moment in the lifespan of the <a href="https://www.earth.com/news/dark-energy-is-ripping-the-universe-apart-but-we-arent-sure-how/" target="_blank" rel="noreferrer noopener">universe</a>.&nbsp;



This brief period highlights the transient nature of such cosmic phenomena, which, while short-lived, provide crucial insights into the mechanics of stellar evolution and the complex interactions within these celestial sculptures.



<h2 class="wp-block-heading" id="h-more-about-messier-76">More about Messier 76</h2>



Messier 76 was discovered by Pierre Méchain in 1780. It was later cataloged by Charles Messier, who included it in his famous list of nebulous objects.



The nebula's faintness and small size require a good telescope to be observed effectively, with larger telescopes able to reveal more of its fine details and structure.



Studying Messier 76 helps astronomers understand the life cycle of stars and the processes that occur during the late stages of stellar evolution. 



The materials expelled by planetary nebulae like Messier 76 eventually contribute to the interstellar medium, from which new stars and planetary systems may form.



Image Credit: ESA Space Agency&nbsp;



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Secrets of the Little Dumbbell Nebula  

Today's Image of the Day from the European Space Agency (ESA) features the distant galaxy LEDA 22057, which is located about 650 million light-years away in the constellation Gemini. 



Within the galaxy lies a pale blue dot - SN 2024PI, a supernova explosion that was discovered by an automated survey in January 2024.



“The survey covers the entire northern half of the night sky every two days and has cataloged more than 10,000 supernovae,” noted <a href="https://www.esa.int/ESA_Multimedia/Images/2025/01/Pale_blue_supernova_dot" target="_blank" rel="noreferrer noopener">ESA</a>.



“The supernova is visible in this image: located just down and to the right of the galactic nucleus, the pale blue dot of SN 2024PI stands out against the galaxy’s ghostly spiral arms.”



<h2 class="wp-block-heading" id="h-remnants-of-a-supernova">Remnants of a supernova </h2>



ESA noted that the image was taken about a month and a half after the supernova was discovered, so it appears many times fainter than its <a href="https://www.earth.com/news/shockingly-bright-carbon-monoxide-detected-in-supernova-remnant/" target="_blank" rel="noreferrer noopener">maximum brilliance</a>.



“SN 2024PI is classified as a Type Ia supernova. This type of supernova requires a remarkable object called a white dwarf, the crystallized core of a star with a mass less than about eight times the mass of the Sun,” explained ESA.



“When a star of this size uses up the supply of hydrogen in its core, it balloons into a red giant, becoming cool, puffy and luminous. Over time, pulsations and stellar winds cause the star to shed its outer layers, leaving behind a white dwarf and a colorful planetary nebula.”&nbsp;



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



Most stars in the <a href="https://www.earth.com/news/stars-at-the-edge-of-our-milky-way-galaxy-travel-more-slowly/" target="_blank" rel="noreferrer noopener">Milky Way</a> will eventually transition to white dwarfs after their death. Whether or not a star becomes a white dwarf depends on its mass.&nbsp;



Stars that are significantly more massive will end their lives differently. Stars that exceed the critical mass threshold of eight times the Sun undergo more violent deaths.&nbsp;



After exhausting their nuclear fuel, they collapse under their immense gravity and trigger a supernova explosion. Depending on the remaining core mass, they may leave behind either a neutron star or a black hole, rather than a <a href="https://www.earth.com/news/hungry-white-dwarf-stars-eat-heavy-metals/" target="_blank" rel="noreferrer noopener">white dwarf</a>.&nbsp;



These remnants represent extreme outcomes of stellar evolution and are fundamentally different from white dwarfs.



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



Gemini is one of the twelve zodiac constellations located in the northern celestial hemisphere.&nbsp;



Its name means "twins" in Latin, reflecting its representation of the mythological twins Castor and Pollux from Greek and Roman mythology.&nbsp;



<h3 class="wp-block-heading" id="h-stars-of-gemini">Stars of Gemini</h3>



The stars Castor and Pollux, which form the heads of the twins, are the brightest stars in Gemini and are key to its identification.&nbsp;



Pollux is a bright orange giant star, while Castor is a multiple <a href="https://www.earth.com/news/exoplanet-found-in-the-habitable-zone-of-a-binary-star-system/" target="_blank" rel="noreferrer noopener">star system</a> made up of six stars.



<h3 class="wp-block-heading" id="h-neighboring-constellations">Neighboring constellations</h3>



Gemini lies between Taurus to the west and Cancer to the east, and it is bordered by several other constellations, including Orion to the south.



It is most visible in the night sky during the winter months in the Northern Hemisphere, particularly in January and February.&nbsp;



<h3 class="wp-block-heading" id="h-significance-of-gemini">Significance of Gemini</h3>



The constellation is part of the ecliptic, the path that the Sun appears to take through the sky, making it significant in both astronomy and astrology.



Astronomically, Gemini is home to several interesting deep-sky objects, including the open star cluster M35, which is easily visible with binoculars or a small telescope.&nbsp;



The constellation also contains several stars and stellar systems of interest, such as variable stars and binary systems.



<h3 class="wp-block-heading" id="h-greek-mythology-nbsp">Greek mythology&nbsp;</h3>



In Greek mythology, Castor and Pollux were the sons of Leda, but they had different fathers - Castor was mortal, while Pollux was divine, being the son of Zeus.&nbsp;



Their story is one of loyalty and brotherhood, as Pollux begged Zeus to share his immortality with Castor after his brother's death. As a result, Zeus placed them in the sky as the constellation Gemini, symbolizing their eternal bond.



<h3 class="wp-block-heading" id="h-modern-culture">Modern culture</h3>



In modern culture, Gemini continues to be associated with duality, adaptability, and communication in astrology.&nbsp;



The constellation also holds significance in space science, lending its name to NASA's Gemini program in the 1960s. This program conducted critical missions that paved the way for the Apollo moon landings.



Image Credit: ESA&nbsp;



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Supernova explosion captured in the constellation Gemini 

It was 1959 when NASA invited Cooper to Washington, D.C. as a potential candidate for the Mercury Project. The project sought to put a man into Earth's orbit and then return him safely, and Cooper was an ideal candidate. Alan Shepard, if you remember, commanded the first flight on&nbsp;Freedom 7. Photo Credit: NASA

Mercury Project

The bison in Yellowstone National Park have captivated visitors for generations. These animals have roamed the region since the park’s establishment in 1872, bringing travelers from around the world to see these majestic creatures up close.



Bison once endured a disastrous period known as the <a href="https://www.biodiversitylibrary.org/item/36694#page/7/mode/1up" target="_blank" rel="noreferrer noopener">population bottleneck</a>, leaving fewer than 25 wild animals in Yellowstone in the early 1900s. 



A small group of domestic bison from Montana and the <a href="https://www.traveltexas.com/cities-and-regions/panhandle-plains/" target="_blank" rel="noreferrer noopener">Texas Panhandle</a> helped rebuild the numbers when they were introduced to bolster the wild survivors.



The national park <a href="https://www.buffalofieldcampaign.org/images/get-involved/students-resource-about-bison/bison-conservation-papers/White-et-al-Management-of-Yellowstone-bison-and-brucellosis-transmission-risk-January-2011.pdf" target="_blank" rel="noreferrer noopener">population</a> rose to about 4,000 - 6,000 individuals over the following century. This growth stands out as a story of resilience, given the dangers once faced by these iconic <a href="https://www.earth.com/news/wolves-are-rebuilding-forests-and-restoring-ecosystem-balance-in-yellowstone/" target="_blank" rel="noreferrer noopener">creatures</a>.



<h2 class="wp-block-heading" id="h-bison-now-form-one-big-herd">Bison now form one big herd</h2>



After years of monitoring their movements, Dr. James Derr from the Department of Veterinary Pathobiology at the College of Veterinary Medicine &amp; Biomedical Sciences (<a href="https://vetmed.tamu.edu" target="_blank" rel="noreferrer noopener">VMBS</a>) at Texas A&amp;M has brought new clarity to how these bison breed.



His team’s genetic findings indicate a shift in behavior that rewrites previous understandings of separate herds within <a href="https://www.earth.com/news/yellowstone-supervolcano-eruption-study-sparks-new-debate-on-where-and-when-it-will-erupt/" target="_blank" rel="noreferrer noopener">Yellowstone</a>.



Management plans have often revolved around the assumption of two distinct herds that needed separate strategies. According to the latest research, that division may no longer exist.



“This finding certainly has a direct impact on the long-term conservation and <a href="https://www.earth.com/news/yellowstone-tourism-generates-over-1-megaton-carbon-annually/" target="_blank" rel="noreferrer noopener">management</a> of this iconic bison population,” said Dr. Derr. In simpler terms, the park’s bison are now breeding in a unified way.



“To get a clearer picture, we examined samples from the two major summer breeding groups and two major winter ranges,” said Dr. Sam Stroupe, a researcher at VMBS.



Evaluations confirmed that genetic exchange is happening throughout Yellowstone, rather than staying within smaller pockets.



Scientists took advantage of new tools to compare markers in bison DNA, offering a fuller picture than was possible two decades ago. 



This helped them pinpoint the extent of gene flow, revealing the <a href="https://www.earth.com/news/giant-viruses-found-in-yellowstones-hot-springs-are-1-5-billion-years-old/" target="_blank" rel="noreferrer noopener">animals</a> function as one interconnected group.



<h2 class="wp-block-heading" id="h-unified-bison-herd-boosts-stability">Unified bison herd boosts stability</h2>



Experts now recommend that these bison be managed as a single population with multiple subunits. This shift in approach aims to preserve genetic diversity for future generations.



One reason for this recommendation is the strong health of the overall gene pool. 



Researchers observed that the bison population carries lineages from both the original <a href="https://www.earth.com/news/yellowstone-lake-maintains-ice-cover-despite-warming-climate/" target="_blank" rel="noreferrer noopener">Yellowstone</a> group and later introductions, which appears to boost stability.



Park officials work alongside wildlife specialists to watch for any sign of genetic risk in the herd. 



Recognizing a single breeding population encourages consistent strategies that keep gene flow open and protect the animals from harmful inbreeding.



Stewardship also involves collaboration with various stakeholders to maintain ecological balance. By monitoring bison migration between seasonal ranges, specialists can refine how they address population numbers and habitat needs.



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



The U.S. national mammal has long served as a symbol of vitality and grit. Part of what makes Yellowstone special is its free-roaming herds that <a href="https://www.earth.com/news/yellowstone-tourism-generates-over-1-megaton-carbon-annually/" target="_blank" rel="noreferrer noopener">remind onlookers of wilder days</a> in American history.



These new findings come with the hope that data-driven strategies will guide the next steps in bison management. 



Experts underscore that clear research on herd structure is key to making solid decisions about when, where, and how to intervene.



These animals continue to face environmental challenges, from harsh winters to pressure at park boundaries. 



Yet the results of this study suggest that a single, large interbreeding population can handle setbacks if carefully supported.



Conservation teams believe that gene flow across herds helps the species maintain the adaptability needed for long-term survival. Watching for any future shifts will remain essential, given Yellowstone’s changing landscape.



<h2 class="wp-block-heading" id="h-tracking-the-yellowstone-bison-herd">Tracking the Yellowstone bison herd</h2>



As rangers and scientists track bison movements, they will look for ways to keep habitats healthy. A wide-ranging herd needs well-managed feeding grounds, especially during winter, to prevent overuse of any single area.



Researchers also emphasize the importance of monitoring herd size. When bison remain robust and widespread, they are less vulnerable to sudden ecological shifts.



Some experts suggest that this united herd might further stabilize <a href="https://www.earth.com/news/wolves-are-rebuilding-forests-and-restoring-ecosystem-balance-in-yellowstone/" target="_blank" rel="noreferrer noopener">Yellowstone’s ecological balance</a>. 



The presence of these formidable grazers recycles nutrients in grasslands and provides food sources for predators and scavengers.



Standing as the largest wild bison herd in the country, these animals offer a unique window into how to handle wildlife management challenges. They also serve as a source of cultural pride and a reminder of North America’s natural heritage.



<h2 class="wp-block-heading" id="h-science-based-animal-protection">Science-based animal protection</h2>



Moving forward, the focus is on using science-based approaches to protect these Yellowstone bison without fragmenting the population. 



This aligns with a broader trend toward <a href="https://www.earth.com/news/bison-slaughter-had-lasting-traumatic-impacts-on-indigenous-communities/" target="_blank" rel="noreferrer noopener">safeguarding genetic variety</a> in national parks across the country.



Keeping tabs on reproduction patterns will remain vital. If different groups started breeding apart again in the future, managers would need to adapt their strategies.



This shift to one breeding population also carries lessons for other species. Large areas of protected habitat, combined with the right research, can help threatened animals recover from historical hardships.



Several wildlife researchers have praised Yellowstone’s example. Their unified effort confirms that even after past declines, thoughtful planning can sustain a species that once hovered on the edge of vanishing.



The study is published in the <a href="https://academic.oup.com/jhered/article/116/1/1/7756833?login=false" target="_blank" rel="noreferrer noopener">Journal of Heredity</a>.



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Yellowstone's iconic bison have finally merged back into a single her after 120 years of effort

The bison in Yellowstone National Park have captivated visitors for...

Fiddler crab mating on the bustling mudflats of southern Europe is about sending seismic love signals beneath the surface - quite literally.



In their quest to attract a mate, male crabs produce ground vibrations as part of an elaborate courtship ritual. For the first time, scientists have recorded and analyzed these signals to understand how they communicate in a chaotic and noisy habitat.



Researchers from the <a href="https://www.ox.ac.uk/" target="_blank" rel="noreferrer noopener">University of Oxford</a> have captured the full courtship display of the European fiddler crab (Afruca tangeri), combining video footage and geophone recordings to listen in on the crabs’ seismic conversations. 



These crabs inhabit the muddy shores of the Iberian Peninsula, where waves, wind, and competing crabs make for a challenging environment to get a message across. 



However, the study reveals that these <a href="https://www.earth.com/news/new-invasive-crustacean-species-discovered-in-the-mediterranean/" target="_blank" rel="noreferrer noopener">crustaceans</a> have developed a clever and consistent way to make themselves heard - and felt.



<h2 class="wp-block-heading" id="h-how-fiddler-crabs-use-vibrations">How fiddler crabs use vibrations</h2>



Male fiddler crabs are known for their oversized claws, which they use to wave at potential mates and generate ground vibrations. These signals are produced by striking the ground with the claw or <a href="https://www.earth.com/news/crab-shells-could-help-pave-the-way-for-sustainable-electronics/" target="_blank" rel="noreferrer noopener">shell</a>, and later by drumming from inside their burrows.



The researchers discovered that fiddler crab mating follows a four-step courtship routine, starting with subtle claw waves, followed by body drops, synchronized movements, and ending with underground drumming if a female shows interest.



As each stage progresses, the energy of the vibrations increases. The recordings, captured with GoPro cameras and precise geophones, allowed the team to measure over 8,000 seismic signals during the courtship routines.



<h2 class="wp-block-heading" id="h-seismic-vibrations-reveal-crab-size">Seismic vibrations reveal crab size</h2>



The key question was whether these vibrations serve as honest signals of the male’s size and strength. The results suggest they do. 



The data showed that larger male crabs with bigger <a href="https://www.earth.com/news/strawberry-claws-the-hermit-crab-that-sings-underwater/" target="_blank" rel="noreferrer noopener">claws</a> produced more powerful seismic signals, especially during drumming. This means the crabs can’t fake their physical traits – what you vibrate is what you are.



“It appears as though the males cannot, or do not, lie about their physical size,” said Tom Mulder from the Department of Biology at the University of Oxford. 



“Females can rely on the loudness of seismic signals to honestly assess a potential mate’s quality, all without needing to see him.”



<h2 class="wp-block-heading" id="h-machine-learning-meets-marine-dating">Machine learning meets marine dating</h2>



When it comes to fiddler crab mating, the frequency of vibrations stays the same - but other features like rhythm, duration, and loudness change depending on the&nbsp;crab’s demeanor.



This allowed the researchers to classify each action (such as a body drop or an underground drum) by analyzing the vibration patterns.



To test this further, the team used <a href="https://www.earth.com/news/scientific-discoveries-machine-learning/">machine learning</a> to teach a computer how to distinguish between different crab behaviors based solely on these recordings.



The program achieved a 70% accuracy rate, showing strong potential for future applications. The technique could lead to the development of non-invasive monitoring systems for a wide range of animals.



From tracking <a href="https://www.earth.com/news/what-is-the-future-of-the-endangered-species-act/" target="_blank" rel="noreferrer noopener">endangered species</a> across the savannah to identifying crop pests or spotting injured livestock, material-bound vibrations could become a new frontier in remote wildlife observation.



<h2 class="wp-block-heading" id="h-vibrations-work-for-the-fiddler-crab">Vibrations work for the fiddler crab</h2>



When it comes to fiddler crabs, relying on seismic signals instead of sound makes perfect sense. Their noisy, open-air environment is difficult to navigate acoustically, but the ground beneath them offers a stable way to communicate.



By altering the strength and tempo of their vibrations, they can get their messages across without saying a word.



“Larger claws have the advantage of overcoming seismic noise so that they can signal to females that are further away, and females will show more interest in them,” explained Dr. Beth Mortimer, also from the Department of Biology.



“However, the advantages are only observed for the percussive signals such as drumming, and fortunately for smaller clawed crabs, these are only part of the courtship routine.”



So, while size matters when it comes to seismic communication, smaller males can still show off through other parts of the ritual. In the unpredictable world of fiddler crab mating, it’s not just about waving your claw - it’s about how hard you drum.



The full study was published in the journal <a href="https://journals.biologists.com/jeb/article/228/7/jeb249323/367607/Constraints-on-percussive-seismic-signals-in-a" target="_blank" rel="noreferrer noopener">Journal of Experimental Biology</a>.



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Fiddler crabs use seismic vibrations to attract mates

Fiddler crab mating on the bustling mudflats of southern Europe...

Launched just seven months ago, the Arctic Weather Satellite is already reshaping the future of weather forecasting.



Despite its compact size and modest development time, the satellite is producing detailed temperature and humidity data that could soon boost short-term forecasts - especially in remote regions like the Arctic.



Developed by scientists from the <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">European Space Agency</a> (ESA), this prototype satellite was built in only three years and at a fraction of the cost of traditional Earth observation missions. ESA designed it to test a new approach: build fast, build affordably, and still deliver high-quality data. 



Early results show this model is working. The satellite’s microwave radiometer has proven capable of producing data that are comparable with those gathered by much larger, more established missions.



<h2 class="wp-block-heading" id="h-small-size-powerful-data">Small size, powerful data</h2>



At the heart of the Arctic Weather Satellite is a 19-channel cross-track scanning microwave radiometer. This tool measures atmospheric <a href="https://www.earth.com/news/global-temperature-increase-2023-blew-past-all-climate-models/" target="_blank" rel="noreferrer noopener">temperature</a> and <a href="https://www.earth.com/news/humidity-increases-urban-heat-stress/" target="_blank" rel="noreferrer noopener">humidity</a> through cloud cover, providing critical information in all weather conditions. 



Though named after the Arctic, the satellite gathers global data. Its insights into water vapor levels are particularly valuable in polar regions, where rapid changes in humidity can dramatically alter forecasts.



What makes this even more impressive is that the satellite weighs just 125 kilograms - roughly the size of a washing machine. It also uses a new 325 GHz sounding channel, a frequency that has never before been applied to operational <a href="https://www.earth.com/news/satellite-data-could-revolutionize-weather-forecasts/" target="_blank" rel="noreferrer noopener">weather monitoring</a>. 



This addition allows for better cloud-ice measurements, potentially improving forecast accuracy even further.



<h2 class="wp-block-heading" id="h-step-toward-a-satellite-constellation">Step toward a satellite constellation</h2>



The Arctic Weather Satellite is just the beginning. It serves as a prototype for the proposed EPS-Sterna constellation, a future group of six similar satellites. 



ESA would build the satellites, and Eumetsat would manage their operations and data distribution - mirroring the approach used for Europe’s Meteosat and MetOp weather missions.



Before making that leap, though, scientists need to confirm how much value this small satellite’s data can add to existing forecasts. That evaluation is already underway.



<h2 class="wp-block-heading" id="h-broad-testing-strong-feedback">Broad testing, strong feedback</h2>



Meteorological agencies across Europe are studying the satellite’s data, including the Danish Meteorological Office, the German Weather Service, and the European Centre for Medium-Range Weather Forecasts. 



Eumetsat is also running its own independent performance assessments. So far, the feedback is overwhelmingly positive.



“Our team has carefully evaluated the quality of the Arctic Weather Satellite’s data and has already been able to demonstrate a positive impact on our forecasts at the global scale, and we plan to include the data in our global prediction system later this year," said Philippe Chambon from Météo-France. 



According to Chambon, this a very promising achievement in view of the EPS-Sterna constellation, which is seen as a key component of the future observing system.



<h2 class="wp-block-heading" id="h-valuable-data-from-small-satellites">Valuable data from small satellites</h2>



“The Arctic Weather Satellite is a great example of the quality of meteorological data that can be achieved from a small satellite," commented Niels Bormann from the European Centre for Medium-Range Weather Forecasts. 



Bormann noted that the initial results are very promising for global weather forecasts and, if they hold up, the data may be used operationally later in the year. From a regional perspective, the data is proving just as useful.



“Together with the Nordic national meteorological services, we are evaluating the Arctic Weather Satellite’s data for regional forecasting over Scandinavia and the Arctic," said Adam Dybbroe from the Swedish Meteorological and Hydrological Institute. 



<h2 class="wp-block-heading" id="h-closing-the-polar-coverage-gap">Closing the polar coverage gap</h2>



Current weather satellites have limitations. For example, <a href="https://www.earth.com/image/meteosat-weather-satellite-captures-earth-in-stunning-detail/" target="_blank" rel="noreferrer noopener">Meteosat satellites</a> orbit 36,000 kilometers above the equator, returning images every 15 minutes, but they can’t cover the high latitudes near the poles. 



MetOp satellites, which follow a polar orbit, can reach these regions but take up to 24 hours for full global coverage.



The proposed EPS-Sterna constellation of six satellites would dramatically shorten this time gap, offering more frequent data - especially over the Arctic.



<h2 class="wp-block-heading" id="h-huge-potential-in-a-small-satellite">Huge potential in a small satellite </h2>



ESA’s Arctic Weather Satellite project manager, Ville Kangas, summarized the progress.



“We have demonstrated that a small satellite, weighing just 125 kg, can match the performance of large meteorological missions," said Kangas.



"And since we are at a relatively early stage, the data still need to be further corrected and analyzed so we expect the Arctic Weather Satellite to shine even more in the months to come."



If approved, the EPS-Sterna constellation will work alongside Europe’s next-generation weather satellites, including MTG-S1 and MetOp-SG-A1, which are scheduled for launch later this year. 



Together, these systems could create a far more complete and timely picture of <a href="https://www.earth.com/news/climate-change-is-shrinking-earths-atmosphere-and-thats-bad-for-satellites/" target="_blank" rel="noreferrer noopener">Earth’s changing atmosphere</a>.



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Small satellite could transform weather forecasting

Launched just seven months ago, the Arctic Weather Satellite is...

Harvest,Pink,Moon,On,Night,Sky,Back,Over,Silhouette,Pines

The Moon has always fascinated humans. But even now, with satellites and science at our fingertips, the <a href="https://www.earth.com/news/young-ridges-on-moons-surface-suggest-that-it-is-still-active/" target="_blank" rel="noreferrer noopener">Moon</a> can still surprise us. This Saturday night, skywatchers will witness one such surprise: a pink micromoon.



While not as dramatic as a total eclipse or as bright as a supermoon, the micromoon holds its own quiet charm. It’s a moment to pause, look up, and remember that the heavens are always in motion - even if the changes aren’t always obvious.



Let’s explore what makes a micromoon special, why our brains sometimes trick us, and how even seasoned scientists are still mystified by the Moon’s shifting appearance.



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



A micromoon occurs when the <a href="https://www.earth.com/news/march-2025-stargazing-a-red-moon-and-a-vanishing-planet/" target="_blank" rel="noreferrer noopener">Moon</a> reaches the farthest point in its elliptical orbit around Earth. That moment, called apogee, coincides with the full moon phase.



When this happens, the Moon looks smaller and dimmer than usual. The effect is subtle - most people won't notice unless they compare photos side by side.



“It’s a very subtle difference,” said astrophysicist Alain Brizard from <a href="https://www.smcvt.edu" target="_blank" rel="noreferrer noopener">Saint Michael’s College</a> in Vermont.



In contrast, a supermoon happens when the Moon is at its closest point to Earth. The difference between a micromoon and a supermoon isn’t huge, but it’s measurable. Supermoons can appear about 14% larger and 30% brighter.



Micromoons and supermoons aren’t rare. They happen several times a year when the Moon’s full phase syncs up with the right point in its orbit. 



Another micromoon will arrive in May. Three supermoons are expected later this year in October, November, and December.



<h2 class="wp-block-heading" id="h-the-moon-illusion">The Moon illusion</h2>



Many people believe the <a href="https://www.earth.com/news/total-lunar-eclipse-will-paint-the-moon-blood-red-tomorrow/" target="_blank" rel="noreferrer noopener">Moon</a> looks biggest when it rises over the horizon. This is true - at least, visually.



When we see the <a href="https://www.earth.com/news/whats-up-in-the-night-sky-during-the-month-of-april-2025/" target="_blank" rel="noreferrer noopener">Moon</a> rise over city skylines, treetops, or mountains, it can seem enormous. The truth is, though, that its size hasn’t changed at all. It’s a trick of the mind.



Photos show the Moon stays the same width, whether near the horizon or overhead. Still, our eyes say otherwise. The Moon looks larger near the horizon, though it's not.



This illusion comes from how our brains handle visual information. It's a perception trick. Even after thousands of years of watching <a href="https://www.earth.com/news/young-ridges-on-moons-surface-suggest-that-it-is-still-active/" target="_blank" rel="noreferrer noopener">the Moon</a>, no one fully understands why we see it this way.



This phenomenon is known as the Moon illusion. It has nothing to do with the Moon itself and everything to do with human perception.



<h2 class="wp-block-heading" id="h-how-to-test-the-micromoon-illusion-yourself">How to test the micromoon illusion yourself</h2>



You don’t need a telescope to prove the illusion is real.



<a href="https://www.nasa.gov" target="_blank" rel="noreferrer noopener">NASA</a> suggests simple tests. Hold out your index finger next to the <a href="https://www.earth.com/news/asteroid-that-once-threatened-earth-may-target-the-moon/" target="_blank" rel="noreferrer noopener">Moon</a>. Your fingernail and the Moon will appear nearly the same size - no matter where the Moon sits in the sky.



You can also look through a paper tube or even bend over and look between your legs. The Moon will suddenly seem much smaller than it did a moment before.



Step outside on a full moon night and watch the Moon as it rises. It can feel magical - so big and beautiful that it might make you say “Wow!” out loud. 



When the Moon is low in the sky, near mountains, buildings, or trees, it looks huge. It seems like it’s towering over the landscape.



But here’s the truth: the Moon hasn’t actually grown. Your brain is just playing a trick on you.



The large size you see is an illusion. It’s not caused by the atmosphere or the Moon’s distance. It’s all about how your mind interprets the scene in front of you.



<h2 class="wp-block-heading" id="h-why-the-micromoon-looks-pinkish">Why the micromoon looks pinkish</h2>



While the Moon doesn’t grow or shrink in size, it can appear to change color.



When the Moon is low in the sky, it often looks pink, yellow, or sometimes orange. This happens because its light must travel through more of Earth’s atmosphere. 



The atmosphere scatters shorter wavelengths of light, like blue and violet. What’s left are the longer wavelengths - pink, orange, and yellow.



Dust or pollution in the air can make this effect stronger, giving the Moon a deeper red or orange tint.



This effect is especially visible during events like lunar eclipses. A total eclipse in March turned the Moon a deep coppery red - a visual reminder of how much the atmosphere shapes what we see.



<h2 class="wp-block-heading" id="h-theories-behind-the-moon-illusion">Theories behind the Moon illusion</h2>



Despite centuries of study, scientists still don’t have a full explanation for the Moon illusion. Here’s the surprising part: scientists still don’t fully understand why the Moon illusion happens.



That might sound frustrating if you like clear answers. But it also shows how mysterious our brains can be. Even after years of research, no one has found a complete explanation for why the Moon looks bigger near the horizon.



So depending on how you see it, this mystery can either be disappointing - or something to wonder about and enjoy.



The most common idea is that our brains misjudge size and distance when the Moon is near the horizon. When objects like buildings, mountains, or trees are in the foreground, they can trick the brain into thinking the Moon is closer - and therefore larger - than it actually is.



One well-known theory is the <a href="https://en.wikipedia.org/wiki/Ponzo_illusion" target="_blank" rel="noreferrer noopener">Ponzo illusion</a>. Imagine railroad tracks converging into the distance. Place two identical lines across the tracks - one higher, one lower. 



The upper line will seem longer. This may be similar to how we view the Moon over a landscape.



But the mystery deepens. Astronauts in space, far from any such cues, also report seeing the Moon illusion. So the story doesn’t end there.



<h2 class="wp-block-heading" id="h-why-the-micromoon-s-mystery-is-worth-enjoying">Why the micromoon’s mystery is worth enjoying</h2>



In the end, maybe we don’t need a perfect answer.



Imagine seeing the Moon rise during the day over mountains. Even without knowing the science behind it, that sight can fill you with wonder.



We may not fully understand why the Moon looks bigger or more dramatic at times. But while scientists keep searching for answers, there's nothing stopping us from enjoying the view.



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What is a pink micromoon? You'll find out tonight

The Moon has always fascinated humans. But even now, with...

Japan loves otters and so does the internet. From squeaky coos to floating belly naps, Asian small-clawed otters have taken over YouTube and Instagram feeds. These animals show up in themed cafés, cozy up to coffee cups, and pose beside smiling tourists. It’s not hard to see why they’ve become a social media sensation.



But this viral fame hides a growing crisis. The adorable otter’s rise to stardom has come at a cost to wild populations. Behind every click, like, and share may lie a deeper story - one of trafficking, genetic decline, and fading <a href="https://www.earth.com/news/sea-otters-help-kelp-forests-recover-but-theres-more-to-the-story/" target="_blank" rel="noreferrer noopener">biodiversity</a>. 



Japan sits at the center of this trade, both as a consumer and as a mirror to a broader wildlife issue across Asia.



<h2 class="wp-block-heading" id="h-japan-s-pet-otter-boom">Japan’s pet otter boom</h2>



Asian small-clawed <a href="https://www.earth.com/news/sea-otters-have-protected-california-kelp-forests-for-a-century/" target="_blank" rel="noreferrer noopener">otters</a>, native to South and Southeast Asia, are now listed as vulnerable by the IUCN. Their populations are threatened by habitat destruction, human-wildlife conflict, and poaching. 



Since 2019, they have been listed in Appendix I of the Convention on International Trade in Endangered Species (<a href="https://cites.org/eng/disc/what.php" target="_blank" rel="noreferrer noopener">CITES</a>), which bans commercial trade except in exceptional cases.



Despite this listing, the otters continue to appear in Japan’s pet stores and animal cafés. Their presence in such places indicates an active, and often illegal, wildlife trade. The allure is strong - cuddly, curious, and highly intelligent, otters are marketed as ideal companions for exotic pet lovers.



But their popularity on social media has created a feedback loop of demand that encourages continued trafficking from wild populations.



<h2 class="wp-block-heading" id="h-illegal-otters-sourced-from-thailand">Illegal otters sourced from Thailand</h2>



To understand how otters are ending up in Japanese cafés, researchers from <a href="https://www.kyoto-u.ac.jp/en" target="_blank" rel="noreferrer noopener">Kyoto University</a> teamed up with Thai scientists. 



They aimed to trace the geographic origins of the otters now living in captivity in Japan. Most attention turned to Thailand - a country previously identified as a key player in the illegal otter trade.



"Collaborative research can help identify the origins of <a href="https://www.earth.com/news/sea-otters-use-tools-to-access-larger-prey-and-protect-their-teeth/" target="_blank" rel="noreferrer noopener">otters</a> kept in Japan and hot spots of illegal trade in Thailand, thus encouraging legal control in both countries," said study first author Mayako Fujihara.



Over the last two decades, more than 100 otters have been seized at airports in Thailand and Japan. Most seizures involve multiple individuals at once, suggesting coordinated smuggling efforts. 



Despite Japanese import bans and Thailand’s export restrictions, traffickers continue to find ways to move these animals across borders.



<h2 class="wp-block-heading" id="h-dna-links-otters-to-wild-origins">DNA links otters to wild origins</h2>



To track where the otters came from, researchers sequenced 1,511 base pairs of mitochondrial DNA from 81 captive otters in Japan.



These included <a href="https://www.earth.com/news/world-wildlife-day-2025-a-global-call-to-protect-nature/" target="_blank" rel="noreferrer noopener">individuals</a> from zoos, aquariums, animal cafés, and customs seizures. The goal was to compare these sequences with those from known wild populations in Thailand and surrounding countries.



The analysis revealed 12 different haplotypes, grouped into three major clades. Six of these haplotypes matched wild otters from southern Thailand - areas known for coastal wetlands and hilly riparian zones. 



This suggests that the majority of otters found in cafés and seized at airports had likely originated from poaching hotspots in southern Thailand.



The findings are troubling. According to the CITES trade database, no legal otter imports from Thailand to Japan have occurred since 1988. This means the otters arriving since then - including those born to trafficked individuals - have entered the country through illegal means.



<h2 class="wp-block-heading" id="h-social-media-stardom-drives-demand">Social media stardom drives demand</h2>



The modern otter craze didn’t start in a forest - it started online. YouTube channels featuring <a href="https://www.earth.com/news/un-report-disturbing-details-about-the-state-of-earths-wildlife/" target="_blank" rel="noreferrer noopener">pet</a> otters have millions of subscribers. One top channel in Japan, showing the lives of two otters, has over 1.8 million followers and a merchandise line. The same owner also runs otter cafés in major cities.



These cafés, known as exotic animal cafés, let customers play with otters while sipping coffee. They are part of a broader industry that has expanded rapidly since the early 2000s. 



As of 2019, Japan hosted at least 137 exotic animal cafés, housing more than 400 species. The Asian small-clawed otter is among the most popular mammals in these cafés.



Some cafés even sell otters, with prices reaching over $10,000 per animal. In 2018, nearly half of the otters advertised for sale in Japan came from unknown sources. This lack of transparency fuels concerns about continued reliance on wild populations and unclear breeding histories.



<h2 class="wp-block-heading" id="h-japan-s-native-otter-is-gone">Japan’s native otter is gone</h2>



Japan’s obsession with otters may also stem from a deep-rooted cultural memory. The kawauso, or river otter, appears in Japanese folklore as a playful and mischievous shapeshifter. But this creature was based on a real animal - the Japanese river otter, once common across the country.



Decades of hunting for fur and destruction of river habitats led to its tragic extinction. It was declared extinct in 2012 after not being seen for over 30 years.



"It is precisely because Japan's endemic otter species has gone extinct that we aim to continue conducting research that will help protect other vulnerable species," said Fujihara.



This extinction leaves a shadow over current efforts to protect other otters in captivity and the wild. It also heightens the urgency to prevent similar outcomes for other species caught in the trade.



<h2 class="wp-block-heading" id="h-uneven-diversity-in-captivity">Uneven diversity in captivity</h2>



One of the most striking findings from the study was the difference in genetic diversity between otters in zoos and those in cafés. 



Otters in zoos and aquariums had higher genetic diversity and more varied haplotypes. This is likely due to more structured breeding programs and a larger pool of founding individuals.



In contrast, the otters found in cafés often shared just a few haplotypes. Many had been bred in-country from a narrow gene pool. Some appeared to be closely related. 



This lack of diversity poses risks. Inbreeding can cause health problems and lower reproductive success. It also weakens the species’ long-term ability to adapt and survive.



Otters in zoos also came from a wider range of regions, including Peninsular Malaysia and Indonesia. This indicates legal or semi-legal acquisition before tighter regulations were in place. But many of the café otters clustered genetically with those from southern Thailand - regions known for illegal poaching activity.



<h2 class="wp-block-heading" id="h-science-as-a-shield-for-conservation">Science as a shield for conservation</h2>



The study's genetic work serves a dual purpose: it not only tracks trafficking routes but also supports captive breeding. 



By understanding the genetic background of individual otters, zoos can avoid inbreeding and maintain genetic health. Otters with rare haplotypes - some found in just one or two individuals - can be prioritized for conservation.



However, mitochondrial DNA offers only part of the story. The researchers suggest that nuclear DNA sequencing could give more precise geographic information. This would allow officials to better identify the origin of seized otters and link them to specific regions.



The findings also highlight a need to build comprehensive genetic reference maps for otters across Southeast Asia. Expanding these databases would help pinpoint where wild-caught animals originate and guide future protection efforts.



<h2 class="wp-block-heading" id="h-breeding-for-a-future-not-a-fad">Breeding for a future, not a fad</h2>



As of late 2022, Japan’s zoos and aquariums housed more than 200 Asian small-clawed otters. Many participate in coordinated breeding programs, but others still rely on imports or unverified sources. Without full genetic records, some valuable lineages may be lost.



For example, rare haplotypes found in only one or two otters could disappear without focused efforts. Losing these variants would narrow the gene pool and reduce future adaptability.



Better genetic planning, stronger import regulations, and broader cooperation between nations can help secure the future of this species. The café boom may fade, but the consequences for wildlife will last unless steps are taken now.



<h2 class="wp-block-heading" id="h-japan-s-love-for-otters-has-limits">Japan’s love for otters has limits</h2>



Otters continue to delight audiences with their charm and antics. But behind every viral video lies a question - where did that otter come from, and what did it cost to bring it here?



If admiration leads to exploitation, then love for animals becomes dangerous. Science, policy, and awareness must align to ensure that what we adore today doesn’t vanish tomorrow.



The study is published in the journal <a href="https://conbio.onlinelibrary.wiley.com/doi/10.1111/csp2.70010" target="_blank" rel="noreferrer noopener">Conservation Science and Practice</a>.



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Japan’s obsession with otters comes at a cost

Japan loves otters and so does the internet. From squeaky...

A recent study suggests that sleep may not only preserve our memories but actually enhance them, especially when it comes to recalling the order in which events occur. 



This discovery points to the significant role that restful sleep plays in consolidating daily experiences. It shows that this effect can remain robust for more than a year after the events in question.



<h2 class="wp-block-heading" id="h-boosting-memory-through-sleep">Boosting memory through sleep</h2>



The research was carried out by a team affiliated with a leading center for aging and brain health. The scientists developed an innovative approach to test how sleep influences the sequence of memories over extended periods.



Study senior author Brian Levine is a scientist at the <a href="https://www.baycrest.org/about-us-rri">Rotman Research Institute</a>, part of the Baycrest Academy for Research and Education.



“While our memory for features such as object size and color declines over time, sleep can improve our memory for event sequence,” said Levine. "This study deepens our understanding of how critical sleep is for integrating experiences into memory,” he added.



According to these findings, sleep organizes daily events in order, strengthens their links, and helps us remember them months later.



<h2 class="wp-block-heading" id="h-museum-tour-and-memory-recall">Museum tour and memory recall</h2>



To achieve these insights, the researchers moved beyond typical laboratory procedures that ask participants to memorize word lists or pictures. Instead, they created a 20-minute, audio-guided tour of selected artworks to provide a more authentic experience.



People who took part in this study walked through the exhibit while listening to narrated explanations. They then completed memory tests at intervals ranging from one hour after the tour to 15 months later.



The tests included both questions about the physical features of each artwork and about which piece came first, second, third, and so on. Although shape and color memory faded, sleep notably improved recall of the order in which tour items appeared.



<h2 class="wp-block-heading" id="h-deep-sleep-boosts-memory">Deep sleep boosts memory</h2>



A second experiment reinforced these results through a design that separated participants into two groups. One set - the sleep group - experienced the art tour in the evening and was tested shortly afterward. They then slept in a monitored environment where their brain activity was recorded using electroencephalography (EEG).



The other set - the wake group - took the tour and the initial test in the morning, stayed awake during the day, and was re-tested that evening. Both groups took additional memory tests a week, a month, and 15 months later.



The data showed that even a single night of slumber made a meaningful difference in how participants remembered the order of the tour items. Their advantage, established early, remained evident more than a year afterward.



Meanwhile, memory for the physical features of each artwork continued to deteriorate for both groups. Detailed EEG readings revealed that deep sleep, particularly the combination of slow waves and sleep spindles, correlated strongly with this sustained memory improvement.



<h2 class="wp-block-heading" id="h-sleep-s-lasting-impact">Sleep’s lasting impact </h2>



Sleep’s effect on memory has long intrigued scientists. These findings show that the sequence of experiences can remain intact over extended periods.



Furthermore, the study suggests that certain types of memory, such as object details, may not benefit in the same way. 



By showing this difference, researchers explore why our brains preserve event order even as other details fade over time. Understanding this pattern also holds relevance for <a href="https://www.earth.com/news/defying-time-three-ways-to-slow-biological-aging/">aging</a> populations and those with cognitive conditions, since it sheds light on why memory for events can change so dramatically in later life.



<h2 class="wp-block-heading" id="h-cognitive-health-and-new-interventions">Cognitive health and new interventions</h2>



The benefits of a good night’s rest extend beyond short-term improvements. “The benefits of sleep on memory are powerful; just one night makes a difference that persists over a year,” Levine said.



This underscores the importance of consistent, high-quality sleep as part of an overall strategy to maintain and strengthen cognitive health. Activities such as regular exercise, a balanced <a href="https://www.earth.com/news/brain-health-and-diet-nutrition-helps-lower-dementia-risk/">diet</a>, and attention to sleep routines can work together to keep the mind functioning at its peak.



Researchers hope studying sleep rhythms, slow waves, and spindles will lead to new memory-boosting interventions. These interventions might prove especially significant in helping older adults or those living with <a href="https://www.earth.com/news/your-sleep-may-predict-memory-loss-years-in-advance/">dementia</a> retain key aspects of their experiences for longer.



<h2 class="wp-block-heading" id="h-ongoing-frontier-of-discovery">Ongoing frontier of discovery </h2>



For anyone interested in preserving the narrative thread of life’s events, these results offer an encouraging perspective: better rest today might translate into clearer, more accurate recollections tomorrow and beyond.



The ways in which sleep shapes our memories remain an ongoing frontier of scientific inquiry, but one message comes through loud and clear. 



Whether you are studying for an exam, trying to remember cherished family moments, or simply hoping to keep your recollections intact over time, sleeping well stands out as a critical part of the formula.



The study is published in the journal <a href="https://www.nature.com/articles/s41562-025-02117-5">Nature Human Behavior</a>.



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Sleep can boost memory in a surprising way

A recent study suggests that sleep may not only preserve...

A,School,Of,Salmon,Swimming,In,The,Clear,Water,,Australia

In a large-scale study considered to be the most extensive of its kind so far, researchers from around the world investigated how pharmaceutical pollution influences the behavior and migratory patterns of Atlantic salmon.



The project was led by the <a href="https://www.slu.se/en/" target="_blank" rel="noreferrer noopener">Swedish University of Agricultural Sciences</a> and focused on commonly detected concentrations of clobazam - a medication used to treat sleep disorders - found in waterways.



In the wild, these levels of clobazam were shown to increase the river-to-sea migration success of juvenile <a href="https://www.earth.com/news/early-summer-fishing-shrinks-atlantic-salmon-size-over-time/" target="_blank" rel="noreferrer noopener">salmon</a> and shorten the time it took them to pass through obstacles like hydropower dams.



<h2 class="wp-block-heading" id="h-pharmaceutical-pollution-in-salmon-habitats">Pharmaceutical pollution in salmon habitats</h2>



The findings involved collaboration between many institutions, including Griffith University’s <a href="https://www.griffith.edu.au/research/sciences/australian-rivers-institute" target="_blank" rel="noreferrer noopener">Australian Rivers Institute</a>. Marcus Michelangeli from Griffith, who played a key role in the study, described it as highlighting a global and growing problem of pharmaceutical pollution in natural habitats.



“<a href="https://www.earth.com/news/antidepressant-prozac-pollution-is-severely-depressing-fish-populations/" target="_blank" rel="noreferrer noopener">Pharmaceutical pollutants</a> are an emerging global issue, with over 900 different substances having now been detected in waterways around the world,” Michelangeli said. 



“Of particular concern are psychoactive substances like antidepressants and pain medications, which can significantly interfere with wildlife brain function and behavior.”



<h2 class="wp-block-heading" id="h-unique-real-world-approach">Unique real-world approach</h2>



One unique aspect of this research is its real-world perspective. According to Michelangeli, most previous studies examining the effects of pharmaceutical pollutants on wildlife have been conducted under controlled laboratory conditions, which don’t fully capture the complexities of natural environments.



“This study is unique because it investigates the effects of these contaminants on wildlife directly in the field, allowing us to better understand how exposure impacts <a href="https://www.earth.com/news/covid-lockdowns-had-unexpected-impacts-on-wildlife-behavior/" target="_blank" rel="noreferrer noopener">wildlife behavior</a> and migration in a natural context.”



Clobazam was not the only drug tested. The team also looked at tramadol, an opioid painkiller frequently detected in water samples. 



The researchers used slow-release pharmaceutical implants in combination with tracking transmitters to monitor how both substances affected juvenile Atlantic salmon (Salmo salar) in Sweden’s River Dal as the fish made their journey toward the Baltic Sea.



In addition, the team conducted a laboratory experiment that revealed clobazam altered the salmon’s shoaling behavior, reinforcing the idea that shifts in social or risk-taking tendencies might be tied to drug-induced changes in the fish’s neural functioning.



<h2 class="wp-block-heading" id="h-consequences-of-pharmaceutical-pollution">Consequences of pharmaceutical pollution</h2>



“While the increased migration success in salmon exposed to clobazam might seem like a beneficial effect, it is important to realize that any change to the natural behavior and ecology of a species is expected to have broader negative consequences both for that species and the surrounding wildlife community,” Michelangeli said.



He also noted how complicated these consequences might be when multiple pollutants and species are involved. 



“When you consider realistic exposure scenarios where entire ecosystems are exposed - encompassing multiple species and a diversity of contaminants - the potential consequences become even more complex."



So far, the decline in Atlantic salmon numbers has largely been blamed on factors like overfishing and habitat loss. However, the study implies that pharmaceutical pollution could be subtly reshaping critical life events like the salmon’s migration.



<h2 class="wp-block-heading" id="h-calls-for-better-wastewater-treatment">Calls for better wastewater treatment</h2>



Addressing this issue may be daunting, since many medications do not degrade quickly in the environment and often slip through conventional <a href="https://www.earth.com/news/reed-beds-a-sustainable-revolution-in-wastewater-management/" target="_blank" rel="noreferrer noopener">wastewater treatment</a> systems.



“Advanced wastewater treatment methods are becoming more effective at reducing pharmaceutical contamination, and there is promising potential in green chemistry approaches,” Michelangeli said.



“By designing drugs that break down more rapidly or become less harmful after use, we can significantly mitigate the environmental impact of pharmaceutical pollution in the future.” Indeed, this study underlines how such pollution can produce biological effects that reverberate throughout ecosystems.



Though improved wastewater practices and drug design might help, Michelangeli argued that the task ahead is to figure out how a multitude of chemicals, each at low concentrations, might collectively influence everything from fish migration to <a href="https://www.earth.com/news/danger-zones-climate-change-is-altering-predator-prey-dynamics/" target="_blank" rel="noreferrer noopener">predator-prey dynamics</a>.



“Pharmaceutical pollutants are an emerging global issue, with over 900 different substances having now been detected in waterways around the world,” Michelangeli said, emphasizing that efforts to reduce contamination could make a crucial difference for both animals and humans who share these water sources.



<h2 class="wp-block-heading" id="h-the-future-of-atlantic-salmon">The future of Atlantic salmon</h2>



Ultimately, the story of clobazam and Atlantic salmon reminds us how connected we are to the world around us. Many people rely on medications for their well-being, yet each pill or patch might release chemical remnants into rivers and lakes far beyond our sight.



As the global usage of medications continues to rise, researchers hope to refine tools and strategies that can minimize these ecological footprints. 



They believe that thoughtful design of medicines and advanced treatment systems could go a long way toward safeguarding species. This includes the Atlantic salmon and the wider tapestry of aquatic life that sustains our planet.



The study is published in the journal <a href="https://www.science.org/doi/10.1126/science.adp7174" target="_blank" rel="noreferrer noopener">Science</a>.



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Pharmaceutical pollution changes the behavior of Atlantic salmon

In a large-scale study considered to be the most extensive...

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

[sendtonews key="0ynNMYkMKa-2340414-12187" type="single"] Today’s Video of the Day from the...

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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

[sendtonews key="G9bUoxcjr4-2511624-12187" type="single"] Today's Video of the Day from the...

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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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Coincidentally, a few years&nbsp;before&nbsp;the Apollo 14 crew launched, Astronaut Gordon Cooper — who had a similar role to that of 14&#8217;s Stuart Roosa — first made a discovery from space that changed the way we saw history.

Gordon Cooper Takes Flight

Either way, as team member Dr. David Kring, of the Universities Space Research Association, said, "it is an extraordinary find that helps paint a better picture of early Earth and the bombardment that modified our planet."

Gordon Cooper Takes Flight

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