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...

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 

Today's Image of the Day from the European Space Agency features the galaxy NGC 2090, located approximately 40 million light-years away in the constellation Columba.



NGC 2090 is a stunning spiral galaxy that is notable for its well-defined structure, featuring a bright central core surrounded by tightly wound spiral arms.&nbsp;



These arms are filled with young, hot stars and interstellar gas, indicating active star formation.&nbsp;



Captured by the Webb Telescope’s MIRI and NIRCam instruments, the image reveals the galaxy's winding spiral arms and the swirling gas and dust of its disc in magnificent and unique detail, noted <a href="https://www.esa.int/ESA_Multimedia/Images" target="_blank" rel="noreferrer noopener">ESA</a>. 



<h2 class="wp-block-heading" id="h-observations-of-ngc-2090">Observations of NGC 2090</h2>



The galaxy’s spiral pattern is relatively symmetrical, making it a fascinating object of study for astronomers interested in galactic evolution and dynamics.&nbsp;



Observations of NGC 2090, including those conducted by the <a href="https://www.earth.com/news/hubble-helps-solve-the-mystery-of-a-young-eruptive-star/" target="_blank" rel="noreferrer noopener">Hubble</a> Space Telescope, have provided valuable insights into the properties of its stellar populations, gas content, and the nature of its spiral structure.



“NGC 2090 was one of many galaxies studied by the NASA/ESA Hubble Space Telescope to refine the measurement of the Universe’s expansion rate, or ‘Hubble constant,’” said ESA.&nbsp;



“This can be done by observing a special type of variable stars named ‘Cepheids’ in relatively nearby galaxies.”



<h2 class="wp-block-heading" id="h-new-insights-into-ngc-2090">New insights into NGC 2090</h2>



A Cepheid-based measurement from 1998 indicated that NGC 2090 is 37 million light-years away from Earth. However, the latest measurements suggest that the galaxy is 40 million light-years away.



“Already before that Hubble project in 1998, NGC 2090 had been well studied as a very prominent nearby example of star formation,” noted ESA.&nbsp;



“Described as a ‘flocculent’ spiral, this galaxy has a patchy, dusty disc and arms that are flaky or not visible at all. We can see those patterns well in Hubble's visible-light images. However, Webb’s NIRCam near-infrared data reveal the spiral arms with remarkable clarity.”&nbsp;



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



<a href="https://www.earth.com/news/the-mesmerizing-beauty-of-spiral-galaxies/" target="_blank" rel="noreferrer noopener">Spiral galaxies</a> are among the most common and visually striking types of galaxies in the universe.&nbsp;



They are characterized by their flat, disk-like shape with a bright central bulge surrounded by sweeping spiral arms.&nbsp;



<h3 class="wp-block-heading" id="h-spiral-arms-and-central-bulge-nbsp">Spiral arms and central bulge&nbsp;</h3>



The arms of a spiral galaxy are regions where stars, gas, and dust are concentrated, often glowing brightly with the light of young, hot stars that form within them.&nbsp;



The central bulge typically contains older stars and can host a supermassive black hole at its core.&nbsp;



<h3 class="wp-block-heading" id="h-types-of-spiral-galaxies-nbsp">Types of spiral galaxies&nbsp;</h3>



Spiral galaxies are classified into different types based on how tightly their arms are wound and the size of their central bulge, ranging from tightly wound "Sa" galaxies to loosely wound "Sc" types.



<h3 class="wp-block-heading" id="h-star-formation-nbsp">Star formation&nbsp;</h3>



The structure of spiral galaxies is maintained by the interplay of gravity and angular momentum, with a rotating disk of stars and gas giving rise to their iconic shape.&nbsp;



They are active sites of <a href="https://www.earth.com/news/massive-star-redefines-our-understanding-of-stellar-evolution/" target="_blank" rel="noreferrer noopener">star formation</a> due to the abundance of gas in their arms.&nbsp;



Spiral galaxies often have a halo of older stars and globular clusters surrounding their disks, which provides clues about their formation and evolution.&nbsp;



<h3 class="wp-block-heading" id="h-barred-spiral-galaxy">Barred spiral galaxy</h3>



The <a href="https://www.earth.com/news/milky-way-galaxy-is-surrounded-by-massive-magnetic-fields/" target="_blank" rel="noreferrer noopener">Milky Way</a>, the galaxy that contains our Solar System, is a prime example of a barred spiral galaxy, a subtype where a bar-shaped structure of stars extends from the central bulge.&nbsp;



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



Columba is a small and relatively faint constellation in the southern sky, whose name means "dove" in Latin. It was introduced in the late 16th century by the Dutch astronomer Petrus Plancius and first appeared in a celestial atlas by Johann Bayer in 1603.&nbsp;



The <a href="https://www.earth.com/news/super-jupiter-discovered-in-the-great-bear-constellation/" target="_blank" rel="noreferrer noopener">constellation</a> is said to represent the dove sent out by Noah during the biblical flood, tying it to themes of hope and peace.



Columba lies near the larger constellation Canis Major and is bordered by others such as Lepus and Puppis.&nbsp;



Although it lacks particularly bright stars, its most notable star, Alpha Columbae (also called Phact), shines at a magnitude of approximately 2.6 and is a hot blue-white star. Beta Columbae, another prominent star in the constellation, is a slightly cooler, yellow-white star.



The constellation is best viewed from the Southern Hemisphere during the summer months, though it can also be seen from lower latitudes in the Northern Hemisphere.&nbsp;



Image Credit: NASA/ESA/CSA James Webb Space Telescope&nbsp;



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Webb unveils a spiral galaxy in magnificent detail

It appears that Big Bertha had formed in circumstances that you wouldn’t have generally expected to find up on the Moon. Moreover, its components – made up of feldspar, zircon and quartz – are said to be rare on the natural satellite. So, what exactly are the implications of these strange details?

21. Rare Materials

Scientists have long wondered how the brain updates itself with new information and memories. Some ideas revolve around chemical changes in specific neurons, while others focus on structural shifts among brain cells.



<a href="https://www.tcd.ie/research/profiles/?profile=tryan6">Dr. Tomás Ryan</a> from <a href="https://www.tcd.ie" target="_blank" rel="noreferrer noopener">Trinity College Dublin</a> is among the neuroscientists who have explored these questions by tracking cells involved in <a href="https://www.earth.com/news/memory-isnt-only-stored-in-our-brains-other-cells-can-remember-too/" target="_blank" rel="noreferrer noopener">learning</a>. 



New <a href="https://www.cell.com/current-biology/fulltext/S0960-9822(23)01512-9">findings</a> suggest memory formation hinges on connections between groups of <a href="https://www.nature.com/articles/s41380-023-02137-5">engram cells</a>, which are neurons thought to capture and store distinct experiences.



<h2 class="wp-block-heading" id="h-how-memories-become-linked">How memories become linked</h2>



Researchers believe each experience leaves a pattern of brain cell activation that can be switched on later. To see this process in action, neuroscientists tracked two sets of engram cells, each tied to a different memory. 



They discovered that when one set of cells was reactivated, the other set sometimes lit up too, as if the memories had become linked.



This idea runs counter to the old notion that an individual neuron stores an entire memory. Instead, the memory might be in the connections these <a href="https://www.earth.com/news/sleep-rewires-the-brain-to-strengthen-memories/" target="_blank" rel="noreferrer noopener">cells</a> build and reshape over time. 



Such structural rearrangements help us handle new information without losing old experiences.



<h2 class="wp-block-heading" id="h-which-brain-cells-store-memories">Which brain cells store memories?</h2>



“Memory engram cells are groups of brain cells that, activated by specific experiences, change themselves to incorporate and thereby hold information in our brain,” said <a href="https://orcid.org/0000-0002-8365-2762" target="_blank" rel="noreferrer noopener">Dr. Clara Ortega-de San Luis</a>, Postdoctoral Research Fellow and lead author on the study. 



She and her colleagues monitored how similar or related memories were stored across different brain areas. 



They used genetic techniques to label neurons that fired for one event, then watched how those same <a href="https://www.earth.com/news/smartphones-are-teaching-us-how-to-supercharge-our-memory/" target="_blank" rel="noreferrer noopener">neurons</a> responded to a second event that felt related.



One major clue came from measuring how well these labeled neurons made new links with cells that were tied to older, separate experiences. 



Optogenetics, a method that turns cells on or off with light, let them test whether blocking these newly formed links disrupted the memory.



<h2 class="wp-block-heading" id="h-how-one-protein-shapes-memory">How one protein shapes memory</h2>



A specific protein, <a href="https://molecularbrain.biomedcentral.com/articles/10.1186/s13041-019-0520-x" target="_blank" rel="noreferrer noopener">PSD-95</a>, emerged as a gatekeeper of these engram cell connections. This protein sits at nerve cell junctions called <a href="https://www.nature.com/articles/24790" target="_blank" rel="noreferrer noopener">synapses</a> and helps anchor receptor molecules.&nbsp;



When the team lowered the amount of PSD-95 in the neurons storing a given memory, these connections behaved differently. Under certain conditions, the memory seemed to linger even when researchers tried to dampen it.



That persistence hints at how the brain can hang on to memories that we might assume should fade. It also hints at why a shortage or disruption of PSD-95 could derail normal learning <a href="https://www.earth.com/news/why-memories-close-in-time-feel-connected/" target="_blank" rel="noreferrer noopener">patterns</a>.



<h2 class="wp-block-heading" id="h-brain-cells-build-on-old-memories">Brain cells build on old memories</h2>



This work taps into a broader shift in neuroscience. Rather than focusing on single cells, many researchers now examine how multiple cells form networks that hold our daily experiences. 



By using cutting-edge genetic tagging, scientists can identify where new links are happening and whether these connections are essential for recalling the <a href="https://www.earth.com/news/forgetting-things-is-a-natural-part-of-the-memory-process/" target="_blank" rel="noreferrer noopener">memory</a> later.



Many of the previous studies mapped separate steps: encoding a memory, storing it, then reactivating it. 



This project took it one step further by showing how the brain might slot fresh information into an existing network, so the old memory is updated instead of replaced.



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



Experts have debated how new learning manages not to overwrite older memories in the same region of the brain. According to Dr. Ryan, “we should search for information ‘between’ cells.”&nbsp;



This view suggests memories are not locked inside one specific location but scattered as connections that can be modified. If true, it may explain how we learn quickly from everyday life without dismantling what we already know.



Therapies could one day target the proteins that enable these shifting connections. If molecules like PSD-95 shape synapses to store a memory, then changing them might help reframe harmful memories tied to fear or trauma, though more studies are needed.



<h2 class="wp-block-heading" id="h-how-brain-cells-shape-daily-memory">How brain cells shape daily memory</h2>



Memory isn’t purely academic. Our daily routines demand constant learning, whether it’s recalling names, navigating busy streets, or picking up a new hobby. 



Understanding how the brain cells keep all that information flexible, yet stable, offers hope for tackling age-related memory issues or conditions that affect learning.



Additional work in the field has shown that certain neurons can take on multiple roles depending on the situation. 



Those roles often shift over time, especially when new experiences pile up. By homing in on the connections, scientists add a piece to the puzzle of how these cells adapt.



<h2 class="wp-block-heading" id="h-where-this-research-could-lead">Where this research could lead</h2>



Unraveling the complicated dance among engram cells might eventually guide how we teach, treat memory disorders, or support mental health. 



If wiring changes are at the core of learning, there might be clever ways to prompt healthy rearrangements in people struggling with conditions like post-traumatic stress or depression.



This study gives a peek into that process. It reveals a fragile, but critical, balance at the heart of learning: strengthen certain neural links for new knowledge, but keep enough structure so older skills and memories remain intact.



The study is published in <a href="https://www.cell.com/current-biology/fulltext/S0960-9822(23)01512-9" target="_blank" rel="noreferrer noopener">Current Biology</a>.



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How does the brain create and retrieve memories? Scientists figured it out

Scientists have long wondered how the brain updates itself with...

The idea that extreme heat could one day cause a mass extinction and end the dominance of humans and other mammals might sound like something out of sci-fi movie.



Yet new findings indicate that the planet might face this crisis if continents fuse into one landmass. Some researchers say it could be the first extinction of its kind since the dinosaurs vanished.



In a recent study, investigators used powerful climate models to show how a future supercontinent, called Pangea Ultima, might alter global conditions. Projections suggest a much hotter and drier environment with limited options for survival.



The work appears in Nature Geoscience and was led by Dr. Alexander Farnsworth, a Senior Research Associate at the <a href="https://www.bristol.ac.uk/" target="_blank" rel="noreferrer noopener">University of Bristol</a>. His team examined tectonic plate movement, solar changes, and greenhouse gas levels.



<h2 class="wp-block-heading" id="h-pangea-ultima-the-next-supercontinent">Pangea Ultima - the next supercontinent</h2>



Geologists have long argued that <a href="https://www.earth.com/earthpedia-articles/supercontinents-101-pannotia-gondwana-and-pangea/" target="_blank" rel="noreferrer noopener">Earth’s continents</a> move gradually over time. Pangea Ultima is the name given to the hypothesized supercontinent that might emerge millions of years from now. 



If this happens, much of the terrain would sit far from oceanic cooling influences, a situation known as the continentality effect.



“The newly-emerged supercontinent would effectively create a triple whammy, comprising the continentality effect, hotter sun and more <a href="https://www.earth.com/news/possible-to-permanently-remove-co2-carbon-dioxide-from-atmosphere-water-storage/" target="_blank" rel="noreferrer noopener">CO₂ in the atmosphere</a>, of increasing heat for much of the planet,” Dr. Farnsworth explained.



<h2 class="wp-block-heading" id="h-three-drivers-of-human-extinction">Three drivers of human extinction</h2>



One factor is the expansive landmass itself, which traps regions in scorching interiors. 



Another is that the sun will brighten over time, delivering stronger radiation. Volcanic activity adds more carbon dioxide to the mix, further <a href="https://www.earth.com/news/climate-experts-predict-global-warming-will-far-exceed-paris-goals/" target="_blank" rel="noreferrer noopener">warming the atmosphere</a>.



“Widespread temperatures of between 40 to 50° Celsius (104 to 122° Fahrenheit), and even greater daily extremes, compounded by high levels of humidity, would ultimately seal our fate,” Dr. Farnsworth added. 



“Humans - along with many other species - would expire due to their <a href="https://www.earth.com/news/humans-have-a-lower-heat-tolerance-than-expected/" target="_blank" rel="noreferrer noopener">inability to shed this heat</a> through sweat, cooling their bodies.” 



With the sun also anticipated to emit about 2.5% more radiation and the supercontinent being located primarily in the hot, humid tropics, much of the planet could be facing temperatures of between 40 to 70°C (104 to 158°F).



<h2 class="wp-block-heading" id="h-impact-on-other-mammals">Impact on other mammals</h2>



Researchers note that mammals have historically endured shifts in temperature, sometimes by growing thicker coats in cold climates or relying on hibernation. 



Yet sustained heat is harder to escape, since sweating is essential for body cooling. As conditions climb, mammals cannot regulate heat for long without access to cooler refuges and reliable water sources.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2024/11/Pangea-Ultima_supercontinent_illustration_UBristol_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2024/11/Pangea-Ultima_supercontinent_illustration_UBristol_1s.webp" alt="Illustration showing the geography of today’s Earth and the projected geography of Earth in 250 million years, when all the continents converge into one supercontinent (Pangea Ultima). Credit: University of Bristol" class="wp-image-1965317"/></a><figcaption class="wp-element-caption">Illustration showing the geography of today’s Earth and the projected geography of Earth in 250 million years, when all the continents converge into one supercontinent (Pangea Ultima). Click image to enlarge. Credit: University of Bristol</figcaption></figure>



Study findings hint that only 8% to 16% of land on the future supercontinent would stay within a tolerable range. 



Dryness complicates matters by limiting <a href="https://www.earth.com/news/world-water-day-2025-preserving-glaciers-protecting-our-future/" target="_blank" rel="noreferrer noopener">water supplies</a> and reducing vegetation. With so much territory turning arid, the quest for food and hydration would become daunting.



<h2 class="wp-block-heading" id="h-humans-should-heed-extinction-warnings">Humans should heed extinction warnings</h2>



“It is vitally important not to lose sight of our current <a href="https://www.earth.com/news/climate-crisis-global-supply-chains-face-25-trillion-in-losses/" target="_blank" rel="noreferrer noopener">Climate Crisis</a>, which is a result of human emissions of greenhouse gases,” urged co-author Dr. Eunice Lo, Research Fellow in Climate Change and Health at the University of Bristol. 



“While we are predicting an uninhabitable planet in 250 million years, today we are already experiencing extreme heat that is detrimental to human health. This is why it is crucial to reach <a href="https://www.earth.com/news/limiting-global-warming-to-1-5c-is-almost-certainly-out-of-reach/" target="_blank" rel="noreferrer noopener">net-zero emissions</a> as soon as possible.”



Recent decades have seen rising temperatures that strain resources. Heat waves threaten crops, disrupt energy grids, and place communities at risk. 



Many call for faster <a href="https://www.earth.com/news/beef-industry-can-cut-emissions-by-30-with-sustainable-practices/" target="_blank" rel="noreferrer noopener">emission cuts</a> to prevent even harsher conditions. Some experts believe effective policies and public awareness could still temper the worst near-term damage.



<h2 class="wp-block-heading" id="h-future-carbon-dioxide-levels">Future carbon dioxide levels</h2>



Projections in the study used tectonic and ocean chemistry models to gauge carbon dioxide levels. 



Higher volcanic outgassing over the coming eons points to an increase from current readings to well above 600 parts per million. Such elevated concentrations would create conditions hostile to many organisms.



<a href="https://www.earth.com/news/2023-climate-change-report-record-high-temperatures-greenhouse-gases-sea-level-rise/" target="_blank" rel="noreferrer noopener">Greenhouse gases</a> would accumulate and trap more heat in the atmosphere. This feedback loop amplifies warming, making survival increasingly difficult on a planet with minimal oceanic influence.



“We think CO₂ could rise from around 400 parts per million (ppm) today to more than 600 ppm many millions of years in the future,” noted Professor Benjamin Mills at the <a href="https://www.leeds.ac.uk/" target="_blank" rel="noreferrer noopener">University of Leeds</a>. 



“Of course, this assumes that humans will stop burning fossil fuels, otherwise we will see those numbers much, much sooner.”



<h2 class="wp-block-heading" id="h-remembering-past-extinction-events">Remembering past extinction events</h2>



Many eras of Earth’s history ended in severe biodiversity loss. 



About 443 million years ago, marine habitats shrank during the <a href="https://www.earth.com/news/fossil-sue-keurbos-susanae-reveals-444-million-year-old-anatomy-of-ancient-arthropod/" target="_blank" rel="noreferrer noopener">Ordovician-Silurian Extinction</a>, removing roughly 85% of sea life. 



Near 360 million years ago, the <a href="https://www.earth.com/news/at-least-two-of-earths-mass-extinctions-caused-by-massive-supernova-explosions/" target="_blank" rel="noreferrer noopener">Late Devonian</a> wiped out up to 75% of species. Later came the Permian-Triassic Extinction about 252 million years ago, erasing over 90% of marine species and 70% on land.



Around 200 million years ago, massive eruptions drove the Triassic-Jurassic Extinction, cutting species by around half. 



Some 66 million years ago, an asteroid impact ended the non-avian dinosaurs in the <a href="https://www.earth.com/news/mammals-ground-dwellers-survived-the-asteroid-impact-that-killed-the-dinosaurs/" target="_blank" rel="noreferrer noopener">Cretaceous-Paleogene Extinction</a>, eliminating about 75% of all species.



<h2 class="wp-block-heading" id="h-human-extinction-and-exoplanets">Human extinction and exoplanets</h2>



This analysis also broadens how scientists evaluate exoplanets. If continents merge, planetary heat can spike, even if a world is inside a so-called habitable zone. 



Researchers think other planets might face analogous shifts, where tectonic movement and solar intensity escalate temperatures. Rotation rates and air chemistry may further affect habitability.



“This work also highlights that a world within the so-called ‘<a href="https://www.earth.com/news/study-expands-the-habitable-zone-where-we-may-find-alien-life/" target="_blank" rel="noreferrer noopener">habitable zone</a>’ of a solar system may not be the most hospitable for humans depending on whether the continents are dispersed, as we have today, or in one large supercontinent,” Dr. Farnsworth concluded. 



“Understanding these configurations can guide experts who look for environments that support life beyond Earth.”



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



Today, we already see the impact of climate stress on our resources and health. Scientists warn us that higher temperatures and more extreme weather events could become the norm if we fail to manage our emissions. 



While the prospect of a distant supercontinent meltdown might seem remote, it underscores the importance of taking meaningful steps now.



The full study was published in the journal&nbsp;<a href="https://www.nature.com/articles/s41561-023-01259-3" target="_blank" rel="noreferrer noopener">Nature Geoscience</a>.



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Study predicts how and when humans and mammals will face extinction

The idea that extreme heat could one day cause a...

A,Young,African-american,Man,Is,Meditating,In,A,Bright,,Minimalist

Recent insights suggest that reflective habits - like meditation and critical thinking - can help people embrace artificial intelligence without succumbing to its drawbacks. As AI weaves itself into daily life, balanced use becomes crucial.



Digital strategy expert Giulio Toscani has interviewed 150 AI specialists across 50 countries. He argues in his new book, <a href="https://www.taylorfrancis.com/books/mono/10.1201/9781003533160/augmented-giulio-toscani" target="_blank" rel="noreferrer noopener">Augmented: prAIority to Enhance Human Judgment through Data and AI</a>, that humans often operate on autopilot, craving instant gratification.



“The growing allure of AI lies in its powerful ability to cater to our desires, providing us with instant gratification whenever and however we want it,” he said.



“This is particularly appealing in an increasingly digital and fast-paced world where people often face isolation and boredom. However, this very convenience and responsiveness of AI also pose a risk - its addictive potential.”



<h2 class="wp-block-heading" id="h-managing-ai-s-addictive-potential">Managing AI’s addictive potential</h2>



Toscani warns that limited awareness of AI’s risks leads many to adopt new tools prematurely, exposing themselves to data privacy breaches, online harassment, and misinformation.



According to Toscani, it is essential to pause and reflect on how these interactions shape and are shaped by our actions to encourage a cultural shift towards valuing long-term thinking over immediate gratification.



Deliberate examination of AI’s role can guide more thoughtful choices. This reflective approach helps us understand the broader implications of <a href="https://www.earth.com/news/current-ai-systems-can-not-be-trusted-to-make-unbiased-decisions/" target="_blank" rel="noreferrer noopener">technology</a>, beyond immediate functionality and efficiency, noted Toscani.



"It allows us to consider how technology impacts our lives, relationships, and ethical considerations, guiding us toward more deliberate and informed decisions."



<h2 class="wp-block-heading" id="h-meditation-and-responsible-ai-use">Meditation and responsible AI use</h2>



Toscani, who has practiced Vipassana <a href="https://www.earth.com/news/meditation-slows-biological-aging-at-the-molecular-level/" target="_blank" rel="noreferrer noopener">meditation</a> at six 10-day silent retreats, sees it as a way to reflect on the responsible use of AI and become aware of one’s digital habits.



“This growing practice encourages individuals to critically assess their technological choices, considering the broader implications for themselves, their communities, and society at large."



“By fostering a culture of mindful reflection on how we interact with technology, meditation plays a crucial role in promoting responsible and ethical use. Emphasizing reflection helps us make more informed, deliberate decisions that enhance the positive impact of technology while mitigating its risks.”



Toscani noted that the cultural shift toward mindfulness encourages us to consider the broader implications of our technological choices, promoting a more responsible and humane relationship with the tools that shape our lives.



<h2 class="wp-block-heading" id="h-critical-thinking-in-action">Critical thinking in action</h2>



Toscani cautions against over-reliance on AI for vital cognitive tasks. He urges practices such as journaling, debate, and handwriting to maintain deep thinking.



“By consciously balancing the use of AI with the development and maintenance of our cognitive skills, we can harness the power of AI without sacrificing our intellectual autonomy."



He also mentioned that as we continue to integrate AI into our lives, we must remain vigilant about its impact on our cognitive processes, ensuring that we remain active participants in our own intellectual development.



<h2 class="wp-block-heading" id="h-using-ai-to-enhance-human-capabilities">Using AI to enhance human capabilities </h2>



Though challenges exist, Toscani calls AI a revolutionary tool in human history. Drawing from ancient philosophy, he proposes the concept of “prAIority,” a focus on data, AI systems, and human judgment underpinned by <a href="https://www.earth.com/news/human-robot-interaction-are-we-prepared-for-the-ethical-challenges/" target="_blank" rel="noreferrer noopener">ethics</a>.



This approach aims to preserve autonomy and trust, all while driving innovation. Moreover, he also advocates applying AI where it matters most, such as healthcare, education, creative fields, and complex decision-making.



“Through strategic prioritization, we can unlock the full potential of AI as a force for good, transforming our world and enriching the human experience in ways that were once unimaginable,” he explained.



“By thoughtfully selecting areas where AI can be most beneficial, we ensure that this powerful technology enhances human capabilities rather than disrupts them." 



<h2 class="wp-block-heading" id="h-keeping-technology-under-control">Keeping technology under control</h2>



Toscani also stated the primary goal is to use AI to augment human intelligence and creativity, enabling us to solve complex problems, innovate in ways previously unimaginable, and improve our overall <a href="https://www.earth.com/news/active-aging-physical-activity-has-a-direct-impact-on-life-quality/" target="_blank" rel="noreferrer noopener">quality of life</a>.



In a world where AI is rapidly evolving, reflection, meditation, and critical thinking help maintain autonomy. 



By examining our reliance on AI, we keep technology under our control rather than the other way around. This mindful balance lets us maximize AI’s benefits while safeguarding our judgment, creativity, and humanity.



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Why meditation and critical thinking matter in the age of AI

Recent insights suggest that reflective habits - like meditation and...

Dna,Molecule.,Medical,And,Heredity,Genetic,Health,Concept.,Technology,Science.

DNA repair is crucial for human well-being. This marcromolecule makes up our chromosomes and is present in our body cells. It carries a detailed code that enables us to make the proteins we need for healthy functioning, but this code can unravel without proper care.



A group of researchers has <a href="https://www.nature.com/articles/s41586-025-08815-4" target="_blank" rel="noreferrer noopener">investigated</a> how a network of repair genes keeps that code safe. <a href="https://mhs.biol.ethz.ch/research/corn.html" target="_blank" rel="noreferrer noopener">Jacob Corn</a>, Professor of Genome Biology at <a href="https://ethz.ch/en.html" target="_blank" rel="noreferrer noopener">ETH Zurich</a>, guided a segment of this effort.



<h2 class="wp-block-heading" id="h-everyday-cell-life-damages-dna">Everyday cell life damages DNA</h2>



Scientists have long recognized that routine cellular processes can harm our <a href="https://www.earth.com/news/dna-changes-supercharged-the-human-brain-but-at-a-cost/" target="_blank" rel="noreferrer noopener">genetic material</a>. Minor twists or breaks can stack up over time and threaten essential information.



“When people read about repairing genetic material, they often think of it being in response to exposure to toxins or radiation,” said Corn, adding that everyday pressures inside cells also lead to damage that demands constant attention.



Even basic cell division can introduce damage. Repetitive segments can become tangled, and random hits can cause cracks in the <a href="https://www.earth.com/news/quantum-computers-knots-dna-loops-and-the-future-of-genetic-modification/" target="_blank" rel="noreferrer noopener">DNA</a> structure.



Each time a cell copies the DNA blueprint, dozens of enzymes rush in to check for faults. They fix small errors before these morph into large-scale troubles.



Specialized DNA repair pathways handle distinct threats, from single-strand nicks to double-strand breaks. These coordinated strategies preserve the code through generations of cells.



<h2 class="wp-block-heading" id="h-repair-genes-patch-dna-damage">Repair genes patch DNA damage</h2>



Scientists have cataloged hundreds of genes that serve as repair tools. Different pathways work together to patch breaks or rearrange <a href="https://www.earth.com/news/hidden-chapter-in-human-evolution-revealed-through-genetics/" target="_blank" rel="noreferrer noopener">DNA</a> fragments that go astray.



Certain genes respond to specific chemical mishaps, while others assist in collecting lost DNA pieces. This efficiency stops mistakes from piling up inside our chromosomes, in the <a href="https://www.cancer.gov/publications/dictionaries/cancer-terms/def/nucleus" target="_blank" rel="noreferrer noopener">nucleus</a> of each cell.



Redundancy matters when something goes wrong, as this ensures that backup helpers are on call. This approach can save a cell from total breakdown. 



Researchers suggest that blocking one repair gene alone often does not produce a dramatic effect. Instead, targeting multiple genes at once can push damaged cells toward collapse.



These insights open fresh avenues for basic genetic science. They also prompt new methods of thinking about diseases that are linked to faulty repair.



<h2 class="wp-block-heading" id="h-cancer-cells-misuse-or-lose-repair-systems">Cancer cells misuse or lose repair systems</h2>



Cells that multiply too fast tend to experience extra glitches. <a href="https://www.science.org/doi/10.1126/science.1235122" target="_blank" rel="noreferrer noopener">Defects</a> in repair genes can give harmful cells a chance to run wild, as is seen in the development of cancer.



By pinpointing vulnerable spots in a cancer cell’s repair setup, therapies can strike in a precise way. This idea drives the concept of <a href="https://www.nature.com/articles/nrg.2017.47" target="_blank" rel="noreferrer noopener">synthetic lethality</a>, where hitting multiple weaknesses topples the cell.



Investigators see a path forward for <a href="https://www.nature.com/articles/nature10760" target="_blank" rel="noreferrer noopener">treatments</a> that exploit these hidden gaps in the defenses of cancer cells. Combinations of targeted drugs might trigger lethal damage in cells that already lack certain repair strengths.



Such tactics could leave healthy tissue less affected. Normal cells have intact DNA repair backups, so they stand a better chance of bouncing back.



Experts hope that mapping <a href="https://www.earth.com/news/subtle-dna-changes-shaped-human-brain-evolution/" target="_blank" rel="noreferrer noopener">DNA</a> repair interactions will guide clinicians. They envision a future where each patient’s tumor is profiled to reveal repair flaws that can then be blocked by targeted treatment.



<h2 class="wp-block-heading" id="h-onward-with-fresh-tools">Onward with fresh tools</h2>



Refined <a href="https://medlineplus.gov/genetics/understanding/genomicresearch/genomeediting/" target="_blank" rel="noreferrer noopener">gene-editing systems</a> make it easier to test which combinations of genes lead to meltdown in cancer cells. This knowledge could guide the design of safer drugs.



Organizations share their findings on public platforms, allowing scientists worldwide to examine the data. Collaborative efforts may speed up discoveries and reduce blind spots.



Basic research still relies on careful lab work to confirm which repair routes matter most for cell survival. Investigators piece together puzzle segments to see where the biggest vulnerabilities lie.



Leaders in the field want to push these insights into real therapies. They look beyond the common sources of <a href="https://www.earth.com/news/bacteria-and-imprint-new-era-dna-transformation/" target="_blank" rel="noreferrer noopener">DNA</a> harm and investigate subtle events that harm cells each day.



Progress in this area could improve how we handle stubborn tumors and <a href="https://www.healthdirect.gov.au/genetic-disorders" target="_blank" rel="noreferrer noopener">genetic disorders</a>. Creative approaches often emerge when researchers connect seemingly unrelated details.



<h2 class="wp-block-heading" id="h-treatments-target-dna-repair-weak-spots">Treatments target DNA repair weak spots</h2>



Researchers aim to refine their methods for scanning entire <a href="https://www.nature.com/scitable/definition/genome-43/" target="_blank" rel="noreferrer noopener">genomes</a>. They plan to automate searches for unusual patterns that signal hidden problems.



Some teams explore how to cut off cancer cells from vital repair options. Others check whether small molecule drugs can disrupt essential repair loops.



Governments and private funders take an interest in this type of <a href="https://www.genome.gov/about-genomics/fact-sheets/Genetic-Mapping-Fact-Sheet" target="_blank" rel="noreferrer noopener">genetic mapping</a>. They see the potential for targeted strategies that avoid harmful side effects.



Patient outcomes may improve if physicians can customize treatment based on a tumor’s repair <a href="https://medicover-genetics.com/our-genetic-tests/oncology/tumor-profile-cancer-panels/" target="_blank" rel="noreferrer noopener">profile</a>. That prospect has motivated clinical trials that examine how combined interventions affect cell survival.



Progress in this area depends on steady collaboration. Every fresh detail about our body's own repair networks can sharpen the tactics used against DNA-related diseases.



These breakthroughs could change how we handle medical conditions in the next decade. Ongoing projects will determine which combination of interventions truly shields our genetic code from lasting harm.



The study was published in <a href="https://www.nature.com/articles/s41586-025-08815-4" target="_blank" rel="noreferrer noopener">Nature</a>.



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Everyday DNA damage requires constant repair, and now we know how the body fixes it

DNA repair is crucial for human well-being. This marcromolecule makes...

Vitamin K may have a more significant role in brain function than expected, particularly as we age. Widely known for its role in blood clotting, this vitamin - contained in green veggies such as spinach, kale, and broccoli - could also guard memory and learning.



In a study from the Jean Mayer USDA Human Nutrition Research Center on Aging at <a href="https://www.tufts.edu/" target="_blank" rel="noreferrer noopener">Tufts University</a>, scientists explored how low vitamin K intake could affect the brain's ability to process information. 



The research was particularly focused on the hippocampus - an area that controls <a href="https://www.earth.com/news/secrets-of-learning-how-the-brain-stores-new-information/" target="_blank" rel="noreferrer noopener">learning</a> and memory.



<h2 class="wp-block-heading" id="h-the-brain-vitamin-k-connection">The brain-vitamin K connection</h2>



Using middle-aged rodents, the researchers observed how a vitamin K-deficient diet impacted brain function over six months. 



The team analyzed menaquinone-4, a form of vitamin K commonly found in brain tissue. Mice lacking this nutrient showed significant changes in behavior and brain structure.



“There is also research that indicates vitamin K contributes to brain function and that brain function declines during the aging process,” noted Tong Zheng, lead author of the study.



“Vitamin K seems to have a protective effect. Our research is trying to understand the underlying mechanism for that effect, so we might one day be able to target those mechanisms specifically.”



<h2 class="wp-block-heading" id="h-vitamin-k-deficiency-impacts-learning">Vitamin K deficiency impacts learning</h2>



To test <a href="https://www.earth.com/news/memory-isnt-only-stored-in-our-brains-other-cells-can-remember-too/" target="_blank" rel="noreferrer noopener">memory</a> and learning abilities, the researchers conducted behavioral assessments with the mice. One such task, the novel object recognition test, revealed that vitamin K-deficient mice struggled to distinguish familiar and new objects. This signaled a clear drop in memory.



In another test, the mice had to locate a hidden platform in a water pool. Again, those lacking vitamin K took noticeably longer to figure out the task. 



The results pointed toward a broader issue in how their brains processed and retained new information. Brain tissue analysis backed this up. The scientists found fewer new neurons in the hippocampus, particularly the dentate gyrus region.



“Neurogenesis is thought to play a critical role in learning and memory, and its impairment could directly contribute to the <a href="https://www.earth.com/news/colorful-foods-can-prevent-cognitive-decline/" target="_blank" rel="noreferrer noopener">cognitive decline</a> observed in the study,” explained Zheng.



<h2 class="wp-block-heading" id="h-inflammation-and-brain-aging">Inflammation and brain aging</h2>



Beyond fewer new brain cells, the team also discovered increased <a href="https://www.earth.com/news/even-mild-inflammation-can-majorly-damage-the-brain/" target="_blank" rel="noreferrer noopener">inflammation</a> in the vitamin K-deficient mice. They found more activated microglia - the immune cells of the brain. 



While these cells typically help maintain brain health, an overactive state can cause long-term inflammation. This kind of chronic inflammation is a known contributor to age-related cognitive issues and neurodegenerative diseases.



While the findings are compelling, the researchers are not advising people to rush to the supplement aisle. There are plenty of vitamin K-rich foods, such as green leafy vegetables like kale, collard greens, and Swiss chard – but also kiwi, asparagus, avocado, and blueberries.



“People need to eat a healthy diet. They need to eat their <a href="https://www.earth.com/news/fruits-vegetables-memory-loss-men/" target="_blank" rel="noreferrer noopener">vegetables</a>," said Sarah Booth, director of the research center and senior author of the study. 



<h2 class="wp-block-heading" id="h-improving-long-term-brain-health">Improving long-term brain health</h2>



Booth's team collaborates closely with scientists at Rush University Medical Center, who conduct observational studies in humans. Meanwhile, the Tufts researchers work with animal models to better understand the biology at play.



“We know that a healthy diet works and that people who don’t eat a healthy diet don’t live as long or do as well cognitively,” said Booth.



“By choreographing animal and human studies together, we can do a better job of improving brain health long-term by identifying and targeting specific mechanisms.”



<h2 class="wp-block-heading" id="h-eating-for-a-sharper-tomorrow">Eating for a sharper tomorrow</h2>



The study reinforces the idea that what we eat doesn’t just affect our bodies - but also our minds.



While vitamin K may not be the sole solution to preserving brain health, making leafy greens a regular part of your diet could be a smart, simple step toward better aging.



Nutrition is just one piece of the puzzle, but it’s a piece we can control. Focus on whole, unprocessed foods and plan meals to ensure you're getting various nutrients. 



Supporting your brain through diet now may help reduce the risk of cognitive decline later. And sometimes, small habits - like eating more vegetables - can lead to meaningful changes in how we age.



The full study was published in the journal <a href="https://linkinghub.elsevier.com/retrieve/pii/S0022316625000306" target="_blank" rel="noreferrer noopener">Journal of Nutrition</a>.



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Vitamin K protects the aging brain in many important ways

Vitamin K may have a more significant role in brain...

Young,Beautiful,Hispanic,Woman,Having,Video,Call,Communicate,With,Sign

For millions of deaf and hard-of-hearing people, using sign language to communicate in a world built around spoken words can be exhausting. 



Whether it’s ordering food, asking for directions, or taking part in a classroom discussion, barriers show up everywhere.



While interpreters and captioning services can help, they’re often limited, costly, or unavailable when most needed. 



As daily life becomes more digital, the need for smart tools that can translate sign language in real time is more urgent than ever.



That’s why researchers from Florida Atlantic University’s <a href="https://www.fau.edu/engineering/" target="_blank" rel="noreferrer noopener">College of Engineering and Computer Science</a> have created a new system that could change the way we think about accessibility.



They’ve developed a real-time American Sign Language (ASL) interpreter powered by <a href="https://www.earth.com/news/can-we-communicate-with-animals-using-artificial-intelligence/" target="_blank" rel="noreferrer noopener">artificial intelligence</a>. 



This system uses deep learning and hand-tracking to convert ASL gestures into written text, all using a regular webcam and off-the-shelf hardware.



<h2 class="wp-block-heading" id="h-recognizing-sign-language-is-tricky-for-machines">Recognizing sign language is tricky for machines</h2>



ASL relies on precise hand shapes and movements to represent letters, words, and phrases. But current recognition tools often miss the mark - especially when signs look alike.



For example, “A” and “T” or “M” and “N” can be hard to tell apart for machines. These tools also struggle in poor lighting, with motion blur, and with differences in hand shape or skin tone, all of which affect how accurate the machine interpretations are.



To solve these issues, the FAU team combined two powerful tools: YOLOv11 for object detection and MediaPipe for detailed hand tracking. 



Together, they allow the system to detect and classify ASL alphabet letters with an accuracy of 98.2% (mean Average Precision at 0.5). The entire process works in real time and with very little delay.



“What makes this system especially notable is that the entire recognition pipeline - from capturing the gesture to classifying it operates seamlessly in real time, regardless of varying lighting conditions or backgrounds,” said Bader Alsharif, lead author on the study.



“And all of this is achieved using standard, off-the-shelf hardware. This underscores the system’s practical potential as a highly accessible and scalable assistive technology, making it a viable solution for real-world applications.”



<h2 class="wp-block-heading" id="h-seeing-and-understanding-sign-language">Seeing and understanding sign language</h2>



At the center of the system is a basic webcam, which captures live video and turns it into digital frames. 



MediaPipe then pinpoints 21 key spots on each hand - fingertips, knuckles, and the wrist - to build a kind of skeleton map. These points help the system understand hand structure and motion.



YOLOv11 uses this skeletal data to match hand gestures accurately to ASL letters.



The researchers also built a massive dataset - 130,000 images strong - to train the model. These images include hands in a variety of lighting conditions, backgrounds, and angles.



This diversity helps the system learn how to generalize across different people and environments, thus reducing the chance of bias.



“This project is a great example of how cutting-edge AI can be applied to serve humanity,” said Imad Mahgoub, a co-author on the publication.



“By fusing deep learning with hand landmark detection, our team created a system that not only achieves high accuracy but also remains accessible and practical for everyday use. It’s a strong step toward inclusive <a href="https://www.earth.com/news/quantum-holograms-future-of-secure-messaging-encryption-internet/" target="_blank" rel="noreferrer noopener">communication technologies</a>.”



<h2 class="wp-block-heading" id="h-a-growing-need">A growing need</h2>



The deaf and hard-of-hearing community is large and diverse. 



In the U.S. alone, about 11 million people - roughly 3.6% of the population - are <a href="https://www.earth.com/news/implant-measures-hearing-quality-through-brain-waves/" target="_blank" rel="noreferrer noopener">deaf</a> or have significant <a href="https://www.earth.com/news/hearing-loss-linked-to-a-greater-risk-of-dementia/" target="_blank" rel="noreferrer noopener">hearing loss</a>. Around 37.5 million adults experience some level of hearing difficulty.



That’s a lot of people who could benefit from better communication tools.



“The significance of this research lies in its potential to transform communication for the deaf community by providing an AI-driven tool that translates American Sign Language gestures into text, enabling smoother interactions across education, workplaces, health care and social settings,” commented Mohammad Ilyas, co-author of the research study.



“By developing a robust and accessible ASL interpretation system, our study contributes to the advancement of assistive technologies to break down barriers for the deaf and hard-of-hearing population.”



<h2 class="wp-block-heading" id="h-helping-the-deaf-community-say-more">Helping the deaf community say more</h2>



While this new tool already shows strong results for recognizing the ASL alphabet, the team isn’t stopping there. They’re now working to expand the system to understand full ASL sentences. 



This would make communication even more natural and fluent, moving from spelling out words to sharing entire ideas.



“This research highlights the transformative power of AI-driven assistive technologies in empowering the deaf community,” said Stella Batalama, Dean of the Department of Electrical Engineering at FAU. 



“By bridging the communication gap through real-time ASL recognition, this system plays a key role in fostering a more inclusive society."



"It allows individuals with hearing impairments to interact more seamlessly with the world around them, whether they are introducing themselves, navigating their environment, or simply engaging in <a href="https://www.earth.com/news/one-daily-conversation-with-a-friend-can-boost-wellbeing/" target="_blank" rel="noreferrer noopener">everyday conversations</a>." 



This technology enhances accessibility and supports greater social integration, helping create a more connected and empathetic community for everyone.



With continued development, this AI-powered tool may soon become part of daily life, helping millions to communicate more freely - one gesture at a time.



The full study was published in the journal <a href="https://www.mdpi.com/1424-8220/25/7/2138" target="_blank" rel="noreferrer noopener">Sensors</a>.



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Remarkable new AI tech translates American Sign Language in real-time

For millions of deaf and hard-of-hearing people, using sign language...

Carbon dioxide has long been a huge source of concern for people who want cleaner air, cooler water, and a healthier planet. Many nations are working to slash emissions of this gas, but experts say that may not be enough.



This is where strategies like sucking <a href="https://www.earth.com/news/global-warming-is-accelerating-beyond-control-as-co2-levels-rise/" target="_blank" rel="noreferrer noopener">CO2</a> from the air and stashing it deep under the Earth's surface gain attention. 



This approach is now being investigated by <a href="https://marcodepaoli.com/contact/" target="_blank" rel="noreferrer noopener">Marco De Paoli</a> from the University of Twente (<a href="https://www.utwente.nl/en/" target="_blank" rel="noreferrer noopener">UT</a>) in Enschede, Netherlands, and the Institute of Fluid Mechanics and Heat Transfer at <a href="https://www.tuwien.at/en/" target="_blank" rel="noreferrer noopener">TU Wien</a>.



<h2 class="wp-block-heading" id="h-why-storing-co-2-underground-is-complex">Why storing CO2 underground is complex</h2>



CO2 does not simply vanish once injected below the surface of the Earth. It occupies spaces in underground rocks and mixes with groundwater, a process that turns out to be more intricate than it first sounds. 



Many scientists have wondered if it could creep back to the surface after decades.



“Pure CO2 has a lower density than water, but the situation changes when <a href="https://www.earth.com/news/natures-grip-on-co2-is-slipping-what-it-means-for-us-all/" target="_blank" rel="noreferrer noopener">CO2</a> is dissolved in water,” stated De Paoli. 



Numerical <a href="https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2025GL114804">experiments</a> on large computers suggest that once CO2 dissolves in water, the resulting liquid is denser than water alone. 



<h2 class="wp-block-heading" id="h-dense-carbon-water-sinks-and-stays-put">Dense carbon water sinks and stays put</h2>



<a href="https://fiveable.me/introduction-chemical-engineering/unit-5/fluid-statics/study-guide/MCni95hbDkArLJW3" target="_blank" rel="noreferrer noopener">Density</a> is crucial for how fluids behave underground. When carbon-rich water is heavier, it tends to move downward instead of floating back up towards the surface. 



This internal sinking motion creates layers of fluid that stay tucked away underground.



Those denser layers mean storage can be more than a temporary band-aid. 



Officials who track environmental tactics see this density-driven process as a real chance to keep <a href="https://www.earth.com/news/co2-emissions-reduction-20-percent-possible-only-2-percent-economic-loss/" target="_blank" rel="noreferrer noopener">CO2</a> locked beneath rock layers. This would help <a href="https://www.researchgate.net/publication/355807661_Leakage_Risk_Assessment_of_a_CO2_Storage_Site_A_Review" target="_blank" rel="noreferrer noopener">minimize leaks</a> that might compromise long-term climate goals.



<h2 class="wp-block-heading" id="h-only-some-places-can-store-carbon-safely">Only some places can store carbon safely</h2>



Not every location is a fit for CO2 storage. There must be a thick, relatively impermeable caprock above a porous layer that holds groundwater. 



A secure lid is vital to keep <a href="https://www.earth.com/news/global-co2-emissions-rise-as-nations-tackle-fossil-fuel-dependence/" target="_blank" rel="noreferrer noopener">CO2</a> in place until it fully dissolves and starts that downward migration.



“Such geological conditions are not that rare,” remarked De Paoli. Several sites already meet these criteria, including regions under the ocean floor. 



Experts point to defunct oil fields and <a href="https://igutek.scripts.mit.edu/terrascope/?page=saline" target="_blank" rel="noreferrer noopener">saline aquifers</a> as promising spots. 



<h2 class="wp-block-heading" id="h-rocks-may-help-or-hurt-carbon-storage">Rocks may help or hurt carbon storage</h2>



A large question is how the rock itself reacts once carbon-laden water sneaks through its tiny channels. 



Certain rocks can dissolve or shift chemically, creating new channels. Others stay intact and seal the carbon-laden water even more tightly.



Researchers are using <a href="https://www.sciencedirect.com/science/article/abs/pii/S0016236121020913?via%3Dihub" target="_blank" rel="noreferrer noopener">advanced techniques</a> to figure out if these chemical changes strengthen or weaken the rock structure. The goal is to avoid unpleasant surprises that might interfere with the permanent storage plan.



<h2 class="wp-block-heading" id="h-smart-ways-to-inject-carbon-water">Smart ways to inject carbon water</h2>



Engineers are eyeing ways to harness this behavior for cost-effective carbon capture. 



They want to design injection methods that send <a href="https://www.earth.com/news/co2-has-regulated-earths-climate-for-millions-of-years/" target="_blank" rel="noreferrer noopener">CO2</a> straight into the sweet spot, where it will meet and merge with groundwater. Then the heavier fluid will settle deeper, away from potential fractures.



Existing industry programs in places like the <a href="https://sequestration.mit.edu/tools/projects/sleipner.html" target="_blank" rel="noreferrer noopener">Sleipner Field</a> in the North Sea have already injected millions of tons of CO2. 



Long-running monitoring there indicates that, if done correctly, carbon stays put and shifts gradually into stable zones.



<h2 class="wp-block-heading" id="h-long-term-outlook">Long-term outlook</h2>



Once dissolved, carbon is far less likely to slip back to the air. The rocky overhang becomes less important once the heavy mixture has migrated downward. 



Even major tremors may not nudge the fluid back to the surface after it has sunk below the seal.



This safety aspect is a primary reason many scientists want to keep exploring permanent underground CO2 storage. 



Calculations suggest there are widespread opportunities to capture and hold significant amounts of carbon over time.



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



De Paoli has an ongoing project funded by the <a href="https://erc.europa.eu/homepage" target="_blank" rel="noreferrer noopener">European Research Council</a> that looks at the finer details of chemical reactions between CO2-rich water and the rocks. 



Early analysis points to possible boosts in how quickly the heavier fluid travels downward, though it varies from site to site.



These insights might help refine future carbon storage plans. If engineers know exactly how fluids mix at various depths, they can scale up designs with confidence, using data-driven methods rather than guesswork.



<h2 class="wp-block-heading" id="h-co2-water-and-climate-change">CO2, water, and climate change</h2>



No single solution will solve the climate puzzle. Reducing emissions, adopting clean energy, and changing the way we use resources are all still high priorities. But taking CO2 out of the air and locking it underground might be a valuable extra measure.



As more research surfaces, scientists in this field hope to give policymakers hard data on success rates and reliable design guidelines. That could boost confidence in any large-scale adoption of this strategy.



In the United States, carbon capture projects are moving forward in industrial hubs. Similar efforts are popping up worldwide, spurred by public and private funding. 



Research centers are joining forces to share knowledge about geology, fluid mechanics, and safe <a href="https://www.researchgate.net/publication/355807661_Leakage_Risk_Assessment_of_a_CO2_Storage_Site_A_Review" target="_blank" rel="noreferrer noopener">storage</a> methods.



It remains to be seen whether global capacity is enough to store billions of tons of CO2 each year. Studies aim to locate the best formations and ensure that the captured carbon never sees daylight again.



The study was published in <a href="https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2025GL114804" target="_blank" rel="noreferrer noopener">Geophysical Research Letters</a>.



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Is it possible to 'permanently' remove CO2 from the atmosphere? Science found a way

Carbon dioxide has long been a huge source of concern...

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



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



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



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



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



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



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



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



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



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



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

Is chocolate the next nutritional powerhouse?

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

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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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

Flu viruses are more flexible than expected

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



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



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



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



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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

Detecting mercury contamination with the tap of a finger

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



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



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



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



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



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



Video/ Image Credit: European Space Agency&nbsp;



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



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

Kainji Lake in north central Nigeria

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This specific project was headed up by two figures associated with the Swedish Museum of Natural History – professor Alexander Nemchin and Jeremy Bellucci. Put simply, the pair analyzed Big Bertha and found that the rock had a number of unusual features.

22. Unusual Features

However, it was quite some time before a study emerged which really painted a picture of Big Bertha’s significance. This finally happened, though, in 2019 – some 48 years after the rock was first discovered by Shepard. But the wait may well have been worth it for any scientists concerned with the study of the Moon.

22. Unusual Features

News coming your way