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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Eagle Nebula: Stars rise in collapsing clouds

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

Today's Image of the Day from the European Space Agency features the Cat's Eye Nebula (NGC 6543), located about 3,300 light-years from Earth in the constellation Draco.&nbsp;



The nebula's name comes from its eye-like appearance when viewed through a telescope. This particular image, which reveals the <a href="https://www.earth.com/news/horsehead-nebula-webb-telescope-captured-unprecedented-detail/" target="_blank" rel="noreferrer noopener">nebula</a> in stunning detail, was captured by the NASA/ESA Hubble Space Telescope.



<h2 class="wp-block-heading" id="h-complex-planetary-nebula">Complex planetary nebula </h2>



According to ESA, the Cat's Eye Nebula is one of the most complex planetary nebulae that has ever been discovered.



“A planetary nebula forms when Sun-like stars gently eject their outer gaseous layers to form bright nebulae with amazing twisted shapes," explained <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"Until recently, it was thought that shells around planetary nebulae were a rare phenomenon. However, astronomers have instead shown that these rings are likely to be the rule rather than the exception."



<h2 class="wp-block-heading" id="h-appearance-of-the-cat-s-eye-nebula-nbsp">Appearance of the Cat's Eye Nebula&nbsp;</h2>



The central focus of the Cat's Eye is a hot, dying star that has shed its outer layers to form the <a href="https://www.earth.com/news/dragons-egg-nebula-is-a-truly-stunning-sight-to-behold/" target="_blank" rel="noreferrer noopener">nebula</a>. It is surrounded by concentric gas shells, jets of high-speed gas, and unusual shock-induced knots of gas.



“Although the rings may be the key to explaining the final ‘gasp’ of the dying central star, the mystery behind the Cat’s Eye Nebula’s nested ‘Russian doll’ structure remains largely unsolved,” noted ESA.



<h2 class="wp-block-heading" id="h-rings-around-the-cat-s-eye">Rings around the cat’s eye</h2>



“This image, taken with Hubble's Advanced Camera for Surveys (ACS), reveals the full pattern of eleven or more concentric rings, or shells, around the Cat’s Eye. Each ‘ring’ is actually the edge of a spherical bubble seen projected onto the sky - which is why it appears bright along its outer edge.”



According to ESA, observations suggest that the star ejected its mass in a series of pulses at 1,500-year intervals. “These convulsions created dust shells that each contains as much mass as all of the planets in our solar system combined.”



Several explanations have been proposed for this phenomenon, including cycles of magnetic activity similar to our Sun's sunspot cycle, the influence of companion stars orbiting the <a href="https://www.earth.com/news/dying-stars-may-be-a-source-of-gravitational-waves/" target="_blank" rel="noreferrer noopener">dying star</a>, or stellar pulsations.&nbsp;



Another theory suggests that the material is ejected smoothly from the star, with the rings forming later due to the creation of waves in the outflowing material.



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



<a href="https://www.earth.com/news/extrasolar-ocean-planet-discovered-in-the-draco-constellation/" target="_blank" rel="noreferrer noopener">Draco</a> is a constellation in the northern sky that represents a dragon. It's one of the largest constellations, winding between the Big and Little Dippers.&nbsp;



In Greek mythology, Draco is often identified as the dragon Ladon, who guarded the golden apples in the garden of the Hesperides.



Draco is a circumpolar constellation for most northern hemisphere observers, meaning it never sets below the horizon and can be seen all year round.



<h2 class="wp-block-heading" id="h-famous-planetary-nebulae">Famous planetary nebulae </h2>



Planetary nebulae are some of the most beautiful and intriguing objects in the universe.&nbsp;



One of the most famous is the Ring Nebula, or M57, located in the constellation Lyra. This nebula is renowned for its nearly perfect ring shape, which is the result of a dying star shedding its outer layers.&nbsp;



Another well-known planetary nebula is the Helix Nebula, or NGC 7293, often referred to as the "Eye of God" due to its eye-like appearance. The Helix Nebula is one of the closest planetary nebulae to Earth, making it a popular target for amateur astronomers.&nbsp;



The Dumbbell Nebula, or M27, in the constellation Vulpecula, is another striking example. It is named for its resemblance to a dumbbell and is notable for being the first planetary nebula ever discovered, by Charles Messier in 1764.&nbsp;



The Butterfly Nebula, or NGC 6302, is located in the constellation Scorpius. Its name comes from its distinctive bipolar structure, resembling the wings of a butterfly. The nebula's central star is one of the hottest known, with a surface temperature of around 250,000 degrees Celsius.&nbsp;



The Eskimo Nebula, or NGC 2392, in the constellation Gemini, is known for its resemblance to a face surrounded by a fur parka, which gives it its name. Its intricate structure, including filaments and bubble-like shapes, makes it a fascinating object of study.&nbsp;



These nebulae not only captivate us with their beauty but also provide valuable insights into the life cycles of stars and the processes that shape our galaxy.



Image Credit: NASA/ESA Hubble Space Telescope



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Cat's Eye Nebula in the constellation Draco

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



“A photo taken in 2015 during space station Expedition 42 captured the lake’s remaining waters and wetlands in dark green, blue, and brown, contrasting with the sandy shades of the surrounding land.” 



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA Earth Observatory&nbsp;



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Lake Chad: A vanishing lifeline in Central Africa

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

Today's Image of the Day from the European Space Agency features 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/">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/">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/">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/">universe</a> might have looked like.



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



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



Image Credit: ESA



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Ghostly galaxy in the constellation Eridanus

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Young, massive stars in the Triangulum Galaxy

Earth is unusually lucky: its global magnetic field deflects harmful charged particles from the Sun and deep space, shielding the atmosphere and life at the surface. 



By contrast, cosmic radiation constantly batters worlds like Mars, which lack a comparable shield.



For decades, geophysicists have explained Earth’s <a href="https://www.earth.com/news/magnetism-at-earths-core-simulations-offer-breakthrough-insights/">magnetism</a> with the dynamo theory. As the planet slowly cools, molten iron-nickel in the outer core circulates in vast convection currents. 



Earth’s rotation twists these flows into helical, screw-like patterns. Moving metal generates electric currents, and those currents, in turn, generate the magnetic field.



There has been a nagging problem, though. Early in Earth’s history, before the <a href="https://www.earth.com/news/earths-inner-core-proven-to-be-rapidly-changing-and-now-rotating-backwards/">inner core</a> crystallized (roughly a billion years ago), the core was entirely liquid. Could the geodynamo have operated back then without the extra energy sources and structure provided by a solid inner core?



<h2 class="wp-block-heading" id="h-magnetism-without-a-solid-core">Magnetism without a solid core</h2>



A team of three geophysicists from <a href="https://ethz.ch/en.html">ETH Zurich</a> and the <a href="https://www.sustech.edu.cn/en/">Southern University of Science and Technology</a> (SUSTech) in China, built a new computer model of the core that shows a completely liquid core could have generated a stable magnetic field in much the same way it does today.



To get there, the researchers tackled a long-standing modeling hurdle: the influence of viscosity - the internal “thickness” or resistance to flow - on the simulated core.



In the real core, viscosity is believed to be extremely small. Yet most numerical models must exaggerate it for computational stability, potentially skewing the physics.



Using high-performance computing (including runs on the Piz Daint supercomputer at the <a href="https://www.cscs.ch/" target="_blank" rel="noreferrer noopener">Swiss National Supercomputing Center</a> in Lugano), the team simulated the correct physical regime where viscosity becomes negligible for the dynamo.



The result: a robust, self-sustaining magnetic field can emerge even when the core is fully molten. “Until now, no one has ever managed to perform such calculations under these correct physical conditions,” said lead author Yufeng Lin.



<h2 class="wp-block-heading" id="h-magnetic-field-no-inner-core">Magnetic field, no inner core</h2>



In the model, the same core ingredients that drive today’s dynamo - buoyancy-driven convection and the twisting effect of rotation - were sufficient to organize flows and magnetic fields even in the absence of a solid inner core.



By minimizing viscosity to effectively “get out of the way” of the physics, the team reproduced a realistic dynamo regime. In this regime, microscopic fluid resistance doesn’t control the outcome - large-scale convection and rotation do the heavy lifting.



That means the early Earth could plausibly have sustained a magnetic shield long before inner-core growth added extra energy from crystallization.



This advances a key idea: the geodynamo is surprisingly resilient. A solid core isn’t required - just the right heat loss, composition, and rotation to drive and organize metal flows.



<h2 class="wp-block-heading" id="h-rethinking-early-earth-s-defenses">Rethinking early Earth’s defenses</h2>



“This finding helps us to better understand the history of the Earth’s magnetic field and is useful in interpreting data from the geological past,” said co-author Andy Jackson, a professor of geophysics at ETH Zurich.



If magnetism arose with a liquid core, Earth’s protective shield may have formed earlier and lasted longer than thought. That, in turn, reframes how we think about early habitability.



A magnetic umbrella blocking high-energy radiation would have helped preserve the atmosphere and supported the conditions under which life could emerge and evolve.



Because the approach captures the essential physics of a low-viscosity dynamo, it could help scientists probe magnetic fields elsewhere. These include the Sun’s sprawling magnetism and the intense fields of Jupiter and <a href="https://www.earth.com/news/saturns-rings-beautiful-iconic-will-disappear-this-weekend-ring-plane-crossing/">Saturn</a>. 



Lower-viscosity models let scientists test how composition, rotation, and cooling shape magnetism across the solar system.



<h2 class="wp-block-heading" id="h-magnetism-protects-technology">Magnetism protects technology</h2>



Modern civilization quietly depends on Earth’s magnetic field. It safeguards satellites and power grids from space weather, stabilizes navigation, and underpins countless technologies.



“It is therefore important to understand how the magnetic field is generated, how it changes over time, and what mechanisms maintain it,” Jackson noted. “If we understand how the magnetic field is generated, we can predict its future development.”



Earth’s field has flipped polarity thousands of times, and in recent decades the magnetic north pole has migrated rapidly toward geographic north. Understanding the dynamo’s resilience helps scientists predict future magnetic shifts, from gradual drifts to full reversals.



<h2 class="wp-block-heading" id="h-a-tougher-shield-than-expected">A tougher shield than expected</h2>



By refining core simulations, scientists show Earth’s magnetic shield could ignite without a solid inner core. A fully molten, vigorously convecting, rapidly rotating core would have done the job.



That insight tightens our picture of early Earth, strengthens links between biodiversity and a protective <a href="https://www.earth.com/earthpedia-articles/earths-magnetic-field-origin-structure-and-impact-on-humanity/">magnetosphere</a>, and equips researchers to explore magnetic lifecycles on other worlds. 



It also offers a firmer foundation for anticipating how our planet’s magnetic shield might evolve in the centuries to come.



The study is published in the journal <a href="https://www.nature.com/articles/s41586-025-09334-y" target="_blank" rel="noreferrer noopener">Nature</a>.



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How Earth’s ancient magnetic shield may have sparked life

Earth is unusually lucky: its global magnetic field deflects harmful...

When clinicians talk to patients about preventing heart disease, they typically describe risk in dry percentages such as “eight out of 100 people like you may have a heart attack in the next decade.” Many Americans find that hard to grasp - and the numbers do not always move them to action.



A research team at Northwestern University <a href="https://www.feinberg.northwestern.edu/index.html">Feinberg School of Medicine</a> thinks there is a clearer, more motivating way to translate cardiovascular danger: tell people the age of their heart.



In a new study, epidemiologist Dr. Sadiya Khan and colleagues introduce an online calculator that converts standard health information - blood pressure, cholesterol, smoking status, and diabetes - into a single “heart age.” 



The metric is anchored to the American Heart Association’s new <a href="https://professional.heart.org/en/guidelines-and-statements/prevent-calculator%C3%B9" target="_blank" rel="noreferrer noopener">PREVENT equations</a>, which Khan also helped develop.



“We hope this tool helps doctors and patients discuss risk for heart disease more effectively so we can better inform what therapies can prevent <a href="https://www.earth.com/news/subtle-warning-signs-what-a-heart-attack-really-feels-like/">heart attacks</a>, stroke, or heart-failure events from ever happening,” Khan said.



<h2 class="wp-block-heading" id="h-testing-heart-age-globally">Testing "heart age" globally</h2>



The premise is intuitive: if laboratory results and lifestyle factors give you the cardiovascular profile of an older person, you probably need to rethink prevention. Conversely, if your heart age matches or beats your birth certificate, you might be on track.



To validate their calculator, Khan’s team mined data from the National Health and Nutrition Examination Survey (<a href="https://www.cdc.gov/nchs/nhanes/index.html" target="_blank" rel="noreferrer noopener">NHANES</a>), a rolling study that measures the health of the U.S. population.



They focused on 14,000 adults aged 30 to 79 who had never been diagnosed with heart disease. For each person, they calculated chronological age and heart age, then compared the two.



The patterns were sobering. Across the board, Americans carried older hearts than their birthdays would suggest. Women averaged a heart age of 55.4 despite being only 51.3 years old. 



The gap was wider for men: an average heart age of 56.7 versus an actual age of 49.7 - roughly seven extra “cardiac birthdays.”



<h2 class="wp-block-heading" id="h-race-and-income-age-hearts">Race and income age hearts</h2>



The researchers drilled deeper into the data to see how these gaps varied by education, income, and race or ethnicity. These factors are known to track with <a href="https://www.earth.com/news/heart-disease-remains-the-leading-cause-of-death-worldwide/">cardiovascular outcomes</a>.



Men with no more than a high-school education showed the greatest disconnect: almost one-third possessed hearts at least a decade older than their bodies.



Racial and ethnic contrasts were stark as well. Among men, Black participants had a heart age 8.5 years older than their chronological age. Hispanic men trailed at 7.9 years, followed by Asian men at 6.7 and white men at 6.4.



Women showed similar but smaller gaps. Black women had the oldest hearts relative to their age (a 6.2-year difference), while Asian women had the youngest (2.8 years).



These numbers, the authors argue, reveal how structural forces - access to health care, exposure to <a href="https://www.earth.com/news/chronic-stress-disrupts-gut-bacteria-and-fuels-cancer-progression/">chronic stress</a>, the cost of nutritious food - literally age the heart faster in some communities than others.



<h2 class="wp-block-heading" id="h-risk-that-feels-personal">Risk that feels personal</h2>



<a href="https://my.clevelandclinic.org/health/diseases/21493-cardiovascular-disease" target="_blank" rel="noreferrer noopener">Cardiovascular disease</a> has remained the nation’s leading cause of death for more than a century, even in the face of better medications and public-health campaigns against <a href="https://www.earth.com/news/smoking-related-deaths-will-surge-by-2030/">smoking</a>.



A key reason, Khan said, is that millions of people who would benefit from preventive therapies never start them - or start too late. She believes the new heart-age tool can turn abstract percentages into something people feel viscerally.



“Many people who should be on medicine to lower their risk for heart attack, <a href="https://www.earth.com/news/stroke-risk-is-elevated-by-air-pollution-and-traffic-noise/">stroke</a>, or heart failure are not on these medications,” Khan explained.



“We hope this new heart-age calculator will help support discussions about prevention and ultimately improve health for all people.”



The idea draws on behavioral research showing that vivid, easily understood messages spur action. 



A person who hears their heart is “ten years older” may grasp the urgency of lowering <a href="https://www.earth.com/news/scientists-identify-minimum-amount-of-physical-activity-needed-to-prevent-high-blood-pressure/">blood pressure</a>, quitting cigarettes, or beginning statin therapy. They may respond more readily than someone handed a 10 percent risk score.



<h2 class="wp-block-heading" id="h-heart-aging-tool-with-limits">Heart aging tool, with limits</h2>



The online tool, available for free, asks for five inputs: age, sex, total cholesterol, <a href="https://medlineplus.gov/hdlthegoodcholesterol.html" target="_blank" rel="noreferrer noopener">HDL</a> (“good”) cholesterol, systolic blood pressure, and whether the user smokes or has diabetes. With one click it produces a heart age and a brief explanation.



Khan’s team is quick to add caveats. The calculator is not a substitute for professional medical advice. Its equations are built on large-population averages, but individual factors - such as family history, kidney disease, or inflammatory conditions - can raise or lower risk outside the scope of the tool. 



Users should discuss results with a clinician before changing medications.



To ensure clinicians embrace the approach, the researchers are planning follow-up studies that track whether framing risk as age improves adherence to <a href="https://www.earth.com/news/scientists-identify-minimum-amount-of-physical-activity-needed-to-prevent-high-blood-pressure/">blood-pressure</a> drugs, statins, or lifestyle programs. They also aim to see whether it reduces heart attacks and strokes over time.



<h2 class="wp-block-heading" id="h-getting-through-to-young-adults">Getting through to young adults</h2>



One finding leapt out of the NHANES analysis: people in their thirties and forties often carried heart ages ten or more years beyond their chronological age. 



Yet they rarely meet intensity thresholds for preventive medications under current guidelines. Khan hopes the metric will spotlight hidden risk among younger adults who still feel invincible.



“The important thing is that we have very good options available in our toolbox to help slow that aging down if we can identify it,” she said. “This may be even more important in younger people who don’t often think about their risk for heart disease.”



<h2 class="wp-block-heading" id="h-why-heart-age-stats-matter">Why "heart age" stats matter</h2>



The heart-age calculator could also equip public-health agencies and employers to tailor interventions. 



Communities where the average heart age dwarfs chronological age might benefit from subsidized blood-pressure screenings, mobile clinics, or healthier food outlets.



Public health campaigns and community-based programs can emphasize the importance and availability of fast walking to improve health outcomes. 



They can also provide resources and support to facilitate increased fast walking within all communities.



Khan echoes that spirit for heart-age awareness. By translating risk into an easy-to-grasp figure, the team hopes to close gaps in prevention and push heart disease - long the country’s top killer - down the leaderboard at last.



The study is published in the journal <a href="https://jamanetwork.com/journals/jamacardiology/article-abstract/2836740">JAMA Cardio</a><a href="https://jamanetwork.com/journals/jamacardiology/article-abstract/2836740" target="_blank" rel="noreferrer noopener">l</a><a href="https://jamanetwork.com/journals/jamacardiology/article-abstract/2836740">ogy</a>.



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Scientists invent new tool that determines your 'heart age' as compared to your actual age

When clinicians talk to patients about preventing heart disease, they...

For many people online gaming is a harmless escape – a chance to unwind with friends, trade tips on strategy, and watch favorite streamers test new releases.



Yet a new study suggests that the same vibrant, hyper-connected space has become fertile ground for extremist recruiters. They see voice chat, livestreams, and in-game banter as open doors to fresh audiences.



<h2 class="wp-block-heading" id="h-gaming-platforms-fly-under-the-radar">Gaming platforms fly under the radar</h2>



Over the past decade, legislators have poured energy into policing <a href="https://www.earth.com/news/social-media-pressure-is-straining-teen-friendships/">social media</a> platforms like Facebook, X, TikTok, and YouTube. 



By comparison, gaming-adjacent platforms such as Discord, Steam communities, or Twitch “have largely flown under the radar, while at the same time becoming digital playgrounds for extremists to exploit,” said lead author William Allchorn from Anglia Ruskin University’s <a href="https://www.aru.ac.uk/international-policing-and-public-protection-research-institute" target="_blank" rel="noreferrer noopener">International Policing and Public Protection Research Institute</a>.



These services enable real-time chat, meme sharing, and private voice channels - making moderation especially difficult. The research team – Allchorn and senior fellow Elisa Orofino – spoke with content moderators, tech-industry specialists, and practitioners who work on preventing violent extremism.



Interviewees repeatedly described a funneling process: a user first encounters edgy jokes or borderline rhetoric on mainstream services, then an extremist invites them to a more lightly policed space tied to gaming culture.



“That’s where you have matchmaking. It’s where you can build quick rapport with people,” one participant said. “But that’s the stuff that very quickly moves to adjacent platforms, where there’s sort of less monitoring.”



<h2 class="wp-block-heading" id="h-extremist-messages-flood-gaming-platforms">Extremist messages flood gaming platforms</h2>



According to the study, the most common <a href="https://www.earth.com/news/why-people-believe-they-are-right-even-when-theyre-wrong/">ideology</a> circulating in these spaces is far-right extremism – white-supremacist propaganda, neo-Nazi symbols, Holocaust denial, and an undercurrent of misogyny and anti-LGBTQ rhetoric.



Islamist material appears too, though less frequently, and moderators also reported “extremist-adjacent” content that glorifies school shootings or promotes conspiracy theories such as QAnon. 



All of it violates platform terms of service, yet often evades detection because the language is coded or hidden behind memes.



Hyper-masculine titles – first-person shooters or combat games that prize aggression, quick reflexes, and leaderboards – offer particularly welcoming environments.



Newcomers can slip into a team channel with strangers, bond over shared tactics, then encounter racist or antisemitic slurs delivered as “jokes.” If a young player laughs along, recruiters test deeper waters. They may share links to fringe forums or private Discord servers where rhetoric becomes more explicit.



<h2 class="wp-block-heading" id="h-moderation-systems-overwhelmed">Moderation systems overwhelmed</h2>



Most gaming companies rely on a mix of automated filters and volunteer or lightly paid moderators. Interviewees told Allchorn and Orofino they feel overwhelmed.



In-game voice chat lacks moderation, while text channels flood with slang and sarcasm that overwhelm AI filters. 



A phrase like “I’m going to kill you” can be normal trash talk during a match but a genuine threat in a different context. Many users don’t know how to report extremist content, and those who do often feel their reports are ignored.



Moderators themselves expressed frustration at “inconsistent enforcement policies” and the heavy burden of deciding when to escalate a user to law enforcement.



Meanwhile, extremists exchange tips on how to dodge bans. These include using numbers or symbols in slurs and encoding messages with historical references or Nordic runes.



<h2 class="wp-block-heading" id="h-younger-gamers-in-the-crosshairs">Younger gamers in the crosshairs</h2>



A recurrent anxiety among professionals interviewed was the vulnerability of minors. Livestreamers who weave extremist talking points into entertaining gameplay accrue followers in the thousands; teenage viewers may tune in daily, forming parasocial bonds. 



Once the streamer invites them to a private server, those young fans are isolated from counter-speech.



Yet parents and teachers rarely recognize gaming platforms as potential vectors of radicalization. The authors argue that digital literacy campaigns must expand beyond traditional social media to cover the unique cultures of gaming.



<h2 class="wp-block-heading" id="h-solutions-span-tech-and-parenting">Solutions span tech and parenting</h2>



Allchorn believes decisive action is possible. “Strengthening moderation systems, both <a href="https://www.earth.com/news/ai-is-taking-scientific-discovery-from-decades-to-minutes/">AI</a> and human, is essential,” he said, but technologies must be paired with clearer platform rules that target content that is harmful but technically lawful.



The paper urges companies to invest in symbol libraries that evolve as extremist language shifts, to give moderators rapid-response channels to local police, and to provide transparent feedback loops when users report violations.



Law enforcement agencies also need to learn how <a href="https://www.earth.com/news/disaster-subculture-helps-people-cope-on-the-frontline-of-the-climate-crisis/">gaming subcultures</a> operate so they don’t dismiss genuine threats as mere smack talk. Educators and parents can play a role by discussing with children why hateful messages spread and by encouraging reporting mechanisms within games.



Ultimately, the study paints gaming platforms as a double-edged sword. They build global community, yet also allow fringe movements to thrive unnoticed.



“These gaming-adjacent platforms offer extremists direct access to large, often young and impressionable audiences,” Allchorn warned. 



Recognizing the phenomenon and naming its tactics is the first step toward keeping virtual playgrounds safe for play rather than propaganda.



The study is published in the journal <a href="https://www.frontiersin.org/journals/psychology/articles/10.3389/fpsyg.2025.1537460/full" target="_blank" rel="noreferrer noopener">Frontiers in Psychology</a>.



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Extremists are using gaming platforms to recruit young followers

For many people online gaming is a harmless escape –...

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