https://www.sciencedaily.com/news/space_time/solar_flare/ Latest research news on solar flares, the solar cycle, geomagnetic storms and more. en-us Tue, 21 Apr 2026 00:20:55 EDT Tue, 21 Apr 2026 00:20:55 EDT 60 https://www.sciencedaily.com/images/scidaily-logo-rss.png https://www.sciencedaily.com/news/space_time/solar_flare/ For more science news, visit ScienceDaily. https://www.sciencedaily.com/releases/2026/04/260417224457.htm As the Moon swallowed the Sun during the April 8, 2024, total solar eclipse, something remarkable happened on the ground—cities went eerily quiet. Scientists analyzing seismic data found that human-generated vibrations, usually caused by traffic, construction, and daily activity, dropped sharply during totality. The effect was so pronounced that it created a clear “seismic hush” across urban areas directly in the eclipse’s path, before quickly rebounding afterward. Sat, 18 Apr 2026 00:18:52 EDT https://www.sciencedaily.com/releases/2026/04/260417224457.htm https://www.sciencedaily.com/releases/2026/04/260409101101.htm A mysterious glow of gamma rays at the center of the Milky Way has long hinted at dark matter, but the lack of similar signals in smaller dwarf galaxies has cast doubt on that idea. Now, researchers propose a bold twist: dark matter might not be a single particle at all, but a mix of two different types that must interact with each other to produce detectable signals. Fri, 10 Apr 2026 08:34:50 EDT https://www.sciencedaily.com/releases/2026/04/260409101101.htm https://www.sciencedaily.com/releases/2026/04/260407193906.htm A bizarre, record-breaking neutrino detected in 2023 may have originated from an exploding primordial black hole—a relic from the early universe. Scientists suggest these black holes could carry a mysterious “dark charge,” causing rare but powerful bursts of energy that current detectors might occasionally catch. This could explain why only one experiment saw the event. The theory also opens the door to discovering entirely new particles and possibly uncovering the nature of dark matter. Wed, 08 Apr 2026 02:52:25 EDT https://www.sciencedaily.com/releases/2026/04/260407193906.htm https://www.sciencedaily.com/releases/2026/03/260326075618.htm Scientists have uncovered a surprising way to study the harsh space weather around young M dwarf stars. Mysterious dips in starlight turned out to be massive rings of plasma swirling in the stars’ magnetic fields. These structures act like built-in space weather monitors, revealing how energetic particles affect nearby planets. The findings could reshape how we think about whether planets around these common stars can survive—or even host life. Fri, 27 Mar 2026 04:53:17 EDT https://www.sciencedaily.com/releases/2026/03/260326075618.htm https://www.sciencedaily.com/releases/2026/03/260325041723.htm A star you can see with the naked eye has kept astronomers guessing for decades with its unusually powerful X-rays. Now, thanks to highly precise observations from Japan’s XRISM space telescope, scientists have finally uncovered the source: a hidden white dwarf companion pulling in material and generating extreme heat. This discovery not only solves a 50-year-old mystery surrounding Gamma Cassiopeiae, but also confirms the existence of a long-predicted type of binary star system. Wed, 25 Mar 2026 04:51:37 EDT https://www.sciencedaily.com/releases/2026/03/260325041723.htm https://www.sciencedaily.com/releases/2026/03/260314030452.htm Mars didn’t always look like the barren world we see today. Over billions of years, the Sun’s solar wind stripped away much of its atmosphere, helping transform it from a warmer, wetter planet into a frozen desert. NASA’s twin-spacecraft ESCAPADE mission aims to watch this process in action by measuring how the solar wind interacts with Mars’ fragile magnetic environment. The findings could reveal how Mars lost its habitability—and help prepare humans for future missions there. Sat, 14 Mar 2026 03:04:52 EDT https://www.sciencedaily.com/releases/2026/03/260314030452.htm https://www.sciencedaily.com/releases/2026/02/260222085206.htm Far beyond Neptune, in the frozen depths of the Kuiper Belt, many ancient objects oddly resemble giant snowmen made of ice and rock. For years, scientists wondered how these delicate two-lobed shapes could form without violent collisions tearing them apart. Now researchers at Michigan State University have recreated the process in a powerful new simulation, showing that simple gravitational collapse can naturally produce these cosmic “snowmen.” Mon, 23 Feb 2026 02:47:10 EST https://www.sciencedaily.com/releases/2026/02/260222085206.htm https://www.sciencedaily.com/releases/2026/02/260206012206.htm Astronomers propose that an ultra-dense clump of exotic dark matter could be masquerading as the powerful object thought to anchor our galaxy, explaining both the blistering speeds of stars near the center and the slower, graceful rotation of material far beyond. This dark matter structure would have a compact core that pulls on nearby stars like a black hole, surrounded by a broad halo shaping the galaxy’s outer motion. Sat, 07 Feb 2026 11:26:18 EST https://www.sciencedaily.com/releases/2026/02/260206012206.htm https://www.sciencedaily.com/releases/2026/02/260203020205.htm Astronomers have produced the most detailed map yet of dark matter, revealing the invisible framework that shaped the Universe long before stars and galaxies formed. Using powerful new observations from NASA’s James Webb Space Telescope, the research shows how dark matter gathered ordinary matter into dense regions, setting the stage for galaxies like the Milky Way and eventually planets like Earth. Tue, 03 Feb 2026 03:48:13 EST https://www.sciencedaily.com/releases/2026/02/260203020205.htm https://www.sciencedaily.com/releases/2026/01/260128075355.htm JWST has revealed a strange early universe filled with ultra-bright “blue monster” galaxies, mysterious “little red dots,” and black holes that seem far too massive for their age. A new study proposes that dark stars—hypothetical stars powered by dark matter—could tie all these surprises together. These exotic objects may have grown huge very quickly, lighting up the early cosmos and planting the seeds of supermassive black holes. Wed, 28 Jan 2026 10:05:20 EST https://www.sciencedaily.com/releases/2026/01/260128075355.htm https://www.sciencedaily.com/releases/2026/01/260127112135.htm A repeating fast radio burst has just given up one of its biggest secrets. Long-term observations revealed a rare signal flare caused by plasma likely ejected from a nearby companion star. This shows the burst source isn’t alone, but part of a binary system. The finding strengthens the case that magnetars interacting with stellar companions can generate repeating cosmic flashes. Tue, 27 Jan 2026 11:21:35 EST https://www.sciencedaily.com/releases/2026/01/260127112135.htm https://www.sciencedaily.com/releases/2026/01/260124003816.htm Astronomers have spotted a rare, rule-breaking quasar in the early Universe that appears to be growing its central black hole at an astonishing pace. Observations show the black hole is devouring matter far faster than theory says it should—about 13 times the usual “speed limit”—while simultaneously blasting out bright X-rays and launching a powerful radio jet. This surprising combination wasn’t supposed to happen, according to many models, and suggests scientists may be catching the black hole during a brief, unstable growth spurt. Sat, 24 Jan 2026 03:27:23 EST https://www.sciencedaily.com/releases/2026/01/260124003816.htm https://www.sciencedaily.com/releases/2026/01/260121034114.htm Solar Orbiter has captured the clearest evidence yet that a solar flare grows through a cascading “magnetic avalanche.” Small, weak magnetic disturbances rapidly multiplied, triggering stronger and stronger explosions that accelerated particles to extreme speeds. The process produced streams of glowing plasma blobs that rained through the Sun’s atmosphere long after the flare itself. Wed, 21 Jan 2026 03:41:14 EST https://www.sciencedaily.com/releases/2026/01/260121034114.htm https://www.sciencedaily.com/releases/2026/01/260118233609.htm Physicists have unveiled a new way to simulate a mysterious form of dark matter that can collide with itself but not with normal matter. This self-interacting dark matter may trigger a dramatic collapse inside dark matter halos, heating and densifying their cores in surprising ways. Until now, this crucial middle ground of behavior was nearly impossible to model accurately. The new code makes these simulations faster, more precise, and accessible enough to run on a laptop. Mon, 19 Jan 2026 07:52:41 EST https://www.sciencedaily.com/releases/2026/01/260118233609.htm https://www.sciencedaily.com/releases/2026/01/260114084113.htm Dark matter, one of the Universe’s greatest mysteries, may have been born blazing hot instead of cold and sluggish as scientists long believed. New research shows that dark matter particles could have been moving near the speed of light shortly after the Big Bang, only to cool down later and still help form galaxies. By focusing on a chaotic early era known as post-inflationary reheating, researchers reveal that “red-hot” dark matter could survive long enough to become the calm, structure-building force we see today. Thu, 15 Jan 2026 00:42:07 EST https://www.sciencedaily.com/releases/2026/01/260114084113.htm https://www.sciencedaily.com/releases/2026/01/260112214310.htm Scientists have pulled back the curtain on one of the most extreme solar regions seen in decades, tracking it almost nonstop for three months as it unleashed powerful space weather. By combining views from two spacecraft—one near Earth and one orbiting the Sun—researchers followed a massive active region as it grew, twisted, and ultimately triggered the strongest geomagnetic storms since 2003. Tue, 13 Jan 2026 06:44:15 EST https://www.sciencedaily.com/releases/2026/01/260112214310.htm https://www.sciencedaily.com/releases/2026/01/260110211158.htm Scientists have discovered an enormous stream of super-hot gas erupting from a nearby galaxy, driven by a powerful black hole at its center. The jets stretch farther than the galaxy itself and spiral outward in a rare, never-before-seen pattern. NASA’s James Webb Space Telescope pierced through thick dust to reveal this violent outflow. The process is so intense it’s robbing the galaxy of star-forming gas at a staggering rate. Sat, 10 Jan 2026 23:02:00 EST https://www.sciencedaily.com/releases/2026/01/260110211158.htm https://www.sciencedaily.com/releases/2026/01/260109220500.htm Hubble has revealed a strange cosmic object called Cloud-9, a dark matter–dominated cloud with no stars at all. Scientists believe it is a “failed galaxy,” a leftover building block from the early Universe that never lit up. Its discovery confirms long-standing theories about starless galaxies. Cloud-9 offers a rare glimpse into the dark side of cosmic evolution. Fri, 09 Jan 2026 22:05:00 EST https://www.sciencedaily.com/releases/2026/01/260109220500.htm https://www.sciencedaily.com/releases/2026/01/260107225530.htm Nearly everything in the universe is made of mysterious dark matter and dark energy, yet we can’t see either of them directly. Scientists are developing detectors so sensitive they can spot particle interactions that might occur once in years or even decades. These experiments aim to uncover what shapes galaxies and fuels cosmic expansion. Cracking this mystery could transform our understanding of the laws of nature. Thu, 08 Jan 2026 08:44:48 EST https://www.sciencedaily.com/releases/2026/01/260107225530.htm https://www.sciencedaily.com/releases/2025/12/251227082708.htm New high-resolution images show that novae are anything but simple stellar fireworks. One exploded with multiple gas streams colliding almost immediately, while another shockingly delayed its eruption for more than 50 days before unleashing a powerful blast. These complex outflows create shock waves that produce intense gamma rays, confirming long-standing theories with direct visual evidence. The findings reveal novae as evolving, multi-stage events rather than single, instant explosions. Wed, 31 Dec 2025 16:22:51 EST https://www.sciencedaily.com/releases/2025/12/251227082708.htm https://www.sciencedaily.com/releases/2025/12/251226045338.htm New observations reveal that the relationship between ultraviolet and X-ray light in quasars has changed over billions of years. This unexpected shift suggests the structure around supermassive black holes may evolve with time, challenging a decades-old assumption. Sat, 27 Dec 2025 00:57:27 EST https://www.sciencedaily.com/releases/2025/12/251226045338.htm https://www.sciencedaily.com/releases/2025/12/251222044106.htm Black holes are among the most extreme objects in the universe, and now scientists can model them more accurately than ever before. By combining Einstein’s gravity with realistic behavior of light and matter, researchers have built simulations that closely match real astronomical observations. These models reveal how matter forms chaotic, glowing disks and launches powerful outflows as it falls into black holes. It’s a major step toward decoding how these cosmic engines actually work. Mon, 22 Dec 2025 05:26:39 EST https://www.sciencedaily.com/releases/2025/12/251222044106.htm https://www.sciencedaily.com/releases/2025/12/251209043034.htm A sudden X-ray flare from a supermassive black hole in galaxy NGC 3783 triggered ultra-fast winds racing outward at a fifth the speed of light—an event never witnessed before. Using XMM-Newton and XRISM, astronomers caught the blast unfold in real time, revealing how tangled magnetic fields can rapidly “untwist” and hurl matter into space much like an enormous, cosmic-scale version of the Sun’s coronal mass ejections. Tue, 09 Dec 2025 09:02:44 EST https://www.sciencedaily.com/releases/2025/12/251209043034.htm https://www.sciencedaily.com/releases/2025/12/251207031327.htm Knotted structures once imagined by Lord Kelvin may actually have shaped the universe’s earliest moments, according to new research showing how two powerful symmetries could have created stable “cosmic knots” after the Big Bang. These exotic objects may have briefly dominated the young cosmos, unraveled through quantum tunneling, and produced heavy right-handed neutrinos whose decays tipped the balance toward matter over antimatter. Sun, 07 Dec 2025 07:31:41 EST https://www.sciencedaily.com/releases/2025/12/251207031327.htm https://www.sciencedaily.com/releases/2025/12/251204024243.htm A network of powerful ground-based telescopes captured rare starspot-crossing events on TOI-3884b, revealing cooler patches on the star’s surface and rapid changes tied to its rotation. By combining multicolor transit observations with months of high-cadence brightness monitoring, researchers nailed down the star’s rotation period with impressive precision. These measurements allowed them to map the system’s geometry—and what they found was surprising: the planet's orbit is wildly tilted relative to the star’s spin. Thu, 04 Dec 2025 09:57:01 EST https://www.sciencedaily.com/releases/2025/12/251204024243.htm https://www.sciencedaily.com/releases/2025/12/251203084928.htm For thirty years, SOHO has watched the Sun from a stable perch in space, revealing the inner workings of our star and surviving crises that nearly ended the mission. Its long-term observations uncovered a single global plasma conveyor belt inside the Sun, detailed how solar brightness subtly shifts over the solar cycle, and turned SOHO into an unexpected comet-hunting champion with more than 5,000 discoveries. Wed, 03 Dec 2025 09:03:57 EST https://www.sciencedaily.com/releases/2025/12/251203084928.htm https://www.sciencedaily.com/releases/2025/11/251129053349.htm Nearly a century after astronomers first proposed dark matter to explain the strange motions of galaxies, scientists may finally be catching a glimpse of it. A University of Tokyo researcher analyzing new data from NASA’s Fermi Gamma-ray Space Telescope has detected a halo of high-energy gamma rays that closely matches what theories predict should be released when dark matter particles collide and annihilate. The energy levels, intensity patterns, and shape of this glow align strikingly well with long-standing models of weakly interacting massive particles, making it one of the most compelling leads yet in the hunt for the universe’s invisible mass. Sat, 29 Nov 2025 09:21:07 EST https://www.sciencedaily.com/releases/2025/11/251129053349.htm https://www.sciencedaily.com/releases/2025/11/251125081923.htm Michigan State University astrophysicists are closing in on one of space science’s biggest mysteries: where the galaxy’s most energetic particles come from. Their studies uncovered a pulsar wind nebula behind a mysterious LHAASO signal and set important X-ray constraints on other potential sources. Wed, 26 Nov 2025 06:49:23 EST https://www.sciencedaily.com/releases/2025/11/251125081923.htm https://www.sciencedaily.com/releases/2025/11/251122234723.htm A massive solar storm in May 2024 gave scientists an unprecedented look at how Earth’s protective plasma layer collapses under intense space weather. With the Arase satellite in a perfect observing position, researchers watched the plasmasphere shrink to a fraction of its usual size and take days to rebuild. The event pushed auroras far beyond their normal boundaries and revealed that a rare “negative storm” in the ionosphere dramatically slowed the atmosphere’s ability to recover. These observations offer valuable insight into how extreme solar activity disrupts satellites, GPS signals, and communication systems. Sun, 23 Nov 2025 01:00:14 EST https://www.sciencedaily.com/releases/2025/11/251122234723.htm https://www.sciencedaily.com/releases/2025/11/251116105513.htm LHAASO has uncovered that micro-quasars, black holes feeding on companion stars, are powerful PeV particle accelerators. Their jets produce ultra-high-energy gamma rays and protons that exceed long-held expectations. Precise cosmic-ray measurements reveal a new high-energy component, suggesting multiple sources within the Milky Way. These findings finally tie the “knee” structure to black hole jet systems. Sun, 16 Nov 2025 11:46:04 EST https://www.sciencedaily.com/releases/2025/11/251116105513.htm https://www.sciencedaily.com/releases/2025/11/251115095924.htm Dark matter may be invisible, but scientists are getting closer to understanding whether it follows the same rules as everything we can see. By comparing how galaxies move through cosmic gravity wells to the depth of those wells, researchers found that dark matter appears to behave much like ordinary matter, obeying familiar physical laws. Still, the possibility of a hidden fifth force lingers, one that must be very weak to have evaded detection so far. Sun, 16 Nov 2025 03:57:55 EST https://www.sciencedaily.com/releases/2025/11/251115095924.htm https://www.sciencedaily.com/releases/2025/11/251114041208.htm Scientists have finally confirmed a powerful coronal mass ejection from another star, using LOFAR radio data paired with XMM-Newton’s X-ray insights. The eruption blasted into space at extraordinary speeds, strong enough to strip atmospheres from close-orbiting worlds. This suggests planets around active red dwarfs may be far less hospitable than hoped. Fri, 14 Nov 2025 09:07:09 EST https://www.sciencedaily.com/releases/2025/11/251114041208.htm https://www.sciencedaily.com/releases/2025/11/251111005954.htm New simulations suggest magnetic fields hold the key to forming black holes that defy known mass limits. When powerful magnetic forces act on a collapsing, spinning star, they eject vast amounts of material, creating smaller yet faster-spinning black holes. This process could explain the puzzling GW231123 collision and the existence of “forbidden” black holes. Tue, 11 Nov 2025 00:59:54 EST https://www.sciencedaily.com/releases/2025/11/251111005954.htm https://www.sciencedaily.com/releases/2025/11/251110021054.htm XRISM’s observations of GX13+1 revealed a slow, fog-like wind instead of the expected high-speed blast, challenging existing models of radiation-driven outflows. The discovery hints that temperature differences in accretion discs may determine how energy shapes the cosmos. Mon, 10 Nov 2025 03:48:49 EST https://www.sciencedaily.com/releases/2025/11/251110021054.htm https://www.sciencedaily.com/releases/2025/11/251107010257.htm A colossal black hole 10 billion light-years away has been caught devouring one of the universe’s biggest stars, unleashing a flare 30 times brighter than any seen before. The flare, detected by Caltech’s ZTF, likely marks a tidal disruption event — when a star is shredded by a black hole’s gravity. Fri, 07 Nov 2025 08:52:52 EST https://www.sciencedaily.com/releases/2025/11/251107010257.htm https://www.sciencedaily.com/releases/2025/11/251107010252.htm Using CERN’s Super Proton Synchrotron, researchers generated plasma fireballs to simulate blazar jets. The beams stayed stable, suggesting plasma instabilities aren’t responsible for missing gamma rays. Instead, the data strengthens the idea of ancient intergalactic magnetic fields, possibly from the Universe’s earliest moments. Fri, 07 Nov 2025 08:43:57 EST https://www.sciencedaily.com/releases/2025/11/251107010252.htm https://www.sciencedaily.com/releases/2025/11/251106003906.htm A new theory claims dark matter and dark energy don’t exist — they’re just side effects of the universe’s changing forces. By rethinking gravity and cosmic timelines, it could rewrite our understanding of space and time itself. Thu, 06 Nov 2025 09:53:54 EST https://www.sciencedaily.com/releases/2025/11/251106003906.htm https://www.sciencedaily.com/releases/2025/11/251104094152.htm Researchers using new simulations suggest that the Milky Way’s past collisions may have reshaped its dark matter core. This distorted structure could naturally explain the puzzling gamma-ray glow long thought to come from pulsars. The findings revive dark matter as a major suspect in one of astronomy’s biggest mysteries and set the stage for crucial future observations. Wed, 05 Nov 2025 04:14:06 EST https://www.sciencedaily.com/releases/2025/11/251104094152.htm https://www.sciencedaily.com/releases/2025/11/251104013010.htm Astronomers are rethinking one of cosmology’s biggest mysteries: dark energy. New findings show that evolving dark energy models, tied to ultra-light axion particles, may better fit the universe’s expansion history than Einstein’s constant model. The results suggest dark energy’s density could be slowly declining, altering the fate of the cosmos and fueling excitement that we may be witnessing the universe’s next great revelation. Tue, 04 Nov 2025 01:30:10 EST https://www.sciencedaily.com/releases/2025/11/251104013010.htm https://www.sciencedaily.com/releases/2025/11/251102205023.htm Astronomers observed a massive, multi-temperature plasma eruption from a young Sun-like star, revealing how early solar explosions could shape planets. These fierce events may have influenced the atmosphere and life-forming chemistry of the early Earth. Mon, 03 Nov 2025 04:09:15 EST https://www.sciencedaily.com/releases/2025/11/251102205023.htm https://www.sciencedaily.com/releases/2025/11/251102011152.htm A team of astronomers used the James Webb Space Telescope to create the first 3D atmospheric map of an exoplanet. The fiery WASP-18b, a massive “ultra-hot Jupiter,” revealed striking temperature contrasts, including regions so hot they destroy water molecules. This pioneering eclipse mapping technique lets scientists visualize alien weather in unprecedented detail and could soon be applied to smaller, rocky planets. Sun, 02 Nov 2025 08:28:08 EST https://www.sciencedaily.com/releases/2025/11/251102011152.htm https://www.sciencedaily.com/releases/2025/10/251030075141.htm Earth’s magnetosphere, once thought to have a simple electric polarity pattern, has revealed a surprising twist. New satellite data and advanced simulations show that the morning side of the magnetosphere carries a negative charge, not positive as long believed. Researchers from Kyoto, Nagoya, and Kyushu Universities found that while the polar regions retain the expected polarity, the equatorial areas flip it entirely. Fri, 31 Oct 2025 01:12:13 EDT https://www.sciencedaily.com/releases/2025/10/251030075141.htm https://www.sciencedaily.com/releases/2025/10/251029002907.htm Rice University researchers have captured the temperature profile of quark-gluon plasma, the ultra-hot state of matter from the dawn of the universe. By analyzing rare electron-positron emissions from atomic collisions, they determined precise temperatures at different phases of the plasma’s evolution. The results not only confirm theoretical predictions but also refine the “QCD phase diagram,” which maps matter’s behavior under extreme conditions. Wed, 29 Oct 2025 01:47:27 EDT https://www.sciencedaily.com/releases/2025/10/251029002907.htm https://www.sciencedaily.com/releases/2025/10/251027023741.htm Researchers have directly observed torsional Alfvén waves twisting through the Sun’s corona — magnetic waves first predicted over 80 years ago. Captured using the Daniel K. Inouye Solar Telescope, these motions could explain why the corona is millions of degrees hotter than the Sun’s surface. The finding helps validate decades of solar physics theories and opens new paths to studying solar energy transfer. Mon, 27 Oct 2025 06:48:09 EDT https://www.sciencedaily.com/releases/2025/10/251027023741.htm https://www.sciencedaily.com/releases/2025/10/251024041755.htm Researchers propose that hydrogen gas from the early Universe emitted detectable radio waves influenced by dark matter. Studying these signals, especially from the Moon’s radio-quiet environment, could reveal how dark matter clumped together before the first stars formed. This approach opens a new window into the mysterious cosmic era just 100 million years after the Big Bang. Sat, 25 Oct 2025 03:02:30 EDT https://www.sciencedaily.com/releases/2025/10/251024041755.htm https://www.sciencedaily.com/releases/2025/10/251022023124.htm Researchers suggest that dark matter might subtly color light red or blue as it passes through, revealing traces of its existence. Using a network-like model of particle connections, they argue that light could be influenced indirectly by Dark Matter through intermediaries. Detecting these tints could unlock a whole new way to explore the hidden 85% of the Universe. The finding could reshape how telescopes search for cosmic mysteries. Thu, 23 Oct 2025 02:27:13 EDT https://www.sciencedaily.com/releases/2025/10/251022023124.htm https://www.sciencedaily.com/releases/2025/10/251018102113.htm Scientists at Johns Hopkins may be closing in on dark matter’s elusive trail, uncovering a mysterious gamma ray glow at the heart of our galaxy that could signal unseen matter colliding — or perhaps the frantic spin of dying stars. Using advanced simulations that account for the Milky Way’s ancient formation, researchers found a near-perfect match between theoretical and observed gamma ray maps, tightening the link between dark matter and this puzzling energy. Yet the mystery remains: could these signals come from millisecond pulsars instead? Sat, 18 Oct 2025 10:21:13 EDT https://www.sciencedaily.com/releases/2025/10/251018102113.htm https://www.sciencedaily.com/releases/2025/10/251015032312.htm Scientists at the University of Hawaiʻi have discovered why it rains on the Sun. Solar rain, made of cooling plasma, forms rapidly during solar flares, a mystery now solved by modeling time-varying elements like iron. The finding upends long-held assumptions about the Sun’s atmosphere and could improve predictions of space weather events. It’s a breakthrough that forces a rewrite of how we understand the Sun’s outer layers. Wed, 15 Oct 2025 09:14:33 EDT https://www.sciencedaily.com/releases/2025/10/251015032312.htm https://www.sciencedaily.com/releases/2025/10/251014014438.htm High above the Sun’s blazing equator lie its mysterious poles, the birthplace of fast solar winds and the heart of its magnetic heartbeat. For decades, scientists have struggled to see these regions, hidden from Earth’s orbit. With the upcoming Solar Polar-orbit Observatory (SPO) mission, humanity will finally gain a direct view of the poles, unlocking secrets about the Sun’s magnetic cycles, space weather, and the forces that shape the heliosphere. Tue, 14 Oct 2025 06:30:56 EDT https://www.sciencedaily.com/releases/2025/10/251014014438.htm https://www.sciencedaily.com/releases/2025/10/251014014430.htm New observations from the James Webb Space Telescope hint that the universe’s first stars might not have been ordinary fusion-powered suns, but enormous “supermassive dark stars” powered by dark matter annihilation. These colossal, luminous hydrogen-and-helium spheres may explain both the existence of unexpectedly bright early galaxies and the origin of the first supermassive black holes. Tue, 14 Oct 2025 04:35:42 EDT https://www.sciencedaily.com/releases/2025/10/251014014430.htm https://www.sciencedaily.com/releases/2025/10/251011102301.htm Scientists using a global array of radio telescopes have detected the universe’s lowest-mass dark object by observing how it warped light through gravitational lensing. The invisible mass, about a million times the Sun’s weight, could be a small clump of dark matter or a dormant dwarf galaxy. The finding supports cold dark matter models and opens the door to uncovering more hidden objects shaping the cosmos. Sat, 11 Oct 2025 10:23:01 EDT https://www.sciencedaily.com/releases/2025/10/251011102301.htm https://www.sciencedaily.com/releases/2025/10/251007081827.htm Scientists have simulated how M87*, the supermassive black hole at the center of the galaxy M87, powers its immense particle jet. The Frankfurt team’s FPIC code shows that magnetic reconnection, where magnetic field lines snap and reform, works alongside the traditional Blandford-Znajek mechanism to release rotational energy. These findings shed new light on how black holes energize the cosmos and shape galaxies. Tue, 07 Oct 2025 08:18:27 EDT https://www.sciencedaily.com/releases/2025/10/251007081827.htm https://www.sciencedaily.com/releases/2025/09/250930034209.htm The LUX-ZEPLIN detector is breaking new ground in the hunt for dark matter, setting unprecedented limits on WIMP particles. Its results not only narrow the possibilities for dark matter but also open exciting paths toward other rare physics discoveries. Wed, 01 Oct 2025 03:21:00 EDT https://www.sciencedaily.com/releases/2025/09/250930034209.htm https://www.sciencedaily.com/releases/2025/09/250918225004.htm Scientists at Rutgers and collaborators have traced the invisible dark matter scaffolding of the universe using over 100,000 Lyman-alpha emitting galaxies. By studying how these galaxies clustered across three eras shortly after the Big Bang, they mapped dark matter concentrations, uncovering cosmic “fingerprints” that reveal how galaxies grow and evolve. Fri, 19 Sep 2025 00:10:48 EDT https://www.sciencedaily.com/releases/2025/09/250918225004.htm https://www.sciencedaily.com/releases/2025/09/250917220957.htm Faint hydrogen signals from the cosmic Dark Ages may soon help determine the mass of dark matter particles. Simulations suggest future Moon-based observatories could distinguish between warm and cold dark matter, providing long-sought answers about the invisible backbone of the Universe. Thu, 18 Sep 2025 03:11:54 EDT https://www.sciencedaily.com/releases/2025/09/250917220957.htm https://www.sciencedaily.com/releases/2025/09/250916221836.htm Scientists from the University of St Andrews have discovered that ions in solar flares can reach scorching temperatures more than 60 million degrees—6.5 times hotter than previously believed. This breakthrough challenges decades of assumptions in solar physics and offers a surprising solution to a 50-year-old puzzle about why flare spectral lines appear broader than expected. Wed, 17 Sep 2025 06:52:31 EDT https://www.sciencedaily.com/releases/2025/09/250916221836.htm https://www.sciencedaily.com/releases/2025/09/250910000302.htm Physicists have unveiled a new superconducting detector sensitive enough to hunt dark matter particles smaller than electrons. By capturing faint photon signals, the device pushes the search into uncharted territory. Wed, 10 Sep 2025 18:03:17 EDT https://www.sciencedaily.com/releases/2025/09/250910000302.htm https://www.sciencedaily.com/releases/2025/09/250906013457.htm For decades, scientists have puzzled over why lunar rocks show signs of strong magnetism when the moon itself has no global magnetic field today. New simulations suggest the answer may lie in a powerful asteroid impact billions of years ago. Sat, 06 Sep 2025 14:31:19 EDT https://www.sciencedaily.com/releases/2025/09/250906013457.htm https://www.sciencedaily.com/releases/2025/09/250903075244.htm Solar Orbiter has identified the Sun’s dual “engines” for superfast electrons: explosive flares and sweeping coronal mass ejections. By catching over 300 events close to their origin, the mission has solved key mysteries about how these particles travel and why they sometimes appear late. The findings will improve space weather forecasts and help shield spacecraft and astronauts from solar radiation. Wed, 03 Sep 2025 10:10:15 EDT https://www.sciencedaily.com/releases/2025/09/250903075244.htm https://www.sciencedaily.com/releases/2025/09/250902085004.htm A new model called StarryStarryProcess lets scientists map star spots with precision, improving how exoplanets are studied. By factoring in both transits and stellar rotation, it provides richer details about stars and their influence on planetary signals. Tue, 02 Sep 2025 10:25:58 EDT https://www.sciencedaily.com/releases/2025/09/250902085004.htm