Articles tagged with Astrophysics
Astronomers captured dark coronal loop strands with unprecedented clarity during an X1.3-class flare, measuring 48.2 km in width, the smallest ever imaged. The team's high-resolution images offer a potential breakthrough in resolving the fundamental scale of solar coronal loops and improving space weather forecasting.
Astronomers have devised a method to map the spottiness of distant stars using observations from NASA missions, improving understanding of planetary atmospheres and potential habitability. The new model, called StarryStarryProcess, can help discover more about exoplanet properties.
Researchers at Nagoya University and the Italian National Institute for Astrophysics have determined how molten rock droplets formed in Jupiter's early days. Their study shows that chondrule characteristics are influenced by the water content of impacting planetesimals, providing a clearer picture of solar system formation.
Researchers at Ohio State University suggest a large cloud of dust and gas occluded Earth's view of the star ASASSN-24fw, causing its brightness to dim by 97% before brightening again. The team proposes that this disk is likely made up of carbon or water ice close in size to a large grain of dust.
Researchers pinpointed the location of the brightest fast radio burst (FRB) ever recorded, RBFLOAT, to a single spiral arm of a galaxy 130 million light-years away. The precision was achieved using the CHIME/Outrigger array, allowing scientists to explore the environment and potentially shed light on the nature and origins of these mys...
Researchers propose that Jupiter-sized exoplanets may accumulate and collapse into detectable black holes due to dark matter. This process could potentially generate multiple black holes in a single exoplanet's lifetime, making exoplanet surveys a promising method for hunting superheavy dark matter particles.
Scientists have detected a near and ultrabright fast radio burst (FRB) from a nearby galaxy, allowing for unprecedented study of the environment around these enigmatic flashes. The burst's proximity and brightness enabled precise localization to a specific region within its host galaxy.
Researchers have discovered a massive gas and dust bubble surrounding the red supergiant star DFK 52, which contains as much mass as our own Sun. The bubble is expanding at an incredible rate and was likely formed when the star ejected part of its outer layers in a powerful explosion around 4000 years ago.
Researchers at Kyoto University discovered that streamers of gas can feed young stars, potentially leading to the rapid formation of high-mass stars. The team used ALMA to observe a system with two streamers, which carried enough matter to quench feedback effects from the central star.
Researchers use numerical relativity to probe the universe's biggest questions, including the Big Bang, cosmic inflation, and multiverse theories. The method allows for exploration of extreme situations beyond current mathematical limits.
The University of Minnesota researchers discovered a new type of plasma wave in Jupiter's aurora, which helps understand the phenomenon and its potential applications for protecting Earth. The study reveals that Jupiter's magnetic field allows particles to flood into the polar cap, unlike on Earth.
Physicists from the University of Copenhagen have discovered a step-like signature that resembles the signature of an elusive axion particle using galaxy clusters. This method has greatly increased what we know about axions, allowing researchers to narrow down the space where it can be found.
Researchers have developed a novel way to reach the unexplored mesosphere using lightweight flying structures that can float using sunlight. The devices, which were built at Harvard and other institutions, levitated in low-pressure conditions and demonstrated potential for climate sensing and exploration.
The Helmholtz-Zentrum Dresden-Rossendorf has developed a model that derives the Sun's known activity cycles from the cyclical influence of the planets' tidal forces. This synchronization automatically curbs solar activity, leading to subdued radiation eruptions and reduced geomagnetic storms.
Researchers measured magnetic field of Sagittarius C, a region in the Central Molecular Zone, to understand interaction between dense clouds, star formation, and strong magnetic field. The study found that the magnetic field wraps around an expanding central bubble of hot, ionized gas created by massive young stars.
A new theoretical study proposes a comprehensive framework for the birth of supermassive black holes, linking their formation to the early universe's 'Population III.1' stars. The 'Pop III.1' model predicts rapid ionization by these stars, shedding light on long-standing cosmological conundrums.
Scientists found that ionic liquids, formed from sulfuric acid and organic compounds, could persist on planets too warm for water to exist. This discovery increases the habitability zone for rocky worlds, suggesting life might be possible without water.
An interstellar mission to test astrophysical black holes is proposed by Cosimo Bambi, harnessing nanocrafts and laser beams to gather data on nearby black holes. The mission aims to answer pressing questions in physics, including the nature of event horizons and general relativity.
Researchers have discovered a rare white dwarf remnant with a carbon signature, suggesting it formed from the merger of two stars. The high-mass white dwarf, WD 0525+526, has a thin atmosphere that allows carbon to reach its surface, providing insights into the early stages of stellar evolution.
A new study by Dartmouth astronomers has mapped 355 candidate satellite galaxies around dwarf galaxies, tripling the number previously surveyed. The researchers aim to understand how external conditions influence satellite formation and uncover insights into dark matter's nature.
The Nancy Grace Roman Space Telescope will feature a 'sunblock' shield made of lightweight yet stiff panels designed to limit heat transfer. The observatory's instruments will benefit from this design, which can detect faint signals from space.
A team of researchers at Kyoto University has successfully developed a method to calculate the vibrations of black holes using exact WKB analysis. The approach reveals complex patterns in spiraling waves, enabling precise capture of frequency structure and bridging theoretical predictions with observational data.
Researchers at Max-Planck-Institut für Kernphysik recreated a reaction under conditions similar to those in the early universe for the first time. They found that the rate of this reaction remains almost constant with decreasing temperature, contradicting previous predictions.
The Near-InfraRed Planet Searcher (NIRPS) spectrograph, combined with HARPS, offers exceptional performance in detecting and characterizing exoplanets. The first scientific results revealed atmospheres of two gas giant exoplanets, including one with an extreme atmosphere containing evaporated iron.
A new study from NYU Abu Dhabi found that high-energy particles from space, known as cosmic rays, could create energy needed to support life underground on planets and moons. This process, called radiolysis, can power life even in dark, cold environments with no sunlight.
Researchers have discovered star-shredding black holes in dusty galaxies, confirming that these events are powered by dormant black hole accretion. The study uses the James Webb Space Telescope to detect clear fingerprints of black hole activity in four galaxies, revealing key differences between active and dormant black holes.
Researchers detected sulfur in both gas and solid phases using data from the XRISM spacecraft, providing unprecedented insight into its presence in the universe. The findings are based on measurements of X-rays from two binary star systems and suggest that sulfur can easily change between these forms.
Researchers at TU Wien found that the solar wind ions' erosive effect on the Moon has been vastly overestimated. The actual yield is up to an order of magnitude lower than previously assumed due to the regolith's porous structure.
The CTAO LST Collaboration presents groundbreaking findings on the nature of gamma-ray bursts, supporting theoretical models of structured, multi-layered jets. The observations of GRB 221009A provide new clues about jet formation mechanisms and the central engine behind these cosmic phenomena.
Researchers propose using soft X-rays to measure reconnection rates and monitor space weather. By analyzing bright X-ray features, they calculated a global reconnection rate of 0.13, closely matching theoretical predictions.
Researchers observed a flare caused by a star falling onto a black hole and surviving the encounter. The discovery suggests that these flares may be part of a longer, more complex story about supermassive black holes.
Roman will scan a large region of the cosmos every five days for two years, detecting around 27,000 type Ia supernovae and 60,000 core-collapse supernovae. These observations will help scientists understand dark energy, the universe's expansion, and fill gaps in our understanding of cosmic history.
Researchers used NASA's TESS mission data to estimate the sizes of over 200 exoplanets and found that many are likely larger than previously thought. This discovery could impact the search for life on distant planets, as water worlds may harbor life but lack features that help life flourish on Earth.
The LIGO-Virgo-KAGRA Collaboration has detected the merger of two massive black holes, producing a final black hole approximately 225 times the mass of our Sun. The signal presents a challenge to current astrophysical models and requires advanced theoretical tools to interpret.
The LIGO-Virgo-KAGRA Collaboration detected the merger of two massive black holes, producing a final black hole over 225 times the mass of our Sun. The signal challenges current astrophysical models and requires the use of theoretical models to interpret its complex dynamics.
Researchers successfully demonstrate Fermi acceleration mechanism with ultracold atoms, unlocking new understanding of cosmic rays behavior. The technology has the potential for high-precision control over particle acceleration and opens new possibilities for investigating phenomena relevant to high-energy astrophysics.
Researchers from Shanghai Jiao Tong University proposed a method for neutron spectrum regulation to enhance the irradiation production efficiency of transuranium isotopes. The new method achieves efficient and precise neutron spectrum optimization, maximizing the production of transuranic isotopes.
The discovery of dense clouds of neutral hydrogen gas within the Fermi bubbles challenges current understanding of their formation and age. These 'ice-like' clouds are found at 12,000 light years above the Milky Way's center and are much younger than previously estimated.
Researchers propose 'dark dwarfs' could be key to understanding dark matter, with lithium-7 serving as a unique marker. A discovery of a dark dwarf would provide compelling evidence for WIMPs as a possible dark matter component.
Researchers discovered plants can select good microbes and suppress harmful ones to thrive in challenging conditions. The concept of functional team selection highlights the importance of microbiome diversity in plant adaptation.
Researchers at GSI/FAIR have conducted high-precision measurements of three extremely neutron-rich tin isotopes, revealing unexpected changes in the behavior of tin nuclei beyond N=82. These findings improve our understanding of nuclear forces far from stability and may alter the path of the r-process on the nuclear chart.
Researchers used machine learning to simulate galaxy evolution and supernova explosions, achieving speeds four times faster than supercomputers. This breakthrough enables the study of galaxy origins, including the creation of the Milky Way's elements essential for life.
The Vera C. Rubin Observatory has unveiled the first images of the sky obtained with its LSST camera, a 3200-megapixel resolution car-sized camera that can photograph 45 times the area of the full moon in just three nights. The high-definition images will provide unprecedented views of the southern sky and reveal faintest and furthest-...
A team of researchers has discovered that a specific radio signal can reveal the masses of the earliest stars, crucial for understanding the Cosmic Dawn. The study utilizes the 21-centimetre signal, created by hydrogen atoms filling gaps between star-forming regions, to inform predictions about future radio telescopes like REACH and SKA.
Dr. Karen I. Perez joins the SETI Institute as the inaugural recipient of the William J. Welch Postdoctoral Fellowship, developing real-time analysis pipelines for detecting signals from intelligent life. Her research will advance radio astronomy and contribute to shaping the next generation of SETI instrumentation.
Researchers surveyed luminous infrared galaxies to gain insight into galaxy formation in the early universe and possibly the Milky Way. They discovered massive clumps of newborn stars, unlike anything seen in the Milky Way.
Scientists at UC Riverside successfully measured the electric dipole moment of aluminum monochloride, a crucial diatomic molecule. The precise measurement will aid in quantum technologies, astrophysics, and planetary science.
Researchers using the James Webb Telescope have discovered silicate clouds in the atmosphere of exoplanet YSES-1-c, which is thought to be linked to the planet's relative youth. The findings offer new insights into planetary formation and atmospheric processes, shedding light on how our own solar system may have formed.
A new study by Southwest Research Institute (SwRI) proposes that compact exoplanetary systems may be surviving remnants of planet accretion during the final stages of stellar formation. This process results in similarly sized planets with characteristic masses determined by infall and disk conditions.
The COSMOS-Web field maps nearly 800,000 galaxies spanning 98% of cosmic time, challenging existing notions of the infant universe. Researchers see roughly 10 times more galaxies than expected at incredible distances, sparking new questions about the early universe and its mysteries.
Researchers have made the most sensitive direct measurement yet of the 12C(12C,a0)23Na reaction down to an excitation energy of 2.22 MeV using a HOPG target and intense carbon beam. The results represent the highest sensitivity achieved for this channel, with a thick-target yield on the order of 10−17 per incident carbon ion.
A team led by UChicago scientist Wendy Freedman has used the James Webb Space Telescope to find no evidence of tension in the Hubble Constant, resolving a decade-long conflict. The new data strengthens the Standard Model of the universe, suggesting that the Hubble Constant may not be the source of inconsistencies.
Scientists have observed ultra-narrow bright and dark stripes on the solar photosphere, offering unprecedented insight into how magnetic fields shape solar surface dynamics. These striations are linked to magnetic fluctuations that alter plasma density and opacity.
Researchers analyzing the atmosphere of WASP-121b using the James Webb Space Telescope detected water, carbon monoxide and silicon monoxide in both the dayside and nightside hemispheres. This is the first conclusive identification of SiO in any planetary atmosphere.
Scientists used NASA's Hubble and Gaia space telescopes to simulate the evolution of the Milky Way and Andromeda over 10 billion years. Contrary to previous beliefs, they found a only 2% probability of collision within five billion years.
Four new studies provide conclusive evidence for the existence of intermediate-mass black holes, offering a window into the universe's first stars. The researchers used data from LIGO detectors to identify these heavy gravitational-wave events, paving the way for future observations using space-based missions like LISA.
A team of astronomers from ICRAR discovered a new type of cosmic phenomenon called ASKAP J1832-0911, which emits pulses of radio waves and X-rays for two minutes every 44 minutes. This is the first time such an object has been detected in X-rays.
Researchers suggest that an ancient, weak magnetic field and a large plasma-generating impact combined to create a strong magnetic field on the moon. This process could explain the presence of highly magnetic rocks near the south pole's far side, where the Imbrium basin is located.
Scientists have successfully measured the structure of liquid carbon using a unique combination of laser compression, X-ray analysis, and large-area detectors. The results reveal that liquid carbon has a water-like structure with special structural properties, and its melting point was precisely determined.
Researchers use NASA's James Webb Space Telescope to investigate a protoplanetary disk around a young star in the Lobster Nebula. They found sufficient solid material to potentially form at least 10 rocky planets and detected various molecules that contribute to planetary atmospheres.