A supermassive filament eruption has been observed on a Sun-like star, EK Draconis. The filament was large and fast, posing severe impacts on planetary environments. This finding sheds light on the origins of life on Earth and potential life on other planets.
Astronomers have discovered an ultra-short-period planet GJ 367 b, which orbits its star in just eight hours and has a radius of 72% that of Earth. The planet's mass is 55% of the Earth's, indicating it likely has an iron-rich core, similar to Mercury's interior.
Astronomers have detected a white dwarf star that spins at an incredible rate of once every 25 seconds, completing one rotation faster than Earth. The star is thought to be the size of the Earth but massive enough to pull material from its companion star, creating a magnetic propeller system.
A new imaging method measures individual photons, greatly reducing interference and improving spatial resolution by three times. The technology could also reduce radiation exposure during x-ray imaging, making it ideal for medical applications.
Researchers used computer simulations to investigate the conversion rates of neutrons and protons in accretion disks surrounding black holes, finding that disks with masses between 0.01 to 0.1 solar masses are optimal for heavy element production. This suggests that neutron star mergers producing such disks could be the origin of a lar...
A new technique developed by University of Hawaii astronomer Nader Haghighipour has successfully detected a transiting circumbinary planet in TESS data. The discovery validates the method, which reduces the time to detect such planets from over a year to just five days.
An international research team has measured neutron form factors with previously unattained precision, filling a blank space on the map. The new data provides a more comprehensive picture of the neutron's size and lifetime, and reveals oscillating patterns in its form factor.
Physicists have precisely determined the neutron form factor in a previously unknown energy range, revealing an oscillating pattern and surprising behavior. The findings suggest that nucleons do not have a simple structure, prompting theoretical models to be developed.
Researchers at Michigan State University have successfully conducted an experiment using 'mirror nuclei' to study the fundamental physics of atoms and neutron stars. The team's findings have the potential to improve our understanding of neutron star sizes and provide new insights into the universe's most extreme environments.
Exoplanets HD3167b and two mini-Neptunes orbit in planes perpendicular to each other, with the innermost planet still in the equatorial plane. The discovery suggests an unknown celestial body responsible for this disorder is likely at play.
Researchers at MIT and UNH find that binary neutron star mergers produce two to 100 times more heavy metals than neutron star-black hole mergers. The study suggests that binary neutron stars are a likely cosmic source for gold, platinum, and other heavy metals.
Researchers measured the alpha-proton reaction of magnesium-22, providing essential data for understanding X-ray burst light curves and environments. The new reaction rate was used to closely reproduce observed X-ray bursts, shedding light on the physics behind these events.
Physicists have made the most precise measurement yet of a neutron's lifetime, revealing that it lives 14.629 minutes with an uncertainty of 0.005 minutes. This result brings scientists closer to understanding why two previous methods disagree and could provide evidence for new physics.
Researchers at Jefferson Lab discovered a thinner neutron skin around calcium nuclei than expected, contrasting with lead measurements. This finding presents an opportunity for further exploration into the underlying reasons for this difference.
A new experiment measures the neutron skin in a calcium nucleus, shedding light on proton-neutron interactions. The results will be presented at the 2021 Fall Meeting of the APS Division of Nuclear Physics.
A new study reveals how supernovae explosions of massive stars can form heavy neutron star binaries, resolving a puzzle from gravitational wave observatories LIGO and Virgo. The team's results show that the explosion energy determines whether a stripped star forms a neutron star or black hole.
Researchers from Osaka University have developed a laser-driven neutron source that can generate fast neutrons in short bursts, enabling rapid imaging. The technique was used to detect hazardous substances in batteries and images materials like boron carbide.
HKU astrophysicists identify historical supernova of AD 1181 with recent discovery of 'Parker's star' and its surrounding nebula Pa30. The team found the event matches ancient Chinese reports within 3.5 degrees, providing a firm historical basis for the rare Type Iax designation.
Researchers used a neutron beam to perform pendellösung interferometry on silicon, achieving the highest precision measurements to date. The technique provided insights into the crystal's mechanical and thermal properties, as well as the neutron's charge radius and short-range forces.
Astronomers discovered a stellar collision that triggered a supernova explosion in a companion star. The collision was detected using the VLA and VLASS survey, revealing a centuries-long death dance between two massive stars.
A recent study sheds light on the formation of planetary systems like our own, suggesting that nearby supernovas may have contaminated gas with radioactive material. The researchers found a 59% chance that the enrichment process in Ophiuchus star-forming region is due to supernovas.
A new study of the Ophiuchus star-forming complex offers an analog for the formation of our solar system, suggesting that short-lived radioactive elements were enriched through supernovas in a nearby cluster. The research provides new insights into the conditions in which our solar system was born.
Astronomers studied a piece of supernova shrapnel to understand how it ended up moving fast out of the galaxy. The metal-rich star's slow rotation rate suggests it survived a massive explosion, shedding light on the original two-star system.
New models of neutron stars show mountains only a fraction of millimetres high, contradicting previous estimates. The research used computational modelling to study the role of ultra-dense nuclear matter in supporting these tiny mountains.
Researchers discovered a new type of stellar explosion, electron-capture supernovae, which sheds light on the historic 1054 supernova and provides insights into the behavior of stars. The study focuses on the supernova SN2018zd, located in the galaxy NGC 2146, which has all the properties expected from an electron-capture supernova.
Astronomers have discovered a rare teardrop-shaped star system that will eventually become a Type Ia supernova. The system, HD265435, is comprised of a hot subdwarf and a white dwarf star orbiting each other closely, with the white dwarf being as heavy as our Sun but slightly smaller than Earth's radius.
Astronomers have discovered a rare binary star system, HD265435, which is spiralling towards a Type Ia supernova. The white dwarf companion will go supernova in around 70 million years, providing valuable insights into the expansion of the universe.
Researchers have found evidence of a 'magneto-rotational hypernova', a previously unknown type of cataclysm that could explain the presence of high amounts of uranium and zinc in ancient stars. The discovery, published in Nature, reveals a new pathway for the formation of heavy elements in the infant universe.
Physicists at MIT have successfully measured a neutron's tiny effect in a radioactive molecule, revealing small nuclear effects and providing a chance to search for subtle symmetry violations related to dark matter and the Big Bang. The team used heavy radioactive molecules with extreme sensitivity to nuclear phenomena.
Using numerical simulations, researchers showed that satellite galaxies can retain gas and experience new episodes of star formation after passing close to their parent galaxy. This process is driven by the satellite's reserve of cold gas and minimum distance from its parent galaxy.
Researchers confirmed detection of two rare events involving collision of black hole and neutron star, producing strong gravitational waves signals. The mergers involved massive objects with masses up to 9 solar masses and 1.9-solar-mass neutron stars, providing new information on binary systems and their properties.
Scientists have detected black holes eating neutron stars for the first time, shedding light on the Universe's most extreme objects. The Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo observatories captured the event, providing valuable insights into space and time.
Researchers have detected two events of black holes merging with neutron stars, providing insights into their origins and merger rates. The findings will enable the drawing of conclusions about the host of astrophysical models of compact object formation and binary evolution.
The LIGO, Virgo, and KAGRA collaborations have detected gravitational waves from the merger of a black hole and a neutron star. Analysis reveals that the signals originated from two mixed binaries, each made up of a neutron star and a black hole, with masses consistent with these objects.
A worldwide team of scientists has found evidence for a new type of stellar explosion - electron-capture supernovae. The discovery sheds new light on the thousand-year mystery of the supernova from A.D. 1054.
Astronomers using the CHEOPS space telescope have detected a unique exoplanet, Nu2 Lupi d, which is 9 times the size of Earth and has masses between those of Earth and Neptune. The discovery reveals that the planet has a mild stellar radiation environment, making it an ideal target for studying its composition.
Researchers have confirmed the existence of an elusive new type of stellar explosion, the electron-capture supernova. This discovery sheds light on a thousand-year-old mystery surrounding the 1054 AD supernova visible globally, now believed to be an electron-capture supernova.
The discovery of exoplanet Nu2 Lupi d reveals a rare planet with no known equivalent, with a mass 8.8 times that of Earth and a radius 2.5 times larger than our own. The planet's mild stellar radiation and long orbital period make it an attractive target for future study.
Researchers at Shinshu University and the National Polar Research Institute found a Forbush decrease in cosmic ray counts during a CME event, but the CR density exceeded its original level before exiting the Magnetic Flux Rope. The high-speed solar wind caused this unusual enhancement of CR density through local compression of the MFR.
Researchers have discovered a unique 'blinking giant' binary star system, where a giant star is eclipsed by an unseen orbital companion every few decades. The system has been spotted near the centre of the Milky Way, more than 25,000 light years away.
Astronomers observed a massive protostar called Cep A HW2, revealing two distinct features: a wide-angle wind near the star and a highly-collimated jet at a greater distance. The discovery raises questions about the formation mechanisms of stars across different mass spectrums.
Researchers at KTH Royal Institute of Technology unveiled a new scanning technology that can detect small amounts of nuclear materials in airports and seaports. The Neutron-Gamma Emission Tomography (NGET) system can pinpoint the origin of neutron and gamma ray emissions from weapons-grade plutonium and other special nuclear materials.
The STARFORGE simulation reveals that protostellar jets play a vital role in determining a star's mass, with jets disrupting the inflow of gas toward the star. This breakthrough helps researchers better understand star formation and its impact on galaxy evolution.
Astronomers have discovered a mysterious yellow star that exploded without the typical hydrogen layer, revealing new insights into the violent death throes of massive stars. The discovery challenges current understanding of stellar evolution and suggests that these stars may undergo catastrophic eruptions before exploding.
Researchers used NASA's Hubble Space Telescope to examine the massive star two-and-a-half years before its explosion. The team found that the star lacked its typical hydrogen layer, making it unusually cool before exploding into a supernova.
A new simulation study led by UCL researchers suggests that studying black hole-neutron star collisions could provide a new measurement of the Universe's expansion rate, helping to resolve a long-standing dispute. The study found that instruments on Earth could detect ripples in space-time caused by up to 3,000 such collisions by 2030.
Researchers made a precise measurement of the lead nucleus's neutron skin, revealing it's thicker than expected. This thickness has implications for the physical processes in neutron stars and their size.
Astronomers capture breathtaking images of AG Carinae, a luminous blue variable star surrounded by a glowing halo of gas and dust. The star is in a constant battle to maintain stability due to its massive form and super-hot temperatures.
Astronomers have found powerful evidence for a neutrino-driven explosion in the remains of a supernova called Cassiopeia A (Cas A). The discovery was made using NASA's Chandra X-ray Observatory and suggests that titanium bubbles play a crucial role in driving the shock wave forward to trigger the supernova explosion.
Astronomers have discovered a pulsar, a dense and rapidly spinning neutron star sending radio waves into the cosmos. The finding is significant as it hints at a large population of pulsars awaiting discovery in the Southern Hemisphere, with the potential to be detected by the Square Kilometre Array telescope.
Researchers at Chinese Academy of Sciences discover abnormal enhancement of α-particle clustering in uranium isotopes, revealing strong proton-neutron interaction influence on α-decay properties. The study reveals systematics trends and anomalies in α-decay reduced widths for polonium-plutonium nuclei near shell closure.
Researchers used NASA's NICER telescope on the International Space Station to measure the size of PSR J0740+6620, the most massive known neutron star. The team's findings provide insights into the squeezability of matter in neutron star cores, shedding light on what happens when neutrons break down into smaller particles.
A Northwestern University study finds that emotional reviews, not star ratings, predict business success in various industries such as movies, books, and restaurants. The research uses computational linguistics to analyze the emotionality of reviews and shows that higher emotionality is associated with greater success.
A global science collaboration using NICER data discovered X-ray surges accompanying giant radio pulses from the Crab Nebula's pulsar. The finding shows that these bursts release dozens to hundreds of times higher total emitted energy than previously estimated.
Researchers at the University of Bath used resonance in spiraling neutron stars to measure symmetry energy, a key property of nuclear matter. This discovery sheds light on the fundamental workings of nuclei and offers insights into the forces that bind sub-atomic particles.
Astronomers discovered over 800 dense gas and dust cores near the Galactic Center, which may be 'stellar eggs' hatching into baby stars despite harsh conditions. The findings suggest that star formation is more resilient than thought, with ALMA observations detecting small outflows indicative of star birth.
Researchers studied 304 developing stars and found that gas-clearing by a star's outflow may not be as important in determining its final mass. The team's results indicate cavities in the surrounding gas cloud do not grow regularly, suggesting another process gets rid of excess gas.
Research from Binghamton University found that star employees take most of the credit for successful collaborations and most of the blame for failed ones, affecting non-star collaborators' careers. Non-stars may benefit from working with stars despite not receiving equal rewards or penalties.
A new study advances a decisive test to investigate the origin of solar-mass black holes, which may be connected to dark matter. The research suggests that such black holes could have formed in the early Universe, contradicting conventional stellar evolution astrophysics.
A team of researchers used radioactivity in meteorites to study the cosmic origin of heaviest elements, shedding light on violent stellar explosions. The study found that specific astronomical events, such as neutron star collisions, likely created these heavy elements.