Researchers at the University of Notre Dame have discovered that the unique binary star system AR Scorpii exhibits variability on a timescale of decades, contrary to initial expectations. The study found that the system's brightness more than doubled in minutes and hours, but also showed long-term changes over decades.
A team of researchers has recovered the location of a nova that was first spotted by Korean astrologers in 1437, providing evidence for a long-term life cycle with multiple stages. The study supports the idea that novae undergo smaller-scale eruptions after fading to obscurity for thousands of years.
Researchers have developed a new algorithm to enhance observations from the Kepler Space Telescope and perform detailed studies of stellar variability. The technique, called halo photometry, reveals pulsations in B-type stars with day-long periods, offering insights into poorly understood processes in their cores.
The Kepler Space Telescope's K2 Mission has observed detailed variations in the brightness of stars in the Seven Sisters star cluster. The team developed a new algorithm to measure relative changes in brightness, overcoming instrumental effects and revealing slow-pulsating B stars.
Researchers at the University of Texas at Arlington predicted an additional Earth-like planet in the Gliese 832 system, with stable orbital configuration and mass range of 1-15 Earth masses. The team analyzed simulated data using injected Earth-mass planet to find a habitable zone for potential new world.
A team of UCSB astrophysicists observed a supernova colliding with a nearby companion star, revealing surprising information about the mysterious star. The study demonstrates that the supernova collided with a non-white dwarf companion, implying the white dwarf was stealing matter from a larger companion to explode.
The study found that gas-rich galaxies in a cluster are located in the outer part of the cluster. This is the first time such a location differentiation has been observed in a galaxy cluster. The researchers believe that gas loss prevents star formation, leading to a decline in stellar birthrate over time.
Researchers found that individuals with trypophobia experience intense disgust and nausea when viewing cluster images, even for disease-irrelevant stimuli. The study suggests a connection between trypophobia and an evolutionary history of infectious disease and parasitism.
Astronomers have discovered an exoplanet, HIP65426b, using the SPHERE/VLT instrument for the first time. The planet is located at three times the Earth-Neptune distance from its star and has a mass 6 to 12 times higher than Jupiter.
An international team of astronomers suggests that the Milky Way contains a staggering number of brown dwarfs, with estimates ranging from 25 to 100 billion. The Substellar Objects in Nearby Young Clusters (SONYC) survey found that brown dwarfs are common in dense star clusters and have a small effect on their formation environment.
Astronomers Dr Jane Greaves and Dr Wayne Holland propose a new model for forming planets in the aftermath of a supernova explosion. They suggest that material caught up in the bow-wave around a moving neutron star could provide raw materials for future planet formation. Further data from ALMA is needed to confirm this theory.
Astronomers found new evidence suggesting that a jet of material ejected from one young star triggered the formation of another protostar. The younger star, HOPS 108, lies in the path of an outflow from the older star, HOPS 370. New measurements support the idea that the older star's outflow led to the younger's star formation process.
Researchers used ALMA to map the magnetic field surrounding a young protostar, finding it was surprisingly weak and wildly disorganized. This discovery suggests that the impact of magnetic fields on star formation is more complex than previously thought.
Researchers discovered new details about the Perseus Cluster's mini-halo, a pool of superfast particles emitting radio waves. The study revealed complex mechanisms causing the radio emission, including particle reacceleration and a powerful black hole's energy kick.
Using the Hubble Space Telescope, astronomers measured the deflection of light rays as they passed near a white dwarf star, providing a solid estimate of its mass. The result confirms theoretical predictions and offers insights into the star's structure and composition.
Astronomers used Hubble Space Telescope to repeat a century-old test of general relativity by measuring the deflection of light from a background star. The result provides a solid estimate of the white dwarf's mass and yields insights into theories of its structure and composition.
Scientists have successfully observed a white dwarf star using the bending of distant starlight by gravity, allowing them to determine its mass for the first time. This observation demonstrates a way to measure the masses of objects that cannot be easily measured by other means.
Scientists have discovered an exoplanet, KELT-9b, hotter than most stars, with a day-side temperature of 4,600 Kelvin. The planet's atmosphere is being evaporated due to intense ultraviolet radiation from its host star.
Astronomers study properties of debris disk around sun-like star by analyzing light passing through it. The transit allows scientists to infer characteristics of the disk and potentially discover analogues in our Solar System.
An international team of astronomers led by University of Warwick discovered a giant gas planet up to 50x Jupiter's mass with rings, causing regular eclipses of the young star PDS 110 in Orion constellation. The next eclipse is predicted for September, allowing amateur astronomers to witness and gather new data.
Astronomers discovered a massive star that collapsed into a black hole without exploding as a supernova, challenging the typical view of star formation. The study suggests that up to 30% of massive stars may quietly collapse into black holes without producing a supernova.
Researchers found a dying star that fizzled out and left behind a black hole, shedding light on why massive stars rarely explode as supernovae. The discovery could help explain the origins of supermassive black holes.
A new observational study found that short sleep times may raise the risk of death in people with a cluster of heart disease and diabetes risk factors, with those who slept less than six hours being twice as likely to die of heart disease or stroke. The study suggests that taking care of sleep is important for reducing mortality risk.
Researchers confirmed the orbit and temperature of TRAPPIST-1h, which orbits its star every 18.77 days and is frigidly cold. The discovery suggests that TRAPPIST-1h may have been habitable in the past, with a possible rotation period and activity level for its host star.
The Abell 370 galaxy cluster is a rich mix of various galaxy shapes, including massive elliptical and spiral galaxies. Nearly a hundred distant galaxies have multiple images caused by the lensing effect, with some featuring mysterious-looking arcs of blue light.
In a study published in PLOS ONE, researchers found that female Drosophila buzzatii fruit flies use courtship songs to pick mates of their own species. The study suggests that this preference may have driven speciation in the cluster. Female preferences for specific songs varied among individuals.
Astronomers have confirmed the existence of separate inner and outer disk structures around epsilon Eridani, similar to the asteroid and Kuiper belts in our solar system. The star's debris disk is thought to be a key to understanding the evolution of our solar system.
A team of scientists found a massive wave of hot gas in the Perseus galaxy cluster using Chandra X-ray Observatory data and computer simulations. The wave is thought to have formed billions of years ago after a small galaxy cluster grazed Perseus, causing its gas supply to slosh around an enormous volume.
Astronomers have discovered a unique star in the constellation of Lacerta, which is millions of times closer to Earth than the galaxy NGC 7250, allowing it to overpower its light
Astronomers report the discovery of a binary solar-type star inside the supernova remnant RCW 86, with calcium abundance exceeding the solar one by a factor of six. This finding suggests that the supernova might belong to the rare type of calcium-rich supernovae.
Astronomers have discovered a unique ultra-slow pulsar XB091D in the Andromeda galaxy, believed to have captured a companion only a million years ago. The pulsar's acceleration is linked to its interaction with an ordinary star, providing new insights into neutron star rejuvenation.
A rocky super-earth, LHS 1140b, has been discovered orbiting an M-type star in the habitable zone, making it a promising candidate for atmospheric study and search for life. The planet's size and mass indicate a rocky composition, and its distance from the star allows for relatively cool temperatures.
The star-nosed mole possesses an extremely efficient nervous system that enables it to identify and eat food in under 2 seconds. Its distinctive star organ contains over 100,000 nerve fibers, making it the most sensitive known touch organ in any mammal.
A large, wispy shell of gas, Sh2-308, is blown out by intense radiation from the extreme Wolf-Rayet star EZ Canis Majoris. The star's ongoing activity pushes the bubble to grow bigger and farther apart.
Astronomers have discovered a super-Earth orbiting a quiet red dwarf star, LHS 1140, in the habitable zone where liquid water can exist. The exoplanet's large size and dense iron core suggest it may have retained an atmosphere long after its star calmed down.
Researchers at the University of East Anglia have developed a novel mass spectrometry method to study iron-sulfur cluster proteins, which are crucial for various biological processes. The study successfully detects all reaction components simultaneously, providing detailed insights into their conversion process.
Astronomers identify sun-like star associated with a Type Ia supernova, sparking investigation into its potential role in the white dwarf's demise. Further studies are needed to confirm if this star is indeed the culprit behind a white dwarf's fiery explosion.
Researchers detect 75% of a typical galaxy's star formation obscured by dust, revealing surprising findings about the early universe. The Large Millimeter Telescope allows for deeper observations, pushing our knowledge of dust production and metal enrichment over cosmic time.
Researchers at Imperial College London found that a weak star's light can cause significant material loss from a protoplanetary disc. The study of the IM Lup system revealed that the disc will lose about 3,300 Earth's worth of material over its lifetime.
Astronomers have mapped the location of optical and ultraviolet light emitted by a star torn apart by a black hole. The team used Swift satellite observations to track the changes in brightness of various wavelengths, finding that they originated from elliptical streams of orbiting matter crashing into each other.
Astronomers have observed a striking spiral pattern in the gas surrounding LL Pegasi and its companion star, shedding light on the final act of a dying red giant star. The observations suggest that a highly elliptical orbit is responsible for the shape of the gaseous emissions.
A massive protostar underwent an intense growth spurt, reshaping its surroundings and emitting nearly 100 times more light. This event supports the theory that young stars can experience dramatic growth spurts, which may be triggered by star-forming gas crashing onto their surfaces.
Astronomers have observed a star orbiting a black hole at a rate of nearly twice an hour, marking the tightest orbital dance between a black hole and a companion star ever seen. The discovery was made using the combined power of three advanced telescopes.
Astronomers have found evidence for a star orbiting a black hole at an unprecedented distance, about twice an hour. The close-in binary system, located 14,800 light years from Earth, provides valuable insights into the behavior of black holes and their companion stars.
Astronomers have found evidence of a star that whips around a likely black hole twice an hour, marking the tightest orbital dance ever seen by a black hole and a companion star in our own Milky Way galaxy. The stellar couple is located in the globular cluster 47 Tucanae, about 14,800 light years away from Earth.
Researchers have discovered young stars in old star clusters, suggesting that our current models of stellar evolution may be incorrect. This finding could mean that star clusters contain multiple generations of stars.
Stella Offner's research aims to understand how stars form and interact with their birth environments. Her team will perform computer simulations to test different theories on star mass origin and compare models to telescope observations of star-forming regions.
Scientists have identified a neutron star consuming material at an incredible rate, producing x-rays that exceed the Eddington limit by 1,000 times. The star's strong, multipolar magnetic field is believed to be responsible for its extreme properties.
Scientists have observed the first time a star pulsates in response to its orbiting planet, HAT-P-2b. The star's brightness oscillates ever so slightly every 87 minutes, suggesting that the massive exoplanet may periodically distort its star, causing it to flare or pulse.
Astronomers have discovered a rare pulsating delta Scuti star 7,000 light years away in the Pegasus constellation. The star's unique pattern of expansion and contraction every 2.5 hours is the result of its heating and cooling hydrogen fuel at its core.
Astronomers have found strong evidence for an intermediate-mass black hole (IMBH) weighing 2,200 solar masses at the center of the globular star cluster 47 Tucanae. The IMBH is believed to be the missing link between stellar-mass and supermassive black holes, potentially providing insight into the formation of galaxies.
The University of Massachusetts Amherst has unveiled a powerful new GPU cluster, housing 400 specialized graphics processing units, to accelerate deep learning research and attract top talent in the field. The cluster is expected to significantly boost the university's capabilities in artificial intelligence, computer vision, and natur...
Researchers have identified an exotic binary star system as the first white dwarf pulsar ever discovered in the universe. The star, AR Scorpii, is a rapidly spinning, burnt-out stellar remnant that emits powerful beams of radiation and particles.
A giant black hole has been found to have fed off a nearby star for over 9 years, breaking the previous record for the longest tidal disruption event. The X-ray data suggests that the radiation from material surrounding this black hole consistently surpassed the Eddington limit.
Scientists have discovered incredibly rapid gas flares from a white dwarf binary star system for the first time. The unusual activity was observed at radio wavelengths in SS Cyg, one of the brightest variable stars in the constellation of Cygnus.
Researchers from Ruhr-Universität Bochum used data from the Astrophysical Journal to determine the age of the star, finding it had formed at the same time as our galaxy. The dual star system's companion star transferred matter to 49 Lib, causing incorrect age estimates.
Astronomers have discovered a shadow sweeping across the face of a vast pancake-shaped gas-and-dust disk surrounding a young star, possibly caused by an unseen planet gravitationally pulling on material. The twisted inner disk is casting its shadow onto the outer region.
Astronomers have discovered three young star systems with doomed comets, suggesting a common mechanism for exocomet destruction. The study provides new insights into the past and present activity of comets in our solar system, potentially making life possible on terrestrial planets.
Researchers have discovered a star that ingested some of its planets, revealing a violent history for the planetary system. The star's composition suggests it devoured four planets, preserving lithium and other elements in its atmosphere.
Researchers found that Neptune-mass worlds are likely the most common type of planet to form in icy outer realms. The study provides insight into the types of planets waiting to be found far from a host star, where scientists suspect planets form most efficiently.