New 3D models reveal that a supernova explosion likely triggered the formation of our Solar System, injecting polluted material into a cloud of dust and gas. The models show that only one or two fingers from the shock wave could have caused the pollution found in primitive meteorites.
Researchers at Caltech found a correlation between the neutrino signal and the gravitational-wave signal that occurs when the proto-neutron star reaches high rotational velocities. This discovery provides new insights into understanding the explosion process in massive stars.
Researchers using Chandra X-ray Observatory and XMM-Newton have found a point-like object, IGR J11014, which may be a rapidly spinning, super-dense star ejected during a supernova explosion. If confirmed, its speed of millions of miles per hour poses a challenge to existing models for supernova explosions.
Researchers observed a supernova's X-ray emission breaking through a cocoon of dense gas surrounding the star. The data support the idea that some supernovas are powered by blast waves interacting with surrounding material. Additionally, the discovery hints at an unrelated ultraluminous X-ray source nearby.
A team of astronomers studied 23 Type Ia supernovae to find signatures of gas around the explosions. They found that more powerful explosions came from systems with outflows of gas, but only a fraction showed evidence for these outflows.
For the first time, astronomers have detected arsenic and selenium in an ancient star, revealing insights into the origin of these elements. The discovery sheds light on how stars produce heavier elements, including those found on Earth.
The Baryon Oscillation Spectroscopic Survey (BOSS) has made precision measurements of the large-scale structure of the universe five to seven billion years ago. By using a technique called baryon acoustic oscillation, BOSS can determine the distances to faraway galaxies with unprecedented accuracy.
Studies using X-ray and ultraviolet observations from NASA's Swift satellite provide new insights into the elusive origins of Type Ia supernovae. The research suggests that the companion to a white dwarf is either a smaller, younger star similar to our sun or another white dwarf.
Yale researchers found that megakaryocytes grow 10-15 times larger than other blood cells through endomitosis, but a malfunction in this process may lead to leukemia. The discovery reveals the formation of functional platelets and provides clues about what may go awry to transform normal megakaryocytes into malignant leukemia cells.
A team of researchers from MIT has detected tellurium, a rare Earth element, for the first time in three ancient stars. The finding supports the theory that tellurium and other heavy elements likely originated from a rare type of supernova during nuclear fusion.
Astrophysicists have uncovered new questions and clarified previous theories about gamma-ray bursts using the Fermi Gamma-Ray Space Telescope. The telescope's unique view allows it to capture the highest energy portion of these bursts, which are difficult to detect due to their brief duration and narrow radiation patterns.
Researchers have used a 'light echo' technique to demonstrate that Eta Carinae's Great Eruption was significantly cooler than expected, differing from previously thought supernova impostors. The team's findings suggest the eruption may have been triggered by alternative models, warranting further investigation.
Astronomers using NASA's Hubble Space Telescope have discovered a distant Type Ia supernova, offering new opportunities to study dark energy. The discovery marks a significant step forward in understanding the mysterious force driving the universe's acceleration.
A team led by LSU Professor Bradley Schaefer and graduate student Ashley Pagnotta discovered the origin of thermonuclear supernovae as a pair of white dwarf stars. The study resolves the decades-long 'progenitor problem' in astrophysics, with no remaining possible explanations for the explosions.
Astronomers have solved a longstanding mystery on the type of star that caused a Type Ia supernova seen in a nearby galaxy. The Hubble Space Telescope detected faint white dwarf remnants, contradicting previous theories and suggesting two tightly orbiting stars may have collided to trigger the explosion.
Researchers have confirmed that Type Ia supernovae are produced by the explosion of carbon-oxygen white dwarf stars. By analyzing a fluke observation of SN2011fe four hours after its explosion, scientists set stricter limits on the size of the progenitor star, ruling out other possibilities.
The Fermi team has discovered hundreds of new energy sources in the high-energy sky, including active galaxies and pulsars. These discoveries will allow astronomers to compare the behavior of different sources across a wider span of gamma-ray energies for the first time.
Astronomers will use a new telescope called X-Calibur to study the polarization of X-rays, providing information about cosmic sources that is not available elsewhere. The instrument will be sensitive to hard X-rays and will be flown at an altitude of 40 kilometers, allowing it to focus on celestial objects with high accuracy.
Supernovas release enormous amounts of energy, but are too far away to harm Earth's ozone layer. Gamma-ray bursts could pose a threat if directed towards our planet, but estimates suggest it's unlikely to occur in the near future.
The study of the closest supernova in 25 years has shed new light on its formation. The team found that the exploding star was a white dwarf, and while they couldn't rule out a white dwarf merger, their results suggest a medium-sized star supplied the white dwarf with extra material to trigger the explosion.
Astronomers have determined how a Type Ia supernova occurs, involving a dense white dwarf and main-sequence star. The study provides new insights into the universe's expansion and cosmic origins.
A team of scientists has observed the early stages of a Type Ia supernova, refining our understanding of these explosive events. The discovery suggests that the primary star was a carbon-oxygen white dwarf, and analysis of matter ejected by the explosion points to a possible subgiant or main-sequence star as the secondary companion.
Astronomers have observed the closest Type Ia supernova in decades, providing direct evidence for what a carbon-oxygen white dwarf looks like before it explodes. The study reveals that the supernova's progenitor was likely a binary system with a small white-dwarf star orbiting a companion.
Astronomers detected a nearby Type Ia supernova with unprecedented observation of initial stages, characterizing the nature of forming stars. NSF's Cyber-Enabled Discovery program supported computational framework for rapid detection and characterization.
Researchers used Hubble Space Telescope data to rule out some proposed progenitor systems for Type Ia supernovae. The study suggests that the companion star was likely a normal star like our sun, a subgiant, or possibly a white dwarf.
An international team of scientists has discovered that a recently exploded supernova was a 'white dwarf' star, challenging the long-held theory that it was a red giant. The finding provides direct evidence that white dwarfs are responsible for Type Ia supernovae.
Researchers will use a three-year, $1.38 million grant to study presolar grains in a sample of the Murchison meteorite. They aim to extract exceptionally large grains that came from supernovae, allowing them to make more comprehensive measurements and understand how elements were forged.
Scientists use NASA's Fermi Gamma-Ray Space Telescope to detect high-energy gamma rays from the remnant of Tycho's supernova. This detection supports the notion that supernova remnants can accelerate cosmic rays, providing clues to their origins.
Astronomers propose two exotic scenarios for the unusual cosmic explosion: a novel supernova billions of light-years away or an unusual collision within our own galaxy. The 'Christmas burst' was caused by either event, with observations suggesting a neutron star and rapid tightening of its orbit.
Researchers studying a binary star system in the Whirlpool Galaxy have detected a star dimming noticeably before its companion exploded in a supernova. The study provides evidence that certain patterns of brightening and dimming may signal an impending doom for stars, making it possible to predict when a star is near death.
The study reveals that Cygnus X has formed a 'cocoon' of trapped cosmic rays, which were accelerated by the intense stellar winds and shockwaves. This finding provides a unique glimpse into the early life of cosmic rays, long before they diffuse into the galaxy.
A team of researchers performed new 3-D calculations to better understand the complex conditions driving Type Ia supernovae. The simulations provide insight into the deflagration-to-detonation transition process, which is crucial for calculating cosmic distances and understanding the evolution of the universe.
Researchers Hu et al. developed a new detonation model named the least-action detonation model (LADM) that takes into account complex movement and transport effects, differing from the classical ZND model. The LADM model predicts detonation product particles to be in a stationary state, which has been observed in experiments.
Researchers have discovered that ancient stars in the Milky Way's halo contain abnormally large amounts of heavy elements like gold and uranium. By analyzing the motions of these stars, they found evidence suggesting that exploding supernovae may have sent jets of enriched gas into space, creating the heavy-element rich stars.
Astronomers found two distinct populations of neutron stars, suggesting different supernova channels. The findings shed light on stellar evolution and open new research areas.
NICER will measure X-rays from hotspots on a neutron star's surface and its magnetic field, revealing the star's size and helping researchers determine an Equation Of State. This will unlock the secret of matter under extreme gravity in these incredibly dense objects.
Scientists have found the first gamma-ray pulsar in a globular cluster, J1823-3021A, which is also the youngest millisecond pulsar discovered to date. Its high luminosity and strong magnetic field challenge current theories on its formation.
Saul Perlmutter, along with Brian Schmidt and Adam Riess, discovered the accelerating expansion of the universe through distant supernovae observations. This discovery implies the existence of dark energy, a mysterious force opposing gravity and increasing galaxy distances.
Astronomers use Hubble's unprecedented precision to map dark matter in 25 massive galaxy clusters, challenging previous assumptions about its distribution. The survey's findings suggest that galaxy cluster assembly may have begun earlier than previously thought.
Researchers have discovered gamma rays with unprecedented energies from the Crab Pulsar in the Crab Nebula, contradicting existing theories. The findings suggest a different mechanism for producing these high-energy particles, which could be detected by the VERITAS observatory.
Scientists have detected pulsed gamma-ray emission from the Crab pulsar at energies far beyond what current theoretical models can explain. The VERITAS telescope array detected gamma-rays with energies exceeding 100 billion electron-volts, putting new constraints on the mechanism for how the gamma-ray emission is generated.
A team of astrophysicists has detected pulsed gamma rays from the Crab Nebula with energies up to 400 billion electronvolts, far exceeding previous detection limits. The high-energy emission challenges existing pulsar models and may require significant adjustments to our understanding of these extreme systems.
A team of researchers from Tel Aviv University has uncovered a record-breaking number of ancient supernovas in the Subaru Deep Field. These explosions are believed to be a major source of iron in the universe, including the Earth's core and blood.
Saul Perlmutter, a physicist at Lawrence Berkeley National Laboratory, won the 2011 Nobel Prize in Physics with colleagues Brian Schmidt and Adam Riess. Their groundbreaking work discovered the accelerating expansion of the universe through observations of distant supernovae.
A NASA team will attempt to send a balloon with an instrument payload to measure gamma rays from the Crab Pulsar, 6,500 light years away. The mission aims to study the polarization of gamma rays, which can provide clues about the source's mechanism.
The Fermi catalog reveals a mix of known and unknown objects, with active galaxies, pulsars, and supernova remnants making up a large portion. Unassociated sources pose an intriguing mystery, sparking research into new types of gamma-ray-emitting objects.
Astronomers propose a new way to search for supernova precursors by studying the spin of white dwarfs. This process could lead to a time delay of up to a billion years before the explosion, allowing for detection by upcoming surveys.
Astronomers caught the PTF 11kly supernova within hours of its explosion, observing it with multiple telescopes and making it one of the most-studied supernovae in history. The early detection allows researchers to study the outer layers of the supernova and gain new insights into its origin.
Scientists have discovered that about a quarter of Type Ia supernovae are born from medium-sized stars similar to our Sun. This finding challenges the long-held assumption that all Type Ia supernovae have the same luminosity, which is crucial for measuring cosmic distances.
Researchers found evidence of gas outflows from the supernova ancestors, suggesting they don't originate from white dwarfs. This discovery is crucial for understanding Type Ia supernovae and their immense luminosity.
Scientists have discovered a pair of white dwarfs that are spiraling into each other at breakneck speeds, allowing them to test Einstein's theory of general relativity. The merger could also shed light on the origin of underluminous supernovae.
Astronomers detect cosmic dust from a supernovae using Herschel Space Observatory, confirming the theory that these explosions create dust. The study reveals a large amount of cold dust formed during the explosion, which could explain the origin of dust in galaxies.
Integral's observations show that quantum 'graininess' must be at much smaller scales than previously predicted, contradicting Einstein's General Theory of Relativity. The results limit the size of these grains to 10^-48 m or smaller, ruling out some string theories and quantum loop gravity theories.
Astrophysicists are using Type Ia supernovae, also known as 'zombie' stars, to build a map of the universe's history and understand dark energy. The stars' explosive deaths can be used to measure distances in the universe.
A team of astronomers led by Caltech has discovered a new type of supernovae that was previously unknown. The four newly found supernovae have similar spectral signatures, indicating they are all part of the same class. This discovery provides insight into star formation, distant galaxies, and the early universe.
Astronomers have discovered a local supernova factory in the Carina Nebula, which may help understand how young stars release newly-forged elements into their surroundings. The Chandra X-ray Observatory detected over 14,000 stars, six possible neutron stars, and a new population of young massive stars.
A newly merged black hole can be detected by observing the tidal disruption of surrounding stars, which will provide accurate distances and precise sky coordinates. This could lead to a better understanding of dark energy and Einstein's general theory of relativity.
A pattern of X-ray 'stripes' in the Tycho supernova remnant supports a theory on how magnetic fields amplify near expanding shock waves, accelerating particles to extreme energies. The discovery may provide direct evidence for the production of cosmic rays.
Astronomers using NASA's Hubble Space Telescope have recalculated the universe's expansion rate with unprecedented accuracy, ruling out an alternate theory on dark energy. The new measurement reduces uncertainty by 30% and solidifies understanding of cosmic ingredients.
Researchers found a superfluid in the neutron star's core that could defy gravity and a superconductor that can sustain electricity forever. This discovery provides insight into the life cycles of stars and behavior at high densities.