Astronomers observe two long gamma-ray bursts that defy the consensus of supernova association, suggesting multiple ways to produce black holes and gamma-rays. The discoveries indicate a rich diversity in cosmic events and challenge the prevailing model of massive stellar death.
Recent gamma-ray bursts suggest a new kind of cosmic explosion involving newly formed black holes swallowing parent star matter. Astronomers observe no supernovae associated with these events, which could be due to massive stars dying without producing explosions.
Researchers found that under certain conditions, the surface of a strange star could fragment into blobs of quark material called strangelets, forming a rigid halo. This contradicts traditional models and raises questions about the nature of collapsed stars' nuclear leftovers.
Researchers found significant peripheral asymmetry but a nearly spherical interior, suggesting the explosion propogates at supersonic speed. The team observed 17 supernovae over 10 years and inferred the shape and structure of debris clouds thrown out from Type Ia supernovae.
Astronomers have observed a rare phenomenon of two supernovas occurring simultaneously in the same galaxy, with implications for our understanding of galaxy mergers. The high frequency of supernovas in NGC 1316 suggests that massive star formation may be driving this activity.
Astronomers have mapped the rate of acceleration of cosmic ray electrons in a supernova remnant, showing close to maximum theoretical rates. The discovery provides evidence that supernova remnants are key sites for energizing charged particles.
A new National Research Council report emphasizes the physical risks of extended space journeys due to space radiation. The report recommends developing storm shelters to protect astronauts from harmful radiation, as well as improving space engineering techniques and enhancing solar forecasting.
Astronomers discover sun was born in a massive star cluster, challenging current theories on planetary formation. The researchers used radioactive isotopes from meteorites to calculate the distance and time of a nearby supernova, suggesting that hundreds or thousands of solar siblings may exist.
A new study reveals the existence of more than one type of Type Ia supernova, with SNLS-03D3bb being over twice as bright and half as massive as typical examples. This finding opens up new possibilities for understanding these cosmic events.
For the first time a star has been observed as it goes supernova – a mind-bogglingly powerful explosion that briefly outshines an entire galaxy. UK scientists used NASA's Swift satellite and a combination of orbiting and ground-based observatories to catch the event in real-time.
Astronomers have linked an X-ray flash to a supernova for the first time, revealing a new class of events with properties distinct from typical gamma-ray bursts. The discovery suggests the existence of dimmer but possibly more numerous cosmic flashes.
Researchers found that at least two objects in the Quintuplet Cluster are binary pairs forming pinwheel stars that live fast and die young. These 'Wolf-Rayet colliding-wind binaries' emit enormous amounts of radiation, with each quintuplet outshining the Sun by 10,000 to 100,000 times.
SNAP, a NASA-supported mission, aims to measure the expansion history of the universe and investigate dark energy. Using two independent techniques, it will analyze thousands of Type Ia supernovae and independently probe the growth structure of the universe.
Astrophysicist Saul Perlmutter wins prestigious International Feltrinelli Prize for his groundbreaking research on dark energy and the accelerating expansion of the universe. The prize recognizes Perlmutter's contributions to our understanding of the universe's mysterious force, dark energy.
Researchers using ESA's XMM-Newton satellite data have found an object in the heart of a 2,000-year-old supernova remnant that exhibits complex and intriguing properties. The object, called 1E161348-5055, has a cycle that repeats every 6.7 hours, which is tens of thousands of times longer than expected for a young neutron star.
Saul Perlmutter, Adam Riess, and Brian Schmidt share the prize for their work on measuring changes in the universe's expansion rate. Their discovery has implications for understanding dark energy and its impact on galaxy distances.
Scientists have long suspected that massive star supernovae produce dust, but previous technology limitations hindered confirmation. A new study reveals that supernovae are indeed a major contributor to the early universe's dust, enabling rapid star formation and heavy element creation.
Researchers found massive-star supernovae to be major space dust factories, producing up to seven thousand earth masses of solid dust particles. This discovery challenges existing theories and provides new insights into the processes that produce dust in the universe, with implications for the formation of comets, planets, and life.
Researchers discovered that supernova remnants in the Small Magellanic Cloud contain up to one-hundredth the amount of dust predicted by current theories. This finding suggests alternative sites of dust formation, such as massive star winds, may be more important contributors to primordial galaxies. The study provides a unique test of ...
The MAGIC team discovered variable gamma-ray emission from microquasar LS I +61 303, revealing a direct relationship between the stars' interplay and gamma-ray production. The findings suggest that gamma-ray emission could be a common property of microquasars, contradicting previous expectations.
Researchers at Ohio State University found that gamma ray bursts are rare and unlikely to occur near our solar system due to the Milky Way's metal content. The study suggests that GRBs pose no danger to life in our galaxy, dismissing theories of mass extinctions caused by these events.
The H.E.S.S. collaboration has discovered gamma-ray emission from a complex of gas clouds near the Milky Way Galaxy's centre, revealing a prehistoric particle accelerator. The density of cosmic rays exceeds that in the solar neighbourhood, suggesting recent acceleration.
Researchers at the University of Illinois created composite images of optical, radio, infrared, ultraviolet and X-ray wavelengths to understand massive stars' impact on their galactic surroundings. The study reveals that massive stars energize and enrich the interstellar medium with strong ultraviolet radiation and fast stellar winds.
Astronomers used Aluminum-26 to estimate supernova frequency and star formation rate in the Milky Way galaxy. The discovery confirms the enrichment process continues to seed elements needed for life.
Researchers at UC Berkeley will invite Internet users to help them search for interstellar dust grains captured by NASA's Stardust spacecraft. The 'virtual microscope' technology allows anyone with an internet connection to scan images of aerogel for tracks left by speeding dust, in hopes of discovering grains from distant stars.
Astronomers have discovered that massive clouds of hot gas in elliptical galaxies are being stirred up by intermittent explosive activity from central super-massive black holes. This finding challenges the long-held assumption that these galaxies are quiet and stable, revealing a more dynamic and stormy reality.
Researchers at McMaster University have discovered 'light echoes' of ancient supernovae, providing a unique opportunity to study the original light from these events. This finding sheds new light on our understanding of the universe and its elements.
Researchers discovered faint visible 'echoes' of three ancient supernovae by detecting centuries-old light reflected by interstellar gas clouds. The oldest echo is likely over 600 years old, offering a chance to study famous supernovae like those observed in 1006 and 400 years ago.
The PULSE collaboration has achieved outstanding scientific results by studying pulsars to test fundamental laws and understand extreme conditions. They discovered the first known double pulsar, confirming Einstein's general theory of relativity.
Researchers confirm that Einstein's cosmological constant behaves like dark energy, driving the acceleration of the universe. The study uses innovative imaging data from the Supernova Legacy Survey, which reveals a precision of 10% and challenges theoretical ideas about dark energy.
A team of researchers discovered that dark energy behaves similarly to Einstein's cosmological constant with a precision of 10%, contradicting several theoretical predictions. The study uses innovative camera technology and observations from multiple telescopes worldwide.
The UltraScience Net enables fast data transfer between research institutions, with speeds of up to 20 Gigabits per second. Fermilab and Caltech successfully tested the system, achieving a rate of 7 Gigabits per second, thousands of times faster than usual high-speed Internet connections.
Physicists Eric Linder and Robert Caldwell separate dark energy scenarios through satellite searches, offering a way to distinguish among dark energy possibilities. The Joint Dark Energy Mission experiments may be able to determine which scenario is correct.
Recent Chandra X-ray Observatory observations have given insight into the behavior of the doomed star before it exploded, indicating that the predicted spectacular brightening of the circumstellar ring has begun. The supernova produced a shock wave that rumbled through the cavity, and recent data indicate that this event has started.
Observations of SN 2003jd reveal aspherical explosion, supporting hypothesis that Type Ic supernovae can produce gamma-ray bursts. The findings also suggest that the direction-dependent shape of the oxygen line is a key indicator of an aspherical explosion.
Astronomers using Spitzer Space Telescope image a new generation of stars at the heads of huge dust pillars created by galactic weather conditions. The Carina Nebula, located 10,000 light years from Earth, is visible to the human eye and contains several dozen massive stars that shape the gigantic dust pillars.
A team of astronomers suggests that Type Ic supernovae could produce gamma-ray bursts through the collapsar model, which proposes an asymmetric explosion mechanism and a jet of particles and energy. The theory is supported by observations with Keck and Subaru telescopes in Hawaii.
Researchers discovered two most chemically primitive stars, HE0107-5240 and HE1327-2326, offering insights into the universe's early stages. These unevolved dwarf stars have iron contents significantly lower than previously known stars, providing a glimpse into the elements produced during supernova explosions.
A total of eight new VHE gamma-ray sources have been found in the Milky Way's disc, doubling known sources at these energies. The discovery includes two 'dark accelerators' without obvious counterparts in other wavelength bands, sparking excitement among astronomers.
A massive gamma-ray flare from a magnetar was detected by the RHESSI satellite, emitting as much energy in two-tenths of a second as the sun gives off in 250,000 years. The event's immense power suggests a solution to the origins of short-duration gamma ray bursts.
A Chinese-American team of scientists has discovered a rare isotope, sulfur-36, associated with sodalite in a meteorite. The finding provides strong evidence for the past presence of chlorine-36 in the early solar system, which was likely formed in a supernova explosion.
The Gemini Observatory has released three striking new images showcasing the 'Fireworks Galaxy', an interacting galaxy pair, and an extremely active stellar nursery. These images highlight the prolific galaxy NGC 6946, which is ablaze with galactic fireworks fueled by the births and deaths of multitudes of brilliant, massive stars.
The Swift X-ray Telescope has successfully captured its first gamma-ray burst afterglow, marking a significant milestone in the mission to understand these mysterious events. The telescope will help scientists pinpoint the location and nature of the explosion, providing crucial clues about the origins of gamma-ray bursts.
Astronomers study remnant of 1,000-year-old supernova to solve long-standing puzzle of cosmic ray origin. They create gamma-ray image using Cherenkov radiation, providing first unequivocal proof that supernovae produce galactic cosmic rays.
A new discovery by Pilar Ruiz-Lapuente and colleagues identifies a clear path for Type Ia supernovae to form in binary star systems. The research found that the companion star is similar to our sun, but slightly older and with high heavy-element content, supporting the theory that Type Ia supernovae originate from these systems.
Using the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory, researchers observed the Kepler's supernova remnant, uncovering a bubble-shaped shroud of gas and dust expanding at 4 million miles per hour. The observations revealed distinct features, including heated interstellar dust and regions of hot gas.
The SNEWS system, an international collaboration of neutrino observatories, aims to provide astronomers with a prompt alert for galactic supernovas. This network can electronically compare data to increase scientists' confidence that a neutrino signal is really from a supernova.
Astronomers have detected high-energy gamma rays emanating from the center of the Milky Way galaxy, sparking debate about the nature of these mysterious emissions. The observation suggests a giant supernova explosion as the possible source, which could accelerate cosmic gamma rays to unprecedented energies.
Astronomers at ESO's Very Large Telescope (VLT) recorded the spectrum of a bright meteor in 2002, providing insights into meteor emissions and atmospheric chemistry. The spectrum revealed telltale emissions of oxygen and nitrogen atoms and molecules, as well as constraints on the role of atmospheric chemistry when life started on Earth.
Astronomers from Johns Hopkins University confirm the Cygnus Loop is closer to Earth than previously thought, with a distance of 1,860 light years. The new findings were obtained using the Far Ultraviolet Spectroscopic Explorer (FUSE) satellite and provide an accurate starting point for understanding this important supernova remnant.
Researchers using European Southern Observatory's Very Large Telescope discovered a unique type Ia supernova that exploded within a flat, dense disk of dust and gas. The findings suggest that this and other precursors resemble protoplanetary nebulae, which may indicate wide differences among their progenitors.
New neutrino research has significant implications for technological advancements and our understanding of the universe. The study aims to improve techniques for making clean materials and detect clandestine nuclear weapons tests, while also shedding light on the role of neutrinos in the early universe and star explosions.
The eSTAR network uses intelligent agents to automatically observe and analyze astronomical events, such as supernovae explosions and black hole activity. The agents can detect and respond to the rapidly changing universe faster than humans, allowing for more efficient science discovery.
A new model suggests that the Big Bang could have been an explosion within a black hole, with the universe expanding into an infinite space. The theory, developed by UC Davis and University of Michigan mathematicians, satisfies Einstein's equations while allowing for expansion.
The study confirms the accelerating expansion of the universe due to dark energy, with data from 11 distant supernovae. It provides more precise measures of matter and dark energy composition in the universe.
A new study analyzing Type 1A supernovae measured with the Hubble Space Telescope sheds light on the nature of dark energy. The results confirm that the universe is expanding at an increasing rate, reinforcing initial discoveries made five years ago.
Gravitational waves are ripples in space-time produced by massive objects' acceleration. The detection of these waves will provide unique information about astrophysical systems like supernovae and black hole formation.
Researchers measured the polarization of light emitted by supernova 2001el, detecting slight flattening at peak brightness, and later spherical symmetry. This discovery helps validate Type Ia supernovae as standard candles for cosmology.
Research by Debra Fischer and Jeff Valenti found a correlation between star metal abundance and planet formation, with metal-rich stars having a 20% chance of harboring planets. The data suggest that a threshold metallicity exists, favoring the formation of planetary systems in stars with higher initial metal content.
A team led by Dr. Loretta Dunne has discovered a thousand times more cosmic dust than previously detected in the remnant of a supernova explosion in our own Galaxy. This finding solves the riddle of how large quantities of dust were formed in the early universe and provides evidence for supernovae as efficient dust factories.