Articles tagged with Type Ii Supernovae
Researchers use Webb to detect large amounts of dust within supernova ejecta, supporting the theory that supernovae supply dust to the early universe. The study reveals over 5,000 Earth masses of dust in one supernova, rivaling previous measurements and suggesting dust can survive internal shocks.
A new study has identified a chemically peculiar star in the Galactic halo as clear evidence of the existence of pair-instability supernovae (PISNe) from very massive first stars. The star's low sodium and cobalt abundances are consistent with predictions for primordial PISN from first-generation stars with 260 solar masses.
Astronomers have imaged a red supergiant star's rapid self-destruction and final death throes before collapsing into a type II supernova. The discovery challenges previous ideas of how red supergiants evolve right before exploding.
Scientists analyzed carbon-rich dust grains extracted from meteorites to determine the timing of supernova dust formation. The study found that these grains formed at least two years after their massive parent stars exploded.
Recent NuSTAR observations of supernova SN 1987A confirm the predicted lopsided nature of stellar giant deaths, with most material moving away from the observer. This finding supports supercomputer simulations that assume asymmetrical core collapse and could help solve the mystery of dual black hole and neutron star formation.
A team of astronomers observed a massive star's mass-loss event about a month before its supernova explosion, providing evidence for a causal link between the two events. The study suggests that predicting such explosions could allow scientists to catch them in action.
Researchers found evidence of a 'penultimate outburst' in a massive star before its final detonation as a supernova, providing the first causal link between the two events. This discovery has significant implications for our understanding of what triggers a supernova.
Scientists used NASA's Chandra X-ray Observatory to capture a rare glimpse of X-radiation from the early phases of a supernova. The observations revealed that the supernova shed a relatively small amount of matter before it exploded, compared to other supernovae.