hypernova
Gamma-ray bursts (GRB) have left astronomers scratching their heads since the late 1960s when they were discovered by U.S. military satellites. Part of the mystery began to unlock when astronomers at Northwestern University detected the first observational evidence for the remnants of hypernovae, explosions hundreds of times more powerful than supernovae, last year. Hypernovae may be the possible source of GRBs, making them the most energetic events known in the Universe besides the Big Bang. Northwestern astronomer Daniel Wang identified two hypernova remnants in galaxy M101, also known as the Pinwheel galaxy some 25 million light years away, in April 1999. The remnants were previously thought to be supernovae remnants, but Wang detected strong X-ray emission from them which led him to believe it was an explosion much more powerful than a supernova. One nebula, MF83, has a radius of over 430 light years and is one of the largest remnants known. The other nebula, NGC5471B, is expanding very fast at a velocity of 100 miles per second. The X-ray light from these nebulae is brighter than the brightest supernova remnants known. After Wang ca
Bohdan Paczynski, of Princeton University, first introduced the concept of a hypernova in 1998 as a why to explain GRBs. Gamma-ray bursts are brief but intense blasts of high-energy radiation. They only last for about 3 seconds, but in that brief time they can release enough energy to be more luminous than the rest of the universe. Paczynski theorized that a hypernova is most likely related to the formation of black holes. The collapse of a massive star and/or its merger with a neutron star could generate more energy than an average star explosion. This is a very possible theory because they have found evidence that GRBs appear close to massive star-forming regions. supernova explosion. Using Hubble's Space Telescope Imaging Spectrograph, On April 25, 1998, The galaxy ESO 184-G82 was host to a combined GRB and The Burst and Transient Source Experiment (BATSE) instrument aboard NASA's Compton Gamma Ray Observatory satellite has recorded more than 2,000 bursts, about one a day, since its launch in 1991. It also plotted their positions all around the sky and found that GRBs don't concentrate in the plane of the Milky Way, where most
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