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One of the most luminous stellar explosions ever detected may now be explained. It came from the detonation of a dead star within the dense shell of matter ejected from that sun's companion star, a new study suggests.
Supernovas are explosions that can happen when stars die, either after the stars burn all their fuel or gain a sudden influx of new fuel. These outbursts can briefly outshine all of the other suns in these stars' galaxies, making them visible from halfway across the universe.
Scientists - Class - Star - Supernovas - Explosions
Recently, scientists discovered a rare class of exploding star known as superluminous supernovas. These explosions are up to 100 times brighter than regular supernovas but account for less than 0.1% of all supernovas.
Much remains unknown about what powers superluminous supernovas; they release far more energy than any standard mechanism for powering supernovas can explain. To learn more about what drives these extraordinary explosions, scientists focused on SN 2006gy, one of the first known superluminous supernovas. SN 2006gy occurred in a galaxy 240 million light-years away and was the brightest and most energetic supernova ever recorded when it was discovered, in 2006.
Year - SN - Researchers - Spectrum - Light
A little more than a year after SN 2006gy was spotted, researchers detected an unusual spectrum of light from the supernova. Now, scientists have deduced that this light came from an envelope of iron around the supernova, revealing clues as to what might have caused the explosion.
The researchers developed computer models of what kind of light would be generated by envelopes of iron with various masses, temperatures, clumping patterns and other properties. They found that the wavelengths and energies of light seen from SN 2006gy likely came from a huge amount of iron — "over a third of the sun's mass" — expanding at about 3,355 mph (5,400 km/h), study lead author Anders Jerkstrand, an astrophysicist at...
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