The supernova's spectrum was unusual, and the analysis indicated that the supernova's precursor star only could have been a giant weighing at least 200 times the mass of our Sun and initially containing few elements besides hydrogen and helium — a star like the very first stars in the early universe.
"Because the core alone was some 100 solar masses, the long-hypothesized phenomenon called pair instability must have occurred," said astrophysicist Peter Nugent, a member of the SNfactory. "In the extreme heat of the star's interior, energetic gamma rays created pairs of electrons and positrons, which bled off the pressure that sustained the core against collapse."
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