A hypernova is an exceptionally energetic explosion that occurs at the end of a massive star's life cycle. It is characterized by an enormous release of energy, significantly surpassing that of a typical supernova. Hypernovae are typically associated with the collapse of very massive stars—those with at least 30 times the mass of our Sun. When such a massive star exhausts its nuclear fuel, it can lead to the formation of a black hole or neutron star.
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