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What is a supernova?

What is a supernova? Here are some definitions.

Noun
  1. (astronomy) A star which explodes, increasing its brightness to typically a billion times that of our sun, though attenuated by the great distance from our sun. Some leave only debris (Type I); others fade to invisibility as neutron stars (Type II).
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A stellar-mass black hole forms when a heavy star collapses under its own weight in a supernova explosion.
Only a dozen such hypergiants are known, and scientists suspect that Rho Cassiopeiae will soon destroy itself in a supernova explosion.
When massive stars die, most of their energy is released as neutrinos in violent supernova explosions.
The astronomers realised that a normal red supergiant alone could not have given rise to such a weird supernova.
The supernova observations call out for some gravitationally repulsive substance to drive the cosmic acceleration.
For nebulas there are emission nebula, reflection nebulas, planetary nebulas, dark nebulas and supernova remnants.

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