Supernovae refer to the sudden expulsion of mass and energy when a large star can no longer fuse material matter. It results from the core collapsing into itself because it no longer has nuclear fusion to counteract it's own gravity and it's too dense for electron degeneracy to prevent collapse.
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No, stars less massive than the Sun do not have enough mass to undergo a supernova explosion. Instead, they may end their lives as a white dwarf or, if they are even less massive, a planetary nebula. Supernovae are events associated with more massive stars.
If enough mass is left over after the supernova explosion, i.e. after material is blown off into space, the star will become a black hole. Less massive stars will become neutron stars. A neutron star can convert to a black hole later, if enough matter falls into it.
it is Supernova
No, our sun is not destined to become a supernova and/or a black hole. It will become a red giant, but it is not massive enough to cross the threshold and become a candidate for a fate like either of those last two.
A supernova is the catastrophic death of a star, characterized by a massive output of energy.
No. A supernova is a massive explosion, usually from a dying supermassive star.
Neutron Star
Never.VY Canis Majoris - WAS a blue supergiant. It is now a red hypergiant and will "soon" become a massive supernova.
Betelgeuse is expected to end its life in a supernova explosion, likely as a Type II supernova due to its massive size and age. This type of supernova occurs when a massive star exhausts its nuclear fuel and collapses under its own gravity.
A supernova occurs at the end of a massive star's life cycle.
Highly unlikely in our lifetime. Altair is still on the main sequence and probably has a few billion years left on it. Even when it comes to the end of the main sequence, it may not have enough mass to become a supernova.
No, the sun will not become a supernova in the future. It is not massive enough to undergo a supernova explosion. Instead, it will eventually expand into a red giant and then shed its outer layers to become a white dwarf.