It is right to conclude that a type I supernova is what it is because it managed to take out so much matter from its surrounding neighbor until it exceeded a 1.4M Chandrasekhar limit. Exceeding that limit meant that it had to tip over.
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, or in the case of a smaller star, a nova.
A likely progenitor of a Type Ia supernova is a white dwarf star in a binary system, accreting material from a companion star until it reaches a critical mass, triggering a thermonuclear explosion.
A Type Ia supernova is created by the merger of two white dwarfs. This type of supernova occurs when the combined mass of the white dwarfs exceeds a critical limit, leading to a thermonuclear explosion that destroys the star.
A type-I supernova occurs when a white dwarf star accumulates mass from a companion star until it reaches a critical threshold, triggering a runaway nuclear fusion reaction. This causes the white dwarf to explode in a bright supernova event.
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.
No. A supernova is a massive explosion, usually from a dying supermassive star.
SN 1572 or Tycho's Supernova was a supernova type Ia, in the constellation Cassiopeia
A supernova, or in the case of a smaller star, a nova.
A likely progenitor of a Type Ia supernova is a white dwarf star in a binary system, accreting material from a companion star until it reaches a critical mass, triggering a thermonuclear explosion.
Supernova.
A Type Ia supernova is created by the merger of two white dwarfs. This type of supernova occurs when the combined mass of the white dwarfs exceeds a critical limit, leading to a thermonuclear explosion that destroys the star.
A Type II supernova occurs when a massive star with about 8-20 times the mass of the Sun exhausts its nuclear fuel and collapses under its own gravity. The mass required for a Type II supernova is typically around 8 solar masses.
A type-I supernova occurs when a white dwarf star accumulates mass from a companion star until it reaches a critical threshold, triggering a runaway nuclear fusion reaction. This causes the white dwarf to explode in a bright supernova event.
Oops! Not all stars end up as a supernova. To become a Type 2 supernova, the star has to be between 8 and 50 times larger than the Sun.
It will end its life as a type II supernova.
Probably type la supernova