The most massive stars will die as black holes.
None at all/ The life cycle of a star is based on it's initial mass, not where it was formed.
The two factors that determine the life cycle path of a star are its mass and composition. A star's mass dictates how it will evolve over time, while its composition affects its energy production and how it will eventually end its life cycle.
mass
a star with 2-3 stellar masses would become a red supergiant then a supernova and then become a neutron star.
High-mass stars might become black holes, if the remaining matter (after the supernova explosion) is sufficiently large.
None at all/ The life cycle of a star is based on it's initial mass, not where it was formed.
The more the mass the shorter their life cycle (the more quickly they use their fuel)
The two factors that determine the life cycle path of a star are its mass and composition. A star's mass dictates how it will evolve over time, while its composition affects its energy production and how it will eventually end its life cycle.
its mass
mass
a star with 2-3 stellar masses would become a red supergiant then a supernova and then become a neutron star.
Yes, a star of low to medium mass, like the sun, will eventually turn into a white dwarf at the end of its life cycle. This occurs after the star has exhausted its nuclear fuel and shed its outer layers.
A star's "life cycle" depends mostly on its initial mass; everything is determined by mass. Small, low-mass stars may shine essentially forever, while very large high-mass stars may grow old and go supernova in only a few dozen million years.
The more massive a star is, the less its life time.
The starting nebula of a medium star cycle and a large star cycle differs primarily in mass and density. Medium stars, like our Sun, typically form from nebulae that have a lower mass and are less dense, allowing for a more gradual accumulation of material. In contrast, large stars originate from more massive and denser nebulae, which can lead to a faster and more violent formation process. This difference in initial conditions influences their subsequent life cycles and eventual fates.
The most important factor in determining a star's life cycle is its mass. The mass of a star determines its size, temperature, and how it will evolve over time. More massive stars have shorter lives and end in a violent supernova explosion, while less massive stars like the Sun will eventually become a white dwarf.
High-mass stars might become black holes, if the remaining matter (after the supernova explosion) is sufficiently large.