A black hole is the last stage of a large star having mass more than 8-9 solar masses . Reason - When a star left with very less fuel in its core that it is not able to raise its core temperature by nuclear synthesis or it receive some extra matter in such way that it can no longer raise its core temperature, in both these cases star's temperature is not high enough to prevent it from collapsing under its own weight and when it happen two beams of high energy blasting out before the collapsing of the rest of the star (these jets of high energy are called the Gamma ray burst) and finally star explodes and in just one second it will blasting out energy 100 times more than our sun will produce in its entire life . Basically gamma ray burst is the baby cry of a black hole .
A star of our suns size will eventually collapse to a white dwarf star, a small but very dense object. It will remain very hot and will continue to shine as a white dwarf for many millions of years until gradually cooling off to become a black dwarf.
A cataclysmic destruction of the star in a supernova explosion.
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The sun will ultimately become a slowly cooling white dwarf.
A red giant and them ultimately a white dwarf.
Neutron star or Black hole
a nova super nova (death of star)
Black hole.
Multi-rehab memberships, and a very violent and painful return to mediocrity
rrrrr
In many binary stars, there can be a flow of material between the two stars, disturbing the normal process of stellar evolution. As the flow progresses, the evolutionary stage of the stars will advance, even as the relative masses change. Eventually, the originally more massive star will reach the next stage in its evolution despite having lost much of its mass to its companion.
Hydrogen, helium, and carbon fuel are found in more massive stars. The diameter of more massive stars is bigger. Helium is found in greater abundance in more massive stars. The weight of more massive stars is greater.
star birth, protostar stage, main sequence stage, red giant stage, then burnout and death
Multi-rehab memberships, and a very violent and painful return to mediocrity
rrrrr
In many binary stars, there can be a flow of material between the two stars, disturbing the normal process of stellar evolution. As the flow progresses, the evolutionary stage of the stars will advance, even as the relative masses change. Eventually, the originally more massive star will reach the next stage in its evolution despite having lost much of its mass to its companion.
Hydrogen, helium, and carbon fuel are found in more massive stars. The diameter of more massive stars is bigger. Helium is found in greater abundance in more massive stars. The weight of more massive stars is greater.
Sometimes if the conditions are just right a huge diamond! (the final stage of nucleosynthesis of stars that are not more massive is carbon Theoretically, they get dimmer and dimmer until they become "black dwarfs".
Sometimes if the conditions are just right a huge diamond! (the final stage of nucleosynthesis of stars that are not more massive is carbon Theoretically, they get dimmer and dimmer until they become "black dwarfs".
In G-type stars, this would be the white dwarf stage. More massive stars could continue to fuse ever heavier elements, until the fusion products consist mainly of iron, and the stellar core collapses into a neutron star or a black hole.
W. Sutantyo has written: 'The effect of stellar evolution on the synchronous rotation of components of massive close binaries' -- subject(s): Double stars, Evolution, Stars
White dwarf stars.
star birth, protostar stage, main sequence stage, red giant stage, then burnout and death
A supernova can be massive but some aren't. Every supernova is a dieing star. Supernovae are exploding stars. They represent the very final stages of evolution for some stars. Supernovae, as celestial events, are huge releases of tremendous energy, as the star ceases to exist, with about 1020 times as much energy produced in the supernova explosion as our Sun releases every second.
Type II supernova. Formation of a neutron star or black hole.