The primary physical property which would determine whether a star would become a black hole at the end of its life once its fuel is exhausted would be its mass. Stars above a certain mass could possibly collapse and become a black hole, those below that mass might end up as a white dwarf or neutron star. In current theories of stellar evolution, supported by astronomical observation, older stars can evidence instabilities and certain mechanisms can cause the star to explode or otherwise shed mass from its outer envelope out into space - thus, mass alone is certainly not the only quality which would determine the star's fate.
The mass of a star is the fundamental quality that indicates its ultimate fate. A star's mass determines whether it will end its life as a white dwarf, neutron star, or black hole. More massive stars are likely to undergo supernova explosions and collapse into neutron stars or black holes, while lower-mass stars will evolve into white dwarfs.
The mass of the remaining core of a star that has exploded as a supernova. (Although some stars can collapse directly to a black hole without a supernova explosion)If the mass exceeds about 3 to 4 solar masses the degeneracy pressure of neutrons is insufficient to stop the collapse, and the object will inevitably collapse into a black hole.See related link for more information.
The factor that determines whether a neutron star or a black hole forms after a supernova explosion is the mass of the collapsing core of the star. If the core's mass is between about 1.4 and 3 times the mass of the sun, a neutron star is formed. If the core's mass exceeds about 3 solar masses, a black hole is likely to form.
I am not sure whether it is possible to predict whether a specific star will become a black hole or not. The general rule is that the most massive stars will become black holes, but what matters is how much mass when a star runs out of fuel and collapses. Please note that during a supernova explosion, a star may lose a lot of its mass - i.e., it gets blown out into space. In extreme cases, a star may blow up completely, leaving no remainder.
False. Only the most massive stars will become black holes.
The mass of a star is the fundamental quality that indicates its ultimate fate. A star's mass determines whether it will end its life as a white dwarf, neutron star, or black hole. More massive stars are likely to undergo supernova explosions and collapse into neutron stars or black holes, while lower-mass stars will evolve into white dwarfs.
The amount of mass in the remnant. If the mass of the remnant exceeds 3 solar masses then it will become a black hole.
The Sun probably won't turn into a black hole. What determines whether a certain star becomes a black hole is basically the amount of mass left over, once the star runs out of energy. Less massive stars turn into white dwarves; more massive stars into neutron stars; and the most massive of all, into black holes.
The black hole property that determines the Schwarzschild radius of the black hole is that it has mass but no angular momentum nor electric charge.
Its mass
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The mass of the remaining core of a star that has exploded as a supernova. (Although some stars can collapse directly to a black hole without a supernova explosion)If the mass exceeds about 3 to 4 solar masses the degeneracy pressure of neutrons is insufficient to stop the collapse, and the object will inevitably collapse into a black hole.See related link for more information.
The key holding of the Court was that, even if segregated black and white schools were of equal quality in facilities and teachers, segregation by itself was harmful to black students and unconstitutional. This aspect was vital because the question was not whether the schools were "equal", but whether the doctrine of separate was constitutional
A supernova can become a neutron star, or a black hole. Whether it becomes one or the other depends on the mass that remains after the supernova explosion (remember, part of the matter is blown into space). The more massive objects become black holes. As to the "why", this is because after a certain mass limit, there is no known force that can stop gravity.
The factor that determines whether a neutron star or a black hole forms after a supernova explosion is the mass of the collapsing core of the star. If the core's mass is between about 1.4 and 3 times the mass of the sun, a neutron star is formed. If the core's mass exceeds about 3 solar masses, a black hole is likely to form.
I am not sure whether it is possible to predict whether a specific star will become a black hole or not. The general rule is that the most massive stars will become black holes, but what matters is how much mass when a star runs out of fuel and collapses. Please note that during a supernova explosion, a star may lose a lot of its mass - i.e., it gets blown out into space. In extreme cases, a star may blow up completely, leaving no remainder.