All dead big stars do not form black holes because sometimes the collapse of the star is stopped at a smaller size before it becomes a black hole.
Yes. When the most massive stars die, their cores collapse to form black holes.
Most black holes are believed to form when very massive stars die.
Yes. When the most massive stars die, their cores collapse to form black holes.
Most black holes form when massive stars exhaust their fuel and their cores collapse. There are also supermassive black holes at the centers of most galaxies. Scientists are not sure how supermassive black holes form.
False. Medium-sized stars become white dwarfs. Only the most massive stars form black holes.
Mostly in galaxies, where they can form Super Massive Black Holes.
No. Only the most massive stars form black holes. When the sun dies it will form a white dwarf.
Most black holes are stellar mass black holes with masses comparable to those of large stars as they form from the collapse of massive stars. Scientists know of the existence of supermassive black holes that are millions to billions of times the mass of our sun and can be found in the centers of most galaxies. Scientists still do not know how these black holes become so massive.
Black holes form when massive stars collapse under their own gravity. The intense gravitational pull of a black hole traps everything, including light. Black holes are hot because of the high temperatures and energy generated by the matter falling into them, which creates intense radiation and heat.
black holes come from dead stars like our sun it may turn into one when they die they become really big then explode and some become into a black hole if not it becomes into a black or white dwarf
Black holes are formed by super massive stars when they collapse. Less massive stars will form neutron stars. Therefore, the original size and mass of the star will determine if a black hole will be created when the star collapses.
There are more white dwarfs. Only the most massive stars can form black holes. White dwarfs form from low to medium mass stars, which far outnumber the supermassive ones.