A stellar black hole is a type of black hole that is formed from the remnants of a massive star that has undergone gravitational collapse. When a massive star runs out of nuclear fuel, it can no longer support its own mass against the force of gravity, leading to a catastrophic collapse. This collapse results in the formation of a black hole with an incredibly strong gravitational pull.
When a massive star exhausts its nuclear fuel, it can no longer produce the energy needed to support its own mass. The force of gravity then causes the star to collapse under its own weight. If the core of the collapsing star has a mass greater than about three times the mass of the Sun, it will continue to collapse until it forms a black hole.
Here are some key points to remember when studying stellar black holes:
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