A star turns into a black hole through a process called gravitational collapse, which occurs at the very end of its life cycle. Throughout its active life, a star maintains stability because the outward pressure from nuclear fusion in its core balances the inward pull of its own gravity. Once the nuclear fuel is completely exhausted, this internal pressure drops to zero, allowing gravity to instantly trigger a catastrophic collapse toward the center. This dramatic fate is reserved exclusively fo
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A star turns into a black hole through a process called gravitational collapse, which occurs at the very end of its life cycle. Throughout its active life, a star maintains stability because the outward pressure from nuclear fusion in its core balances the inward pull of its own gravity. Once the nuclear fuel is completely exhausted, this internal pressure drops to zero, allowing gravity to instantly trigger a catastrophic collapse toward the center. This dramatic fate is reserved exclusively fo
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