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  • The End of Massive Stars: Black Holes and Supernovae Explained
    The final life cycle stage of most massive stars is a black hole.

    Here's why:

    * Massive Stars: These are stars with initial masses 8 times greater than our Sun.

    * Short Lifespan: They burn through their fuel quickly due to their high mass, resulting in a shorter lifespan than smaller stars.

    * Supernova Explosion: When a massive star runs out of fuel, it collapses under its own gravity, triggering a catastrophic explosion known as a supernova.

    * Remnant Core: The core of the star collapses further after the supernova, forming a dense and incredibly strong object.

    * Black Hole Formation: If the core is massive enough (more than about 3 times the mass of our Sun), its gravity becomes so strong that not even light can escape – creating a black hole.

    Other Possible Outcomes:

    While a black hole is the most common outcome, some massive stars can also end their lives as neutron stars. These are incredibly dense objects that form when the core of a massive star collapses, but the mass isn't sufficient to form a black hole.

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