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  • Supernova Remnants: How Star Mass Dictates the Final Outcome
    The factor that determines what happens to a star after a supernova is its mass.

    - If the star is less massive than about 8 solar masses, it will collapse into a white dwarf. A white dwarf is a very dense star that is supported by electron degeneracy pressure.

    - If the star is between about 8 and 25 solar masses, it will collapse into a neutron star. A neutron star is an even denser star that is supported by neutron degeneracy pressure.

    - If the star is more massive than about 25 solar masses, it will collapse into a black hole. A black hole is a region of spacetime where gravity is so strong that nothing, not even light, can escape.

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