Stellar Life Cycle
When stars exhaust their nuclear fuel, they undergo dramatic transformations, collapsing under gravity. A white dwarf, incredibly dense yet small, can evolve into a neutron star, where neutron degeneracy pressure fights against gravitational collapse. If mass continues to accumulate, the neutron star can ultimately become a black hole, a region where gravity is so intense that even light cannot escape, challenging our understanding of reality itself.In this clip
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Black Holes
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