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Why do stars die?

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Answer: Nuclear fuel depletes

Nuclear fuel depletesCorrect! Stars shine through nuclear fusion—hydrogen fusing to helium in cores. Eventually fuel exhausts. Low-mass stars (like sun): become red giants, shed outer layers (planetary nebulae), leave white dwarf cores. Massive stars (>8 solar masses): fuse heavier elements up to iron, then collapse explosively—supernovae—leaving neutron stars or black holes. Stellar death depends on mass!

Space friction slows themWrong. Space is nearly a vacuum—no friction. Stars die when nuclear fuel exhausts and can't support themselves against gravity.

Black holes consume themWrong. Some stars are consumed by black holes, but most die from fuel depletion—becoming white dwarfs, neutron stars, or black holes.

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