All evolutionary differences between high- and low-mass stars can be attributed to differences in the amount of gravity each star possesses.
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Q1: Most of the uranium Q5: The production of large numbers of neutrons Q6: We can determine the age of a Q6: Gravitational lensing allows us to see distant Q6: Einstein's special theory of relativity implies that Q11: As a high-mass main-sequence star evolves off Q17: The densest state of matter found in Q18: Black holes emit no light whatsoever. Q18: Fusion reactions that create chemical elements heavier Q19: High-mass stars differ from low-mass stars in![]()
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