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Main sequence stars obey a massluminosity relation of the form LNMV with v z 3. Use this fact to argue that more massive stars have
Main sequence stars obey a massluminosity relation of the form LNMV with v z 3. Use this fact to argue that more massive stars have shorter main-sequence lifetimes that less massive ones. The Sun's main-sequence lifetime is approximately 9 billion years. a What are the main-sequence lifetimes of stars with masses of 100 solar masses and 0.1 solar masses
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