For the PP chain 0.7% of the mass participating in nuclear fusion is liberated as energy which produces a star's luminosity. Assume that the core of a main sequence star consists of 10% of its total mass. Hence, estimate the lifetime of a star on the main sequence in terms of its luminosity L/Lo. Give your answer in years. You may use the observed mass-luminosity relation L x M³.5, where M is the star's total mass. Using typical values, calculate estimates for the main sequence lifetime of a KO star and a 05 star. Describe briefly why your estimate might be more accurate for K stars compared to O stars.

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For the PP chain 0.7% of the mass participating in nuclear fusion is liberated as energy which
produces a star's luminosity. Assume that the core of a main sequence star consists of 10% of its
total mass. Hence, estimate the lifetime of a star on the main sequence in terms of its luminosity
L/L. Give your answer in years. You may use the observed mass-luminosity relation L x M³.5,
where M is the star's total mass.
Using typical values, calculate estimates for the main sequence lifetime of a KO star and a 05
star. Describe briefly why your estimate might be more accurate for K stars compared to O stars.
Transcribed Image Text:For the PP chain 0.7% of the mass participating in nuclear fusion is liberated as energy which produces a star's luminosity. Assume that the core of a main sequence star consists of 10% of its total mass. Hence, estimate the lifetime of a star on the main sequence in terms of its luminosity L/L. Give your answer in years. You may use the observed mass-luminosity relation L x M³.5, where M is the star's total mass. Using typical values, calculate estimates for the main sequence lifetime of a KO star and a 05 star. Describe briefly why your estimate might be more accurate for K stars compared to O stars.
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