(a) Estimate the Eddington luminosity of a 0.072 Mo star and compare your answer to the main-sequence luminosity given in Problem tion pressure likely to be significant in the stability of a low-mass main-sequence star? 21. Assume k = 0.001 m² kg¯'. Is radia-

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(a) Estimate the Eddington luminosity of a 0.072 M, star and compare your answer to the
main-sequence luminosity given in Problem 21. Assume k = 0.001 m² kg¯'. Is radia-
tion pressure likely to be significant in the stability of a low-mass main-sequence star?
(b) If a 120 Mo star forms with log1o T. = 4.727 and log1o(L/Lo) = 6.252, estimate its
Eddington luminosity. Compare your answer with the actual luminosity of the star.
Transcribed Image Text:(a) Estimate the Eddington luminosity of a 0.072 M, star and compare your answer to the main-sequence luminosity given in Problem 21. Assume k = 0.001 m² kg¯'. Is radia- tion pressure likely to be significant in the stability of a low-mass main-sequence star? (b) If a 120 Mo star forms with log1o T. = 4.727 and log1o(L/Lo) = 6.252, estimate its Eddington luminosity. Compare your answer with the actual luminosity of the star.
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