Use the following formula (fitted to data) L Mo/year gR M = -4x10-13n for the mass loss of asymptotic giant branch stars to: a) explain why L, g (gravity on surface), and R enter the equation the way they do (nominator or denominator). b) show that the expression for M is equivalent to LR M = -4x10-137 Mo/year - M c) estimate the mass loss rate of a star with M = 1 Mo, L = 7000 Lo,T = 3000 K. Assume n = 1 and use the Stefan-Boltzmann equation to calculate R (in Ro). %3D
Use the following formula (fitted to data) L Mo/year gR M = -4x10-13n for the mass loss of asymptotic giant branch stars to: a) explain why L, g (gravity on surface), and R enter the equation the way they do (nominator or denominator). b) show that the expression for M is equivalent to LR M = -4x10-137 Mo/year - M c) estimate the mass loss rate of a star with M = 1 Mo, L = 7000 Lo,T = 3000 K. Assume n = 1 and use the Stefan-Boltzmann equation to calculate R (in Ro). %3D
Stars and Galaxies (MindTap Course List)
10th Edition
ISBN:9781337399944
Author:Michael A. Seeds
Publisher:Michael A. Seeds
Chapter12: Stellar Evolution
Section: Chapter Questions
Problem 7P
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