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Does anyone know what is (roughly) the duration of the Hydrogen burning process
for the sun? Wiki mentions an average lifespan of 10^10 years for sun-like stars, but this includes the red-giant phase. I am interested in knowing (roughly) when Hydrogen fuel gets exhausted as a function of a sun-like star's lifespan, i.e. for stars with: Mass ~ M_{sol} and Type ~ G2V. Many thanks, -- Ioannis |
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