question archive Theory: Luminosity=4⋅π⋅σ⋅R2⋅T4 where R is the radius of the star, T=temperature, σ=a constant
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Theory: Luminosity=4⋅π⋅σ⋅R2⋅T4 where R is the radius of the star, T=temperature, σ=a constant.
What is the temperature of a star whose luminosity is 1,000⋅LSun and whose radius is 10⋅RSun
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