For stars on the main sequence, how does luminosity (L) typically scale in relation to mass (M)?
Answer
Luminosity is proportional to mass raised to a power around 3.5 ($L arar ext extvisiblespace M^{3.5}$)
For stars on the main sequence, luminosity scales steeply with mass, specifically being proportional to the mass raised to a power around 3.5 ($L arar ext extvisiblespace M^{3.5}$).
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