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ppy
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Homework Statement
For main sequence stars, the mass–luminosity relation can be approximated by L[itex]\propto[/itex]M[itex]^{3.5}[/itex]
f) If luminosity and mass are both measured in solar units, what is the constant of
proportionality? {2}
I know that the luminosity value of the sun is 4x10[itex]^{26}[/itex]W and
M = 2x10[itex]^{30}[/itex] kg