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Physics Dad
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I have a question for my Astro homework and I am a little unsure as to whether I am going in the right direction
Question
Using an expression that relates luminosity, size and temperature of a star, and assuming all Main Sequence stars have the same mean density, determine the relationship between stellar radius and effective temperature.
Relevant equations
L=4πR2σT4
L∝M3.5
Attempt at a solution
My thinking is to use the solar version of the above equation and this one, dividing one by the other to get rid of the 4π and σ and making...
R=RΘ(√(L/LΘ))(TeffΘ/Teff)2
However I don't know if I am supposed to just have R and T with no other variable.
Any guidance would be appreciated.
Question
Using an expression that relates luminosity, size and temperature of a star, and assuming all Main Sequence stars have the same mean density, determine the relationship between stellar radius and effective temperature.
Relevant equations
L=4πR2σT4
L∝M3.5
Attempt at a solution
My thinking is to use the solar version of the above equation and this one, dividing one by the other to get rid of the 4π and σ and making...
R=RΘ(√(L/LΘ))(TeffΘ/Teff)2
However I don't know if I am supposed to just have R and T with no other variable.
Any guidance would be appreciated.
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