- #1
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Hi all,
I have an exam tomorrow on the evolution of stars. Revision is going OK, but I've come across this equation. Some quick help would be very appreciated!
P = αT4
I'll give you some context:
I'm solving a question that states a star in Virial equilibrium is contracting quasi-statically (slowly). What effect would this have on the temperature of a very large star. (can assume gas pressure is a negligible fraction of the total pressure and temperature is uniform).
I've started the question with:
Ω = -3 ∫ P/ρ dm
Cancelled density ρ, by subbing dm = 4πr2ρ
Then the solution I have shows a substitution for pressure P as above:
P = αT4
Using this we can solve the problem by showing temperature T ∝ 1/R
I'm sure the equation is a correct one. I was just wondering if anyone knew a little more on it? When can/can't I use this substitution.
Thanks
I have an exam tomorrow on the evolution of stars. Revision is going OK, but I've come across this equation. Some quick help would be very appreciated!
P = αT4
I'll give you some context:
I'm solving a question that states a star in Virial equilibrium is contracting quasi-statically (slowly). What effect would this have on the temperature of a very large star. (can assume gas pressure is a negligible fraction of the total pressure and temperature is uniform).
I've started the question with:
Ω = -3 ∫ P/ρ dm
Cancelled density ρ, by subbing dm = 4πr2ρ
Then the solution I have shows a substitution for pressure P as above:
P = αT4
Using this we can solve the problem by showing temperature T ∝ 1/R
I'm sure the equation is a correct one. I was just wondering if anyone knew a little more on it? When can/can't I use this substitution.
Thanks