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Radius of a star acting like perfect black body is R, then at what temperature the rate of radiation will be Q ? (Where sigma= Stefun - Boltzman constant) |
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Answer» `(Q)/(4piR^(2)SIGMA)` Here, Q is taken in place of P. `:.Q=AsigmaeT^(4)` `:.Q=4pir^(2)sigmaT^(4)""(because e=1)` `:.T=((Q)/(4pir^(2)sigma))^(1/4)` |
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