1.

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)

Answer»

`(Q)/(4piR^(2)SIGMA)`
`((Q)/(4piR^(2)sigma))^(-1/2)`
`((4piR^(2)Q)/(sigma))^(1/4)`
`((Q)/(4piR^(2)sigma))^(1/4)`

SOLUTION :From Stefan-Boltzmann.s LAW,
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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