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Mechanical Properties Of Fluids

Question
CBSEENPH11019849

Derive the expression for the surface temperature, of sun using solar constant.

Solution
Consider the sun to be a perfectly black body of radius r at temperature T.
According to Stefan’s law, total radiant power of the sun i.e. total energy emitted by the sun in one second is,
straight P subscript sun equals AσT to the power of 4 equals 4 πσr squared straight T to the power of 4 space space space space space space space space space space space space space space space space space.... left parenthesis 1 right parenthesis
Let R be the mean distance between the sun and the earth,
S be the mean value of solar constant.
Then total radiant power of the sun is,
space space space space space space space space space space space straight P subscript sun equals 4 πR squared straight S space space space space space space space space space space space space space space space space... left parenthesis 2 right parenthesis
From (1) and (2),
     4 πσr squared straight T to the power of 4 equals 4 πR squared straight S space

rightwards double arrow space space space space space space space straight T equals fourth root of fraction numerator straight R squared straight S over denominator σr squared end fraction end root