1.

Assuming the sun to be a spherical body of radius R at a temperature of TK, evaluate the total radiant power, incident on earth, at a distance 'r' from the sun (where r_0 is the radius of the earth and sigma is stefan's constant)

Answer»

`(R^(2) sigma T^(4))/( r^(2) )`
`( 4pir_(0)^(2) R^(2) sigma T^(4) )/( r^(2) )`
`( PI r_(0)^(2) R^(2) sigma T^(4) )/( r^(2) )`
`( r_(0)^(2)R^(2) sigma T^(4) )/( 4pir^(2) )`

ANSWER :C


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