Assuming the Sun to be a spherical body of radius R at a temperature of TK, evaluate the total radiant powered incident of Earth at a distance r from the sun
where `r_0` is the radius of the Earth and `sigma` is Stefan's constant.

Options

A. `4pir_(0)^(2)R^(2)sigmaT^(4)//r^(2)`
B. `pir_(0)^(2)R(2)sigmaT^(4)//r^(2)`
C. `r_(0)^(2)R^(2)sigmaT^(4)//4pir^(2)`
D. `R^(2)sigmaT^(4)//r^(2)`

Explanation

(b)