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Assuming the Sun to be a spherical body ...

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.

A

`(r_0^2R^2sigmaT^4)/(4pir^2)`

B

`(4pir_0^2R^2sigmaT^4)/(r^2)`

C

`(pir_0^2R^2sigmaT^4)/(r^2)`

D

`(R^2sigmaT^4)/(r^2)`

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