Correct option (c) r2σ(t+273)4/R2
Explanation:
Power P radiated by the sun with its surface temperature (t + 273) K is given by Stefan's Boltzmann law.

where r is the radius of the sun and the sun is treated as a black body where e = 1. The radiant power per unit area received by the surface at a distance R from the centre of the sun is given by
