Correct option (c) equal in both cases
Explanation:
The energy radiated per second E, by a body of surface area A, at temperature T K is given by,
E = K σAT4 (Stefan’s Law), where K is relative emissivity
E1 = energy radiated per sec. by first sphere
= Kσ(4π(1)2)(4000)4 = Kσπ (1024 × 1012)J
Similarly, E2 = Kσ [4π(4)2] (2000)4
= K σπ(1024 × 1012)J
∴ E1 = E2