Answer:
Step-by-step explanation:
Use radiant energy formula according for Stefan-Boltzmann law,
Qnet/t = AeσT4
Qnet is radiant energy, t is time, σ is Stefan constant, e is emissivity , A is cross sectional area and T is temperature.
Qnet(A)/t = (L0)2eσ(4T0)4 = 256L02eσT04
Qnet(B)/t = (2L0)2eσ(3T0)4 = 85L02eσT04
Qnet(C)/t = (3L0)2eσ(2T0)4 = 25L02eσT04
Thus, Qnet(A)/t > Qnet(B)/t > Qnet(C)/