Question

The total rate of emission of energy
by a body per unit area is proportional
to :
(A) T2
(B) T!
(C) T3
(D) T
Here, T is the temperature.​

Answer 1

Answer:

It states that the rate of emission of radiant energy by unit area of a perfectly black body is directly proportional to the fourth power of its absolute temperature. exchange, i.e., is the net loss of heat really the difference in the heat radiated by hot body and that absorbed by it from its surroundings