Correct option is C
Stefan's law of radiation, also known as the Stefan-Boltzmann law, states that the total energy radiated per unit surface area of a black body per unit time (also known as the radiant heat power) is directly proportional to the fourth power of the black body's absolute temperature (T).
Mathematically, it is expressed as:
Eb=σ×T4
where Eb is the emissive power of a blackbody,
T is absolute temperature, and σ =5.67×10-8)