According to Stefan Boltzmann law, the total radiation from a black body per second per unit area is directly proportional to the
A
Absolute temperature
B
Square of the absolute temperature
C
Cube of the absolute temperature
D
Fourth power of the absolute temperature
Correct Answer: Fourth power of the absolute temperature
Stefan-Boltzmann law, statement that the total radiant heat power emitted from a surface is proportional to the fourth power of its absolute temperature.