The total radiant energy emitted per unit area from a blackbody's surface is proportional to what power of the blackbody's Kelvin temperature? A) T B) 1/T C) T² D) T⁴

Question

Quizplus · Accepted Answer

The total radiant energy emitted per unit area from a blackbody's surface is proportional to the fourth power of the blackbody's Kelvin temperature, as described by the Stefan-Boltzmann law. This is represented by $T^4$.

The Total Radiant Energy Emitted Per Unit Area from a Blackbody's