Toddsterpatriot
Diamond Member
This is known as Stefan-Boltzmann law, which states that the rate of outward radiative energy (per unit area) emitted by an object with temperature T is proportional to the 4th power of T
Did you notice, it doesn't say, "Unless a warmer object is nearby, in that case it stops radiating" It also failed to say, "Unless an object above 0K is nearby, in which case it emits more slowly"
They assume you can grasp the equation one uses when the radiator is not a perfect black body in a vacuum at 0 degrees K....in which P decreases as the difference between T and Tc decreases till P = 0.
Again...sorry this is all so difficult for you to understand.
rate of outward radiative energy (per unit area) emitted by an object with temperature T is proportional to the 4th power of T
Again, no caveats...sorry this is all so difficult for you to understand