Alexander Fufaev
My name is Alexander FufaeV and here I will explain the following topic:

Emitted Radiant Power of a Black Body

Emitted Radiant Power of a Black Body
A black body (for example, approximately our Sun), with the surface \( A \) and the temperature \( \class{red}{T} \), emits a specific radiant power \( \class{green}{P} \) given by the Stefan-Boltzmann law.