Stefan–Boltzmann Law

Stefan-Boltzmann law, states that the total radiant heat energy emitted from a surface is proportional to the fourth power of its absolute temperature. The radiation energy per unit time from a black body is proportional to the fourth power of the absolute temperature and can be expressed with Stefan-Boltzmann Law as: The Stefan-Boltzmann Constant. Radiate energy = (Emissivity) * (Stefan-Boltzmann … Read moreStefan–Boltzmann Law