What is Stefan Boltzmann law?

1 Answer
May 9, 2018

The Stefan-Boltzmann law is L=AσT4, where:

  • A = surface area (m2)
  • σ = Stefan-Boltzmann (~5.67108Wm2K4)
  • T = surface temperature (K)

This law is used to find the luminosity (the rate of energy released), for an object given its surface temperature. This law assumes the body acts as a black-body radiator (an object that emits energy from the entire EM spectrum)

For a given object with a constant surface area, the Stefan-Boltzmann law says that luminosity is proportional to the temperature raised to the fourth power.