+The [Stefan Boltzmann Law](/wiki/stefan_boltzmann_law) elegantly describes the total radiant energy emitted by an ideal [Black Body](/wiki/black_body) surface. It reveals that this power, across all wavelengths, is profoundly proportional to the fourth power of its absolute [Temperature](/wiki/temperature).
+## See also
+- [Thermal Radiation](/wiki/thermal_radiation)
+- [Planck's Law](/wiki/plancks_law)
+- [Wien's Law](/wiki/wiens_law)
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