Describe the spectral distribution of energy in black body radiation?

The spectral distribution of energy in black body radiation is described by Planck's law, which shows that the intensity of radiation emitted by a black body as a function of wavelength is dependent on its temperature. As the temperature increases, the peak of the emitted radiation shifts to shorter wavelengths, a phenomenon known as Wien's displacement law. The distribution is continuous and features a characteristic curve that rises steeply at lower wavelengths, reaches a maximum, and then falls off at higher wavelengths. This distribution illustrates that black bodies emit a wide range of wavelengths, with the total energy emitted increasing with temperature, as described by the Stefan-Boltzmann law.