He assumed that the lines in the spectrum come from electrons moving from one stable orbit to another, and the wavelength of the light emitted equals the energy difference of the orbits.
This page explores blackbody radiation, emphasizing its importance in physics and key laws such as Stefan-Boltzmann and Wien’s Displacement Law, which link emitted power and peak wavelength to tempera...This page explores blackbody radiation, emphasizing its importance in physics and key laws such as Stefan-Boltzmann and Wien’s Displacement Law, which link emitted power and peak wavelength to temperature. It details historical contributions from scientists like Kirchhoff and discusses thermal radiation concepts, including the sun's output. The Rayleigh-Jeans Law's limitations are highlighted, notably the ultraviolet catastrophe, which arises from its failure at high frequencies.
