Calculate the peak wavelength of blackbody radiation based on temperature using Wien's displacement law
Learn how to use the Temperature Wavelength Calculator and understand Wien's displacement law
Wien's displacement law states that the wavelength at which the emission of a blackbody is at its maximum intensity is inversely proportional to its temperature. This relationship is crucial in physics and astronomy for determining the temperature of stars and other celestial objects.
This calculator can be used to:
Note: This calculator assumes ideal blackbody radiation. Real objects may deviate from this behavior.