This law is often used in astronomy to determine the temperature of stars.  Its namesake constant, usually signified by a lower-case beta or sigma, is equal to 0.0029 Kelvin meters.  Derived directly from the inverse of the P
This law is often used in astronomy to determine the temperature of stars.  Its namesake constant, usually signified by a lower-case beta or sigma, is equal to 0.0029 Kelvin meters.  Derived directly from the inverse of the Planck equation, this law can be stated as the result of changing the Planck curve with respect to temperature.  Also related to the Stefan-Boltzmann equation, FTP, identify this law of physics that states that the temperature of a blackbody is inversely proportional to the wavelength of the emitted energy and is not the Rayleigh-Jeans law.
This law is often used in astronomy to determine the temperature of stars.  
Wien's displacement law