`lambda_(max) = (0.0029Km)/ T `

Enter a value for all fields

According to Wien's Law for Blackbody Radiation:
 The peak wavelength is inversely proportional to its temperature in Kelvin.

Anything that emits any kind of heat (or cold) has a peak wavelength. Wien's Law is the equation to use to solve for this:

`Lambda_(max)=0.0029/T`

• `Lambda_(max)` is the wavelength of maximum emission
• `T` is the temperature