Every object with a temperature above absolute zero emits electromagnetic radiation that follows a characteristic distribution known as blackbody radiation. The wavelength at which this distribution reaches its maximum intensity is governed by Wien’s displacement law, which links the peak wavelength directly to the object’s temperature.
In stellar astrophysics, Wien’s law is a powerful tool for estimating a star’s surface temperature from its observed spectrum. Hotter stars peak at shorter (bluer) wavelengths, while cooler stars emit most strongly at longer (redder) wavelengths. This relationship underpins the spectral classification of stars and helps astronomers infer physical properties such as luminosity and radius.
The calculator below implements Wien’s law, allowing you to input a temperature in kelvin and instantly obtain the corresponding peak wavelength. You can view the result in meters, nanometers, or micrometers, making it easy to compare with observational data.
T = temperature of the blackbody in kelvin (K)
What is Wien’s displacement law?
How do I use this calculator for a star?
What does it mean if a star has a shorter peak wavelength?
Can this calculator be used for planets too?
What units should I use for the temperature?
How accurate is this calculator?
What is the significance of the peak wavelength in astronomy?
Results are for informational purposes only and do not constitute professional advice.
