Calculate the surface temperature of a star from the wavelength at which it emits maximum radiation. Wien's displacement law relates peak wavelength inversely to temperature.
Enter your values below
Wavelength of maximum emission
Default: 2.898×10⁻³ m·K
How this calculator works
Temperature equals Wien's displacement constant (2.898×10⁻³ m·K) divided by the peak emission wavelength.
Common questions about this calculator
These calculators are for educational and informational purposes only. While we strive for accuracy, results should be verified for critical applications. Always consult authoritative sources for engineering or scientific work.
