Wien's Law Calculator
Find the peak emission wavelength of a blackbody.
Wien's law gives the wavelength at which a hot object radiates most strongly.
The math behind it
λ_max = b ÷ T, with Wien's constant b ≈ 2.898 × 10⁻³ m·K. Hotter objects peak at shorter (bluer) wavelengths.
Worked example
The Sun (5778 K) → peak near 502 nm (green).
FAQ
Why do hot metals glow blue-white?
Higher temperature shifts the peak toward shorter wavelengths.