Blackbody Radiation Calculator
Find radiated power per area from temperature (Stefan–Boltzmann).
A hot object radiates energy that grows steeply with temperature.
The math behind it
Stefan–Boltzmann: j = σ·T⁴. Wien's law gives the peak wavelength λ = b/T.
Worked example
300 K → about 459 W/m², peaking near 9659 nm (infrared).
FAQ
Why does T⁴ matter?
Doubling temperature multiplies radiated power 16-fold.