Physics
Blackbody Radiation Calculator
Find radiated power per area from temperature (Stefan–Boltzmann).
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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).
Frequently Asked Questions
Why does T⁴ matter?
Doubling temperature multiplies radiated power 16-fold.
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