Heat Transfer

Thermal Radiation Calculator

Stefan–Boltzmann net radiation and the radiation coefficient.

Tool no.
ECT-F10
Rev
1.0
Updated
Oct 2026
Method
Stefan–Boltzmann law
How to use this calculator

Pick a surface to fill in its emissivity, then enter the area and the surface and surroundings temperatures in any scale.

Formulas

Net exchange (small surface, large surroundings)Q = εσA(Ts⁴ − Tsur⁴)  σ = 5.670 × 10⁻⁸ W/m²·K⁴
Radiation coefficienthr = εσ(Ts + Tsur)(Ts² + Tsur²)

Worked example

1 m² black-painted surface at 100 °C in a 20 °C room (the default)

  1. Ts = 373.15 K, Tsur = 293.15 K.
  2. Q = 0.95 × 5.670 × 10⁻⁸ × 1 × (373.15⁴ − 293.15⁴) = 647 W.
  3. hr ≈ 8.1 W/m²·K, comparable to natural convection in air.

Frequently asked questions

Why must temperatures be in kelvin?

The law depends on T⁴ of absolute temperature. Using Celsius would give completely wrong numbers.

What is emissivity?

How well a surface radiates compared with a perfect black body, from 0 to 1. Shiny metals reflect most radiation and emit little; most painted or oxidized surfaces are 0.8–0.95.