Loi de Stefan-Boltzmann
Last updated: 2026-08-24
Loi de Stefan-Boltzmann — Calculez la puissance rayonnée par un corps noir.
Inputs
Result
Enter values and press Calculate
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How to use it
- Temperature T = 500 K, surface A = 2.m², emissivity ε = 0.85
- Calculate Tâ´ = 500â´ = 6.25×10¹â°
- Multiply: σ × ε × A × Tâ´
- P = 5.670374×10â»â¸ × 0.85 × 2.5 × 6.25×10¹â° ≈ 7533.16 W
Common mistakes
- ⚠️ Using Celsius instead of Kelvin (must be absolute temperature)
- ⚠️ Forgetting emissivity facteur (assumes blackbody)
- ⚠️ Wrong power of temperature (must be T⁴)
Worked example
Find radiated power from a 2.m² surface at 500 K with emissivity 0.85.
The radiated power {power} W is emitted according to the Stefan-Boltzmann law.
Input guide
| Field | Typical range |
|---|---|
| area | Surface area: 0.001 to 1000 m² |
| emissivity | Emissivity: 0.01 to 1.0 |
| T | Temperature: 100 to 5000 K |