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Paano Kalkulahin si Stefan Boltzmann

Ano ang Stefan Boltzmann?

The Stefan-Boltzmann law quantifies thermal radiation emitted by objects. It states that radiated power is proportional to the fourth power of absolute temperature.

Pormula

The calculator applies P = σ × ε × A × T⁴
P
σ × ε × A × T⁴ — σ × ε × A × T⁴
A
A value — Variable used in the calculation

Step-by-Step na Gabay

  1. 1Enter the object's surface area, emissivity, and temperature
  2. 2The calculator applies P = σ × ε × A × T⁴
  3. 3Results show total radiated power in watts

Mga Nalutas na Halimbawa

Input
A = 1 m², T = 5778 K (Sun), ε = 1
Resulta
P ≈ 63 MW
Intense thermal radiation

Mga Karaniwang Mali na Dapat Iwasan

  • Using Celsius instead of Kelvin for temperature
  • Forgetting to apply the fourth power to temperature

Mga madalas itanong

Why is the T⁴ dependence important?

Small temperature increases dramatically increase radiation; doubling absolute temperature increases power by 16×.

What is emissivity?

Emissivity (0-1) indicates how efficiently an object radiates; 1 is a perfect blackbody, less than 1 reflects some heat.

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