स्टेफॉन वोल्ज़मान नियम
Also known as Stefan's law, Stefan-Boltzmann's law
physical law on the emissive power of black body
AI overview
The Stefan-Boltzmann law describes how much energy a perfectly absorbing and emitting object (called a black body) radiates based on its temperature. This law matters because it helps scientists understand heat radiation from stars, planets, and other objects, and is fundamental to fields like astronomy and climate science.
AI-generated from the Wikipedia summary — may contain errors.
Wikidata facts
Show 1 more fact
- Commons category
- Stefan-Boltzmann law
Sources (1)
via Wikidata · CC0