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**See also:** Stefan Stefan's

**1.** What is *Stefan boltzmann* Law? According to *Stefan boltzmann* law, the amount of radiation emitted per unit time from an area A of a black body at absolute temperature T is directly proportional to the fourth power of the temperature

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**2.** *Stefan boltzmann* Constant is denoted by Greek letter σ

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**3.** The *Stefan boltzmann* Constant, σ, is equal to 5.67 x 10-8 W/(m2 • K4)

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**4.** *Stefan boltzmann* constant – Uses and application

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**5.** *Stefan boltzmann* Law is also known as Stefan's Law

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**6.** The *Stefan boltzmann* Law is a means of determining total energy radiated by any object, based entirely on its temperature

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**7.** Set this parameter equal to the *Stefan boltzmann* constant

Set, Strong, Stefan

**8.** For example, *Stefan boltzmann* = 5.669 × 10 −8 joule per sec m 2 kelvin 4 in SI units

Strong, Stefan, Sec, Si

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