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Option 3 : Wm-2k-4
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CONCEPT:

  • Stefan's Law: According to it the radiant energy emitted by a perfectly black body per unit area per sec (i.e. emissive power of black body) is directly proportional to the fourth power of its absolute temperature i.e.

\(E \propto {T^4}\)

\( \Rightarrow E = \sigma {T^4}\)

Where, is a constant called Stefan’s constant.

  • The value of Stefan's constant is 5.67 × 10-8 W/m2K4.

EXPLANATION:

  • From the above, it is clear that the unit of Stefan's constant is Wm-2k-4. Therefore option 3 is correct.
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