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Questions  

A black body is at a temperature 300 K. It emits energy at a rate, which is proportional to

a
(300)4
b
(300)3
c
300
d
(300)2

detailed solution

Correct option is A

From Stefan's law the total radiant energy (E) emitted per second per unit surface area of a black body is proportional to the fourth power of the absolute temperture (T) of the bodyi.e., E = σT4where σ is Stefan's constantHence, E directly proportional to (300)4

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