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Question

Parallel rays of light of intensity l=912Wm2 are incident on a spherical black body kept in surroundings of temperature 300 K. Take Stefan-Boltzmann constant σ=5.7× 105Wm2K4 and assume that the energy exchange with the surroundings is only through radiation. The final steady state temperature of the black body is close to:

A
330 K
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B
660 K
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C
990 K
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D
1550 K
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Solution

The correct option is A 330 K
Rate of radiation energy incident on it=Rate of radiation energy lost by the sphere:
Using Stefan Boltzmann's law:
912πr2=σ4πr2(T43004)
where, σ=5.7×105
T330K i.e. option A

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