Parallel rays of light of intensity $I =912 \ Wm ^{-2}$ are incident on a spherical balck body kept in surroundings of temperature $300 \ K$. Take Stefan-Boltzmann constant $\sigma=5.7 \times 10^{-8} Wm ^{-2} K ^{-4}$ and assume that the energy exchange with the surroundings is only through radiation. Th final steady state temperature of the black body is close to:
IIT 2014, Diffcult
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In steady state

$I \pi R ^2= $$ \sigma\left( T ^4- T _0^4\right) 4 \pi R ^2$

$\Rightarrow $$ I =\sigma\left( T ^4- T _0^4\right) 4$

$\Rightarrow $$ T ^4- T _0^4=40 \times 10^8$

$\Rightarrow $$ T ^4-81 \times 10^8=40 \times 10^8$

$\Rightarrow $$ T ^4=121 \times 10^8$

$\Rightarrow $$ T \approx 330 K$

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