Rate of radiation by a black body is 'R' at temperature 'T'. Another body has same area but emissivity is 0…
- $\quad(162) \mathrm{R}$
- $\quad(81) \mathrm{R}$
- $\quad(16.2) \mathrm{R}$
- $(8.1) \mathrm{R}$
Solution
For another body, $\begin{aligned} \left(\frac{\mathrm{dQ}}{\mathrm{dt}}\right)_2 & =\mathrm{e}^{\prime} \mathrm{A}^{\prime} \sigma\left(\mathrm{T}^{\prime}\right)^4 \\ & =0.2 \mathrm{~A} \sigma(3 \mathrm{~T})^4 \\ & =16.2 \mathrm{~A} \sigma \mathrm{~T}^4 \\ & =16.2\left(\frac{\mathrm{dQ}}{\mathrm{dt}}\right)_1=16. 2 \mathrm{R} \end{aligned}$
Asked in: MHT CET 2024 (10 May Shift 2)
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