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Q. The solar constant for the earth is $S$. The surface temperature of the sun is $T K$. The sun subtends an angle $\theta$ at the earth.
(1) $S \propto T^{4}$
(2) $S \propto T^{2}$
(3) $S \propto \theta^{2}$
(4) $S \propto \theta$

BHUBHU 2010

Solution:

If $R$ is the radius of the sun and $T$ its temperature, then the energy emitted by the sun per $\sec$ through radiation in accordance with Stefan's law will be given by
$P=A \sigma T^{4}=4 \pi R^{2} \sigma T^{4}$
image
Energy received per unit area per second on the earth of radius $r$
$S=\frac{P}{4 \pi r^{2}}=\frac{4 \pi R^{2} \sigma T^{4}}{4 \pi r^{2}} $
$=\left(\sigma T^{4}\right)\left(\frac{R}{r}\right)^{2}$
$=\frac{1}{4} \sigma T^{4}\left(\frac{2 R}{r}\right)^{2}$
Angle subtended by the sun at the earth,
$\theta=\left(\frac{2 R}{r}\right)$
Or $S=\frac{1}{4} \sigma T^{4} \theta^{2}$