Q. Assuming the sun to be a spherical body of radius $R\ $at a temperature of $T\ K$, evaluate the total radiant power, incident on earth, at a distance $r$ from the sun Where $r_{0}$is the radius of the earth and $\sigma$ is stefan’s constant.v

A) $\frac{4\pi r_{0}^{2}R^{2}\sigma T^{4}}{r^{2}}$
B) $\frac{\pi r_{0}^{2}R^{2}\sigma T^{4}}{r^{2}}$
C) $\frac{r_{0}^{2}R^{2}\sigma T^{4}}{4\pi r^{2}}$
D) $\frac{R^{2}\sigma T^{4}}{r^{2}}$
Explanation

(b) From Stefan’s law, the rate at which energy is radiated by sun at its surface is$P = \sigma \times 4\pi r^{2}T^{4}$
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[Sun is a perfectly black body as it emits radiations of all wavelengths and so for it $e$=1.]
The intensity of this power at earth’s surface(under the assumption $r$>>$r_{0})$ is
$I = \frac{P}{4\pi R^{2}} = \frac{\sigma \times 4\pi r^{2}T^{4}}{4\pi R^{2}} = \frac{\sigma R^{2}\sigma T^{4}}{r^{2}}$
The area of earth which receives this energy is only one-half of total surface area of earth, whose projection would be $\pi r_{0}^{2}$.
$\therefore$ Total radiant power as received by earth
$= \ \pi r_{0}^{2} \times I$
= $\frac{\pi r_{0}^{2} \times \sigma R^{2}T^{4}}{r^{2}} = \frac{\pi r_{0}^{2}R^{2}\sigma T^{4}}{r^{2}}$

Dr. Abubacker
Reviewed by Dr. Abubacker

Physics Educator & NEET/JEE Specialist

Ph.D. in Physics with 19+ years of teaching experience.