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Question

The surface temperature of the Sun is T0 and it is at average distance d from a planet. The radius of the Sun is R. If θ is the angle subtended by the Sun at the planet, then temperature at which planet radiates energy is proportional to

A
θ1/2
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B
θ2
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C
θ1/2
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D
θ
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Solution

The correct option is C θ1/2
Let, r= Radius of planet
T1= Temperature of planet at which energy is radiated

Power radiated by Sun, P=πR2σT40

Energy received by planet

=P4πd2×πr2=R2T40πr2σd2

Energy radiated by planet

=4πr2σT41

For thermal equilibrium,

=R2T40πr2σd2=4πr2σT41

R2T40=4d2T41

R2T4=4d2T41

T1=TR2d

As we know from the figure that
2R=d×θ

d=2Rθ

T1=TR×θ2×2R

T1=Tθ4

T1θ1/2

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