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Question

The radiant energy from the sun, incident normally at the surface of earth, is 20kcal/m2 min. What would have been the radiant energy incident normally on the earth, if the sun had a temperature twice of the present one?

A
40 kcal/(m2 - min)
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B
80 kcal/(m2 - min)
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C
160 kcal/(m2 - min)
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D
320 kcal/(m2 - min)
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Solution

The correct option is C 320 kcal/(m2 - min)
From the stefan's-boltzman law ET4
E1=20(kcal)/(m2min)
T=200.25=2.11oC
If temperature will increased two times so final temperature will be 2T=T2=4.22oC
Now, the final radiative power E2=T24=320kcalm2min

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