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When the sun is directly overhead, the thermal energy incident on the earth is 1.4 kWm−2. Assuming that the sun behaves like a perfect blackbody of radius 7 × 105km, which is 1.5 × 108km from the earth show that the total intensity of radiation emitted from the sun is 6.4 × 107 Wm−2 and hence estimate the sun’s temperature.

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The Solar constant S is the heat energy received by 1m2 of earth’s surface per second. If R is the radius of the sun and r the earth-sun distance, then the total intensity of radiation emitted from the sun will be σT4 Wm−2 and from the sun’s surface σT4.4π R2. The radiation received per second per m2 of earth’s surface will be

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