The surface of the Sun has a temperature of5500 °C. (a) Treating the Sun as a perfect blackbody, with an emissivity of 1.0, find the power that it radiates into space. The radius ofthe Sun is 7.0 * 108m, and the temperature of space can be takento be 3.0 K. (b) The solar constant is the number of watts of sunlightpower falling on a square meter of the Earth’s upper atmosphere.Use your result from part (a) to calculate the solar constant, giventhat the distance from the Sun to the Earth is 1.5 * 1011m.

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Chapter1: Units, Trigonometry. And Vectors
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The surface of the Sun has a temperature of
5500 °C. (a) Treating the Sun as a perfect blackbody, with an emissivity of 1.0, find the power that it radiates into space. The radius of
the Sun is 7.0 * 108m, and the temperature of space can be taken
to be 3.0 K. (b) The solar constant is the number of watts of sunlight
power falling on a square meter of the Earth’s upper atmosphere.
Use your result from part (a) to calculate the solar constant, given
that the distance from the Sun to the Earth is 1.5 * 1011m.

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