Question

Using the Stephan- Boltzmann law, explain why the sun emits more energy than the earth

Answer 1

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Although much hotter on the inside, we can closely approximate the surface of the sun, from which its emission occurs, as a black body at a temperature of about 5800 K. The Stefan-Boltzmann equation then gives the energy flux emitted at the sun’s surface.

SS = (5.67 × 10–8 W·m–2·K–4)(5800 K)4 = 63 × 106 W·m–2

Answer 2

Answer:

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