Use eqn. 8.4 (F = σT4) to show why the total flux of solar radiant energy is about 105 times greater than that from the Earth.

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Chapter9: The Formation And Structure Of Stars
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Problem 15RQ: Step-by-step, explain how energy flows from the center of the Sun to Earth.
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Chapter #8, Question #2:

Use eqn. 8.4 (F = σT4) to show why the total flux of solar radiant energy is about 105 times greater than that from the Earth.

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