21st Century Astronomy
21st Century Astronomy
6th Edition
ISBN: 9780393428063
Author: Kay
Publisher: NORTON
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Chapter 14, Problem 25QP
To determine

The effect of sun on orbiting satellites and telescopes.

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Calculate the total amount of radiative energy per second intercepted by Mars from the Sun using the flux of radiation from the Sun at Mars' orbital radius. Flux of radiation from the Sun at Mars' orbital radius is 597 W m-2. The luminosity of the Sun Ls = 3.8×1026 W. Mars orbits at a distance of 2.25×1011 m (1.5 AU) from the Sun. Note: Consider carefully the cross-sectional area Mars presents to the outwards flow of radiative energy when answering this question.
If there were a planet about 9 times as far from the Sun as Earth is, what would its solar constant be?  The solar constant of the Earth is 1350 watts per square meter. This question is not multiple choice. Provide an answer that is in watts per square meter (round to the nearest 10 watts per square meter).
Why is nearly all of the Sun's energy produced in the inner 1.5% of its volume?
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