Physics: Principles with Applications (7th Edition)

Published by Pearson
ISBN 10: 0-32162-592-7
ISBN 13: 978-0-32162-592-2

Chapter 33 - Astrophysics and Cosmology - Questions - Page 980: 6

Answer

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Work Step by Step

Adjustments needed when measuring parallaxes from the moon (2 methods): i. See figure 33-11. You could perform measurements two weeks apart, letting the moon and Earth play the role of the Earth and the sun in the diagram, respectively. The distance d shown in that diagram would be the Earth–moon distance. ii. See figure 33-11. You could perform measurements six months apart, and at full moon both times. In that case, since you’re observing from the moon, the distance d shown in that diagram would then be the Earth–moon distance plus the distance between the Earth and the sun. Adjustments needed when measuring parallaxes from Mars: See figure 33-11. Let Mars play the role of the Earth in the diagram. You would need to know the length T of a Martian “year” (which, incidentally, is 687 Earth days) and make measurements spaced in time by T/2. Also, the distance d shown in that diagram would be the sun-Mars distance.
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