Universe
11th Edition
ISBN: 9781319039448
Author: Robert Geller, Roger Freedman, William J. Kaufmann
Publisher: W. H. Freeman
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Chapter 11, Problem 14Q
To determine
The surface features found on Mercury, and compare them with the features of the Earth’s Moon. Also state the reasons behind the fact that the features of Mercury are much older than most surface features of Earth.
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Despite being within the sun’s “habitable zone”, both Venus and Mars have average surface temperatures that do not permit the existence of liquid water. Besides albedo, name three other important properties of a planet that can influence its temperature.
Chapter 11 Solutions
Universe
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- Why is there so much more carbon dioxide in the atmosphere of Venus than in that of Earth? Why so much more carbon dioxide than on Mars?arrow_forwardWhy is it not surprising that there is no evidence of plate tectonics on Mercurys surface?arrow_forwardWhat is the composition of the polar caps on Mars?arrow_forward
- Would you expect as many impact craters per unit area on the surface of Venus as on the surface of Mars? Why or why not?arrow_forwardWhat are the advantages of using radar imaging rather than ordinary cameras to study the topography of Venus? What are the relative advantages of these two approaches to mapping Earth or Mars?arrow_forwardHow might Venus’ atmosphere have evolved to its present state through a runaway greenhouse effect?arrow_forward
- What do our current ideas about the origins of the Moon and Mercury have in common? How do they differ?arrow_forwardWhat is the composition of clouds on Mars?arrow_forwardThe smallest detail visible through Earth-based telescopes is about 1 arc second in diameter. What linear size does that correspond to on Mercury when Mercury is at a distance of 1 AU? Can Caloris Basin be resolved? (Hint: Use the small-angle formula, Eq. 3-1.) (Note: 1 AU is 1.5 108 km.)arrow_forward
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