Universe
11th Edition
ISBN: 9781319039448
Author: Robert Geller, Roger Freedman, William J. Kaufmann
Publisher: W. H. Freeman
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Chapter 12, Problem 27Q
To determine
The reason behind more oblateness of the Saturn than Jupiter by knowing that Saturn rotates more slowly.
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Compare Titan to Rhea. Estimate the strength of surface gravity on Titan compared to the gravity on Titan. How does this affect the possibility of an atmosphere on each?
Use g=GM/R2
Titan Radius: 2,575 km, Mass: 2.31 x 1021 kg
Rhea Radius: 764 km, Mass: 1.35 x 1023 kg
Chapter 12 Solutions
Universe
Ch. 12 - Prob. 1CCCh. 12 - Prob. 2CCCh. 12 - Prob. 3CCCh. 12 - Prob. 4CCCh. 12 - Prob. 5CCCh. 12 - Prob. 6CCCh. 12 - Prob. 7CCCh. 12 - Prob. 8CCCh. 12 - Prob. 9CCCh. 12 - Prob. 10CC
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- Describe and compare the rings of Saturn and Uranus, including their possible origins.arrow_forwardDescribe the location of the equinoxes and solstices in the Uranian sky. What are the seasons like on Uranus?arrow_forwardHow long does the eastward wind at the equator of Saturn take to circle the planet once at a speed of 500 m/s? Compare this value with the rotation period of the planet. (Note: Necessary data are given in Celestial Profile: Saturn.)arrow_forward
- Both Uranus and Neptune have a blue-green tint when observed through a telescope. What does this color tell you about their atmospheric composition?arrow_forwardUse the information in Appendix G to calculate what you would weigh on Titan, Io, and Uranus’ moon Miranda.arrow_forwardDescribe the interior heat source of Saturn.arrow_forward
- Given the size of Tritons orbit (r = 355,000 km) and its orbital period (P = 5.88 days), calculate the mass of Neptune. (Hint: Use the formula for circular velocity, Eq. 5-1a. The formula requires input quantities in kg and m.)arrow_forwardSaturn’s E ring is broad and thin, and far from Saturn. It requires fresh particles to sustain itself. What is the source of new E-ring particles?arrow_forwardDescribe the composition of Saturn from its center outward. What causes these different internal layers?arrow_forward
- The ions in the inner parts of Jupiter’s magnetosphere rotate with the same period as Jupiter. Calculate how fast they are moving at the orbit of Jupiter’s moon Io (see Appendix G). Will these ions strike Io from behind or in front as it moves about Jupiter?arrow_forwardCompare the interior cutaway sketches of the four Jovian planets in their Celestial Profiles. What interior layer(s) is (are) shown in Jupiter and Saturn but not in Uranus and Neptune, and vice versa?arrow_forward
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