Chapter 14: Problem 1
Could astronomers in antiquity have seen Uranus? If so, why was it not recognized as a planet?
Chapter 14: Problem 1
Could astronomers in antiquity have seen Uranus? If so, why was it not recognized as a planet?
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Get started for freeCompare the rings that surround Jupiter, Saturn, Uranus, and Neptune. Briefly discuss their similarities and differences.
It is thought that Pluto's tenuous atmosphere may become even thinner as the planet moves toward aphelion (which it will reach in 2113), then regain its present density as it again moves toward perihelion. Why should this be?
Briefly describe the evidence supporting the idea that Triton was captured by Neptune.
Why do you suppose the tilt of Uranus's rotation axis was deduced from the orbits of its satellites and not by observing the rotation of the planet itself?
Use the Stary Night Enthusiast \({ }^{\text {TM }}\) program to observe the five large satellites of Uranus. Open the Favourites pane and click on Guides \(>\) Atlas to display the entire celestial sphere. Open the Find pane and double- click the entry for Uranus to center this planet in the view. (Clicking once on the Space bar will speed up this centering). You can reduce the confusion in this view by removing the background stars by clicking on View \(>\) Stars \(>\) Stars and by ensuring that the celestial grid is removed by clicking on View > Celestial Grid. Using the controls at the right-hand end of the toolbar, zoom in to a field of view of about \(2^{\prime} \times 1^{\prime}\). In the toolbar, set the year to 1986 and the Time Flow Rate to 1 hour. Then click on the Run Time Forward button, the right-pointing triangle on the toolbar. You can scroll on and off the labels for the moons by clicking on Labels > Planets-Moons. (a) Describe how the satellites move, and relate your observations to Kepler's third law (see Sections 4-4 and 4-7). (b) Set the year to 2007 and again click on the Run Time Forward button. How do the orbits look different than in (a)? Explain any differences.
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