Horizons: Exploring the Universe (MindTap Course List)
14th Edition
ISBN: 9781305960961
Author: Michael A. Seeds, Dana Backman
Publisher: Cengage Learning
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Chapter 18, Problem 6P
If Uranus’s epsilon ring is 50 km wide and the orbital velocity of Uranus is 6.8 km/s, how long should the occultation last that you expect to observe from Earth when the ring crosses in front of the star? (For the purposes of this problem, ignore the motion of Earth.)
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One way to recognize a distant planet is by studying the planet’s motion along its orbit. If Uranus circles the Sun in 84.0 years, how many arc seconds will it move in 1 earth day? Assume a circular orbit for Uranus, and pretend that earth is not moving.
Chapter 18 Solutions
Horizons: Exploring the Universe (MindTap Course List)
Ch. 18 - Why is Jupiter so much richer in hydrogen and...Ch. 18 - How can Jupiter have a liquid interior and not...Ch. 18 - How does the dynamo effect account for the...Ch. 18 - Why are the belts and zones on Saturn less...Ch. 18 - Why do astronomers conclude that none of the...Ch. 18 - How can a moon produce a gap in a planetary ring...Ch. 18 - Explain why the amount of geological activity on...Ch. 18 - Prob. 8RQCh. 18 - Prob. 9RQCh. 18 - Prob. 10RQ
Ch. 18 - What are the seasons on Uranus like?Ch. 18 - Prob. 12RQCh. 18 - What evidence is there that Neptune’s moon Triton...Ch. 18 - How do astronomers account for the origin of...Ch. 18 - What evidence indicates that catastrophic impacts...Ch. 18 - Prob. 16RQCh. 18 - Some astronomers argue that Jupiter and Saturn are...Ch. 18 - Prob. 2DQCh. 18 - What is the maximum angular diameter of Jupiter as...Ch. 18 - What is the angular diameter of Jupiter as seen...Ch. 18 - Measure the polar and equatorial diameters of...Ch. 18 - If you observe light reflected from Saturn’s...Ch. 18 - One way to recognize a distant planet is by its...Ch. 18 - If Uranus’s epsilon ring is 50 km wide and the...Ch. 18 - If Neptune’s clouds have a temperature of 60 K, at...Ch. 18 - Prob. 8PCh. 18 - Prob. 9PCh. 18 - The orbital period of Charon is given in the...Ch. 18 - Prob. 1LTLCh. 18 - Prob. 2LTLCh. 18 - Prob. 3LTL
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Need a deep-dive on the concept behind this application? Look no further. Learn more about this topic, physics and related others by exploring similar questions and additional content below.Similar questions
- Does Uranus have enough mass to have formed by gravitational collapse? How do you know?arrow_forwardWhen during Uranuss seasonal cycle does every portion of the planet experience some sunlight during each rotation?arrow_forwardWhat is the orbital velocity of Miranda around Uranus? (Hint: Use the formula for circular velocity, Eq. 5-1a. The formula requires input quantities in kg and m.) (Note: Necessary data are given in Celestial Profile: Uranus and Appendix Table A-11.)arrow_forward
- Why were the rings of Uranus not observed directly from telescopes on the ground on Earth? How were they discovered?arrow_forwardUranus is about 26,000 km in radius, and its main ring is about 51,000 km from the planets center. If you represent the planet with a ball 5 inches in radius, how far from the center would you place its main ring?arrow_forwardThe image to the left shows how Uranus would look to the unaided human eye, whereas the right image shows how Uranus would look through a red filter, which enhances the methane clouds. What do the visible atmospheric features tell you about circulation on Uranus?arrow_forward
- Calculate Uranuss Roche radius. Are all of Uranuss rings inside the Roche limit? Are any of the moons within the Roche limit? (Notes: The Roche limit is defined in Chapter 22. Necessary data are given in Celestial Profile: Uranus and Appendix Table A-11. The structure of the Uranian system is displayed in the Concept Art: Uranuss and Neptunes Rings.)arrow_forwardWhat is the maximum angular diameter of Uranus as seen from Earth? Of Neptune? (Hint: Use the small-angle formula, Eq. 3-1.) (Note: Necessary data are given in their Celestial Profiles.)arrow_forward
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