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 3P
Measure the polar and equatorial diameters of Saturn in the photograph in Celestial Profile 8 and calculate the planet’s oblateness using the definition given in this chapter.
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What is the angular diameter of Saturn (in degrees) as seen from the surface of Rhea?
Use the small-angle formula to calculate the angular diameter (in degrees) of Saturn (including its rings) (diameter = 9.64 ✕ 105 km) as seen from Earth if Saturn were at the location of the Moon (distance = 384,000 km).
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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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- What is the angular diameter of Jupiter as seen from Earth when the two planets are closest together? When the two planets are farthest apart? (Hint: Use the small-angle formula, Eq. 3-1) (Note: Necessary data to calculate the two distances are given in the Celestial Profiles for Earth and Jupiter.)arrow_forwardWhat is the maximum angular diameter of Jupiter as seen from Earth? Repeat this calculation for Neptune. Relevant data can be found in Celestial Profiles 7 and 10. (Hint: Use the small-angle formula in Reasoning with Numbers 3-1.)arrow_forwardWhat is the angular diameter of Jupiter as seen from the surface of Callisto? (Hint: Use the small-angle formula, Eq. 3-1) (Note: Necessary data are given in Celestial Profile: Jupiter and Appendix Table A-11.)arrow_forward
- How 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_forwardWhat is understood to be the cause of ripples in ring systems?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
- What is the Roche limit, and what does it have to do with planetary rings?arrow_forwardThe ratio of charon to pluto's roche limit? or How close is Charon to Pluto's Roche limit? please solve accurate and exactarrow_forwardAt what average distances (in AU) from the Sun would you expect to find Kirkwood gaps where the orbital period of asteroids are respectively four-ninths, and two-fifths, of the orbital period of Jupiter? (Hint: use Kepler's third law.) inner gap at AU outer gap at AU Compare your results with the figure. 7:2 3:1 8,3 5;2 7:3 9:4 2;1 9:5 7:4 53 8:5 3:2 Resonances Gap Gap Gap Gap GapGap Gap Distance from sun (AU) O The results agree with the figure. O The results do not agree with the figure.arrow_forward
- Tutorial Based on the orbital properties of Uranus, how far across the sky in arc seconds does it travel in one Earth day? The average orbital radius is 2.88 x 109 km and the period is 84.0 years. (Assume Uranus and the Earth are at the closest point to one another in their orbits.) How many full Moons does this distance cover if the Moon has an angular diameter of 0.5 degrees? Part 1 of 4 We first need to determine how fast the planet is moving across the sky. If we know the period and the distance between the Sun and the planet we can calculate the velocity using: 2ar which will tell us how many kilometers the planet travels in a day if we convert the period into days. days = (P years' |days/year Pdays days Submit Skip (you cannot come back)arrow_forward6arrow_forward4) Science fiction movies often portray asteroid belts as crowded, dense regions that require spaceships to maneuver quickly to get through them. In this problem, we will calculate the fraction of volume in an asteroid belt that is actually occupied by asteroids. a) If there are 300,000 large asteroids between 2 and 3 AU from the Sun, and each asteroid is assumed to be spherical with a radius of 100 km, determine the total volume occupied by asteroids in this region. Recall that the volume of a sphere is given by the equation V = 4TR³ /3. b) Let's assume the region in which these asteroids orbit is an annulus with an inner radius of 2 AU, an outer radius of 3 AU, and a thickness of 2Ro. Determine the volume of this region. Recall that the area of a circle is given by the equation A = TR². Here are two conversions that you'll need: 1 AU = 1.496 × 108 km and 1 Ro = 6.955 × 105 km. c) What is the ratio of the volume occupied by asteroids to the volume of the asteroid belt (i.e., the…arrow_forward
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