Universe
11th Edition
ISBN: 9781319039448
Author: Robert Geller, Roger Freedman, William J. Kaufmann
Publisher: W. H. Freeman
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Chapter 12, Problem 34Q
To determine
The reason why Saturn's rings look solid when viewed from a telescope even when they are not.
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Chapter 12 Solutions
Universe
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- Saturn is about 60,000 km in radius, and its rings are only about 0.01 km thick with ripples 100 m high. Design a really big model with Saturn 60 inches in radius (10 ft in diameter). How thick must the rings be in your model and how high can the ripples be? A sheet of paper is about 0.004 inches thick.arrow_forwardWhy do the upper levels of Neptune’s atmosphere appear blue?arrow_forwardThe water clouds believed to be present on Jupiter and Saturn exist at temperatures and pressures similar to those in the clouds of the terrestrial atmosphere. What would it be like to visit such a location on Jupiter or Saturn? In what ways would the environment differ from that in the clouds of Earth?arrow_forward
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- What is the Roche limit, and what does it have to do with planetary rings?arrow_forwardThe solar flux at the top of Earth's atmosphere is 1366W/m2. If Jupiter is 5.2 AU from Sun, what is the solar flux at the top of Jupiters atmosphere? Jupiter's albedo is 0.52, how does that influence its energy budget?arrow_forwardWhy does Saturn have a less varied appearance than Jupiter?arrow_forward
- 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).arrow_forwardWhat is the orbital velocity and period of a ring particle at the outer edge of Saturn's A ring? (Note: The radius of the edge of the A ring is 136,500 km. Hint: Use the formula for orbital velocity, GM Vc = V orbital velocity km/s period hr Need Help? Read It Submit Answerarrow_forwardWhat is the angular diameter of Saturn (in degrees) as seen from the surface of Rhea?arrow_forward
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