21st Century Astronomy
21st Century Astronomy
6th Edition
ISBN: 9780393428063
Author: Kay
Publisher: NORTON
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Chapter 11, Problem 3QP
To determine

The reason for the possibility of life on the moons of the outer planets.

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Due to tidal forces, a moon orbiting a planet will eventually   a always keep the same side toward the planet   b collide with the planet   c break up into a number of fragments   d develop a warmer climate as time goes on Jupiter's moon Io is very volcanically active, which means it has plate tectonics.   a. true   b. false
QUESTION 3 The surface of Venus receives   a. a lot more sunlight than the surface of the Earth   b. much less sunlight than the surface of the Earth   c. about as much sunlight as the surface of the Earth   QUESTION 4 Venus has very low surface wind speed because   a. the greenhouse effect makes the surface temperature nearly uniform   b. it has a very thin atmosphere   c. the thick clouds don't allow for much convection in the atmosphere   d. it doesn't have a large moon
6 Why isn't there a planet where the asteroid belt is located? A The temperature in this portion of the solar nebula was just right to prevent rock from sticking together. B C D There was too much rocky material to form a terrestrial planet, but not enough gaseous material to form a jovian planet. There was not enough material in this part of the solar nebula to form a planet. Gravitational tugs from Jupiter prevented material from collecting together to form a planet. E A planet once formed here, but it was broken apart by a catastrophic collision.
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