21st Century Astronomy
21st Century Astronomy
6th Edition
ISBN: 9780393428063
Author: Kay
Publisher: NORTON
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Chapter 3, Problem 2QP
To determine

What happens when Earth catches up to a slower-moving outer planet and passes it in its orbit.

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Which of the following is a measurable effect of the tidal interactions between the Earth and the moon? choose 1 of the following: a. The moon is constantly getting closer to the Earth, and will one day collide with our planet. b. The rotation rate of the Earth is gradually slowing down. c. The rotation rate of the moon is gradually speeding up. d. The moon pulls more strongly on the far side of the Earth than it does on the near side.
The rotation of the planets around the sun is governed by: A. The gravitational field of the sun. B. The gravity of the stars. C. The heat energy of the sun. D. The gravity of the other planets of the solar system. Kelper's second law relates between them: O A. The time period of rotation of the orbiting planet around the sun and the average distance of the planet to the sun. OB. The time period of rotation of the orbiting planet around the sun and the average distance of the planet to the earth. C. The time period of rotation of the orbiting planet around the sun and the average distance of the planet to the moon. OD. The time period of rotation of the orbiting planet around the earth and the average distance of the planet to the sun.
When tidal bulges are NOT in a direct Earth-moon line but slightly ahead of the moon,   a. Earth’s gravity weakens.   b. their gravitational field pulls the moon forward in its orbit, causing it to recede from Earth.   c. their gravitational field pulls the moon back in its orbit, causing the moon to fall toward Earth.   d. Earth’s gravity strengthens, causing the moon to orbit faster.   e. the tidal bulges have no effect on the moon.
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