21ST C ASTRO EBOOK+SW5=SS+VGCRD+LEARN/DO
21ST C ASTRO EBOOK+SW5=SS+VGCRD+LEARN/DO
6th Edition
ISBN: 9780393870152
Author: PALEN
Publisher: Norton, W. W. & Company, Inc.
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Chapter 4.4, Problem 4.4CYU
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2. Show that the divergence of the geostrophic wind is – v,(cot $)/a if the variations in fwith latitude are accounted for (i.e., use the full definition of the Coriolis parameter f = 2.0 sin p). To derive this relationship, recall that on a spherical planet, the distance north is y = aø, where ø is latitude (in radians) and a is the radius of Earth (6,370,000 m). Thus, a derivative in y can be expressed as a derivative in latitude o via the following relationship: a 1 a ду а дф
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
1. The tides are present on earth because... A) the sun causes the earth to orbit  B) the moon has a negligible gravitational effect on the earth except for in the oceans C) there is a different force of gravity acting on either side of the earth resulting from the moon D) tectonic plates shift as the earth rotates causing the water levels to vary.
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