University Physics with Modern Physics (14th Edition)

Published by Pearson
ISBN 10: 0321973615
ISBN 13: 978-0-32197-361-0

Chapter 13 - Gravitation - Problems - Exercises - Page 426: 13.20

Answer

(a) The period of one revolution is 2.93 hours. (b) The radial acceleration of the satellite is $3.70~m/s^2$.

Work Step by Step

(a) Let $M$ be the mass of the earth. We can use the speed to find the radius of the satellite's orbit. $v = \sqrt{\frac{G~M}{R}}$ $R = \frac{G~M}{v^2}$ $R = \frac{(6.67\times 10^{-11}~m^3/kg~s^2)(5.98\times 10^{24}~kg)}{(6200~m/s)^2}$ $R = 1.04\times 10^7~m$ We can find the time of one revolution. $t = \frac{distance}{speed}$ $t = \frac{2\pi~R}{v}$ $t = \frac{(2\pi)(1.04\times 10^7~m)}{6200~m/s}$ $t = 10,540~s = 2.93~hours$ The period of one revolution is 2.93 hours. (b) We can find the radial acceleration. $a_c = \frac{v^2}{R}$ $a_c = \frac{(6200~m/s)^2}{1.04\times 10^7~m}$ $a_c = 3.70~m/s^2$ The radial acceleration of the satellite is $3.70~m/s^2$.
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