Physics Technology Update (4th Edition)

Published by Pearson
ISBN 10: 0-32190-308-0
ISBN 13: 978-0-32190-308-2

Chapter 12 - Gravity - Problems and Conceptual Exercises - Page 409: 8

Answer

a) $F_E=3.56\times 10^{22}N$ toward the Sun. b) $F_M=2.40\times 10^{20}N$ toward the Sun. c) $F_S=3.58\times 10^{22}N$ toward the Earth-Moon system.

Work Step by Step

(a) We can find the required force as $F_E=GM_E(\frac{M_s}{r_{Es}^2}+\frac{M_m}{r_{Em}^2})$ We plug in the known values to obtain: $F_E=(6.67\times 10^{-11})(5.97\times 10^{24})[\frac{2.00\times 10^{30}}{(1.50\times 10^{11})^2}+\frac{7.35\times 10^{22}}{(3.84\times 10^8)^2}]$ $F_E=3.56\times 10^{22}N$ toward the Sun. (b) We can find the required force exerted on the Moon as $F_E=GM_m(\frac{M_s}{r_{sm}^2}+\frac{M_E}{r_{Em}^2})$ We plug in the known values to obtain: $F_E=(6.67\times 10^{-11})(7.35\times 10^{22})[\frac{2.00\times 10^{30}}{(1.50\times 10^{11}-3.84\times 10^8)^2}+\frac{5.97\times 10^{24}}{(3.84\times 10^8)^2}]$ $F_M=2.40\times 10^{20}N$ toward the Sun. (c) We can find the required force on the Sun as $F_S=GM_S(\frac{M_m}{r_{sm}^2}+\frac{M_E}{r_{sE}^2})$ We plug in the known values to obtain: $F_S=(6.67\times 10^{-11})(2.00\times 10^{30})[\frac{7.35\times 10^{22}}{(1.50\times 10^{11}-3.84\times 10^8)^2}+\frac{5.97\times 10^{24}}{(1.50\times 10^{11})^2}]$ $F_S=3.58\times 10^{22}N$ toward the Earth-Moon system.
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