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: 9

Answer

$4.79\times 10^{20}N$ at $24.4^{\circ}$ toward the Earth off the line from the Moon to the Sun.

Work Step by Step

We can find the required force as follows: $F_S=G\frac{M_M M_S}{r_{MS}^2}$ $F_S=(6.67\times 10^{-11}N.m^2/Kg^2)\frac{(7.35\times 10^{22}Kg)(2.00\times 10^{30}Kg)}{(1.50\times 10^{11}m)^2}=4.36\times 10^{20}N$ The force exerted on the Earth is given as $F_E=G\frac{M_M M_E}{r_{ME}^2}$ $F_S=(6.67\times 10^{-11}N.m^2/Kg^2)\frac{(7.35\times 10^{22}Kg)(5.97\times 10^{24}Kg)}{(3.84\times 10^{11}m)^2}=1.98\times 10^{20}N$ Now $F=\sqrt{F_x^2+F_y^2}$ We plug in the known values to obtain: $F=\sqrt{(4.36\times 10^{20})^2+(1.98\times 10^{20})^2}$ $F=4.79\times 10^{20}N$ and the direction can be determined as $\theta=tan^{-1}\frac{F_y}{F_x}$ $\theta=tan^{-1}(\frac{1.98\times 10^{20}}{4.36\times 10^{20}})=24.4^{\circ}$ toward the Earth off the line from the Moon to the Sun.
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