Fundamentals of Physics Extended (10th Edition)

Published by Wiley
ISBN 10: 1-11823-072-8
ISBN 13: 978-1-11823-072-5

Chapter 13 - Gravitation - Problems - Page 381: 40b

Answer

The projectile reaches a radial distance of $~~2~R_E$

Work Step by Step

Let $M_E$ be the mass of the Earth. Let $m$ be the mass of the projectile. In order to escape the Earth: $K+U = 0$ $K = -U$ $K = \frac{G~M_E~m}{R_E}$ If the kinetic energy is half of the required kinetic energy: $K_1 = \frac{G~M_E~m}{2~R_E}$ We can use conservation of energy to find the radial distance $r$ that a projectile reaches: $K_2+U_2 = K_1+U_1$ $0-\frac{GM_E~m}{r} = \frac{G~M_E~m}{2~R_E}-\frac{GM_E~m}{R_E}$ $-\frac{1}{r} = \frac{1}{2~R_E}-\frac{1}{R_E}$ $-\frac{1}{r} = \frac{1}{2~R_E}-\frac{2}{2~R_E}$ $-\frac{1}{r} = -\frac{1}{2~R_E}$ $r = 2~R_E$ The projectile reaches a radial distance of $~~2~R_E$
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