College Physics (4th Edition)

Published by McGraw-Hill Education
ISBN 10: 0073512141
ISBN 13: 978-0-07351-214-3

Chapter 6 - Problems - Page 228: 28

Answer

(a) The energy that is saved is $1.176\times 10^7~J$ (b) The energy that is saved is $3.125\times 10^6~J$

Work Step by Step

(a) We can find the gravitational potential energy: $U_g = mgh = (100~kg)(9.80~m/s^2)(12,000~m) = 1.176\times 10^7~J$ The energy that is saved is $1.176\times 10^7~J$ (b) We can find the kinetic energy: $KE = \frac{1}{2}mv^2 = \frac{1}{2}(100~kg)(250~m/s)^2 = 3.125\times 10^6~J$ The energy that is saved is $3.125\times 10^6~J$.
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