University Physics with Modern Physics (14th Edition)

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

Chapter 3 - Motion in Two or Three Dimensions - Problems - Exercises - Page 94: 3.23

Answer

(a) $a_R = 0.0337~m/s^2$ $a_R = 0.00344~g$ (b) The rotation period would have to be 84.5 minutes.

Work Step by Step

(a) We can find the speed on the equator. $v = \frac{2\pi r}{t} = \frac{(2\pi) (6.38\times 10^6~m)}{24 \times 3600~s}$ $v = 464~m/s$ We can use the speed to find the radial acceleration. $a_R = \frac{v^2}{r} = \frac{(464~m/s)^2}{6.38\times 10^6~m}$ $a_R = 0.0337~m/s^2$ $a_R = \frac{0.0337~m/s^2}{9.80~m/s^2} = 0.00344~g$ (b) $a_R = \frac{v^2}{r} = g$ $\frac{(2\pi~r)^2}{t^2~r} = g$ $t^2 = \frac{4\pi^2~r}{g}$ $t = {2\pi}\sqrt{\frac{r}{g}}$ $t = {2\pi}\sqrt{\frac{6.38\times 10^6~m}{9.80~m/s^2}}$ $t = 5069.6~s = 84.5~min$ The rotation period would have to be 84.5 minutes.
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