University Physics with Modern Physics (14th Edition)

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

Chapter 10 - Dynamics of Rotational Motion - Problems - Exercises - Page 332: 10.46

Answer

The mass of the asteroid should be $\frac{M}{10}$.

Work Step by Step

We can find $\omega_2$ in terms of $\omega_1$ when the length of the day increases by 25%. $T_2 = 1.25~T_1$ $\frac{2\pi}{\omega_2} = 1.25\times \frac{2\pi}{\omega_1}$ $\omega_2 = 0.80~\omega_1$ We can use conservation of angular momentum to solve this question. Let $M$ be the mass of the earth and let $m$ be the mass of the asteroid. $L_2 = L_1$ $I_2\omega_2 = I_1\omega_1$ $(\frac{2}{5}MR^2+mR^2)(0.80~\omega_1) = \frac{2}{5}MR^2\omega_1$ $(M+\frac{5}{2}m)(0.80)= M$ $2.0~m = 0.20~M$ $m = \frac{M}{10}$ The mass of the asteroid should be $\frac{M}{10}$.
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