Physics Technology Update (4th Edition)

Published by Pearson
ISBN 10: 0-32190-308-0
ISBN 13: 978-0-32190-308-2

Chapter 10 - Rotational Kinematics and Energy - Problems and Conceptual Exercises - Page 330: 106

Answer

(a) $-2.22\times 10^{-9}rad/s^2$ (b) $2718.2years$ (c) $20ms$

Work Step by Step

(a) We can find the required angular acceleration as follows: The initial angular speed is given as: $ \omega=\frac{\Delta \theta}{\Delta t}$ $\omega=\frac{2\pi rad}{33.0\times 10^{-3}s}$ $\omega=190.399rad/s$ and $\Delta t_{100}=33.0\times 10^{-3}s+1.26\times 10^{-3}s=0.03426s$ The final angular speed is given as: $\omega_{100}=\frac{\Delta \theta}{\Delta t_{100}}$ $\omega_{100}=\frac{2\pi rad}{0.03426s}$ $\omega_{100}=183.397rad/s$ We can convert 100 years into seconds as $\Delta t=(100 years)(365days/yr)(24h/yr)(60min/h)(60s/min)=3.1536\times 10^9s$ Now $\alpha_{avg}=\frac{\Delta \omega}{\Delta t}$ We plug in the known values to obtain: $\alpha=\frac{183.397rad/s-190.399rad/s}{3.1536\times 10^9s}$ $\alpha=-2.22\times 10^{-9}rad/s^2$ (b) We can find the required time taken as follows: $\Delta t=\frac{\Delta \omega}{\alpha_{avg}}$ We plug in the known values to obtain: $\Delta t=\frac{-190.3rad/s}{-2.22\times 10^{-9}rad/s}$ $\Delta t=8.572\times 10^{10}s$ Now we convert this time into years as $\Delta t=(8.572\times 10^{10}s)(\frac{1min}{60s})(\frac{1h}{60min})(\frac{1day}{24h})(\frac{1year}{365days})$ $\Delta t=2718.2years$ (c) As given that $1054A.D=1054$ $\implies 2008-1054=954years$ Now the time period of the pulsar when it was created is $(1.25\times 10^{-5}s/y)(954y)=0.01202s$ and $t=0.033s-0.01202s$ $t=0.02098s$ $t=20ms$
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