Physics Technology Update (4th Edition)

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

Chapter 25 - Electromagnetic Waves - Problems and Conceptual Exercises - Page 905: 91

Answer

$1.2\times 10^7m/s$ away from Earth

Work Step by Step

We can find the required speed of the quasar as follows: $f^{\prime}=f(1\pm\frac{u}{c})$ $\implies \frac{c}{\lambda^{\prime}}=\frac{c}{\lambda}(1\pm\frac{u}{c})$ Since the quasar is moving along the line of sight, we will use the negative sign. $\implies \frac{c}{\lambda^{\prime}}=\frac{c}{\lambda}(1-\frac{u}{c})$ This simplifies to: $\frac{\lambda}{\lambda^{\prime}}=1-\frac{u}{c}$ $\implies \frac{u}{c}=1-\frac{\lambda}{\lambda^{\prime}}$ $\implies u=c(1-\frac{\lambda}{\lambda^{\prime}})$........eq(1) Given that $\lambda=486\times 10^{-9}m$ and the same line is lengthened by $20nm$, that is $\lambda^{\prime}=(486+20)\times10^{-9}m=506\times 10^{-9}m$ Now, we plug in the known values in eq(1) to obtain: $u=(3\times 10^8)(1-\frac{486\times 10^{-9}}{506\times 10^{-9}})$ $u=1.2\times 10^7m/s$ away from Earth
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