Physics: Principles with Applications (7th Edition)

Published by Pearson
ISBN 10: 0-32162-592-7
ISBN 13: 978-0-32162-592-2

Chapter 33 - Astrophysics and Cosmology - Problems - Page 981: 1

Answer

The star is 3.1 light-years away.

Work Step by Step

We can use this equation to find the distance $D$ to the star: $D = \frac{d}{\phi}$, where d = 1 AU and $\phi$ is the parallax angle measured in radians. To use this equation, first we must find $\phi$: $\phi = (0.00029^{\circ})(\frac{2\pi ~rad}{360^{\circ}}) = 5.06\times 10^{-6}~radians$ Now, $D = \frac{d}{\phi} = \frac{1.50\times 10^{11}~m}{5.06\times 10^{-6}~radians} = 2.96\times 10^{16}~m$ We can convert this distance to light-years. $D = (2.96\times 10^{16}~m)(\frac{1 ~light~year}{9.46\times 10^{15}~m}) = 3.1 ~light~years$ The star is 3.1 light-years away.
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