Physics: Principles with Applications (7th Edition)

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

Chapter 5 - Circular Motion; Gravitation - General Problems - Page 135: 67

Answer

The centripetal acceleration is $5.96\times 10^{-3}~m/s^2$ The net force exerted on the Earth is $3.56\times 10^{22}~N$. This force comes from the gravitational force exerted on the Earth by the Sun.

Work Step by Step

We can find the speed of the Earth as it orbits the Sun; $v = \frac{d}{t}$ $v = \frac{2\pi~r}{t}$ $v = \frac{(2\pi)(1.50\times 10^{11}~m)}{(365)(24)(3600)~s}$ $v = 2.99\times 10^4~m/s$ We then use the speed to find the centripetal acceleration; $a_c = \frac{v^2}{r}$ $a_c = \frac{(2.99\times 10^4~m/s)^2}{1.50\times 10^{11}~m}$ $a_c = 5.96\times 10^{-3}~m/s^2$ The centripetal acceleration is $5.96\times 10^{-3}~m/s^2$. Also, we find the net force exerted on the Earth: $F = M~a_c$ $F = (5.98\times 10^{24}~kg)(5.96\times 10^{-3}~m/s^2)$ $F = 3.56\times 10^{22}~N$ The net force exerted on the Earth is $3.56\times 10^{22}~N$. This force comes from the gravitational force exerted on the Earth by the Sun.
Update this answer!

You can help us out by revising, improving and updating this answer.

Update this answer

After you claim an answer you’ll have 24 hours to send in a draft. An editor will review the submission and either publish your submission or provide feedback.