Fundamentals of Physics Extended (10th Edition)

Published by Wiley
ISBN 10: 1-11823-072-8
ISBN 13: 978-1-11823-072-5

Chapter 4 - Motion in Two and Three Dimensions - Problems - Page 88: 61c

Answer

The answers to part (a) and part (b) both increase.

Work Step by Step

We can write an expression for the speed at the equator: $v = \frac{2\pi~r}{T}$ If the star rotates faster, the period $T$ decreases. Therefore, the speed $v$ increases. We can write an expression for the acceleration: $a = \frac{v^2}{r}$ As shown above, if the star rotates faster, the speed $v$ increases. Therefore, the magnitude of the acceleration increases.
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