Calculus (3rd Edition)

Published by W. H. Freeman
ISBN 10: 1464125260
ISBN 13: 978-1-46412-526-3

Chapter 14 - Calculus of Vector-Valued Functions - 14.6 Planetary Motion According to Kepler and Newton - Exercises - Page 751: 7

Answer

Using Theorem 2, we show that the angular velocity $\theta '\left( t \right)$ is constant. Hence, the planet in a circular orbit travels at constant speed.

Work Step by Step

We have ${\bf{J}} = {\bf{r}}\left( t \right) \times {\bf{r}}'\left( t \right)$. By Theorem 1, ${\bf{J}}$ is constant. So, $J = ||{\bf{J}}||$ is constant. By Theorem 2, we have $J = r{\left( t \right)^2}\theta '\left( t \right)$. Since the orbit of the planet is circular, the radius of the orbit $r\left( t \right)$ is constant. Therefore, the angular velocity $\theta '\left( t \right)$ is also constant. Hence, the planet in a circular orbit travels at constant speed.
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