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 752: 15

Answer

We evaluate the magnitude $J$ at the perihelion and aphelion. Then, using the result from Exercise 13 we prove that ${v_{per}}\left( {1 - e} \right) = {v_{ap}}\left( {1 + e} \right)$

Work Step by Step

Since ${\bf{J}} = {\bf{r}} \times {\bf{r}}'$ is constant and ${\bf{r}}$ is perpendicular to ${\bf{r}}'$ at the perihelion and aphelion; for convenience we evaluate the magnitude $J$ at the perihelion and aphelion: $||{\bf{J}}|| = ||{{\bf{r}}_{per}}||||{{\bf{r}}_{per}}'||\sin \frac{\pi }{2} = {r_{per}}{v_{per}}$ $||{\bf{J}}|| = ||{{\bf{r}}_{ap}}||||{{\bf{r}}_{ap}}'||\sin \frac{\pi }{2} = {r_{ap}}{v_{ap}}$ So, (1) ${\ \ \ \ }$ ${r_{per}}{v_{per}} = {r_{ap}}{v_{ap}}$ From Exercise 13, we obtain ${r_{per}} = \frac{p}{{1 + e}}$ and ${r_{ap}} = \frac{p}{{1 - e}}$. Substituting these in equation (1) gives $\frac{p}{{1 + e}}{v_{per}} = \frac{p}{{1 - e}}{v_{ap}}$ Hence, ${v_{per}}\left( {1 - e} \right) = {v_{ap}}\left( {1 + e} \right)$.
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