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: 13

Answer

Using the fact that ${r_{per}} + {r_{ap}} = 2a$, we obtain ${r_{per}} = \frac{p}{{1 + e}} = a\left( {1 - e} \right)$ ${r_{ap}} = \frac{p}{{1 - e}} = a\left( {1 + e} \right)$

Work Step by Step

At $\theta=0$, we obtain the distance from the sun at the perihelion: ${r_{per}} = \frac{p}{{1 + e}}$ Similarly, at $\theta = \pi $, we obtain the distance from the sun at the aphelion: ${r_{ap}} = \frac{p}{{1 - e}}$ Using the fact that ${r_{per}} + {r_{ap}} = 2a$, so $\frac{p}{{1 + e}} + \frac{p}{{1 - e}} = 2a$ $p\left( {\frac{1}{{1 + e}} + \frac{1}{{1 - e}}} \right) = 2a$ $p\left( {\frac{2}{{\left( {1 + e} \right)\left( {1 - e} \right)}}} \right) = 2a$ $p = a\left( {1 + e} \right)\left( {1 - e} \right)$ Substituting $p$ in ${r_{per}}$ and ${r_{ap}}$ gives ${r_{per}} = \frac{p}{{1 + e}} = a\left( {1 - e} \right)$ ${r_{ap}} = \frac{p}{{1 - e}} = a\left( {1 + e} \right)$
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