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: 16

Answer

${r_{per}} \simeq 4.38\times{10^{10}}$ m ${r_{ap}} \simeq 7.2\times{10^{10}}$ m

Work Step by Step

We have the eccentricity $e=0.244$ for the orbit of Mercury. From Exercise 13, we obtain ${r_{per}} = a\left( {1 - e} \right)$ and ${r_{ap}} = a\left( {1 + e} \right)$. From the table in Exercise 1, the semimajor axis of Mercury is $a = 5.79 \times {10^{10}}$ m. So, ${r_{per}} = a\left( {1 - e} \right) = 5.79 \times {10^{10}}\left( {1 - 0.244} \right)$ ${r_{per}} \simeq 4.38\times{10^{10}}$ m ${r_{ap}} = a\left( {1 + e} \right) = 5.79 \times {10^{10}}\left( {1 + 0.244} \right)$ ${r_{ap}} \simeq 7.2\times{10^{10}}$ m
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.