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: 10

Answer

The velocity of a satellite in geosynchronous orbit about the earth: $v \simeq 3071.85$ m/s

Work Step by Step

Since the satellite is a geosynchronous orbit about the earth, we can use the results from Exercise 6 and 9. Using the result in Exercise 6, the radius of the orbit is $R \approx 42246$ km. Now, the velocity of the satellite using result in Exercise 9 is $v = \sqrt {\frac{k}{R}} = \sqrt {\frac{{GM}}{R}} $, ${\ \ \ }$ where $k = GM$. $G$ is the gravitational constant: $G \simeq 6.673 \times {10^{ - 11}}$ ${m^3}k{g^{ - 1}}{s^{ - 2}}$ and $M$ is the mass of the earth: $M \approx 5.974 \times {10^{24}}$ kg. Substituting $G$, $M$, and $R$ in $v$ gives the velocity of a satellite in geosynchronous orbit about the earth: $v = \sqrt {\frac{{6.673 \times {{10}^{ - 11}} \times 5.974 \times {{10}^{24}}}}{{42.246 \times {{10}^6}}}} \simeq 3071.85$ m/s
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