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: 5

Answer

The mass of the portion of the Milky Way inside the sun's orbit: $M \simeq 2.623 \times {10^{41}}$ kg

Work Step by Step

We have the radius of the orbit $a \simeq 2.8 \times {10^{17}}$ km and velocity $v \simeq 250$ km/s. So, the period of the orbit is $T = \frac{{2\pi a}}{v} = \frac{{2\pi \times 2.8 \times {{10}^{17}}}}{{250}} = 7.037 \times {10^{15}}$ s From Exercise 2 we obtain the mass of the Milky Way galaxy: $M = \left( {\frac{{4{\pi ^2}}}{G}} \right)\left( {\frac{{{a^3}}}{{{T^2}}}} \right)$, where $G$ is the gravitational constant, $G \simeq 6.673 \times {10^{ - 11}}$ ${m^3}k{g^{ - 1}}{s^{ - 2}}$ So, $M = \left( {\frac{{4{\pi ^2}}}{{6.673 \times {{10}^{ - 11}}}}} \right)\frac{{{{\left( {2.8 \times {{10}^{20}}} \right)}^3}}}{{{{\left( {7.037 \times {{10}^{15}}} \right)}^2}}} \simeq 2.623 \times {10^{41}}$ kg
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