Fundamentals of Physics Extended (10th Edition)

Published by Wiley
ISBN 10: 1-11823-072-8
ISBN 13: 978-1-11823-072-5

Chapter 13 - Gravitation - Problems - Page 381: 41b

Answer

The speed of each neutron star is $~~1.8\times 10^7~m/s$

Work Step by Step

Let $R_1 = 1.0\times 10^{10}~m$ We can find the separation distance of the centers when they are about to collide: $R_2 = (2)(1.0\times 10^5~m) = 2.0\times 10^5~m$ We can use conservation of energy to find the kinetic energy of the system when the separation distance is $\frac{R_0}{2}$: $K_2+U_2 = K_1+U_1$ $K_2-\frac{GM^2}{R_2} = 0-\frac{GM^2}{R_1}$ $K_2 = \frac{GM^2}{R_2}-\frac{GM^2}{R_1}$ $K_2 = GM^2~(\frac{1}{R_2}-\frac{1}{R_1})$ Since both neutron stars have the same mass, each star has half of the kinetic energy of the system. We can find the speed of each neutron star: $K = \frac{GM^2}{2}~(\frac{1}{R_2}-\frac{1}{R_1})$ $\frac{1}{2}Mv^2 = \frac{GM^2}{2}~(\frac{1}{R_2}-\frac{1}{R_1})$ $v^2 = GM~(\frac{1}{R_2}-\frac{1}{R_1})$ $v = \sqrt{GM~(\frac{1}{R_2}-\frac{1}{R_1})}$ $v = \sqrt{(6.67\times 10^{-11}~N~m^2/kg^2)(1.0\times 10^{30}~kg)~(\frac{1}{2.0\times 10^5~m}-\frac{1}{1.0\times 10^{10}~m})}$ $v = 1.8\times 10^7~m/s$ The speed of each neutron star is $~~1.8\times 10^7~m/s$
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