University Physics with Modern Physics (14th Edition)

Published by Pearson
ISBN 10: 0321973615
ISBN 13: 978-0-32197-361-0

Chapter 12 - Fluid Mechanics - Problems - Exercises - Page 390: 12.6

Answer

(a) The average density of the sun is $1.409\times 10^3~kg/m^3$. (b) The average density of a neutron star is $5.94\times 10^{16}~kg/m^3$.

Work Step by Step

(a) We can find the volume of the sun. $V = \frac{4}{3}\pi~r^3$ $V = \frac{4}{3}\pi~(6.96\times 10^8~m)^3$ $V = 1.412\times 10^{27}~m^3$ We can find the average density of the sun. $\rho = \frac{M}{V}$ $\rho = \frac{1.989\times 10^{30}~kg}{1.412\times 10^{27}~m^3}$ $\rho = 1.409\times 10^3~kg/m^3$ The average density of the sun is $1.409\times 10^3~kg/m^3$ (b) We can find the volume of a neutron star. $V = \frac{4}{3}\pi~r^3$ $V = \frac{4}{3}\pi~(2.00\times 10^4~m)^3$ $V = 3.351\times 10^{13}~m^3$ We can find the average density of a neutron star. $\rho = \frac{M}{V}$ $\rho = \frac{1.989\times 10^{30}~kg}{3.351\times 10^{13}~m^3}$ $\rho = 5.94\times 10^{16}~kg/m^3$ The average density of a neutron star is $5.94\times 10^{16}~kg/m^3$.
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