A pair of stars revolves about their common center of mass
as in Fig. 1. One of the stars has a mass M that is twice the
mass m of the other star. Their centers are a distance d apart
(d being large compared to the size of either star). All units
are in SI.
(a) (4 marks) Derive an expression for the period of
revolution of the stars about their common center of mass in
terms of d, m, and G.
(b) (3 marks) Compare the angular momenta of the two stars
about their common center of mass by calculating the ratio
Lm /LM .
(c) (3 marks) Compare the kinetic energies of the two stars by
calculating the ratio Km /KM .
a)
stars will rotate about their c.m. position of centre of mass:
"0=\\frac{2m(-x)+m(d-x)}{2m+m}\\implies x=d\/3"
force of atraction will provide required centripetal force:
"\\frac{2mv^2_M}{d\/3}=\\frac{GMm}{d^2}\\implies v_M=\\sqrt{\\frac{Gm}{3d}}"
period of revolution of the stars:
"T=\\frac{2\\pi (d\/3)}{v_M}=\\frac{2\\pi d^{3\/2}}{\\sqrt{3Gm}}"
b)
for angular momentum:
"\\frac{L_M}{L_m}=\\frac{Mv_1d_1}{mv_2d_2}=\\frac{M}{m}(\\frac{m}{M})^2=m\/M=1\/2"
c)
for kinetic energies:
"\\frac{K_M}{K_m}=\\frac{Mv_1^2}{mv_2^2}=\\frac{M}{m}(\\frac{m}{M})^2=m\/M=1\/2"
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