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Two stars of mass m=1.70 and M=10.0 (in units of solar masses) separated by a distance d=5.00 (in units of AU, the earth-sun distance) revolve
Two stars of mass m=1.70 and M=10.0 (in units of solar masses) separated by a distance d=5.00 (in units of AU, the earth-sun distance) revolve in circular orbits about their (common) center of mass as shown in the figure below.
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