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Two stars of mass m = 0.670 and M = 19.0 (in units of solar masses) separated by a distance d = 9.00 (in
Two stars of mass m = 0.670 and M = 19.0 (in units of solar masses) separated by a distance d = 9.00 (in units of AU, the earth-sun distance) revolve in circular orbits about their (common) center of mass as shown in the figure below. m 12 NO c.m. 0 MI 5 What is the orbital period of the smaller star in years?
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Physics
Authors: Alan Giambattista, Betty Richardson, Robert Richardson
2nd edition
77339681, 978-0077339685
