A certain triple-star system consists of two stars, each of mass m = 1.9×1030 kg, revolving in the same circular orbit of radius r= 8.3x1011 m about a central star of mass M = 7.9x1033 kg (the figure). The two orbiting stars are always at opposite ends of a diameter of the orbit. Calculate the period of revolution of the stars.

A certain triple-star system consists of two stars, each of mass m = 1.9×1030 kg, revolving in the same circular orbit of radius r= 8.3x1011 m about a central star of mass M = 7.9x1033 kg (the figure). The two orbiting stars are always at opposite ends of a diameter of the orbit. Calculate the period of revolution of the stars.

College Physics

11th Edition

ISBN:9781305952300

Author:Raymond A. Serway, Chris Vuille

Publisher:Raymond A. Serway, Chris Vuille

Chapter1: Units, Trigonometry. And Vectors

Section: Chapter Questions

Problem 1CQ: Estimate the order of magnitude of the length, in meters, of each of the following; (a) a mouse, (b)...

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