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A certain triple-star system consists of two stars, each of mass m = 6.2×1030 kg, revolving in the same circular orbit of radius r = 8.9x10¹1 m about a central star of mass M=9.8x1033 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. Number i Units

A certain triple-star system consists of two stars, each of mass m = 6.2×1030 kg, revolving in the same circular orbit of radius r = 8.9x10¹1 m about a central star of mass M=9.8x1033 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. Number i Units

College Physics
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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A certain triple-star system consists of two stars, each of mass m = 6.2x1030 kg, revolving in the same circular orbit of radius r = 8.9x1011 m about a central star of mass M = 9.8x1033 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. Number i Units m
Transcribed Image Text:A certain triple-star system consists of two stars, each of mass m = 6.2x1030 kg, revolving in the same circular orbit of radius r = 8.9x1011 m about a central star of mass M = 9.8x1033 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. Number i Units m
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