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A certain triple-star system consists of two stars, each of mass m = 6.7×1030 kg, revolving in the same circular orbit of radius r = 3.9×10¹¹ m about a central star of mass M = 4.4x1033 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. m M m

A certain triple-star system consists of two stars, each of mass m = 6.7×1030 kg, revolving in the same circular orbit of radius r = 3.9×10¹¹ m about a central star of mass M = 4.4x1033 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. m M m

Principles of Physics: A Calculus-Based Text
Principles of Physics: A Calculus-Based Text
5th Edition
ISBN:9781133104261
Author:Raymond A. Serway, John W. Jewett
Publisher:Raymond A. Serway, John W. Jewett
Chapter3: Motion In Two Dimensions
Section: Chapter Questions
Problem 27P: The astronaut orbiting the Earth in Figure P3.27 is preparing to dock with a Westar VI satellite....
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A certain triple-star system consists of two stars, each of mass m = 6.7×1030 kg, revolving in the same circular orbit of radius r = 3.9×10¹¹ m about a central star of mass M = 4.4x1033 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. m M m
Transcribed Image Text:A certain triple-star system consists of two stars, each of mass m = 6.7×1030 kg, revolving in the same circular orbit of radius r = 3.9×10¹¹ m about a central star of mass M = 4.4x1033 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. m M m
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