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
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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Transcribed Image Text:A certain triple-star system consists of two stars, each of mass \( m = 6.7 \times 10^{30} \, \text{kg} \), revolving in the same circular orbit of radius \( r = 3.9 \times 10^{11} \, \text{m} \) about a central star of mass \( M = 4.4 \times 10^{33} \, \text{kg} \) (see 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.
**Diagram Explanation:**
- The diagram shows a circular orbit with a central star of mass \( M \) located at the center.
- Two smaller stars, each with mass \( m \), are positioned on the orbit at opposite ends of a diameter.
- The distance from the center to the orbit is marked as \( r \).
- Arrows indicate the direction of the stars' motion along the orbit.
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