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)...
icon
Related questions
Question
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.
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.
Expert Solution
trending now

Trending now

This is a popular solution!

steps

Step by step

Solved in 2 steps

Blurred answer
Knowledge Booster
Kepler's Laws
Learn more about
Need a deep-dive on the concept behind this application? Look no further. Learn more about this topic, physics and related others by exploring similar questions and additional content below.
Similar questions
  • SEE MORE QUESTIONS
Recommended textbooks for you
College Physics
College Physics
Physics
ISBN:
9781305952300
Author:
Raymond A. Serway, Chris Vuille
Publisher:
Cengage Learning
University Physics (14th Edition)
University Physics (14th Edition)
Physics
ISBN:
9780133969290
Author:
Hugh D. Young, Roger A. Freedman
Publisher:
PEARSON
Introduction To Quantum Mechanics
Introduction To Quantum Mechanics
Physics
ISBN:
9781107189638
Author:
Griffiths, David J., Schroeter, Darrell F.
Publisher:
Cambridge University Press
Physics for Scientists and Engineers
Physics for Scientists and Engineers
Physics
ISBN:
9781337553278
Author:
Raymond A. Serway, John W. Jewett
Publisher:
Cengage Learning
Lecture- Tutorials for Introductory Astronomy
Lecture- Tutorials for Introductory Astronomy
Physics
ISBN:
9780321820464
Author:
Edward E. Prather, Tim P. Slater, Jeff P. Adams, Gina Brissenden
Publisher:
Addison-Wesley
College Physics: A Strategic Approach (4th Editio…
College Physics: A Strategic Approach (4th Editio…
Physics
ISBN:
9780134609034
Author:
Randall D. Knight (Professor Emeritus), Brian Jones, Stuart Field
Publisher:
PEARSON