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2. Two identical stars with radius R and mass M, orbits around their center of mass. The orbit is circular, and the stars are always on the opposite side of the circle. (a) Find the gravitational force of one star on the another. (b) Find the orbital speed of each star and their periods. (c):, How much energy would be needed to separate the two stars to the infinity?

2. Two identical stars with radius R and mass M, orbits around their center of mass. The orbit is circular, and the stars are always on the opposite side of the circle. (a) Find the gravitational force of one star on the another. (b) Find the orbital speed of each star and their periods. (c):, How much energy would be needed to separate the two stars to the infinity?

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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2. Two identical stars with radius R and mass M, orbits around their center of mass. The orbit is circular, and the stars are always on the opposite side of the circle. (a) Find the gravitational force of one star on the another. (b) Find the orbital speed of each star and their periods. (c):, How much energy would be needed to separate the two stars to the infinity? Page 1 of 2
Transcribed Image Text:2. Two identical stars with radius R and mass M, orbits around their center of mass. The orbit is circular, and the stars are always on the opposite side of the circle. (a) Find the gravitational force of one star on the another. (b) Find the orbital speed of each star and their periods. (c):, How much energy would be needed to separate the two stars to the infinity? Page 1 of 2
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