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?

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
Chapter11: Gravity, Planetary Orbits, And The Hydrogen Atom
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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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