Two identical stars with mass M orbit around their center of mass. Each orbit is circular and has radius R, so that the two stars are always on opposite sides of the circle. Part A Find the gravitational force of one star on the other. Exproc r in torms of C MR

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Chapter1: Units, Trigonometry. And Vectors
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Part C
Find the the period of the orbit of each star.
Express your answer in terms of G, M, R.
T =
Part D
How much energy would be required to separate the two stars to infinity?
Express your answer in terms of G, M, R.
?
ΔΕΞ
Transcribed Image Text:Part C Find the the period of the orbit of each star. Express your answer in terms of G, M, R. T = Part D How much energy would be required to separate the two stars to infinity? Express your answer in terms of G, M, R. ? ΔΕΞ
Two identical stars with mass M orbit around their center of
mass. Each orbit is circular and has radius R, so that the two
stars are always on opposite sides of the circle.
Part A
Find the gravitational force of one star on the other.
Express your answer in terms of G, M, R.
Πν ΑΣφ
?
F =
Part B
Find the orbital speed of each star.
Express your answer in terms of G, M, R.
να ΑΣΦ7
?
Part C
Transcribed Image Text:Two identical stars with mass M orbit around their center of mass. Each orbit is circular and has radius R, so that the two stars are always on opposite sides of the circle. Part A Find the gravitational force of one star on the other. Express your answer in terms of G, M, R. Πν ΑΣφ ? F = Part B Find the orbital speed of each star. Express your answer in terms of G, M, R. να ΑΣΦ7 ? Part C
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