Two Celestial Bodies in Orbit (Centripetal & Gravitational Forces)

  • #1
amandela
10
3
Homework Statement
Two identical stars, a fixed distance D apart, revolve in a circle about their mutual center of mass, as shown above. Each star has mass M and speed 𝜈. G is the universal gravitational constant. Which of the following is a correct relationship among these quantities?
Relevant Equations
F_g = Gm_1m_2/r^2
F_c = ma_c
So I did set the two above equations equal for the solution. But is that not in effect ignoring one of the m's in the orbital motion? I feel like it should be F_c = 2ma. How should I think about it?

Thank you.
del.png
 
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  • #2
Please show your actual work
 
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Likes jbriggs444
  • #3
amandela said:
I feel like it should be F_c = 2ma. How should I think about it?
What you feel is not what each of the stars "feels". Draw a free body diagram of only one of the stars. Put in the force(s) acting on it and only it. Find the net force and set it equal to its mass time its acceleration.

By the way, where are the "following" options from which you have to choose one?
 

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