Binary Star initial positions and velocities

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The discussion focuses on computing binary star orbits based on their initial positions and velocities, with an emphasis on expressing these parameters in terms of mass. The stars are positioned on the x-axis at time t=0, with the primary star on the negative side and the secondary on the positive side. The user has determined the mass ratios of the stars but struggles to express their initial positions and velocities in terms of mass. There is a request for assistance in understanding how to relate these parameters, particularly in the context of circular orbits and the forces involved. The conversation highlights the need for clarity on the relationship between mass and orbital mechanics.
Astro_Husky
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Hi all,

I've been tasked with computing binary star orbits based on their initial parameters, positions and velocities.
In this problem everything must be expressed in terms of the masses, but I am struggling to define positions and velocities in terms of mass.
It is assumed that the stars are in circular orbits around a common center of mass at the origin (0,0) and the stars are on the x-axis (y=0) at time t=0. The primary star is on the negative x-axis and the secondary is on the positive x axis.

Using the relevant dimensionless properties:
Massprimary ≡ Massprimary/M
Masssecondary ≡ Masssecondary/M
where M = Massprimary + Masssecondary

Distance = Xprimary ≡ Xprimary/a
Xsecondary ≡ Xsecondary/a
where, a = initial binary separation

Time = t ≡ t/(sqrt(a^3/GM))

The Attempt at a Solution


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I got as far as determining the masses of the stars: Primary = 4/5, Secondary = 1/5.
I cannot even begin to express the initial positions and velocities in terms of mass.
Any help would be very much appreciated.
 
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Astro_Husky said:
I got as far as determining the masses of the stars: Primary = 4/5, Secondary = 1/5.
How? I don't see any given data in your problem statement from which such results could be derived.
I cannot even begin to express the initial positions and velocities in terms of mass.
Any help would be very much appreciated.
For circular orbits, what forces are always in balance?
 

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