Binary Star initial positions and velocities

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SUMMARY

The discussion focuses on computing binary star orbits based on initial parameters, specifically positions and velocities expressed in terms of mass. The stars are positioned along the x-axis, with the primary star at (-x, 0) and the secondary star at (x, 0), orbiting around a common center of mass at the origin. The relevant dimensionless properties are defined as Massprimary ≡ Massprimary/M and Masssecondary ≡ Masssecondary/M, where M is the total mass of the system. The user successfully determined the mass ratios as Primary = 4/5 and Secondary = 1/5 but struggles to express initial positions and velocities in terms of these mass ratios.

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  • Understanding of binary star systems and orbital mechanics
  • Familiarity with center of mass calculations
  • Knowledge of dimensionless properties in physics
  • Basic principles of circular motion and gravitational forces
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  • Research the concept of center of mass in binary systems
  • Study the equations of motion for circular orbits in celestial mechanics
  • Learn how to express positions and velocities in terms of mass ratios
  • Explore gravitational force balance in circular orbits
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Astronomers, astrophysicists, and students studying celestial mechanics who are interested in understanding binary star dynamics and orbital calculations.

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


[/B]
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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