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Binary Star Orbital Period Calculator

Binary Star Orbital Period Calculator computes period, velocity for two stars, plots orbit data.

Binary Star Orbital Dynamics

The calculator computes the orbital properties of a binary star system using Kepler’s Third Law for circular orbits:

Orbital Period:

\\[ T = 2\pi \sqrt{\frac{a^3}{G (M_1 + M_2)}} \\]

Orbital Velocity:

\\[ v = \sqrt{\frac{G (M_1 + M_2)}{a}} \\]

Where:

  • \\(T\\): Orbital period (yr)
  • \\(v\\): Orbital velocity (km/s)
  • \\(a\\): Separation (AU)
  • \\(M_1, M_2\\): Masses of the primary and secondary stars (\\(M_\odot\\))
  • \\(G\\): Gravitational constant (\\(4.302 \times 10^{-3} \, \text{pc} \, M_\odot^{-1} \, (\text{km/s})^2\\))

Example Calculation

Example: \\(M_1 = 1 M_\odot, M_2 = 1 M_\odot, a = 1 \, \text{AU}\\)

\\[ T = 2\pi \sqrt{\frac{1^3}{4.302 \times 10^{-3} \cdot (1 + 1)}} \approx 1.00 \, \text{yr} \\] \\[ v = \sqrt{\frac{4.302 \times 10^{-3} \cdot (1 + 1)}{1}} \approx 29.8 \, \text{km/s} \\]

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