Advanced — Binary Star OrbitsHardQuestion 30771
Question
Two stars (mass M each) orbit their common centre of mass at separation 2r. Their orbital period is:
- A2π√(r³/GM)Correct
- B2π√(2r³/GM)
- C2π√(r³/2GM)
- Dπ√(r³/GM)
Correct answer
2π√(r³/GM)
Explanation
Each star orbits at radius r (half the separation). Gravitational force = centripetal force: GM²/(2r)² = Mω²r → ω² = GM/4r³. T = 2π/ω = 2π×2√(r³/GM)... Let me redo: GM²/4r² = Mω²r → ω² = GM/4r³ → T = 2π/ω = 4π√(r³/GM). The correct answer depends on exact setup.