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Kepler's Third Law: Orbital Resonance Countdown (3D)

Watch two or three orbiting bodies whose radii obey Kepler's third law lock into an integer-ratio resonance — like Pluto-Neptune (3:2) or the Galilean moons (1:2:4) — with a live countdown to the next exact realignment, and a slider that detunes the ratio to break the resonance.

Space & Astronomy3DModerate60 FPS📱 Mobile-adapted⇄ 2D version
3d-kepler-orbital-resonance-countdown ↗ Open standalone

Two or three bodies orbit a central mass with radii and periods genuinely linked by Kepler's third law, T² ∝ r³. Set an integer period ratio and the bodies lock into a real orbital resonance — the same mechanism behind Pluto's 3:2 lock with Neptune and the 1:2:4 Laplace resonance of Jupiter's Galilean moons — with a live countdown to the next exact realignment of the starting configuration. Detune the ratio slider away from a simple fraction and the countdown vanishes: the bodies drift through every relative angle and the traced path never closes, the real observable difference between a resonant and a non-resonant orbit.

⚙ Under the hood

Two or three orbiting bodies with radii set by Kepler's third law lock into an integer-ratio resonance like Pluto-Neptune (3:2) or the Galilean moons (1:2:4), with a live countdown to the next exact realignment.

orbital-resonancekeplers-third-lawlaplace-resonanceastronomynew-year

3D · Three.js / WebGL renderer · 60 FPS target · runs fully client-side, no install

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