HomeSpace & AstronomyKuiper Belt Resonances: Plutinos & the 3:2 Lock with Neptune

Kuiper Belt Resonances: Plutinos & the 3:2 Lock with Neptune

Interactive 3D Kuiper Belt: watch Plutinos librate in Neptune's 3:2 mean-motion resonance and Twotinos in the 2:1, alongside the classical belt and scattered disk, with a live resonant-argument readout.

Space & Astronomy3DAdvanced60 FPS
kuiper-belt-space ↗ Open standalone

The Kuiper Belt is not a uniform ring of debris — it is carved into sharply defined populations by Neptune's gravity. This simulator renders the Sun, Neptune and hundreds of trans-Neptunian objects on real Keplerian orbits, sized and colored by dynamical class: the classical belt, the resonant Plutinos locked in Neptune's 3:2 mean-motion resonance (the class Pluto itself belongs to), the Twotinos in the 2:1 resonance, and the eccentric scattered disk. A live readout tracks one Plutino's resonant argument φ = 3λ − 2λN − ϖ librating back and forth like a pendulum instead of circulating through 360° — the defining signature of orbital resonance — while sliders let you speed up time and dial the libration amplitude up or down to see gently- versus deeply-captured resonant orbits.

⚙ Under the hood

Watch trans-Neptunian objects on real Keplerian orbits split into dynamical classes -- Plutinos librating in Neptune's 3:2 mean-motion resonance, Twotinos in the 2:1, the classical belt, and the scattered disk -- with a live resonant-argument readout.

kuiper-beltorbital-resonanceneptuneplutinocelestial-mechanics

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

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