🪐 Orbital Resonance Dynamics (2D): Kirkwood Gaps from a Restricted Three-Body Integration with Jupiter
2D companion of the orbital resonance sim: a restricted three-body leapfrog integration of up to 400 asteroids with Jupiter, showing mean-motion resonances pumping eccentricity and opening Kirkwood gaps, with Kepler III and conservation checks.
⚙ Under the hood
The 2D companion of the orbital resonance dynamics sim: a restricted three-body integration of an asteroid belt with Jupiter, showing mean-motion resonances pumping eccentricity and opening Kirkwood gaps, with checks of Kepler's third law and conservation laws.
Orbital ResonanceKirkwood GapsThree-Body ProblemAsteroid BeltCelestial Mechanics
2D · HTML5 Canvas 2D · 60 FPS target · runs fully client-side, no install