HomeSpace & AstronomyGalactic Tide & the Oort Cloud Loss Cone (2D)

Galactic Tide & the Oort Cloud Loss Cone (2D)

A 2D secular-perturbation model of the galactic tide: track a population of Oort Cloud comets' eccentricity and perihelion distance evolving under the Milky Way's own gravity, via orbit-averaged Gauss perturbation equations, until some dip into the loss cone.

Space & Astronomy2DAdvanced60 FPS📱 Mobile-adapted⇄ 3D version
2d-oort-cloud-space ↗ Open standalone

The same physical mechanism as the 3D flagship version, seen from directly above: instead of integrating fast day-to-day orbital motion, this model evolves each of 220 comets' orbital shape and orientation directly using the orbit-averaged (secular) Gauss perturbation equations for the Milky Way disk's vertical tidal field — the same mathematical machinery behind the Kozai–Lidov mechanism. Watch eccentricity and perihelion distance slowly rock back and forth over tens of millions of simulated years as each ellipse's argument of perihelion precesses, until some comets' perihelion dips below the loss-cone threshold and they flash red — the trickle-feed mechanism believed to supply long-period comets without needing a passing star. Adjust the local galactic density, coupling strength, playback speed and loss-cone threshold, and track live readouts of elapsed time, population inside the loss cone, and mean perihelion.

⚙ Under the hood

Evolve 220 Oort Cloud comets' eccentricity and perihelion via the orbit-averaged Gauss perturbation equations for the Milky Way's own vertical tidal force, and watch their ellipses slowly rock until some dip into the giant-planet loss cone.

Oort cloudgalactic tideorbital mechanicssecular perturbationKozai-Lidov mechanismloss cone

2D · HTML5 Canvas 2D · 60 FPS target · runs fully client-side, no install

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