Disk Accretion

A disk of bodies around a star: 1/r² gravity (Barnes-Hut), leapfrog, perfect merging on contact. Scroll to zoom, drag to pan, double-click to re-centre, space to pause.

What this model simplifies

Each preset checks the simulation against a known answer. The full list, with tolerances and measured values, is in VALIDATION.md; the science results are in FINDINGS.md.