🌌 Stellar Endpoints: From Star to Black Hole

Squeeze a dead star's remnant mass past the Chandrasekhar and Tolman-Oppenheimer-Volkoff limits and watch it cross from white dwarf to neutron star to black hole, with radius, escape velocity and a spacetime-curvature grid updating from real astrophysics formulas.

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