Explore general relativity through interactive 3D spacetime curvature. Choose a scenario to begin.
Weak-field nearly Newtonian elliptical orbit
Classic GR prediction of orbital precession
Exact circular geodesic at r = 70M (Venus-like distance)
Stable circular orbit just above the ISCO at r = 7M
Spiraling past the event horizon
Near-critical photon orbit grazing r = 3M
Multiple photon paths bending around mass