Click near the orbit to jump · drag to pan · scroll/pinch to zoom

Comet at Perihelion: Closest Approach (2D)

Seen from directly above the orbital plane, a comet's headlong rush past the Sun becomes a clean geometric fact: the two shaded wedges in this simulation always cover equal area for equal time, no matter how eccentric the orbit or how close the perihelion — that is Kepler's second law, made visible rather than asserted. Drag to pan and scroll to zoom around the scene, or click anywhere near the orbit to drop the comet at that exact point and read off its instantaneous speed and tail state.