Earth Gravitational capture disc Resonant-return keyhole Orbit-solution clones
B-plane view. Axes independently normalised — not to true relative scale. Drag to pan, scroll to zoom.
Keyhole-capture probability vs. observation arc (log/log)

Asteroid Impact Risk: B-Plane Keyhole Analysis (2D)

Planetary-defense teams don't track a single predicted path for a hazardous asteroid — they track a whole cloud of orbit solutions consistent with the observations, projected onto the b-plane at the moment of closest approach. This 2D simulator generates that cloud as a real 2D-Gaussian "line of variations" scatter plot, lets you shrink it by lengthening the observation arc, and places a small gravitational keyhole nearby — a patch of the b-plane so narrow that only a tiny slice of the uncertainty cloud passing through it would set up a resonant return and a possible future impact, the same logic used to rule Apophis's 2029 keyhole in and back out. Drag and zoom the scatter plot to inspect the cloud, adjust the approach speed to see Earth's gravitationally focused capture disc grow or shrink, and watch the live analytical readouts and the risk-vs-arc-length curve track how a wider observation arc reshapes the impact risk.