Trajectory from Horizons state vectors
99942 Apophis's position is interpolated between 937 heliocentric state-vector samples from JPL Horizons that run through 2032-01-01. Past the last sample the marker holds its final position.
A 340 m near-Earth asteroid. On April 13, 2029 it passes ~31,600 km above Earth's surface - inside the geostationary satellite ring - visible to the naked eye from Europe, Africa and western Asia. Impact ruled out for at least a century.
One record per aspect. The origin says what kind of thing each value is; the source says where it came from; the limit says what it cannot tell you.
99942 Apophis's position is interpolated between 937 heliocentric state-vector samples from JPL Horizons that run through 2032-01-01. Past the last sample the marker holds its final position.
99942 Apophis: mean radius 0.2 km; mass 6.100 × 10^10 kg. These values are bundled with the object record and drive the rendered size.
The surface is a procedural shape unless a source record above says otherwise. It is not a measured shape model.
The short description and the fact list are written by the Space Time authors for orientation. They are not quoted from a catalog field and carry no citation of their own.
Trajectory coverage: 2026-06-01 to 2032-01-01 (937 samples). Outside that window the marker holds its last known position.
| Dataset | Last refreshed | Horizon | Automated |
|---|---|---|---|
| Spacecraft trajectories (baked keyframes) | no snapshot date | Per craft: each evidence page states the first and last sample date | No, refreshed by hand scripts/bake-trajectories.mjs |