Orbit from osculating elements
Arrokoth is placed by solving a Keplerian orbit around sun at the simulation time (a = 44.1 AU, e = 0.03555717645015258, i = 2.5°, period 106,796.1 d).
A primordial contact binary in the Kuiper belt visited by New Horizons in 2019.
Also known as 486958, 486958 Arrokoth, 2014 MU69.
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.
Arrokoth is placed by solving a Keplerian orbit around sun at the simulation time (a = 44.1 AU, e = 0.03555717645015258, i = 2.5°, period 106,796.1 d).
Arrokoth is presented using mission-derived shape; approximate reflectance and orientation data.
Arrokoth: mean radius 18 km. 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 navigable silhouette uses the Porter 2024 mission shape model. Uniform reddish reflectance is illustrative; this reference image is not a global surface map.
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.
| Dataset | Last refreshed | Horizon | Automated |
|---|---|---|---|
| Current comets and near-Earth asteroids | no snapshot date | Osculating elements at the snapshot epoch; propagated as two-body conics | Yes, weekly (Monday data job) npm run fetch:data |