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.
Orbit from osculating elements
4179 Toutatis is placed by solving a Keplerian orbit at the simulation time (a = 2.5 AU, e = 0.625, i = 0.4°, period 1,480 d).
Epoch2025-11-21T00:00:00Z
MethodTwo-body propagation of the stored elements by the shared orbit service; no perturbations.
LimitA two-body orbit ignores planetary perturbations and non-gravitational forces; the dated JPL snapshot in the app's live catalog supersedes these bundled elements.
4179 Toutatis source record
4179 Toutatis is identified from the cited source record.
Bulk properties
4179 Toutatis: mean radius 2.7 km. These values are bundled with the object record and drive the rendered size.
Close-up appearance
The surface is a procedural shape unless a source record above says otherwise. It is not a measured shape model.
SourceSpace Time rendering contract
LimitNot a resolved observation.
Description and facts
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.
SourceSpace Time editorial text
LimitBackground reading is linked under Further reading; it is not the source of the displayed numbers.
Space Time