Orbit from mean elements
Miranda is placed by solving a Keplerian orbit around uranus at the simulation time (a = 129,900 km, e = 0.0013, i = 4.2°, period 1.4 d).
A small Uranian moon with striking ridged coronae and faulted terrain.
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.
Miranda is placed by solving a Keplerian orbit around uranus at the simulation time (a = 129,900 km, e = 0.0013, i = 4.2°, period 1.4 d).
Miranda: mean radius 235.8 km. These values are bundled with the object record and drive the rendered size.
Voyager-based southern terrain from NASA’s display model, not a calibrated global albedo or relief map. The unobserved north remains plain gray.
Voyager-based southern terrain from NASA’s display model, not a calibrated global albedo or relief map. The unobserved north remains plain gray.
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 |
|---|---|---|---|
| Planetary satellite mean elements | no snapshot date | Mean elements (a, e, i, period) for every known natural satellite | No, refreshed by hand npm run generate:moons |