Skip to main content

Dwarf-system satellite

Xiangliu

Gonggong’s small companion on an elongated orbit.

Xiangliu is faint and distant, but its orbit helps constrain the total mass of the Gonggong system. The available source set supports a representative eccentric path rather than a complete pole solution.

Orbit representation
Representative mean elements
Surface
procedural reconstruction

Reference measurements

The numbers that shape this world

Mean radius
50 km
Mean orbital distance
24,020 km
Orbital period
25.22 days
Eccentricity
0.29
Inclination
UnresolvedRepresentative parent-equatorial visual plane; source-backed pole unresolved
Orbit plane
Representative

System portrait

Useful measurements at the edge of visibility

The page is deliberately honest about what is known: mean scale, period and eccentricity are useful, while the full three-dimensional orientation is not asserted.

System geometry

Xiangliu around Gonggong

Xiangliu orbits at a mean distance of 24,020 km with a period of 25.22 days. Its catalogued eccentricity is 0.29, and the orbital inclination is not asserted relative to Representative parent-equatorial visual plane; source-backed pole unresolved. Missing angular orientation stays explicitly representative.

Representation notes

What Explore is showing

A representative eccentric orbit is shown; pole and longitude are not asserted.

Reference-guided visual reconstruction based on cited mission records; no source raster is reproduced.

Provenance

Sources and related destinations