55637 Uni

55637 Uni
Uni and Tinia as seen by the Hubble Space Telescope
Discovery
Discovered bySpacewatch (291)
Discovery siteKitt Peak National Obs.
Discovery date30 October 2002
Designations
Designation
(55637) Uni
Pronunciation/ˈjn/
Named after
Uni
2002 UX25
Cubewano (MPC)
Extended (DES)
Orbital characteristics
Epoch 5 May 2025 (JD 2460800.5)
Uncertainty parameter 0
Observation arc33.35 yr (12,182 days)
Earliest precovery date12 October 1991
Aphelion49.291 AU
Perihelion36.716 AU
43.003 AU
Eccentricity0.1462
282.01 yr (103,005 days)
4.54 km/s
309.49°
0° 0m 12.24s / day
Inclination19.400°
204.57°
≈ 5 September 2066
±3 days
275.27°
Known satellites1 (Tinia)
Physical characteristics
659±38 km
Mass(1.25±0.03)×1020 kg
Mean density
0.82±0.11 g/cm3
(assuming equal densities
for primary and satellite)
0.80±0.13 g/cm3
0.075 m/s2
0.227 km/s
14.382±0.001 h
Albedo0.107+0.005
−0.008

0.1±0.01
Temperature≈ 43 K
Spectral type
B–V=1.007±0.043
V−R=0.540±0.030
V−I=1.046±0.034
19.8
3.87±0.02, 4.0

55637 Uni (provisional designation 2002 UX25) is a large trans-Neptunian object that orbits the Sun in the Kuiper belt beyond Neptune. It briefly garnered scientific attention when it was found to have an unexpectedly low density of about 0.82 g/cm3. It was discovered on 30 October 2002, by the Spacewatch program.

Uni has an absolute magnitude of about 4.0, and Spitzer Space Telescope results estimate it to be about 660 km in diameter. The low density of this and many other mid-sized TNOs implies that they have never compressed into fully solid bodies, let alone differentiated or collapsed into hydrostatic equilibrium, and so are not likely to be dwarf planets.

Uni has one known moon, Tinia, discovered in 2005.