| Minorplanet: | yes |
| Background: |
|
| Discoverer: | Spacewatch (291) |
| Discovered: | 30 October 2002 |
| Earliest Precovery Date: | 12 October 1991 |
| Mp Category: | Cubewano (MPC) Extended (DES) |
| Epoch: | 4 September 2017 (JD 2458000.5) |
| Uncertainty: | 2 |
| Observation Arc: | 25.26 yr (9,228 days) |
| Perihelion: | 36.485 AU |
| Time Periastron: | ≈ 5 September 2066[1] ±3 days |
| Semimajor: | 42.488 AU |
| Eccentricity: | 0.1413 |
| Period: | 276.95 yr (101,157 days) |
| Mean Motion: | / day |
| Inclination: | 19.484° |
| Asc Node: | 204.68° |
| Arg Peri: | 279.00° |
| Satellites: | 1 (ø: 190–260 km) |
| Mean Diameter: | |
| Density: | (assuming equal densities for primary and satellite) |
| Surface Grav: | 0.075 m/s2 |
| Escape Velocity: | 0.227 km/s |
| Spectral Type: | B–V= V−R= V−I= |
| Magnitude: | 19.8 |
| Abs Magnitude: | , 4.0 |
| Albedo: | |
| Single Temperature: | ≈ 43 K |
(provisional designation ) is a 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; as of June 2024, the object has yet to be named.
has an absolute magnitude of about 4.0, and Spitzer Space Telescope results estimate it to be about 681 km in diameter. The low density of this and many other mid sized TNOs implies that they have likely never compressed into fully solid bodies, let alone differentiated or collapsed into hydrostatic equilibrium, and so are highly unlikely to be dwarf planets.[2]
This minor planet was numbered (55637) by the Minor Planet Center on 16 February 2003 ., it has not been named.
has a perihelion of 36.7 AU, which it will next reach in 2065. As of 2020, is 40 AU from the Sun.
The Minor Planet Center classifies as a cubewano while the Deep Ecliptic Survey (DES) classifies it as scattered-extended. The DES using a 10 My integration (last observation: 2009-10-22) shows it with a minimum perihelion (qmin) distance of 36.3 AU.
It has been observed 212 times with precovery images dating back to 1991.
A variability of the visual brightness was detected which could be fit to a period of 14.38 or 16.78 h (depending on a single-peaked or double peaked curve). The light-curve amplitude is ΔM = .
The analysis of combined thermal radiometry of from measurements by the Spitzer Space Telescope and Herschel Space Telescope indicates an effective diameter of and albedo of 0.107. Assuming equal albedos for the primary and secondary it leads to the size estimates of ~664 km and ~190 km, respectively. If the albedo of the secondary is half of that of the primary the estimates become ~640 and ~260 km, respectively. Using an improved thermophysical model slightly different sizes were obtained for UX25 and its satellite: 659 km and 230 km, respectively.
has red featureless spectrum in the visible and near-infrared but has a negative slope in the K-band, which may indicate the presence of the methanol compounds on the surface. It is redder than Varuna, unlike its neutral-colored "twin", in spite of similar brightness and orbital elements.
With a density of 0.82 g/cm3, assuming that the primary and satellite have the same density, is one of the largest known solid objects in the Solar System that is less dense than water. Why this should be is not well understood, because objects of its size in the Kuiper belt often contain a fair amount of rock and are hence pretty dense. To have a similar composition to others large KBOs, it would have to be exceptionally porous, which was believed to be unlikely given the compactability of water ice; this low density thus astonished astronomers. Studies by Grundy et al. suggest that at the low temperatures that prevail beyond Neptune, ice is brittle and can support significant porosity in objects significantly larger than, particularly if rock is present; the low density could thus be a consequence of this object failing to warm sufficiently during its formation to significantly deform the ice and fill these pore spaces.[3]
| align=left | Settled snow | 0.2–0.3 | ||
| align=left | Slush/firn | 0.7–0.8 | ||
| align=left | 0.82 | |||
| align=left | Glacier ice | 0.83–0.92 | ||
| align=left | Tethys | 0.984 | [4] | |
| align=left | Liquid water | 1 |
| S/2005 (55637) 1 | |
| Discoverer: | Brown et al. |
| Discovered: | 2007 |
| Period: | (prograde) |
| Inclination: | 63.1° |
| Satellite Of: | 2002 UX25 |
The discovery of a minor-planet moon was reported in IAUC 8812 on 22 February 2007. The satellite was detected using the Hubble Space Telescope in August 2005. The satellite was found at 0.16 arcsec from the primary with an apparent magnitude difference of 2.5. It orbits the primary in days, at a distance of, yielding a system mass of . The eccentricity of the orbit is .
This moon is estimated to be in diameter. Assuming the same albedo as the primary, it would have a diameter of 190 km, assuming an albedo of 0.05 (typical of other cold, classical KBOs of similar size) a diameter of 260 km.