| Minorplanet: | yes |
| Background: |
|
| Discovered: | 29 April 2011 |
| Epoch: | 4 September 2017 (JD 2458000.5) |
| Uncertainty: | 6 |
| Observation Arc: | (354 days) |
| Perihelion: | 27.660 AU |
| Semimajor: | 30.219 AU |
| Eccentricity: | 0.0847 |
| Period: | 166.12 yr (60,675 days) |
| Mean Motion: | / day |
| Inclination: | 29.348° |
| Asc Node: | 100.97° |
| Arg Peri: | 151.24° |
| Dimensions: | 100 km |
| Abs Magnitude: | 8.1 |
is the ninth Neptune trojan discovered. It was first observed on 29 April 2011, during the New Horizons KBO Search using the Magellan II (Clay) Telescope at Las Campanas Observatory in Chile. It has the same orbital period as Neptune and orbits at the Lagrangian point about 60° backwards of Neptune.
Neptune trojans are resonant trans-Neptunian objects (TNO) in a 1:1 mean-motion orbital resonance with Neptune. These Trojans have a semi-major axis (a) very similar Neptune's (30.10 AU).
orbits the Sun with a semi-major axis of 30.219 AU at a distance of 27.7–32.8 AU once every 166 years and 1 month (60,675 days). Its orbit has an eccentricity of 0.08 and an inclination of 29° with respect to the ecliptic. Among the first 17 Neptune trojans discovered so far, it is the one with the highest inclination.
Based on a generic magnitude-to-diameter conversion, it measures approximately 100 kilometers in diameter using an absolute magnitude of 8.1 and an assumed albedo of 0.10. It is an averaged-sized body among the first 17 Neptune trojans discovered so far, which measure between 60 and 200 kilometers (for an absolute magnitude of 9.3–6.6 and an assumed albedo of 0.10).
Observations with NIRSpec showed that the spectrum of 2011 HM102 does not exhibit clear Triton-like ice tholin features. The surface is likely covered in a thin layer of water ice and CO2 ice. Due to the variable color classification of this object, it is suspected that inhomogeneities in the surface composition exist.[1]
Due to its orbital uncertainty, this minor planet has not been numbered and its official discoverers have not been determined. If named, it will follow the naming scheme already established with 385571 Otrera, which is to name these objects after figures related to the Amazons, an all-female warrior tribe that fought in the Trojan War on the side of the Trojans against the Greek.[2]
In October 2012, was the closest known object of any kind to the New Horizons spacecraft. In mid- to late 2013, New Horizons passed within 1.2 AU of, where it would be detectable with one of the onboard instruments. An observation from New Horizons would measure the phase curve of at phase angles unobtainable from Earth. The New Horizons team eventually decided that they would not target for observations because the preparations for the Pluto approach took precedence.