2011 HM102

Orbit and classification

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.

Physical properties

Diameter and albedo

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).

Surface

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.

Numbering and naming

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.

Exploration

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.

References

References

1. (6 Oct 2023). "First Near-IR Spectroscopic Survey of Neptune Trojans with JWST: Distinct Surface Compositions of Red vs Ultra-Red Neptune Trojans".
2. (10 April 2018). "DIVISION F / Working Group for Small Body Nomenclature Working Group for Small Body Nomenclature. THE TRIENNIAL REPORT (2015 Sept 1 - 2018 Feb 15)". IAU.