Nuclear and Orbital Characterization of the Transition Object (4015) 107P/Wilson-Harrington

TL;DR

This study investigates the nature of the transition object 107P/Wilson-Harrington through spectral analysis and orbital history, suggesting a primarily asteroidal origin with implications for understanding volatile retention on near-Earth objects.

Contribution

It provides new spectral data and orbital analysis of Wilson-Harrington, proposing a predominantly asteroidal origin and linking it to meteorite types and sample return targets.

Findings

Spectrum matches carbonaceous chondrites like Murchison and Ivuna.

Orbital history shows no high-temperature surface alteration.

Surface properties suggest a possible asteroidal origin.

Abstract

Comet 107P/Wilson-Harrington, cross-listed as asteroid 4015, is one of the original transition objects whose properties do not neatly fit into a cometary or asteroidal origin. Discovered in a period of apparently gas-dominated activity in 1949, it was subsequently lost and recovered as the inactive asteroid 1979 VA. We obtained new and re-analyzed archival observations of the object, compared to meteorites, and conducted new orbital integrations in order to understand the nature of this object and to understand where it falls on the asteroid-comet continuum. Wilson-Harrington's reflectance spectrum is approximately neutral from visible to near-infrared wavelengths, but has a reflectance maximum near 0.8-0.9 microns. The object's spectrum is well matched by laboratory spectra of carbonaceous chondrite meteorites like the CM Murchison or the CI Ivuna. The object's phase curve is compatible with either an asteroidal or cometary origin, and its recent orbital history has no periods with high enough temperatures to have altered its surface. While it is possible that some unknown process has acted to change the surface from an originally cometary one, we instead prefer a fundamentally asteroidal origin for Wilson-Harrington which can explain its surface and orbital properties. However, this would require a way to maintain significant (hyper-)volatile supplies on the near-Earth objects beyond what is currently expected. Wilson-Harrington's similar meteorite affinity and possible orbital link to sample return targets (162173) Ryugu and (101955) Bennu suggest that the returned samples from the Hayabusa-2 and OSIRIS-REx missions might hold the key to understanding this object.