Close-to-fission dumbbell Jupiter-Trojan (17365) Thymbraeus
Abstract
Every population of small bodies in the Solar system contains a sizable fraction of multiple systems. Among these, the Jupiter Trojans have the lowest number of known binary systems and the least characterized. We aim at characterizing the reported binary system (17365) Thymbraeus, one of the only seven multiple systems known among Jupiter Trojans. We conducted light curves observing campaigns in 2013, 2015, and 2021 with ground-based telescopes. We model these lightcurves using dumbbell equilibrium figures. We show that Thymbraeus is unlikely a binary system. Its light curves are fully consistent with a bilobated shape: a dumbbell equilibrium figure. We determine a low density of 830 +/- 50 kg.m-3 , consistent with the reported density of other Jupiter Trojan asteroids and small Kuiper-belt objects. The angular velocity of Thymbraeus is close to fission. If separated, its components would become a similarly-sized double asteroid such as the other Jupiter Trojan (617) Patroclus.
Keywords
Cite
@article{arxiv.2309.15537,
title = {Close-to-fission dumbbell Jupiter-Trojan (17365) Thymbraeus},
author = {B. Carry and P. Descamps and M. Ferrais and J. -P. Rivet and J. Berthier and E. Jehin and D. Vernet and L. Abe and P. Bendjoya and F. Vachier and M. Pajuelo and M. Birlan and F. Colas and Z. Benkhaldoun},
journal= {arXiv preprint arXiv:2309.15537},
year = {2023}
}
Comments
accepted for publication in A&A