The Hungaria region as a possible source of Trojans and satellites in the inner Solar system

Author(s)
Mattia Galiazzo, Richard Schwarz
Abstract

The Hungaria family (the closest region of the Main Belt to Mars) is an important source of planet-crossing asteroids and even impactors of terrestrial planets. We present the possibility of asteroids coming from the Hungaria family being captured into co-orbital motion with the terrestrial planets in the inner Solar system. Therefore, we have carried out long-term numerical integrations (up to 100 Myr) to analyse migrations from their original location - the Hungaria family region - into the inner Solar system. During the integration time, we observed whether or not the Hungarias are captured into co-orbital motion with the terrestrial planets. Our results show that 5.5 per cent of 200 Hungarias, selected as a sample of the whole group, escape from the Hungaria region and the probability of becoming co-orbital objects (Trojans, satellites or horseshoes) turns out to be ~3.3 per cent: 1.8 per cent for Mars and 1.5 per cent for Earth. In addition, we distinguished the classes of co-orbital motion into which the asteroids are captured and how long they stay there in stable motion. Most of the escaped Hungarias become quasi-satellites and the ones captured as Trojans favour the L5 Lagrangian point. This work highlights the fact that the Hungaria region is a source of Mars and also Earth co-orbital objects.

Organisation(s)
Department of Astrophysics
Journal
Monthly Notices of the Royal Astronomical Society
Volume
445
Pages
3999 - 4007
No. of pages
9
ISSN
0035-8711
DOI
https://doi.org/10.1093/mnras/stu2016
Publication date
12-2014
Peer reviewed
Yes
Austrian Fields of Science 2012
103003 Astronomy, 103004 Astrophysics
Keywords
ASJC Scopus subject areas
Astronomy and Astrophysics, Space and Planetary Science
Portal url
https://ucrisportal.univie.ac.at/en/publications/the-hungaria-region-as-a-possible-source-of-trojans-and-satellites-in-the-inner-solar-system(0389e027-21b1-4127-bb03-1011e1bf0d11).html