Binary asteroids in mean-motion resonances

Natasa Todorovic; Ivana Milic Zitnik

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arXiv · 2512.09868

Binary asteroids in mean-motion resonances

Natasa Todorovic·Ivana Milic Zitnik

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Abstract

The purpose of this study is to investigate the relation between binary asteroids and mean motion resonances (MMRs). For more than 700 asteroids from two catalogues, the Johnston Archive [Johnston, 2024] and the Gaia DR3 VizieR list of binary candidates from Liberato et al. [2024], we applied a resonance identification algorithm, treating all planetary perturbations. Our results showed that the presence of binary asteroids in MMRs largely depends on their dynamical class. The highest percentage, more than 30%, is found in the Trans- Neptunian region, where most of these objects have exhibited resonant librations longer than 10 Myr. For the main-belt asteroid pairs, this percentage is about 10-12%. Contrary to expectations, the more unstable region populated with NEOs, showed a higher percentage of resonant pairs (above 17%), but with temporal resonant captures. These results could indicate that the mean motion resonances, particularly the stronger ones, could play a role in the evolution and formation of binary systems. Finally, we highlight that in the present paper, 82 resonant binary asteroids are newly identified.

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Natasa Todorovic, Ivana Milic Zitnik. 2025-12-10. Binary asteroids in mean-motion resonances. https://arxiv.org/abs/2512.09868

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