Mean-motion resonances in the Solar system
A curated collection of essential papers on mean-motion resonances in the asteroid belt, TNO, and beyond.
Carruba, V. et al. (2021)
A neural network classified Mars-resonant asteroid orbits with over 85% accuracy, extending resonance studies to many known asteroids.
This study brings artificial neural networks into asteroid dynamics by automatically identifying orbital behavior in asteroids influenced by the Mars 1:2 mean-motion resonance. The authors report better than 85% performance on standard classification metrics and use supervised learning, optimized with genetic algorithms, to assign orbital status across numbered and multi-opposition asteroids in the region. The work shows that machine learning can scale resonance classification and reinforces that this resonance chiefly affects the Massalia, Nysa, and Vesta asteroid families.
The paper uses supervised artificial neural network classification, with genetic algorithm optimization, to label resonance-related asteroid orbital behavior.
Basic background in asteroid orbital dynamics, mean-motion resonances, and introductory machine learning is helpful.
A curated collection of essential papers on mean-motion resonances in the asteroid belt, TNO, and beyond.
A companion collection for the ACM 2026 talk by Valerio Carruba