Astronomy19 papers
Mean-motion resonances in the Solar system
A curated collection of essential papers on mean-motion resonances in the asteroid belt, TNO, and beyond.
ES
Evgeny Smirnov
All Reviews
AstronomyNiche
intermediate
Identification of Asteroids in Two-Body Resonances
E. A. Smirnov & I. S. Dovgalev (2018)
- Published
- Jul 1, 2018
- Journal
- Solar System Research · Vol. 52 · No. 4
- DOI
- 10.1134/S0038094618040056
At a Glance
Large-scale overview of two-body resonances WITH ALL planets in the Solar System
Summary
The authors, using numerical integration of the equations of motion of numbered asteroids from the AstDyS catalog, identify asteroids that are in two-body resonances with the planets. Unlike previous studies, all eight planets are considered, rather than only Jupiter or Mars. The prevalence of two-body resonances in the Solar System is analyzed.
Method Snapshot
numerical integration
BackgroundAI
Celestial mechanics and basic concepts of mean-motion resonances and asteroid orbital dynamics.
The first survey of two-body MMRs in the Solar System
— ES