Mapping the structure of the planetary 2:1 mean motion resonance: the TOI-216, K2-24, and HD27894 systems

DOI10.1007/S10569-022-10112-5OpenAlexW4315628470WikidataQ117748312 ScholiaQ117748312MaRDI QIDQ2685194

Viviam Alencastro, Fernando Roig, Cristian Giuppone, Tabaré Gallardo, Adrián Rodríguez

Publication date: 20 February 2023

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10569-022-10112-5

zbMATH Keywords

stabilitybifurcationsemi-numerical methodasymmetric librationdynamical mapextrasolar planetstable resonant equilibriumsymmetric libration

Mathematics Subject Classification ID

Computational methods for problems pertaining to mechanics of particles and systems (70-08) Astronomy and astrophysics (85A99) Celestial mechanics (70F15)

Cites Work

• Phase space structure of multi-dimensional systems by means of the mean exponential growth factor of nearby orbits
• Asymmetric librations in exterior resonances
• Unnamed Item

This page was built for publication: Mapping the structure of the planetary 2:1 mean motion resonance: the TOI-216, K2-24, and HD27894 systems