Dynamics of two satellites in the 2/1 mean-motion resonance: application to the case of Enceladus and Dione
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Publication:880945
DOI10.1007/S10569-007-9066-9zbMath1111.70011OpenAlexW2171779574MaRDI QIDQ880945
Publication date: 21 May 2007
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10569-007-9066-9
Three-body problems (70F07) Celestial mechanics (70F15) Generalized coordinates; event, impulse-energy, configuration, state, or phase space for problems in mechanics (70G10)
Related Items (4)
Dynamic expansion points: an extension to Hadjidemetriou's mapping method ⋮ The orbit of Aegaeon and the 7:6 Mimas-Aegaeon resonance ⋮ Dynamics of Enceladus and Dione inside the 2:1 mean-motion resonance under tidal dissipation ⋮ The current orbit of Methone (S/2004 S 1)
Cites Work
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- Motion of two planets with periods commensurable in the ratio 2?1 solutions of the hori auxiliary system
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