Rotation of a Planet in a Three-Body System: a Non-Resonant Case
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Publication:6054845
DOI10.20537/ND221001zbMath1528.70020OpenAlexW4312400116MaRDI QIDQ6054845
Publication date: 28 September 2023
Published in: Nelineinaya Dinamika (Search for Journal in Brave)
Full work available at URL: http://mathnet.ru/eng/nd809
small parameteraveragingangular momentum axisnutation angleKeplerian ellipseHamilton evolution equationsexo-Earthexo-Moonexo-Sun
Cites Work
- Impact of a Moon on the evolution of a planet's rotation axis: a non-resonant case
- Mathematical aspects of classical and celestial mechanics. Transl. from the Russian by E. Khukhro.
- A second fundamental model for resonance
- The analysis of restricted circular twice-averaged three body problem in the case of close orbits
- Solar System Dynamics
- On evolution of the planet's obliquity in a non-resonant planetary system
- Resonance rotation of celestial bodies and Cassini's laws
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