Evolution of the obliquity of an exoplanet: A non-resonant case

Author:

Podvigina O.M.,Krasilnikov P.S.

Funder

Russian Foundation for Fundamental Investigations

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference55 articles.

1. The doubly averaged elliptical restricted three-body problem;Aksenov;Sov. Astron.,1979

2. Cours De Mécanique Céleste;Andoyer,1923

3. Effects of extreme obliquity variations on the habitability of Exoplanets;Armstrong;Astrobiology,2014

4. Mathematical Aspects of Classical and Celestial Nechanics;Arnold,2006

5. Obliquity evolution of extrasolar terrestrial planets;Atobe;Icarus,2007

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1. On the exo-planet precession under torqes due to three celestial bodies with the evolution of the satellite's orbit;Vestnik Udmurtskogo Universiteta. Matematika. Mekhanika. Komp'yuternye Nauki;2022-06

2. Impact of a moon on the evolution of a planet’s rotation axis: a non-resonant case;Celestial Mechanics and Dynamical Astronomy;2022-04-20

3. Averaging method and coherence applied to Rabi oscillations in a two-level system;Journal of Physics Communications;2021-09-01

4. Displacements of Points of a Viscoelastic Ball Caused by Tides;Journal of Physics: Conference Series;2020-12-01

5. On the exoplanet obliquity variations in planetary four – body problem with evolving satellite’s orbit;IOP Conference Series: Materials Science and Engineering;2020-09-01

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