Methods for the Study of the Dynamics of the Oort Cloud Comets I: Modelling the Stellar Perturbations

DOI10.1007/978-3-540-72984-6_9zbMath1157.85304OpenAlexW1882049040MaRDI QIDQ3613186

Giovanni B. Valsecchi, Marc Fouchard, Hans Rickman, Christiane Froeschlé

Publication date: 12 March 2009

Published in: Topics in Gravitational Dynamics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/978-3-540-72984-6_9

Mathematics Subject Classification ID

Celestial mechanics (70F15) Galactic and stellar dynamics (85A05)

Related Items (1)

Long-term orbital dynamics of trans-Neptunian objects

Cites Work

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• On solving Kepler's equation for nearly rectilinear hyperbolic orbits
• The structure and evolution of the Solar System comet cloud
• The solution of Kepler's equation, III
• Stellar perturbations on the scattered disk

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