A second order Jupiter-Saturn planetary theory
From MaRDI portal
Publication:5895492
DOI10.1007/BF00929996zbMath0557.70015OpenAlexW4253975687MaRDI QIDQ5895492
Abdel Aziz Bakry, Osman M. Kamel
Publication date: 1982
Published in: The Moon and the Planets (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/bf00929996
von Zeipel's methodPoincaré canonical variablesJacobi-Radau referentialsecond order secular Jupiter-Saturn planetary theory
Related Items (3)
Second order secular planetary theory for the four major planets ⋮ The construction of a fifth-order Jupiter-Saturn motion: Analytical theory. I: Outline ⋮ A second order Jupiter-Saturn planetary theory
Cites Work
- Expansion of the inverse of mutual distance between two bodies raised to any power
- Elimination of the critical terms in a first-order general planetary theory
- Invariance in Von Zeipel method
- [https://portal.mardi4nfdi.de/wiki/Publication:4118118 Perturbations des syst�mes diff�rentiels et r�sultats de g�om�trie diff�rentielle]
- Canonical transformations depending on a small parameter
- A discussion of Hill's method of secular perturbations and its application to the determination of the zero-rank effects in non-singular vectorial elements of a planetary motion
- Explicit recursive algorithms for the construction of equivalent canonical transformations
- The influence of the great inequality on the secular disturbing function of the planetary system
This page was built for publication: A second order Jupiter-Saturn planetary theory
