New approach to determining planetary perturbations in lunar theory

DOI10.1007/BF01233186zbMath0511.70014OpenAlexW2036911032MaRDI QIDQ4749263

T. V. Ivanova, V. A. Brumberg

Publication date: 1982

Published in: Celestial Mechanics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf01233186

zbMATH Keywords

successive approximationssemi-analyticalBESM-6 computerKepler's third lawintermediary orbitcoplanar circular motionsnumerical Fourier seriessemi-major axessolar and planetary perturbations of Moonuniversal Poisson series processor

Mathematics Subject Classification ID

Hamilton's equations (70H05) Celestial mechanics (70F15) Orbital mechanics (70M20) Canonical and symplectic transformations for problems in Hamiltonian and Lagrangian mechanics (70H15) Software, source code, etc. for problems pertaining to mechanics of particles and systems (70-04)

Related Items (1)

Celestial coordinate reference systems in curved space-time

Cites Work

• A new solution to the Main Problem of Lunar Theory
• Construction of a general planetary theory of the first order
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