Long-term evolution of orbits about a precessing oblate planet. II: The case of variable precession

DOI10.1007/s10569-006-9046-5zbMath1117.70024arXivastro-ph/0607522OpenAlexW2000621959MaRDI QIDQ861393

Michael Efroimsky

Publication date: 29 January 2007

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0607522

zbMATH Keywords

equinoctial precessionnonosculating elementsosculating elements

Mathematics Subject Classification ID

Celestial mechanics (70F15) Orbital mechanics (70M20)

Related Items (4)

Planetary orbital equations in externally-perturbed systems: position and velocity-dependent forces ⋮ Tidal torques: a critical review of some techniques ⋮ A resonant-term-based model including a nascent disk, precession, and oblateness: application to GJ 876 ⋮ Long-term evolution of orbits about a precessing oblate planet: III: A semianalytical and a purely numerical approach

Cites Work

• Unnamed Item
• The Serret-Andoyer formalism in rigid-body dynamics. I. Symmetries and perturbations
• Motion of the orbital plane of a satellite due to a secular change of the obliquity of its mother planet
• Long-term evolution of orbits about a precessing oblate planet. I: The case of uniform precession
• Long-term evolution of orbits about a precessing oblate planet: III: A semianalytical and a purely numerical approach
• The theory of canonical perturbations applied to attitude dynamics and to the Earth rotation. Osculating and nonosculating Andoyer variables
• Gauge Freedom in Orbital Mechanics
• Gauge symmetry of the N-body problem in the Hamilton–Jacobi approach
• Gauge freedom in theN-body problem of celestial mechanics

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