Long period variations of the motion of a satellite due to non-resonant tesseral harmonics of a gravity potential

DOI10.1007/BF00692472zbMath0785.70022OpenAlexW4233080858MaRDI QIDQ1311632

Y. Boudon, Gilles Métris, F. Barlier, Pierre Exertier

Publication date: 27 April 1994

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

Full work available at URL: https://doi.org/10.1007/bf00692472

zbMATH Keywords

PhobosEarth's geodetic satellitesKaula eccentricity and inclination functionssecond order perturbationssecular effects

Mathematics Subject Classification ID

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

Related Items (3)

Closed-form perturbation theory in the restricted three-body problem without relegation ⋮ Dynamics of a satellite orbiting a planet with an inhomogeneous gravitational field ⋮ Exploring the long-term dynamics of perturbed Keplerian motion in high degree potential fields

Cites Work

• Unnamed Item
• Tesseral harmonic perturbations in radial transverse and binormal components
• Tesseral harmonic perturbations for high order and degree harmonics
• On the motion of a satellite in resonance with its rotating planet
• Canonical transformations depending on a small parameter
• Tesseral resonance effects on satellite orbits
• The main problem of artificial satellite theory for small and moderate eccentricities

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