An analytical theory for tesseral gravitational harmonics

DOI10.1023/A:1008345403145zbMath0963.70020OpenAlexW1627606612MaRDI QIDQ1593009

A. M. Segerman, Shannon L. Coffey

Publication date: 28 June 2001

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

Full work available at URL: https://doi.org/10.1023/a:1008345403145

zbMATH Keywords

geopotentialEarth's rotational perioditerative Lie transformation techniquesatellite's orbital periodtesseral harmonic perturbations

Mathematics Subject Classification ID

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

Related Items (8)

Closed-form perturbation theory in the restricted three-body problem without relegation ⋮ Exact Delaunay normalization of the perturbed Keplerian Hamiltonian with tesseral harmonics ⋮ Dynamics of a satellite orbiting a planet with an inhomogeneous gravitational field ⋮ Relegation-free closed-form perturbation theory and the domain of secular motions in the restricted three-body problem ⋮ Delaunay variables approach to the elimination of the perigee in artificial satellite theory ⋮ Analytic orbit theory with any arbitrary spherical harmonic as the dominant perturbation ⋮ Reducing inter-satellite drift of low Earth orbit constellations using short-periodic corrections ⋮ A First Order Automated Lie Transform

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