Lunisolar apsidal resonances at low satellite orbits

DOI10.1023/A:1008379908163zbMath0956.70019OpenAlexW2148008340MaRDI QIDQ1976126

Sławomir Breiter

Publication date: 20 July 2000

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

Full work available at URL: https://doi.org/10.1023/a:1008379908163

zbMATH Keywords

artificial satellitessecular resonancesstable pointsluni-solar perturbationsEarth's potentialunstable pointsfamily of 10 resonancesHill-type approximationlibration widthsmaximum variation of eccentricityperigee heights' librationsecond-order zonal harmonic

Mathematics Subject Classification ID

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

Related Items (6)

The dynamical structure of the MEO region: long-term stability, chaos, and transport ⋮ Bifurcation of Lunisolar Secular Resonances for Space Debris Orbits ⋮ Resonant dynamics of medium Earth orbits: space debris issues ⋮ Unnamed Item ⋮ A frequency portrait of low Earth orbits ⋮ Phase space description of the dynamics due to the coupled effect of the planetary oblateness and the solar radiation pressure perturbations

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