Secular motion around synchronously orbiting planetary satellites
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Publication:3529591
DOI10.1063/1.2038547zbMath1144.37366OpenAlexW2045308397WikidataQ82189890 ScholiaQ82189890MaRDI QIDQ3529591
Martin Lara, Juan Félix San-Juan, Sebastián Ferrer
Publication date: 14 October 2008
Published in: Chaos: An Interdisciplinary Journal of Nonlinear Science (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1063/1.2038547
Related Items (4)
Mission design through averaging of perturbed Keplerian systems: the paradigm of an Enceladus orbiter ⋮ Hill problem analytical theory to the order four: application to the computation of frozen orbits around planetary satellites ⋮ Polynomial equations for science orbits around Europa ⋮ The bifurcation of periodic orbits and equilibrium points in the linked restricted three-body problem with parameter ω
Cites Work
- Frozen orbits for satellites close to an Earth-like planet
- The Keplerian regime of charged particles in planetary magnetospheres
- The critical inclination in artificial satellite theory
- The constrained normal form algorithm
- Canonical transformations depending on a small parameter
- A Hill problem with oblate primaries and effect of oblateness on Hill stability of orbits
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