Earth-Moon weak stability boundaries in the restricted three- and four-body problem

DOI10.1007/S10569-008-9169-YzbMath1167.70006OpenAlexW2078315712MaRDI QIDQ1011855

Christian Circi, Daniele Romagnoli

Publication date: 14 April 2009

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

Full work available at URL: https://doi.org/10.1007/s10569-008-9169-y

zbMATH Keywords

lunar captureescape trajectorieslow-energy transfer

Mathematics Subject Classification ID

Three-body problems (70F07) Stability for nonlinear problems in mechanics (70K20) Celestial mechanics (70F15) Orbital mechanics (70M20) (n)-body problems (70F10)

Related Items (8)

Analytic estimates and topological properties of the weak stability boundary ⋮ Constructing ballistic capture orbits in the real solar system model. ⋮ Energy analysis of the single impulsive Earth-Moon transfer with the temporary lunar capture ⋮ Computation of weak stability boundaries: Sun-Jupiter system ⋮ Indirect transfer to the Earth-Eoon L1 libration point ⋮ Stable and unstable orbits around Mercury ⋮ Connection between Hill stability and weak stability in the elliptic restricted three-body problem ⋮ A flow-informed strategy for ballistic capture orbit generation

Cites Work

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• A note on weak stability boundaries
• Sun-perturbed Earth-to-Moon transfers with low energy and moderate flight time
• Heteroclinic connections between periodic orbits and resonance transitions in celestial mechanics
• BURRAU'S PROBLEM OF THREE BODIES
• On the dynamics of weak stability boundary lunar transfers
• Low energy transfer to the Moon

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