Collinear Earth-Moon libration points have emerged as locations with immediate applications. These libration point orbits are inherently unstable and must be maintained regularly which constrains operations and maneuver locations. Stationkeeping is challenging due to relatively short time scales for divergence effects of large orbital eccentricity of the secondary body, and third-body perturbations. Using the Acceleration Reconnection and Turbulence and Electrodynamics of the Moon's Interaction with the Sun (ARTEMIS) mission orbit as a platform, the fundamental behavior of the trajectories is explored using Poincare maps in the circular restricted three-body problem. Operational stationkeeping results obtained using the Optimal Continuation Strategy are presented and compared to orbit stability information generated from mode analysis based in dynamical systems theory.
Earth-Moon Libration Point Orbit Stationkeeping: Theory, Modeling and Operations
Acta Astronautica ; 94 , 1
2013-02-08
Miscellaneous
No indication
English
Earth–Moon libration point orbit stationkeeping: Theory, modeling, and operations
Online Contents | 2014
|British Library Conference Proceedings | 2012
|