Abstract
Local toroidal coordinate systems are introduced to characterize relative motion near a periodic orbit with an oscillatory mode in the circular restricted three-body problem. These coordinate systems are derived from a first-order approximation of invariant tori relative to a periodic orbit and supply a geometric interpretation that is consistent across distinct periodic orbits. First, the local toroidal coordinate sets are used to rapidly generate first-order approximations of quasi-periodic relative motion. Then, geometric properties of these first-order approximations are used to predict the minimum and maximum separation distances between a spacecraft following quasi-periodic motion relative to another spacecraft located on a periodic orbit. Implementation of the local toroidal coordinate systems and associated geometric analyses is demonstrated in the context of spacecraft formations operating near members of the Earth–Moon \(L_2\) southern halo orbit family.
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Acknowledgements
This work was supported by a Graduate Assistance in Areas of National Need fellowship from the Smead Department of Aerospace Engineering Sciences at the University of Colorado Boulder. An earlier version of this work was presented as AAS 20-620 at the AAS/AIAA Astrodynamics Specialist Virtual Conference in August 2020. The authors also wish to thank each of the reviewers for their feedback.
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This work was supported by a Graduate Assistance in Areas of National Need fellowship from the Smead Department of Aerospace Engineering Sciences at the University of Colorado Boulder.
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Elliott, I., Bosanac, N. Describing relative motion near periodic orbits via local toroidal coordinates. Celest Mech Dyn Astr 134, 19 (2022). https://doi.org/10.1007/s10569-022-10074-8
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DOI: https://doi.org/10.1007/s10569-022-10074-8