Abstract
Stable or weakly unstable orbits in cislunar space are attractive as potential locations that natural objects including dust particles may be trapped. Identifying such orbits is not straightforward especially in high-dimensional, many-body dynamical systems. The present paper adopts a strategy of limiting the search space around symmetric periodic orbits in the Earth–Moon spatial circular restricted three-body problem. We find a variety of linearly stable or weakly unstable periodic orbits near the \(1:1\) retrograde resonance with the Moon. Characteristics of the periodic orbits are explored and their stabilities under solar gravitational perturbations are assessed to understand representative behaviours of retrograde co-orbital orbits around the Earth.
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This study has been partially supported by JSPS Grants-in-Aid No. 20K14951.
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Oshima, K. 3D stable and weakly unstable periodic orbits around the Earth near the retrograde co-orbital resonance with the Moon. Astrophys Space Sci 367, 42 (2022). https://doi.org/10.1007/s10509-022-04071-4
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DOI: https://doi.org/10.1007/s10509-022-04071-4