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On the retrograde planar co-orbital asteroid motion with Jupiter
Published online by Cambridge University Press: 16 October 2024
Abstract
We study the motion of an asteroid being in retrograde 1/1 resonance with Jupiter (co-orbital motion). We consider the planar case (i=180°) and Jupiter is on a circular or elliptic orbit (e′ = 0.048). In the cirular model we compute families of symmetric periodic orbits and their stability type. In the elliptic model we have isolated periodic orbits which affect the orbital modes of motion as it is shown by the FLI dynamical maps.
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- © The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union