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Jovian encounter manifolds

Published online by Cambridge University Press:  16 October 2024

Nataša Todorović Open the ORCID record for Nataša Todorović [Opens in a new window]  and
Nikola Knežević
Nataša Todorović*
Affiliation:
Belgrade Astronomical Observatory, Volgina 7, 11000 Belgrade, Serbia
Nikola Knežević
Affiliation:
Belgrade Astronomical Observatory, Volgina 7, 11000 Belgrade, Serbia
*
email: ntodorovic@aob.rs
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Abstract

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Recent numerical studies have shown that the entire solar system is permeated with arch-like structures originating from all planets. Particles placed on such arches experience planetary close encounters after only one or few orbital revolutions. In this work, we are interested how thece arches, which we associate to encounter manifolds of Jupiter, appear in three dimensions for higher inclinations.

Our results show that about 0.5% of the observed domain [a, e, i] = [2 AU, 11.5 AU] × [0, 0.7] × [0°, 90°] is covered by the manifolds. For inclinations up to ∼5°, the arch-like structures are almost unchanged compared to those initially observed in the orbital plane of Jupiter. At higher inclinations, the number of encounter orbits rapidly decreases to narrow domains where the manifolds stretch up to inclinations of 90° (and above) in a very steep manner.

Keywords

manifoldsJupiterencounterschaos
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S382: Complex Planetary Systems II: Latest Methods for an Interdisciplinary Approach , December 2022 , pp. 180 - 184
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Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

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