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Latitudinal variations of charged dust in co-orbital resonance with Jupiter

Published online by Cambridge University Press:  30 May 2022

Stefanie Reiter Open the ORCID record for Stefanie Reiter [Opens in a new window]  and
Christoph Lhotka Open the ORCID record for Christoph Lhotka [Opens in a new window]
Stefanie Reiter
Affiliation:
Department of Astrophysics, University of Vienna, Türkenschanzstrasse 17,1180 Vienna, Austria email: stefanie.reiter@univie.ac.at
Christoph Lhotka
Affiliation:
Department of Astrophysics, University of Vienna, Türkenschanzstrasse 17,1180 Vienna, Austria email: stefanie.reiter@univie.ac.at Department of Mathematics, University of Rome Tor Vergata, Via della Ricerca Scientifica 1, 00133 Rome, Italy email: lhotka@mat.uniroma2.it
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Abstract

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The interplanetary magnetic field may cause large amplitude changes in the orbital inclinations of charged dust particles. In order to study this effect in the case of dust grains moving in 1:1 mean motion resonance with planet Jupiter, a simplified semi-analytical model is developed to reduce the full dynamics of the system to the terms containing the information of the secular evolution dominated by the Lorentz force. It was found that while the planet causes variations in all orbital elements, the influence of the magnetic field most heavily impacts the long-term evolution of the inclination and the longitude of the ascending node. The simplified secular-resonant model recreates the oscillations in these parameters very well in comparison to the full solution, despite neglecting the influence of the magnetic field on the other orbital parameters.

Keywords

Dust dynamicsLagrange probleminterplanetary magnetic field
Type
Research Article
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S364: Multi-scale (Time and Mass) Dynamics of Space Objects (Oct 2021) , October 2019 , pp. 102 - 107
Copyright
© The Author(s), 2022. Published by Cambridge University Press on behalf of International Astronomical Union

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