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Orbital resonances in configurations with arbitrary relative inclination

Abstract

The existence of asteroids like the coorbital 2015BZ509 and the transneptunians Niku and Drac whose orbits have high relative inclination with respect to the planets' orbital plane is problematic in the context of the current theories for formation and evolution of the solar system. The recent modelling and subsequent identification of orbital resonances with the giant planets was essencial to the understanding of these configurations. We propose the continuation of the dynamical modelling of resonant orbital configurations in 3 dimensions, as well as the study of the dynamical evolution of retrograde and polar orbits, and the possible capture mechanisms in these configurations. (AU)

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Scientific publications
(References retrieved automatically from Web of Science and SciELO through information on FAPESP grants and their corresponding numbers as mentioned in the publications by the authors)
NAMOUNI, F.; MORAIS, M. H. M. An interstellar origin for high-inclination Centaurs. Monthly Notices of the Royal Astronomical Society, v. 494, n. 2, p. 2191-2199, MAY 2020. Web of Science Citations: 0.
NAMOUNI, E.; MORAIS, M. H. M. Resonance libration and width at arbitrary inclination. Monthly Notices of the Royal Astronomical Society, v. 493, n. 2, p. 2854-2871, APR 2020. Web of Science Citations: 0.
MORAIS, M. H. M.; NAMOUNI, F. Periodic orbits of the retrograde coorbital problem. Monthly Notices of the Royal Astronomical Society, v. 490, n. 3, p. 3799-3805, DEC 2019. Web of Science Citations: 0.

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