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(Reference retrieved automatically from Web of Science through information on FAPESP grant and its corresponding number as mentioned in the publication by the authors.)

Coorbital capture at arbitrary inclination

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Namouni, Fathi [1] ; Morais, Helena [2]
Total Authors: 2
[1] Univ Cote Azur, CNRS, Observ Cote Azur, CS 34229, F-06304 Nice - France
[2] Univ Estadual Paulista UNESP, Inst Geociencias & Ciencias Exatas, Ave 24-A, 1515, BR-13506900 Rio Claro, SP - Brazil
Total Affiliations: 2
Document type: Journal article
Source: COMPUTATIONAL & APPLIED MATHEMATICS; v. 37, n. 1, SI, p. 65-71, DEC 2018.
Web of Science Citations: 3

The process of capture in the coorbital region of a solar system planet is studied. Absolute capture likelihood in the 1:1 resonance is determined by randomly constructed statistical ensembles numbering 7.24x105 of massless asteroids that are set to migrate radially from the outer to the inner boundaries of the coorbital region of a Jupiter-mass planet. Orbital states include coorbital capture, ejection, collisions with the Sun and the planet and free-crossing of the coorbital region. The relative efficiency of retrograde capture with respect to prograde capture is confirmed as an intrinsic property of the coorbital resonance. Half the asteroids cross the coorbital region regardless of eccentricity and for any inclination less than 120 degrees. We also find that the recently discovered retrograde coorbital of Jupiter, asteroid 2015 BZ509, lies almost exactly at the capture efficiency peak associated with its orbital parameters. (AU)

FAPESP's process: 15/17962-5 - Topics of orbital dynamics and machine learning tools applied to planetary systems data
Grantee:Maria Helena Moreira Morais
Support type: Regular Research Grants