Resonance Capture for a Mercurian Orbiter in the Vicinity of Sun

In this work, the problem of resonance caused by some gravitational potentials due to Mercury and a third body, namely the Sun, together with some non-gravitational perturbations, specifically coronal mass ejections and solar wind in addition to radiation pressure, are investigated. Some simplifyi...

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Bibliographic Details
Main Authors: Elamira Hend Khattab, Fawzy Ahmed Abd El-Salam, Walid A. Rahoma
Format: Article
Language:English
Published: Korean Space Science Society (KSSS) 2021-06-01
Series:Journal of Astronomy and Space Sciences
Subjects:
Online Access:http://koreascience.or.kr/article/JAKO202118248968703.page
Description
Summary:In this work, the problem of resonance caused by some gravitational potentials due to Mercury and a third body, namely the Sun, together with some non-gravitational perturbations, specifically coronal mass ejections and solar wind in addition to radiation pressure, are investigated. Some simplifying assumptions without loss of accuracy are employed. The considered force model is constructed. Then the Delaunay canonical set is introduced. The Hamiltonian of the problem is obtained then it is expressed in terms of the Deluanay canonical set. The Hamiltonian is re-ordered to adopt it to the perturbation technique used to solve the problem. The Lie transform method is surveyed. The Hamiltonian is doubly averaged. The resonance capture is investigated. Finally, some numerical simulations are illustrated and are analyzed. Many resonant inclinations are revealed.
ISSN:2093-5587
2093-1409