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...
Main Authors: | , , |
---|---|
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 |
id |
doaj-54a5cdfab2304685a168952ee5fcd744 |
---|---|
record_format |
Article |
spelling |
doaj-54a5cdfab2304685a168952ee5fcd7442021-07-14T14:11:05ZengKorean Space Science Society (KSSS)Journal of Astronomy and Space Sciences2093-55872093-14092021-06-013829310310.5140/JASS.2021.38.2.93Resonance Capture for a Mercurian Orbiter in the Vicinity of SunElamira Hend Khattab0https://orcid.org/0000-0001-5109-7410Fawzy Ahmed Abd El-Salam1https://orcid.org/0000-0002-4107-9347Walid A. Rahoma2https://orcid.org/0000-0002-3529-2731Cairo University, Cairo 12613, EgyptCairo University, Cairo 12613, EgyptCairo University, Cairo 12613, EgyptIn 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.http://koreascience.or.kr/article/JAKO202118248968703.pageresonance capturemerecurian gravitythird body perturbations |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Elamira Hend Khattab Fawzy Ahmed Abd El-Salam Walid A. Rahoma |
spellingShingle |
Elamira Hend Khattab Fawzy Ahmed Abd El-Salam Walid A. Rahoma Resonance Capture for a Mercurian Orbiter in the Vicinity of Sun Journal of Astronomy and Space Sciences resonance capture merecurian gravity third body perturbations |
author_facet |
Elamira Hend Khattab Fawzy Ahmed Abd El-Salam Walid A. Rahoma |
author_sort |
Elamira Hend Khattab |
title |
Resonance Capture for a Mercurian Orbiter in the Vicinity of Sun |
title_short |
Resonance Capture for a Mercurian Orbiter in the Vicinity of Sun |
title_full |
Resonance Capture for a Mercurian Orbiter in the Vicinity of Sun |
title_fullStr |
Resonance Capture for a Mercurian Orbiter in the Vicinity of Sun |
title_full_unstemmed |
Resonance Capture for a Mercurian Orbiter in the Vicinity of Sun |
title_sort |
resonance capture for a mercurian orbiter in the vicinity of sun |
publisher |
Korean Space Science Society (KSSS) |
series |
Journal of Astronomy and Space Sciences |
issn |
2093-5587 2093-1409 |
publishDate |
2021-06-01 |
description |
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. |
topic |
resonance capture merecurian gravity third body perturbations |
url |
http://koreascience.or.kr/article/JAKO202118248968703.page |
work_keys_str_mv |
AT elamirahendkhattab resonancecaptureforamercurianorbiterinthevicinityofsun AT fawzyahmedabdelsalam resonancecaptureforamercurianorbiterinthevicinityofsun AT walidarahoma resonancecaptureforamercurianorbiterinthevicinityofsun |
_version_ |
1721302559923109888 |