Two Periodic Models for the Earth-Moon System

This paper discusses two alternative models to the Restricted Three Body Problem (RTBP) for the motion of a massless particle in the Earth-Moon system. These models are the Bicircular Problem (BCP) and the Quasi-Bicircular Problem (QBCP). While the RTBP is autonomous, the BCP and the QBCP are period...

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Main Authors: Marc Jorba-Cuscó, Ariadna Farrés, Àngel Jorba
Format: Article
Language:English
Published: Frontiers Media S.A. 2018-07-01
Series:Frontiers in Applied Mathematics and Statistics
Subjects:
Online Access:https://www.frontiersin.org/article/10.3389/fams.2018.00032/full
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author Marc Jorba-Cuscó
Ariadna Farrés
Àngel Jorba
author_facet Marc Jorba-Cuscó
Ariadna Farrés
Àngel Jorba
author_sort Marc Jorba-Cuscó
collection DOAJ
description This paper discusses two alternative models to the Restricted Three Body Problem (RTBP) for the motion of a massless particle in the Earth-Moon system. These models are the Bicircular Problem (BCP) and the Quasi-Bicircular Problem (QBCP). While the RTBP is autonomous, the BCP and the QBCP are periodically time dependent due to the inclusion of the Sun's gravitational potential. Each of the two alternative models is suitable for certain regions of the phase space. More concretely, we show that the BCP is more adequate to study the dynamics near the triangular points while the QBCP is more adequate for the dynamics near the collinear points.
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spelling doaj.art-968eecc64b10482eb27442634ea19d752022-12-21T19:54:16ZengFrontiers Media S.A.Frontiers in Applied Mathematics and Statistics2297-46872018-07-01410.3389/fams.2018.00032392773Two Periodic Models for the Earth-Moon SystemMarc Jorba-Cuscó0Ariadna Farrés1Àngel Jorba2Departament de Matemàtiques i Informàtica, Universitat de Barcelona, Barcelona, SpainGoddard Planetary Heliophysics Institute, University of Maryland Baltimore Country, Baltimore, MD, United StatesDepartament de Matemàtiques i Informàtica, Universitat de Barcelona, Barcelona, SpainThis paper discusses two alternative models to the Restricted Three Body Problem (RTBP) for the motion of a massless particle in the Earth-Moon system. These models are the Bicircular Problem (BCP) and the Quasi-Bicircular Problem (QBCP). While the RTBP is autonomous, the BCP and the QBCP are periodically time dependent due to the inclusion of the Sun's gravitational potential. Each of the two alternative models is suitable for certain regions of the phase space. More concretely, we show that the BCP is more adequate to study the dynamics near the triangular points while the QBCP is more adequate for the dynamics near the collinear points.https://www.frontiersin.org/article/10.3389/fams.2018.00032/fullRestricted Three Body ProblemBicircular ProblemQuasi-Bicircular Problemperiodic hamiltonianstroboscopic mapinvariant manifolds
spellingShingle Marc Jorba-Cuscó
Ariadna Farrés
Àngel Jorba
Two Periodic Models for the Earth-Moon System
Frontiers in Applied Mathematics and Statistics
Restricted Three Body Problem
Bicircular Problem
Quasi-Bicircular Problem
periodic hamiltonian
stroboscopic map
invariant manifolds
title Two Periodic Models for the Earth-Moon System
title_full Two Periodic Models for the Earth-Moon System
title_fullStr Two Periodic Models for the Earth-Moon System
title_full_unstemmed Two Periodic Models for the Earth-Moon System
title_short Two Periodic Models for the Earth-Moon System
title_sort two periodic models for the earth moon system
topic Restricted Three Body Problem
Bicircular Problem
Quasi-Bicircular Problem
periodic hamiltonian
stroboscopic map
invariant manifolds
url https://www.frontiersin.org/article/10.3389/fams.2018.00032/full
work_keys_str_mv AT marcjorbacusco twoperiodicmodelsfortheearthmoonsystem
AT ariadnafarres twoperiodicmodelsfortheearthmoonsystem
AT angeljorba twoperiodicmodelsfortheearthmoonsystem