Basins of Convergence in a Multi-Perturbed CR3BP

The circular restricted three-body problem (CR3BP) is analyzed to introduce additional factors into the dynamic model, such as radiation forces, flattening of the primary bodies, relativity effects, and the presence of natural satellites. The introduction of these factors increases the accuracy when...

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Main Authors: Alicia Herrero, Santiago Moll-Lopez, José-A. Moraño, Erika Vega-Fleitas, Daniel Villalibre
Format: Article
Language:English
Published: MDPI AG 2024-12-01
Series:Applied Sciences
Subjects:
Online Access:https://www.mdpi.com/2076-3417/15/1/106
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author Alicia Herrero
Santiago Moll-Lopez
José-A. Moraño
Erika Vega-Fleitas
Daniel Villalibre
author_facet Alicia Herrero
Santiago Moll-Lopez
José-A. Moraño
Erika Vega-Fleitas
Daniel Villalibre
author_sort Alicia Herrero
collection DOAJ
description The circular restricted three-body problem (CR3BP) is analyzed to introduce additional factors into the dynamic model, such as radiation forces, flattening of the primary bodies, relativity effects, and the presence of natural satellites. The introduction of these factors increases the accuracy when obtaining the position of the Lagrange points and the basins of convergence of the system. The Newton–Raphson methodis used to implement a searching algorithm. Finally, an application to the Sun–Mars system including the presence of Phobos and Deimos is developed.
format Article
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institution Kabale University
issn 2076-3417
language English
publishDate 2024-12-01
publisher MDPI AG
record_format Article
series Applied Sciences
spelling doaj-art-8b10c51428eb40d7be5147de316ca5a92025-01-10T13:14:27ZengMDPI AGApplied Sciences2076-34172024-12-0115110610.3390/app15010106Basins of Convergence in a Multi-Perturbed CR3BPAlicia Herrero0Santiago Moll-Lopez1José-A. Moraño2Erika Vega-Fleitas3Daniel Villalibre4Instituto de Matemática Multidisciplinar, Universitat Politècnica de València, 46022 Valencia, SpainDepartamento de Matemática Aplicada, Universitat Politècnica de València, 46022 Valencia, SpainInstituto de Matemática Multidisciplinar, Universitat Politècnica de València, 46022 Valencia, SpainInstituto de Diseño y Fabricación, Universitat Politècnica de València, 46022 Valencia, SpainDepartamento de Matemática Aplicada, Universitat Politècnica de València, 46022 Valencia, SpainThe circular restricted three-body problem (CR3BP) is analyzed to introduce additional factors into the dynamic model, such as radiation forces, flattening of the primary bodies, relativity effects, and the presence of natural satellites. The introduction of these factors increases the accuracy when obtaining the position of the Lagrange points and the basins of convergence of the system. The Newton–Raphson methodis used to implement a searching algorithm. Finally, an application to the Sun–Mars system including the presence of Phobos and Deimos is developed.https://www.mdpi.com/2076-3417/15/1/106modified circular restricted three-body problemLagrange pointsbasins of convergenceNewton–Raphson methodradiation effectsrelativistic effects
spellingShingle Alicia Herrero
Santiago Moll-Lopez
José-A. Moraño
Erika Vega-Fleitas
Daniel Villalibre
Basins of Convergence in a Multi-Perturbed CR3BP
Applied Sciences
modified circular restricted three-body problem
Lagrange points
basins of convergence
Newton–Raphson method
radiation effects
relativistic effects
title Basins of Convergence in a Multi-Perturbed CR3BP
title_full Basins of Convergence in a Multi-Perturbed CR3BP
title_fullStr Basins of Convergence in a Multi-Perturbed CR3BP
title_full_unstemmed Basins of Convergence in a Multi-Perturbed CR3BP
title_short Basins of Convergence in a Multi-Perturbed CR3BP
title_sort basins of convergence in a multi perturbed cr3bp
topic modified circular restricted three-body problem
Lagrange points
basins of convergence
Newton–Raphson method
radiation effects
relativistic effects
url https://www.mdpi.com/2076-3417/15/1/106
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