{"title":"Analyzing the position and stability of the Lagrangian points under the gravitational effect of the Sun, Moon and the Earth including its oblateness","authors":"M. Kumar , S. Yadav , P.K. Behera","doi":"10.1016/j.ascom.2025.100966","DOIUrl":null,"url":null,"abstract":"<div><div>The present study explores the existence and stability of the Lagrangian points in the Earth–Moon–Sun system, consider the artificial satellite moving around the Earth under the gravitational attraction of the Sun, the Earth and the Moon. Equations of motion of the satellite are determined in spherical polar coordinate system with the help of potential of the Earth. The positions and stability of the Lagrangian points lie on the <span><math><mi>x</mi></math></span>-axis and <span><math><mi>y</mi></math></span>-axis are investigated including the effect of <span><math><msub><mrow><mi>J</mi></mrow><mrow><mn>2</mn></mrow></msub></math></span> (oblateness of the Earth), <span><math><mi>ν</mi></math></span> (orbital angle of the Moon around the bary-center), <span><math><mi>α</mi></math></span> (orbital angle of the bary-center system around the Sun) and <span><math><mi>θ</mi></math></span> (longitude of the satellite). Finally, the zero velocity curves are drawn by taking different values of Jacobi constant. It is observed that region of possible motion decreases on increasing the values of Jacobi constants</div></div>","PeriodicalId":48757,"journal":{"name":"Astronomy and Computing","volume":"52 ","pages":"Article 100966"},"PeriodicalIF":1.9000,"publicationDate":"2025-04-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomy and Computing","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S2213133725000393","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
The present study explores the existence and stability of the Lagrangian points in the Earth–Moon–Sun system, consider the artificial satellite moving around the Earth under the gravitational attraction of the Sun, the Earth and the Moon. Equations of motion of the satellite are determined in spherical polar coordinate system with the help of potential of the Earth. The positions and stability of the Lagrangian points lie on the -axis and -axis are investigated including the effect of (oblateness of the Earth), (orbital angle of the Moon around the bary-center), (orbital angle of the bary-center system around the Sun) and (longitude of the satellite). Finally, the zero velocity curves are drawn by taking different values of Jacobi constant. It is observed that region of possible motion decreases on increasing the values of Jacobi constants
Astronomy and ComputingASTRONOMY & ASTROPHYSICSCOMPUTER SCIENCE,-COMPUTER SCIENCE, INTERDISCIPLINARY APPLICATIONS
CiteScore
4.10
自引率
8.00%
发文量
67
期刊介绍:
Astronomy and Computing is a peer-reviewed journal that focuses on the broad area between astronomy, computer science and information technology. The journal aims to publish the work of scientists and (software) engineers in all aspects of astronomical computing, including the collection, analysis, reduction, visualisation, preservation and dissemination of data, and the development of astronomical software and simulations. The journal covers applications for academic computer science techniques to astronomy, as well as novel applications of information technologies within astronomy.