{"title":"Effect of perturbed potential of heterogeneous triaxial rigid bodies of N layers on the stability of libration points in the R3BP","authors":"Kumari Shalini , Pankaj Sharma , Kumari Ranjana","doi":"10.1016/j.newast.2024.102202","DOIUrl":null,"url":null,"abstract":"<div><p>In this paper, we investigate the motion of an infinitesimal mass <span><math><msub><mrow><mi>m</mi></mrow><mrow><mn>3</mn></mrow></msub></math></span> in the restricted three-body problem by taking both the primaries as heterogeneous triaxial rigid bodies with <em>N</em> layers. The potential of the proposed model and the equations of motion for the infinitesimal mass <span><math><msub><mrow><mi>m</mi></mrow><mrow><mn>3</mn></mrow></msub></math></span> are derived. Our findings reveal the existence of five libration points denoted as <span><math><msub><mrow><mi>L</mi></mrow><mrow><mi>i</mi></mrow></msub></math></span> <span><math><mrow><mo>(</mo><mi>i</mi><mo>=</mo><mn>1</mn><mo>,</mo><mn>2</mn><mo>,</mo><mn>3</mn><mo>,</mo><mn>4</mn><mo>,</mo><mn>5</mn><mo>)</mo></mrow></math></span> in the proposed model, with three being collinear and two being non-collinear. We observed that the collinear libration points <span><math><mrow><msub><mrow><mi>L</mi></mrow><mrow><mi>i</mi></mrow></msub><mrow><mo>(</mo><mi>i</mi><mo>=</mo><mn>1</mn><mo>,</mo><mn>2</mn><mo>,</mo><mn>3</mn><mo>)</mo></mrow></mrow></math></span> are unstable, whereas the non-collinear libration points <span><math><msub><mrow><mi>L</mi></mrow><mrow><mn>4</mn><mo>,</mo><mn>5</mn></mrow></msub></math></span> are conditionally stable for the mass parameter <span><math><mrow><mi>μ</mi><mo>∈</mo><mrow><mo>(</mo><mn>0</mn><mo>,</mo><msub><mrow><mi>μ</mi></mrow><mrow><mi>c</mi></mrow></msub><mo>)</mo></mrow></mrow></math></span>, where <span><math><mrow><msub><mrow><mi>μ</mi></mrow><mrow><mi>c</mi></mrow></msub><mo>=</mo><mn>0</mn><mo>.</mo><mn>25681</mn><mspace></mspace><msub><mrow><mi>k</mi></mrow><mrow><mn>1</mn></mrow></msub><mo>−</mo><mn>1</mn><mo>.</mo><mn>31619</mn><mspace></mspace><msub><mrow><mi>k</mi></mrow><mrow><mn>2</mn></mrow></msub><mo>−</mo><mn>2</mn><mo>.</mo><mn>24318</mn><mspace></mspace><msub><mrow><mi>k</mi></mrow><mrow><mn>3</mn></mrow></msub><mo>−</mo><mn>6</mn><mo>.</mo><mn>10258</mn><mspace></mspace><msub><mrow><mi>k</mi></mrow><mrow><mn>4</mn></mrow></msub></mrow></math></span>.</p></div>","PeriodicalId":54727,"journal":{"name":"New Astronomy","volume":"109 ","pages":"Article 102202"},"PeriodicalIF":1.9000,"publicationDate":"2024-02-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"New Astronomy","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S1384107624000162","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
In this paper, we investigate the motion of an infinitesimal mass in the restricted three-body problem by taking both the primaries as heterogeneous triaxial rigid bodies with N layers. The potential of the proposed model and the equations of motion for the infinitesimal mass are derived. Our findings reveal the existence of five libration points denoted as in the proposed model, with three being collinear and two being non-collinear. We observed that the collinear libration points are unstable, whereas the non-collinear libration points are conditionally stable for the mass parameter , where .
期刊介绍:
New Astronomy publishes articles in all fields of astronomy and astrophysics, with a particular focus on computational astronomy: mathematical and astronomy techniques and methodology, simulations, modelling and numerical results and computational techniques in instrumentation.
New Astronomy includes full length research articles and review articles. The journal covers solar, stellar, galactic and extragalactic astronomy and astrophysics. It reports on original research in all wavelength bands, ranging from radio to gamma-ray.