Effect of perturbed potential of heterogeneous triaxial rigid bodies of N layers on the stability of libration points in the R3BP

IF 1.9 4区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS New Astronomy Pub Date : 2024-02-03 DOI:10.1016/j.newast.2024.102202
Kumari Shalini , Pankaj Sharma , Kumari Ranjana
{"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 ,&nbsp;Pankaj Sharma ,&nbsp;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":null,"pages":null},"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 m3 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 m3 are derived. Our findings reveal the existence of five libration points denoted as Li (i=1,2,3,4,5) in the proposed model, with three being collinear and two being non-collinear. We observed that the collinear libration points Li(i=1,2,3) are unstable, whereas the non-collinear libration points L4,5 are conditionally stable for the mass parameter μ(0,μc), where μc=0.25681k11.31619k22.24318k36.10258k4.

查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
N层异质三轴刚体的扰动势能对R3BP中枰点稳定性的影响
在本文中,我们研究了受限三体问题中无穷小质量 m3 的运动,将两个基体均视为具有 N 层的异质三轴刚体。本文推导了所提模型的势和无穷小质量 m3 的运动方程。我们的研究结果表明,在所提出的模型中存在五个天平动点,用 Li(i=1,2,3,4,5)表示,其中三个为共线天平动点,两个为非共线天平动点。我们观察到,对于质量参数μ∈(0,μc),其中μc=0.25681k1-1.31619k2-2.24318k3-6.10258k4,共线枰点Li(i=1,2,3)是不稳定的,而非共线枰点L4,5是有条件稳定的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 去求助
来源期刊
New Astronomy
New Astronomy 地学天文-天文与天体物理
CiteScore
4.00
自引率
10.00%
发文量
109
审稿时长
13.6 weeks
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.
期刊最新文献
Slowly rotating charged Bardeen stellar structure Composition tracking for collisions between differentiated bodies in REBOUND NcorpiON : A O(N) software for N-body integration in collisional and fragmenting systems Study of solar activities associated with a Halo CME on 17 Feb 2023 event Discovery of 226 δ Scuti and γ Doradus Stars near NGC 6871 with TESS
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1