A perturbative treatment of the Yarkovsky-driven drifts in the 2:1 mean motion resonance

Pan Tan, Xi-Yun Hou
{"title":"A perturbative treatment of the Yarkovsky-driven drifts in the 2:1 mean motion resonance","authors":"Pan Tan, Xi-Yun Hou","doi":"10.1051/0004-6361/202449770","DOIUrl":null,"url":null,"abstract":"Our aim is to gain a qualitative understanding as well as to perform a quantitative analysis of the interplay between the Yarkovsky effect and the Jovian 2:1 mean motion resonance under the planar elliptic restricted three-body problem. We adopted the semi-analytical perturbation method valid for arbitrary eccentricity to obtain the resonance structures inside the Jovian 2:1 resonance. We averaged the Yarkovsky force so it could be applied to the integrable approximations for the 2:1 resonance and the $ secular resonance. The rates of Yarkovsky-driven drifts in the action space were derived from the quasi-integrable approximations perturbed by the averaged Yarkovsky force. Pseudo-proper elements of test particles inside the 2:1 resonance were computed using N-body simulations incorporated with the Yarkovsky effect to verify the semi-analytical results. In the planar elliptic restricted model, we identified two main types of systematic drifts in the action space: (Type I) for orbits not trapped in the $ resonance, the footprints are parallel to the resonance curve of the stable center of the 2:1 resonance; (Type II) for orbits trapped in the $ resonance, the footprints are parallel to the resonance curve of the stable center of the $ resonance. Using the semi-analytical perturbation method, a vector field in the action space corresponding to the two types of systematic drifts was derived. The Type I drift with small eccentricities and small libration amplitudes of 2:1 resonance can be modeled by a harmonic oscillator with a slowly varying parameter, for which an analytical treatment using the adiabatic invariant theory was carried out.","PeriodicalId":8585,"journal":{"name":"Astronomy & Astrophysics","volume":"38 5","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-07-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomy & Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1051/0004-6361/202449770","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0

Abstract

Our aim is to gain a qualitative understanding as well as to perform a quantitative analysis of the interplay between the Yarkovsky effect and the Jovian 2:1 mean motion resonance under the planar elliptic restricted three-body problem. We adopted the semi-analytical perturbation method valid for arbitrary eccentricity to obtain the resonance structures inside the Jovian 2:1 resonance. We averaged the Yarkovsky force so it could be applied to the integrable approximations for the 2:1 resonance and the $ secular resonance. The rates of Yarkovsky-driven drifts in the action space were derived from the quasi-integrable approximations perturbed by the averaged Yarkovsky force. Pseudo-proper elements of test particles inside the 2:1 resonance were computed using N-body simulations incorporated with the Yarkovsky effect to verify the semi-analytical results. In the planar elliptic restricted model, we identified two main types of systematic drifts in the action space: (Type I) for orbits not trapped in the $ resonance, the footprints are parallel to the resonance curve of the stable center of the 2:1 resonance; (Type II) for orbits trapped in the $ resonance, the footprints are parallel to the resonance curve of the stable center of the $ resonance. Using the semi-analytical perturbation method, a vector field in the action space corresponding to the two types of systematic drifts was derived. The Type I drift with small eccentricities and small libration amplitudes of 2:1 resonance can be modeled by a harmonic oscillator with a slowly varying parameter, for which an analytical treatment using the adiabatic invariant theory was carried out.
对 2:1 平均运动共振中雅科夫斯基驱动漂移的微扰处理
我们的目的是在平面椭圆受限三体问题下,对雅尔科夫斯基效应与约维亚 2:1 平均运动共振之间的相互作用进行定性理解和定量分析。我们采用了适用于任意偏心率的半解析扰动法,得到了约维天体2:1共振内部的共振结构。我们对Yarkovsky力进行了平均,从而将其应用于2:1共振和$世俗共振的可积分近似。亚尔科夫斯基驱动的漂移在作用空间中的速率是由平均亚尔科夫斯基力扰动的准积分近似推导出来的。为了验证半解析结果,我们使用结合了雅科夫斯基效应的 N-体模拟计算了 2:1 共振内测试粒子的伪精确元素。在平面椭圆受限模型中,我们发现了作用空间中的两种主要系统漂移类型:(第一类)未被困在$共振中的轨道,其足迹平行于2:1共振稳定中心的共振曲线;(第二类)被困在$共振中的轨道,其足迹平行于$共振稳定中心的共振曲线。利用半解析扰动法,得出了两类系统漂移对应的作用空间矢量场。2:1共振的小偏心率和小振幅的第一类漂移可以用一个参数缓慢变化的谐振子来模拟,并利用绝热不变量理论对其进行了分析处理。
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 求助全文
来源期刊
自引率
0.00%
发文量
0
×
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
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
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 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信