Xiaoyu Fu, Stefania Soldini, Hitoshi Ikeda, Daniel J. Scheeres, Yuichi Tsuda
{"title":"The dynamics about asteroid (162173) Ryugu","authors":"Xiaoyu Fu, Stefania Soldini, Hitoshi Ikeda, Daniel J. Scheeres, Yuichi Tsuda","doi":"10.1007/s10569-024-10199-y","DOIUrl":null,"url":null,"abstract":"<p>The dynamical environment around the asteroid (162173) Ryugu is analyzed in detail using a constant-density polyhedron model based on the measurements from the Hayabusa2 mission. Six exterior equilibrium points (EPs) are identified along the ridge line of Ryugu, and their topological classifications fall into two distinctive categories. The initial periodic orbit (PO) families are computed and analyzed, including distant retrograde/prograde orbit (DRO/DPO) families and fifteen PO families emanating from the exterior EPs. The fifteen PO families are further divided into three categories: seven converge to an EP, seven reach Ryugu’s surface, and one exhibits cyclic behavior during its progression. The existence of initial PO families converging to an EP is analyzed using the bifurcation of a degenerate EP. Connection between these families and similar ones in the circular restricted three-body problem (CRTBP) is also examined. Bifurcated PO families are identified and computed from the initial PO families, including ten families from the DROs, fifteen from the DPOs, and twenty-five associated with the EPs. The bifurcated families are separately analyzed and categorized in terms of their corresponding initial families. Connections established by the same bifurcation points between different bifurcated families are identified. A comparison is made for the dynamical environments of Ryugu and Bennu to evaluate the similarities and differences in the evolution of EPs and the progression of PO families in top-shaped asteroids.</p>","PeriodicalId":72537,"journal":{"name":"Celestial mechanics and dynamical astronomy","volume":"27 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-07-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Celestial mechanics and dynamical astronomy","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1007/s10569-024-10199-y","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
The dynamical environment around the asteroid (162173) Ryugu is analyzed in detail using a constant-density polyhedron model based on the measurements from the Hayabusa2 mission. Six exterior equilibrium points (EPs) are identified along the ridge line of Ryugu, and their topological classifications fall into two distinctive categories. The initial periodic orbit (PO) families are computed and analyzed, including distant retrograde/prograde orbit (DRO/DPO) families and fifteen PO families emanating from the exterior EPs. The fifteen PO families are further divided into three categories: seven converge to an EP, seven reach Ryugu’s surface, and one exhibits cyclic behavior during its progression. The existence of initial PO families converging to an EP is analyzed using the bifurcation of a degenerate EP. Connection between these families and similar ones in the circular restricted three-body problem (CRTBP) is also examined. Bifurcated PO families are identified and computed from the initial PO families, including ten families from the DROs, fifteen from the DPOs, and twenty-five associated with the EPs. The bifurcated families are separately analyzed and categorized in terms of their corresponding initial families. Connections established by the same bifurcation points between different bifurcated families are identified. A comparison is made for the dynamical environments of Ryugu and Bennu to evaluate the similarities and differences in the evolution of EPs and the progression of PO families in top-shaped asteroids.
根据隼鸟2号任务的测量结果,利用恒定密度多面体模型详细分析了小行星(162173)龙宫周围的动力学环境。沿龙宫的脊线确定了六个外部平衡点(EP),其拓扑分类可分为两个不同的类别。计算并分析了初始周期轨道(PO)族,包括遥远逆行/顺行轨道(DRO/DPO)族和源自外部平衡点的15个PO族。这15个PO族进一步分为三类:7个汇聚到一个EP,7个到达龙宫表面,1个在前进过程中表现出循环行为。利用退化 EP 的分岔分析了收敛到 EP 的初始 PO 族的存在。此外,还研究了这些族与圆形受限三体问题(CRTBP)中类似族之间的联系。从初始 PO 族中识别并计算出分叉 PO 族,包括来自 DRO 的 10 个族、来自 DPO 的 15 个族以及与 EP 相关的 25 个族。分叉族根据其对应的初始族分别进行分析和分类。确定了不同分岔族之间由相同分岔点建立的联系。对龙宫和贝努的动力学环境进行了比较,以评估顶形小行星中 EPs 演化和 PO 族进展的异同。