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The orbital configuration of the two interacting Jupiters in HD 155358 system
Ma, Da-Zhu1,2,3; Fu, Yan-Ning1; Wang, Xiao-Li4
2017-08-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume470Issue:1Pages:706-712
Corresponding AuthorMa, Da-Zhu(madz@pmo.ac.cn) ; Fu, Yan-Ning(fyn@pmo.ac.cn) ; Wang, Xiao-Li(wangxl@ynao.ac.cn)
AbstractRecent observation reveals two interacting Jupiters possibly trapped in a 2: 1 mean motion resonance (MMR) around the star HD 155358. For the 2:1 MMR, Beauge et al. found that as long as the orbital decay was sufficiently slow, the trapped planets should also be in apsidal co-rotation. So it is very interesting to explore whether HD 155358 did undergo such an evolution and presents an apsidal co-rotation. Based on the existing results of spectroscopic orbital determination, the global dynamics of the system shows that the two planets are in an apsidal co-rotation if the eccentricity of the outer planet (ec) takes values very close to the lower limit of its 1 sigma confidence interval. This makes us conjecture that the globally minimizing solution could be missed in the previous orbital determination. Using an efficient global optimization method, we do find a better solution, reducing chi(2) from 1.4 to 1.2. This new solution is significantly different from the previous one, and in particular, with smaller ec. However, the increased possibility for the system to be trapped in a 2: 1 MMR with apsidal co-rotation is still not high. A set of simulations of the adiabatic convergent migration process are then performed. The results consistently indicate that the 2: 1 MMR forms before apsidal co-rotation. Finally, the long-term stability of the formed system and of its resonant structure is extensively explored, and the resulting statistics are given. A conclusion is that the 2: 1 MMR with apsidal co-rotation is a very stable structure.
Keywordmethods: numerical planetary systems
DOI10.1093/mnras/stx1230
WOS KeywordMEAN-MOTION RESONANCE ; LINED SPECTROSCOPIC BINARIES ; RADIAL-VELOCITY DATA ; PLANETARY SYSTEM ; EXTRASOLAR PLANETS ; GIANT PLANETS ; EVOLUTION ; MIGRATION ; ORIGIN ; DISC
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000406842600042
PublisherOXFORD UNIV PRESS
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Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/22611
Collection中国科学院紫金山天文台
Corresponding AuthorMa, Da-Zhu; Fu, Yan-Ning; Wang, Xiao-Li
Affiliation1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
3.Hubei Univ Nationalities, Sch Sci, Enshi 445000, Peoples R China
4.Chinese Acad Sci, Yunnan Observ, Kunming 650011, Yunnan, Peoples R China
Recommended Citation
GB/T 7714
Ma, Da-Zhu,Fu, Yan-Ning,Wang, Xiao-Li. The orbital configuration of the two interacting Jupiters in HD 155358 system[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,470(1):706-712.
APA Ma, Da-Zhu,Fu, Yan-Ning,&Wang, Xiao-Li.(2017).The orbital configuration of the two interacting Jupiters in HD 155358 system.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,470(1),706-712.
MLA Ma, Da-Zhu,et al."The orbital configuration of the two interacting Jupiters in HD 155358 system".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 470.1(2017):706-712.
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