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Terrestrial planet formation in inclined systems application to the OGLE-2006-BLG-109L system
Sheng Jin ; Jianghui Ji
2011
Source PublicationMonthly Notices of the Royal Astronomical Society
Volume418Issue:2Pages:1335-1345
AbstractIn this paper, we carry out an extensive investigation of terrestrial planetary formation in inclined planetary systems at the late stage. We consider the OGLE-2006-BLG-109L system as a prototype. In the simulations, we show that the occurrence of terrestrial planets is common, in the final assembly stage. Moreover, we find that 40 per cent of the runs finally have one planet occupying the habitable zone. However, the numerical results also indicate that the inner region of the planetesimal disc, which ranges from ∼0.1 to 0.3 au, plays an important role in the development of terrestrial planets. By examining all the simulations, we note that the survivals are located either between 0.1 and 1.0 au or beyond 7 au, or at the 1 : 1 mean-motion resonance of OGLE-2006-BLG-109Lb at ∼2.20 au. These outcomes suggest that there might be a moderate possibility for inclined systems to harbour terrestrial planets, even planets in the habitable zone.
KeywordPlanets Satellites Formation Stars Individual Ogle-2006-blg-109l
Subject AreaAstronomy & Astrophysics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/4424
Collection行星科学与深空探测实验室
Recommended Citation
GB/T 7714
Sheng Jin,Jianghui Ji. Terrestrial planet formation in inclined systems application to the OGLE-2006-BLG-109L system[J]. Monthly Notices of the Royal Astronomical Society,2011,418(2):1335-1345.
APA Sheng Jin,&Jianghui Ji.(2011).Terrestrial planet formation in inclined systems application to the OGLE-2006-BLG-109L system.Monthly Notices of the Royal Astronomical Society,418(2),1335-1345.
MLA Sheng Jin,et al."Terrestrial planet formation in inclined systems application to the OGLE-2006-BLG-109L system".Monthly Notices of the Royal Astronomical Society 418.2(2011):1335-1345.
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