PMO OpenIR  > 近地天体探测和太阳系天体研究团组
Forming short-period earth-like planets via a collision-merger scenario
Jin, Sheng ; Ji, Jianghui ; Tinney, Chris G.
2011
Source PublicationThe Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution, Proceedings of the International Astronomical Union, IAU Symposium,
Volume276Pages:432-433
AbstractWe present a new formation mechanism to produce short-period Earth-like planets in the late stage of planet formation, through a collision-merger scenario. In this scenario, a planetary embryo is directly thrown into a close-in orbit after a collision with another embryo, and then the larger merged body is seized by the central star as a hot Earth-like planet.
KeywordMethods: N-body Simulations, Celestial Mechanics, Planetary Systems: Formation
Subject AreaAstronomy & Astrophysics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/4421
Collection近地天体探测和太阳系天体研究团组
Recommended Citation
GB/T 7714
Jin, Sheng,Ji, Jianghui,Tinney, Chris G.. Forming short-period earth-like planets via a collision-merger scenario[J]. The Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution, Proceedings of the International Astronomical Union, IAU Symposium,,2011,276:432-433.
APA Jin, Sheng,Ji, Jianghui,&Tinney, Chris G..(2011).Forming short-period earth-like planets via a collision-merger scenario.The Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution, Proceedings of the International Astronomical Union, IAU Symposium,,276,432-433.
MLA Jin, Sheng,et al."Forming short-period earth-like planets via a collision-merger scenario".The Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution, Proceedings of the International Astronomical Union, IAU Symposium, 276(2011):432-433.
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