Exoplanet orbital eccentricities derived from LAMOST–Kepler analysis

The nearly circular (mean eccentricity [Formula: see text]) and coplanar (mean mutual inclination [Formula: see text]) orbits of the solar system planets motivated Kant and Laplace to hypothesize that planets are formed in disks, which has developed into the widely accepted theory of planet formatio...

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Detalhes bibliográficos
Publicado no:Proc Natl Acad Sci U S A
Main Authors: Xie, Ji-Wei, Dong, Subo, Zhu, Zhaohuan, Huber, Daniel, Zheng, Zheng, De Cat, Peter, Fu, Jianning, Liu, Hui-Gen, Luo, Ali, Wu, Yue, Zhang, Haotong, Zhang, Hui, Zhou, Ji-Lin, Cao, Zihuang, Hou, Yonghui, Wang, Yuefei, Zhang, Yong
Formato: Artigo
Idioma:Inglês
Publicado em: National Academy of Sciences 2016
Assuntos:
Physical Sciences
Acesso em linha:https://ncbi.nlm.nih.gov/pmc/articles/PMC5068330/
https://ncbi.nlm.nih.gov/pubmed/27671635
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1073/pnas.1604692113
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