期刊文献+

Forming different planetary systems 被引量:2

Forming different planetary systems
下载PDF
导出
摘要 With the increasing number of detected exoplanet samples, the statistical properties of planetary systems have become much clearer. In this review, we sum- marize the major statistical results that have been revealed mainly by radial velocity and transiting observations, and try to interpret them within the scope of the classical core-accretion scenario of planet formation, especially in the formation of different orbital architectures for planetary systems around main sequence stars. Based on the different possible formation routes for different planet systems, we tentatively classify them into three major catalogs: hot Jupiter systems, standard systems and distant giant planet systems. The standard systems can be further categorized into three sub-types under different circumstances: solar-like systems, hot Super-Earth systems, and sub- giant planet systems. We also review the theory of planet detection and formation in binary systems as well as planets in star clusters. With the increasing number of detected exoplanet samples, the statistical properties of planetary systems have become much clearer. In this review, we sum- marize the major statistical results that have been revealed mainly by radial velocity and transiting observations, and try to interpret them within the scope of the classical core-accretion scenario of planet formation, especially in the formation of different orbital architectures for planetary systems around main sequence stars. Based on the different possible formation routes for different planet systems, we tentatively classify them into three major catalogs: hot Jupiter systems, standard systems and distant giant planet systems. The standard systems can be further categorized into three sub-types under different circumstances: solar-like systems, hot Super-Earth systems, and sub- giant planet systems. We also review the theory of planet detection and formation in binary systems as well as planets in star clusters.
出处 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2012年第8期1081-1106,共26页 天文和天体物理学研究(英文版)
基金 supported by the National Natural Science Foundation of China (Nos. 10833001, 10925313, 11078001 and 11003010) Fundamental Research Funds for the Central Universities (No. 1112020102) the Research Fund for the Doctoral Program of Higher Education of China (Nos. 20090091110002 and 20090091120025)
关键词 planetary systems: dynamical evolution and stability -- formation --planet-disk interactions -- stars: binary: general -- clusters: general planetary systems: dynamical evolution and stability -- formation --planet-disk interactions -- stars: binary: general -- clusters: general
  • 相关文献

参考文献271

  • 1Aarseth, S. J., Lin, D. N. C., & Palmer, E L. 1993, ApJ, 403, 351.
  • 2Adams, E C. 2010, ARA&A, 48, 47.
  • 3Agol, E., Steffen, J., Sari, R., & Clarkson, W. 2005, MNRAS, 359, 567.
  • 4Armitage, E J. 2007, arXiv:astro-ph/0701485.
  • 5Artymowicz, P., & Lubow, S. H. 1994, ApJ, 421,651.
  • 6Backer, D. C., Foster, R. S., & Sallmen, S. 1993, Nature, 365, 817.
  • 7Barbieri, M., Marzari, E, & Scholl, H. 2002, A&A, 396, 219.
  • 8Batalha, N. M., Rowe, J. F., Bryson, S. T., et al. 2012, arXiv: 1202.5852.
  • 9Batygin, K., & Morbidelli, A. 2012, arXiv: 1204.2791.
  • 10Batygin, K., Morbidelli, A., & Tsiganis, K. 2011, A&A, 533, A7.

引证文献2

二级引证文献4

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部