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The dynamical architecture and habitable zones of the planetary system 55 Cancri

Published online by Cambridge University Press:  21 October 2010

Jianghui Ji ,
Hiroshi Kinoshita ,
Lin Liu  and
Guangyu Li
Jianghui Ji
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China email: jijh@pmo.ac.cn National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Hiroshi Kinoshita
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo 181-8588, Japan
Lin Liu
Affiliation:
Department of Astronomy, Nanjing University, Nanjing 210093, China
Guangyu Li
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China email: jijh@pmo.ac.cn National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
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Abstract

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We performed numerical simulations to study the secular orbital evolution and dynamical structure of the quintuplet planetary system 55 Cancri using the self-consistent orbital solutions of Fischer et al. (2008).

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 704
Copyright
Copyright © International Astronomical Union 2010

References

Fischer, D. A., Marcy, G. W., Butler, R. P. et al. 2008, ApJ 675, 790CrossRefGoogle Scholar
Ji, J., Kinoshita, H., Liu, L., & Li, G. 2009, Res. Astron. & Astrophys. 9, 703CrossRefGoogle Scholar