Searching for stable orbits in the HD 10180 planetary system
A planetary system with at least seven planets has been found around the star HD 10180. However, the traditional Keplerian and n-body fits to the data provide an orbital solution that becomes unstable very quickly, which may quest the reliability of the observations. Here we show that stable orbit...
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| Hauptverfasser: | , |
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| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
EDP Sciences
2011-02-01
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| Schriftenreihe: | EPJ Web of Conferences |
| Online-Zugang: | http://dx.doi.org/10.1051/epjconf/20101105001 |
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