Searching for stable orbits in the HD 10180 planetary system

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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Main Authors: Laskar J., Correia A.C.M.
Format: Article
Language:English
Published: EDP Sciences 2011-02-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20101105001
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spelling doaj-17ad27adc8aa4ecfa3b8f367d2bcc8192021-08-02T05:10:13ZengEDP SciencesEPJ Web of Conferences2100-014X2011-02-01110500110.1051/epjconf/20101105001Searching for stable orbits in the HD 10180 planetary systemLaskar J.Correia A.C.M.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 orbital configurations can be obtained if general relativity and long-term dissipation raised by tides on the innermost planet are taken into account. http://dx.doi.org/10.1051/epjconf/20101105001
collection DOAJ
language English
format Article
sources DOAJ
author Laskar J.
Correia A.C.M.
spellingShingle Laskar J.
Correia A.C.M.
Searching for stable orbits in the HD 10180 planetary system
EPJ Web of Conferences
author_facet Laskar J.
Correia A.C.M.
author_sort Laskar J.
title Searching for stable orbits in the HD 10180 planetary system
title_short Searching for stable orbits in the HD 10180 planetary system
title_full Searching for stable orbits in the HD 10180 planetary system
title_fullStr Searching for stable orbits in the HD 10180 planetary system
title_full_unstemmed Searching for stable orbits in the HD 10180 planetary system
title_sort searching for stable orbits in the hd 10180 planetary system
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2011-02-01
description 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 orbital configurations can be obtained if general relativity and long-term dissipation raised by tides on the innermost planet are taken into account.
url http://dx.doi.org/10.1051/epjconf/20101105001
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AT correiaacm searchingforstableorbitsinthehd10180planetarysystem
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