{ "id": "1402.2728", "version": "v1", "published": "2014-02-12T04:32:40.000Z", "updated": "2014-02-12T04:32:40.000Z", "title": "A dynamical test for terrestrial planets in the habitable zone of HD 204313", "authors": [ "E. Thilliez", "L. Jouvin", "S. T. Maddison", "J. Horner" ], "comment": "13 pages, 6 figures. Accepted for publication in the peer-reviewed proceedings of the 13th annual Australian Space Science Conference", "categories": [ "astro-ph.EP" ], "abstract": "With improvements in exoplanet detection techniques, the number of multiple planet systems discovered is increasing, while the detection of potentially habitable Earth-mass planets remains complicated and thus requires new search strategies. Dynamical studies of known multiple planet systems are therefore a vital tool in the search for stable and habitable planet candidates. Here, we present a dynamical study of the three-planet system HD 204313 to determine whether it could harbour an Earth-like planet within its habitable zone for a sufficient time to develop life. We found two semi-stable regions in the system, but neither prove stable for long enough for a terrestrial planet to develop life. Our investigations suggest that overlapping weak and high order resonances may be responsible for these semi-stable regions. This study established a framework for a larger project that will study the dynamical stability of the habitable zone of multiple planet systems, providing a list of interesting targets for future habitable low-mass planet searches.", "revisions": [ { "version": "v1", "updated": "2014-02-12T04:32:40.000Z" } ], "analyses": { "keywords": [ "habitable zone", "terrestrial planet", "multiple planet systems", "dynamical test", "earth-mass planets remains" ], "tags": [ "conference paper" ], "note": { "typesetting": "TeX", "pages": 13, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2014arXiv1402.2728T" } } }