A seven-planet resonant chain in TRAPPIST-1

The TRAPPIST-1 system is the first transiting planet system found orbiting an ultra-cool dwarf star. At least seven planets similar to Earth in radius and in mass were previously found to transit this host star. Subsequently, TRAPPIST-1 was observed as part of the K2 mission and, with these new data...

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Veröffentlicht in:arXiv.org 2017-05
Hauptverfasser: Luger, Rodrigo, Sestovic, Marko, Kruse, Ethan, Grimm, Simon L, Brice-Olivier Demory, Agol, Eric, Bolmont, Emeline, Fabrycky, Daniel, Fernandes, Catarina S, Valérie Van Grootel, Burgasser, Adam, Gillon, Michaël, Ingalls, James G, Jehin, Emmanuël, Raymond, Sean N, Selsis, Franck, Amaury H M J Triaud, Barclay, Thomas, Barentsen, Geert, Howell, Steve B, Delrez, Laetitia, de Wit, Julien, eman-Mackey, Daniel, Holdsworth, Daniel L, Leconte, Jérémy, Lederer, Susan, Turbet, Martin, Yaseen Almleaky, Benkhaldoun, Zouhair, Magain, Pierre, Morris, Brett, Heng, Kevin, Queloz, Didier
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Sprache:eng
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Zusammenfassung:The TRAPPIST-1 system is the first transiting planet system found orbiting an ultra-cool dwarf star. At least seven planets similar to Earth in radius and in mass were previously found to transit this host star. Subsequently, TRAPPIST-1 was observed as part of the K2 mission and, with these new data, we report the measurement of an 18.77 d orbital period for the outermost planet, TRAPPIST-1h, which was unconstrained until now. This value matches our theoretical expectations based on Laplace relations and places TRAPPIST-1h as the seventh member of a complex chain, with three-body resonances linking every member. We find that TRAPPIST-1h has a radius of 0.727 Earth radii and an equilibrium temperature of 173 K. We have also measured the rotational period of the star at 3.3 d and detected a number of flares consistent with a low-activity, middle-aged, late M dwarf.
ISSN:2331-8422
DOI:10.48550/arxiv.1703.04166