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A seven-planet resonant chain in TRAPPIST-1

Authors :
Luger, Rodrigo
Sestovic, Marko
Kruse, Ethan
Grimm, Simon L.
Demory, Brice-Olivier
Agol, Eric
Bolmont, Emeline
Fabrycky, Daniel
Fernandes, Catarina S.
Van Grootel, Valérie
Burgasser, Adam
Gillon, Michaël
Ingalls, James G.
Jehin, Emmanuël
Raymond, Sean N.
Selsis, Franck
Triaud, Amaury H. M. J.
Barclay, Thomas
Barentsen, Geert
Howell, Steve B.
Delrez, Laetitia
De Wit, Julien
Foreman-Mackey, Daniel
Holdsworth, Daniel L.
Leconte, Jérémy
Lederer, Susan
Turbet, Martin
Almleaky, Yaseen
Benkhaldoun, Zouhair
Magain, Pierre
Morris, Brett M.
Heng, Kevin
Queloz, Didier
Publisher :
Nature Publishing Group

Abstract

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.

Details

Language :
English
Database :
OpenAIRE
Accession number :
edsair.doi...........812fd925e51c2d66dbb44a9e3802eeeb