A seven-planet resonant chain in TRAPPIST-1

作者：Luger, Rodrigo^*; Sestovic, Marko; Kruse, Ethan; Grimm, Simon L.; Demory, Brice-Olivier; Agol, Eric; Bolmont, Emeline; Fabrycky, Daniel; Fernandes, Catarina S.; Van Grootel, Valerie; Burgasser, Adam; Gillon, Michael; Ingalls, James G.; Jehin, Emmanuel; 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, Jeremy; Lederer, Susan

来源：Nature Astronomy, 2017, 1(6): 0129.

DOI：10.1038/s41550-017-0129

• HOT SUPER-EARTHS
• TRANSITING PLANETS
• HABITABLE ZONES
• KINEMATICS
• SYSTEMS
• II.
• EXOPLANETS
• MIGRATION
• ALGORITHM
• EVOLUTION

The TRAPPIST-1 system is the first transiting planet system found orbiting an ultracool dwarf star(1). At least seven planets similar in radius to Earth were previously found to transit this host star(2). Subsequently, TRAPPIST-1 was observed as part of the K2 mission and, with these new data, we report the measurement of an 18.77 day orbital period for the outermost transiting planet, TRAPPIST-1 h, which was previously unconstrained. This value matches our theoretical expectations based on Laplace relations(3) and places TRAPPIST-1 h as the seventh member of a complex chain, with three-body resonances linking every member. We find that TRAPPIST-1 h has a radius of 0.752 R-circle plus and an equilibrium temperature of 173 K. We have also measured the rotational period of the star to be 3.3 days and detected a number of flares consistent with a low-activity, middle-aged, late M dwarf.

• 出版日期2017-6
• 单位中国地震局