A terrestrial-sized exoplanet at the snow line of TRAPPIST-1 [EPA]

http://arxiv.org/abs/1703.04166


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 18.764 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 0.715 Earth radii and an equilibrium temperature of 169 K, placing it at the snow line. We have also measured the rotational period of the star at 3.3 d and detected a number of flares consistent with an active, middle-aged, late M dwarf.

Read this paper on arXiv…

R. Luger, M. Sestovic, E. Kruse, et. al.
Tue, 14 Mar 17
35/74

Comments: 36 pages, 8 figure, 2 tables. Submitted to Nat. Astron. on 3/10/2017

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