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arxiv: 1703.04166 · v2 · pith:MQBVQRY2new · submitted 2017-03-12 · 🌌 astro-ph.EP · astro-ph.IM· astro-ph.SR

A seven-planet resonant chain in TRAPPIST-1

classification 🌌 astro-ph.EP astro-ph.IMastro-ph.SR
keywords startrappist-1trappist-1hchaindwarfearthfoundmember
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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.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. A single power law for the TRAPPIST-1 flare distribution across four orders of magnitude in energy

    astro-ph.SR 2026-05 unverdicted novelty 6.0

    TRAPPIST-1 flares follow a single power law N(≥E_TESS) ∝ E_TESS^{-0.753} from 10^{29} to 10^{33} erg after sensitivity corrections and bandpass conversion.

  2. A single power law for the TRAPPIST-1 flare distribution across four orders of magnitude in energy

    astro-ph.SR 2026-05 unverdicted novelty 5.0

    TRAPPIST-1 flares obey a single power law N(≥E) ∝ E^{-0.753} from 10^29 to 10^33 erg in TESS energy after sensitivity corrections.