# A seven-planet resonant chain in TRAPPIST-1

**Authors:** Rodrigo Luger, Marko Sestovic, Ethan Kruse, Simon L. Grimm,, Brice-Olivier Demory, Eric Agol, Emeline Bolmont, Daniel Fabrycky, Catarina, S. Fernandes, Val\'erie Van Grootel, Adam Burgasser, Micha\"el Gillon, James, G. Ingalls, Emmanu\"el Jehin, Sean N. Raymond, Franck Selsis, Amaury H.M.J., Triaud, Thomas Barclay, Geert Barentsen, Steve B. Howell, Laetitia Delrez,, Julien de Wit, Daniel Foreman-Mackey, Daniel L. Holdsworth, J\'er\'emy, Leconte, Susan Lederer, Martin Turbet, Yaseen Almleaky, Zouhair Benkhaldoun,, Pierre Magain, Brett Morris, Kevin Heng, and Didier Queloz

arXiv: 1703.04166 · 2017-05-23

## TL;DR

The paper reports the discovery of a seven-planet resonant chain in the TRAPPIST-1 system, with new orbital data, resonance relations, and planetary characteristics, enhancing understanding of its complex orbital dynamics.

## Contribution

It provides the first measurement of TRAPPIST-1h's orbital period and confirms a resonant chain with three-body resonances linking all seven planets.

## Key findings

- TRAPPIST-1h has an orbital period of 18.77 days.
- The planetary system forms a complex resonant chain.
- TRAPPIST-1's star has a rotational period of 3.3 days.

## 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.

## Full text

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## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/1703.04166/full.md

## References

29 references — full list in the complete paper: https://tomesphere.com/paper/1703.04166/full.md

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Source: https://tomesphere.com/paper/1703.04166