A Six-Planet Resonance Chain in K2-138?
M. Cerioni (1), C. Beaug\'e (1) ((1) Instituto de Astronom\'ia, Te\'orica y Experimental (IATE), Observatorio Astron\'omico, Universidad, Nacional de C\'ordoba, Argentina)

TL;DR
This paper investigates the dynamical structure of the K2-138 system, revealing a unique first-order three-planet resonance that explains its current configuration and evolutionary history.
Contribution
It is the first to identify a pure first-order three-planet mean-motion resonance in a multi-planet system and links it to the system's dynamical evolution.
Findings
The outermost planet g is in a three-planet resonance with its neighbors.
The system's current configuration can be explained by tidal interactions over time.
The resonance capture is robust for similar planetary masses.
Abstract
The K2-138 system hosts six planets and presents an interesting case study due to its distinctive dynamical structure. Its five inner planets are near a chain of 3/2 two-body mean-motion resonances, while the outermost body (planet {\it g}) is significantly detached, having a mean-motion ratio of with its closest neighbor. We show that the orbit of is actually consistent with the first-order three-planet resonance (3P-MMR) characterized by the relation and is the first time a pure first-order 3P-MMR is found in a multi-planet system and tied to its current dynamical structure. Adequate values for the masses allow to trace the dynamical history of the system from an initial capture in a 6-planet chain (with in a 3/1 resonance), up to its current configuration due to tidal interactions over the age of the star. The increase in…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astro and Planetary Science · Astrophysics and Star Formation Studies
