The habitable zone of Kepler-16: impact of binarity and climate models
2019
We continue to investigate the binary system
Kepler-16, consisting of a
K-type main-sequence star, a
red dwarf, and a circumbinary
Saturnianplanet. As part of our study, we describe the system's habitable zone based on different
climate models. We also report on stability investigations for possible
Earth-mass
Trojanswhile expanding a previous study by
B.
L. Quarles and collaborators given in 2012. For the
climate modelswe carefully consider the relevance of the system's parameters. Furthermore, we pursue new stability simulations for the
Earth-massobjects starting along the orbit of
Kepler-16b. The eccentricity distribution as obtained prefers values close to circular, whereas the inclination distribution remains flat. The stable solutions are distributed near the co-orbital
Lagrangian points, thus enhancing the plausibility that
Earth-mass
Trojansmight be able to exist in the
Kepler-16(AB) system.
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