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• W3100355989 abstract "The planet Kepler-16b is known to follow a circumbinary orbit around a system of two main-sequence stars. We construct stability diagrams in the pericentric distance–eccentricity plane, which show that Kepler-16b is in a hazardous vicinity to the chaos domain—just between the instability teeth in the space of orbital parameters. Kepler-16b survives, because it is close to the stable half-integer 11/2 orbital resonance with the central binary, safe inside a resonance cell bounded by the unstable 5/1 and 6/1 resonances. The neighboring resonance cells are vacant, because they are purged by Kepler-16b, due to overlap of first-order resonances with the planet. The newly discovered planets Kepler-34b and Kepler-35b are also safe inside resonance cells at the chaos border." @default.
• W3100355989 created "2020-11-23" @default.
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• W3100355989 date "2013-05-15" @default.
• W3100355989 modified "2023-10-18" @default.
• W3100355989 title "KEPLER-16b: SAFE IN A RESONANCE CELL" @default.
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• W3100355989 doi "https://doi.org/10.1088/0004-637x/769/2/152" @default.
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