Kepler-16b: safe in a resonance cell
arXiv:1207.0101 · doi:10.1088/0004-637X/769/2/152
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.
17 pages, including 5 figures
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Cited by in corpus (16)
- On the Fate of Unstable Circumbinary Planets: Tatooine's Close Encounters with a Death Star
- A dynamical stability study of Kepler Circumbinary Planetary systems with one planet
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- Formation of S-type planets in close binaries: scattering induced tidal capture of circumbinary planets
- Circumbinary Planet Formation in the Kepler-16 System. II. A Toy Model for In-situ Planet Formation within a Debris Belt
- Three-lane and multi-lane signatures of planets in planetesimal disks
- Coevolution of Binaries and Gaseous Discs
- Habitability properties of circumbinary planets
- Evolution of a ring around the Pluto-Charon binary
- On the Estimation of Circumbinary Orbital Properties
- Tidal decay of circumbinary planetary systems
- Simulations of the dynamics of the debris disks in the systems Kepler-16, Kepler-34, and Kepler-35
- Massive evaluation and analysis of Poincaré recurrences on grids of initial data: a tool to map chaotic diffusion
- Structure of the Stellar Neighborhood of CQ Tau in the Presence of a Companion in an Elongated Orbit
- Dynamical environments of relativistic binaries: The phenomenon of resonance shifting
- The resilience of the sailboat stable region