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Table 2
Effect of the 1:6 mean-motion resonance and ejection duration for different eccentricities of the binary, starting with a planet eccentricity of e = 0.05.
| Binary eccentricity | Effect of the 1:6 MMR |
|
|
|
| eB = 0.0 | no ejection |
| eB = 0.2 | no ejection |
| eB = 0.4 | ejection in 100–1000 yr |
| eB = 0.6 | ejection in 100–1000 yr |
| eB = 0.8 | ejection in 100 yr |
Notes. For aB = 0.4 au, the 1:6 resonance corresponds to a planet semi-major axis around a = 1.3 au.
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