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Table 3
First unstable resonance and corresponding ejection time for different eccentricities of the binary and different migration velocities, starting with e = 0.05 and a = 2 au.
| Migration | 10-3 au/yr | 10-4 au/yr | 10-5 au/yr | 10-6 au/yr |
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| eB = 0 | 1:4, 50 yr | 1:4, 103 yr | 1:5, 104 yr | 1:5, 105 yr |
| eB = 0.2 | 1:5, 50 yr | 1:6, 103 yr | 1:6, 104 yr | 1:7, 5 × 104 yr |
| eB = 0.4 | 1:6, 100 yr | 1:6, 500 yr | 1:6, 2 × 103 yr | 1:7, 2 × 104 yr |
| eB = 0.6 | 1:6, 100 yr | 1:6, 100 yr | 1:6, 2 × 103 yr | 1:6, 104 yr |
| eB = 0.8 | 1:6, 100 yr | 1:7, 500 yr | 1:8, 104 yr | 1:7, 2 × 104 yr |
Notes. The ejection time corresponds to the time needed to eject the planet starting from the beginning of the MMR trapping.
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