Table 4
Percentage of population A, B, C, and D planetary systems that experienced catastrophic events.
| Nominal setup | ||
|---|---|---|
| Pop. A | Pop. B | |
| No catastrophic events | 82.5% | 49% |
| Ejections or scatterings only | 8.6% | 20.6% |
| Collisionsp–p only | 6.1% | 15.2% |
| Close approach to the binary | 0.8% | 0.2% |
| Multiple catastrophic events | 2% | 15% |
| Resonant setup | ||
| Pop. C | Pop. D | |
| No catastrophic events | 65.6% | 0% |
| Ejections or scatterings only | 11.2% | 39.2% |
| Collisionsp–p only | 7% | 4.8% |
| Close approach to the binary | 0% | 0% |
| Multiple catastrophic events | 16.2% | 56% |
Notes. Population A multiple catastrophic events (2%) arise from 1.8% of ejections or scatterings plus collisionsp–p, 0.1% of ejections or scatterings plus close approach to the binary and 0.1% of ejections or scatterings plus collisionsp–p plus close approach to the binary; population B multiple catastrophic events (15%) arise from: 5.4% of ejections or scatterings plus collisionsp–p, 7.4% of ejections or scatterings plus close approach to the binary, 0.4% of collisionsp–p plus close approach to the binary and 1.8% of ejections or scatterings plus collisionsp–p plus close approach to the binary; population C multiple catastrophic events (16.2%) arise from 4.6% of ejections or scatterings plus collisionsp–p, 7.8% of ejections or scatterings plus close approach to the binary, 0.2% of collisionsp–p plus close approach to the binary and 3.6% of ejections or scatterings plus collisionsp–p plus close approach to the binary; population D multiple catastrophic events (56%) arise from 38.4% of ejections or scatterings plus collisionsp–p, 11% of ejections or scatterings plus close approach to the binary and 6.6% of ejections or scatterings plus collisionsp–p plus close approach to the binary.
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