Open Access
Table 8
Percentage of the population A, B, and C planetary systems that experienced catastrophic events.
| Pop. A | |||
|---|---|---|---|
| Ns = 2 | Ns = 3 | Ns = 4 | |
| No catastrophic events | 100% | 87.1% | 54.8% |
| Ejections or scatterings only | 0% | 6.7% | 21.3% |
| Collisionsp–p only | 0% | 6.2% | 11.7% |
| Close approach to the binary | 0% | 0% | 3.5% |
| Multiple catastrophic events | 0% | 0% | 8.7% |
| Pop. B | |||
| Ns = 2 | Ns = 3 | Ns = 4 | |
| No catastrophic events | 100% | 45.8% | 20.9% |
| Ejections or scatterings only | 0% | 23.2% | 28.2% |
| Collisionsp–p only | 0% | 18.4% | 17.3% |
| Close approach to the binary | 0% | 0.3% | 0% |
| Multiple catastrophic events | 0% | 12.3% | 33.6% |
| Pop. C | |||
| Ns = 2 | Ns = 3 | Ns = 4 | |
| No catastrophic events | 100% | 48.4% | 5% |
| Ejections or scatterings only | 0% | 19.2% | 15% |
| Collisionsp–p only | 0% | 11.2% | 15% |
| Close approach to the binary | 0% | 0% | 0% |
| Multiple catastrophic events | 0% | 21.2% | 65% |
Notes. The Table is divided by taking into account the initial number of planets (see Table 2 to know how many simulations had initially two, three, and four planets).
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