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Table 1
Summary of results from Chanut et al. (2008).
| Mass ratio | Collision radius | Co-orbitals | Collisions | Crossings | Others |
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|
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| μ2 = 10-7 | 0.005 RHill | 3% | 12% | 68% | 17% |
| 0.05 RHill | 3% | 43% | 41% | 13% | |
| μ2 = 10-6 | 0.005 RHill | 8% | 7% | 79% | 6% |
| 0.05 RHill | 7% | 28% | 59% | 6% | |
| μ2 = 10-5 | 0.005 RHill | 5% | 4% | 88% | 3% |
| 0.05 RHill | 5% | 23% | 69% | 3% | |
| μ2 = 10-4 | 0.005 RHill | <1% | 1% | 98% | <1% |
| 0.05 RHill | <1% | 24% | 75% | <1% | |
| μ2 = 10-3 | 0.005 RHill | − | 23% | 77% | − |
| 0.05 RHill | − | 27% | 73% | − | |
Notes.Distribution of trapping in 1:1 resonance, collisions, crossings, and other events related to the dynamics of a pebble submitted to the effect of gaseous drag. The range of planet eccentricity was 0 ≤ e2 ≤ 0.07.
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