Table C.1
Variation of numerical parameters.
| Sim # | Mk+1 /Mk (1) | Nann | min size(2) (m) | ϵ1 (3) | ϵ2 (4) | ξ (5) | b (6) | dmin (km) (7) |  (8) |
|---|---|---|---|---|---|---|---|---|---|
| 1 | 1.37 | 60 | 10 | 0.05 | 10−6 | −1.0 | 10−2 | 1.6 | 3.4 |
| 1A | 1.88 | 60 | 10 | 0.05 | 10−6 | −1.0 | 10−2 | 1.4 | 3.0 |
| 1B | 1.17 | 60 | 10 | 0.05 | 10−6 | −1.0 | 10−2 | 1.7 | 3.6 |
| 1C | 1.37 | 30 | 10 | 0.05 | 10−6 | −1.0 | 10−2 | 1.7 | 3.4 |
| 1D | 1.37 | 120 | 10 | 0.05 | 10−6 | −1.0 | 10−2 | 1.5 | 3.3 |
| 1E | 1.37 | 60 | 100 | 0.05 | 10−6 | −1.0 | 10−2 | 1.4 | 3.4 |
| 1F | 1.37 | 60 | 1.0 | 0.05 | 10−6 | −1.0 | 10−2 | 1.5 | 3.3 |
| 1G | 1.37 | 60 | 10 | 0.01 | 10−7 | −1.0 | 10−2 | 1.6 | 3.4 |
| 1H | 1.37 | 60 | 10 | 0.1 | 10−5 | −1.0 | 10−2 | 1.6 | 3.4 |
| 1I | 1.37 | 60 | 10 | 0.05 | 10−6 | −1.5 | 10−2 | 1.6 | 3.5 |
| 1J | 1.37 | 60 | 10 | 0.05 | 10−6 | 0.0 | 10−2 | 1.6 | 3.3 |
| 1K | 1.37 | 60 | 10 | 0.05 | 10−6 | −1.0 | 10−1 | 1.6 | 3.5 |
| 1L | 1.37 | 60 | 10 | 0.05 | 10−6 | −1.0 | 10−4 | 1.6 | 3.3 |
Notes. (1) Ratio of the mass between successive mass bins. (2)Radius of the smallest body considered in the simulation. (3)Parameter which goes into determining the coagulation time step; see Sect. A.6.1. (4) Parameter which goes into determining the coagulation time step; see Sect. A.6.1. (5) Slope of the fragment mass distribution; see Eq. (A.8). (6)Smallest possible ratio of the mass of the largest rubble particle to the total mass in the collision; see Eq. (A.7). (7) Smallest initial planetesimal size which results in a 300 km body forming within 1 Myr, assuming solid planetesimals. (8) Smallest initial planetesimal size which results in a 300 km body forming within 1 Myr, assuming rubble-pile planetesimal composition.
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