Table 1
General characteristics of the most distinctive planets formed in the S1–S3 simulations of the first set, using ad hoc initial conditions.
| Simulation | Planet | ai (au) | af (au) | ⟨ e ⟩ 100 Myr | ⟨ i ⟩ 100 Myr | M (M⊕) | W (%) | TLGI (Myr) |
|
|
||||||||
| S1 | Innermost | 0.68 | 0.62 | 0.07 |
|
1.57 | 5.47 | 56.1 |
| Planet a in HZ | 4.52 | 1.41 | 0.06 |
|
2.21 | 32.55 | 35 | |
| Most massive | 4.52 | 1.41 | 0.06 |
|
2.21 | 32.55 | 35 | |
|
|
||||||||
| S2 | Innermost | 0.78 | 0.47 | 0.14 |
|
0.6 | 7.12 | 5.55 |
| Planet b in HZ | 1.30 | 0.90 | 0.08 |
|
1.19 | 4.51 | 35 | |
| Planet c in HZ | 3.13 | 1.35 | 0.06 |
|
1.65 | 39.48 | 22 | |
| Most massive | 3.25 | 3.35 | 0.05 |
|
2.15 | 43.66 | 96.8 | |
|
|
||||||||
| S3 | Innermost | 0.50 | 0.63 | 0.08 |
|
1.13 | 6.66 | 11.45 |
| Planet d in HZ | 0.64 | 0.98 | 0.07 |
|
0.66 | 8.10 | 6.00 | |
| Planet e in HZ | 3.43 | 1.53 | 0.05 |
|
2.27 | 32.46 | 71.9 | |
| Most massive | 4.69 | 2.77 | 0.04 |
|
3.08 | 47.86 | 44.3 | |
Notes. ai is the initial and af is the final semi-major axis. The initial semi-major axis of a planet represents the initial location of the most massive embryo from which the planet formed. ⟨ e ⟩ 100 Myr and ⟨ i ⟩ 100 Myr represent the mean eccentricity and inclination in the last 100 Myr of evolution. M(M⊕) represents the final mass, W(%) the final percentage of water by mass, and TLGI the timescale in Myr associated with the last giant impact produced by an embryo.
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