Table 1
Potentially habitable planets from both scenarios when tidal and GR effects are included in the simulations (S1t and S2t) and when these effects are neglected in the case of S1 (S1wt).
| Scenario | Embryo | a | e | M | H2O | IHZ |
|---|---|---|---|---|---|---|
| [au] | [M⊕] | [%] | ||||
| S1t | 39 | 0.020 | 0.23 | 0.004 | 0.01 | b |
| S1t | 132 | 0.025 | 0.18 | 0.010 | 0.01 | b |
| S1t | 113 | 0.026 | 0.23 | 0.008 | 0.01 | b |
| S1t | 113 | 0.027 | 0.27 | 0.013 | 0.01 | b |
| S1t | 132 | 0.024 | 0.43 | 0.007 | 0.01 | b |
| S1t | 33 | 0.018 | 0.07 | 0.001 | 0.01 | b |
| S1t | 126 | 0.046 | 0.19 | 0.010 | 0.01 | a |
| S1t | 115 | 0.022 | 0.23 | 0.013 | 0.01 | b |
| S1t | 63 | 0.022 | 0.30 | 0.006 | 0.01 | b |
| S1t | 142 | 0.052 | 0.08 | 0.013 | 0.01 | a |
| S1t | 62 | 0.019 | 0.28 | 0.007 | 0.01 | b |
| S1wt | 163 | 0.066 | 0.195 | 0.017 | 0.01 | a |
| S1wt | 90 | 0.022 | 0.18 | 0.007 | 0.01 | b |
| S2t | 59 | 0.051 | 0.45 | 0.337 | 0.01 | a |
| S2t | 39 | 0.053 | 0.20 | 0.370 | 0.01 | a |
Notes. The initial numbers of embryos that become the resulting planet are listed in Col. 2 with their respective final semimajor axes, eccentricity, mass, and percentage of water in mass. In their final locations, the planets are located in the IHZ at 100 Myr (IHZ = a) or in the IHZ at 1 Gyr (IHZ = b).
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