Table 2
Check-table indicating if a simulation for a given viscous α-value, aspect ratio, h, and planet mass reached the observed orbit.
| Kepler- | α = 10−3, | α = 10−4, | α = 10−4, | α = 10−4, | α = 10−4, | obs. |
|---|---|---|---|---|---|---|
| System | h = 0.04 | h = 0.04 | h = 0.03 | h = 0.04, 2 mp | h = 0.04, 10 mp | ap, ep |
| 47 | 6.6 abin, 0.23 | 6.6 abin, 0.23 | 5.0 abin, 0.18 | 5.0 abin, 0.18 | ✓ | 3.53 abin, 0.03 |
| 413 | 6.0 abin, 0.21 | 5.7 abin, 0.18 | 4.8 abin, 0.15 | 5 abin, 0.15 | < 3.1 abin, 0.025 | 3.55 abin, 0.12 |
| 453 | eject | eject | 4.8 abin, 0.12 | 5.2 abin, 0.15 | < 3.1 abin, 0.025 | 4.26 abin, 0.036 |
| 38 | 3.8 abin, 0.02 | ✓ | 3.16 abin, 0.03 | |||
| 1661 | ✓ | 3.39 abin, 0.06 | ||||
| 35 | 4.7 abin, 0.1 | ✓ | 3.43 abin, 0.04 | |||
| TOI-1338 | 4.2 abin, 0.08 | (✓), 0.05 | 3.49 abin, 0.09 | |||
| 16 | 4.1 abin, 0.04 | ✓ | 3.14 abin, 0.006 | |||
| 64 | 4.8 abin, 0.08 | ✓ | ✓ | 3.64 abin, 0.05 | ||
| 34 | > 9 abin, 0.15 | 7.8 abin, 0.18 | 6.4 abin, 0.17 | < 4.5 abin, < 0.05 | 4.5 abin, 0.025 | 4.76 abin, 0.18 |
Notes. The systems are ordered from lowest ebin to highest. Every cell contains the semi-major axis and eccentricity of the final planet orbit of the stated simulation. If not stated (Cols. 2–4), the planet mass corresponds to the observed mass in Table 1. For boxes with a “✓”, the planet’s final location lies within 0.1 abin of the observed position. In Cols. 5 and 6 the planet mass in the simulations have been increased by a factor of two and ten, respectively. For comparison, the inferred parameters from the Kepler data are on the right. Blank fields were not simulated.
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