Table B.2
Detailed median radii per mass per model for planets that form at 4 AU from their host stars.
| Model A | Model B | |||||||||
|---|---|---|---|---|---|---|---|---|---|---|
| Median radius (R⊕) | Radius difference (%) | Median radius (R⊕) | Radius difference (%) | |||||||
| Mass (M⊕) | Thin | Thick | Halo | Thick–Thin | Halo–Thick | Thin | Thick | Halo | Thick–Thin | Halo–Thick |
| 1 | 1.261 | 1.303 | 1.323 | 3.31 | 1.53 | 1.270 | 1.309 | 1.326 | 3.05 | 1.35 |
| 2 | 1.545 | 1.596 | 1.620 | 3.28 | 1.51 | 1.535 | 1.580 | 1.601 | 2.98 | 1.31 |
| 3 | 1.733 | 1.790 | 1.817 | 3.26 | 1.50 | 1.706 | 1.757 | 1.779 | 2.94 | 1.27 |
| 4 | 1.877 | 1.938 | 1.967 | 3.26 | 1.49 | 1.836 | 1.890 | 1.913 | 2.94 | 1.24 |
| 5 | 1.994 | 2.059 | 2.089 | 3.25 | 1.48 | 1.940 | 1.997 | 2.021 | 2.92 | 1.24 |
| 6 | 2.092 | 2.160 | 2.192 | 3.25 | 1.48 | 2.028 | 2.087 | 2.112 | 2.90 | 1.22 |
| 7 | 2.178 | 2.249 | 2.282 | 3.25 | 1.47 | 2.104 | 2.165 | 2.192 | 2.89 | 1.21 |
| 8 | 2.254 | 2.327 | 2.361 | 3.24 | 1.47 | 2.172 | 2.234 | 2.261 | 2.87 | 1.20 |
| 9 | 2.322 | 2.398 | 2.433 | 3.24 | 1.47 | 2.232 | 2.297 | 2.324 | 2.89 | 1.20 |
| 10 | 2.384 | 2.461 | 2.497 | 3.24 | 1.46 | 2.297 | 2.353 | 2.381 | 2.88 | 1.20 |
| Mean | 3.26 | 1.49 | 2.93 | 1.24 | ||||||
Notes. The water mass fraction is extracted from the stoichiometric model outlined in Sect. 3.3. The median radius per stellar population is shown in earth radii R⊕ and the median radius difference between different stellar populations is calculated as a percentage.
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