Table A.1
Predicted thicknesses di of interior layers for exoplanets with well known masses and radii.
| Planet | Observation Mass (M⊕) | Radius (R⊕) | Teq (K) | References | Prediction dCore | dMantle | dWater | dGas |
|---|---|---|---|---|---|---|---|---|
| GJ 1214 b | 8.17±0.43 | 2.742±0.053 | 596.0±19.0 | Cloutier et al. 2021 (Carter et al. 2011) |  |
 |
 |
 |
| GJ 486 b | 2.82±0.12 | 1.305±0.067 | 701.0±13.0 | Trifonov et al. 2021 |  |
 |
 |
 |
| HD 136352 b | 4.72±0.42 | 1.664±0.043 | 905.0±14.0 | Delrez et al. 2021 (Kane et al. 2020) |  |
 |
 |
 |
| HD 136352 с | 11.24±0.65 | 2.916±0.075 | 677.0±11.0 | Delrez et al. 2021 (Kane et al. 2020) |  |
 |
 |
 |
| HD 191939 b | 10.4±0.9 | 3.39±0.07 | 893.0±36.0 | Lubin et al. 2022 |  |
 |
 |
 |
| HD 219134 с | 4.36±0.22 | 1.511±0.047 | 782.0±6.0 | Gillon et al. 2017 |  |
 |
 |
 |
| HIP 97166 b | 20.0±1.5 | 2.74±0.13 | 757.0±25.0 | MacDougall et al. 2021 |  |
 |
 |
 |
| Kepler-36 b | 3.83±0.11 | 1.498±0.061 | 978.0±11.0 | Vissapragada et al. 2020 (Carter et al. 2012) |  |
 |
 |
 |
| Kepler-36 с | 7.13±0.18 | 3.679±0.096 | 928.0±10.0 | Vissapragada et al. 2020 (Carter et al. 2012) |  |
 |
 |
 |
| LHS 1140 b | 6.38±0.46 | 1.635±0.046 | 379.0±4.0 | Lillo-Box et al. 2020 (Dittmann et al. 2017) |  |
 |
 |
 |
| LHS 1140 с | 1.76±0.17 | 1.169±0.038 | 709.0±8.0 | Lillo-Box et al. 2020 |  |
 |
 |
 |
| LHS 1478 b | 2.33±0.2 | 1.242±0.051 | 595.0±10.0 | Soto et al. 2021 |  |
 |
 |
 |
| TOI-220 b | 13.8±1.0 | 3.03±0.15 | 805.0±21.0 | Hoyer et al. 2021 |  |
 |
 |
 |
| TOI-270 с | 6.15±0.37 | 2.355±0.064 | 488.0±12.0 | Van Eylen et al. 2021 |  |
 |
 |
 |
| TOI-270 d | 4.78±0.43 | 2.133±0.058 | 387.0±10.0 | Van Eylen et al. 2021 |  |
 |
 |
 |
| TOI-421 с | 16.42±1.06 | 5.09±0.16 | 674.0±11.0 | Carleo et al. 2020 |  |
 |
 |
 |
| TRAPPIST-1 b | 1.374±0.069 | 1.116±0.014 | 400.0±8.0 | Agol et al. 2021 (Gillon et al. 2017) |  |
 |
 |
 |
| TRAPPIST-1 с | 1.308±0.056 | 1.097±0.014 | 342.0±7.0 | Agol et al. 2021 (Gillon et al. 2017) |  |
 |
 |
 |
| TRAPPIST-1 d | 0.388±0.012 | 0.788±0.011 | 288.0±6.0 | Agol et al. 2021 (Gillon et al. 2017) |  |
 |
 |
 |
| TRAPPIST-1 e | 0.692±0.022 | 0.92±0.013 | 251.0±5.0 | Agol et al. 2021 (Grimm et al. 2018) |  |
 |
 |
 |
| TRAPPIST-1 f | 1.039±0.031 | 1.045±0.013 | 219.0±4.0 | Agol et al. 2021 |  |
 |
 |
 |
| TRAPPIST-1 g | 1.321±0.038 | 1.129±0.015 | 199.0±4.0 | Agol et al. 2021 (Gillon et al. 2017) |  |
 |
 |
 |
Notes: Here, we give the median of each predicted distribution and the 5% and 95% percentiles. For planets with nonsymmetric mass or radius uncertainties, the larger value was used. Separate references for Teq are given in parentheses. For planets where no uncertainty of Teq was given, an uncertainty of 2% is assumed. A more extensive data set of 75 planets with radius and mass uncertainties of 10% and 20%, respectively, including both mass fractions and thickness, is available in electronic form at the CDS.
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