Table 3.
Planetary radii Rp, masses Mp, and semi-major axes a taken from the literature and adopted in this work, followed by the main results obtained with PASTA (median values and 1-σ confidence interval), that is the stellar rotation period at 150 Myr (Prot,150), the theoretically-estimated planetary mass (
), and the atmospheric mass fraction at t = tdisk = 5 Myr (
).
| Planet | Rp [R⊕] | Mp [M⊕] | a [AU] | Source | Prot,150 [d] |
 [M⊕] |
 |
|---|---|---|---|---|---|---|---|
| HD 3167 b |
 |
5.02 ± 0.38 | 0.01815 ± 0.00023 | Ch17 |
 |
 |
 |
| HD 3167 c |
 |
 |
0.1795 ± 0.0023 | Ch17 | 9.9 ± 1.3 |
 |
|
| K2-24 b | 5.4 ± 0.2 |
 |
0.154 ± 0.002 a | Pe18 |
 |
 |
 |
| K2-24 c | 7.5 ± 0.3 |
 |
0.247 ± 0.004 a | Pe18 | 15.4 ± 1.7 |
 |
|
| K2-285 b | 2.59 ± 0.06 |
 |
 |
Pa19 |
 |
 |
0.48 ± 0.33 |
| K2-285 c | 3.53 ± 0.08 |
 |
0.0824 ± 0.0018 | Pa19 |
 |
 |
|
| K2-285 d | 2.48 ± 0.06 | < 6.5 | 0.1178 ± 0.0029 | Pa19 |
 |
0.47 ± 0.36 | |
| K2-285 e | 1.95 ± 0.05 | < 10.7 |
 |
Pa19 |
 |
 |
|
| KOI-94 c | 4.32 ± 0.41 |
 b |
0.1013 ± 0.0013 | We13 |
 |
 |
0.51 ± 0.34 |
| KOI-94 d | 11.27 ± 1.06 |
 b |
0.1684 ± 0.0022 | We13 |
 |
 |
|
| KOI-94 e | 6.56 ± 0.62 |
 b |
0.3046 ± 0.0040 | We13 |
 |
 |
|
| Kepler-11 b |
 |
 c |
0.091 ± 0.001 | Li13 |
 |
 |
0.49 ± 0.34 |
| Kepler-11 c |
 |
 c |
0.107 ± 0.001 | Li13 |
 |
 |
|
| Kepler-11 d |
 |
 d |
0.155 ± 0.001 | Li13 |
 |
 |
|
| Kepler-11 e |
 |
 d |
0.195 ± 0.002 | Li13 |
 |
 |
|
| Kepler-11 f |
 |
 d |
0.25 ± 0.002 | Li13 |
 |
0.50 ± 0.33 | |
| Kepler-11 g |
 |
< 25 | 0.466 ± 0.004 | Li13 | 16.3 ± 9.2 |
 |
|
| Kepler-18 b | 2 ± 0.1 | 6.9 ± 3.4 | 0.0447 ± 0.0006 | Co11 |
 |
 |
 |
| Kepler-18 c | 5.49 ± 0.26 | 17.3 ± 1.9 | 0.0752 ± 0.0011 | Co11 |
 |
 |
|
| Kepler-18 d | 6.98 ± 0.33 | 16.4 ± 1.4 | 0.1172 ± 0.0017 | Co11 | 15.9 ± 1.5 |
 |
|
| Kepler-20 c |
 |
 |
 |
Bu16 |
 |
 |
 |
| Kepler-20 d |
 |
 |
 |
Bu16 |
 |
 |
|
| Kepler-20 e |
 |
< 3.08 e |
 |
Bu16 |
 |
 |
|
| Kepler-20 f |
 |
< 14.3 e |
 |
Bu16 |
 |
 |
|
| Kepler-25 b |
 |
 |
0.06999 ± 0.00051 f | Mi19 |
 |
 |
 |
| Kepler-25 c |
 |
 |
0.11255 ± 0.00081 f | Mi19 |
 |
 |
|
| Kepler-36 b |
 |
 |
0.1153 ± 0.0015 g | Vi20 |
 |
3.80 ± 0.10 | 0.50 ± 0.34 |
| Kepler-36 c |
 |
7.13 ± 0.18 | 0.1283 ± 0.0016 g | Vi20 |
 |
0.51 ± 0.33 | |
| Kepler-411 c | 4.421 ± 0.062 | 26.4 ± 5.9 | 0.0739 ± 0.001 | Su19 |
 |
 |
 |
| Kepler-411 d | 3.319 ± 0.104 | 15.2 ± 5.1 | 0.279 ± 0.004 | Su19 | 15.4 ± 4.9 |
 |
|
| Kepler-48 b | 1.88 ± 0.10 | 3.9 ± 2.1 | 0.05302 ± 0.00044 f | Ma14 |
 |
 |
0.50 ± 0.34 |
| Kepler-48 c | 2.71 ± 0.14 | 14.6 ± 2.3 | 0.08485 ± 0.00071 f | Ma14 |
 |
0.50 ± 0.34 | |
| Kepler-48 d | 2.04 ± 0.11 | 7.9 ± 4.6 | 0.22902 ± 0.00192 f | Ma14 |
 |
 |
|
| WASP-47 d | 3.576 ± 0.046 | 13.1 ± 1.5 |
 f |
Va17 |
 |
 |
 |
| WASP-47 e | 6.35 ± 0.64 | 6.83 ± 0.66 |
 f |
Va17 |
 |
 |
References. Ch17: Christiansen et al. (2017); Pe18: Petigura et al. (2018); Pa19: Palle et al. (2019); We13: Weiss et al. (2013); Li13: Lissauer et al. (2013); Co11: Cochran et al. (2011); Bu16: Buchhave et al. (2016); Mi19: Mills et al. (2019); Vi20: Vissapragada et al. (2020); Su19: Sun et al. (2019); Ma14: Marcy et al. (2014); Va17: Vanderburg et al. (2017).
From Petigura et al. (2016).
From Masuda et al. (2013).
Combination of estimates from Lissauer et al. (2011), Lissauer et al. (2013), Borsato et al. (2014), and Hadden & Lithwick (2014).
Same as (c) + Hadden & Lithwick (2017).
From Fressin et al. (2012).
From Carter et al. (2012).
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