Table B.4
Results for water-rich rocky planets observed by TESS after 30,000 runs (Monte Carlo method).
Exoplanet | Mp | Rp | S:O | Prot | a | D2 | D3 | Seff | Prob. | CMF | MMF | IMF | Roℓ | Regime | ℳ/ℳ⊕ |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
GJ 143 b | 22.884 ±1.186 | 2.615 ±0.095 | 1:1 | 35.613 | 0.191 | 0.433 | 0.823 | 5.6 | 1.00 | 0.11 ±0.02 | 0.63 ±0.10 | 0.26 ±0.12 | 5.18 ±0.47 | Multip. | 0.04 ± 0.01 |
HD 108236 b | 3.290 ±0.190* | 1.615 ±0.029 | 1:1 | 3.796 | 0.045 | 0.792 | 1.429 | 345.3 | 0.99 | 0.11 ±0.01 | 0.65 ±0.06 | 0.24 ± 0.07 | 0.48 ± 0.05 | Multip. | 0.04 ± 0.01 |
HD 108236 c | 5.020 ±0.288* | 2.071 ± 0.030 | 1:1 | 6.203 | 0.063 | 0.780 | 1.429 | 179.3 | 0.99 | 0.03 ±0.01 | 0.20 ±0.08 | 0.77 ± 0.09 | 0.70 ±0.07 | Multip. | 0.01 ± 0.002 |
HD 110113 b | 4.630 ±0.346 | 2.026 ± 0.060 | 1:1 | 2.541 | 0.036 | 0.881 | 1.606 | 690.0 | 0.76 | 0.03 ± 0.02 | 0.20 ±0.11 | 0.77 ±0.13 | 0.25 ± 0.03 | Multip. | 0.02 ±0.003 |
HD 15337 c | 8.522 ±0.903 | 2.371 ±0.065 | 1:1 | 17.178 | 0.126 | 0.644 | 1.201 | 29.0 | 0.75 | 0.03 ± 0.02 | 0.20 ±0.11 | 0.77 ±0.13 | 2.39 ± 0.24 | Multip. | 0.01 ± 0.002 |
HD 207897 b | 14.396 ± 0.925 | 2.503 ±0.046 | 1:1 | 16.202 | 0.117 | 0.573 | 1.071 | 26.6 | 1.00 | 0.08 ±0.01 | 0.45 ±0.08 | 0.47 ± 0.09 | 2.56 ±0.26 | Multip. | 0.03 ± 0.01 |
HD 23472 c | 10.315 ±3.781 | 2.203 ± 0.182 | 1:1 | 29.652 | 0.171 | 0.469 | 0.891 | 8.0 | 0.59 | 0.10 ±0.04 | 0.59 ±0.22 | 0.31 ± 0.25 | 5.42 ±0.54 | Multip. | 0.02 ±0.003 |
HD 63433 b | 5.413 ±0.300* | 2.130 ±0.050 | 1:1 | 7.108 | 0.072 | 0.802 | 1.470 | 144.6 | 0.77 | 0.03 ± 0.02 | 0.16 ±0.09 | 0.81 ±0.11 | 0.76 ± 0.08 | Multip. | 0.01 ± 0.002 |
HD 86226 c | 7.285 ± 0.666 | 2.160 ±0.046 | 1:1 | 3.984 | 0.049 | 0.986 | 1.798 | 480.4 | 1.00 | 0.07 ± 0.02 | 0.39 ±0.11 | 0.54 ±0.13 | 0.50 ±0.05 | Multip. | 0.04 ± 0.01 |
HIP 97166 b | 19.996 ±0.868 | 2.740 ±0.075 | 1:1 | 10.289 | 0.089 | 0.644 | 1.199 | 58.6 | 1.00 | 0.07 ± 0.02 | 0.40 ±0.10 | 0.53 ±0.12 | 1.42 ± 0.14 | Multip. | 0.05 ± 0.01 |
HR 858 b | 5.094 ±0.286* | 2.085 ± 0.037 | 3:2 | 2.391 | 0.048 | 1.350 | 2.440 | 1037 | 0.95 | 0.03 ±0.01 | 0.18 ±0.08 | 0.79 ±0.10 | 0.23 ± 0.02 | Multip. | 0.02 ±0.003 |
HR 858 c | 4.484 ±0.259* | 1.939 ± 0.040 | 1:1 | 5.973 | 0.067 | 1.354 | 2.440 | 510.3 | 1.00 | 0.06 ± 0.02 | 0.33 ±0.09 | 0.61 ±0.10 | 0.75 ± 0.08 | Multip. | 0.02 ±0.003 |
HR 858 d | 5.482 ±0.298* | 2.149 ± 0.043 | 3:2 | 7.487 | 0.103 | 1.348 | 2.440 | 224.9 | 0.76 | 0.02 ±0.01 | 0.14 ±0.08 | 0.84 ±0.09 | 0.76 ± 0.08 | Multip. | 0.01 ± 0.002 |
L 98-59 b | 0.371 ± 0.076 | 0.864 ±0.030 | 1:1 | 2.253 | 0.022 | 0.115 | 0.215 | 24.4 | 0.74 | 0.12 ±0.02 | 0.68 ±0.15 | 0.20 ±0.17 | 0.20 ±0.02 | Multip. | 0.01 ± 0.002 |
L 98-59 c | 2.204 ±0.144 | 1.407 ± 0.044 | 1:1 | 3.691 | 0.030 | 0.109 | 0.215 | 12.6 | 0.85 | 0.12 ±0.01 | 0.72 ± 0.07 | 0.16 ±0.08 | 0.44 ± 0.04 | Multip. | 0.03 ± 0.01 |
L 98-59 d | 1.942 ±0.161 | 1.531 ±0.062 | 1:1 | 7.451 | 0.048 | 0.110 | 0.215 | 4.9 | 0.99 | 0.06 ± 0.03 | 0.38 ±0.16 | 0.56 ±0.18 | 1.10 ±0.11 | Multip. | 0.01 ± 0.002 |
LTT 1445A b | 1.835 ±0.588 | 1.399 ±0.071 | 3:2 | 3.573 | 0.038 | 0.097 | 0.190 | 6.4 | 0.42 | 0.10 ±0.04 | 0.61 ± 0.23 | 0.29 ± 0.26 | 0.52 ±0.05 | Multip. | 0.02 ±0.003 |
LTT 3780 c | 8.787 ±0.822 | 2.302 ±0.088 | 1:1 | 12.252 | 0.077 | 0.123 | 0.250 | 2.6 | 0.97 | 0.06 ± 0.03 | 0.33 ±0.15 | 0.61 ±0.18 | 1.83 ±0.18 | Multip. | 0.02 ±0.003 |
TOI-1062 b | 10.139 ± 0.478 | 2.268 ± 0.054 | 1:1 | 4.113 | 0.049 | 0.672 | 1.245 | 214.9 | 1.00 | 0.08 ±0.01 | 0.49 ± 0.08 | 0.43 ± 0.09 | 0.50 ±0.05 | Multip. | 0.08 ± 0.01 |
TOI-1260 b | 8.618 ±0.813 | 2.346 ± 0.056 | 1:1 | 3.127 | 0.036 | 0.343 | 0.665 | 91.1 | 0.95 | 0.04 ± 0.02 | 0.25 ±0.12 | 0.71 ±0.13 | 0.35 ± 0.05 | Multip. | 0.04 ± 0.01 |
TOI-1266 b | 14.874 ±4.645 | 2.397 ± 0.079 | 1:1 | 10.895 | 0.074 | 0.163 | 0.326 | 4.9 | 0.74 | 0.10 ±0.04 | 0.60 ±0.22 | 0.31 ± 0.26 | 1.61 ± 0.16 | Multip. | 0.06 ± 0.01 |
TOI-1266 c | 2.695 ±0.756 | 1.575 ± 0.078 | 1:1 | 18.801 | 0.106 | 0.167 | 0.326 | 2.4 | 0.65 | 0.10 ±0.04 | 0.57 ±022 | 0.33 ± 0.26 | 3.03 ± 0.30 | Multip. | 0.01 ± 0.002 |
TOI-1634 b | 4.899 ±0.397 | 1.790 ± 0.046 | 1:1 | 0.989 | 0.015 | 0.170 | 0.341 | 122.9 | 1.00 | 0.11 ±0.01 | 0.65 ±0.09 | 0.24 ± 0.10 | 0.10 ±0.01 | Dipolar | 2.54 ±0.51 |
TOI-1685 b | 3.782 ±0.364 | 1.700 ±0.041 | 1:1 | 0.669 | 0.012 | 0.175 | 0.349 | 214.9 | 1.00 | 0.10 ±0.02 | 0.61 ±0.10 | 0.29 ±0.11 | 0.06 ± 0.003 | Dipolar | 1.67 ±0.33 |
TOI-1749 b | 2.536 ±0.146* | 1.492 ± 0.064 | 1:1 | 2.388 | 0.029 | 0.265 | 0.509 | 81.3 | 0.53 | 0.11 ±0.02 | 0.67 ± 0.10 | 0.22 ±0.12 | 0.28 ± 0.03 | Multip. | 0.04 ± 0.01 |
TOI-1749 d | 15.00 ±0.00 | 2.520 ±0.086 | 1:1 | 9.051 | 0.071 | 0.259 | 0.509 | 13.7 | 1.00 | 0.08 ±0.02 | 0.46 ±0.11 | 0.46 ± 0.13 | 1.29 ±0.13 | Multip. | 0.05 ± 0.01 |
TOI-178 c | 4.634 ±0.348 | 1.703 ±0.050 | 1:1 | 3.238 | 0.037 | 0.358 | 0.689 | 95.5 | 0.73 | 0.12 ±0.01 | 0.74 ± 0.07 | 0.14 ±0.08 | 0.41 ± 0.04 | Multip. | 0.07 ± 0.01 |
TOI-1807 b | 4.138 ±0.239* | 1.849 ±0.025 | 1:1 | 0.549 | 0.012 | 0.450 | 0.845 | 1486 | 1.00 | 0.07 ± 0.01 | 0.42 ±0.06 | 0.51 ±0.08 | 0.05 ± 0.01 | Dipolar | 1.20 ± 0.24 |
TOI-2257 b | 5.614 ±0.308* | 2.159 ±0.048 | 5:2 | 14.076 | 0.145 | 0.109 | 0.221 | 0.68 | 0.64 | 0.02 ±0.01 | 0.15 ± 0.09 | 0.83 ±0.10 | 1.60 ±0.40 | Multip. | 0.01 ± 0.002 |
TOI-237 b | 2.686 ±0.156* | 1.483 ± 0.046 | 1:1 | 5.436 | 0.034 | 0.066 | 0.133 | 3.6 | 0.62 | 0.12 ±0.01 | 0.72 ± 0.07 | 0.16 ±0.08 | 0.71 ± 0.07 | Multip. | 0.03 ± 0.01 |
TOI-431 c | 2.831 ±0.215 | 1.526 ±0.060 | 1:1 | 4.849 | 0.052 | 0.505 | 0.935 | 99.5 | 0.66 | 0.12 ±0.02 | 0.69 ±0.10 | 0.19 ±0.11 | 0.64 ± 0.06 | Multip. | 0.03 ± 0.01 |
TOI-451 b | 4.374 ± 0.252* | 1.910 ±0.070 | 1:1 | 1.859 | 0.029 | 0.759 | 1.388 | 778.9 | 1.00 | 0.06 ± 0.02 | 0.36 ±0.14 | 0.58 ±0.16 | 0.19 ±0.02 | Multip. | 0.04 ± 0.01 |
TOI-561 b | 1.590 ±0.208 | 1.423 ±0.038 | 1:1 | 0.447 | 0.011 | 0.732 | 1.309 | 5167 | 1.00 | 0.07 ± 0.03 | 0.44 ±0.15 | 0.49 ±0.17 | 0.04 ± 0.002 | Dipolar | 0.41 ± 0.08 |
TOI-561 d | 11.962 ±0.735 | 2.529 ± 0.075 | 1:1 | 25.620 | 0.157 | 0.710 | 1.309 | 23.4 | 0.99 | 0.05 ±0.02 | 0.27 ±0.12 | 0.68 ±0.14 | 4.44 ± 0.44 | Multip. | 0.01 ± 0.002 |
TOI-561 e | 16.003 ± 1.327 | 2.670 ±0.064 | 1:1 | 77.229 | 0.328 | 0.710 | 1.309 | 5.4 | 1.00 | 0.05 ±0.02 | 0.31 ±0.11 | 0.64 ±0.13 | 15.27 ±1.53 | Multip. | 0.01 ± 0.002 |
TOI-763 b | 9.793 ±0.452 | 2.280 ± 0.064 | 1:1 | 5.606 | 0.060 | 0.748 | 1.380 | 177.8 | 1.00 | 0.08 ±0.02 | 0.45 ±0.10 | 0.47 ±0.11 | 0.79 ± 0.08 | Multip. | 0.05 ± 0.01 |
TOI-776 b | 4.021 ±0.511 | 1.847 ±0.074 | 1:1 | 8.247 | 0.065 | 0.224 | 0.442 | 11.7 | 0.97 | 0.07 ± 0.03 | 0.40 ±0.17 | 0.53 ±0.20 | 1.12 + 0.11 | Multip. | 0.01 ± 0.002 |
TOI-776 c | 5.489 ±0.966 | 2.008 ± 0.078 | 1:1 | 15.665 | 0.100 | 0.222 | 0.442 | 5.0 | 0.88 | 0.07 ± 0.03 | 0.39 ±0.18 | 0.54 ±0.21 | 2.40 ±0.24 | Multip. | 0.01 ± 0.002 |
TOI-824 b | 18.608 ± 1.062 | 2.865 ±0.078 | 1:1 | 1.393 | 0.022 | 0.427 | 0.813 | 405.1 | 0.65 | 0.03 ± 0.02 | 0.18 ±0.10 | 0.79 ±0.12 | 0.12 ±0.01 | Dipolar | 1.68 ±0.34 |
TOI-849 b | 39.409 ± 1.473 | 3.406 ±0.047 | 1:1 | 0.766 | 0.016 | 0.751 | 1.389 | 2503 | 0.55 | 0.02 ±0.01 | 0.09 ± 0.05 | 0.89 ±0.06 | 0.04 ± 0.01 | Dipolar | 1.29 ±0.52 |
pi Men c | 4.855 ±0.471 | 2.040 ±0.028 | 1:1 | 6.268 | 0.068 | 1.087 | 1.968 | 307.3 | 0.94 | 0.04 ± 0.02 | 0.22 ±0.10 | 0.74 ±0.12 | 0.73 ± 0.07 | Multip. | 0.01 ± 0.002 |
Notes. Mp is the planetary mass normalized to the Earth mass. Those values highlighted with an asterisk have been estimated following (Chen & Kipping 2017). Rp is the planetary radius normalized to the Earth radius. S:O shows the Spin:Orbit resonance. Prot is the planetary rotational period in days, a, D2 and D3 are respectively are the semi-major axis, inner and outer boundaries of the HZ expressed in A.U. Seff is normalized mean effective flux considering orbital eccentricity. Prob. It is the probability of being water-rich rocky planet. All the planets are tidally locked. Errors in the rotational period have not been included because they are so small that they have no impact on the magnetic properties of exoplanets.
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