Table B.3
Results for dry 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 | Roℓ | Regime | ℳ/ℳ⊕ |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| GJ 1252 b | 2.119 ±0.311 | 1.190 ± 0.042 | 1:1 | 0.518 | 0.009 | 0.144 | 0.282 | 234.7 | 0.94 | 0.47 ± 0.20 | 0.53 ± 020 | 0.03 ± 0.01 | Dipolar | 3.50 ± 1.40 |
| GJ 3473 b | 1.965 ±0.135 | 1.252 ± 0.025 | 1:1 | 1.198 | 0.016 | 0.124 | 0.245 | 59.2 | 0.54 | 0.15 ±0.10 | 0.85 ±0.10 | 0.14 ± 0.03 | Multip. | 0.05 ± 0.02 |
| GJ 357 b | 1.884 ±0.171 | 1.202 ± 0.043 | 1:1 | 3.931 | 0.034 | 0.129 | 0.252 | 13.5 | 0.77 | 0.29 ± 0.16 | 0.71 ± 0.16 | 0.47 ± 0.09 | Multip. | 0.04 ± 0.02 |
| GJ 367 b | 0.546 ± 0.045 | 0.718 ± 0.031 | 1:1 | 0.322 | 0.007 | 0.182 | 0.343 | 588.2 | 1.00 | 0.92 ± 0.015 | 0.08 ± 0.015 | 0.01 ± 0.002 | Dipolar | 0.86 ±0.38 |
| HD 15337 b | 7.547 ± 0.607 | 1.640 ± 0.035 | 1:1 | 4.756 | 0.053 | 0.644 | 1.201 | 160.9 | 1.00 | 0.48 ± 0.10 | 0.52 ±0.10 | 0.37 ± 0.07 | Multip. | 0.33 ±0.15 |
| HD 213885 b | 8.835 ±0.379 | 1.744 ± 0.030 | 1:1 | 1.008 | 0.020 | 1.067 | 1.939 | 3420 | 1.00 | 0.39 ± 0.07 | 0.61 ± 0.07 | 0.07 ± 0.01 | Dipolar | 12.59 ± 1.50 |
| HD 21749 c | 0.670 ± 0.038* | 0.886 ±0.031 | 1:1 | 7.790 | 0.069 | 0.458 | 0.823 | 41.4 | 0.84 | 0.36 ± 0.16 | 0.64 ± 0.16 | 1.03 ± 0.21 | Multip. | 0.01 ± 0.002 |
| L 168-9 b | 4.600 ± 0.323 | 1.390 ±0.052 | 1:1 | 1.402 | 0.021 | 0.259 | 0.512 | 157.7 | 1.00 | 0.64 ± 0.13 | 0.36 ±0.13 | 0.04 ± 0.01 | Dipolar | 9.11 ± 1.09 |
| LHS 1478 b | 2.330 ±0.116 | 1.243 ± 0.029 | 1:1 | 1.950 | 0.019 | 0.088 | 0.173 | 20.3 | 1.00 | 0.40 ±0.11 | 0.60 ±0.11 | 0.15 ±0.03 | Multip. | 0.17 ± 0.08 |
| LHS 1678 b | 0.350 ± 0.000 | 0.696 ± 0.025 | 3:2 | 0.573 | 0.012 | 0.130 | 0.242 | 98.0 | 1.00 | 0.60 ± 0.13 | 0.40 ± 0.13 | 0.05 ± 0.01 | Dipolar | 0.64 ±0.03 |
| LHS 1678 c | 1.400 ± 0.000 | 0.983 ± 0.037 | 1:1 | 3.694 | 0.032 | 0.124 | 0.242 | 13.9 | 1.00 | 0.77 ± 0.12 | 0.23 ± 0.12 | 0.15 ±0.03 | Multip. | 0.14 ± 0.01 |
| LHS 1815 b | 1.356 ± 0.077* | 1.085 ± 0.036 | 1:1 | 3.814 | 0.038 | 0.205 | 0.396 | 27.6 | 0.96 | 0.34 ± 0.16 | 0.66 ± 0.16 | 0.42 ± 0.08 | Multip. | 0.04 ± 0.02 |
| LHS 3844 b | 2.295 ± 0.127* | 1.302 ±0.012 | 1:1 | 0.463 | 0.006 | 0.054 | 0.108 | 71.2 | 0.95 | 0.17 ± 0.08 | 0.83 ±0.08 | 0.04 ± 0.01 | Dipolar | 1.53 ± 0.69 |
| LP 791-18 b | 1.508 ± 0.086* | 1.093 ± 0.061 | 1:1 | 0.948 | 0.010 | 0.046 | 0.093 | 20.8 | 0.79 | 0.44 ± 0.23 | 0.54 ± 0.23 | 0.07 ± 0.01 | Dipolar | 2.01 ± 0.96 |
| LTT 3780 b | 2.681 ± 0.257 | 1.323 ± 0.040 | 1:1 | 0.768 | 0.012 | 0.126 | 0.250 | 103.8 | 0.86 | 0.29 ± 0.15 | 0.71 ±0.15 | 0.06 ± 0.01 | Dipolar | 2.97 ± 1.34 |
| TOI-1235 b | 5.992 ± 0.342 | 1.677 ± 0.038 | 1:1 | 3.445 | 0.038 | 0.294 | 0.577 | 60.1 | 0.72 | 0.17 ± 0.10 | 0.83 ± 0.10 | 0.42 ± 0.08 | Multip. | 0.10 ±0.04 |
| TOI-1444 b | 3.871 ±0.408 | 1.397 ± 0.037 | 1:1 | 0.470 | 0.012 | 0.760 | 1.388 | 4838 | 1.00 | 0.46 ± 0.14 | 0.54 ± 0.14 | 0.03 ± 0.01 | Dipolar | 6.59 ± 1.32 |
| TOI-1749 c | 14.00 ± 0.00 | 2.069 ± 0.040 | 1:1 | 4.493 | 0.044 | 0.260 | 0.509 | 34.7 | 0.58 | 0.14 ± 0.08 | 0.86 ± 0.08 | 0.57 ±0.11 | Multip. | 0.15 ±0.01 |
| TOI-178 b | 1.589 ± 0.196 | 1.141 ± 0.039 | 1:1 | 1.915 | 0.026 | 0.368 | 0.689 | 192.6 | 0.67 | 0.31 ±0.17 | 0.69 ± 0.17 | 0.20 ± 0.04 | Multip. | 0.07 ± 0.03 |
| TOI-2285 b | 19.50 ±0.00 | 1.740 ± 0.046 | 3:2 | 18.180 | 0.137 | 0.168 | 0.338 | 1.6 | 1.00 | 0.92 ± 0.06 | 0.08 ± 0.06 | 0.48 ± 0.10 | Multip. | 0.57 ± 0.03 |
| TOI-270 b | 1.677 ± 0.109 | 1.198 ± 0.021 | 1:1 | 3.360 | 0.032 | 0.144 | 0.281 | 19.0 | 0.56 | 0.15 ± 0.09 | 0.85 ± 0.09 | 0.46 ±0.09 | Multip. | 0.02 ±0.01 |
| TOI-431 b | 3.069 ±0.202 | 1.280 ± 0.023 | 1:1 | 0.490 | 0.011 | 0.504 | 0.935 | 2112 | 1.00 | 0.57 ± 0.08 | 0.43 ± 0.08 | 0.02 ± 0.004 | Dipolar | 5.86 ± 1.17 |
| TOI-540 b | 0.699 ± 0.039* | 0.899 ± 0.028 | 1:1 | 1.239 | 0.012 | 0.062 | 0.120 | 23.1 | 0.90 | 0.35 ±0.15 | 0.65 ± 0.15 | 0.12 ±0.02 | Dipolar | 0.75 ± 0.30 |
| TOI-700 b | 1.143 ± 0.065* | 1.034 ±0.036 | 1:1 | 9.977 | 0.067 | 0.156 | 0.304 | 5.0 | 0.95 | 0.34 ± 0.16 | 0.66 ± 0.16 | 1.30 ±0.26 | Multip. | 0.02 ±0.01 |
| TOI-700 d | 1.620 ± 0.092* | 1.144 ± 0.035 | 1:1 | 37.425 | 0.163 | 0.155 | 0.304 | 0.87 | 0.98 | 0.33 ±0.15 | 0.67 ± 0.15 | 5.66 ± 0.94 | 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:0 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 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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