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Table 5

Atmospheric parameters retrieved for the planets whose composition can accommodate a water-dominated atmosphere (see text).

Planet Tirr (K) T300 (K) zatm (km) Ab
K2-138 b 1291 4110 ± 44 932 ± 151 0.213 ± 0.001
K2-138 c 1125 3900 ± 23 711 ± 103 0.214 ± 0.002
K2-138 d 978 3614 ± 56 635 ± 84 0.218 ± 0.002
K2-138 e 850 3383 ± 39 673 ± 90 0.231 ± 0.001
K2-138 f 735 3396 ± 116 1483 ± 546 0.260 ± 0.004
TOI-178 c 873 3344± 33 500 ± 60 0.226 ± 0.001
TOI-178 d 691 3254 ± 45 1181 ± 224 0.264 ± 0.004
TOI-178 e 600 2930 ± 31 690.7 ± 133 0.225 ± 0.018
TOI-178 f 521 2610 ± 23 368 ± 60 0.298 ± 0.007
Kepler-11 b 953 3697 ± 133 840 ± 313 0.221 ± 0.005
Kepler-102 e 694 2947 ± 29 360 ± 55 0.243 ± 0.004
Kepler-102 f 501 2784 ± 102 837 ± 290 0.347 ± 0.013
Kepler-80 b 750 3344± 33 1133 ± 148 0.253 ± 0.002
Kepler-80 c 679 3219 ± 29 1128±114 0.266 ± 0.003

Notes. These parameters are the equilibrium temperature assuming a null albedo (Tirr), the atmospheric temperature at 300 bar (T300), the thickness of the atmosphere from the 300 bar to 20 mbar (zatm), and the planetary Bond albedo (AB).

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