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Table 4

Internal heat fluxes, melting, and terran and ocean probabilities of planets.

Planet Ftid,W m−2 Frad,W m−2 P melt, % Pterran, % Pocean, %
Ross 128 b 98 71 99.93 98.65
Teegardens b 98 45 100.00 98.45
Proxima Centauri b 98 16 100.00 98.16
GJ 1061 d 99 65 96.61 96.27
TRAPPIST-1 d 95 91 100.00 95.91
GJ 1061 c 99 88 93.88 93.77
Teegardens c 92 84 100.00 92.84
TRAPPIST-1 e 87 56 100.00 87.56
TOI-1452 b 75 03 100.00 75.03
TOI-700 d 93 52 73.67 68.89
Kepler-296 e 84 96 77.41 65.77
Kepler-1649 b 58 18 88.08 51.25
Kepler-186f 70 35 69.34 48.78
K2-72 e 91 67 46.59 42.71
Kepler-296 f 70 11 60.03 42.09
TRAPPIST-1 f 41 90 100.00 41.90
GJ 273 b 93 79 44.00 41.27
GJ 667 C e 90 39 30.42 27.50
GJ 667 C f 91 61 29.43 26.96
Kepler-1229 b 89 51 28.49 25.50
TRAPPIST-1 g 21 88 100.00 21.88
Kepler-442 b 77 61 27.49 21.34
K2-3 d 92 94 22.66 21.06
Kepler-1652b 68 64 13.00 8.92
K2-288 B b 90 41 6.30 5.70
Kepler-452 b 27 21 17.23 4.69
Kepler-62 f 14.31 24.01 3.44
Kepler-62 e 0 28 7.82 0.02

Notes. Median values for tidal and radiogenic heat flux at the rock-HPP boundary are summarized for each planet. The first and third quartiles are show in the lower and upper index of the median value, respectively. Melting probabilities (Pmelt) are shown in the fourth column. The Pterran column shows the probability of each planet having a rocky composition based on its measured and generated masses and radii. The values for the ocean probabilities (Pocean) are shown in the last column.

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