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Table 7

Connection between cloud condensates in the upper atmosphere and the crust composition as in Table 6, but for 700 < Tsurf < 1000 K.

Tsurf [K] Planet MP [M ] RP [R ] Teq [K] Ref. C[s] NH4Cl[s] S2[s] FeS[s] FeS2[s] KCl[s] NaCl[s] AlF3[s] Fe2O3[s]
700–750 GJ 143 c 3.69919 0.89 ± 0.07 703 ± 24 (19) CI BSE CC Earth
K2 155 b 4.7 ± 0.4 1.81 ± 0.16 708 ± 40 (5) PWD MORB BSE12 PWD BSE
K2 154 b 6.8 ± 2.5 1.99 ± 0.21 715 ± 9 (17) BSE15
GJ 9827 c 1.9 ± 0.5 1.20 ± 0.05 722 ± 25 (20) MORB
Kepler-114 b 7 ± 4 1.26 ± 0.14 722.0 (15) PWD CI
Archean
Solar

750–800 KOI-1599.01 4.6 ± 0.3 1.9 ± 0.4 755.0 (21) PWD MORB BSE CC Earth
GJ 3473 b 1.9 ± 0.3 1.264 ± 0.006 773 ± 16 (22) BSE12 PWD BSE
TOI-1235 b 5.9 ± 0.7 1.69 ± 0.08 775 ± 13 (23) BSE15
K2 257 b 0.7 ± 0.5 0.83 ± 0.06 789 ± 14 (17) MORB
K2 254 b 5.2 ± 2.6 1.63 ± 0.28 791 ± 26 (16) PWD CI
Archean
Solar

800–900 L 168-9 b 4.6 ± 0.6 1.390 ± 0.09 820 ± 160 (24) PWD MORB PWD CI CC BSE MORB BSE Earth
TOI-178 c 4.8 ± 0.7 1.67 ± 0.11 873 ± 18 (25) PWD BSE BSE12
LTT 3780 b 3.1 ± 0.6 1.33 ± 0.08 892.0 (26) BSE15
Archean
Solar

900–1000 HD 136352 b 4.6 ± 0.5 1.48 ± 0.06 911 ± 18 (27) PWD MORB PWD BSE BSE MORB BSE Earth CC
K2 228 b 3.2 ± 1.7 1.21 ± 0.10 914 ± 14 (17) BSE12
TOI-1634 b 4.9 ± 0.7 1.79 ± 0.09 924 ± 22 (28) BSE15
K2 158 c 3.6 ± 2.0 1.28 ± 0.13 948 ± 13 (17) PWD BSE
K2 224 b 4.9 ± 2.4 1.56 ± 0.16 1002 ± 11 (17) PWD CI
Kepler-93 b 4.5 ± 0.9 1.57 ± 0.11 1037.0 (29) Archean
K2-233 b 3 ± 3 1.40 ± 0.07 1040 ± 27 (30) Solar
TOI-178 b 1.5 ± 0.5 1.15 ± 0.08 1040 ± 22 (25)
GJ 9827 b 4.9 ± 0.4 1.53 ± 0.06 1040 ± 40 (20)

Notes. The listed confirmed planets are all transiting and have planetary masses of MP < 8 M, planetary radii of RP < 2 R and equilibrium temperatures of 750 K < Teq < 1050 K. For these planets, we assume Teq = Tsurf and a surface pressure of psurf = 1 bar. The temperature ranges are determined by comparable cloud condensate composition in the upper atmosphere as shown in Fig. 4.

References.(5) Hirano et al. (2018); (16) Batalha et al. (2013); (17) Livingston et al. (2018); (19) Dragomir et al. (2019); (20) Niraula et al. (2017); (21) Panichi et al. (2019); (22) Kemmer et al. (2020); (23) Bluhm et al. (2020); (24) Astudillo-Defru et al. (2020); (25) Leleu et al. (2021); (26) Cloutier et al. (2020); (27) Kane et al. (2020); (28) Cloutier et al. (2021); (29) Ballard et al. (2014); (30) Lillo-Box et al. (2020).

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