2022A&A...658A.180H


Query : 2022A&A...658A.180H

2022A&A...658A.180H - Astronomy and Astrophysics, volume 658A180-180 (2022/2-1)

The atmospheres of rocky exoplanets. II. Influence of surface composition on the diversity of cloud condensates.

HERBORT O., WOITKE P., HELLING C. and ZERKLE A.L.

Abstract (from CDS):

Clouds are an integral part of planetary atmospheres, with most planets hosting clouds. Understanding not only the formation, but also the composition of clouds, is crucial to understand future observations. As observations of the planet's surface will remain very difficult, it is essential to link the observable high atmosphere gas and cloud composition to the surface conditions. We present a fast and simple chemical equilibrium model for the troposphere of rocky exoplanets, which is in chemical and phase equilibrium with the crust. The hydrostatic equilibrium atmosphere is built from bottom to top. In each atmospheric layer, chemical equilibrium is solved and all thermally stable condensates are removed, depleting the atmosphere above in the effected elements. These removed condensates build an upper limit for cloud formation and can be separated into high and low temperature condensates. The most important cloud condensates for 1000 K ≥ Tgas ≥ 400 K are KCl[s], NaCl[s], FeS[s], FeS2[s], FeO[s], Fe2O3[s], and Fe3O4[s]. For Tgas ≥ 400 K H2O[l,s], C[s], NH3[s], NH4Cl[s], and NH4SH[s] are thermally stable, while for even lower temperatures of Tgas ≤ 150 K CO2[s], CH4[s], NH3[s], and H2S[s] become stable. The inclusion of clouds with trace abundances results in the thermal stability of a total of 72 condensates for atmospheres with different surface conditions (300 K ≤ Tsurf ≤ 1000 K and psurf = 1 bar, 100 bar). The different cloud condensates are not independent of each other, but follow sequences of condensation, which are robust against changes in crust composition, surface pressure, and surface temperature. Independent of the existence of water as a crust condensate, H2O[l,s] is a thermally stable cloud condensate for all investigated elemental abundances. However, the water cloud base depends on the hydration level of the crust. Therefore, the detection of water condensates alone does not necessarily imply stable water on the surface, even if the temperature could allow for water condensation.

Abstract Copyright: © ESO 2022

Journal keyword(s): planets and satellites: terrestrial planets - planets and satellites: atmospheres - planets and satellites: composition - planets and satellites: surfaces - astrochemistry

Simbad objects: 56

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Number of rows : 56
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 TOI-178c Pl 00 29 12.3029193648 -30 27 13.466857032           ~ 29 0
2 TOI-178b Pl 00 29 12.3029193648 -30 27 13.466857032           ~ 29 0
3 NAME G 268-38b Pl 00 44 59.3309137511 -15 16 17.542839990           ~ 237 0
4 NAME G 245-61b Pl 02 57 18.2595506687 +76 33 11.253543067           ~ 41 0
5 HD 21749c Pl 03 26 59.2226447548 -63 29 56.762928961           ~ 14 0
6 NAME PM J03455+3706b Pl 03 45 33.6408895592 +37 06 43.999247912           ~ 34 0
7 NAME LP 415-17d Pl 04 21 52.4852745864 +21 21 12.937879152           ~ 10 0
8 NAME LP 415-17b Pl 04 21 52.4852745864 +21 21 12.937879152           ~ 12 0
9 NAME L 231-32b Pl 04 33 39.7200127728 -51 57 22.435373160           ~ 49 0
10 NAME L 181-1b Pl 06 04 20.3587517402 -55 18 46.838313863           ~ 16 0
11 TOI-700d Pl 06 28 23.2285331376 -65 34 45.520447908           ~ 64 0
12 CoRoT-7b Pl 06 43 49.4690164104 -01 03 46.826642700           ~ 422 1
13 NAME G 50-16b Pl 08 02 22.8829177661 +03 20 19.691170937           ~ 30 0
14 * rho01 Cnc e Pl 08 52 35.8111044043 +28 19 50.954994470           ~ 682 1
15 NAME L 678-39b Pl 09 36 01.6372169407 -21 39 38.877606712           ~ 86 0
16 LSPM J1008+6916b Pl 10 08 51.8069885952 +69 16 35.560317504           ~ 44 0
17 NAME G 162-44b Pl 10 18 35.1372361341 -11 43 00.243355403           ~ 44 0
18 K2-239b Pl 10 42 22.6342566960 +04 26 28.885936560           ~ 13 0
19 K2-239c Pl 10 42 22.6342566960 +04 26 28.885936560           ~ 14 0
20 K2-239d Pl 10 42 22.6342566960 +04 26 28.885936560           ~ 14 0
21 GALEX J104341.5+085558 WD* 10 43 41.5313708256 +08 55 58.340933400           DAZ 70 0
22 K2-3d Pl 11 29 20.3917077216 -01 27 17.281697868           ~ 57 0
23 K2-3c Pl 11 29 20.3917077216 -01 27 17.281697868           ~ 49 0
24 K2-42b Pl 11 46 39.7706942640 -05 10 18.871289040           ~ 8 0
25 NAME LP 961-53b Pl 11 54 18.3921193416 -37 33 09.837719244           ~ 47 0
26 K2-158c Pl 11 59 45.5948191776 -05 43 18.179438520           ~ 4 0
27 K2-252b Pl 12 09 27.9281902224 -08 18 34.261833348           ~ 4 0
28 K2-244b Pl 12 13 52.5346690920 -03 49 54.824136744           ~ 8 0
29 K2-254b Pl 12 22 12.1833994896 -04 43 02.058708432           ~ 3 0
30 K2-228b Pl 12 29 10.7449406112 -06 50 03.337215612           ~ 6 0
31 K2-257b Pl 12 33 06.8370164304 -01 57 11.391970752           ~ 8 0
32 K2-154b Pl 12 36 00.3633247176 -02 40 10.103369268           ~ 5 0
33 K2-224b Pl 12 38 48.9817892712 -10 03 38.340223812           ~ 5 0
34 Wolf 437b Pl 12 47 56.6245693190 +09 45 05.035666747           ~ 95 0
35 NAME Proxima Centauri b Pl 14 29 42.9461331854 -62 40 46.164680672           ~ 445 0
36 K2-240c Pl 15 11 23.9071822656 -17 52 30.795194136           ~ 9 0
37 * nu.02 Lup b Pl 15 21 48.1499105161 -48 19 03.469906910           ~ 49 1
38 BD-19 4086b Pl 15 21 55.1983073496 -20 13 53.990924232           ~ 8 0
39 NAME G 139-21b Pl 17 15 18.9339850845 +04 57 50.066612336           ~ 845 1
40 Kepler-62c Pl 18 52 51.0518497680 +45 20 59.399622996           ~ 33 1
41 BD+38 3583b Pl 19 25 40.3885404552 +38 40 20.413186860           ~ 121 0
42 Kepler-167d Pl 19 30 38.0261896920 +38 20 43.437246900           ~ 30 0
43 Kepler-114c Pl 19 36 29.1357624552 +48 20 58.291722816           ~ 38 0
44 Kepler-114b Pl 19 36 29.1357624552 +48 20 58.291722816           ~ 32 0
45 Kepler-1659c Pl 19 53 29.7223329192 +40 37 06.379732380           ~ 27 0
46 NAME L 119-213b Pl 22 41 58.1171811377 -69 10 08.320741850           ~ 146 0
47 TRAPPIST-1e Pl 23 06 29.3684948589 -05 02 29.037301866           ~ 384 0
48 TRAPPIST-1 LM* 23 06 29.3684948589 -05 02 29.037301866     18.798 16.466 14.024 M7.5e 1306 0
49 TRAPPIST-1c Pl 23 06 29.3684948589 -05 02 29.037301866           ~ 282 0
50 TRAPPIST-1d Pl 23 06 29.3684948589 -05 02 29.037301866           ~ 263 0
51 TRAPPIST-1b Pl 23 06 29.3684948589 -05 02 29.037301866           ~ 380 0
52 CD-60 8051b Pl 23 20 07.5245143451 -60 03 54.644648069           ~ 67 0
53 BD-02 5958c Pl 23 27 04.8376907739 -01 17 10.582653030           ~ 35 0
54 BD-02 5958b Pl 23 27 04.8376907739 -01 17 10.582653030           ~ 78 0
55 BD-02 5958d Pl 23 27 04.8376907739 -01 17 10.582653030           ~ 82 0
56 TOI-237b Pl 23 32 58.2700309449 -29 24 54.190916756           ~ 15 0

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