Radiative equilibrium calculations show silicate clouds (SiO2, Mg2SiO4) remain thermally stable across wide conditions while sulfide clouds (ZnS, Na2S, MnS) readily reach sublimation temperatures in upper exoplanet atmospheres.
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Radiatively Controlled Thermal Stability of High-Altitude Clouds in Exoplanetary Atmospheres
Radiative equilibrium calculations show silicate clouds (SiO2, Mg2SiO4) remain thermally stable across wide conditions while sulfide clouds (ZnS, Na2S, MnS) readily reach sublimation temperatures in upper exoplanet atmospheres.