Comparison of molecular partial pressures computed by GGCHEM (solid lines) to the results by Sharp & Huebner (1990, dotted lines). Calculations are based on the solar element abundances listed in Sharp & Huebner (1990) for a constant pressure of p = 0.5 mbar. The shown elements are chosen to match Fig. 1 in Sharp & Huebner (1990). Upper panel: GGCHEM only uses the molecules and condensates selected by Sharp & Huebner (1990) and applies their thermo-chemical data. Lower panel: GGCHEM uses all molecules and condensates found in its own database and uses its own thermo-chemical data. The agreement is very good. The only visible difference is in FeS, which is slightly depleted in the lower panel.