Hydrocarbon nucleation and aerosol formation in Neptune's atmosphere
The present theoretical analysis of particle formation mechanisms at conditions relevant to the troposphere and stratosphere of Neptune indicates that the hydrocarbon-nucleation process in the lower stratosphere is very inefficient, because saturation ratios much greater than unity are required in the cases of aerosol formation by homogeneous, heterogeneous, and ion-induced nucleation. The latter two of these, however, should be possible on Neptune for most of the complex hydrocarbon species in question. The relative effectiveness of heterogeneous and ion-induced nucleation depends on the physical and thermodynamic properties of the species in question, condensable-species abundance, supersaturation temperatures, and the number and type of available condensation ions or nuclei.