NH4SH and cloud cover in the atmospheres of the giant planets

Details NH4SH and cloud cover in the atmospheres of the giant planets NH4SH and cloud cover in the atmospheres of the giant planets

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991kfnt....7...58i&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 7, Jan.-Feb. 1991, p. 58-63. In Russian.

Physics

Ammonium Sulfates, Cloud Cover, Gas Giant Planets, Planetary Atmospheres, Aqueous Solutions, Cloud Physics, Reaction Kinetics

Scientific paper

The probability of the formation of NH4SH and (NH4)2S is examined on the basis of the Le Chatelier principle. It is shown that it is very doubtful if NH4SH can be created in the atmospheres of the giant planets in quantities sufficient for cloud formation. Thus (NH4)2S is considered as a more likely candidate for cloud formation in the atmospheres of these planets, inasmuch as the conditions for its production there are more favorable.

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