Trace metal chloride gases from Venus's surface should condense into K2SO4, Na2SO4, and FeS2 hazes at 15.5, 9.5, and 2.4 km, matching Pioneer Venus's three haze layers.
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Prediction of sulphate hazes in the lower Venus atmosphere
Trace metal chloride gases from Venus's surface should condense into K2SO4, Na2SO4, and FeS2 hazes at 15.5, 9.5, and 2.4 km, matching Pioneer Venus's three haze layers.