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Chemistry and thermodynamics of sulfur on Venus
Author(s) -
Young A. T.
Publication year - 1979
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/gl006i001p00049
Subject(s) - venus , sulfur , atmosphere of venus , stratosphere , astrobiology , chemistry , sulfur cycle , atmospheric chemistry , photochemistry , atmospheric sciences , geology , physics , organic chemistry , ozone
While photochemical reactions convert SO 2 to H 2 SO 4 and remove O 2 from the Venus stratosphere, thermochemical reactions near the surface probably make the SO 2 , regenerate CO 2 from photolytic CO, and produce free sulfur. Venera data suggest a light drizzle of liquid sulfur above 18 km, and several per cent of sulfur vapor below.

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