On the stability of carbonic acid under conditions in the atmosphere of Venus

Details On the stability of carbonic acid under conditions in the atmosphere of Venus On the stability of carbonic acid under conditions in the atmosphere of Venus

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994icar..112..541k&link_type=abstract

Icarus (ISSN 0019-1035), vol. 112, no. 2, p. 541-544

Computer Science

4

Abundance, Atmospheric Composition, Carbonic Acid, Quantum Mechanics, Venus Atmosphere, Absorption Spectra, Pressure Effects, Temperature Effects, Venera Satellites, Water

Scientific paper

Results of quantum statistical mechanical calculations and thermodynamic evaluation of the structure of H2CO3 and its stability against dissociation are reported. Under temperature and pressure conditions near the surface of Venus, carbonic acid would predominatly dissociate into H2O and CO2 and, hence, could not contribute to any significant absorption there.

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