Atmospheres of Venus-like Planets: Stability Constraints on Mineral Reaction Buffers

Details Atmospheres of Venus-like Planets: Stability Constraints on Mineral Reaction Buffers Atmospheres of Venus-like Planets: Stability Constraints on Mineral Reaction Buffers

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2146t&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2146

Computer Science

Scientific paper

The composition of Venus’ atmospphere (and those of similar
exoplanets) might be buffered by chemical reactions with surface
materials. However, many such reactions cannot act as buffers in an
atmosphere that follows a dry adiabatic lapse rate.

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