Physics
Scientific paper
Mar 1964
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1964sci...143.1161w&link_type=abstract
Science, Volume 143, Issue 3611, pp. 1161
Physics
1
Scientific paper
The carbon dioxide pressure of the atmosphere of Venus may be controlled
by one or more of several decarbonation reactions. One of these is the
formation of carbonate-rich liquids. The pressure-temperature
equilibrium conditions of these reactions are in the range of those
proposed for the surface of Venus.
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