title: Petrology of Venus: Further Deducftons.
abstract: 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.
authors.forename: L S
authors.initials: LS
authors.lastname: Walter