Is CO2 capable to keeping early Mars warm?

One of the goals of NASA's Exobiology Research Program is to determine whether life exists today on Mars (unlikely) or whether it might have existed there at some time in the past (more likely). Speculation about extinct life is driven by the observation of channels on the Martian surface, thought to indicate the past presence of liquid water and, hence, the existence of a warmer climate. Current thinking suggests that such a climate could have been maintained if early Mars had a dense CO2 atmosphere with a surface pressure of 1 to 5 bars. One of the phenomena that Martian climate modelers have not looked at very carefully is the process of CO2 condensation. Reexamination of some of my own calculations indicates that condensation should occur at high altitudes in some high-CO2, Martian atmospheres, particularly those in which the solar constant is set to its initial main sequence value (about 70 percent of present. CO2 condensation should affect the surface temperature in two ways: (1) if it occurs in the convective lower atmosphere, condensation will reduce the magnitude of the greenhouse effect by decreasing the lapse rate; and (2) condensation at any altitude will produce clouds, which can either warm or cool the climate depending on their altitude and optical depth. Preliminary calculations with a 1-D, radiative-convective climate model indicate that the lapse rate change is substantial for low solar luminosity models. Other aspects of this study are discussed.