Stability against freezing of aqueous solutions on early Mars

  title={Stability against freezing of aqueous solutions on early Mars},
  author={Alberto G. Fair{\'e}n and Alfonso F. Davila and Luis Gago-Duport and Ricardo Amils and Christopher P. McKay},
Many features of the Martian landscape are thought to have been formed by liquid water flow and water-related mineralogies on the surface of Mars are widespread and abundant. Several lines of evidence, however, suggest that Mars has been cold with mean global temperatures well below the freezing point of pure water. Martian climate modellers considering a combination of greenhouse gases at a range of partial pressures find it challenging to simulate global mean Martian surface temperatures… 
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