“…Now that extensive vulcanism is known to exist on Mars, as well as probable thermokarst terrains (Sharp, et al, 1971;Belcher, et al, 1971) a previous suggestion (Lederberg and Sagan, 1964) that there may be locales of geothermal penetration of the subsurface permafrost layer and consequent patches of subterranean liquid water appears somewhat more plausible. It has also been suggested (Sagan at al., 1968;Farmer, 1976) that ice, deposited in soil interstices, may enter a temporary liquid phase due to the soil diffusion barrier.…”