Chemical and physical microenvironments at the Viking landing sites.
Physical and chemical considerations permit the division of the near-surface regolith on Mars into at least six zones of distinct microenvironments. The zones are euphotic, duricrust/peds, tempofrost, permafrost, endolithic, and interfacial/transitional. Microenvironments vary significantly in temperature extremes, mean temperature, salt content, relative pressure of water vapor, UV and visible light irradiance, and exposure to ionizing radiation events (100 Mrad) and oxidative molecular species. From what is known of the chemistry of the atmosphere and regolith fines (soil), limits upon the aqueous chemistry of soil pastes may be estimated. Heat of wetting could reach 45 cal/g dry soil; initial pH is indeterminate between 1 and 10; ionic strength and salinity are predicted to be extremely high; freezing point depression is inadequate to provide quantities of liquid water except in special cases. The prospects for biotic survival are grim by terrestrial standards, but the extremes of biological resiliency are inaccessible to evaluation. Second-generation in situ experiments which will better define Martian microenvironments are clearly possible. Antarctic dry valleys are approximations to Martian conditions, but deviate significantly by at least half-a-dozen criteria.
D055598:Chemical Phenomena; D002621:Chemistry; D002980:Climate; D005118:Extraterrestrial Environment; D055593:Geological Phenomena; D005844:Geology; D008027:Light; D008834:Microclimate; D055585:Physical Phenomena; D010825:Physics; D011839:Radiation, Ionizing; D012987:Soil / Q000032:analysis; D013696:Temperature; D013997:Time Factors; D014466:Ultraviolet Rays
D012987:Soil