The possibility that life may once have evolved on Mars is strongly linked to the availability of liquid water over long time periods. Thus, the selection of sites for exobiology exploration is related to photo-geologic evidence of water activity. Here is a table which will help you in interpreting the Viking orbiter images of the martian landscape, especially fluvial features and in judging the length of time that the water may have persisted.
Feature Duration
Shorter Longer
Channel : Straight Meandering Floodplain : Absent Broad Drainage networks : Simple Dendritic Drainage basin : Small, many divides Large, few divides Tributary : None to first order Second to higher order Stream terrace : Single level Multiple level, incised meanders Delta : Absent or small Large, multi-lobed Other : Only young, crisp Craters show various degree of featured craters present erosion
Although the Viking images are of extraordinary quality, their resolution generally does not allow us to see features as small as a football field. Nor, at this time do we have much information about surface composition. This inability to identify small geological features and to identify surface compositions of Mars limits our ability to select sites of exobiology importance. This explains the need for high resolution orbital imaging in future missions. A minimum resolution of 75 m is required to recognize most geological features critical for site selection. Even better resolution may be required to recognize such potentially exciting features as deposits from ancient hydrothermal springs.
Here are some clues to give priority levels to sites for exobiology exploration.
The weighting factors used to score each feature include :
Features/deposits Weighting factors
Visibility Process Value for of feature uniqueness Exobiology (0-3) (1-3) (1-3)
Fluvial Dendritic drainage networks Channel widens downslope Floodplains Channel meandering Stream terraces Visible layering Score subtotals
Lacustrine Basin fed by channels Shoreline terraces Delta at stream mouth Lava/aoelian cover Channels on basin floor Impact craters Score subtotals
Thermal spring Simple channel morphology Channel head a point source Channels branch downslope Associated with volcanic center Possible subsurface heat source Score subtotals
Ground ice Polygonal terrain Irregular depressions Mounds (possible pingos) Lobate crater ejecta Debris flows (possible rock glaciers) Laminated terrain Latitude Score Subtotals
Total Score
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