Can a time-stratigraphic classification system be developed for Venus?

Mathematics – Logic

Scientific paper

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Classifications, Geomorphology, Meteorite Craters, Planetary Evolution, Planetary Geology, Stratigraphy, Venus (Planet), Venus Surface, Cratering, Landforms, Magellan Spacecraft (Nasa), Radar Data, Radar Imagery

Scientific paper

Magellan radar images reveal that Venus' exposed geologic record covers a relatively short and recent time span, as indicated by the low density of impact craters across the planet. Therefore, because impact cratering in itself will not be a useful tool to define geologic ages on Venus, it was questioned whether a useful stratigraphic scheme can be developed for the planet. We believe that a venusian stratigraphy is possible and that it can be based on the following: (1) an examination of the rationale and methods that have been used to develop such schemes for the other planets; and (2) what can be gleaned from Magellan and other datasets of Venus.

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