Ma'adim Vallis and Gusev crater (Aeolis subquadrangle of Mars) formed
a complex hydrogeologic system through time. Crater statistics over fi
ve geologic units, coupled with morphologic and geologic observations,
show that this system was active over a period ranging from 0.7 to ab
out 2 billion years. These results make the floor of Gusev crater one
of the most prominent martian depositional features. The last aqueous
sedimentary deposition could have occurred during Early Amazonian. (C)
1998 Academic Press.