Observations indicate that a Martian analog to the Earth's salt pans a
nd saline lakes of arid regions may have existed in crater-basins duri
ng Mars' early (Noachian) epoch. Terraced and channelized crater-basin
s point to pending of surface water as well as possible prolonged and
evolving base levels. In addition, supportive (evaporite basin) analog
s are offered for three other morphologic features of Martian crater-b
asins. An evaporite basin model for crater-basins on Mars has major im
plications for the mechanical, chemical, and even biological processes
that potentially have operated in Mars' past, and represent a spectru
m of potential mineral resources.