One of main objectives of Mars exploration in the 21st century is to search
for evidence of present or ancient life. Sedimentary processes are importa
nt on the Martian surface. However, styles of Martian sedimentation can be
different from its terrestrial counterpart in some aspects because of the r
elatively stable Martian crust and the lack of a continuous and active surf
ace hydrological cycle. Certain types of sedimentary deposits on Earth are
closely linked to biological activities, and searching for such deposits on
Mars can potentially enhance the chance of finding life or evidence of anc
ient life on the planet. A wide range of hypothesized siliciclastic and non
-siliciclastic sedimentary deposits on Mars are of particular interest for
the future exobiological exploration. Searching the substrate of sedimentar
y deposits is the preferred strategy because it is difficult to preserve or
ganic matter or geochemical evidence of biological activity in the photoche
mically active and oxidizing surface environment of Mars. (C) 2000 Elsevier
Science Ltd. All rights reserved.