Observations permitted by the newly acquired Mars Observer Laser Altimeter
data have revealed a system of gigantic valleys northwest of the huge Marti
an shield volcano, Arsia Mons, in the western hemisphere of Mars (northwest
ern slope valleys (NSVs)). These features, which generally correspond spati
ally to gravity lows, are obscured by veneers of materials including volcan
ic lava flows, air fall deposits, and eolian materials. Geologic investigat
ions of the Tharsis region suggest that the system of gigantic valleys pred
ates the construction of Arsia Mons and its extensive associated lava flows
of mainly late Hesperian and Amazonian age and coincides stratigraphically
with the early development of the outflow channels that debouch into Chrys
e Planitia. Similar to the previously identified outflow channels, which is
sued tremendous volumes of water into topographic lows such as Chryse Plani
tia, the NSVs potentially represent flooding of immense magnitude and, as s
uch, a source of water for a northern plains ocean.