Possible configuration of ancient oceans on Mars: In this topographic portrayal of Mars, above, the northern
lowlands are occupied by an ocean (blue) whose shoreline is placed at the
position of
Contact 2, the line that Parker and co-workers interpreted as an ancient
shoreline. Thus, this view shows Mars as it might have looked mid-way
through its history according to the oceans hypothesis. The Tharsis
region, with numerous very large shield volcanoes is seen in the central
part of the globe. In the upper right, many channels flow into the northern
lowlands at Chryse Planitia. In this topographic portrayal of Mars, above, giant
channels emerge from the Tharsis region (left), Valles Marineris (bottom),
and the ancient heavily
cratered terrain (right), and flow down slope into the northern lowlands in
Chryse Planitia (center). The ancient shoreline proposed by Parker and
co-workers is at the position where the channels change from heavy scouring
of the background terrain into smooth terrain typical of the northern
lowlands, suggesting that they once flowed into a standing body of water,
or ocean, as portrayed in the blue area here. |