A computer-generated perspective view of Reull Vallis was created
using data obtained from the High-Resolution Stereo Camera (HRSC) on
ESA’s Mars Express. Credit and Copyright: ESA/DLR/FU Berlin (G. Neukum)
So, is this really an ancient river?
High-Resolution Stereo Camera image of Reul Vallis taken on May 14,
2012 by ESA’s Mars Express. Credit: ESA/DLR/FU Berlin (G. Neukum)
There are various theories as to how it may have formed, however. Some scientists say that this feature may have been created quickly in a sudden deluge or runoff event, as the entire system look like stream beds cut by sudden runoff in desert regions on the Earth.
Reull Vallis in context. Credit: NASA MGS MOLA Science Team.
There is also evidence of deposits of volatiles in the walls of the channel that could be ice.
In the wider context image above, the tributary intersecting the main channel appears to be part of a forking of the main valley into two distinct branches further upstream before merging back into a single main valley.
The right (northern) part of the main image is dominated by the Promethei Terra Highlands with their high and soft-rounded mountains shown in these images, rising around 2500 m above the surrounding flat plains.
The perspective view below shows one of these mountains with nearby sediment-filled impact craters:
This
computer-generated perspective view shows part of the Promethei Terra
highlands adjacent to Reull Vallis. Credit: ESA/DLR/FU Berlin (G.
Neukum)
And so it appears Reull Vallis provides evidence of past water on Mars. And if so, it means that the planet’s climate has changed dramatically since these features were formed between 3.5 billion and 1.8 billion years ago.
One of the first images taken by Mars Express in 2004 of Reull Vallis. Credit: Credit: ESA/DLR/FU Berlin (G. Neukum)
INFO/SOURCE : http://www.lpi.usra.edu/meetings/lpsc97/pdf/1355.PDF
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