Mamers Vallis

Scaled Image

Image Credit: NASA/JPL/ASU

About this image

This sinuous channel begins at the edge of Cerulli Crater in northern Arabia and snakes its way across 1000 km of cratered highlands before reaching Deuteronilus Mensae at the boundary of the northern lowlands. The fluid that carved the channel, either lava or water, flowed from the bottom of this scene to the top. The quasi-streamlined features on the channel floor may have nothing to do with flow and instead may be due to a permafrost creep process.

Please see the THEMIS Data Citation Note for details on crediting THEMIS images. 

Context

Image ID: 
V05055010 (View data in Mars Image Explorer)
31.287
19.091
5055
2003-02-03 10:37
Fri, 2003-02-21
VIS
1024 pixels (19 km)
3648 pixels (67 km)
0.01862 km/pixel
0.018755 km/pixel

Downloads

PNG | JPEG (high res) | JPEG (reduced res) | PDF | TIFF