Mars Express image browser
Click on the flags on the Martian surface to see images from ESA's Mars Express.
ARKIVERAT INNEHÅLL
14 JUL. 2008
Publiceringsdatum
8338
Visningar
A 4000-m-high cliff marks the edge of the source area of Kasei Valles in its western part. Gigantic water falls may have once plunged over these cliffs on to the valley floor. The original shoreline is still partially visible. The remarkably smooth valley floor was later flooded by basaltic lava.
Images acquired in different orbits were combined to create the image mosaics, the map, as well as the colour-coded elevation model.
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The colour scenes have been derived from the three HRSC-colour channels and the nadir channel. The perspective views have been calculated from the digital terrain model derived from the stereo channels.
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The anaglyph image was calculated from the nadir and one stereo channel. The black and white high resolution images were derived from the nadir channel, which provides the highest level of detail.
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Echus Chasma
The High-Resolution Stereo Camera (HRSC) on board ESA’s Mars Express has returned images of Echus Chasma, one of the largest water source regions on the Red Planet.
Echus Chasma, page two
A 4000-m-high cliff marks the edge of the source area of Kasei Valles in its western part. Gigantic water falls may have once plunged over these cliffs on to the valley floor. The original shoreline is still partially visible. The remarkably smooth valley floor was later flooded by basaltic lava.
Crater in martian valley Mamers Valles
The High-Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images of a region at the end of Mamers Valles, a long, winding valley. The focus is on a circular depression that contains a crater.
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HRSC at DLR
Behind the lens...
This is the camera behind the stunning European imagery from Mars. The High Resolution Stereo Camera on ESA’s Mars Express is now mapping most of the Martian surface with unprecedented detail.
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