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|  |  |  |  | | | |  | Perspective view of Echus Chasma | | Echus Chasma, page two
14 July 2008 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.
 | | | Echus Chasma, perspective view |
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. Echus Chasma, nadir view 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. Perspective view of Echus Chasma Perspective view of Echus Chasma Echus Chasma in 3-D Back to page one | |
|  | Mars Express image browser Related articles Echus ChasmaCrater in martian valley Mamers VallesHebes Chasma, a trough in the Grand Canyon of MarsIcy Promethei PlanumDeep valleys of Candor ChasmaESA presents Mars in 3DTraces of the martian past in the Terby craterNoctis Labyrinthus, labyrinth of the nightHummocky and shallow Maunder craterThe mysterious ridges at the mouth of Tiu VallesImpact Craters in Tyrrhena TerraTectonic signatures at Aeolis MensaeRelated links High Resolution Stereo CameraBehind the lens...Frequently asked questionsFor specialists ESA Planetary Science archive (PSA)NASA Planetary Data SystemHRSC data viewer
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