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Deep valleys of Candor Chasma
15 February 2008
| Mars Express took snapshots of Candor Chasma, a valley in the northern part of Valles Marineris, as it was in orbit above the region on 6 July 2006.
The High Resolution Stereo Camera on the orbiter obtained the data in orbit number 3195, with a ground resolution of approximately 20 m/pixel. Candor Chasma lies at approximately 6° south and 290° east.
Valles Marineris is an approximately 3000-km-long canyon system on Mars. Candor Chasma, situated in its northern part, is part of a radial graben system. A graben is a feature bound by parallel normal faults, where the graben floor moves downward relative to the adjoining material. The grabens in the area were created radially, as the Tharsis bulge formed due to volcanic uplift.
Credits: ESA/ DLR/ FU Berlin (G. Neukum) | |  |  | |
| | | | | Candor Chasma context map.
Mars Express took snapshots of the region, situated in the northern part of Valles Marineris, on 6 July 2006.
The High Resolution Stereo Camera on the orbiter obtained the data in orbit number 3195, with a ground resolution of approximately 20 m/pixel. Candor Chasma lies at approximately 6° south and 290° east.
Credits: FU Berlin/ MOLA | | | | |
| | | | | Mars Express took snapshots of Candor Chasma, a valley in the northern part of Valles Marineris, as it was in orbit above the region on 6 July 2006.
The High Resolution Stereo Camera on the orbiter obtained the data in orbit number 3195, with a ground resolution of approximately 20 m/pixel. Candor Chasma lies at approximately 6° south and 290° east.
Valles Marineris is an approximately 3000-km-long canyon system on Mars. Candor Chasma, situated in its northern part, is part of a radial graben system. A graben is a feature bound by parallel normal faults, where the graben floor moves downward relative to the adjoining material. The grabens in the area were created radially, as the Tharsis bulge formed due to volcanic uplift.
Credits: ESA/ DLR/ FU Berlin (G. Neukum) | | | | |
| | | | | Mars Express took snapshots of Candor Chasma, a valley in the northern part of Valles Marineris, as it was in orbit above the region on 6 July 2006.
The High Resolution Stereo Camera on the orbiter obtained the data in orbit number 3195, with a ground resolution of approximately 20 m/pixel. Candor Chasma lies at approximately 6° south and 290° east.
Credits: ESA/ DLR/ FU Berlin (G. Neukum) | | | | |
| | | | | Mars Express took snapshots of Candor Chasma, a valley in the northern part of Valles Marineris, as it was in orbit above the region on 6 July 2006.
The High Resolution Stereo Camera on the orbiter obtained the data in orbit number 3195, with a ground resolution of approximately 20 m/pixel. Candor Chasma lies at approximately 6° south and 290° east.
Credits: ESA/ DLR/ FU Berlin (G. Neukum) | | | | |
| | | | | Mars Express took snapshots of Candor Chasma, a valley in the northern part of Valles Marineris, as it was in orbit above the region on 6 July 2006.
The High Resolution Stereo Camera on the orbiter obtained the data in orbit number 3195, with a ground resolution of approximately 20 m/pixel. Candor Chasma lies at approximately 6° south and 290° east.
Valles Marineris is an approximately 3000-km-long canyon system on Mars. Candor Chasma, situated in its northern part, is part of a radial graben system. A graben is a feature bound by parallel normal faults, where the graben floor moves downward relative to the adjoining material. The grabens in the area were created radially, as the Tharsis bulge formed due to volcanic uplift.
The steep walls of the graben (1) rise to a height of 8500 m above the floor.
They are characterised by remnant rock (small veins of rock branching from the main material) and branching gullies.
The upper part shows rugged, irregular material and appears to be a remnant of the older, basaltic plateau. In contrast, the lower part is smoother and is made up of run-off rock debris and material from larger landslides that formed a slope (2,3).
The graben floor shows flat-topped, hilly deposits (4) which rise up to 1200 m. The deposits show characteristic layering which is known as ‘Interior Layered Deposits’.
Credits: ESA/ DLR/ FU Berlin (G. Neukum) | | | | |
| | | | | Mars Express took snapshots of Candor Chasma, a valley in the northern part of Valles Marineris, as it was in orbit above the region on 6 July 2006.
The High Resolution Stereo Camera on the orbiter obtained the data in orbit number 3195, with a ground resolution of approximately 20 m/pixel. Candor Chasma lies at approximately 6° south and 290° east.
Valles Marineris is an approximately 3000-km-long canyon system on Mars. Candor Chasma, situated in its northern part, is part of a radial graben system. A graben is a feature bound by parallel normal faults, where the graben floor moves downward relative to the adjoining material. The grabens in the area were created radially, as the Tharsis bulge formed due to volcanic uplift.
Credits: ESA/ DLR/ FU Berlin (G. Neukum) | | | | |
| | | | | Mars Express took snapshots of Candor Chasma, a valley in the northern part of Valles Marineris, as it was in orbit above the region on 6 July 2006.
The High Resolution Stereo Camera on the orbiter obtained the data in orbit number 3195, with a ground resolution of approximately 20 m/pixel. Candor Chasma lies at approximately 6° south and 290° east.
This anaglyph image was calculated from the nadir and one stereo channel, stereoscopic glasses are required for viewing.
Credits: ESA/ DLR/ FU Berlin (G. Neukum) | | | | |
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