Iani Chaos
| Chaotisches Terrain auf dem Mars | ||
|---|---|---|
| Iani Chaos | ||
 (c) ESA/DLR/FU Berlin (G. Neukum), CC BY-SA 3.0 igo | ||
| ||
| Position | 2° 11′ S, 17° 2′ W | |
| Ausdehnung | 451 km | |
Iani Chaos ist, wie viele Regionen östlich der Valles Marineris, als chaotische Region charakterisiert. Morphologisch wird das Gebiet von stark erodierten, isolierten Restbergen geprägt.
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Chaotic terrain in Iani Chaos ESA224356.jpg
(c) ESA/DLR/FU Berlin (G. Neukum), CC BY-SA 3.0 igo
Iani Chaos is one of many regions east of Valles Marineris characterized by disrupted or chaotic terrain. The morphology of this terrain is dominated by large-scale remnant massifs, which are large relief masses that have been moved and weathered as a block. These are randomly oriented and heavily eroded. To the south (south is to the left) in this image, these mesas, which appear as flat-topped hills, range from less than one kilometre to roughly 8 kilometres wide, with a maximum relative elevation of approximately 1000 metres. This colour image was captured on 14 October 2004 by the High-Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express with a ground resolution of approximately 13.0 metres per pixel.
(c) ESA/DLR/FU Berlin (G. Neukum), CC BY-SA 3.0 igo
Iani Chaos is one of many regions east of Valles Marineris characterized by disrupted or chaotic terrain. The morphology of this terrain is dominated by large-scale remnant massifs, which are large relief masses that have been moved and weathered as a block. These are randomly oriented and heavily eroded. To the south (south is to the left) in this image, these mesas, which appear as flat-topped hills, range from less than one kilometre to roughly 8 kilometres wide, with a maximum relative elevation of approximately 1000 metres. This colour image was captured on 14 October 2004 by the High-Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express with a ground resolution of approximately 13.0 metres per pixel.
Mars Géolocalisation.jpg
Carte de Mars reconstituée à partir des mesures de Mars Global Surveyor (MOLA) et des observations de Viking.
Carte de Mars reconstituée à partir des mesures de Mars Global Surveyor (MOLA) et des observations de Viking.