Scaled Image

Image Credit: NASA/JPL/ASU

About this image

Ius Chasma is at the western end of Valles Marineris, south of Tithonium Chasma. Valles Marineris is over 4000 kilometers long, almost as wide as the United States. Ius Chasma is almost 850 kilometers long (528 miles), 120 kilometers wide and over 8 kilometers deep. In comparison, the Grand Canyon in Arizona is about 175 kilometers long, 30 kilometers wide, and only 2 kilometers deep. The canyons of Valles Marineris were formed by extensive fracturing and pulling apart of the crust during the uplift of the vast Tharsis plateau. Landslides have enlarged the canyon walls and created deposits on the canyon floor. Weathering of the surface and influx of dust and sand have modified the canyon floor, both creating and modifying layered materials. There are many features that indicate flowing and standing water played a part in the chasma formation. The rugged floor of Ius Chasma in this image is the result of many large landslides.

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

Context

Image ID: 
V97510006 (View data in Mars Image Explorer)
-7.47384
276.956
97510
2023-12-08 06:29
Mon, 2024-05-06
VIS
512 pixels (18 km)
1824 pixels (64 km)
0.035228 km/pixel
0.0358674 km/pixel

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