Hebes and Ophir Chasmata

Scaled Image

Image Credit: NASA/JPL/ASU

About this image

Today's VIS image shows part of two chasmatas - Hebes Chasma at the top of the image and Ophir Chasma at the bottom. Both chasmata have large landslide deposits. Ophir Chasma has a large layered deposit, which has subsequently been eroded by wind and fluvial processes (bottom of image). Hebes Chasma is an inclosed basin not connected to Valles Marineris. It is 319 km long (east/west, 198 miles), 130 km wide (north/south, 81miles) and up to 8km (5 miles) deep. Ophir Chasma is approximately 317km long (197 miles) and is part of the Valles Marineris system of canyons.

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

Context

Image ID: 
V94365004 (View data in Mars Image Explorer)
-2.67943
286.449
94365
2023-03-24 07:37
Fri, 2023-07-07
VIS
256 pixels (18 km)
3792 pixels (265 km)
0.070088 km/pixel
0.0713732 km/pixel

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