Investigating Mars: Hebes Chasma

Scaled Image

Image Credit: NASA/JPL/ASU

About this image

This image shows the north central cliff face of Hebes Chasma. The cliff face and downslope movement of material is very different in appearance than the same features of the large mesa in the center of the chasma. Hebes Chasma is an enclosed basin not connected to Valles Marineris.

The Odyssey spacecraft has spent over 15 years in orbit around Mars, circling the planet more than 69000 times. It holds the record for longest working spacecraft at Mars. THEMIS, the IR/VIS camera system, has collected data for the entire mission and provides images covering all seasons and lighting conditions. Over the years many features of interest have received repeated imaging, building up a suite of images covering the entire feature. From the deepest chasma to the tallest volcano, individual dunes inside craters and dune fields that encircle the north pole, channels carved by water and lava, and a variety of other feature, THEMIS has imaged them all. For the next several months the image of the day will focus on the Tharsis volcanoes, the various chasmata of Valles Marineris, and the major dunes fields. We hope you enjoy these images!

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

Context

Image ID: 
V26886025 (View data in Mars Image Explorer)
-0.142089
283.512
26886
2008-01-06 02:43
Mon, 2017-08-21
VIS
1024 pixels (18 km)
3648 pixels (65 km)
0.01788 km/pixel
0.0180891 km/pixel

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