Mars Odyssey THEMIS images - February 1-5, 2010
Mon Feb 8, 2010 at 13:08 UTC
The following new images taken by the Thermal Emission Imaging System (THEMIS) on the Mars Odyssey spacecraft are now available:
- Proctor Crater Dunes (Released 1 February 2010)
This VIS image of the floor of Proctor Crater shows part of the sand sheet and dune forms that are located there. - Arkhangelsky Crater (Released 2 February 2010)
This VIS image shows part of the floor of Arkhangelsky Crater. - Lycus Sulci (Released 3 February 2010)
Dark slope streaks are found throughout Lycus Sulci. - Patapsco Vallis (Released 4 February 2010)
This VIS image shows a portion of Patapsco Vallis, a channel located on the eastern margin of Elysium Mons. - Coprates Chasma (Released 5 February 2010)
The floor of Coprates Chasma contains many different geologic landforms.
| Source: Arizona State University | |
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