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Alpine Glaciers
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Caption:
Released 27 August 2003
This image shows part of the western flank of Arsia Mons, the southernmost of the three great Tharsis Montes. The surface shows parallel ridges more reminiscent of a Zen garden than any typical geological feature. These ridges are not typical of lava flow fronts, so a different explanation has been proposed by Mars scientists. These ridges may instead be ancient signs of previously existing glaciers that formed high on the volcano's flank. As glaciers retreat with the seasons and shifting climate, they leave behind a mound of debris along their receding edge. Successive retreats can produce a series of parallel ridges similar to those seen here.
Image information: VIS instrument. Latitude -6.9°, Longitude 230.5° East (129.5%deg; West). 19 meter/pixel resolution.
Cataloging Keywords:
| Name | Value | Additional Values |
|---|---|---|
| Target | Mars | |
| System | ||
| Target Type | Planet | |
| Mission | 2001 Mars Odyssey | |
| Instrument Host | Mars Odyssey | |
| Host Type | Orbiter | |
| Instrument | Thermal Emission Imaging System (THEMIS) | |
| Detector | ||
| Extra Keywords | Grayscale, Mountain, Volcano | |
| Acquisition Date | ||
| Release Date | 2003-09-03 | |
| Date in Caption | 2003-08-27 | |
| Image Credit | NASA/JPL/Arizona State University | |
| Source | photojournal.jpl.nasa.gov/catalog/PIA04715 | |
| Identifier | PIA04715 | |
