Mars Odyssey Mission THEMIS: Feature Image: Hebes Chasma Dust Avalanches (Released 7 June 2005)

Vital Statistics
Location: -1.4N, 286.6E	Released: 2005-06-07
Image Size: 18.5 x 12.6 km, 1036 x 702 px
Resolution: 17m	Instrument: VIS

Image Credit: NASA/JPL/ASU

Image Context:
Context image for 20050607A

Context image credit: NASA/JPL/MOLA
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Detailed information on this image is available at the THEMIS Data Releases website.

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

Dust avalanches, also called slope streaks, occur on many Martian terrains. The deposition of airborne dust on surfaces causes a bright tone in the THEMIS VIS images. Any movement of the dust downhill, a dust avalanche, will leave behind a streak where the darker, dust-free surface is exposed. These dust avalanches are located in Hebes Chasma.