PIA17079: Martian Features Formed When Material Moves Downslope
 Target Name:  Mars
 Is a satellite of:  Sol (our sun)
 Mission:  2001 Mars Odyssey
Mars Reconnaissance Orbiter (MRO)
Mars Global Surveyor (MGS)
 Spacecraft:  2001 Mars Odyssey
Mars Reconnaissance Orbiter (MRO)
Mars Global Surveyor Orbiter
 Instrument:  HiRISE
Mars Orbiter Camera (MOC)
 Product Size:  960 x 608 pixels (w x h)
 Produced By:  JPL
 Full-Res TIFF:  PIA17079.tif (1.752 MB)
 Full-Res JPEG:  PIA17079.jpg (100.9 kB)

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Original Caption Released with Image:

As on the Earth, many processes can move material down a Martian slope. This graphic compares seven different types of features observed on Mars that appear to result from material flowing or sliding or rolling down slopes.

Processes that explain one type of downslope feature may be irrelevant to another type. Some processes depend on the presence of a fluid, some are driven by seasonal changes in the environment, and others occur randomly when gravity is able to pull down unstable slope material.

These different processes can generate a wide range of feature shapes, though sometimes different processes can yield similar-looking results. Thus, to figure out how a feature may have formed, more must be considered than its shape. For example, researchers examining images from Mars orbiters have found differences in
   1. the season when the features are formed or are active (e.g., the features called "recurring slope lineae" or RSLs appear
       during late spring and summer, but linear gullies are active only during early spring);
   2. the features' sizes (e.g., slope streaks can extend for miles or kilometers, but dark frost streaks on dunes extend only up to
       100 yards, or meters); and
   3. the types of terrain on which a feature is found (e.g., gullies with an alcove-channel-apron shape are found both on rocky
       slopes and on sandy slopes, but linear gullies are only found on sandy slopes; dark frost streaks are formed on frozen dune
       slopes, but RSLs are formed on dark, warm slopes).

Scientists consider all of these factors -- and more -- when trying to form a complete picture about a feature's formation history and in figuring out what the presence of that feature means about the environment.

The seven images of different types of downslope features come from three different NASA Mars orbiters. The image of a landslide comes from the Thermal Emission Imaging System (THEMIS) on NASA's Mars Odyssey. The images of alcove-channel-apron gullies and of slope streaks come from the Mars Orbiter Camera (MOC) in NASA's Mars Global Surveyor. The other images come from the High Resolution Imaging Science Experiment (HiRISE) on NASA's Mars Reconnaissance Orbiter.

The University of Arizona, Tucson, operates THEMIS. Malin Space Science Systems, San Diego, operated MOC. The University of Arizona, Tucson, operates HiRISE. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, has managed the Mars orbiter projects for NASA's Science Mission Directorate, Washington.

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