Ponded Lava, Slope Streaks, and Inadvertent Change Detection
NASA/JPL/University of Arizona
Ponded Lava, Slope Streaks, and Inadvertent Change Detection
ESP_020963_1810  Science Theme: Volcanic Processes
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In this fascinating observation that shows part of an impact crater, there is a very small breach (gap) in the crater rim. From examining the texture of the surrounding plains and the crater floor, we can conclude that a large lava flow overtopped and cut through a low part of the crater rim and then flowed down the wall of the crater and onto the crater floor, incising (cutting) a channel as it went. This observation is focused on the channel, but a portion of the ponded lava on the crater floor is also visible.

If you want to get a better look at the crater floor, check out this CTX image and this really neat anaglyph. From this you can see that the lava covered almost the entire crater floor, however the crater central peak sticks up from the center, an island in the sea of lava.

This observation was taken to study the channel and breach to learn about the properties of the lava when the flow was active a long time ago. Since part of the science rationale for taking this observation was to find the relative heights of the ponded lava surface and the surrounding plains as well as to measure the depth of the channel, this site was chosen for stereo coverage. In this case the target was imaged a second time 3.5 years (almost 2 Mars years) after the first image was acquired.

Sometimes when the two parts of a stereo pair are taken far apart in time, the stereo pair turns into an inadvertent change detection pair. So did anything in this landscape change in the intervening 3.5 years? Yes! And it has nothing to do with the old lava flow (the reason the observation was taken).

If you look closely at the crater wall, you can see streaks going down the slope in many different areas. These are slope streaks which are thought to form from dust avalanches that remove a thin layer of bright dust from the surface (see PSP_005369_1925 for a more thorough explanation). Now going back to the stereo pair, this subimage shows two cutouts of the same part of the crater wall, but in the later image (the one on the right) we can see that an entirely new slope streak formed in the time between the acquisition of the first and second image! The new slope streak is approximately 725 meters (roughly 0.45 miles) long. This is merely one example of a new slope streak.

If you look closely, you should be able to identify many slope streaks that have formed in this small area since this observation was originally acquired.

Written by: Anjani Polit  (26 January 2011)

This is a stereo pair with PSP_004151_1810.
Acquisition date
15 January 2011

Local Mars time:

Latitude (centered)

Longitude (East)

Range to target site
294.1 km (183.8 miles)

Original image scale range
29.4 cm/pixel (with 1 x 1 binning) so objects ~88 cm across are resolved

Map projected scale
25 cm/pixel and North is up

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Emission angle:

Phase angle:

Solar incidence angle
57°, with the Sun about 33° above the horizon

Solar longitude
218.0°, Northern Autumn

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North azimuth:  97°
Sub-solar azimuth:  345.4°
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NASA’s Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, Calif., manages the Mars Reconnaissance Orbiter for NASA’s Science Mission Directorate, Washington. The HiRISE camera was built by Ball Aerospace and Technology Corporation and is operated by the University of Arizona.