NASA Mars Odyssey THEMIS Image: Dynamic Mars
Image Context: Context image credit: NASA/Mars Orbiter Laser Altimeter (MOLA) Team [ Find on map: Javascript version ] [ Find on map: CGI version ] Several interesting impact craters are observed in this THEMIS image taken near Scamander Vallis that illustrate the dynamic nature of the Martian surface. The smallest crater at the bottom of the image shows dark streaks running down the crater walls that are likely due to small dust avalanches. The larger nearby crater has a well developed central peak and fluidized ejecta material that covers part of the eroded crater to the top of the image. The morphology of the ejecta suggests the impact may have occurred in a volatile rich surface. [Source: ASU THEMIS Science Team] Note: this THEMIS visual image has not been radiometrically nor geometrically calibrated for this preliminary release. An empirical correction has been performed to remove instrumental effects. A linear shift has been applied in the cross-track and down-track direction to approximate spacecraft and planetary motion. Fully calibrated and geometrically projected images will be released through the Planetary Data System in accordance with Project policies at a later time.
Image Credit: NASA/JPL/Arizona State University | ||||||||||||||||||||
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