NASA Mars Odyssey THEMIS Image: Crater Interior with Internal Craters
Image Context: Context image credit: NASA/Mars Orbiter Laser Altimeter (MOLA) Team [ Find on map: Javascript version ] [ Find on map: CGI version ]
Today’s crater interior contains smaller craters, sand dunes, and erosional features caused the wind. Additionally, the crater rim appears subdued, likely due to dust cover. Note how the ejecta surrounding the small craters has be eroded by the wind. [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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