NASA Mars Odyssey THEMIS Image: Tinto Vallis Fluvial Channel
Image Context: Context image credit: NASA/Mars Orbiter Laser Altimeter (MOLA) Team [ Find on map: Javascript version ] [ Find on map: CGI version ]
Full data on this image has now been released via the THEMIS Data Releases website. This night time IR image shows a small fluvial channel located near Tinto Vallis. These channels are northeast of Tyrrhena Patera and its related lava flows. Tyrrhena Patera is one of the larger volcanic complexs in the southern hemisphere of Mars. Small channels are easy to see in nighttime IR, with the cold channel floor (dark) contrasting from the warmer (bright) surroundings. NOTE: in nighttime images North is to the bottom of the image. [Source: ASU THEMIS Science Team] Note: this THEMIS infrared 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 | ||||||||||||||||||||
[ Show Full-Size Image (GIF) ] [ Show Full-Size Image (JPG) ] | ||||||||||||||||||||
[ Show Full-Size Image (PNG) ] [ Show Full-Size Image (TIF) ] | ||||||||||||||||||||
[ Printer-friendly version ] |