MARS RECONNAISSANCE ORBITER HIRISE IMAGES August 3, 2011
o The Western Edge of a Layered Mound in Juventae Chasma http://hirise.lpl.arizona.edu/ESP_020470_1755 The CRISM instrument on MRO has detected high sulfates at the base of this mound, and the resolution power of HiRISE gives us a better look at the area's morphology. o Striated Highlands near Claritas Rupes http://hirise.lpl.arizona.edu/ESP_020551_1545 These striated highlands are probably the result of what is termed "mass wasting" when material higher up collapses and flows downslope. o Crater Rim with Bedrock Layers and Gullies http://hirise.lpl.arizona.edu/ESP_022999_1335 This observation reveals some of the materials that have largely filled the crater. o Slope of Gale Crater above MSL Landing Site http://hirise.lpl.arizona.edu/ESP_023034_1755 It is possible that hydrothermal deposits formed here in association with the creation and cooling of Gale Crater billions of years ago. All of the HiRISE images are archived here: http://hirise.lpl.arizona.edu/ Information about the Mars Reconnaissance Orbiter is online at http://www.nasa.gov/mro. The mission is managed by NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology, for the NASA Science Mission Directorate, Washington, D.C. Lockheed Martin Space Systems, of Denver, is the prime contractor and built the spacecraft. HiRISE is operated by the University of Arizona. Ball Aerospace and Technologies Corp., of Boulder, Colo., built the HiRISE instrument. ______________________________________________ Visit the Archives at http://www.meteoritecentral.com/mailing-list-archives.html Meteorite-list mailing list [email protected] http://six.pairlist.net/mailman/listinfo/meteorite-list
