Which Clays are Really Present on Mars? or Are you sure about those squiggly lines? Ralph Milliken (JPL/Caltech) 50 m Clays in Shalbatana Vallis (HiRISE)
AQUEOUS SEDIMENTARY DEPOSITS IN HOLDEN CRATER: LANDING SITE FOR ... Excluding uncontrolled wind effects during parachute descent. 10 km. Landing ellipse radius ...
Black area is topography 2.0 km. Lines at 50 , 60 latitude ... Day 3 - Friday. What's Next? (MRO/Maps) Summary Discussion. Break. Discussion and Prioritization ...
Martian Depressions Implications for Large Scale Evaporite Deposits Zackery E. Smith, Jason A. Tullis, Kenneth F. Steele Arkansas Center for Space and Planetary Science,