Martian volatile inventory, planetary climatic and atmospheric evolution, and the interpretation of various remote sensing data were discussed. A number of morphologies that were cited as potential indicators of subsurface volatiles were reviewed. Rampart craters and terrain softening were the focus of more in-depth discussion because of the popular attention they have received and the fact that their areal distributions are by far the most extensive of all the proposed indicators.
Martian Geomorphology and Its Relation to Subsurface Volatiles
1986
54 pages
Report
No indication
English
Astrogeology , Astrophysics , Conferences , Cratering , Geomorphology , Lithology , Mars surface , Volatility , Structural properties (Geology) , Ice , Lava , Water , Weathering
Detecting water in the Martian subsurface
NTRS | 2001
|Technologies for exploring the Martian subsurface
IEEE | 2006
|