Figures and Tables
From the following article:
Water and the martian landscape
Victor R. Baker
Nature 412, 228-236(12 July 2001)
doi:10.1038/35084172
Figure 1
Glaciated terrain east of Hellas Planitia, at latitude 42° S, longitude 252° W.
Full size figure and legend (93K)Figure 2
High-resolution Mars Orbiter Camera (MOC) image of a fluvial channel system at latitude 7.9° N, longitude 205.8° W, south of Cerberus Rupes (MOC Image M21-01914).
Full size figure and legend (390K)Figure 3
Large contraction-crack polygons developed on the floor of a northern-plains crater at approximately 67.5° N, 312.5° W (MOC Image M01-00294).
Full size figure and legend (132K)Figure 4
Oblique view of topographic data from the Mars Orbiter Laser Altimeter (MOLA) showing downstream portions of the outflow channel Kasei Vallis.
Full size figure and legend (61K)Figure 5
Comparison of simplified channel cross-sections for cataclysmic flood channels on Mars (upper two channels) and Earth (lower channels).
Full size figure and legend (51K)Figure 6
MOC image (M09-04718) of small gullies and other hillslope features in the central peak area of Hale Crater (latitude 36° S, longitude 37° W).
Full size figure and legend (145K)Figure 7
Morphogenetic regions for climate-related landforms on Earth91.
Full size figure and legend (84K)Figure 8
Esker-like ridges in southern Argyre Planitia (latitude 56° S, longitude 40° W).
Full size figure and legend (131K)Figure 9
Portion of MOC Image MOO-01511 showing detail of esker-like ridge in southern Argyre Planitia (Fig. 8).
Full size figure and legend (154K)








