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

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Figure 1 - Unfortunately we are unable to provide accessible alternative text for this. If you require assistance to access this image, or to obtain a text description, please contact npg@nature.com

Figure 1

Glaciated terrain east of Hellas Planitia, at latitude 42° S, longitude 252° W.

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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).

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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).

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Figure 4

Oblique view of topographic data from the Mars Orbiter Laser Altimeter (MOLA) showing downstream portions of the outflow channel Kasei Vallis.

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Figure 5

Comparison of simplified channel cross-sections for cataclysmic flood channels on Mars (upper two channels) and Earth (lower channels).

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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).

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Figure 7

Morphogenetic regions for climate-related landforms on Earth91.

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Figure 8

Esker-like ridges in southern Argyre Planitia (latitude 56° S, longitude 40° W).

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Figure 9

Portion of MOC Image MOO-01511 showing detail of esker-like ridge in southern Argyre Planitia (Fig. 8).

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