Definition
Terrain displaying rounded and subdued topography.
Subtypes
“Softened terrain” may refer to (Kreslavsky et al. 2008):
- (1)
The soft appearance of topographic features at high latitudes on Mars, caused by smoothing of topography with a characteristic vertical scale on the order of several meter(s). Terrain softening affects all types of landforms, but it is particularly evident on softened craters (Fig. 1). It is characterized with broad slope inflections and convex slope segments (Squyres et al. 1992, p. 543).
- (2)
Latitude-dependent trends in crater depth, concentric crater infill, etc., related to creep of a hundreds-of-meters-thick layer (lineated valley fill).
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Jankowski DG, Squyres SW (1992) The topography of impact craters in “softened” terrain on Mars. Icarus 100(1):26–39
Kreslavsky MA, Head J, Marchant DR (2008) Periods of active permafrost layer formation during the geological history of Mars: implications for circum-polar and mid-latitude surface processes. Planet Space Sci 56:289–302
Soderblom LA, Kreidler TJ, Masursky H (1973) Latitudinal distribution of a debris mantle on the Martian surface. J Geophys Res 78:4117–4122
Squyres SW, Carr MH (1986) Geomorphic evidence for the distribution of ground ice on Mars. Science 231:249–252
Squyres SW, Clifford SM, Kuzmin RO, Zimbelman JR, Costard FM (1992) Ice in the Martian regolith. In: Kieffer HH (ed) Mars. University of Arizona Press, Arizona, 1498 pp
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Hargitai, H., Kereszturi, Á. (2015). Softened Terrain (Mars). In: Hargitai, H., Kereszturi, Á. (eds) Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-3134-3_587
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DOI: https://doi.org/10.1007/978-1-4614-3134-3_587
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