Definition
Specific shallow (meter to ten meters deep) flat-floored depression on dust-covered steep slopes on Mars; a triangular scar has a triangular planform with a sharp upslope apex and extends hundreds of meters to over a kilometer downslope.
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Description
Triangular scars are outlined by pairs of perfectly linear scarps of a remarkably constant height of about 1–10 m; the scarps form a sharp apex when they join upslope (Figs. 1 and 2). Many triangular scarps have specific mounds at their downslope termination (Fig. 1; Gerstell et al. 2004; Phillips et al. 2007), but many do not. The small-scale texture of the triangular scarp floor often differs from surrounding surface texture (Chuang et al. 2010).
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References
Chuang FC, Beyer RA, McEwen AS, Thomson BJ (2007) HiRISE observations of slope streaks on Mars. Geophys Res Lett 34, L20204. doi:10.1029/2007GL031111
Chuang FC, Beyer RA, Bridges NT (2010) Modification of Martian slope streaks by Eolian processes. Icarus 205:154–164
Gerstell MF, Aharonson O, Schorghofer N (2004) A distinct class of avalanche scars on Mars. Icarus 168:122–130
Kreslavsky MA, Head JW (2009) Slope streaks on Mars: a new “wet” mechanism. Icarus 201:517–527
Phillips CB, Burr DM, Beyer RA (2007) Mass movement within a slope streak on Mars. Geophys Res Lett 34:21202
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Kreslavsky, M.A., Schörghofer, N., Kereszturi, Á. (2014). Triangular Scar (Mars). In: Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-9213-9_594-1
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DOI: https://doi.org/10.1007/978-1-4614-9213-9_594-1
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