Definition
Arc-shaped sinuous ridges on the floor of impact craters or other depressions in the middle- and high-latitude zones of Mars.
Description
Concave depressions containing elevated sharp ridges on crater floors, at the base of many gully on Mars (Berman et al. 2004). Inside the concave depressions, the rims enclose smooth floors and occasionally are associated with lineated or rough-textured crater floors (Howard 2003) (Figs. 1 and 2). Tongue ridges may merge to produce a complex, scalloped appearance (arcuate ridges). Arcuate ridges run parallel to the crater perimeter (Figs. 3 and 4).
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References
Berman DC (2003) Hillside gullies and possible glacial landforms associated with the degradation of highland craters on Mars. Master’s thesis, University of Arizona, Tucson
Berman DC, Hartmann WK, Crown DA (2004) The distribution of gullies and tongue-shaped ridges and their role in the degradation of martian craters. In: 35th lunar and planetary science, League City, Texas, #1391
Berman DC, Hartmann WK, Crown DA, Baker VR (2005) The role of arcuate ridges and gullies in the degradation of craters in the Newton Basin region of Mars. Icarus 178:465–486
Howard AD (2003) Tongue ridges and rumpled crater floors in mid-southern-latitude martian craters. In: 34th lunar and planetary science, League City, Texas, #1065
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Kereszturi, Á., Hargitai, H. (2014). Tongue-shaped and arcuate ridges inside depressions (Mars). In: Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-9213-9_377-1
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DOI: https://doi.org/10.1007/978-1-4614-9213-9_377-1
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