Definition
A pedestal crater with pits along its margins.
Description
Pitted pedestal craters display an outward facing marginal scarp (a characteristic feature of pedestal craters) interrupted by pits (Fig. 1). Both crater floor and pedestal are elevated above the surrounding surface (a characteristic feature of perched craters), but the crater is not infilled. They also have an excess ejecta (Excess Ejecta Crater). Pitted pedestal craters are perched an average of ~100 m above surrounding plains, much higher than normal pedestal craters. Individual pits are characterized by cuspate shapes and alcove-like features and have a typical depth of ~20 m. Pits show no preferential orientation. Pits form at the pedestal margin, rather than in the adjacent surrounding terrain. Pits may contain small isolated mesas. Pits often appear to coalesce to form a moat-like structure that extends along a significant part of the pedestal circumference (Kadish et al. 2008).
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References
Kadish SJ, Head JW, Barlow NG, Marchant DR (2008) Martian pedestal craters: marginal sublimation pits implicate a climate-related formation mechanism. Geophys Res Lett 35:L16104. doi:10.1029/2008GL034990
Kadish SJ, Barlow NG, Head JW (2009) Latitude dependence of Martian pedestal craters: evidence for a sublimation-driven formation mechanism. J Geophys Res 114:E10001. doi:10.1029/2008JE003318
Kadish SJ, Head JW, Barlow NG (2010) Pedestal crater heights on Mars: a proxy for the thicknesses of past, ice-rich, Amazonian deposits. Icarus 210:92–101
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Hargitai, H. (2014). Pitted Pedestal Crater. In: Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-9213-9_270-1
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DOI: https://doi.org/10.1007/978-1-4614-9213-9_270-1
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