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Pit Crater

Encyclopedia of Planetary Landforms

Definition

Pit craters are rimless steep-sided depressions that are inferred to have formed by collapse processes of volcanic/magmatic origin (e.g., Halliday et al. 2011). Some authors also include those of faulting origin (Ferrill et al. 2004, 2011; Wyrick et al. 2004).

Category

A type of pit.

Synonyms

Collapse crater, Collapse depression (Greeley and Gault 1979), Collapse pit, Subsidence crater

Description

Pit craters are circular to elliptical, shallow, steep-sided depressions which lack the elevated rim and ejecta deposits typical of impact craters or lava flows typically associated with calderas (Wyrick et al. 2004). Pit craters commonly have a conical shape, with or without a flat floor (Wyrick et al. 2004). They are sometimes found in alignments (pit crater chains), which in many cases coalesce into linear troughs and are bounded by a graben (Fig. 1). Volcanic pit craters have little or no overflow of their lava lakes (Halliday et al. 2012).

Fig. 1
figure 1

Cyane Catena pit crater...

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References

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Correspondence to Carolyn H. van der Bogert .

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van der Bogert, C.H., Ashley, J.W., Ferrill, D. (2014). Pit Crater. In: Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-9213-9_260-1

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  • DOI: https://doi.org/10.1007/978-1-4614-9213-9_260-1

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Chapter history

  1. Latest

    Pit Crater
    Published:
    11 February 2015

    DOI: https://doi.org/10.1007/978-1-4614-9213-9_260-2

  2. Original

    Pit Crater
    Published:
    05 September 2014

    DOI: https://doi.org/10.1007/978-1-4614-9213-9_260-1