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Butterfly Ejecta

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Encyclopedia of Planetary Landforms
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Definition

Impact crater ejecta morphology with an uprange and a downrange forbidden zone.

Synonyms

Asymmetric ejecta; Bilateral symmetric ejecta; Downrange and uprange forbidden zone (crater); Fly wing (crater)

A type of ejecta often found in association with an elliptical crater (oblique impact)

Variations in formation and modification:

  1. (1)

    Dry ejecta crater emplaced solely ballistically (Mercury [Fig. 1], Moon [Fig. 2]).

  2. (2)

    Butterfly ejecta emplaced ballistically and then modified by surface flow (Mars) (Fig. 3) (Herrick and Hessen 2006). They can have smooth or textured blanket and may possess rampart.

  3. (3)

    Butterfly ejecta formed on Venus, in a dense and hot atmosphere (Venus) (Fig. 4).

Fig. 1
figure 1

MESSENGER mosaic of Hovnatanian crater (43 × 22 km, 7.7°S, 172.8°E), shows butterfly ejecta pattern on Mercury. Impact direction was from bottom to top of image (NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington)

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References

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Correspondence to Robert R. Herrick .

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Herrick, R.R. (2014). Butterfly Ejecta. In: Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-9213-9_27-2

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  • DOI: https://doi.org/10.1007/978-1-4614-9213-9_27-2

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