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Fine-Ejecta Halo

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Encyclopedia of Planetary Landforms
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Definition

A halo of material characterized by anomalous radar or thermal properties around impact craters interpreted as fine-grained ejecta.

Category

A type of Crater-associated radar-dark diffuse feature

Synonyms

Low nighttime temperature halo (Mars); Nonparabolic (radar-) dark halo; Radar-dark halo; Radar-dark mantle (this term is used also for pyroclastic deposits on the Moon)

Description

  1. (1)

    Anomalous radar properties: A clear or faint radar-dark halo that surrounds an impact crater and extends beyond its radar-bright continuous ejecta (Venus, Moon).

  2. (2)

    Anomalous thermal properties: Crater halos characterized by low nighttime surface temperatures and relatively low values of thermal inertia (Mars). Venusian and Martian fine-ejecta halos are larger than on the Moon.

Interpretation

Low radar backscatter indicates fine-grained (smooth) material.

Venusian radar-dark halos represent a veneer of fine-particulate, rock-poor material covering the local bedrock (Basilevsky et al. 2012).

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References

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Correspondence to Rebecca Ghent .

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Ghent, R. (2014). Fine-Ejecta Halo. In: Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-9213-9_291-1

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  • DOI: https://doi.org/10.1007/978-1-4614-9213-9_291-1

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  • Online ISBN: 978-1-4614-9213-9

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