2017
DOI: 10.1002/2016gl071429
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Impact melt of the lunar Crisium multiring basin

Abstract: New geological mapping of the Crisium basin on the Moon has revealed exposures of the basin impact melt sheet. The melt sheet has a feldspathic highland composition, somewhat more mafic than the melt sheet of the Orientale basin, but less mafic than comparable deposits around the Imbrium basin. These newly recognized deposits would be ideal locations to directly sample Crisium basin impact melt, material whose study would yield insight into the composition of the lunar crust, the time of formation of the basin… Show more

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Cited by 15 publications
(30 citation statements)
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“…We mapped five individual kipukas that comprise the northern Crisium Archipelago, shown in Figure . While the Northern Archipelago lacks fractures, its terrain is rough and knobby, similar to impact melt in Orientale (Spudis & Sliz, ). The Archipelago measured ~18 × 18 km in its approximately NS and approximately EW dimensions.…”
Section: Resultsmentioning
confidence: 99%
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“…We mapped five individual kipukas that comprise the northern Crisium Archipelago, shown in Figure . While the Northern Archipelago lacks fractures, its terrain is rough and knobby, similar to impact melt in Orientale (Spudis & Sliz, ). The Archipelago measured ~18 × 18 km in its approximately NS and approximately EW dimensions.…”
Section: Resultsmentioning
confidence: 99%
“…Spudis and Sliz () used fractures as one criterion to help identify impact melt deposits. However, fractures are not unique to impact melt deposits on the Moon and therefore should be used with caution when identifying potential impact melt facies.…”
Section: Resultsmentioning
confidence: 99%
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“…The ages of the three groups were thoroughly studied by Hiesinger et al (2011) based on LROC WAC images using crater sizefrequency distribution measurement (CSFD). Sliz and Spudis (2016) and Spudis and Sliz (2017) remapped the geological units inner and surrounding of Crisium basin using LRO imagery, Clementine maps of Fe and Ti and LOLA maps, which showed much different from that outlined by Head et al (1978).…”
Section: Introductionmentioning
confidence: 83%