Photometric Properties within the Reiner Gamma Swirl: Constraining Formation Mechanisms

Author:

Domingue DeborahORCID,Weirich JohnORCID,Chuang FrankORCID,Courville SamuelORCID,Clark RogerORCID,Sickafoose AmandaORCID,Palmer EricORCID,Gaskell RobertORCID

Abstract

Abstract The area in the Reiner Gamma swirl studied by Weirich et al. for topographic correlations also displays correlations with the Hapke-model-derived single-scattering albedo, surface roughness, and particle scattering properties with swirl unit. The correlations with single-scattering albedo associate compositional variations in plagioclase and FeO content with swirl unit. The correlations with photometric surface roughness show a rougher surface on-swirl, implying a potentially more porous surface on-swirl compared to off-swirl. This suggests the variations in single-scattering albedo are dominated by the compositional differences and not structural differences, such as compaction. Grain-size differences could still contribute to the albedo variations. Differences in particle scattering properties between on-swirl and off-swirl are counter-indicative of the trend expected from variations in space weathering, unless there is a process to initiate either size sorting or compositional differences. The photometric properties point to a complex interaction of multiple processes to form the swirl units, not a singular dominant process. Variations in weathering, dust mobilization and entrapment, and impact modification may all play a key role.

Funder

NASA Lunar Data Analysis Program

NASA Solar System Exploration Research Virtual Institute

Publisher

American Astronomical Society

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