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Quantifying the 3-Dimensional Shape of Lunar Regolith Particles Using X-Ray Computed Tomography and Scanning Electron Microscopy at Sub-γ Resolution

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Impacts are the dominant process shaping the regoliths of most airless solar system bodies. The impact process that controls the particle size and shape distribution of, for example, lunar soils… Click to show full abstract

Impacts are the dominant process shaping the regoliths of most airless solar system bodies. The impact process that controls the particle size and shape distribution of, for example, lunar soils is both destructive (comminution) and constructive (agglutinization) and is very different from processes that form terrestrial soils or result from grinding analogs in a mortar and pestle. Describing particle shapes as ‘irregular’ is only a qualitative description, and there are an infinite number of quantitatively different shapes that are irregular.

Keywords: dimensional shape; shape; microscopy; quantifying dimensional; shape lunar

Journal Title: Microscopy and Microanalysis
Year Published: 2017

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