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Grain Size Effects on UV-MIR Spectra of Aubrites: Clues for Interpreting E-type Near-Earth Asteroids

  • Authors: David C. Cantillo, Neil C. Pearson, Kaycee I. Ridenhour, Vrinda McBride, Miren Miranda, Adam Battle, Thomas Joyce, Juan A. Sanchez, Vishnu Reddy

David C. Cantillo et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 12.

R. B. contrast as a function of grain size for our eight aubrites. Finer <45 μm samples generally show the smallest contrast among each aubrite, with maximum contrast values typically seen in moderate–large grain sizes (150–1000 μm).

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