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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 7.

Absorption depth of the 0.9 μm low-iron pyroxene feature as a function of grain size for our eight aubrite meteorites. The absorption depths for Rantila are plotted separately due to their deeper band depth values. Uncertainty values are generally smaller than the marker size for each meteorite. A general trend of increasing 0.9 μm band depth with increasing grain size is observed.

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