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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 4.

Absolute reflectance (top row) and normalized reflectance (bottom row) of our eight aubrite meteorites at the same 45–90 μm grain size bin. The normalized row has the same normalization wavelength (1.5 μm) and scaling as in Figure 3. While the top absolute reflectance row illustrates general differences in albedo, the normalized row highlights differences in spectral slope and absorption depths.

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