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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 9.

Spectral slope from 0.8 to 1.8 μm as a function of grain size for our eight aubrite meteorites. A red versus blue spectral slope refers to either a positive or negative value, respectively. The general trend of decreasing spectral slope with increasing grain size is observed.

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