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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 2.

Absolute reflectance of the seven grain size bins from our eight aubrite meteorites across the full 0.18–14.5 μm wavelength range. Each meteorite contains two panels that correspond to a set wavelength range, consisting of 0.18–2.5 μm (Panel (1)) and 2.5–14.5 μm (Panel (2)). Meteorite names are given for each in Panel (2). Color is utilized to indicate the spectrometer used for data collection: blue is Avantes UV, black is ASD Vis-NIR, and red is FTIR NIR-MIR. UV and NIR-MIR data are scaled and connected with the black Vis-NIR data at 0.4 and 2.1 μm, respectively.

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