Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 11.

The 9.0 μm Reststrahlen band (R. B.) maxima offset relative to each meteorite’s 45–90 μm sample. Most R. B. maxima remain relatively fixed across grain size for each meteorite, excluding occasional prominent jumps where a stronger band becomes the highest local maxima.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse