Grain Size Effects on Visible and Near-infrared (0.35–2.5 μm) Laboratory Spectra of Rare Meteorite Classes

Linking near-Earth asteroids to associated meteorites can be a challenging process for many reasons, one being grain size differences. To address this issue for rarer meteorites, we studied visible and near-infrared (0.35–2.5 μ m) reflectance spectra of 11 rare meteorite classes over five different...

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Bibliographic Details
Main Authors: K. I. Ridenhour, V. Reddy, A. Battle, D. Cantillo, N. C. Pearson, J. A. Sanchez
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Planetary Science Journal
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Online Access:https://doi.org/10.3847/PSJ/ad7116
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