Identifying and Quantifying Mineral Abundance through VSWIR Microimaging Spectroscopy: A Comparison to XRD and SEM
- Creators
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Leask, Ellen K.
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Ehlmann, Bethany L.
Abstract
Visible-shortwave infrared microimaging reflectance spectroscopy is a new technique to identify minerals, quantify abundances, and assess textural relationships at sub-millimetre scale without destructive sample preparation. Here we used a prototype instrument to image serpentinized igneous rocks and carbonate-rich travertine deposits to evaluate performance, relative to traditional techniques: XRD (mineralogical analysis of bulk powders with no texture preservation) and SEM/EDS (analysis of phases and textures using chemical data from polished thin sections). VSWIR microimaging spectroscopy is ideal for identifying spatially coherent rare phases, below XRD detection limits. The progress of alteration can also be inferred from spectral parameters and may correspond to phases that are amorphous in XRD. However, VSWIR microimaging spectroscopy can sometimes be challenging with analyses of very dark materials (reflectance <0.05) and mineral mixtures occurring at a spatial scales multiple factors below the pixel size. Abundances derived from linear unmixing typically agree with those from XRD and EDS within ~10%.
Additional Information
© 2016 IEEE. Thanks to A. Fraeman, C. Sanders, and B. Van Gorp for assistance with sample data acquisition and to the entire JPL UCIS team. This work was partially supported by a NASA Mars Fundamental Research Program grant (#NNX12AB42G) to B.L.E., a JPL-RTD/PDF to B.L.E. and D. Blaney, and a private grant to Caltech from the Rose Hills Foundation.Attached Files
Accepted Version - WHISPERS_2016_paper_58.pdf
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Additional details
- Eprint ID
- 70145
- Resolver ID
- CaltechAUTHORS:20160902-093920758
- NASA
- NNX12AB42G
- JPL Research and Technology Development Fund
- Rose Hills Foundation
- Created
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2016-09-02Created from EPrint's datestamp field
- Updated
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2021-11-11Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences