Abstract
The sharp, nonoverlapping Raman bands for plagioclase, pyroxene, and olivine would be advantageous for on-surface, active mineralogical analysis of lunar materials. A robust, light-weight, low-power, rover-based Raman spectrometer with a laser exciting source, entirely transmission-mode holographic optics, and a charge-coupled device (CCD) detector could fit within a <20 cm cube. A modern micro-Raman spectrometer with its beam broadened and set for low resolution, was used to simulate the spectra anticipated from a rover instrument. The paper presents spectra for lunar mineral grains, <1 mm soil fines, breccia fragments, and glasses. -from Authors
| Original language | English |
|---|---|
| Pages (from-to) | 21,189-21,199 |
| Journal | Journal of Geophysical Research: Biogeosciences |
| Volume | 100 |
| Issue number | E10 |
| DOIs | |
| State | Published - 1995 |
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