The effects of magmatic evolution, crystallinity, and microtexture on the visible/near-infrared and thermal-infrared spectra of volcanic rocks
The natural chemical and physical variations that occur within volcanic rocks (petrology) provide critical insights into mantle and crust conditions on terrestrial bodies. Visible/near-infrared (VNIR; 0.3-2.5 µm) and thermal infrared (TIR; 5-50 µm) spectroscopy are the main tools available to remotely characterize these materials from satellites in orbit. However, the accuracy of petrologic information that can be gained from spectra when rocks exhibit complex variations in mineralogy, crystallinity, microtexture, and oxidation state occurring together in natural settings is not well constrained. Here, we compare the spectra of a suite of volcanic planetary analog rocks from the Three Sisters, OR to their mineralogy, chemistry, and microtexture from X-ray diffraction, X-ray fluorescence, and electron microprobe analysis. Our results indicate that TIR spectroscopy is an effective petrologic tool in such rocks for modeling bulk mineralogy, crystallinity, and mineral chemistry. Given a library with appropriate glass endmembers, TIR modeling can derive glass abundance with similar accuracy as other major mineral groups and provide first-order estimates of glass wt.% SiO2 in glass-rich samples, but cannot effectively detect variations in microtexture and minor oxide minerals. In contrast, VNIR spectra often yield non-unique mineralogic interpretations due to overlapping absorption bands from olivine, glass, and Fe-bearing plagioclase. In addition, we find that sub-micron oxides hosted in transparent matrix material that are common in fine-grained extrusive rocks can lower albedo and partially to fully suppress mafic absorption bands, leading to very different VNIR spectra in rocks with the same mineralogy and chemistry. Mineralogical interpretations from VNIR spectra should not be treated as rigorous petrologic indicators, but can supplement TIR-based petrology by providing unique constraints on oxide minerals, microtexture, and alteration processes.
Funding
SIGNATURES OF BASALT WEATHERING UNDER COLD AND ICY CONDITIONS ON MARS
National Aeronautics and Space Administration
Find out more...THE SURFACE OF MARS EXHIBITS CLEAR GEOMORPHIC EVIDENCE FOR EXTENSIVE PAST GLACIATION, BUT THE ROLE OF GLACIERS IN THE GEOCHEMICAL HISTORY OF MARS IS NOT WELL UNDERSTOOD. ON EARTH, THE LOW TEMPERATURE AND ANOXIC CONDITIONS OF SUBGLACIAL ENVIRONMENTS PROMOT
National Aeronautics and Space Administration
Find out more...THE INDIANA SPACE GRANT CONSORTIUM (INSGC) CONSISTS OF 25 ACADEMIC (COLLEGES AND UNIVERSITIES) AND OUTREACH (MUSEUMS AND SCIENCE CENTERS) AFFILIATES WHO WORK TOGETHER TO PROMOTE STEM EDUCATION INITIATIVES RELATED TO NASA THEMES AND CAREERS IN THE STATE OF
National Aeronautics and Space Administration
Find out more...History
Degree Type
- Master of Science
Department
- Earth, Atmospheric and Planetary Sciences
Campus location
- West Lafayette