1. Raman spectra of Martian glass analogues: A tool to approximate their chemical composition
- Author
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Claudia Romano, Donald B. Dingwell, Werner Ertel-Ingrisch, Alessandro Vona, Daniel R. Neuville, Kai-Uwe Hess, S. Kolzenburg, Magdalena Oryaëlle Chevrel, Danilo Di Genova, Università degli Studi Roma Tre, Ludwig-Maximilians-Universität München (LMU), Institut de Physique du Globe de Paris (IPGP), Centre National de la Recherche Scientifique (CNRS)-Université de La Réunion (UR)-Université Paris Diderot - Paris 7 (UPD7)-IPG PARIS-Institut national des sciences de l'Univers (INSU - CNRS), Dipartimento di Scienze Geologiche [Roma TRE], Department of Earth and Environmental Sciences [Munich], Università degli studi di Torino (UNITO), Laboratoire Magmas et Volcans (LMV), Institut national des sciences de l'Univers (INSU - CNRS)-Université Jean Monnet [Saint-Étienne] (UJM)-Institut de Recherche pour le Développement et la société-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Centre National de la Recherche Scientifique (CNRS)-Observatoire de Physique du Globe de Clermont-Ferrand (OPGC), Institut national des sciences de l'Univers (INSU - CNRS)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Centre National de la Recherche Scientifique (CNRS), Università degli Studi Roma Tre = Roma Tre University (ROMA TRE), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Jean Monnet [Saint-Étienne] (UJM)-Institut de Recherche pour le Développement et la société-Université Clermont Auvergne (UCA)-Centre National de la Recherche Scientifique (CNRS)-Observatoire de Physique du Globe de Clermont-Ferrand (OPGC), Institut national des sciences de l'Univers (INSU - CNRS)-Université Clermont Auvergne (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Università degli studi di Torino = University of Turin (UNITO), Institut national des sciences de l'Univers (INSU - CNRS)-Université Jean Monnet - Saint-Étienne (UJM)-Institut de Recherche pour le Développement et la société-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Centre National de la Recherche Scientifique (CNRS)-Observatoire de Physique du Globe de Clermont-Ferrand (OPGC), Di Genova, Danilo, Kolzenburg, Stephan, Vona, Alessandro, Chevrel, Magdalena Oryaëlle, Hess, Kai Uwe, Neuville, Daniel R., Ertel Ingrisch, Werner, Romano, Claudia, and Dingwell, Donald B.
- Subjects
Atmospheric Science ,010504 meteorology & atmospheric sciences ,Planetary Volcanism ,Oceanography ,010502 geochemistry & geophysics ,01 natural sciences ,Microanalysis ,Peralkaline rock ,remote sensing ,Planetary Sciences: Solar System Objects ,[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/Geochemistry ,Earth and Planetary Sciences (miscellaneous) ,Chemical composition ,Experimental Volcanism ,Research Articles ,Water Science and Technology ,Melt inclusions ,Martian ,Ecology ,Remote Sensing and Disasters ,Forestry ,Mars Exploration Program ,Mar ,Geophysics ,Raman spectroscopy ,symbols ,Planetary Sciences: Comets and Small Bodies ,Chemical analysis ,Glasses ,Mars ,Remote sensing ,Volcanology ,Geochemistry and Petrology ,Space and Planetary Science ,Geology ,Research Article ,glasse ,Soil Science ,Mineralogy ,Aquatic Science ,glasses ,symbols.namesake ,volcanology ,Volcanism ,[SDU.STU.VO]Sciences of the Universe [physics]/Earth Sciences/Volcanology ,Remote Sensing of Volcanoes ,Geophysic ,Planetary Sciences: Solid Surface Planets ,0105 earth and related environmental sciences ,Spectrometer ,Paleontology ,Tectonophysics ,13. Climate action ,Earth-Surface Processe ,chemical analysis ,chemical analysi ,Natural Hazards - Abstract
Raman spectrometers will form a key component of the analytical suite of future planetary rovers intended to investigate geological processes on Mars. In order to expand the applicability of these spectrometers and use them as analytical tools for the investigation of silicate glasses, a database correlating Raman spectra to glass composition is crucial. Here we investigate the effect of the chemical composition of reduced silicate glasses on their Raman spectra. A range of compositions was generated in a diffusion experiment between two distinct, iron‐rich end‐members (a basalt and a peralkaline rhyolite), which are representative of the anticipated compositions of Martian rocks. Our results show that for silica‐poor (depolymerized) compositions the band intensity increases dramatically in the regions between 550–780 cm−1 and 820–980 cm−1. On the other hand, Raman spectra regions between 250–550 cm−1 and 1000–1250 cm−1 are well developed in silica‐rich (highly polymerized) systems. Further, spectral intensity increases at ~965 cm−1 related to the high iron content of these glasses (~7–17 wt % of FeOtot). Based on the acquired Raman spectra and an ideal mixing equation between the two end‐members we present an empirical parameterization that enables the estimation of the chemical compositions of silicate glasses within this range. The model is validated using external samples for which chemical composition and Raman spectra were characterized independently. Applications of this model range from microanalysis of dry and hydrous silicate glasses (e.g., melt inclusions) to in situ field investigations and studies under extreme conditions such as extraterrestrial (i.e., Mars) and submarine volcanic environments., Key Points Raman spectra of glasses are presented for a large range of chemical compositions, analogous to Martian compositionsSpectral intensities are parameterized to derive a model for estimation of the glass composition from Raman spectraThis enables in situ estimations of glass compositions in extraterrestrial or submarine volcanic settings
- Published
- 2016