Quantification of Crystal Chemistry of Fe-Mg Carbonates by Raman Microspectroscopy and Near-Infrared Remote Sensing

被引:1
|
作者
Beck, Pierre [1 ]
Beyssac, Olivier [2 ]
Schmitt, Bernard [1 ]
Royer, Clement [3 ]
Mandon, Lucia [1 ]
Boulard, Eglantine [2 ]
Rividi, Nicolas [2 ]
Cloutis, Edward A. [4 ]
机构
[1] Univ Grenoble Alpes, CNRS, IPAG, Grenoble, France
[2] Sorbonne Univ, Museum Natl Hist Nat, CNRS, UMR 7590,Inst Mineral Phys Mat & Cosmochim, Paris, France
[3] Paris Saclay Univ, CNRS, Inst Astrophys Spatiale, Paris, France
[4] Univ Winnipeg, Dept Geog, Winnipeg, MB, Canada
关键词
Mars; asteroid; carbonate; Raman; infrared; CALCITE; IDENTIFICATION; REFLECTANCE; SPECTRA; ORIGIN;
D O I
10.1029/2024EA003666
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
On Earth, carbonate minerals are widely used as recorders of the geological environments in which they formed. Here, we present a method designed to retrieve the crystal chemistry of Fe-Mg carbonate minerals using infrared remote sensing or Raman spectroscopy. We analyzed a suite of well-characterized Fe-Mg carbonate minerals for which Raman spectra were obtained in two different laboratories, and IR spectra were measured in reflectance and transmission from the visible range to 25-mu m. We built calibration lines for the dependence of fundamental and harmonic vibrational modes position to the Mg# (defined as Mg# = 100 x Mg/(Mg + Fe + Ca + Mn)). These calibrations should enable retrieval of Mg# based on spectroscopic observations with a typical accuracy of 10. We discuss the framework of applicability of these calibrations and apply them to a typical CRISM spectrum of carbonates from the Nilli Fossae region of Mars. Fundamental FeMg carbonate mode position have a linear dependence to Mg# for Fe-Mg carbonate mineral Harmonic bands at 2.3 and 2.5 also have a linear dependence of their position with Mg# for Fe-Mg carbonate minerals We present calibration curves of Mg# versus fundamental and harmonic vibration position than can be used to retrieve crystal chemistry
引用
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页数:16
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