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Detection and discrimination of sulfate minerals using reflectance spectroscopy

  • Edward A. Cloutis
  • , Frank C. Hawthorne
  • , Stanley A. Mertzman
  • , Katherine Krenn
  • , Michael A. Craig
  • , Dionne Marcino
  • , Michelle Methot
  • , Johnathon Strong
  • , John F. Mustard
  • , Diana L. Blaney
  • , James F. Bell
  • , Faith Vilas

Research output: Contribution to journalArticlepeer-review

Abstract

A suite of sulfate minerals were characterized spectrally, compositionally, and structurally in order to develop spectral reflectance-compositional-structural relations for this group of minerals. Sulfates exhibit diverse spectral properties, and absorption-band assignments have been developed for the 0.3-26 μm range. Sulfate absorption features can be related to the presence of transition elements, OH, H2O, and SO4 groups. The number, wavelength position, and intensity of these bands are a function of both composition and structure. Cation substitutions can affect the wavelength positions of all major absorption bands. Hydroxo-bridged Fe3+ results in absorption bands in the 0.43, 0.5, and 0.9 μm regions, while the presence of Fe2+ results in absorption features in the 0.9-1.2 μm interval. Fundamental S{single bond}O bending and stretching vibration absorption bands occur in the 8-10, 13-18, and 19-24 μm regions (1000-1250, 550-770, and 420-530 cm-1). The most intense combinations and overtones of these fundamentals are found in the 4-5 μm (2000-2500 cm-1) region. Absorption features seen in the 1.7-1.85 μm interval are attributable to H{single bond}O{single bond}H/O{single bond}H bending and translation/rotation combinations, while bands in the 2.1-2.7 μm regions can be attributed to H2O- and OH-combinations as well as overtones of S{single bond}O bending fundamentals. OH- and H2O-bearing sulfate spectra are fundamentally different from each other at wavelengths below ∼6 μm. Changes in H2O/OH content can shift S{single bond}O band positions due to change in bond lengths and structural rearrangement. Differences in absorption band wavelength positions enable discrimination of all the sulfate minerals used in this study in a number of wavelength intervals. Of the major absorption band regions, the 4-5 μm region seems best for identifying and discriminating sulfates in the presence of other major rock-forming minerals.

Original languageEnglish (US)
Pages (from-to)121-157
Number of pages37
JournalIcarus
Volume184
Issue number1
DOIs
StatePublished - Sep 2006
Externally publishedYes

Keywords

  • Asteroids
  • Europa
  • Mars
  • Meteorites
  • Mineralogy
  • Spectroscopy
  • composition
  • surface

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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