Characterization of alteration products in tephra from Haleakala, Maui: A visible-infrared spectroscopy, Mossbauer spectroscopy, XRD, EMPA and TEM study

被引:41
作者
Bishop, Janice L.
Schiffman, Peter
Murad, Enver
Dyar, M. Darby
Drief, Ahmed
Lane, Melissa D.
机构
[1] SETI Inst, Mountain View, CA 94043 USA
[2] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[3] Univ Calif Davis, Dept Geol, Davis, CA 95616 USA
[4] Bayer Landesamt Umwelt, D-95603 Marktredwitz, Germany
[5] Mt Holyoke Coll, S Hadley, MA 01075 USA
[6] Clorox Co, Pleasanton, CA 94588 USA
[7] Planetary Sci Inst, Tucson, AZ 85719 USA
关键词
altered tephra; alunite; EMPA; infrared Spectroscopy; jarosite; Mars; Mossbauer; SEM; smectite; solfataric alteration; XRD; MERIDIANI-PLANUM; GUSEV CRATER; EAST MAUI; VOLCANO; SULFATE; HAWAII; IDENTIFICATION; MINERALS; HEMATITE; JAROSITE;
D O I
10.1346/CCMN.2007.0550101
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
Altered basaltic tephra from Haleakala, Maui, are characterized using multiple techniques in order to identify the minerals formed under a variety of conditions and to understand the soil formation processes here. We collected samples that are representative of typical bulk weathered material in the crater, as well as solfataric alteration in a hydrothermal environment. For this study X-ray diffraction, electron probe microanalysis, scanning electron microscopy and transmission electron microscopy are coupled with spectroscopic techniques including Mossbauer, visible-infrared reflectance, transmission infrared, and thermal infrared emission spectroscopies to analyze these samples. The unaltered tephra are composed of feldspar, glass, pyroxene and olivine. Observed alteration products include Fe oxides, phyllosilicates and sulfates, as well as SAED amorphous Al-Si-bearing material. These samples are potential analogs for altered volcanic material on Mars as the pedogenic influences and contact with plants and animals are minimal. Results from this study may help to determine spectral signatures of these samples that could be used for identification on Mars of the minerals observed here.
引用
收藏
页码:1 / 17
页数:17
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