P43D-2154
Characterizing Amorphous Silicates in Extraterrestrial Materials

Thursday, 17 December 2015
Poster Hall (Moscone South)
Xiaohui Fu, National Astronomical Observatories, Beijing, China, Alian Wang, Washington University in St. Louis, Dept. Earth and Planetary Sciences and McDonnell Center for Space Sciences, St. Louis, MO, United States and Michael J Krawczynski, Department of Geological Sci, Cleveland, OH, United States
Abstract:
Amorphous silicates are common in extraterrestrial materials. They are seen in the matrix of carbonaceous chondrites as well as in planetary materials. Tagish Lake is one of the most primitive carbonaceous meteorites in which TEM and XRD analyses found evidence for poorly crystalline phyllosilicate-like species; Raman spectra revealed amorphous silicates with variable degree of polymerization and low crystallinity. On Mars, CheMin discovered amorphous phases in all analyzed samples, and poorly crystalline smectite in mudstone samples. These discoveries pose questions on the crystallinity of phyllosilicates found by remote sensing on Mars, which is directly relevant to aqueous alteration during geologic history of Mars.

Our goal is to use spectroscopy to better characterize amorphous silicates. We use three approaches: (1) using silicate glasses synthesized with controlled chemistry to study the effects of silicate polymerization and (2) using phyllosilicates synthesized with controlled hydrothermal treatment to study the effect of crystallinity on vibrational spectroscopy, finally (3) to use the developed correlations in above two steps to study amorphous phases in meteorites, and those found in future missions to Mars.

In the 1st step, silicate glasses were synthesized from pure oxides in a range of NBO/T ratios (from 0 to 4). Depending on the targeted NBO/T and composition of mixed oxides, temperatures for each experiment fell in a range from 1260 to 1520 °C, run for ~ 4 hrs. The melt was quenched in liquid N2 or water. Homogeneity of glass was checked under optical microscopy. Raman spectra were taken over 100 spots on small chips free of bubbles and crystals. We have observed that accompanying an increase of NBO/T, there is a strengthening and a position shift of the Raman peak near 1000 cm-1 (Si-Onon-bridging stretching mode), and the weakening of broad Raman peaks near 500 cm-1 (ring breathing mode) and 700cm-1 (Si-Obridging-Si mode). We are building the correlation between peak area ratio, A(500+700)/A1000, and NBO/T.

In the 2nd step, we are synthesizing Mg-saponite using a sol-gel method. The crystallinity of sol-gel starting materials will be increased by a controlled hydrothermal treatment. The products will be characterized using XRD/TEM/Raman/NIR. The results will be reported at the conference.

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