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Identification of Carbonate and Oxyhydroxide in Lunar
sample 65903, 16-7
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| Identification of siderite: The Raman
spectra taken from some grains and veins show a strong peak near 1084cm-1 indicates
the existence of (CO3)2- as major anionic group; the spectral pattern suggests a
calcite-like structure (R3-c); the positions of major peaks (near 1084, 735, 287, 188cm-1)
distinguish this carbonate to be mainly siderite composition (FeCO3), different from
calcite, magnesite, and other carbonates of similar structure. Identification
of goethite: The Raman spectra obtained from the bright rims around inner
siderite grains and along the out edges of some siderite vein show a characteristic
spectral pattern of goethite (alpha-FeOOH), with a major peak near 395cm-1 and several
minor peaks match well with the spectrum of standard goethite. No OH stretching vibration
peak in 3500-4000cm-1 spectral range were observed in both standard goethite and studied
lunar sample, caused by the non-symmetric locations of protons in goethite structure.
Another two polymorphes lepidocrocite (gama-FeOOH) and akaganeite (beta-FeOOH) have
completely different spectral patterns. |
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| Structural features of siderite and goethite -- poor
& variable crystallinity
Comparing with the Raman spectra of standard siderite and goethite, the major
peak of siderite and goethite (~1084cm-1 and 395cm-1) in studied sample are weak relative
to other minor peaks. The Raman peaks of goethite also show an obvious broadening.
These two features are sensitive to the degree of crystallinity of analyzed sample. A
general trend observed is that the siderite grains at the outside of the rock chip have
better crystallinity, the siderite identified from the "inner grains" and
from the veins have much poor crystallinity, which could be the result of a fast
solidification in a much confined space.
Compositional variation of siderite
The exact Raman peak positions of siderite vary among the spectra taken from the
different locations in the same grain or from different grains, which indicates the cation
substitutions in these siderites. |
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Reference: Ryan Zeigler et al., abstract #1243 for 32th LPSC (2001)

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