TY - JOUR
T1 - Carbonatitic mineralogy of natural diamond-forming fluids
AU - Kopylova, M.
AU - Navon, O.
AU - Dubrovinsky, L.
AU - Khachatryan, G.
PY - 2010/3/1
Y1 - 2010/3/1
N2 - A suite of 20 cuboid fibrous diamonds from the Democratic Republic of Congo was studied to determine mineral phases crystallized from diamond-forming fluids that were trapped as inclusions in diamonds. We identified minerals and non-crystalline components using their compositional trends in the electron microprobe analyses of inclusions, an innovative bulk X-ray diffraction analysis and characteristic FTIR and Raman peaks. The DRC diamonds contain fluid inclusions of the Ca-carbonatitic-silicic composition. Most common phases precipitated from the fluid are found to be high-Si micas (90-30% of the solids volume), complex non-crystalline Na-Ca-Mg-Fe carbonate matter and apatite (together 5-70%), leaving a residual aqueous solution of K, Cl and carbonate ions and gaseous CO2. A notable absence of carbonate minerals in bulk X-ray diffraction patterns combined with the vibrational spectroscopy observations on the C-O bonds indicates that C may be included in dissolved or amorphous carbonate matter. The modes of the most abundant phases are controlled by chemical trends of the bulk fluid compositions. Other relatively rare ∼ 30 minerals, including various minerals with structural and coordinated H2O, are detected by the vibrational spectroscopic and X-ray analyses. The fluid also contains some hydrocarbons associated with the carbonate material. The presence of some rare minerals and exotic compositions of solid-solution minerals in the fluid suggest crystallization from a closed system with high salinity-high aH2O-high aCO2 composition that persisted to relatively low temperatures and pressures. The bulk of the fluid crystallized in the diamond stability field (P < 7 GPa, T < 950 °C), but continued to form hydrocarbons, accessory and deuteric phases down to 200 °C and 0.2 GPa. Overall, the mineralogy of the fluid resembles carbonatite.
AB - A suite of 20 cuboid fibrous diamonds from the Democratic Republic of Congo was studied to determine mineral phases crystallized from diamond-forming fluids that were trapped as inclusions in diamonds. We identified minerals and non-crystalline components using their compositional trends in the electron microprobe analyses of inclusions, an innovative bulk X-ray diffraction analysis and characteristic FTIR and Raman peaks. The DRC diamonds contain fluid inclusions of the Ca-carbonatitic-silicic composition. Most common phases precipitated from the fluid are found to be high-Si micas (90-30% of the solids volume), complex non-crystalline Na-Ca-Mg-Fe carbonate matter and apatite (together 5-70%), leaving a residual aqueous solution of K, Cl and carbonate ions and gaseous CO2. A notable absence of carbonate minerals in bulk X-ray diffraction patterns combined with the vibrational spectroscopy observations on the C-O bonds indicates that C may be included in dissolved or amorphous carbonate matter. The modes of the most abundant phases are controlled by chemical trends of the bulk fluid compositions. Other relatively rare ∼ 30 minerals, including various minerals with structural and coordinated H2O, are detected by the vibrational spectroscopic and X-ray analyses. The fluid also contains some hydrocarbons associated with the carbonate material. The presence of some rare minerals and exotic compositions of solid-solution minerals in the fluid suggest crystallization from a closed system with high salinity-high aH2O-high aCO2 composition that persisted to relatively low temperatures and pressures. The bulk of the fluid crystallized in the diamond stability field (P < 7 GPa, T < 950 °C), but continued to form hydrocarbons, accessory and deuteric phases down to 200 °C and 0.2 GPa. Overall, the mineralogy of the fluid resembles carbonatite.
KW - X-ray diffraction
KW - carbonatite
KW - diamond
KW - fluid inclusion
KW - mineralogy
KW - vibrational spectroscopy
UR - http://www.scopus.com/inward/record.url?scp=75949116415&partnerID=8YFLogxK
U2 - 10.1016/j.epsl.2009.12.056
DO - 10.1016/j.epsl.2009.12.056
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AN - SCOPUS:75949116415
SN - 0012-821X
VL - 291
SP - 126
EP - 137
JO - Earth and Planetary Science Letters
JF - Earth and Planetary Science Letters
IS - 1-4
ER -