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Carbon and Nitrogen Isotopic, and Mineral Inclusion Studies on the Diamonds from the Pozanti‐Karsanti Chromitite, Turkey
Author(s) -
LIAN Dongyang,
YANG Jingsui,
WIEDENBECK Michael,
ROCHOLL Alexander,
DILEK Yildirim,
WU Weiwei
Publication year - 2019
Publication title -
acta geologica sinica ‐ english edition
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.444
H-Index - 61
eISSN - 1755-6724
pISSN - 1000-9515
DOI - 10.1111/1755-6724.14159
Subject(s) - ophiolite , geology , cathodoluminescence , geochemistry , chromitite , diamond , carbon fibers , mineralogy , materials science , metallurgy , composite material , paleontology , composite number , tectonics , optoelectronics , luminescence
He Pozanti‐Karsanti ophiolite (PKO) is one of the largest oceanic remnants in the Tauride belt, Turkey. Micro‐diamonds were recovered from the podiform chromitites, and these were investigated based on morphology, color, cathodoluminescence, nitrogen content, carbon and nitrogen isotopes, internal structure and inclusions. The diamonds recovered from the PKO are mainly mixed‐habit diamonds with sectors of different brightness under the cathodoluminescence images. The total δ 13 C range of the PKO diamonds ranges between −18.8 ‰ and −28.4 ‰, with a principle δ 13 C mode at −25 ‰. Nitrogen contents of the diamonds range from 7 to 541 μg/g with a mean value of 171 μg/g, and the δ 15 N values range from −19.1 ‰ to 16.6 ‰, with a δ 15 N mode of −9 ‰. Stacking faults and partial dislocations are commonly observed in the Transmission Electron Microscopy foils whereas inclusions are rather rare. Combinations of (Ca 0.81 Mn 0.19 )SiO 3 , NiMnCo‐alloy and nano‐size, quenched fluid phases were observed as inclusions in the PKO diamonds, confirming a natural origin of these diamonds. We believe that the δ 13 C‐depleted carbon signature of the PKO diamonds is a remnant of previously subducted crustal matter. These diamonds may have crystallized in metal‐rich melts in the asthenospheric mantle at depth below 250 km which were subsequently carried rapidly upward by asthenospheric melts/fliuds. We concluded that diamond‐bearing asthenospheric melts were likely involved in the formation of the Pozanti‐Karsanti podiform chromitite.