Oxygen Isotope Composition of the Silicate Minerals and Chrome Ores in the Guleman Ophiolite in Southeastern Türkiye
Oxygen crystallising was obtained from olivine, chromite separates from host rock samples, and gabbro from ultramafic cumulates, harzburgite, and dunite samples collected from tectonites of the Guleman ophiolites. The study includes the oxygen isotope compositions from the Guleman ophiolite and the...
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Published in | Doklady earth sciences Vol. 515; no. 2; pp. 722 - 733 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
Moscow
Pleiades Publishing
01.04.2024
Springer Nature B.V |
Subjects | |
Online Access | Get full text |
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Summary: | Oxygen crystallising was obtained from olivine, chromite separates from host rock samples, and gabbro from ultramafic cumulates, harzburgite, and dunite samples collected from tectonites of the Guleman ophiolites. The study includes the oxygen isotope compositions from the Guleman ophiolite and the evolutionary scenarios of geochemical and isotopic signatures. The olivine and chromitite δ
18
O
olivine/chromite
and δ
18
O
melt
values point out these minerals and melt isotopic compositions similar to mantle values and rich, heavy stable isotopes. The highest δ
18
O
chromite
isotopic composition values indicate that as the heavy isotope in the melt increases, the concentration in the mineral increases. Excluding a dunite sample, the values of the δ
18
O
whole rock
of the dunite and pyroxenite samples are similar to mantle values. The gabbro samples have higher δ
18
O
whole rock
values than the two harzburgites. Hereby, the chromite formations are the later fractional crystallisation products than olivine and dunites due to the lowering of δ
18
O. The lower oxygen isotopic composition in studied samples than the normal mantle values, and these values point out subducted hydrothermally alteration. The higher δ
18
O isotopic compositions could be explained by serpentinization on the ocean floor at low temperatures. |
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ISSN: | 1028-334X 1531-8354 |
DOI: | 10.1134/S1028334X23602651 |