Graphite to diamond transformation during sediment–peridotite interaction at 7.5 and 10.5 GPa
Autor: | Gerhard P. Brey, Alan B. Woodland, Andrei V. Girnis, Heidi E. Höfer, V.K. Bulatov |
---|---|
Rok vydání: | 2018 |
Předmět: |
Peridotite
Recrystallization (geology) 010504 meteorology & atmospheric sciences Nucleation Geochemistry Diamond Geology engineering.material 010502 geochemistry & geophysics 01 natural sciences Silicate chemistry.chemical_compound Chemical engineering chemistry Geochemistry and Petrology engineering Graphite Dissolution 0105 earth and related environmental sciences Magnesite |
Zdroj: | Lithos. :302-313 |
ISSN: | 0024-4937 |
DOI: | 10.1016/j.lithos.2018.04.010 |
Popis: | Diamond nucleation and growth were investigated experimentally at 7.5 and 10.5 GPa and temperatures up to 1500 °C. Samples consisted of two layers: i) H2O- and CO2-bearing model sediment and ii) graphite-bearing garnet harzburgite comprising natural minerals. Two experimental series were conducted, one under a controlled temperature gradient with the sedimentary layer usually in the cold zone and the other under isothermal conditions. In the latter case, diamond seeds were added to the sedimentary mixture. During the experiments, the sedimentary layer partially or completely melted, with the melt percolating and interacting with the adjacent harzburgite. The graphite-to-diamond transition in the peridotite was observed above 1300 °C at 7.5 GPa and 1200 °C at 10.5 GPa in the temperature-gradient experiments, and at temperatures ~100 °C lower in the isothermal experiments with diamond seeds. Newly formed diamond occurs mostly as individual grains up to 10 μm in size and is separate from graphite aggregates. In some cases, an association of diamond with magnesite was observed. Diamond nucleation occurs in hydrous and CO2-bearing silicate melt following graphite dissolution and recrystallization. In the case of the diamond–magnesite association, diamond was probably formed through carbonate reduction coupled with graphite oxidation. The composition of the melts ranged from “carbonatitic” with ~10 wt% SiO2 and >50 wt% volatiles to hydrous silicate with ~40 wt% SiO2 and |
Databáze: | OpenAIRE |
Externí odkaz: |