4.0 Article

Isotope fractionation of carbon during diamond crystallization in model systems

Journal

RUSSIAN GEOLOGY AND GEOPHYSICS
Volume 56, Issue 1-2, Pages 239-244

Publisher

RUSSIAN ACAD SCIENCES, SIBERIAN BRANCH, VS SOBOLEV INST GEOL & MINEROL
DOI: 10.1016/j.rgg.2015.01.017

Keywords

diamond; carbon isotopes; fractionation; experiment; high pressures; oxygen fugacity

Funding

  1. Russian Science Foundation [14-27-00054]

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A systematic experimental study of fractionation of carbon isotopes during diamond crystallization in model systems near the IW and CCO buffers helped to estimate the effective partition coefficients of carbon isotopes between diamond and crystallization medium. In the systems Fe(Ni, Co)-C, near the IW buffer, diamond is heavier than the solution of carbon in metal melt by 4.5% at 5.5 GPa and 1400-1500 degrees C. In the system (Na2CO3 center dot CO2)-C, near the CCO buffer, diamond is lighter than the carbonate fluid by 2.6% at 7.5 GPa and 1400-1700 degrees C. The values of fractionation are close but not equal to calculated equilibrium values and decrease as the rate of diamond crystallization increases. With regard to the low effectiveness of carbon isotope diffusion in diamond, the effective partition coefficients of carbon isotopes obtained during real diamond crystallization are the most informative for interpretation of data for natural diamonds. Based on the experimental results, we propose a scheme of the primary isotope specialization of diamonds. Isotopically heavy diamonds (delta C-13(VPDB) of 0 to -5%) crystallize in zones of metal melts (in the case of isotope depletion, delta C-13(VPDB) decreases to -10% or lower). Isotopically light diamonds (delta C-13(VPDB) of -7 to -10%) crystallize in more oxidized mantle zones. The interaction of different types of mantle matter with contrasting redox characteristics causes wide variations in the carbon isotope composition of diamond and in the composition of diamond-hosted inclusions. (C) 2015, V.S. Sobolev IGM, Siberian Branch of the RAS. Published by Elsevier B.V. All rights reserved.

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