Title of article :
Experimental study of trace element partitioning between lunar orthopyroxene and anhydrous silicate melt: Effects of lithium and iron
Author/Authors :
van Kan Parker، نويسنده , , Mirjam and Mason، نويسنده , , Paul R.D. and van Westrenen، نويسنده , , Wim، نويسنده ,
Issue Information :
روزنامه با شماره پیاپی سال 2011
Pages :
14
From page :
1
To page :
14
Abstract :
Orthopyroxene (Opx) was present during a significant portion of crystallisation of the lunar magma ocean, but its influence on co-existing melt trace element contents is not well quantified. We performed high-pressure (P, 1.1 to 3.2 GPa), high-temperature (T, 1400 to 1600 °C) experiments on synthetic Fe-rich compositions at reducing conditions relevant to the lunar mantle to constrain trace element partitioning between Opx and anhydrous silicate melts. Opx–melt partition coefficients (DOpx-melt) for a wide range of trace elements (LILE: Li, Ba; REE: La, Ce, Nd, Sm, Dy, Eu, Er, Tm Y, Yb, Lu; HFSE: Zr, Nb, Hf, Ta, Th, U); and transition metals (Sc, V, Mn, Co, Mo) show only very minor variations across the considered P–T range. REE partition coefficients increase from DLaopx-melt = 0.0014 ± 0.0008 to DLuopx-melt = 0.051 ± 0.007. D values for highly charged elements vary from DThopx-melt = 0.0013 ± 0.0008 through DNbopx-melt = 0.0018 ± 0.0006 and DUopx-melt = 0.0015 ± 0.0006 to DTiopx-melt = 0.068 ± 0.0010. DLuopx-melt/DHfopx-melt values of 6.3 ± 2.4 are at the high end of reported values for minerals that played a role during crystallisation of the lunar magma ocean, and higher than previously reported for Opx under identical oxygen fugacity conditions, implying Opx-rich cumulates in the lunar mantle have highly superchondritic Lu–Hf ratios. e strain modelling of our REE partitioning data suggests that varying the concentration of divalent Fe in Opx very slightly decreases the ideal cation radius for M3+ elements entering the M2 site, r0M2, whereas the partitioning of M3+ elements entering the M1 site is unaffected. A subtle increase in the maximum partition coefficient for M3+ elements entering both the M1 and M2 sites with decreasing T is identified, when experiments carried out at similar reducing oxygen fugacities are considered. The presence of Li at concentrations of up to ~ 350 ppm does not have a measureable effect on the Opx–melt partitioning behaviour of REE or any other element, showing that charge-balancing of M3+, M4+ and M5+ elements in Opx is likely dominated by a vacancy mechanism.
Keywords :
High-pressure–temperature experiments , Lunar magma ocean , Orthopyroxene , partition coefficient , Substitution mechanisms
Journal title :
Chemical Geology
Serial Year :
2011
Journal title :
Chemical Geology
Record number :
2260447
Link To Document :
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