Os isotope heterogeneity of the upper mantle: Evidence from the Mayari-Baracoa ophiolite belt in eastern Cuba

被引:30
|
作者
Frei, R
Gervilla, F
Meibom, A
Proenza, JA
Garrido, CJ
机构
[1] Univ Copenhagen, Inst Geol, DK-1350 Copenhagen, Denmark
[2] Univ Granada, CSIC, Fac Ciencias, Dept Mineral & Petrol, Granada 18002, Spain
[3] Univ Granada, CSIC, Fac Ciencias, Inst Andaluz Ciencias Tierra, Granada 18002, Spain
[4] Museum Natl Hist Nat, Lab Etud Mat Extraterrestre, USM 0205, F-75005 Paris, France
[5] Univ Barcelona, Fac Geol, Dept Cristallog Mineral & Diposits Minerals, E-08028 Barcelona, Spain
关键词
Os isotopes; chromite; ophiolite; SUMA; Cuba;
D O I
10.1016/j.epsl.2005.11.043
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
In an attempt to quantify the extent of geochemical heterogeneity within a restricted and well dated portion of the upper mantle, 27 chromite separates from the 90 My old chromite deposits in the Mayari-Baracoa ophiolite belt in eastern Cuba have been investigated for platinum group element (PGE) concentrations and Re-Os isotopic systematics. The samples are characterized by systematically subchondritic initial Os-187/Os-188 ratios and substantial heterogeneity. The initial Os-187/Os-188 ratios vary with chromite chemistry and with geographical distribution, reflecting differences in the Os isotopic evolution for the different upper mantle sections represented by the ophiolite. Accordingly, the Os isotope data might be divided into three groups. In the Moa-Baracoa district, where the chromite bodies are located in the mantle-crust transition zone, the calculated initial gamma Os values average - 0.97 +/- 0.69 (n = 13). In the Sagua de Tanamo district, where chromite chemistry is highly variable and their location in relation the mantle sequence is less clear, the initial gamma Os values are intermediate, with an average of - 1.77 +/- 0.80 (n = 7). In the Mayari district, where the chromite bodies are located in the lower part of the mantle sequence, initial gamma Os values average -2.66 +/- 0.29 (n = 7). These subchondritic (i.e. negative) initial gamma Os values are most simply explained by Re depletion during ancient partial melting and/or melt percolation events. The Os isotope heterogeneity documented here indicates a high degree of geochemical complexity on small to intermediate length scales in the upper mantle. Our results, in combination with data on chromites from the literature, show that an "average present-day Os isotopic composition" for the hypothetical depleted MORB mantle (DMM) reservoir cannot be precisely established beyond the statement that it is "broadly chondritic". Indeed, the upper mantle cannot be considered a sufficiently homogeneous geochemical "reservoir" to serve meaningfully as a baseline against which geochemical "anomalies" are evaluated. On the other hand, our findings are consistent with the "Statistical Upper Mantle Assemblage" or "SUMA"-concept, according to which a high level of geochernical heterogeneity is maintained in the upper mantle at all relevant length scales, as a result of the plate-tectonic cycle and intra-mantle processes such as melt-migration and metasomatism. (c) 2005 Elsevier B.V. All rights reserved.
引用
收藏
页码:466 / 476
页数:11
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