Analyses of enriched mantle (EM)-basalts, using lithophile element-based isotope systems, have long provided evidence for discrete mantle reservoirs with variable composition. Upon partial melting, the mantle reservoir imparts its isotopic fingerprint upon the partial melt produced. However, it has increasingly been recognised that it may not be simple to delimit these previously well-defined mantle reservoirs; the "mantle zoo" may contain more reservoirs than previously envisaged. Here we demonstrate that a simple model with varying contributions from two populations of compositionally distinct mantle sulphides can readily account for the observed heterogeneities in Os isotope systematics of such basalts without additional mantle reservoirs. Osmium elemental and isotopic analyses of individual sulphide grains separated from spinel lherzolites from Kilbourne Hole, New Mexico, USA demonstrate that two discrete populations of mantle sulphide exist in terms of both Re-Os systematics and textural relationship with co-existing silicates. One population, with a rounded morphology, is preserved in silicate grains and typically possesses high [Os] and low [Re] with unradiogenic, typically sub-chondritic Os-187/(188) Os attributable to long term isolation in a low-Re environment. By contrast, irregular-shaped sulphides, preserved along silicate grain boundaries, possess low [Os], higher [Re] and a wider range of, but generally supra-chondritic Os-187/Os-188 ([Os] typically <= 1-2 ppm, Os-187/Os-188 <= 0.3729; this study). This population is thought to represent metasomatic sulphide. Uncontaminated silicate phases contain negligible Os (<100 ppt) therefore the Os elemental and isotope composition of basalts is dominated by volumetrically insignificant sulphide ([Os] <= 37 ppm; this study). During the early stages of partial melting, supra-chondritic interstitial sulphides are mobilised and incorporated into the melt, adding their radiogenic Os-187/Os-188 signature. Only when sulphides armoured within silicates are exposed to the melt through continued partial melting will enclosed sulphides add their high [Os] and unradiogenic Os-187/Os-188 to the aggregate melt. Platinum-group element data for whole rocks are also consistent with this scenario. The sequence of (i) addition of all of the metasomatic sulphide, followed by (ii) the incorporation of small amounts of armoured sulphide can thus account for the range of both [Os] and Os-187/Os-188 of EM-basalts worldwide without the need for contributions from additional silicate mantle reservoirs. (C) 2011 Elsevier Ltd. All rights reserved.
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Univ Montpellier 2, Geosci Montpellier, UMR 5243, CC 60,CNRS, Place E Bataillon, F-34095 Montpellier, France
Macquarie Univ, Dept Earth & Planetary Sci, GEMOC ARC Natl Key Ctr, Sydney, NSW 2109, AustraliaUniv Montpellier 2, Geosci Montpellier, UMR 5243, CC 60,CNRS, Place E Bataillon, F-34095 Montpellier, France
Marchesi, Claudio
Griffin, William L.
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Macquarie Univ, Dept Earth & Planetary Sci, GEMOC ARC Natl Key Ctr, Sydney, NSW 2109, AustraliaUniv Montpellier 2, Geosci Montpellier, UMR 5243, CC 60,CNRS, Place E Bataillon, F-34095 Montpellier, France
Griffin, William L.
Garrido, Carlos J.
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Univ Granada, CSIC, Inst Andaluz Ciencias Tierra IACT, Granada 18002, SpainUniv Montpellier 2, Geosci Montpellier, UMR 5243, CC 60,CNRS, Place E Bataillon, F-34095 Montpellier, France
Garrido, Carlos J.
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Bodinier, Jean-Louis
O'Reilly, Suzanne Y.
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Macquarie Univ, Dept Earth & Planetary Sci, GEMOC ARC Natl Key Ctr, Sydney, NSW 2109, AustraliaUniv Montpellier 2, Geosci Montpellier, UMR 5243, CC 60,CNRS, Place E Bataillon, F-34095 Montpellier, France
O'Reilly, Suzanne Y.
Pearson, Norman J.
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Macquarie Univ, Dept Earth & Planetary Sci, GEMOC ARC Natl Key Ctr, Sydney, NSW 2109, AustraliaUniv Montpellier 2, Geosci Montpellier, UMR 5243, CC 60,CNRS, Place E Bataillon, F-34095 Montpellier, France
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Univ Montpellier 2, Geosci Montpellier, UMR 5243, CC 60,CNRS, Place E Bataillon, F-34095 Montpellier, France
Macquarie Univ, Dept Earth & Planetary Sci, GEMOC ARC Natl Key Ctr, Sydney, NSW 2109, AustraliaUniv Montpellier 2, Geosci Montpellier, UMR 5243, CC 60,CNRS, Place E Bataillon, F-34095 Montpellier, France
Marchesi, Claudio
Griffin, William L.
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Macquarie Univ, Dept Earth & Planetary Sci, GEMOC ARC Natl Key Ctr, Sydney, NSW 2109, AustraliaUniv Montpellier 2, Geosci Montpellier, UMR 5243, CC 60,CNRS, Place E Bataillon, F-34095 Montpellier, France
Griffin, William L.
Garrido, Carlos J.
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Univ Granada, CSIC, Inst Andaluz Ciencias Tierra IACT, Granada 18002, SpainUniv Montpellier 2, Geosci Montpellier, UMR 5243, CC 60,CNRS, Place E Bataillon, F-34095 Montpellier, France
Garrido, Carlos J.
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Bodinier, Jean-Louis
O'Reilly, Suzanne Y.
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Macquarie Univ, Dept Earth & Planetary Sci, GEMOC ARC Natl Key Ctr, Sydney, NSW 2109, AustraliaUniv Montpellier 2, Geosci Montpellier, UMR 5243, CC 60,CNRS, Place E Bataillon, F-34095 Montpellier, France
O'Reilly, Suzanne Y.
Pearson, Norman J.
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Macquarie Univ, Dept Earth & Planetary Sci, GEMOC ARC Natl Key Ctr, Sydney, NSW 2109, AustraliaUniv Montpellier 2, Geosci Montpellier, UMR 5243, CC 60,CNRS, Place E Bataillon, F-34095 Montpellier, France