Journal of Petrology Advance Access published online on July 20, 2005
Journal of Petrology, doi:10.1093/petrology/egi060
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1 DEPARTMENT OF TERRESTRIAL MAGNETISM, CARNEGIE INSTITUTION OF WASHINGTON, 5241 BROAD BRANCH ROAD, NW, WASHINGTON, DC 20015, USA
* To whom correspondence should be addressed. Hafnium isotope and incompatible trace element data are presented for a suite of mid-ocean ridge basalts (MORB) from 13 to 47°E on the Southwest Indian Ridge (SWIR), one of the slowest spreading and most isotopically heterogeneous mid-ocean ridges. Variations in Nd-Hf isotope compositions and Lu/Hf ratios clearly distinguish an Atlantic-Pacific-type MORB source, present west of 26°E, characterized by relatively low
Received July 6, 2004
Accepted June 10, 2005
Article
Hafnium Isotope and Trace Element Constraints on the Nature of Mantle Heterogeneity beneath the Central Southwest Indian Ridge (13°E to 47°E)
2 DEPARTMENT OF GEOLOGICAL SCIENCES, UNIVERSITY OF CAPE TOWN, PRIVATE BAG, RONDEBOSCH 7701, SOUTH AFRICA
P. E. JANNEY, E-mail: pjanney{at}fieldmuseum.org
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Abstract
Hf values for a given
Nd relative to the regression line through all Nd-Hf isotope data for oceanic basalts (termed the Nd-Hf mantle array line; the deviation from this line is termed 
Hf) and low Lu/Hf ratios, from an Indian Ocean-type MORB signature, present east of 32°E, characterized by relatively high 
Hf values and Lu/Hf ratios. Additionally, two localized, isotopically anomalous areas, at 13-15°E and 39-41°E, are characterized by distinctly low negative and high positive 
Hf values, respectively. The low 
Hf MORB from 13 to 15°E appear to reflect contamination by HIMU-type mantle from the nearby Bouvet mantle plume, whereas the trace element and isotopic compositions of MORB from 39 to 41°E are most consistent with contamination by metasomatized Archean continental lithospheric mantle. Relatively small source-melt fractionation of Lu/Hf relative to Sm/Nd, compared with MORB from faster-spreading ridges, argues against a significant role for garnet pyroxenite in the generation of most central SWIR MORB. Correlations between 
Hf and Sr and Pb isotopic and trace element ratios clearly delineate a high-
Hf Indian Ocean mantle component that can explain the isotope composition of most Indian Ocean MORB as mixtures between this component and a heterogeneous Atlantic-Pacific-type MORB source. The Hf, Nd and Sr isotope compositions of Indian Ocean MORB appear to be most consistent with the hypothesis that this component represents fragments of subduction-modified lithospheric mantle beneath Proterozoic orogenic belts that foundered into the nascent Indian Ocean upper mantle during the Mesozoic breakup of Gondwana.![]()
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