4.7 Article

Sulfide and whole rock Re-Os systematics of eclogite and pyroxenite xenoliths from the Slave Craton, Canada

Journal

EARTH AND PLANETARY SCIENCE LETTERS
Volume 283, Issue 1-4, Pages 48-58

Publisher

ELSEVIER
DOI: 10.1016/j.epsl.2009.03.023

Keywords

Re-Os isotopes; kimberlite-borne xenolith; eclogite; pyroxenite; sulfide petrology; Slave Craton

Funding

  1. NSERC
  2. Diavik Diamond Mines Inc.
  3. Macquarie University International Postgraduate Award and Postgraduate Research Fund (SA)
  4. Kennecott Canada Inc.
  5. ARC Large and Discovery Grants
  6. ARC LIEF
  7. DEST Systemic Infrastructure Grants

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We characterized single sulfides in eclogite and pyroxenite xenoliths from the Diavik kimberlites (central Slave Craton, Canada) with regard to their petrography, major-element composition and Re-Os isotope systematics. Together with trace-element and Re-Os isotope compositions of whole rocks, these data allow identification of the major Re-Os host phases and provide constraints on the origin(s) of sulfides in these samples. The majority of sulfide minerals contain 8 to 28 at.% Ni, with intragranular sulfides having on average significantly lower contents (similar to 6 at.%) than intergranular sulfides (similar to 12 at.%). These high Ni-sulfides are not in equilibrium with an eclogitic assemblage and were likely introduced from a peridotitic source subsequent to eclogite formation. In contrast, their Re-Os abundances and Re/Os ratios (average similar to 825 ppb, 190 ppb and 10, respectively) overlap those of primary eclogitic sulfides. These conflicting compositional characteristics may document open-system disequilibrium processes accompanying the introduction of sulfides into eclogites. The general association of high Os-187/Os-188 with high Re-187/Os-188 of sulfides in three low-temperature eclogite xenoliths suggests that the addition is not young. In contrast, sulfides in a high-temperature eclogite plot on a similar to 90 Ma errorchron with radiogenic initial Os-187/Os-188, perhaps indicative of young introduction of sulfides from a deep enriched source. Sulfides in a single pyroxenite xenolith have Ni, Re and Os contents intermediate between pristine eclogitic and peridotitic sulfides, and correlated Re-Os isotope systematics defining an age of 1.84 +/- 0.14 Ga with a radiogenic Os-187/Os-188, (0.16 +/- 0.01). The age and Os-187/Os-188(i) are identical to those obtained for eclogitic sulfide inclusions in diamonds from Diavik, thus supporting a link between eclogite and pyroxenite formation. Several eclogite and pyroxenite whole rocks show evidence for addition of secondary sulfides, but many plot on Paleoproterozoic Re-Os age arrays - particularly so at low Re/Os - coincident with previously determined ages using Lu-Hf and Pb-Pb techniques. They may represent sulfide-poor varieties that did not suffer secondary sulfide addition and that may be best suited to yielding meaningful Re-Os ages. (C) 2009 Elsevier B.V. All rights reserved.

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