4.2 Article Proceedings Paper

Mineral inclusions in diamonds from Karowe Mine, Botswana: super-deep sources for super-sized diamonds?

Journal

MINERALOGY AND PETROLOGY
Volume 112, Issue -, Pages 169-180

Publisher

SPRINGER WIEN
DOI: 10.1007/s00710-018-0604-9

Keywords

Zimbabwe Craton; Orapa kimberlite cluster; Sublithospheric; Majorite

Funding

  1. Government of Botswana as part of Pre-University Academic Programmes under Botswana International University of Science and Technology (BIUST)
  2. Natural Sciences and Engineering Research Council (NSERC)
  3. Canada Research Chairs program

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Mineral inclusions in diamonds play a critical role in constraining the relationship between diamonds and mantle lithologies. Here we report the first major and trace element study of mineral inclusions in diamonds from the Karowe Mine in north-east Botswana, along the western edge of the Zimbabwe Craton. From a total of 107 diamonds, 134 silicate, 15 oxide, and 22 sulphide inclusions were recovered. The results reveal that 53% of Karowe inclusion-bearing diamonds derived from eclogitic sources, 44% are peridotitic, 2% have a sublithospheric origin, and 1% are websteritic. The dominant eclogitic diamond substrates sampled at Karowe are compositionally heterogeneous, as reflected in wide ranges in the CaO contents (4-16wt%) of garnets and the Mg# (69-92) and jadeite contents (14-48mol%) of clinopyroxenes. Calculated bulk rock REEN patterns indicate that both shallow and deep levels of the subducted slab(s) were sampled, including cumulate-like protoliths. Peridotitic garnet compositions largely derive from harzburgite/dunite substrates (90%), with almost half the garnets having CaO contents <1.8wt%, consistent with pyroxene-free (dunitic) sources. The highly depleted character of the peridotitic diamond substrates is further documented by the high mean and median Mg# (93.1) of olivine inclusions. One low-Ca garnet records a very high Cr2O3 content (14.7wt%), implying that highly depleted cratonic lithosphere at the time of diamond formation extended to at least 220km depth. Inclusion geothermobarometry indicates that the formation of peridotitic diamonds occurred along a 39-40mW/m(2) model geotherm. A sublithospheric inclusion suite is established by three eclogitic garnets containing a majorite component, a feature so far unique within the Orapa cluster. These low- and high-Ca majoritic garnets follow pyroxenitic and eclogitic trends of majoritic substitution, respectively. The origin of the majorite-bearing diamonds is estimated to be between 330 to 420km depth, straddling the asthenosphere-transition zone boundary. This new observation of superdeep mineral inclusions in Karowe diamonds is consistent with a sublithospheric origin for the exceptionally large diamonds from this mine.

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