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Geology

Article: pp. 565–568 | Full Text | PDF (269K)

Subducting oceanic crust: The source of deep diamonds

Ralf Tappert1, Thomas Stachel1, Jeff W. Harris2, Karlis Muehlenbachs3, Thomas Ludwig4, and Gerhard P. Brey5

1. Department of Earth and Atmospheric Sciences, 1-26 Earth Science Building, University of Alberta, Edmonton, Alberta T6G 2E3, Canada, 2. Division of Earth Sciences, Gregory Building, Lilybank Gardens, University of Glasgow, Glasgow G12 8QQ, UK, 3. Department of Earth and Atmospheric Sciences, 1-26 Earth Science Building, University of Alberta, Edmonton, Alberta T6G 2E3, Canada, 4. Institut für Mineralogie, Ruprecht Karls Universität, Im Neuenheimer Feld 236, 69120 Heidelberg, Germany, 5. Institut für Mineralogie, J.W. Goethe Universität, Senckenberganlage 28, 60054 Frankfurt, Germany

Inclusions of majoritic garnet in diamonds from the Jagersfontein kimberlite formed at unusually great depths of ∼250 to >500 km in the asthenosphere and transition zone. The original host rocks were derived from a much shallower, basaltic (eclogitic) source. The presence of negative Eu anomalies in all majoritic garnets requires a crustal origin, thereby linking these very deep diamond sources to subducting oceanic crust. The carbon isotope values (δ13C) of the host diamonds fall within a narrow range at ∼−20‰, which is fundamentally different from the broad range (−24‰ to −2‰) and bimodal distribution of carbon isotopes of Jagersfontein diamonds that formed in the shallower lithosphere. This indicates that majoritic garnet-bearing diamonds at Jagersfontein inherited their light carbon isotopic composition directly from organic matter contained in a subducting slab. These diamonds were likely formed by direct conversion from graphite, well within the diamond stability field.

Keywords: majorite, diamonds, inclusions, mantle, Eu anomalies, organic carbon

Received: 15 February 2005; Revised: 8 March 2005; Accepted: 10 March 2005

DOI: 10.1130/G21637.1

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