Kimberlite genesis from a common carbonate-rich primary melt modified by lithospheric mantle assimilation

Author:

Giuliani Andrea123ORCID,Pearson D. Graham4ORCID,Soltys Ashton1ORCID,Dalton Hayden1ORCID,Phillips David1ORCID,Foley Stephen F.2ORCID,Lim Emilie1ORCID,Goemann Karsten5ORCID,Griffin William L.2,Mitchell Roger H.6

Affiliation:

1. KiDs (Kimberlites and Diamonds), School of Earth Sciences, The University of Melbourne, Parkville, 3010 Victoria, Australia.

2. Australian Research Council Centre of Excellence for Core to Crust Fluid Systems (CCFS) and GEMOC, Department of Earth and Planetary Sciences, Macquarie University, North Ryde, 2109 New South Wales, Australia.

3. Institute of Geochemistry and Petrology, Department of Earth Sciences, ETH Zurich, Clausiusstrasse 25, Zurich 8092, Switzerland.

4. Department of Earth and Atmospheric Sciences, University of Alberta, Edmonton, Alberta T6G 2E3, Canada.

5. Central Science Laboratory, University of Tasmania, Hobart 7001 Tasmania, Australia.

6. Department of Geology, Lakehead University, P7B 5E1 Ontario, Canada.

Abstract

Diamond-bearing kimberlites were born from similar melts in the deep Earth and variably modified during ascent.

Funder

Australian Research Council

Swiss National Science Foundation

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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