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Timmerman S, Stachel T, Koornneef JM, Smit KV, Harlou R, Nowell GM, Thomson AR, Kohn SC, Davies JHFL, Davies GR, Krebs MY, Zhang Q, Milne SEM, Harris JW, Kaminsky F, Zedgenizov D, Bulanova G, Smith CB, Cabral Neto I, Silveira FV, Burnham AD, Nestola F, Shirey SB, Walter MJ, Steele A, Pearson DG. Sublithospheric diamond ages and the supercontinent cycle. Nature 2023; 623:752-756. [PMID: 37853128 PMCID: PMC10665200 DOI: 10.1038/s41586-023-06662-9] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/28/2023] [Accepted: 09/20/2023] [Indexed: 10/20/2023]
Abstract
Subduction related to the ancient supercontinent cycle is poorly constrained by mantle samples. Sublithospheric diamond crystallization records the release of melts from subducting oceanic lithosphere at 300-700 km depths1,2 and is especially suited to tracking the timing and effects of deep mantle processes on supercontinents. Here we show that four isotope systems (Rb-Sr, Sm-Nd, U-Pb and Re-Os) applied to Fe-sulfide and CaSiO3 inclusions within 13 sublithospheric diamonds from Juína (Brazil) and Kankan (Guinea) give broadly overlapping crystallization ages from around 450 to 650 million years ago. The intracratonic location of the diamond deposits on Gondwana and the ages, initial isotopic ratios, and trace element content of the inclusions indicate formation from a peri-Gondwanan subduction system. Preservation of these Neoproterozoic-Palaeozoic sublithospheric diamonds beneath Gondwana until its Cretaceous breakup, coupled with majorite geobarometry3,4, suggests that they accreted to and were retained in the lithospheric keel for more than 300 Myr during supercontinent migration. We propose that this process of lithosphere growth-with diamonds attached to the supercontinent keel by the diapiric uprise of depleted buoyant material and pieces of slab crust-could have enhanced supercontinent stability.
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Affiliation(s)
- Suzette Timmerman
- Department of Earth and Atmospheric Sciences, University of Alberta, Edmonton, Alberta, Canada.
- Institute for Geological Sciences, University of Bern, Bern, Switzerland.
| | - Thomas Stachel
- Department of Earth and Atmospheric Sciences, University of Alberta, Edmonton, Alberta, Canada
| | | | - Karen V Smit
- School of Geosciences, University of Witwatersrand, Johannesburg, South Africa
| | - Rikke Harlou
- Department of Earth Sciences, University of Durham, Durham, UK
| | - Geoff M Nowell
- Department of Earth Sciences, University of Durham, Durham, UK
| | - Andrew R Thomson
- Department of Earth Sciences, University College London, London, UK
| | - Simon C Kohn
- School of Earth Sciences, University of Bristol, Bristol, UK
| | - Joshua H F L Davies
- Département des sciences de la Terre et de l'atmosphère, Université du Québec à Montréal, Montreal, Quebec, Canada
| | - Gareth R Davies
- Faculty of Sciences, Vrije Universiteit, Amsterdam, The Netherlands
| | - Mandy Y Krebs
- Department of Earth and Atmospheric Sciences, University of Alberta, Edmonton, Alberta, Canada
| | - Qiwei Zhang
- Department of Earth and Atmospheric Sciences, University of Alberta, Edmonton, Alberta, Canada
| | - Sarah E M Milne
- Department of Earth and Atmospheric Sciences, University of Alberta, Edmonton, Alberta, Canada
| | - Jeffrey W Harris
- School of Geographical and Earth Sciences, University of Glasgow, Glasgow, UK
| | - Felix Kaminsky
- V. I. Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian Academy of Sciences, Moscow, Russian Federation
| | - Dmitry Zedgenizov
- A. N. Zavaritsky Institute of Geology and Geochemistry, Russian Academy of Sciences, Ekaterinburg, Russian Federation
| | - Galina Bulanova
- School of Earth Sciences, University of Bristol, Bristol, UK
| | - Chris B Smith
- School of Earth Sciences, University of Bristol, Bristol, UK
| | | | | | - Antony D Burnham
- Research School of Earth Sciences, Australian National University, Canberra, Australian Capital Territory, Australia
| | | | - Steven B Shirey
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA
| | - Michael J Walter
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA
| | - Andrew Steele
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA
| | - D Graham Pearson
- Department of Earth and Atmospheric Sciences, University of Alberta, Edmonton, Alberta, Canada
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Brill S, Lilimu N, Chetty D. Diamond fingerprinting for source discrimination using laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) and Fourier transform infrared spectrometry (FTIR). Heliyon 2020; 6:e05592. [PMID: 33305049 PMCID: PMC7711147 DOI: 10.1016/j.heliyon.2020.e05592] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/06/2019] [Revised: 02/03/2020] [Accepted: 11/16/2020] [Indexed: 11/24/2022] Open
Abstract
The Kimberley Process Certification Scheme (KPCS) was established in 2000 as a means of controlling the flow of conflict diamonds, mostly, from the African continent. In 2013, the KPCS imposed an embargo on diamonds from the Central African Republic (CAR). Since then the embargo has been lifted in certain prefectures of the country, however, smuggling is suspected from non-compliant areas. Three parcels of diamonds suspected to have mining origins in the CAR, were analysed. These diamonds were investigated for their morphological and chemical characteristics, to establish a diamond fingerprint and to determine if these diamonds had the same fingerprint as previously analysed diamonds from CAR or the Democratic Republic of the Congo (DRC). The analyses of these diamonds were included in the already established diamond database of rough diamonds from the African continent. The morphological characteristics identified included the mass (ct), colour, surface coatings, dominant, secondary and tertiary form, shape, breakage, inclusions, abrasion and surface features that are specific to octahedral, dodecahedral and cubic shapes. The morphological characteristics determined from the diamonds revealed that morphology alone cannot be used as a discriminatory method for diamond fingerprinting. Fourier transform infrared spectroscopy (FTIR) identified the nitrogen concentration and aggregation state of that N. This allowed for the typing of the diamonds as Type I (containing N) and Type II (containing no measureable N). The concentration of N in the three parcels is less than 600 ppm. Further classification of Type I diamonds was performed according to the N aggregation state as single, double or four-fold. The vast majority of diamonds show a combination of nitrogen aggregation states while few were classified as Type II. Fourier transform IR showed no discernible trends between the current study and the established database. Laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) was used as a means of determining the trace element concentrations of 69Ga, 88Sr, 89Y, 90Zr, 93Nb, 133Cs, 137Ba, 139La, 140Ce, 141Pr, 146Nd, 147Sm, 153Eu, 157Gd, 159Tb, 163Dy, 165Ho, 166Er, 169Tm, 172Yb, 175Lu, 178Hf, 181Ta, 232Th and 238U. Laser ablation ICP-MS determined that not all elements produce statistically viable data, however, the data could still be used to discern trace element differences and trends among the parcels. In the current set of diamonds, laser ablation ICP-MS data for parcels A and B showed an excellent agreement with each other as well as those from diamonds previously analysed from CAR. None of the three parcels showed any similarity to data from Bria River or the DRC. It is concluded that the diamonds from parcels A and B are very likely to have mining origins in the same area in the CAR, whereas parcel C is distinct and of possible mixed origin.
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Affiliation(s)
- Susan Brill
- Mintek, Private Bag X3015, Randburg, 2125, South Africa
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An Evaluation of the Potential for Determination of the Geographic Origin of Ruby and Sapphire Using an Expanded Trace Element Suite Plus Sr–Pb Isotope Compositions. MINERALS 2020. [DOI: 10.3390/min10050447] [Citation(s) in RCA: 6] [Impact Index Per Article: 1.5] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/16/2022]
Abstract
The geographic origin of gem corundum has emerged as one of its major value factors. Combined with gemological observations, trace element analysis is a powerful tool for the determination of corundum provenance. However, owing to similar properties and features of gem corundum from different localities, but similar geological settings, and very low levels of many trace elements in gem corundum, the determination of geographic origin remains challenging. In this study, we present trace elements compositions determined by laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) for rubies and blue sapphires from several different localities of geologically similar deposits: high-Fe amphibolite-type rubies, low-Fe marble-type rubies, and metamorphic blue sapphires. In addition, we determined Sr and Pb isotopic ratios by offline laser ablation sampling followed by thermal ionization mass spectroscopy (TIMS). By applying new and existing elemental discrimination schemes and the multivariate statistical method linear discriminant analysis (LDA), we show that, in addition to the commonly used discriminators Mg, Fe, V, Ti, and Ga, the elements Ni, Zr, Cr, and Zn show potential for geographic origin determination. Amphibolite-type rubies from different localities can be discriminated using Sr and Pb isotope ratios, whereas the discrimination of marble-type ruby and metamorphic blue sapphires is limited. Our results re-emphasize the challenge of geographic origin determination and the need for a more powerful discriminatory tool.
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Timmerman S, Honda M, Burnham AD, Amelin Y, Woodland S, Pearson DG, Jaques AL, Le Losq C, Bennett VC, Bulanova GP, Smith CB, Harris JW, Tohver E. Primordial and recycled helium isotope signatures in the mantle transition zone. Science 2019; 365:692-694. [PMID: 31416962 DOI: 10.1126/science.aax5293] [Citation(s) in RCA: 15] [Impact Index Per Article: 3.0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/31/2019] [Accepted: 07/16/2019] [Indexed: 11/02/2022]
Abstract
Isotope compositions of basalts provide information about the chemical reservoirs in Earth's interior and play a critical role in defining models of Earth's structure. However, the helium isotope signature of the mantle below depths of a few hundred kilometers has been difficult to measure directly. This information is a vital baseline for understanding helium isotopes in erupted basalts. We measured He-Sr-Pb isotope ratios in superdeep diamond fluid inclusions from the transition zone (depth of 410 to 660 kilometers) unaffected by degassing and shallow crustal contamination. We found extreme He-C-Pb-Sr isotope variability, with high 3He/4He ratios related to higher helium concentrations. This indicates that a less degassed, high-3He/4He deep mantle source infiltrates the transition zone, where it interacts with recycled material, creating the diverse compositions recorded in ocean island basalts.
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Affiliation(s)
- S Timmerman
- Research School of Earth Sciences, Australian National University, 142 Mills Road, Acton, ACT 2601, Australia.
| | - M Honda
- Research School of Earth Sciences, Australian National University, 142 Mills Road, Acton, ACT 2601, Australia
| | - A D Burnham
- Research School of Earth Sciences, Australian National University, 142 Mills Road, Acton, ACT 2601, Australia
| | - Y Amelin
- Research School of Earth Sciences, Australian National University, 142 Mills Road, Acton, ACT 2601, Australia
| | - S Woodland
- Earth and Atmospheric Sciences, University of Alberta, 116 Street and 85 Avenue, Edmonton, Alberta T6G 2R3, Canada
| | - D G Pearson
- Earth and Atmospheric Sciences, University of Alberta, 116 Street and 85 Avenue, Edmonton, Alberta T6G 2R3, Canada
| | - A L Jaques
- Research School of Earth Sciences, Australian National University, 142 Mills Road, Acton, ACT 2601, Australia
| | - C Le Losq
- Research School of Earth Sciences, Australian National University, 142 Mills Road, Acton, ACT 2601, Australia
| | - V C Bennett
- Research School of Earth Sciences, Australian National University, 142 Mills Road, Acton, ACT 2601, Australia
| | - G P Bulanova
- School of Earth Sciences, University of Bristol, Queens Road, Bristol BS8 1QU, UK
| | - C B Smith
- School of Earth Sciences, University of Bristol, Queens Road, Bristol BS8 1QU, UK
| | - J W Harris
- School of Geographical and Earth Sciences, Gregory Building, University of Glasgow, Glasgow G12 8QQ, UK
| | - E Tohver
- University of Sao Paolo, Sao Paolo, Brazil
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Garanin VK, Biller AY, Skvortsova VL, Bovkun AV, Bondarenko GV. Polyphase hydrocarbon inclusions in garnet from the Mir diamondiferous pipe. ACTA ACUST UNITED AC 2011. [DOI: 10.3103/s0145875211020049] [Citation(s) in RCA: 10] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/30/2022]
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Dalpé C, Hudon P, Ballantyne DJ, Williams D, Marcotte D. Trace Element Analysis of Rough Diamond by LA-ICP-MS: A Case of Source Discrimination?*,†. J Forensic Sci 2010; 55:1443-56. [DOI: 10.1111/j.1556-4029.2010.01509.x] [Citation(s) in RCA: 15] [Impact Index Per Article: 1.1] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/30/2022]
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