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<title lang=en>Olivine inclusions in Siberian diamonds and mantle xenoliths: Contrasting water and trace-element contents</title>
<creator>Jean, M. m.</creator>
<creator>Taylor, L. a.</creator>
<creator>Howarth, G. h.</creator>
<creator>Peslier, A. h.</creator>
<creator>Fedele, L.</creator>
<creator>Bodnar, R. j.</creator>
<creator>Guan, Y.</creator>
<creator>Doucet, L. s.</creator>
<creator>IONOV, Dmitri</creator>
<creator>Logvinova, A. m.</creator>
<creator>Golovin, A. V.</creator>
<creator>Sobolev, N. v.</creator>
<contributor>The University of Tennessee [Knoxville]</contributor>
<contributor>University of Cape Town</contributor>
<contributor>NASA Johnson Space Center (JSC) ; NASA</contributor>
<contributor>Department of Geosciences, Virginia Tech, Blacksburg</contributor>
<contributor>California Institute of Technology, Pasadena</contributor>
<contributor>Université Libre de Bruxelles [Bruxelles] (ULB)</contributor>
<contributor>Géosciences Montpellier ; Université des Antilles et de la Guyane (UAG) - Institut national des sciences de l'Univers (INSU - CNRS) - Université de Montpellier (UM) - Centre National de la Recherche Scientifique (CNRS)</contributor>
<contributor>Manteau et Interfaces ; Géosciences Montpellier ; Université des Antilles et de la Guyane (UAG) - Institut national des sciences de l'Univers (INSU - CNRS) - Université de Montpellier (UM) - Centre National de la Recherche Scientifique (CNRS) - Université des Antilles et de la Guyane (UAG) - Institut national des sciences de l'Univers (INSU - CNRS) - Université de Montpellier (UM) - Centre National de la Recherche Scientifique (CNRS)</contributor>
<contributor>Sobolev Institute of Geology and Mineralogy [Novosibirsk] ; Siberian Branch of the Russian Academy of Sciences (SB RAS)</contributor>
<description>International audience</description>
<source>ISSN: 0024-4937</source>
<source>Lithos</source>
<publisher>Elsevier</publisher>
<identifier>hal-01467731</identifier>
<identifier>https://hal.archives-ouvertes.fr/hal-01467731</identifier>
<source>https://hal.archives-ouvertes.fr/hal-01467731</source>
<source>Lithos, Elsevier, 2016, 265, pp.31-41. 〈10.1016/j.lithos.2016.07.023〉</source>
<identifier>DOI : 10.1016/j.lithos.2016.07.023</identifier>
<relation>info:eu-repo/semantics/altIdentifier/doi/10.1016/j.lithos.2016.07.023</relation>
<language>en</language>
<subject lang=en>Nominally anhydrous minerals (NAM)</subject>
<subject lang=en>Mantle water</subject>
<subject lang=en>Olivine trace elements</subject>
<subject lang=en>SIMS</subject>
<subject lang=en>Diamond inclusions</subject>
<subject lang=en>Siberian craton</subject>
<subject>[SDU.STU.GC] Sciences of the Universe [physics]/Earth Sciences/Geochemistry</subject>
<type>info:eu-repo/semantics/article</type>
<type>Journal articles</type>
<description lang=en>A subject of continuing debate is how the Earth's lithospheric portion of the upper mantle has remained the thickest (> 200 km) and oldest (> 3 Gy) beneath cratons and is yet surrounded by a vigorously convecting asthenosphere. It is generally admitted that water is a key parameter in the strength and longevity of cratonic roots, because olivine, the main phase of the lithospheric mantle, becomes stronger if its water content decreases. Expanding upon the work presented in Novella et al. (2015) and Taylor et al. (2016), we report new water contents for additional olivine inclusions in diamonds together with the trace-element composition for all olivine inclusions, as well as for mantle xenoliths from various kimberlite pipes located on the Siberian craton. The olivine diamond inclusions from this study have systematically low-water contents (< 50 ppmw H2O), moderate to high forsterite (e.g., Fo91–94) contents and low Ni, Co, and Zn ppm contents (e.g., < 2848, < 108, and < 47 ppm, respectively). In contrast, olivines from Siberian craton mantle xenoliths have a wide range of water contents (6–323 ppmw H2O) and extend to lower-Fo (91–92), Ni, Co, and Zn-rich compositions, compared to the diamond inclusions. Depleted incompatible trace-element concentrations in olivine (0.1–0.001 × Primitive Mantle) advance our hypothesis for the protogenetic origins for the majority of Siberian diamond inclusions. These observations are consistent with the peridotite xenoliths as representing a part of the cratonic lithosphere that has experienced melt re-fertilization, which has also transported water. The olivine diamond inclusions, on the other hand, preserve “micro-samples” of an initial, dry cratonic lithosphere, mostly resulting from melting events. These inclusions are likely sourced from the initial cratonic mantle lithosphere, which thereby, resisted delamination over time, due to its buoyancy and strength, imparted from melt and water depletion, respectively. And thus, our data provides a major argument that the kimberlite-hosted mantle xenoliths may be more metasomatized than common rocks at the base of the Siberian and other cratonic roots away from kimberlite fields.</description>
<date>2016-11-15</date>
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