Vis enkel innførsel

dc.contributor.authorKostrovitsky, S.I.
dc.contributor.authorTappe, Sebastian
dc.contributor.authorYakovlev, D.A.
dc.contributor.authorIvanov, A.S.
dc.contributor.authorSpetsius, Z.V.
dc.contributor.authorAshchepkov, I.V.
dc.date.accessioned2025-02-13T08:45:15Z
dc.date.available2025-02-13T08:45:15Z
dc.date.issued2023-11-22
dc.description.abstractThis contribution reports some 16,000 major and minor element analyses of garnet xenocrysts derived from 18 (out of the 21 known) kimberlite fields of the Yakutian Kimberlite Province (YaKP) on the Siberian craton in Russia. Using TiO<sub>2</sub>–in–garnet as an indicator of heterogeneity within the subcontinental lithospheric mantle (SCLM), as well as garnet mg# (mg#=Mg<sup>2+</sup>/(Mg<sup>2+</sup>+Fe<sup>2+</sup>)*100), we distinguish three subpopulations of garnet: 1) high content of TiO<sub>2</sub> (0.26–0.50 wt%) and high mg# (80.6–82.6) garnet xenocrysts are common in the southern diamondiferous kimberlite fields; 2) garnet xenocrysts with low content of TiO<sub>2</sub> (0.06–0.26 wt%) and relatively high values of mg# (78.8–81.7), which prevail in the northern ‘barren’ kimberlite fields; and 3) three anomalous northern kimberlite fields (Chomurdakh, Ogoner-Yuryakh, Toluopka) characterized by the predominance of garnet xenocrysts with high TiO<sub>2</sub> content (0.53–0.78 wt%) at relatively low mg# (76.9–78.3).<p> <p>It is reasonable to assume that relatively thin cratonic mantle lithosphere beneath the three anomalous kimberlite fields underwent intense metasomatic overprinting by melts and fluids injected from the underlying asthenosphere, which changed the compositions of peridotitic garnets significantly. An interpretation of the data presented in this study is that the generally high TiO<sub>2</sub> contents of kimberlites in the northern YaKP (>1.5 wt% TiO<sub>2</sub>) are a primary magmatic feature of asthenospheric origin because the lithospheric mantle traversed by these kimberlite magmas is TiO<sub>2</sub> depleted. We propose a model in which the relatively thin SCLM of the northern Siberian craton provided less opportunity for high-TiO<sub>2</sub> asthenospheric kimberlite melts to interact and change compositions on their way to the Earth’s surface. The high-TiO<sub>2</sub> kimberlites of the northern YaKP may thus represent a good approximation of the primary compositions of natural kimberlite melts.en_US
dc.identifier.citationKostrovitsky, Tappe, Yakovlev, Ivanov, Spetsius, Ashchepkov. Lithospheric mantle heterogeneity beneath the Siberian craton: Evidence from garnet xenocryst database with implications for kimberlite compositions. Gondwana Research. 2024;128:298-314
dc.identifier.cristinIDFRIDAID 2235318
dc.identifier.doi10.1016/j.gr.2023.10.021
dc.identifier.issn1342-937X
dc.identifier.issn1878-0571
dc.identifier.urihttps://hdl.handle.net/10037/36490
dc.language.isoengen_US
dc.publisherElsevieren_US
dc.relation.journalGondwana Research
dc.rights.holderCopyright 2024 The Author(s)en_US
dc.titleLithospheric mantle heterogeneity beneath the Siberian craton: Evidence from garnet xenocryst database with implications for kimberlite compositionsen_US
dc.type.versionacceptedVersionen_US
dc.typeJournal articleen_US
dc.typeTidsskriftartikkelen_US
dc.typePeer revieweden_US


Tilhørende fil(er)

Thumbnail

Denne innførselen finnes i følgende samling(er)

Vis enkel innførsel