Инд. авторы:	Agashev A.M., Nakai S., Serov I.V., Tolstov A.V., Garanin K.V., Kovalchuk O.E.
Заглавие:	Geochemistry and origin of the mirny field kimberlites, siberia
Библ. ссылка:	Agashev A.M., Nakai S., Serov I.V., Tolstov A.V., Garanin K.V., Kovalchuk O.E. Geochemistry and origin of the mirny field kimberlites, siberia // Mineralogy and Petrology. - 2018. - P.1-12. - ISSN 0930-0708. - EISSN 1438-1168.
Внешние системы:	DOI: 10.1007/s00710-018-0617-4; РИНЦ: 35753843; SCOPUS: 2-s2.0-85049647113; WoS: 000453937200020;
Реферат:	eng: Here we present new data from a systematic Sr, Nd, O, C isotope and geochemical study of kimberlites of Devonian age Mirny field that are located in the southernmost part of the Siberian diamondiferous province. Major and trace element compositions of the Mirny field kimberlites show a significant compositional variability both between pipes and within one diatreme. They are enriched in incompatible trace elements with La/Yb ratios in the range of (65–300). Initial Nd isotope ratios calculated back to the time of the Mirny field kimberlite emplacement (t = 360 ma) are depleted relative to the chondritic uniform reservoir (CHUR) model being 4 up to 6 ɛNd(t) units, suggesting an asthenospheric source for incompatible elements in kimberlites. Initial Sr isotope ratios are significantly variable, being in the range 0.70387–0.70845, indicating a complex source history and a strong influence of post-magmatic alteration. Four samples have almost identical initial Nd and Sr isotope compositions that are similar to the prevalent mantle (PREMA) reservoir. We propose that the source of the proto-kimberlite melt of the Mirny field kimberlites is the same as that for the majority of ocean island basalts (OIB). The source of the Mirny field kimberlites must possess three main features: It should be enriched with incompatible elements, be depleted in the major elements (Si, Al, Fe and Ti) and heavy rare earth elements (REE) and it should retain the asthenospheric Nd isotope composition. A two-stage model of kimberlite melt formation can fulfil those requirements. The intrusion of small bodies of this proto-kimberlite melt into lithospheric mantle forms a veined heterogeneously enriched source through fractional crystallization and metasomatism of adjacent peridotites. Re-melting of this source shortly after it was metasomatically enriched produced the kimberlite melt. The chemistry, mineralogy and diamond grade of each particular kimberlite are strongly dependent on the character of the heterogeneous source part from which they melted and ascended.
Ключевые слова:	Lithospheric mantle; kimberlite; geochemistry; siberia; Sr-Nd isotopes;
Издано:	2018
Физ. характеристика:	с.1-12