Mineralogy and geochemistry of silicate dyke rocks associated with carbonatites from the Khibina complex (Kola, Russia) -: isotope constraints on genesis and small-scale mantle sources

被引:18
|
作者
Sindern, S
Zaitsev, AN
Demény, A
Bell, K
Chakmouradian, AR
Kramm, U
Moutte, J
Rukhlov, AS
机构
[1] Rhein Westfal TH Aachen, Inst Mineral & Lagerstattenlehre, D-52056 Aachen, Germany
[2] St Petersburg State Univ, Dept Mineral, St Petersburg 199034, Russia
[3] Hungarian Acad Sci, Lab Geochem Res, H-1112 Budapest, Hungary
[4] Carleton Univ, Dept Geol, Ottawa Carleton Ctr Geosci Studies, Ottawa, ON K1S 5B6, Canada
[5] Univ Manitoba, Dept Geol Sci, Winnipeg, MB R3T 2N2, Canada
[6] Ecole Mines, Ctr SPiN, F-42100 St Etienne, France
[7] WWU Munster, Inst Mineral, Munster, Germany
[8] Univ Freiburg, Inst Mineral Petrol & Geochem, D-7800 Freiburg, Germany
关键词
D O I
10.1007/s00710-003-0016-2
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The eastern part of the agpaitic Khibina complex is characterized by the occurrence of dykes of various alkali silicate rocks and carbonatites. Of these, picrite, rnonchiquite, nephelinite and phonolite have been studied here. Whole rock and mineral geochemical data indicate that monchiquites evolved from a picritic primary magma by olivine+magnetite fractionation and subsequent steps involving magma mixing at crustal levels. None of these processes or assimilation/magma mixing of wall rocks or other plutonic rocks within the complex can entirely explain the geochemical and Nd-Sr-isotopic characteristics of the monchiquites (i.e. a covariant alignment between (Sr-87/Sr-86)(370)=0.70367, (Nd-143/Nd-144)(370)=0.51237 and (Sr-87/Sr-86)(370)=0.70400, (Nd-143/Nd-144)(370)=0.51225 representing the end points of the array). This signature points to isotopic heterogeneities of the mantle source of the dyke-producing magma. The four mantle components (i.e. depleted mantle, lower mantle plume component, EMI-like component and EMII-like component) must occur in different proportions on a small scale in order to explain the isotopic variations of the dyke rocks. The EMII-Iike component might be incorporated into the source area of the primary magma by carbonatitic fluids involving subducted crustal material. The most likely model to explain the small-scale isotopic heterogeneity is plume activity. The results of this study do not provide any support to a cogenetic origin (e.g. fractionation or liquid immiscibility) for carbonatite and monchiquite or other alkali-silicate dyke rocks occurring in spatial proximity. Instead, we propose that both, carbonatite and picrite/monchiquite, originated by low-degree partial melting of peridotite. Textural observations, mineralogical data, and C and O isotopic compositions suggest incorporation of calcite from carbonatite in monchiquite and the occurrence of late-stage carbothermal fluids.
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页码:215 / 239
页数:25
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