Загрузил Viktoria Osipenko

Theses Osypenko

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ACCESSORY MINERALS TRACE ELEMENT GEOCHEMISTRY AS A TOOL FOR
CARBONATITES GENETIC FEATURES STUDY
Sergiy Shnyukov, Viktoriia Osypenko, Olexandr Andreev
Institute of Geology, Kyiv National Taras Shevchenko University, Kyiv, Ukraine
[email protected]
Precambrian shields alkaline rocks are important objects for abyssal Earth processes
study despite on their low prevalence [1]. There are near 40 alkaline rocks massifs studied to
varying degrees within Ukrainian Shield [4]. Genesis of most of them is not fully explored
and geochemical features of rocks are different. In this paper the attempt to investigate the
cause of such difference for carbonatite massifs was made by mantle sources for their
formation geochemical differences estimation.
Proskurovka (PM) and Chernigovka carboantite (ChCM) massifs (Dnister-Bug and
West Pre-Azov Regions respectively) [2, 4] were chosen as objects of study. Low indicator
elements (P, LREE, Sr, Ba, Nb) contents for alkaline rocks are observed in PM unlike ChCM
[2-4, 7].
PM belongs to central structural-morphological type. It’s composed of ijolitemelteigites, alkaline pyroxenites, alkaline and nepheline syenites and surrounded by fenitized
rocks and fenites formed on Chudnov-Berdichev granites and Bt-Pl crystalline shale host
rocks [10]. ChCM is stretched along the Chernigov fault zone and represents linear structuralmorphological type. It’s composed of carbonatitic dykes, and some nepheline syenites and
alkaline pyroxenites bodies. Massive is surrounded by wide fenite halo developed on
amphibolites, gneisses and granites [5, 6].
Metasomatic columns of host rocks alteration were formed for fenitization process
investigation in both massifs. Geochemical research on the rock level has shown [5-7], that
contrast types host rocks compositions converge during fenitization process. At the same time
final products of PM and ChCM fenitization significantly differ between themselves and with
alkaline rocks and carbonatites. It can be traced distinctly on trace-elements content. The
leading role in fenitization belongs to so-called «forward wave» metasomatic fluids which
were preceding of alkaline rocks and carbonatites intruded the fenite halo. In general, such
fluids composition apparently carries information about mantle source for each massive
forming. It can be assumed accessory apatite of different generations (corresponded to fenite
halos zones) is sensitive indicator to fenitization fluid trace element composition [9]. Trace
element composition alterations of accessory apatite [9] in formed PM and ChCM
metasomatic columns were traced to confirm this suppose.
PM. Because of the basic host rocks limited distribution the metasomatic column for
them is a two-member: 0 – initial host rocks, 1 – fenitization rocks. Unfortunately, the apatite
is not observed in last one. For granites the metasomatic column is a three-member: 0 – initial
host rocks, 1 – fenitized rocks; 2 – apogranitic fenites [6].
ChCM. For different composition host rocks (basic, intermediate, felsic) three-member
columns were formed: 0 – initial host rocks, 1 – fenitized rocks; 2 – fenites [5, 7, 9].
Obtained data are represented on figure 1. Arrows show trace elements composition
alteration trends of apatites during different host rocks fenitization. The plots show, that
apatite from ChCM fenites has higher indicator trace elements content (in particular Sr)
compared with such PM rocks. It allows suggesting the different fluid composition for both
massifs.
Apatite composition from the most altered rocks will allow obtaining more precisely
trace elements composition of fenitization fluids if apatite-fluid distribution coefficients for
trace elements will be known. These estimations are the task for further research.
Figure 1. Composition variations of accessory apatites from PM (a) and ChCM (b) fenite
halo rocks [9]. 1-3 – basic (1), intermediate (2) and felsic (3) host rocks; 4-9 – their
metasomatic alterated products (4, 6, 8 – fenitized rocks; 5, 7, 9 – fenites); 10 – alkaline
syenites; 11 – nepheline syenites; 12 – ijolites; 13 – apatite composition fields boundaries.
Arrows show composition alteration trends of apatites from fenite halos rocks. Statistic
justified fields of apatite compositions are marked by roman numerals (from [8]): I –
metamorphic carbonate and silica-carbonate rocks; II – calc-alkaline ultrabasic, basic and
intermediate rocks; III – the same for moderately felsic rocks; IV – high-felsic granites; V –
carbonatites, alkaline rocks and associated metasomatic rocks (together with mantle
xenolithes lherzolites); VI – alkaline metasomatites (including fenites).
References
1. Igneous rocks. Vol. 2. Alkaline rocks. M., 1986. (In Russian).
2. Kryvdik S. G. Alkaline magmatism of Ukrainian Shield: geochemical and petrogenetical
aspects // Mineral. Journal. 2000. Vol. 22. № 2/3. P. 48-56. (In Ukrainian).
3. Kryvdik S. G., Dubyna O. V. Alkaline rocks geochemical features of Dnister-Bug of
Ukrainian Shield // Mineral. Journal. 2006. Vol. 28. № 4. P. 32-42. (In Russian).
4. Kryvdik S. G., Tkachuk V. I.,. Petrology of Ukrainian Shield nepheline rocks. K.: Nauka,
1990. 406 p. (In Russian).
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features of Ukrainian Shield, Yenisey Range and Voronezh Massif linear carbonatite
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potential // International Scientific Conference «Metasomatism and Ore-formation».
Kyiv, 2016. P. 51-53. (In Ukrainian).
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Pre-Azov Region) // Geol. Journal. 1983. Vol. 43. № 4. P. 52-61. (In Russian).
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elements as formational affiliation and metasomatic zoning criterion // Geol. Journal.
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10. Tsarovskiy I. D., Bratslavskiy P. F. Dniester-Bug region nepheline rocks (geology, age
and material composition). K., 1980. 46 p. (In Russian).
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