ABOUT THE AGE AND NATURE OF
KREMENKUL RARE-METAL LEUCOGRANITE
(SOUTH URAL) – EVIDENCE
FROM ISOTOPIC AND GEOCHRONOLOGY DATA
Kallistov G.A., Osipova T.A.
Institute of Geology and
Geochemistry UrD RAS, Ekaterinburg, Russia
Kallistov@igg.uran.ru,
osipova@igg.uran.ru
The Kremenkul
rare-metal (W-Mo) massif is located not far from the Chelyabinsk city
(South Ural, East-Ural Raise). According to the geophysical data
(Kuznetsov, 1999) the Kremenkulsky massif is a steeply-dipping stock
3 km size and 6 km deep. It is hosted by the subduction-related
granite rocks of the Chelyabinsky batholite with the zircon Pb-Pb
evaporation age 360-330 Ma (Bea et al., 2002). The Kremenkulsky
granite is a pinkish leucocratic fluorite-bearing two-feldspar
granite with ~ 1 wt.% (Grabezhev et. al., 1987) magnetite content.
The Kremenkul leucogranite is quite close to the Central-Kazakhstan
rare-metal granites on their geochemistry signature (Grabezhev, etc.,
1987; Kallistov, 2007). The modern isotopic and geochronology data
allow to approach the of South Ural rare-metal leucogranite magma
sources problem.
The Kremenkul
leucogranite
isotopic Sr and Nd composition (87Sr/86Sri
= 0.7057;
143Nd/144Ndi
= 0,51209) is rather different from the majority of the South Ural
Early-Permian granites which are notably primitive (87Sr/86Sri
is less than 0.706 and 143Nd/144Ndi
varies 0.51225-0.51235 - Shatagin et. al., 2000; Popov et. al.,
2002).
According to
the recent data the Kremenkul granite is the youngest in Chelyabinsk
batolite. Up today there are K-Ar biotites and muskovites age 260-280
Ma (Grabezhev et. al., 1998) which is in good agreement with Rb-Sr
whole-rocks plus both microcline and biotite isochrone age 274.52.5
Ma (author's data).
Now we have
new U-Pb-SHRIMP zircon data. 2 different zircon types due to their
morphology and chemistry composition were determined in the Kremenkul
leucogranite: zircon-I have the typical middle-level granites
morphology (Krasnobaev, 1986), and rather high U (200-600 ppm) and Th
(120-650 ppm) content, Early Permian age 2715
Ma; zircon-II have the typical abissal-level granites morphology
(Krasnobaev, 1986) and lower U (20-60 ppm) and Th (10-50 ppm)
content, Late-Silurian – Early Devonian age 4167
Ma. It is of great important that host rocks have the Early
Carboniferous age 360-330 Ma. So, the zircon-II can’t be the
host rock xenocrysts, but can be the relic zircon from the protolite
– Middle Paleozoic intrusive granite rock.
The reliable
isotopic-geochronology data about Late-Silurian – Early
Devonian granites in East zone of South Ural are very limited. There
are only three granite massifs can be discussed. They are the
tonalite-plagiogranite Rassypn’ansky, Plastovsky and
Nizhnesanarsky; and independently of its different geological and
tectonic settings, all of them are considered to be formed due to the
ensimatic island arc evolution (Fershtater et al., 2007; Yazeva,
Botchkarev, 1995; Shatagin et al., 2000). According to (Yazeva,
Botchkarev, 1995) the Nizhnesanarsky granitoids are the typical
examples of “young” Paleozoic “continental”
crust of the South Ural. So, it can be considered as the Kremenkul
leucogranite source.
But the isotopic Sr and Nd data
are in contradiction with the both hypothesis of Kremenkul
leucogranite origin: as due to isochemic remelting of the Middle
Paleozoic granite rock, as due to the mixture of this melt with the
basic magmas.
There is one more important
fact: the Early Proterozoic metaterrigene gneisses are identificated
in the contact zone of Chelyabinsk batolite (Krasnobaev et al.,
1998). Due to the absence of the isotopic Sr and Nd data for this
very gneisses it is impossible get the correct conclusion on the
significance of this source for the granite origin. But it is clear
that the Kremenkul leucogranites isotopic signature can’t be
explained by the Middle Paleozoic crust remelting model. So, we
suggest that the Kremenkul leucogranite were generated by remelting
of Proterozoic material as (Popov et al., 2002) did, but we consider
the two-episode remelting of the metaterrigene Proterozoic material
and involving the mantle-derivated magma or solution.
This work has been supported by
the Russian Fond for Basic Research (RFFI) grant 07-05-01023.
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