AGE ESTIMATION FOR
GARGINSKY GNEISS-GRANITE BLOCK OF
BARGUZIN-
VITIM SUPERTERRAIN
Rytsk E.Y., Makeev A.F., Salnikova E.B.,Fedoseenko A.M..
Institute
of Precambrian Geology and Geochronlogy RAS, S-Petersburg, Russia,
ERytsk@geogem.spb.ru
Angara-Vitim
batholite of upper Paleozoic (Hercynian) age (Yarmolyuk et al.,
1997; Neimark et al., 1993; Zygankov et al., 2007) occupies the
larger part of Barguzin-Vitim super terrain. Earlier gneiss-granite
complexes of local occurrence are not dated accurately – their
age estimations vary from Paleozoic to early Proterozoic. At the
same time, information on the age of “pre-batholite”
gneiss-granite complexes has essential significance for of tectonic
evolution of the super terrain.
“Pre-batholite”
gneiss-granites occur in the area between two rivers – the
Garga and Ikata, where Garginsky block of early Precambrian basement
had been marked out (Salop, 1964). According geological survey-50
(Pervukhin et al., 1980) Garginsky block is represented by a cupola
structure formed by early Paleozoic (?) sin-metamorphic
gneiss-granites. The latter are represented by homogeneous fine
grained biotite granite-gneisses and gneiss-like granites with
xenolithes of migmatizated chlorite-sericite-quartz schists of
possibly Ikat epoch of Cambrian period and are cut by pegmatoid
granites. For isotope investigations within the cupola structure
there were taken two samples of sin-metamorphic granite-gneisses on
the right bank (¹ 2091) and on the left bank (¹ 1069) of the Garga
river valley in 4 km up from the mouth of the Ikata river
(collection of Fishev N.A. and Shelgachev K.N., FSUE
“Buryatgeocentre”).
U-Pb
studies have been carried out for five weights of magmatic zircon of
different size fractions and micro-weight of monazite from
granite-gneiss (sample N2091). Three signatures of zircon isotope
composition form the line of regression and are close to its lower
intersection with concordia which corresponds to the age of 493±6
Ma, the upper intersection corresponds to 1273±34 ,
MSWD=0.97. Isotope signatures for zircons of larger size are a
little further from discordia, this can be explained by different
age of inherited component of radiogenic lead in the studied zircon.
Monazite is characterized by concordant age 425±2 Ma
(MSWD=1.3, probability=0.26) and reflects the overprinted thermal
event. Taking into consideration magmatic origin of zircon, it is
possible to interpret the obtained age estimation 493±6 Ma as
the age of its crystallization and correspondently formation of
gneiss-granites.
U-Pb
isotope data obtained for sample N1069 from granite-gneiss show
linear age discordance t(206Pb/238U)<t(207Pb/235U)<
t(207Pb/206Pb)
for four zircon size fractions and on the diagram with concordia
the signatures of their isotope composition are approximated by
regression line with upper intersection with concordia corresponding
to the age 681±18 Ma and the lower corresponds to the age
estimation of 248±84 Ma (MSWD=1.3).
So,
in the course of Garginsky cupola structure formation there have
been not less than three episodes of granite formation – at
700-660, 490 and 440-420 Ma. Estimated early Ordovician age of
gneiss-granites of Garginsky structure precisely corresponds to the
main collision stage in the evolution of Caledonian structures of
CAFB and Barguzin-Vitim super terrain as its part. Age estimations
of post collision thermal events in the interval 440-420 Ma coincide
with the age of large granite-gneiss massifs of “pre-batholite”
Ogemi-Davansky complex of Kater zone (Rytsk et al., 1999). According
Koshkin V. (FSUE “Buryatgeocentre”) such “pre-batholite”
(“pre-vitimkansky”) granite-diorite massifs and
gneiss-granite cupola structures are widely spread in the area
between the Garga, Ikata and Vitimkan rivers and gravitate to the
wide zone of hidden tectonic contact between Barguzin and
Vitimkan-Zipinsky terrains. Original data evidence that among
gigantic granite blocks of the Easter Baikal region which are
traditionally attached to Angara-Vitim batholite considerable number
of them could belong to sin- and post collision granites of
Caledonian stage and to Precambrian formations.
The
Work was carried out under financial support of RFFI, grant
05-05-65316 and Foundation for development of geology.
References
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E.Yu., Rizvanova N.G. (1993). The Hercynian age and Pre-Cambrian
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Paleozoic granitoid formation
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