Rare and rare-earth
elements in Late Archaean moderately alkaline intrusive units of
Karelia. Examples from the Syargozero complex
Dmitrieva
А.V.*
*FBGU, KarRC, RAS, IG,
Petrozavodsk, Russia
dmitrievaa-v@yandex.ru
Rare and rare-earth
elements, such as Ta, Nb, Sr, Y and lanthanoids, are known to be
associated with the rocks of alkaline igneous formations and
carbonatites. As the application range of these metals is wide, they are
in great demand. Rare-earth elements are used in modern high-tech
devices and plants; in the production of monocrystals for solid-body
lasers, control rods for nuclear reactors, permanent magnets, special
radiation-protecting coatings, in medicine, metallurgy, electronics,
optics, car production, luminophors, audio systemsа,
as catalysts, etc. In the Kola Peninsula, most rare earths are
concentrated in the alkaline rocks and apatite-nepheline ores of the
Khibiny massif. The Tikshozero massif is an example of such localities
in Karelia. Moderately alkaline rocks occupy an intermediate position in
igneous series. High-Pt (Kondersky massif in Siberia) and REE deposits
are occasionally associated with the ultramafic members of this series.
The high-alkali massifs,
formed at final stages in the evolution of Late Archaean greenstone
belts and identified as sanukitoids (~2.74-2.7 Ga), e.g. the Panozero,
Syargozero, Amindomaoya, Sharavalampi, Elmus, Hautavaara and other
intrusive units (Lobach-Zhuchenko et al., 2005), are common in Central
Karelia. The Syargozero, Sharavalampi and Torosozero massifs are
collectively named the Syargozero moderately alkaline complex (Slyusarev
et al., 2001). The Panozero pluton has been studied in most detail (Lobach-Zhuchenko
et al., 2007). The intrusives are differentiated from pyroxenites to
quartz monzonites and syenites. As the rocks are typically rich in
alkalies, P and Ti, Ba, Sr and REE, they are considered to be the
possible source of rare and rare-earth elements.
The detailed study of the
massifs of the Syargozero complex has shown that early phases are
represented by gabbro and pyroxenites and late phases by monzodiorites
and syenites. The percentage of SiO2 varies from 43.5 in
pyroxenites to 63.5 % in syenites. Total alkalies increase from 1.7 to
11.4 % (Fig. 1).
As silica increases, the
percentages of TiO2, FeO*, MgO, CaO and P2O5
decrease, while Al2O3 rises slightly. Associated
with gabbro-pyroxenites are low-grade apatite-magnetite and titanite-apatite
ores, REE and noble-metal concentrations, which exceed background values
(Pt – 0.038 g/t, Pd – 0.074, Au – 0.02; the Pt and Au minerals, such as
keithconnite, moncheite and electrum, were identified). The percentage
of TiO2 in ore zones is as high as 2.17 % and that of P2O5
is 2.16 %. The bodies vary in thickness from 40 to 100 m, but high
REE, Ba and Sr concentrations in pyroxenites indicated their Ti-P-TR-specialization.
The concentrations of these elements are shown in the Table in
comparison with alkaline-ultramafic gabbro-carbonatite massifs of
Proterozoic age (Eletozero and Tikshozero massifs) in Karelia.
Syargozero rocks are
typically rich in REE, especially LREE. In pyroxenites, the
concentration of ∑REE is as high as 1262 ppm, that of Ba is 105-439,
that of Sr is 546-2749 and that of Zr is 84-264. In gabbro, the
concentration of ∑REE is 830 ppm, that of Ba is 1263, that of Sr is 1058
and that of Zr is 167. In monzodiorites, the concentration of ∑REE
452 is ppm, that of Ba is up to 2144 and those of Sr and Zr are about
the same. In syenites, total ∑REE declines to 332 ppm, Ba is
1986, Sr is 1385 and Zr is 143. Based on REE distribution spectra, their
concentrations were clearly shown to decrease with a rise in SiO2
(Fig. 1), which is possible upon the fractionation of a permanent
association of the minerals which concentrate these elements, e.g.
sphene and apatite. The REE content of Syargozero rocks is slightly
higher than that of the Panozero pluton.
Pyroxenites and gabbro
(phase I). Early alkaline metasomatism, induced by the intrusion of
phase-II monzodiorites, is accompanied by phenites – the appearance of
Ba-bearing К-feldspar
(up to 2.75 % Bao) and phlogopite in pyroxenites and gabbro; sphene,
ilmenite and F-apatite were identified. Sphene is often zonal, which is
due to the presence of impurities: 1.48-2.29 % Ce2O3
and 2.2% Nd2O3. Upon lower-temperature
alterations, associated with the intrusion of albitite veins, epidote-group
minerals which also contain lanthanoids are formed in these rocks.
Ce-epidote contains 7.3-8.6% Ce2O3 and orthite
carries 18.68% ∑Ce2O3, Nd2O3
and La2O3. Carbonates, e.g. parasite which
contains Ce, La, Nd and Pr, are formed at later stages. Barite with Sr
as impurity (SrO 1-10 %) is abundant.
Monzodiorites and
syenites (phase
II) consist dominantly of feldspars (albite with BaO impurity 0.09-0.81
%, К-feldspar
- 0.22-1.46 % BaO). Lanthanoids in these rocks are part of Ce-epidote
and orthite (14.4-16.26% ∑La2O3, Ce2O3,
Nd2O3). Later barite with Sr impurity (1.64% SrO)
is common in both rock types; even celestine (45.70% SrO) appears in
syenites at late alteration stages.
Syargozero rocks are
generally specialized for P, Ti, Ba and Sr and are enriched in REE.
Maximum REE concentrations (up to 1262 ppm) are typical of pyroxenites.
Sphene, epidote-group minerals and late F-bearing carbonates are REE-concentrator
minerals. Ba accumulates in the feldspars of more felsic differentiates
of the complex and associated metasomatic rocks. In late processes, Ba
and Sr are concentrated in barite and celestine.
Fig.
1. Percentages
of alkalies (%), Ba, Sr and Zr (ppm) in the rocks of the Syargozero
complex.
Fig.
2.
REE distribution in the
phase-I (a) and phase-II (b) rocks of the Syargozero complex in
comparison with the Panozero pluton (after S.B.Lobach-Zhuchenko) and
host granodiorites. Normalization for chondrite (Sun & McDonough, 1989).
А:
1 – pyroxenites, 2 – gabbro, 3 – mafic complex of the Panozero pluton;
B: 1 – monzodiorites, 2 – syenites, 3 - host granodiorites; monzonites
(phases I-III) and quartz monzonites of the Panozero pluton.
Table.
Rare and rare-earth
element concentrations in the AR moderately alkaline rocks of the
Syargozero complex against those of the Panozero pluton and PR alkaline
formation.
|
Locality
(age) |
Rock |
Y |
Sr |
Ba |
Ta |
Nb |
∑REE |
P2O5 |
TiO2
|
Moderately alkaline |
Syargozero
complex
(~2.74
Ga) |
Pyroxenites
Gabbro
Monzodiorites
Syenites |
51.92
37.73
22.16
12.22 |
1312.21
1024.61
1621.41
1394.61 |
104.92
1261.80
2144.20
1985.80 |
1.59
3.21
1.28
0.68 |
14.24
27.65
13.06
10.02 |
1262.05
830.14
452.81
332.98 |
2.16
0.8
0.59
0.32 |
1.68
1.06-1.51
0.93
0.54 |
Panozero
complex
(~2.74
Ga) |
Gabbro
Monzonites
Quartz monzonites |
31
23
12 |
1406
1416
890 |
2115
1904.76
1606 |
|
|
380.06
267.61
145.1 |
|
|
Alkalinе |
Tikshozero
massif
(1.9-1.8
Ga) |
Pyroxenites
Iolite
Carbonatite |
<15
<15
25 |
78
575
4364 |
|
0.3
5.8
35.5 |
<5
47
260-930 |
41.91*
299.19*
423.9-1251.3* |
0.12
7.80 |
2.28
0.08 |
Eletozero
massif
(1.9-1.8
Ga) |
Pyroxenite
Pegmatoid gabbro
Ore gabbro
Alkaline pegmatite
Syenite |
<15
|
220
676.5
845.6 |
626.96
3224.38 |
1.29
0.32
0.67
37.3
5.61 |
17
|
94.81*
35.27*
35.72*
971.97*
108.3* |
0.27
1.22 |
5.44
9.09
0.39 |
* Total REE (La,
Сe,
Nd, Sm, Eu, Tb, Yb, Lu), Northern GE data; REE, Y, Sr, Ba, Ta, Nb (ppm),
P2O5
and TiO2 (%).
References:
Slyusarev V.D., Kuleshevich
L.V., Pavlov G.М.,
Lavrov М.М.,
Zemtsov V.А.
Subalkaline magmatism of the Syargozero area //Geology and useful
minerals of Karelia. Petrozavodsk. 2001. No. 3. P. 66-86.
Lobach-Zhuchenko S.B.,
Rollinson H., Chekulaev V.P., Guseva N.S., Arestova N.А.,
Kovalenko А.V.
Geology and petrology of the Archaean high-K and high-Mg Panozero
massif, Central Karelia // Petrologia. 2007. V.15. No. 5. P. 493-523.
Lobach-Zhuchenko S.B.,
Rollinson H.R., Chekulaev V.P., Arestova N.A., Kovalenko A.V., Ivanikov
V.V. Guseva N.S., Matukov D.I., Jarvis K.E. The Archean sanukitoid
series of the Baltic Shield: geological setting, geochemical
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