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Svecofennian complexes<br />

The Palaeoproterozoic greenstones are overla<strong>in</strong> by<br />

volcanic <strong>and</strong> sedimentary rocks compris<strong>in</strong>g several<br />

different but stratigraphically related units. Regionally,<br />

they exhibit considerable variation <strong>in</strong> lithological<br />

composition due to partly rapid changes from<br />

volcanic- to sedimentary-dom<strong>in</strong>ated facies. Stratigraphically<br />

lowest <strong>in</strong> the Kiruna area are rocks of<br />

the Porphyrite Group <strong>and</strong> the Kurravaara Conglomerate.<br />

The former represents a volcanic-dom<strong>in</strong>ated<br />

unit <strong>and</strong> the latter is a ma<strong>in</strong>ly epiclastic unit (Offerberg<br />

1967) deposited as one or two fan deltas<br />

(Kumpula<strong>in</strong>en 2000). The Sammakkovaara Group<br />

<strong>in</strong> northeastern Norrbotten comprises a mixed volcanic-epiclastic<br />

sequence that is <strong>in</strong>terpreted to be stratigraphically<br />

equivalent to the Porphyrite Group <strong>and</strong><br />

the Kurravaara Conglomerate, <strong>and</strong> the Pahakurkio<br />

Group, south of Masugnsbyn. The Muorjevaara<br />

Group <strong>in</strong> the Gällivare area is also considered to be<br />

equivalent to the Sammakkovaara Group <strong>in</strong> the Pajala<br />

area <strong>and</strong> is dom<strong>in</strong>ated by <strong>in</strong>termediate volcaniclastic<br />

rocks <strong>and</strong> epiclastic sediments. In the Kiruna<br />

area, these volcanic <strong>and</strong> sedimentary units are overla<strong>in</strong><br />

by the Kiirunavaara Group that is followed by<br />

the Hauki <strong>and</strong> Maattavaara quartzites constitut<strong>in</strong>g<br />

the uppermost Svecofennian units <strong>in</strong> the area.<br />

In northern F<strong>in</strong>l<strong>and</strong>, pelitic rocks <strong>in</strong> the Lapl<strong>and</strong><br />

Granulite Belt were deposited after 1.94 Ga<br />

(Tuisku & Huhma 2006). Svecofennian units are<br />

ma<strong>in</strong>ly represented by the Kumpu Group <strong>in</strong> the<br />

CLGB (Lehtonen et al. 1998) <strong>and</strong> by the Paakkola<br />

Group <strong>in</strong> the Peräpohja area (Perttunen & Vaasjoki<br />

2001). The molasse-like conglomerates <strong>and</strong> quartzites<br />

compris<strong>in</strong>g the Kumpu Group were deposited<br />

<strong>in</strong> deltaic <strong>and</strong> fluvial fan environments after 1913<br />

Ma <strong>and</strong> before c. 1800 Ma (Rastas et al. 2001).<br />

The Kumpu rocks apparently are equivalent to the<br />

Hauki <strong>and</strong> Maattavaara quartzites, <strong>and</strong> Porphyrite<br />

Group rocks <strong>and</strong> the Kurravaara Conglomerate of<br />

the Kiruna area.<br />

With the present knowledge of ages <strong>and</strong> petrochemistry<br />

of the Porphyrite <strong>and</strong> Kumpu Groups,<br />

it is possible to attribute these rocks completely to<br />

the same event of collisional tectonics <strong>and</strong> juvenile<br />

convergent marg<strong>in</strong> magmatism. This period of convergence<br />

was manifested by the numerous <strong>in</strong>trusions<br />

of Jörn- (south of the craton marg<strong>in</strong>) <strong>and</strong> Hapar<strong>and</strong>a-<br />

(with<strong>in</strong> the craton) type calc-alkal<strong>in</strong>e <strong>in</strong>trusions, as<br />

described by Mellqvist et al. (2003). With<strong>in</strong> a few<br />

million years, this period of convergent marg<strong>in</strong> magmatism<br />

was followed by a rapid uplift recorded <strong>in</strong><br />

extensive conglomeratic units, more alkal<strong>in</strong>e <strong>and</strong><br />

terrestrial volcanism (Vargfors-Arvidsjaur Groups<br />

south of the craton marg<strong>in</strong> <strong>and</strong> the Kiirunavaara<br />

Group with<strong>in</strong> the craton) <strong>and</strong> plutonism (Gallejaur-<br />

Arvidsjaur type south of the craton marg<strong>in</strong>, Perthite<br />

Monzonite Suite with<strong>in</strong> the craton). This took place<br />

between 1.88 <strong>and</strong> 1.86 Ga <strong>and</strong> the ma<strong>in</strong> volcanic episode<br />

probably lasted less than 10 million years.<br />

The evolution after c. 1.86 is ma<strong>in</strong>ly recorded<br />

by an extensive S-type magmatism (c. 1.85 Ga<br />

Jyryjoki, <strong>and</strong> 1.81–1.78 Ga L<strong>in</strong>a-type <strong>and</strong> the Central<br />

Lapl<strong>and</strong> Granitoid Complex) derived from anatectic<br />

melts <strong>in</strong> the middle crust. In the western part of the<br />

shield, extensive I- to A-type magmatism (Revsund-<br />

Sorsele type) formed roughly N-S trend<strong>in</strong>g batholiths<br />

(the Transc<strong>and</strong><strong>in</strong>avian Igneous Belt) coeval with the<br />

S-type magmatism. Scattered <strong>in</strong>trusions of this type<br />

<strong>and</strong> age also occur further east (e.g. Edefors <strong>in</strong> Sweden,<br />

Nattanen <strong>in</strong> F<strong>in</strong>l<strong>and</strong>). The period from c. 1.87<br />

to 1.80 Ga possibly also <strong>in</strong>volved a shift <strong>in</strong> orogenic<br />

vergence from NE-SW to E-W <strong>in</strong> the northern part of<br />

the Shield as suggested by Weihed et al. (2002).<br />

Palaeoproterozoic magmatism<br />

Early rift<strong>in</strong>g <strong>and</strong> emplacement of<br />

layered igneous complexes<br />

The beg<strong>in</strong>n<strong>in</strong>g of the rift<strong>in</strong>g period between 2.51 <strong>and</strong><br />

2.43 Ga is <strong>in</strong>dicated by <strong>in</strong>trusion of numerous layered<br />

mafic igneous complexes (Alapieti et al. 1990,<br />

Weihed et al. 2005). Most of the <strong>in</strong>trusions are located<br />

along the marg<strong>in</strong> of the Archaean granitoid<br />

area, either at the boundary aga<strong>in</strong>st the Proterozoic<br />

supracrustal sequence, totally enclosed by Archaean<br />

granitoid, or enclosed by a Proterozoic supracrustal<br />

sequence. Most of the <strong>in</strong>trusions are found <strong>in</strong> Wtrend<strong>in</strong>g<br />

Tornio-Näränkävaara belt of layered <strong>in</strong>trusions<br />

(Ilj<strong>in</strong>a & Hanski 2005). Rest of the <strong>in</strong>trusions<br />

are found <strong>in</strong> NW Russia, central F<strong>in</strong>nish Lapl<strong>and</strong> <strong>and</strong><br />

NW F<strong>in</strong>l<strong>and</strong>. Alapieti <strong>and</strong> Laht<strong>in</strong>en (2002) divided<br />

the <strong>in</strong>trusions <strong>in</strong>to three types, (1) ultramafic–mafic,<br />

(2) mafic <strong>and</strong> (3) <strong>in</strong>termediate megacyclic. They also<br />

<strong>in</strong>terpret the ultramafic–mafic <strong>and</strong> the lowermost part<br />

of the megacyclic type to have crystallised from a<br />

similar, quite primitive magma type, which is characterised<br />

by slightly negative <strong>in</strong>itial εNd values <strong>and</strong><br />

relatively high MgO <strong>and</strong> Cr, <strong>in</strong>termediate SiO 2, <strong>and</strong><br />

low TiO 2 concentrations, resembl<strong>in</strong>g the bon<strong>in</strong>itic<br />

magma type. The upper parts of megacyclic type <strong>in</strong>trusions<br />

<strong>and</strong> most mafic <strong>in</strong>trusions crystallised from<br />

an evolved Ti-poor, Al-rich basaltic magma.<br />

Amel<strong>in</strong> et al. (1995) suggested two age<br />

groups for the <strong>in</strong>trusions for Fennosc<strong>and</strong>ian Shield,<br />

the first with U–Pb ages at 2.505–2.501 Ga, <strong>and</strong> the<br />

second at 2.449–2.430 Ga. All F<strong>in</strong>nish layered <strong>in</strong>trusions<br />

belong to the younger age group. The <strong>in</strong>trusions<br />

were later deformed <strong>and</strong> metamorphosed dur<strong>in</strong>g the<br />

13

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