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Revised Eburnean geodynamic evolution of the ... - Tectonique.net

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Gravity anomalies are dominantly controlled by <strong>the</strong> distribution<br />

<strong>of</strong> <strong>the</strong> relatively dense metavolcanic group (Sefwi Group) and <strong>the</strong><br />

less dense metasedimentary groups (Kumasi and Tarkwa groups).<br />

The small differences between <strong>the</strong> observed and modelled gravity<br />

anomalies are difficult to determine given <strong>the</strong> model resolution is<br />

higher than <strong>the</strong> gravity data.<br />

5. Discussion<br />

5.1. Eoeburnean phase (2187–2158 Ma)<br />

Paleoproterozoic rocks <strong>of</strong> <strong>the</strong> sou<strong>the</strong>rn Ashanti Belt were<br />

strongly deformed, mineralised and intruded by granitoids during<br />

<strong>the</strong> “<strong>Eburnean</strong> Orogeny” (Fig. 17). Previous interpretations <strong>of</strong> <strong>the</strong><br />

regional tectonic <strong>evolution</strong> (e.g. Allibone et al., 2002a; Feybesse<br />

S. Perrouty et al. / Precambrian Research 204– 205 (2012) 12– 39 35<br />

Fig. 16. (Continued)<br />

et al., 2006) suggest <strong>the</strong> <strong>Eburnean</strong> Orogeny initiated during <strong>the</strong><br />

first phase <strong>of</strong> volcanic accretion and subduction that could correlate<br />

to D1 deformation. This hypo<strong>the</strong>sis is in agreement with <strong>the</strong><br />

interpretation <strong>of</strong> Sefwi Group mafic and ultramafic rocks as an ophiolitic<br />

suite (Attoh et al., 2006; Dampare et al., 2008). Our structural<br />

interpretation gives this accretionary phase a structural context<br />

whereby N-S shortening during D1 produced regional scale E-W<br />

trending folds within <strong>the</strong> Sefwi Group along with <strong>the</strong> intrusion <strong>of</strong><br />

syn-tectonic granitoids (Fig. 13).<br />

D1 occurred across south-eastern part <strong>of</strong> <strong>the</strong> Ashanti belt<br />

(Fig. 13) and below <strong>the</strong> Tarkwa Basin (Fig. 14). In Obuasi, Allibone<br />

et al. (2002a) described transfer faults and lineaments oriented E-<br />

W that were attributed to <strong>the</strong>ir NW-SE D2 shortening (our D3). The<br />

Obuasi deposit is mainly hosted within Kumasi Group metasediments.<br />

However, minor exposures <strong>of</strong> metavolcanics indicate <strong>the</strong>

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