New geochronological data (UPb and SmNd) are used to constrain the Archean crustal growth and evolution of the southwestern part of the Reguibat Rise (Amsaga area) in the West African craton. The results are summarized as follows. (1) UPb zircon data indicate an emplacement age of 2986 ± 8 Ma for the magmatic protolith of a charnockitic pluton, in agreement with a whole-rock SmNd isochron at 3012 ± 142 Ma. Positive ϵ Nd(3.0) values ranging between 0.89 and 1.95 and agreement between Nd model ages (between 3.23 and 3.10 Ga) and UPb age indicate a juvenile origin for the magmatic protolith and imply a crustal growth event at ca 3.0 Ga. Seven rims of the charnockitic zircons yield discordant 207Pb/ 206Pb ages ranging from 2979 ± 11 to 2737 ± 11 Ma and are interpreted as resulting from growth during the granulitic event. (2) Whole-rock SmNd data on migmatitic orthogneisses that form the central part of the area indicate an Archean age for their magmatic protolith ( T DM ranging from 3.24 to 2.87 Ga) in agreement with a previous single zircon evaporation age of 2836 ± 16 Ma (Potrel, 1994). (3) Two late-tectonic, postgranulite plutons (both granite and gabbro) dated at ca 2.73 Ga mark the end of the granulitic event. The granite provides a UPb age of 2726 ± 7 Ma and the gabbro a mineral SmNd isochron age of 2706 ± 54 Ma. The T DM ages ranging from 3.1 to 3.2 Ga indicate an origin by crustal reworking of the granite and negative ϵ Nd(2.7) value (−0.7) of the gabbro indicate crustal contamination during emplacement. These results, combined with previous work (Potrel et al., 1996), indicate that the Archean Reguibat Rise formed through a succession of crustal growth events from at least 3.50-3.45 Ga until 2.73 Ga. A major granulitic event took place at ca 2.73 Ga and was accompanied by emplacement of crustally derived magmas.
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