PRECAMBRIAN BASEMENT AROUND WADI-HALFA, SUDAN - A NEW PERSPECTIVE ON THE EVOLUTION OF THE EAST SAHARAN CRATON

Citation
Rj. Stern et al., PRECAMBRIAN BASEMENT AROUND WADI-HALFA, SUDAN - A NEW PERSPECTIVE ON THE EVOLUTION OF THE EAST SAHARAN CRATON, Geologische Rundschau, 83(3), 1994, pp. 564-577
Citations number
61
Categorie Soggetti
Geology
Journal title
ISSN journal
00167835
Volume
83
Issue
3
Year of publication
1994
Pages
564 - 577
Database
ISI
SICI code
0016-7835(1994)83:3<564:PBAWS->2.0.ZU;2-4
Abstract
This paper provides new geochemical and isotopic data on the evolution of the western foreland to the Nubian shield of north-east Africa. Th ere is abundant evidence for early to middle Proterozoic crust west of the River Nile, but this was severely affected by the Pan-African (al most-equal-to 500-900 Ma) orogenic cycle. The results are reported of Rb-Sr whole rock and zircon evaporation geochronological studies and w hole rock Sm-Nd and feldspar Pb isotopic analyses for four rock units around Wadi Halfa in northern-most Sudan. These results indicate the p resence of heterogeneous pre-Pan-African crustal components, preserved in mylonitic gneisses and in conglomerates that unconformably overlie the gneisses. Several episodes of crust formation, inferred from zirc on ages, are preserved in the gneisses: 2.6, 2.4, 2.0, 1.7, 1.2 and 0. 72 Ga. Nd model ages for the same units are invariably older than the zircon ages, yet still record a predominantly late Archaean and Palaeo proterozoic history, with depleted mantle model ages between 1.3 and 2 .8 Ga. The earliest recorded Pan-African magmatic event is about 720 M a and dates the beginning of collisional deformation. A younger Pan-Af rican volcanic sequence (almost-equal-to 650 Ma) has isotopic composit ions of Sr and Nd compatible with derivation from late Proterozoic ast henospheric mantle. A almost-equal-to 530 Ma anorogenic 'A-type' grani te also has isotopic compositions suggesting derivation from a primiti ve source. The inferred tectonic evolution began with rifting to form an oceanic re-entrant. This was followed by subduction leading to coll ision at about 700 Ma, accompanied by post-orogenic rifting at about 6 50 Ma.