05.02.2013 Views

2. Mineralogy – Petrology – Geochemistry - SWISS GEOSCIENCE ...

2. Mineralogy – Petrology – Geochemistry - SWISS GEOSCIENCE ...

2. Mineralogy – Petrology – Geochemistry - SWISS GEOSCIENCE ...

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

36<br />

Symposium 1: Structural Geology, Tectonics and Geodynamics<br />

1.19<br />

Did Laurentia and Gondwana play terrane tennis in the Palaeozoic? The<br />

implications of a Iapetus convergent margin in the Merida Terrane,<br />

Venezuela<br />

Van der Lelij Roelant 1 , Spikings Richard 1 , Ulianov Alexey 2 , & Chiaradia Massimo 1<br />

1Départment de Minéralogie, Section des Sciences de la Terre et de l’Environnement, Université de Genève, Rue des Maraîchers 13,<br />

CH-1205 Genève, roelant.vanderlelij@unige.ch<br />

2Institute of <strong>Mineralogy</strong> and <strong>Geochemistry</strong>, University of Lausanne, Switzerland<br />

The tectonic, metamorphic and palaeogeographic origin of the basement terranes of the circum-Maracaibo region,<br />

Venezuela and Colombia, are poorly understood. A majority of the reconstructions of western Pangaea place the Merida<br />

Terrane of western Venezuela between the Guyana Shield, Mexican and Central American terranes, and hence unravelling<br />

its tectonic history is a key step to reconstructing western Pangaea. We aim to develop a robust framework for the age and<br />

tectonic origin of the Merida Terrane by using new, in-situ LA-ICP-MS zircon U-Pb geochronology on isotopically and geochemically<br />

characterised igneous and metamorphic rocks of the basement complexes.<br />

Widespread I- and S-type arc magmatism and amphibolite facies metamorphism of sedimentary rocks of the Iglesias<br />

Complex occurred between the late Cambrian and early Devonian (500-415 Ma), corresponding to a north facing Iapetus<br />

continental arc. Detrital zircons from these metasedimentary rocks are early Cambrian and older, which provide a maximum<br />

age for deposition. A magmatic hiatus in the Merida Terrane spans the Devonian to Permian, from ~415- 75 Ma.<br />

A compilation of previous work suggests that faunal assemblages from several locations in the Merida Terrane reveal significant<br />

assemblage transitions. Faunal affinities change from Gondwanan in the Cambrian, to Acado-Baltic in the<br />

Ordovician, to Appalachian in the Silurian. This shift is also characteristic of the Avalonia microcontinent, which rifted<br />

off Gondwana in the Cambrian and accreted to Baltica and finally Laurentia in the Silurian.<br />

To the south of the Merida Andes, the Apure Fault separates the Early Palaeozoic igneous and metamorphic belt from the<br />

Guyana Shield. The latter exhibits extensive Cambrian rifts which were reactivated in the Jurassic, and K/Ar dates obtained<br />

from biotite and feldspar from the basement rocks of the Guyana Shield suggest that the Palaeoproterozoic crust has not<br />

experienced a significant thermal event since ~1Ga. Therefore, we propose that the Apure Fault is the south-eastern<br />

boundary of the Merida Terrane.<br />

We propose two contrasting scenarios for the evolution of NW Gondwana and the Iapetus and Rheic oceans:<br />

A) The Merida Terrane may be autochthonous or para-autochthonous to Gondwana, which would imply that the NW<br />

corner of Gondwana was a Cambrian to Silurian active margin. This implicitly means that the rift to drift transition<br />

which led to the opening of the Rheic Ocean in the Cambrian-Ordovician did not occur this far west, precluding the<br />

Rheic Ocean separating NW Gondwana from Laurentia, which in turn suggests that these two supercontinents were<br />

close or perhaps connected by the Silurian. A simultaneous back-arc to rift-to drift transition, as required for the opening<br />

of the Rheic Ocean in the Cambrian-Ordovician, would lead to scenario B:<br />

B) The Merida Terrane may be an allochthonous, Avalonia type terrane which separated from Gondwana in the Cambrian-<br />

Ordovician due to back-arc basin becoming an oceanic spreading centre (Figure 1). In this scenario, NW Gondwana<br />

would become the southern passive margin of the Rheic Ocean; the Merida Terrane would at the same time be the<br />

southern Iapetus active margin and the Rheic Ocean northern passive margin (Figure 1). In the Silurian, the Merida<br />

Terrane would, like Avalonia, collide with Laurentia during as the Iapetus closed, resulting in the Acadian orogeny in<br />

the Appalachians. Following the Amalgamation of Pangaea it would have been re-accreted to Gondwana.<br />

Swiss Geoscience Meeting 2011<br />

Platform Geosciences, Swiss Academy of Science, SCNAT

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!