INVESTIGADORES
RAPELA Carlos Washington
congresos y reuniones científicas
Título:
Early Palaeozoic evolution of the Gondwana margin of South America
Autor/es:
PANKHURST, R.J; RAPELA, C.W.; CASQUET, C.; BALDO, E.G; SAAVEDRA, J.; GALINDO, C.
Lugar:
Cape Town
Reunión:
Congreso; Gondwana 10: Event Stratigraphy of Gondwana; 1998
Institución organizadora:
University of Johannesburg
Resumen:
Two main pre-Silurian
tectonomagmatic episodes (Pampean and
Famatinian cycles or orogenies) wore involved in the construction of the western margin of Gondwana (Fig. 1). From a
multi-disciplinary study of a 500 km transect in the
Sierras Pampeanas, central-west Argentina, these are identified and re-defined more precisely than in previous literature and interpreted in a more
tightly constrained context. Each of these
cycles culminated in a microcontinental collision against the proto-Andean margin of Gondwana, but the first entirely pre-dated
the rifting of the Argentine Precordillera Terrane from Laurentia (Astini et al, 1995; Keller el al.,
in press), and the second,
we believe, pre-dated the final accretion of that terrane the earliest recognized event is
deposition of an Early Cambrian
passive margin sequence (Puncoviscana Formation and
equivalents over an unexposed Mesoproterozoic cratonic basement (Nd model ages
of 1 500 ¡À 200 Ma, inherited zircons 800-1400 Ma; Pankhurst et al., in press).
The Pampean Orogeny (Rapela et al., in press), previously thought to
be Neoproterozoic in age,
started in Early Cambrian times with a short subduction phase, indicated by
530¡À3 Ma calc-alkaline granitoids in the Sierras de C¨®rdoba (dated by
conventional U-Pb on abraded zircons). During the Pampean Terrane collision, the mar gin was buried to
granulite4acies conditions (M2: 8.6 ¡À0.8 kbar, 810 ¡À 50¡ãC,
determined using the TWEEQU
thermo-barometric programme of
Berman, 1991), generating widespread migmatites. Relaxation of P to ca 4
kbar following the climax of metamorphism led to anatexis and formation of
highly peraluminous granites
in the Eastern Sierras Pampeanas. These events were essentially synchronous at ca
525 Ma according (o concordant results from SHRIMP U-Pb data on orthogneiss
monazite, Rb-Sr whole rock on the mw-grade passive margin rocks, and Rb-Sr isochron and conventional U-Pb
zircon dating on the anatectic granites.
After a brief period of quiescence, subduction of the southern lapetus Ocean
floor beneath Gondwana recommenced. The second major episode, the Famatinian
cycle is predominatly represented by intense subduction- relted magmatism of
early-Middle Ordovician age (Pankhurst et al., in press). A wid volcanic and
plutonic arc and ensialic back-arc basin developed to the west of the Pampean
accreted terrane. The main granodiorite phase of the batholith of the southern
Famatinian arc is associated with an S2 fabric and shear zone
formation, and was emplaced late in the deformational history of the passive
margin metasediment. Conventional SHRIMP U-Pb zircon dating yielded a combined
age of 490 ¡À 5 Ma. Younger
monzogranites gave Rb-Sr whole rock age of 470-450 Ma., typical of granites in
the Sierra de Famatina, but geochemical continuity with the main granodiorite
suite raises the possibility than these are partially reset age. All the
calc-alkaline rocks of the southern Famatinian arc have high initial 87Sr/86Sr
(0.7075 ¨C 0.7105) and low ¦ÅNdt (-4.6 to -6.3), inherited from lower
crust. Sm-Nd model ages of 1600-1700 Ma., indicated than the underlining crust
is identical to that beneath the foreland to the east. This part of Famatinian
arc at least was thus a continental one, developed on the margin of Gondwana during
the rifting and drifting of Precordillera Terrane.
The Precordillera Terrane itself consists of a lower
Paleozoic Carbonate platform, formed over subsided Grenvillian crust while
still part of Laurentia (Keller et al., in press). It finally collided with
Gondwana in Silurian-Devonian times.