Ae. Rapalini et Ra. Astini, PALEOMAGNETIC CONFIRMATION OF THE LAURENTIAN ORIGIN OF THE ARGENTINE PRECORDILLERA, Earth and planetary science letters, 155(1-2), 1998, pp. 1-14
Several recent tectonic models have portrayed the Argentine Precordill
era has been recently portrayed as an Early Paleozoic Laurentian deriv
ed exotic terrane now found in southwestern South America. These model
s have primarily been based on strong biogeographic and stratigraphic
evidence, however, no paleomagnetic data have previously been availabl
e to independently test them. A paleomagnetic study was, therefore, ca
rried out on the Early Cambrian Cerro Totora Formation, exposed in the
northern reaches of the Argentine Precordillera. After stepwise therm
al demagnetization a pre-folding remanence was identified in ten sites
of this formation, yielding a paleomagnetic pole (CT) at 37.0 degrees
N, 314.1 degrees E, A(95) = 5.8 degrees. This pole is not consistent
with the latest Proterozoic-Early Paleozoic apparent polar wander path
for Gondwana, but it agrees with the Early Cambrian Section of the La
urentian path if the Argentine Precordillera is positioned as the conj
ugate margin of the Ouachita embayment in southeast Laurentia. This re
sult confirms that the Precordillera is an allochthonous terrane deriv
ed from Laurentia in Cambrian times, that was later accreted to Gondwa
na, probably in Middle Ordovician times. (C) 1998 Elsevier Science B.V
.