Puncoviscana, folded belt in northwestern Argentina: testimony of Late Proterozoic Rodinia fragmentation and pre-Gondwana collisional episodes: a reply
Rh. Omarini et al., Puncoviscana, folded belt in northwestern Argentina: testimony of Late Proterozoic Rodinia fragmentation and pre-Gondwana collisional episodes: a reply, INT J E SCI, 90(4), 2001, pp. 894-902
Franz and Lucassen (2000) rise several important points, which are primaril
y related to the Puncoviscana belt role in northwestern Argentina. Their di
scussion consisted of three major overviews: (a) the Puncoviscana belt evol
ution related to the Proterozoic Rodinia fragmentation; (b) the geochemical
data associated with volcanic rock interlayered in the Puncoviscana format
ion and (c) the central Andes residual gravity field interpretations. It wi
ll be shown in this reply that their claim against our interpretation is th
e consequence of an equivocal handling of the geological times, the tectoni
c episodes and the associated lithologies in the wide context of the Puncov
iscana belt type paleogeographic connections.
Some present geochronological data oldest that 1.1 to 0.9 Ga. are consisten
t with an autochthonous basement integrated by very ancient protoliths adjo
ins to the typical Grenville belt rocks before the Rodinia fragmentation. T
he autochthonous condition must be interpreted only as the Rodinia supercon
tinental reality, that after remains into the new Laurentia-Cabalonia-Panno
tia continental units. In this context, the Theia, Candelaria, Iapetus and
other proto-oceanic rifts begins an allochthonous reality for lot of the dr
ifting crustal slivers during the Pannotian Cycle, (Late Proterozoic - Earl
y Paleozoic) in the break-up geotectonic times of the post-Rodinian superco
ntinent.
The Puncoviscana geochemical interpretation presented in this reply shows a
n very clear plate tectonic evolution in various steps: (1) the proto-rift
lineaments from the extensional regimen of the Candelaria triple point (t(D
M) similar to0.70 to 0.78 Ga.); (2) the passive continental margin sequence
s (700 to 600 Ma); and (3) the magmatic arc in the compressive regimen belo
nging to the Pampean orogeny (580 to 534 Ma).