INVESTIGADORES
RAPELA Carlos Washington
artículos
Título:
Las orogénesis del Paleozoico Inferior en el margen proto-andino de América del Sur, Sierras Pampeanas, Argentina
Autor/es:
RAPELA, C.W.; CASQUET, C.; BALDO, E.G.; DAHLQUIST, J.A.; PANKHURST, R.J; GALINDO, C.; SAAVEDRA, J.
Revista:
JOURNAL OF IBERIAN GEOLOGY
Editorial:
SERVICIO PUBLICACIONES
Referencias:
Lugar: Madrid; Año: 2001 vol. 27 p. 23 - 41
ISSN:
1698-6180
Resumen:
The proto-Andean margin of Gondwana was
the site of at least two orogenies
between the break-up of the Rodinia
supercontinent, at the end of the
Neoproterozoic, and the new continental
amalgamation of Pangea at the end of the
Carboniferous. Both orogenies were
preceded by a period of ocean opening and
passive margin sedimentation and ended
with ocean subduction, development of
cordilleran-type magmatic arcs and
continent-continent collision. The Pampean
orogeny took place in a relatively short
period of time in the early Cambrian (535-
520 Ma; subduction ? magmatic arc stage
and continental collision), and ended
with the orthogonal accretion of a
semiautochthonous microcontinental fragment -
the Pampean Terrane- to the Gondwana margin.
On the other hand, the Famatinian
orogeny spanned a longer period of time in
the Ordovician and Silurian (499-435
Ma). During this orogeny the exotic
Precordillera Terrane was accreted to the margin
of Gondwana (460 Ma). This terrane,
probably of Laurentian provenance, consists
of a Grenvillian basement (1.1 Ga) and a
Lower Paleozoic sedimentary cover
of the carbonate platform type. Accretion
was probably oblique to the Gondwana
margin, and the eastern margin of the
Precordillera Terrane was thoroughly affected
by Famatinian deformation and regional
metamorphism. The basement to the
Upper Paleozoic and Mesozoic Andean belts,
situated to the west of the
Precordillera, also appears to be formed
by Grenvillian metamorphic rocks, so that
the greater part of the Central Andes
between 26ºS and 34ºS are established upon
allocthonous terranes. The Lower Paleozoic
paleogeography of continental masses
involved in the
collision is not still fully understood.