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Calc-alkaline and tholeiitic dyke swarms of Tandilia, Rio de laPlata craton, Argentina: U�/Pb, Sm�/Nd, and Rb�/Sr 40Ar/39Ardata provide new clues for intraplate rifting shortly after the
Trans-Amazonian orogeny
W. Teixeira a,�, J.P.P. Pinese b, M. Iacumin c, V.A.V. Girardi a, E.M. Piccirillo c,H. Echeveste d, A. Ribot d, R. Fernandez d, P.R. Renne e, L.M. Heaman f
a Centro de Pesquisas Geochronological, Institute of Geosciences, University of Sao Paulo, Rua do Lago 562, 05422-970 Sao Paulo, Brazilb Department of Geoscience, University of Londrina, P.O. Box 6001, 86051-990 Londrina, Brazil
c Dipartimento di Scienze della Terra, University of Trieste, Via Weiss 8, 34127 Trieste, Italyd University of La Plata, INREMI and LEMIT, Calle 52, P.O. Box 128, 1900 La Plata, Argentina
e Berkeley Geochronology Center, 2455 Ridge Road, Berkeley, CA 94709, USAf Department of Earth and Atmospheric Sciences, University of Alberta, Edmonton, Alta., Canada T6G 2E3
Received 1 April 2001; received in revised form 28 November 2001; accepted 19 March 2002
Abstract
The Tandilia system, Argentina, southernmost part of Rio de la Plata craton (RLPC), is intruded by two
Paleoproterozoic unmetamorphosed dyke swarms which are: (i) intermediate (I) and acid (A); and (ii) basic (B1 and B2)
in composition. The latter dykes have tholeiitic characteristics, while for both I and A dykes major, minor, and trace
elements, including REE (e.g. the higher values of SiO2, K2O and Ba compared to tholeiitic dykes) are characteristic of
calc-alkaline suites. The calc-alkaline dykes (I and A) yielded 40Ar/39Ar step-heating plateau ages of emplacement of
20209/24 and 20079/24 Ma. These ages are within error in agreement with a Rb�/Sr errorchron of 19569/110 Ma (1s)
[initial 87Sr/86Sr�/0.70389/0.0025 (MSWD�/19)]. An upper intercept U�/Pb age on two baddeleyites from a tholeiitic
(B1) dyke places the intrusion at 15889/11 Ma. The tholeiitic dykes (B1 and B2) have K�/Ar whole-rock ages from 8039/
14 to 11939/18 Ma and a 40Ar�/39Ar plateau age of 8119/36 Ma (2s) on plagioclase. These discordant apparent ages
suggest variable Ar loss of the mineral systems. Calc-alkaline dykes mainly trend E�/W, and were emplaced during the
transtensional stage of the Trans-Amazonian orogeny during which the plutonic rocks of the Tandilia system were
formed. Such a scenario has similarities with the Eburnean evolution of the Richtersveld plutonic arc complex of the
southern African subcontinent (Namaqualand) that faces the RLPC in the West Gondwana reconstruction. The
significantly younger tholeiitic dykes of Tandilia (1.59 Ga) trend mainly NW-SE. Their presence constrains the time of
crustal extension at the Paleo-Mesoproterozoic boundary during which basin-formation tectonics and anorogenic
magmatism took place worldwide within a stabilized Paleoproterozoic lithosphere. Such an intraplate regime for the
emplacement the youngest dykes of Tandilia is consistent with transcontinental scale, diachronous extensional episodes
� Corresponding author. Tel.: �/55-11-3091-4274; fax: �/55-11-3091-4295
E-mail address: [email protected] (W. Teixeira).
Precambrian Research 119 (2002) 329�/353
www.elsevier.com/locate/precamres
0301-9268/02/$ - see front matter # 2002 Elsevier Science B.V. All rights reserved.
PII: S 0 3 0 1 - 9 2 6 8 ( 0 2 ) 0 0 1 2 8 - 6
within the South American continent which initiated shortly after the Trans-Amazonian orogeny, as illustrated by the
1.73 Ga Florida tholeiitic dyke swarm and coeval, anorogenic granitoids scattered across the RLPC (Uruguay and
Tandilia). Paleoproterozoic geologic features of the RLPC*/namely, the occurrence of plutonic arc rocks (2.14�/2.07
Ga) succeeded by emplacement of anorogenic granitoids and mafic dykes (1.73�/1.59 Ga)*/allow direct correlation
with the postulated Gondwana counterpart, mirrored by broadly contemporary plutonic rocks of the Richtersveld and
Bushmanland subprovinces of Namaqualand. The broad picture reinforces the idea that the Trans-Amazonian/
Eburnean orogenies played an important role for juvenile crustal accretion within the southern South America and its
southern Africa counterpart, which was followed by a tendency to dispersion of the stabilized continental fragments
during the Mesoproterozoic, preceding the assembly of the Rodinia supercontinent.
# 2002 Elsevier Science B.V. All rights reserved.
Keywords: Geochronology; Paleoproterozoic dykes; Tandilia; Rio de la Plata craton; Africa
1. Introduction
Precambrian mafic dyke swarms record initial
stages of intraplate rifting or at least manifesta-
tions of crustal extension, which may be associated
with the orogenic collapse of mobile belt evolu-
tion. However, in most cases, mafic dykes cannot
be dated reliably by Rb�/Sr and K�/Ar methods
when minor post-crystallization alteration is pre-
sent. Fortunately, accurate dating of dyke empla-
cement can be obtained by the U�/Pb method
applied to baddeleyite and zircon. In general,
baddeleyite is better because, unlike zircon, it
tends to be concordant (i.e. 98�/100% concordant),
and since baddeleyite is rare in crustal rocks,
inheritance is not common in mafic rocks (Le-
Cheminant and Heaman, 1989; Heaman, 1991). In
addition, the 40Ar�/39Ar technique has been useful
for dating either primary biotite minerals from
mafic dykes or micas from contact-baked meta-
morphic country rocks in sharp contact with them
(Renne et al., 1990; Teixeira et al., 1999).
This paper presents results of isotopic dating
(40Ar�/39Ar mineral step heating, U�/Pb badde-
leyite, and Rb�/Sr and Sm�/Nd whole-rock ana-
lyses) on two distinct Proterozoic dyke swarms
that occur in the Tandilia system, Rio de la Plata
craton (RLPC)*/an igneous�/metamorphic com-
plex (Cingolani and Dalla Salda, 2000) formed
during the Trans-Amazonian orogeny (2.2�/2.0
Ga). Geochronologic data along with geochemical
results, constrain the origin of these dykes, as well
as their relationship with Paleoproterozoic crustal
evolution. Comparison of these rocks with coeval
geologic units within the southern African con-
tinent is presented, providing a better understand-
ing of the nature of the tectonism at the Paleo-
Mesoproterozoic boundary, as well as new insights
on the reconstruction of supercontinents during
the Proterozoic.
2. Geologic and geochronologic overview
The RLPC is one of the cratons in the contin-
uous network of mobile belts developed during the
Brasiliano/Pan-African orogenies of Western
Gondwanaland (Brito Neves and Cordani, 1991).Basement of the RLPC is known as the Piedra
Alta terrane in the western part of the Uruguayan
Shield (Fig. 1). This terrane includes three distinct
volcano-sedimentary sequences with low-grade
metamorphism and plutonic suites of TTG affinity
(Cingolani et al., 2001) all involved in the Trans-
Amazonian orogeny. The Florida dyke swarm
(Bossi et al., 1993; Mazzucchelli et al., 1995) wasemplaced into the Piedra Alta terrane at 1730 Ma
and was not later deformed, thereby constraining
the minimum age of tectonic stabilization of the
RLPC (Teixeira et al., 1999). The Piedra Alta
terrane is separated from the Nico Perez terrane
(Fig. 1) by an expressive subvertical shear zone
(Bossi et al., 1993). The latter terrane is allochto-
nous and has a different geologic history from itsneighbours*/the western Paleoproterozoic Piedra
Alta and the eastern Neoproterozoic terranes.
Piedra Alta granitoids display Rb�/Sr isochron
whole-rock ages between 2.4 and 2.0 Ga with
relatively low initial 87Sr/86Sr ratios (Preciozzi and
Bourne, 1992; Cingolani et al., 2001). SHRIMP
W. Teixeira et al. / Precambrian Research 119 (2002) 329�/353330
U�/Pb zircon analyses on volcanic rock from a
supracrustal belt yielded an age of 21409/10 Ma
while intrusive tonalite and granodiorite yielded
20809/15 Ma (Bossi et al., 2001). These plutons
are contemporary with granitic rocks of the Isla
Mala suite, as indicated by SHRIMP U�/Pb zircon
ages between 20659/9 and 20749/6 Ma (Hartmann
et al., 2000) and a conventional U�/Pb zircon age
of 20889/12 on granodiorite from this suite (Pre-
ciozzi et al., 1999). Migmatites, gneisses and
granitoids in the Piedra Alta terrane give Nd
model ages (TDM) between 2.45 and 2.06 Ga
Fig. 1. Distribution of main (Paleoproterozoic) cratons in the West Gondwana (a), showing the adjacent Meso- and Neoproterozoic
tectonic framework in the southern South America and southwest corner of Africa (b). (c) Geologic sketch map of the Rio de la Plata
craton (Piedra Alta (PA) terrane and the Tandilia system), showing the dyke occurrences and the adjoinging the Nico Perez (NP)
terrane and the Neoproterozoic Dom Feliciano belt (adapted from Bossi et al., 1993; Dalla Salda et al., 1988). See text for details.
W. Teixeira et al. / Precambrian Research 119 (2002) 329�/353 331
(Preciozzi et al., 1999). Therefore, the Trans-Amazonian orogeny was a period juvenile accre-
tion and regional metamorphism. Regional cool-
ing of the Piedra Alta terrane took place around
2.0�/1.9 Ga, based on K�/Ar and 40Ar�/39Ar ages
on the gneissic rocks (Teixeira et al., 1999).
The Nico Perez terrane has had a contrasting
crustal evolution compared with that of the Piedra
Alta terrane. Geologic mapping supported bySHRIMP U�/Pb zircon dating indicates the occur-
rence of an Archean nucleus of about 3100 Ma
(protoliths as old as 3410 Ma) which is surrounded
by a 2600 Ma granulite facies gneissic complex
(Bossi et al., 2001). This complex was further
subjected to reworking and crustal shortening at
2100 and 1200 Ma, respectively (Bossi et al., 2001;
Cingolani et al., 2002). Rapakivi granites (1.75 Ga)are also present in the Nico Perez terrane, as well
as felsic and mafic magmatism, dated between 0.70
and 0.56 Ga (Rivalenti et al., 1995; Girardi et al.,
1996; Preciozzi et al., 1999; Bossi et al., 2001). This
younger igneous activity is probably linked to the
Brasiliano orogeny (Dom Feliciano belt) that
affected the eastern region of the Uruguayan
Shield (Basei et al., 2000, for review).The RLPC continues to the south under the
Pampas (Chaco-Parana basin) sedimentary rocks
down to the Martin Garcia island and further to
the isolated ranges of Bayas, Azul, Balcarce, Alta
de Vela, Del Tigre and Tandil in Argentina (Figs. 1
and 2) where the basement rocks are collectively
known as the Buenos Aires complex (Marchese
and Di Paola, 1975; Cingolani and Dalla Salda,2000). This complex consists of gneisses, schists
and migmatites intruded by tonalitic�/granitic and
leuco-monzogranitic plutons, which make up a
WNW-ESE igneous-metamorphic belt*/the Tan-
dilia system (Dalla Salda et al., 1988, 1992).
The oldest tonalitic�/granitic plutonic suite of
the Tandilia system (based on Rb�/Sr isochron
ages between 2150 and 1970 Ma) occurs mainlyalong an east�/west shear belt in the northern part
of the complex, and is interpreted to reflect the
syn-collisional phase of the Trans-Amazonian
orogeny (Halpern and Linares, 1970; Ramos et
al., 1990; Dalla Salda et al., 1992; Dalla Salda,
1999; Cingolani et al., 2001). New SHRIMP U�/Pb
ages (2228�/2051 Ma) which are also comparable
with a Sm/Nd whole-rock isochron of 21409/80Ma on the same plutonic rocks, confirm that the
magmatic crystallization took place in the Paleo-
proterozoic. However, crustal-signature Nd model
ages are in the 2.7�/2.4 Ga range (Cingolani et al.,
2001; Pankhurst et al., 2001). Younger leucocratic
monzogranites (Rb�/Sr isochron age of 17709/88
Ma; Varela et al., 1988) occur in the Tigre and
Alta de Vela Ranges, together with acid metavol-canic rocks; their emplacement was associated
with wrench faults striking NNE-SSW (Dalla
Salda, 1981; Ramos et al., 1990). Transcurrent
tectonics have led to the appearance of several
wide W�/E shear zones in Tandilia (Fig. 2) that
produced cataclastic phenomena including mylo-
nitic fabrics in both the oldest plutonic suite and
monzogranites. The record of multiple deforma-tion events and intrusive magmatism in the
Tandilia system suggest that the Trans-Amazonian
orogeny involved continent�/continent collision
(tonalitic�/granitic plutons) as well as postcolli-
sional events including generation of leuco-mon-
zogranites and activity of strike-slip faults. The
geologic scenario is consistent with a plutonic arc
setting in late Paleoproterozoic times, which wasfollowed by crustal recycling within the southern-
most part of the RLPC (Dalla Salda, 1981; Dalla
Salda et al., 1992).
The tonalitic�/granitic suite yields initial87Sr/86Sr ratios between 0.702 and 0.706, suggest-
ing that Trans-Amazonian mantle-derived magma
was important in its genesis (Varela et al., 1988). In
contrast, the monzogranitic suite yields a highinitial 87Sr/86Sr value (0.7181), indicating it had an
anatectic origin (Varela et al., 1988; Dalla Salda et
al., 1988, 1992). The Montecristo leucogranite has
a contrasting origin, as supported by its TDM of
2.2 Ga (Cingolani et al., 2002). The above Sr and
Nd data suggest that, although the major period of
juvenile crust production was Paleoproterozoic,
late Archean crustal components have been im-portant during the history of the Tandilia rocks.
The Tandilia system contains two swarms of
unmetamorphosed Paleoproterozoic mafic dykes.
Most of the studied dykes occur in the vicinity of
Tandil (e.g. Del Tigre, Tandil, Alta da Vela ranges;
Fig. 2), but another swarm of dykes crops out in
the northwest part of study area, near Azul (Fig.
W. Teixeira et al. / Precambrian Research 119 (2002) 329�/353332
Fig. 2. Geologic sketch of the Tandilia system (after Dalla Salda et al., 1992). Keys: Tandilia dykes (1); Buenos Aires complex
(Paleoproterozoic): granitoids (2), migmatites, gneisses and schists (3), S-type leucomonzogranites (4); shear zones (5); faults (6). (a)
shows the main occurrences of dykes in Azul region.
W. Teixeira et al. / Precambrian Research 119 (2002) 329�/353 333
2a). Previous K�/Ar ages for these dykes vary
from 1750 to 1070 Ma (Teruggi et al., 1974a,b;
Cortelezzi and Rabassa, 1976), suggesting that
variable Ar losses have affected the mineral
systems.
Field relations indicate that the relatively oldest
dykes exhibit dominantly E�/W trends, and are
related to the transational stage of the Trans-
Amazonian orogeny (Teruggi et al., 1973, 1974a).
The relatively youngest dykes have dominantly
NW trends and crosscut both the 1.77 Ga leuco-
monzogranites and the regional E�/W shear zones
(Dalla Salda, 1981; Teruggi et al., 1988; Dalla
Salda et al., 1988). Their emplacement is asso-
ciated with late extensional stress, following cra-
tonization of the Tandilia system (Fig. 2). Detailed
mapping of a thick N30W dyke in the Del Tigre
Range (Fernandez et al., 2001) reveals that,
locally, the late extensional stress may follow
pre-existing weakness planes of the E�/W shear
zone, so a few branches of coeval dykes trend
similarly E�/W (not shown in Fig. 2).
The Tandilia basement rocks have K�/Ar whole-
rock ages between 980 and 790 Ma (Linares,
1977), suggesting the influence of low-grade ther-
mal overprints related to the Neoproterozoic Dom
Feliciano belt that flanks the RLPC (see above).
The La Tinta Group*/a 400 m thick sedimentary
marine sequence*/partly overlies the Tandilia
system (Rapela et al., 1974; Dalla Salda and
Iniguez, 1979; Cingolani and Bonhomme, 1982).87Sr/86Sr measurements in La Tinta argillites show
that diagenesis took place between 7349/48 and
7259/36 Ma (Kawashita et al., 1999), in agreement
with a Rb�/Sr isochron age of 7239/19 Ma for
shales of the middle La Tinta Group (Bonhomme
and Cingolani, 1980; Dalla Salda et al., 1988).
However, a Rb�/Sr isochron age of 7699/23 Ma
was reported for pelites of the lower La Tinta
Group (Bonhomme and Cingolani, 1980). The
isotopic signatures and the stratigraphy of the La
Tinta Group support its correlation with the lower
Nama Group in South Africa, thereby suggesting
that a continuous sedimentary basin covered the
South America/Africa boundary during the Neo-
proterozoic (Dalla Salda et al., 1988; Kawashita et
al., 1999).
3. Petrography and geochemistry of the Tandiliadykes
In general, the Tandilia dykes are very fresh,
although minor alteration may be locally present.
Petrography and whole-rock geochemistry (Iacu-
min, 1998; Iacumin et al., 2001) allow distinction
of four types dykes in Tandilia, as summarized
below (Table 1): (1) basic dykes with subophiticand sometimes intergranular textures (designated
here as B1 type*/63% of the dykes); (2) basic
dykes with ophitic texture (B2*/12% of the dykes);
(3) intermediate dykes with porphyritic to inter-
granular texture (I*/10%) and (4) acid dykes with
porphyritic texture (A*/15%). The acid and inter-
mediate dykes may have a cataclastic fabric.
The (B1) dykes, which occur in the Azul andTandil ranges, are fine-grained at the borders and
coarse-grained in the center. They characteristi-
cally have labradoritic plagioclase, somewhat
altered to clay, and pyroxene (augite and minor
pigeonite) which may be locally replaced by
hornblende, tremolite, and chlorite. In general,
olivine is scarce and exclusive to low-Ca pyroxene-
free dykes. Accessory minerals include magnetite,ilmenite, quartz, apatite, and epidote. The scarce
(B2) dykes crop out in the Tandileiufu Hill and
Alta da Vela, Del Tigre and Tandil Ranges. They
are medium- to fine-grained, in contrast to the (B1)
dykes. Their mineralogy also differs from that of
the (B1) dykes, as they contain Ti-augite and have
no olivine. The labradoritic plagioclase in the (B2)
dykes is somewhat altered to clay and sericite, andis locally albitized. The clinopyroxene is locally
replaced by hornblende, actinolite�/tremolite and
chlorite. Accessory minerals are ilmenite, magne-
tite, and apatite.
The (I) dykes, which are exposed in the Tandi-
leiufu Hill and Del Tigre and Tandil ranges,
exhibit medium-fine grained texture. They have
phenocrysts of andesine-plagioclase and augite,both locally altered to clay minerals and amphi-
bole, respectively. The groundmass is made up of
plagioclase, epidote, biotite, opaques, alkali-feld-
spar, and quartz. Where the fabric is intergranular
the plagioclase and augite are partly altered to clay
and amphibole. Granophyric quartz�/feldspar in-
tergrowths are common. The (A) dykes are
W. Teixeira et al. / Precambrian Research 119 (2002) 329�/353334
Table 1
Main petrographic and geochemical characteristics of the Tandilia dykes
Tandilia dykes
Suite Tholeiitic Calc-alkaline
Type B1 B2 I A
Occurrence Azul and Tandil Tandil Tandil, Tigre, Albion and Tandileufu Tanges Tandil, Tigre, Albion and
Tandileufu ranges
Thickness (m) 10�/50 0.5�/10 0.5�/10 0.5�/30
Strike (domi-
nant trend)
NW-SE NW-SE E�/W E�/W
Petrography Subophitic and intergranular tex-
tures. Labradorite, augite or pigeo-
nite and olivine
Ophitic texture. Labradorite, au-
gite (high TiO2) and pigeonite
Porphyritic to intergranular textures. Labra-
dorite to andesine, salitic�/augitic pyroxenes
and Qz-Kf intergrowths
Porphyritic texture. Oligo-
clase, alkali-feldspar and
augite
Geochemistry Low TiO2 (0.87�/1.66), low contents
of IE. REE patterns similar to E-
MORB, with mean (La/Yb)N of
1.559/0.48
High TiO2 (1.71�/3.74 wt.%), high
contents of P2O5, Zr, Nb and other
IE. REE pattern: high (La/Yb)N of
6.72
Lower mean contents of TiO2 and higher P2O5,
Sr, REE and Zr, relative to B1. REE patterns:
higher (La/Yb)N mean values (10.939/0.64),
differing from the B1 and B2 types. Negative
spikes of Nb
SiO2�/65�/75 wt.%. High-
est contents of IE and very
high (La/Yb)N values (15�/
40)
Data from this paper and Iacumin et al. (2001). See text for details.
W.
Teix
eiraet
al.
/P
recam
bria
nR
esearch
11
9(
20
02
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29�
/35
33
35
parallel with and sometimes intruded by (I) dykes.
They contain phenocrysts of oligoclase�/plagio-
clase, alkali-feldspar, and augite, which also con-
stitute the groundmass. Secondary zeolites or
quartz and K-feldspars may fill vesicles or frac-
tures.
The (B1) dykes correspond to tholeiitic basalts
and subordinately to tholeiitic andesitic basalts
and latibasalts (Iacumin, 1998). The (B2) dykes
vary from tholeiitic andesitic basalts to latibasalts
and trachybasalts (Fig. 3). The (I) dykes plot in the
andesitic basalt and subordinately andesite fields,
while the (A) dykes fall in the rhyolite field. In an
AFM diagram (Fig. 4), (B1) and (B2) dykes plot in
the tholeiitic field whereas both (I) and (A) dykes
plot in the calc-alkaline field.
Averages of major, minor and trace elements (54
samples), including REE, reveal genetic differences
between the tholeiitic and calc-alkaline dykes (Fig.
5; Tables 2 and 3), as illustrated by the (I) dykes
that have higher SiO2, K2O, Na2O, Ba and Rb
than the tholeiites. The latter dykes have otherwise
higher mean contents of TiO2, FeOt, CaO and Ni
(Table 2). It is noteworthy that the tholeiitic dykes
with TiO2 higher than 1.7 wt.% (B2 type) are more
enriched, for a given MgO content, in P2O5, FeOt,
K2O, Ba, Sr, La, Ce, Nd, Zr, Y and Nb relative to
those with TiO2 B/1.7 wt.% (B1 type).
The (I, A) dykes are characterized by REE
patterns with (La/Lu)N much higher (I�/12�/10,
A�/14�/40) than those of the tholeiitic dykes
(B1�/1.3�/2.8, B2�/6.63; see average values in
Table 3). The genetic differences between the
calc-alkaline and tholeiitic dykes are also sup-
Fig. 3. R1 versus R2 diagram (de la Roche et al., 1980, modified
by Bellieni et al. (1981)) for the Tandilia dykes. B1 and B2,
basic, tholeiitic types. (I), intermediate dykes; (A), acid dykes (I
and A, calc-alkaline types. R1�/[4Si�/11(Na�/K)�/2(Fe�/Ti)]
and R2�/[6Ca�/2Mg�/Al].
Fig. 4. AFM diagram for the Tandilia dykes (A�/Na2O�/
K2O; F�/FeO; M�/MgO). Calc-alkaline-tholeiitic boundary
(solid curve) as proposed by Irvine and Baragar (1971);
tholeiitic field (dashed curve) after Macdonald and Katsura
(1964). Symbols and legend as in Fig. 3.
Fig. 5. Diagrams of REE abundance patterns normalized to
chondrite (after Boynton, 1984) for selected Tandilia dykes.
Symbols and legend as in Fig. 3.
W. Teixeira et al. / Precambrian Research 119 (2002) 329�/353336
ported by the significant negative Eu anomaly of
the (A) dykes, as well as the characteristic flat REE
pattern of the (B1) dykes (Fig. 5). The calc-alkaline
dykes are more enriched in LREE [(La/Sm)N
ranging from 3.1 to 6.3] relative to the (B1) types
(B1�/0.9�/1.9). The B2 (high-Ti) dykes also have
an enriched LREE pattern, but in conjunction
with the B1 (low-Ti) are generally more enriched in
HREE than the calc-alkaline dykes (Fig. 5; Table
3).
Calc-alkaline dykes have incompatible elements
(IE) contents and calculated 87Sr/86Sr initial values
(Sr0) typically lower than or similar to those of the
Tandilia tonalitic�/granitic suite (see previous sec-
tion and Table 6). Thus, crustal contamination is
not easy to detect. These dykes are characterized
by oNd values similar to those of an enriched
mantle component. Tholeiitic dykes with low-Ti
(B1 type) and high-Ti (B2) contents display sig-
nificant Sr0 variations up to 0.711 (Table 6), but
the Sr0 increases are not correlated with SiO2,
MgO, K2O Rb, Ba, La, Zr and Nd. This feature,
coupled with mass balance calculations, led Iacu-
min et al. (2001) to exclude appreciable crustal
contamination for (B1) and (B2) dykes having Sr0
values lower than 0.705. In addition, the Sr0 values
higher than 0.707 do not even conform to AFC
mixing contamination curves, thereby suggesting
that processes like low-grade alteration in some of
the studied dykes (see above) may have locally
contributed towards reaching these highest Sr0
values. Mass balance calculations, coupled with
chemical characteristics and differences in discri-
mination variation diagrams (Zr�/Ni and La�/
Table 2
Average major (wt.%) and trace (ppm) element contents for the Tandilia dykes
B1 B2 I A
N�/34 S.D. N�/7 S.D. N�/5 S.D. N�/8 S.D.
SiO2 50.66 0.05 49.06 0.85 57.51 1.82 73.19 3.16
TiO2 1.34 0.13 2.01 0.32 0.69 0.17 0.20 0.14
Al2O3 13.67 0.95 14.16 0.19 14.55 0.51 13.59 0.57
FeOt 12.57 0.95 14.80 0.43 8.79 0.50 2.54 1.34
MnO 0.22 0.01 0.22 0 0.17 0.01 0.06 0.03
MgO 7.53 0.09 6.36 0.56 5.80 1.62 0.54 1.09
CaO 11.22 0.49 9.01 0.22 7.51 1 1.62 0.94
Na2O 2.17 0.23 2.49 0.17 2.88 0.69 4.08 0.54
K2O 0.49 0.22 0.97 0.05 1.83 0.44 4.11 0.68
P2O5 0.12 0.03 0.85 0.15 0.28 0.11 0.05 0.06
LOI 2.92 0.83 2.71 0.62 2.62 0.72 1.62 1.24
Mg# 54.81 2.18 46.43 1.93 56.27 6.94 16.90 18.11
Cr 168 4. 105 24 103 67 12 24
Ni 100 0.7 87 12 17 4 3 4
Rb 22 11 46 4 88 48 149 31
Ba 78 69 482 56 529 166 1140 207
Sr 197 11 412 28 523 131 263 129
Nb 3 0.7 15 1.3 8 2.2 11 1.4
Zr 78 27 192 27 113 27 212 35
Y 18 5 24 0.50 21 6 26 6
La 4 0.7 30 1.6 23 8 54 7
Ce 10 4 67 9 53 14 100 12
Nd 8 2 40 4 27 9 45 6
See Iacumin et al. (2001) for details. Major elements recalculated to 100% on volatile-free basis. N , number of samples; S.D.,
standard deviations (1s). Symbols and legend as in Fig. 3. Major and trace elements were determined by X-ray fluorescence, at
University of Trieste (Italy), using a PW 1404 XRF spectrometer, following the procedures of Philips (1994) for the correction of
matrix effects. The accuracy of the results are within 2�/3% for major and minor elements and better than 7�/10% for trace elements.
Loss on ignition (LOI) was determined at 1100 8C (12 h) and corrected for FeO oxydation.
W. Teixeira et al. / Precambrian Research 119 (2002) 329�/353 337
Ni) all support the idea that (B1) and (B2) dykesmust be related to distinct parental magmas. The
available oNd data (Table 7) reflect that (B1) dykes
may have been derived from a depleted source
mantle, whereas the (B2) dykes were derived from
an enriched mantle source (Iacumin et al., 2001,
for details).
In summary, chemical and isotopic data indicate
that calc-alkaline (I, A) dykes, low-Ti (B1) andhigh-Ti (B2) tholeiitic dykes of Tandilia derived
from heterogeneous source mantle. The variable
metasomatic enrichment may have occurred in
Late Archean to Early Paleoproterozoic times,
based on Sm�/Nd geochemistry (Iacumin et al.,
2001, for details).
4. Dating techniques
40Ar�/39Ar analyses (Table 4; see Iacumin, 1998)
were performed on biotite from two baked wall
rocks directly adjacent to the contact with (A) and
(I) calc-alkaline dykes, respectively. A plagioclase
from a tholeiitic (B1) dyke was also analysed. The
minerals were irradiated for 100 h in the Triga
reactor at Oregon State University, along with
Fish Canyon sanidine (FCs�/28.02 Ma; Renne et
al., 1998), a neutron fluence monitor. The fluence
parameter ‘J ’ was determined from individual
analysis of 15 sanidine grains in each of two
positions bracketing the unknown samples. The
separates were step-heated using furnace heating.
Ar isotopic compositions were measured at the
Berkeley Geochronology Center (USA) in static
mode by a MAP-215-50 spectrometer, using the
procedures described by Renne (1995).
Isotopic run data were corrected for mass
discrimination, radioactive decay and nucleogenic
interferences. Atmosphere-corrected data are
plotted as apparent-age spectra, which are accom-
panied by compositional Ca/K data derived from
corrected relative abundances of 37Ar and 39Ar for
Table 3
Average compositions of REE (ppm) and La/YbN, La/LuN, La/SmN, Gd/YbN and Eu/Eu� ratios normalized by chondrite (Boynton,
1984) for the Tandilia dykes
B1 B2 I A
N�/7 S.D. N�/1 N�/2 S.D. N�/4 S.D.
La 4.36 1.53 43.66 25.17 0.81 52.12 9.23
Ce 10.89 2.75 87.12 55.65 0.84 102.04 16.01
Pr 1.55 0.34 9.82 6.48 0.04 10.51 1.55
Nd 7.92 1.53 44.49 26.92 0.77 37.98 5.47
Sm 2.51 0.41 9.87 4.88 0.02 6.09 0.63
Eu 0.89 0.13 3.55 1.28 0.19 1.15 0.04
Gd 3.01 0.49 10.45 3.78 0.06 4.37 0.79
Tb 0.46 0.07 1.41 0.50 0.02 0.58 0.12
Dy 3.12 0.54 7.73 3.01 0.12 3.18 0.91
Ho 0.72 0.13 1.66 0.65 0.01 0.61 0.17
Er 1.86 0.34 3.95 1.56 0.04 1.53 0.37
Tm 0.27 0.05 0.61 0.23 0.01 0.23 0.06
Yb 1.90 0.30 4.38 1.55 0.04 1.60 0.47
Lu 0.28 0.04 0.68 0.24 0.01 0.25 0.08
(La/Yb)N 1.55 0.48 6.72 10.93 0.64 22.00 11.39
(La/Lu)N 1.61 0.54 6.63 10.60 0.76 21.78 11.65
(La/Sm)N 1.10 0.35 2.78 3.24 0.09 5.38 0.83
(Gd/Yb)N 1.28 0.06 1.93 1.97 0.03 2.21 0.38
Eu/Eu� 0.98 0.06 1.06 0.91 0.14 0.68 0.07
See Iacumin et al. (2001) for details. N , number of samples; S.D., standard deviations (1s). Symbols and legend as in Fig. 3. Rare
earth elements*/REE have been determined by the inductively coupled plasma atomic emission spectrometry (ICP-AES), at the
‘Centre de Recherches Petrographiques et Geochimiques’, CNRS, France Govindaraju and Mevelle (1987).
W. Teixeira et al. / Precambrian Research 119 (2002) 329�/353338
Table 440Ar�/
39Ar (selected steps) analytical data of tholeiitic dyke A4 (plagioclase) and baked country rocks (A54 biotite; A48 biotite) at the very contact with calc-alkaline dykes
(data from Iacumin, 1998)
T (8C) 40Ar (mol) 40/39 38/39 37/39 36/39 40�/39 %40 Age (Ma) 9/s (Ma)
Tholeiitic dyke A4 (plagioclase)
600 6.16E�/15 819.42 0.91785 5699.1 3.36600 �/83.6 34.2 1.00E�/20 4135.7
650 4.27E�/15 782.15 0.94617 3453.1 2.65834 �/166.48 34.9 1.00E�/20 4077.9
700 6.00E�/15 450.99 0.42421 855.50 1.12779 537.39 41.3 4882.2 1372.0
750 6.47E�/15 130.24 0.11633 187.91 0.34243 51.47 33.8 1532.4 37.5
800 6.27E�/15 43.00 4.60E�/02 90.02 0.10188 21.58 46.7 803.5 11.8
850 5.05E�/15 36.64 4.45E�/02 86.94 7.86E�/02 21.83 55.6 811.0 11.1
900 4.32E�/15 40.00 2.34E�/02 89.14 9.34E�/02 20.94 48.8 784.2 25.2
950 2.75E�/15 49.38 4.90E�/02 123.80 0.135672 21.19 38.9 791.9 103.8
1000 3.64E�/15 69.91 3.89E�/02 120.95 0.188898 26.18 34.0 936.8 63.9
1050 5.38E�/15 111.23 8.11E�/02 131.89 0.331039 26.64 21.5 949.6 55.7
1100 2.79E�/15 62.71 2.07E�/02 158.72 0.173709 27.39 38.4 970.2 45.3
1150 2.91E�/15 66.62 0.047534 135.19 0.132860 42.56 57.3 1344.3 22.3
1200 3.83E�/15 79.75 0.055627 139.15 0.187276 39.77 44.6 1280.9 40.1
1250 4.00E�/15 57.54 4.84E�/02 141.61 9.58E�/02 45.49 70.5 1408.2 27.7
1350 4.00E�/15 52.25 7.82E�/02 104.22 4.31E�/02 51.99 91.6 1542.9 14.1
1600 1.42E�/15 211.26 0.360343 93.52 0.466592 87.13 38.3 2134.9 31.7
A54 (biotite)*/baked country rock
600 4.74E�/14 682.76 0.427544 0 2.139767 50.46 7.4 1512.1 628.2
640 1.40E�/13 336.19 0.206281 0 1.032772 31.01 9.2 1066.7 131.1
680 2.38E�/13 72.22 4.16E�/02 4.59E�/02 0.144400 29.55 40.9 1028.6 10.8
710 6.07E�/13 72.54 2.03E�/02 9.96E�/02 3.68E�/02 61.68 85.0 1726.4 4.1
740 1.55E�/12 82.64 1.58E�/02 4.80E�/02 1.40E�/02 78.52 95.0 2006.9 6.8
770 2.74E�/12 79.47 1.38E�/02 6.70E�/02 3.86E�/03 78.34 98.6 2004.1 3.5
760 8.29E�/13 79.36 1.39E�/02 0.214999 3.26E�/03 78.43 98.8 2005.4 3.1
770 7.56E�/13 79.50 1.36E�/02 0.148473 2.62E�/03 78.74 99.0 2010.3 3.1
780 6.66E�/13 79.20 1.35E�/02 0.125110 1.81E�/03 78.68 99.3 2009.4 3.7
790 5.81E�/13 78.92 1.38E�/02 0.217852 1.67E�/03 78.45 99.4 2005.8 4.6
800 4.87E�/13 78.84 1.37E�/02 0 1.75E�/03 78.33 99.3 2003.8 5.2
820 4.63E�/13 79.21 1.36E�/02 0.203633 1.97E�/03 78.66 99.3 2008.9 4.6
840 3.65E�/13 79.10 1.39E�/02 0.150645 2.39E�/03 78.41 99.1 2005.2 5.2
860 3.38E�/13 78.79 1.39E�/02 0 2.61E�/03 78.02 99.0 1999.1 5.5
880 4.38E�/13 79.27 1.35E�/02 0.179101 2.54E�/03 78.55 99.1 2007.2 3.3
900 6.38E�/13 80.05 1.37E�/02 0.203168 2.40E�/03 79.37 99.1 2019.8 4.9
920 6.60E�/13 80.07 1.41E�/02 0.130750 2.02E�/03 79.50 99.3 2021.8 9.4
940 5.64E�/13 79.67 1.36E�/02 0.314538 2.37E�/03 79.02 99.2 2014.5 4.7
960 5.21E�/13 79.77 1.42E�/02 0.134934 2.32E�/03 79.10 99.2 2015.8 3.4
990 5.84E�/13 79.81 1.36E�/02 0.140124 2.67E�/03 79.04 99.0 2014.8 3.2
1020 3.95E�/13 80.09 1.40E�/02 0.261024 3.18E�/03 79.19 98.9 2017.15 4.5
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Table 4 (Continued )
T (8C) 40Ar (mol) 40/39 38/39 37/39 36/39 40�/39 %40 Age (Ma) 9/s (Ma)
1060 1.41E�/13 80.00 1.45E�/02 1.388759 4.95E�/03 78.73 98.3 2010.1 6.9
1100 6.36E�/14 81.54 1.75E�/02 6.938283 1.65E�/02 77.62 94.7 1992.9 11.7
1150 7.75E�/14 80.40 1.49E�/02 2.475953 5.32E�/02 79.18 98.3 2017.0 9.1
1270 3.25E�/14 87.45 1.80E�/02 2.361412 2.22E�/02 81.23 92.7 2048.1 20.0
1350 1.62E�/15 69.24 0.058738 124.1467 0.178192 29.29 38.3 1021.5 1356.4
1500 4.32E�/15 128.24 4.18E�/02 18.89543 0.408957 9.02 6.9 380.4 1119.1
A48 (biotite)*/baked country rock
600 9.04E�/14 352.89 0.184 3.9683 0.880437 93.32 26.4 2221.8 78.9
630 7.74E�/14 154.62 7.61E�/02 2.7505 0.319461 60.57 39.1 1706.3 33.7
660 5.89E�/14 74.69 3.03E�/02 1.3800 8.19E�/02 50.64 67.7 1515.8 15.5
690 2.57E�/13 65.73 0.018107 0.334615 2.53E�/02 58.29 88.7 1664.4 4.9
720 1.49E�/12 82.77 1.53E�/02 0.113612 1.31E�/02 78.91 95.3 2012.8 4.4
750 3.64E�/12 80.43 1.34E�/02 0.113765 4.20E�/03 79.21 98.5 2017.4 3.3
780 4.39E�/12 79.94 1.30E�/02 9.12E�/02 1.76E�/03 79.43 99.4 2020.8 3.4
810 3.14E�/12 79.96 1.30E�/02 0.158878 1.31E�/03 79.59 99.5 2023.3 3.0
850 1.64E�/12 80.05 1.27E�/02 0.184319 1.66E�/03 79.59 99.4 2023.2 6.2
890 2.53E�/12 79.86 0.012897 0.179104 1.65E�/03 79.39 99.4 2020.3 3.1
930 2.92E�/12 79.91 1.27E�/02 0.124480 1.42E�/03 79.50 99.5 2021.9 3.8
970 1.56E�/12 79.79 1.30E�/02 0.185273 1.67E�/03 79.33 99.4 2019.2 4.1
1010 1.62E�/12 79.76 1.31E�/02 0.231745 0.001688 79.30 99.4 2018.7 4.3
1050 1.99E�/12 81.79 1.31E�/02 0.382454 1.54E�/03 81.39 99.5 2050.6 3.0
1100 8.10E�/13 84.54 0.013439 0.952865 2.83E�/03 83.84 99.1 2087.0 3.9
1150 1.69E�/13 85.66 1.36E�/02 1.212999 9.22E�/03 83.11 96.9 2076.3 5.9
1220 1.06E�/13 86.32 1.59E�/02 1.037633 1.34E�/02 82.51 95.5 2067.4 8.5
1300 3.26E�/15 101.85 0.071091 54.7559 0.349681 3.02 2.8 136.7 889.9
1500 5.54E�/15 195.06 9.77E�/02 89.1162 0.648261 11.39 5.4 468.1 1340.6
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each step. Errors are reported at 2s level and donot include uncertainty in the age of FCs or 40K
decay constants (Min et al., 2000). The decay
constants recommended by Steiger and Jager
(1977) were used.
U�/Pb analyses for tholeiitic (B1) dyke A-17
were performed at the University of Alberta
Radiogenic Isotope Facility, Canada (Table 5). A
small number (B/50) of very small (B/30 mm in thelongest dimension) baddeleyite grains were recov-
ered from this sample. The two baddeleyite
analyses represent small multi-grain fractions (12
and 18 grains, respectively) of irregular tan to dark
brown fragments and parts of blades. The frac-
tions were initially dissolved with HF/HNO3 (10:1)
in teflon pressure vessels together with a mixed205Pb�/
235U tracer solution. This material was laterconverted to chloride form by evaporating to
dryness and re-dissolving in 3.1N HCl. U and Pb
were purified by standard anion exchange chro-
matography using micro-columns modified after
Krogh (1973) and closely following the procedure
outlined in Heaman and Machado (1992). The
total procedural blanks during the period of study
were less than 5 pg Pb and 0.5 pg U, respectively.The purified U and Pb were loaded together using
a silica gel-phosphoric acid mixture (Cameron et
al., 1969) onto zone-refined Re ribbon. All ana-
lyses were performed on a VG-354 mass spectro-
meter operated in single Faraday or Daly
(analogue) collector peak-hopping mode. All ana-
lyses were corrected for mass discrimination (Pb,
0.088% per a.m.u.; U, 0.155% per a.m.u.) based onreplicate measurements of the NBS-981 and U500
standards. In addition, all measurements obtained
with the Daly photomultiplier detector were ad-
justed for detector bias (Pb, 0.13% a.m.u.; U,
0.15% a.m.u.). The isotopic composition of com-
mon Pb in excess of analytical blank was calcu-
lated using the two-stage model of Stacey and
Kramers (1975). Discordia line calculation wasperformed using ISOPLOT (Ludwig, 1992) with
the 238U (1.55125�/10�10 a�1) and 235U
(9.8485�/10�10 a�1) decay constants recom-
mended by Jaffey et al. (1971). All errors reported
in Table 5 are quoted at 1s and were calculated by
numerical propagation of all known sources of
uncertainty. The error ellipses shown on the
concordia diagram and age uncertainties arereported at 2s.
Twenty-two Rb�/Sr whole-rock analyses (Table
6) were performed, using isotope dilution techni-
que, at the Geochronological Research Center
(CPGeo) of University of Sao Paulo, Brazil. The87Sr/86Sr ratios are listed with absolute errors (2s),
and have been corrected to the mean value of the
NBS-987 standard (0.7102549/0.000022 (2s)). Theoverall blank for the chemical procedure was 4 ng
for Sr. Isotope ratios were measured on VG-354
multicollector and single collector mass spectro-
meters, and the 87Sr/86Sr ratios were normalized to86Sr/88Sr�/0.1194. Isochron calculation followed
the procedure of Ludwig (1999), and the decay and
other constants used are from Steiger and Jager
(1977).Ten Sm�/Nd whole-rock analyses (Table 7) were
carried out at the CPGeo, using the two-column
technique, as described by Richard et al. (1976)
with modifications described by Sato et al. (1995).
The first ion-exchange resin was used for primary
separation of the REE, followed by the second
HDEHP-coated Teflon-powder column, for se-
paration of Sm and Nd elements. The laboratoryblanks for the chemical procedure during the
period of analyses yielded maximum values of
0.4 ng for Nd and 0.7 ng for Sm. The measured143Nd/144Nd ratio obtained for the La Jolla
standard was 0.5118579/0.000046 (2s).
5. Results and discussion
The emplacement age of the calc-alkaline dykes
was defined from the 40Ar�/39Ar analyses (Table 4)
of outgassed biotites from baked granitic rocks
sampled at a maximum distance of 10 cm from the
contact with the dykes. The biotite collected at the
contact with the A54 dyke (I type; Del Tigre
Range) was degassed, yielding a concordant spec-
trum with an integrated age of 19749/24 Ma and aplateau age of 20079/24 Ma (11 steps; Fig. 6a).
The biotite from the other granitic rock at sharp
contact with A48 dyke (A type; Tandileufu Hill)
yielded a comparable age spectrum with an
integrated age of 20199/24 Ma and a plateau age
of 20209/24 Ma (9 steps; Fig. 6b). The relatively
W. Teixeira et al. / Precambrian Research 119 (2002) 329�/353 341
Table 5
U�/Pb baddeleyite results for A17 B1 tholeiitic dyke from Tandilia (RLPC)
Description� Weight
(mg)
U
(ppm)
Th
(ppm)
Pb
(ppm)
Th/
U
TCPb
(pg)
206Pb/204Pb 206Pb/238U 207Pb/235U 207Pb/206Pb 206Pb/238Pb 207Pb/235U 207Pb/206Pb %
Disc
Model ages (Ma)
A17 1 dark brown
108 Nm (12)
3 362.0 74.0 99.0 0.21 16 1122 0.2641�/5 3.525�/9 0.09681�/
¯
12
1510.8�/
¯2 1532.9�/
¯2 1563.5�/
¯2 3.8
2 tan 158 M (18) 4.0 91.4 7.5 25.8 0.08 9 613 0.2709�/
¯6 3.639�/
¯12 0.09741�/
¯
23
1545.8�/
¯2 1558.2�/
¯2 1575.1�/
¯4 2.1
Notes : 108 Nm refers to a non-magnetic fraction at a side tilt of 108 on a Frantz Isodynamic Separator. Number in parentheses refers to the total number of grains
analysed. Th concentration calculated from the amount of 208Pb and model 207Pb/206Pb age. All uncertainties reported at 1s.
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small and statistically insignificant difference (13
Ma) between the plateau ages of the biotites
suggests a moderate to rapid cooling after calc-
alkaline dyke emplacement (Baldwin et al., 1990),
or implies preferential Ar loss from the biotite
during a possible subsequent reheating. Following
the first interpretation the crystallization age is
taken as 20209/24 Ma.A plagioclase concentrate from tholeiitic dyke
A4 (B1 type; Azul Range) was also degassed,
yielding a plateau age of 8119/36 Ma (6 steps;
Fig. 6c; Table 4) which does not represent the
Table 6
Rb�/Sr (isotope dilution) analytical data and [87Sr/86Sr] initial ratios (Sr�/IR0) for the Tandilia dykes
Lab. no/sample Type Rb (ppm) Sr (ppm) 87Rb/86Sr 1s 87Sr/86Sr 2s oSr Sr�/IR0
13169/A-1 B1 40.89 166.93 0.7100 0.0099 0.72416 0.00010 �/75(1.6 Ga) 0.70787
13170/A-2 B1 16.50 149.62 0.3193 0.0044 0.71025 0.00008 �/4.2(1.6 Ga) 0.70292
13171/A-8 B1 16.70 157.18 0.3077 0.0043 0.71314 0.00012 �/49(1.6 Ga) 0.70608
13172/A-33 B1 29.79 195.91 0.4404 0.0061 0.71508 0.00009 �/33(1.6 Ga) 0.70497
13173/A-35 B1 42.09 171.38 0.7121 0.0107 0.72639 0.00010 �/106(1.6 Ga) 0.71006
13174/MT65 B1 29.71 192.44 0.4472 0.0063 0.71540 0.00007 �/36(1.6 Ga) 0.70513
13749/A-4 B1 16.85 166.20 0.2937 0.0027 0.71370 0.00007 �/62(1.6 Ga) 0.70696
13750/A-5 B1 5.74 134.16 0.1239 0.0011 0.70717 0.00009 �/24(1.6 Ga) 0.70433
13191/MT68 B2 38.68 370.56 0.3024 0.0042 0.71785 0.00008 �/118(1.6 Ga) 0.71091
13192/MT70 B2 33.21 393.17 0.2447 0.0041 0.71425 0.00017 �/86(1.6 Ga) 0.70863
13756/A-39 B2 37.53 453.13 0.2398 0.0026 0.71218 0.00009 �/58(1.6 Ga) 0.70667
13762/A53 B2 29.84 330.84 0.2611 0.0024 0.70895 0.00009 �/4.7(1.6 Ga) 0.70295
13751/MT67 B2 39.26 404.26 0.2813 0.0023 0.71705 0.00009 �/113(1.6 Ga) 0.71059
13752/MT69 B2 45.87 360.57 0.3684 0.0031 0.71228 0.00009 �/17(1.6 Ga) 0.70382
13175/A-40 I 42.00 577.84 0.2104 0.0035 0.70987 0.00007 �/24(2.0 Ga) 0.70381
13758/A-49 I 51.96 577.19 0.2606 0.0022 0.71125 0.00008 �/23(2.0 Ga) 0.70375
13761/A-52 I 43.76 507.00 0.2499 0.0021 0.71046 0.00009 �/16(2.0 Ga) 0.70327
13787/A-54 I 147.76 378.90 1.1319 0.0097 0.73667 0.00008 �/29(2.0 Ga) 0.70416
13759/A-45 A 129.55 186.57 2.0195 0.0167 0.75789 0.00009 �/30(2.0 Ga) 0.70001
13788/A-47 A 142.52 142.55 2.9161 0.0271 0.78779 0.00008 �/33(2.0 Ga) 0.70446
13789/BR-1 A 194.15 313.57 1.7998 0.0149 0.75290 0.00009 �/12(2.0 Ga) 0.70129
13786/BR-2 A 117.50 251.61 1.3572 0.0112 0.74389 0.00009 �/40(2.0 Ga) 0.70497
B1 and B2, Tholeiitic dykes; I and A, Calc-alkaline dykes. See text for explanation.
Table 7
Sm�/Nd whole rock analytical data of selected Tandilia dykes
Lab. no/sample Type Sm (ppm) Nd (ppm) 147Sm/144Nd 1s 143Nd/144Nd 2s TDM (Ga) fSm/Nd oNdt
1046/A-4 B1 1.90 7.64 0.1505 0.0005 0.512778 0.000039 �/ �/0.23 �/12.2 (1.6 Ga)
1047/A-5 B1 2.28 6.93 0.1991 0.0007 0.512893 0.000041 �/ �/0.01 �/4.5 (1.6 Ga)
1048/A-16 B1 2.57 9.63 0.1614 0.0005 0.512250 0.000020 �/ �/0.18 �/0.4 (1.6 Ga)
1049/A-38 B2 10.43 48.00 0.1314 0.0004 0.511895 0.000020 �/ �/0.33 �/1.2 (1.6 Ga)
1060/MT-70 B2 7.29 38.94 0.1131 0.0004 0.511394 0.000037 2.51 �/0.42 �/7.2 (1.6 Ga)
1050/A-41 I 4.93 26.68 0.1116 0.0004 0.511323 0.000040 2.59 �/0.43 �/3.9 (2.0 Ga)
1058/A-40 I 4.67 25.06 0.1126 0.0004 0.511375 0.000038 2.53 �/0.42 �/3.2 (2.0 Ga)
1061/A-54 I 5.18 26.70 0.1173 0.0004 0.511392 0.000010 2.63 �/0.40 �/4.0 (2.0 Ga)
1051/A-51 A 7.06 40.71 0.1049 0.0003 0.511190 0.000010 2.61 �/0.47 �/4.8 (2.0 Ga)
1059/A-48 A 4.26 22.53 0.1143 0.0004 0.511372 0.000040 2.58 �/0.42 �/3.7 (2.0 Ga)
Model TDM ages were calculated using DePaolo (1981) model parameters: a�/0.25; b�/�/3; c�/8.5 and 146Nd/144Nd�/0.7219 to
normalize the isotopic ratios [143Nd/144Nd�/Nd(Chur)0�/0.512638 and 147Sm/144Nd (Chur)0�/0.1967]. The oNd values were calculated
using the simplified equation oNd (T )�/oNd(0)�/QNdfSm/NdT , with the (Chur)0 values above and QNd�/25.09. See text for explanation.
W. Teixeira et al. / Precambrian Research 119 (2002) 329�/353 343
crystallization age. The discordant age spectrum at
high temperature degassing (�/1150 8C) is accom-
panied by elevated Ca/K, which could reflect the
presence of cryptic secondary phases within this
concentrate. Additionally, the age spectrum shows
a ‘saddle-shaped’ pattern which is, in many cases,
evidence for samples containing excess 40Ar from
older, K-rich host rocks (Lanphere and Dalrymple,
1976). However, considering the typical low Ar
blocking temperature of plagioclase (�/176 8C;
Berger and York, 1981), the age spectrum may also
be related to episodic 40Ar loss at 810 Ma. In a
similar matter, two K�/Ar whole-rock apparent
ages of 8039/14 and 11939/18 Ma reported for (B2)
dykes (A38 and A39; Iacumin, 1998) reflect
variable Ar loss from the mineral systems.
Fig. 6. 40Ar�/39Ar spectra for the plagioclase of tholeiitic dyke and biotite from baked country rocks in sharp contact with calc-alkaline
dykes; Tandilia system: (a) and (b) baked country rocks; (c) tholeiitic dyke. Keys: biotite (bt), plagioclase (plg). See text for
explanation.
W. Teixeira et al. / Precambrian Research 119 (2002) 329�/353344
The tholeiitic (B1) dyke A17 intruded at 15889/
11 Ma (Fig. 7; Table 5), according to a discordia
upper intercept age (two baddeleyite analyses).
This is probably an estimate of crystallization age
for all the tholeiitic dykes of Tandilia, as they have
similar N30W trends oblique to the shear zones
(e.g. Del Tigre Range; see Fig. 2), and crosscutting
relations with the 1.77 Ga leuco-monzogranites
(see previous section).Rb�/Sr whole-rock determinations (Table 6)
were carried out on eight calc-alkaline (four
samples each of I and A types) and 14 tholeiitic
dykes (eight B1 and six B2 types) in an attempt to
estimate the age of crystallization of each swarm.
The calc-alkaline dykes yielded an errorchron of
19569/110 Ma (1s) and Sr0�/0.70389/0.0025
(Fig. 8). The MSWD value (19) reflects the data
scatter around the best line, as expected from
samples collected in a large area and by the
possibility that the intermediate and acid dykes
may have variable Sr0 ratios. Thus, the initial ratio
of the errorchron is a rough estimate of the average
Sr0 of the calc-alkaline magma. The individual
samples have Sr0 for t0�/2.0 Ga (40Ar/39Ar age)
ranging from 0.70129 to 0.70497 (Table 6). This
limited range suggests that Rb and Sr have not
been further reset at the whole-rock scale since the
dyke’s emplacement and is not compatible with the
possibility of appreciable crustal contamination, in
agreement with petrological and geochemical in-
ferences reported by Iacumin et al. (2001). The (I)
dykes have calculated Sr0 values between 0.70327
and 0.70416 (average 0.703759/0.00037), slightly
higher than the (A) dykes (0.70129�/0.70497), but
not significantly different within the errors (A
dykes have mean Sr0 values�/0.702689/0.00241).
In any case the Sr0 mean ratios are comparable
within the errors with those of the tonalitic�/
granitic plutons of Tandilia (with Sr0 as low as
0.7020), thereby reinforcing the idea that crustal
contamination, if present, was negligible for the
calc-alkaline dykes (see previous section).
(B1) and (B2) dykes did not yield an Rb�/Sr
isochron, as shown by the large data scatter in the
diagram (Fig. 9). This situation probably results
from low-grade hydrothermal fluids that may have
contributed towards increasing the Sr0 values
higher than 0.705 (Table 6, see previous section).
Fig. 7. U�/Pb concordia diagram for A-17 tholeiitic dyke.
W. Teixeira et al. / Precambrian Research 119 (2002) 329�/353 345
It should be noted that not all of the studied dykes
contain secondary minerals (e.g. clay, sericite and
albite overprinting the plagioclase) although they
occur in a same area; this indicates that mobility of
Rb and Sr can be considered to be a local-scale
phenomenum, but linked with the late-magmatic
crystallization process of the tholeiitic dykes.
Ten Sm�/Nd whole-rock analyses were per-
formed on five calc-alkaline (I, A) and five
tholeiitic (B1 and B2) dykes. The oNd and oSr
parameters (samples A40 and A54), recalculated
for t0�/2.0 Ga (40Ar/39Ar age for the emplace-
ment; see above), vary from �/4.8 to �/3.2 and �/
24 to �/29, respectively (Table 7). These data plot
Fig. 8. Rb�/Sr whole-rock errorchron for the calc-alkaline dykes. Symbols as in Fig. 3.
Fig. 9. Rb�/Sr correlation diagram for the tholeiitic dykes. Symbols as in Fig. 3.
W. Teixeira et al. / Precambrian Research 119 (2002) 329�/353346
in the enriched quadrant with respect to bulkEarth (Iacumin et al., 2001), and suggest that the
calc-alkaline dykes may be derived from partial
melting of a mantle source with low Sm/Nd,
similar to those of an enriched source mantle
(Iacumin et al., 2001). The calc-alkaline dykes
display TDM from 2.53 to 2.63 Ga (Table 7),
indicating that such an enrichment of the source
mantle may have occurred in late Archean�/
Paleoproterozoic times.
Three tholeiitic (B1) dykes (A4; A5; A16) do not
allow calculation of single-stage Nd model ages, as
indicated by fSm/Nd values of �/0.23, �/0.18 and �/
0.01, respectively (Table 7). Sample A4 yields
anomalous high oNd(1.6 Ga) (�/12.2) and Sr0 values
(0.70696; Table 6), which probably reflect altera-
tion (see previous section). Samples A5 and A16have oNd(1.6 Ga) values of �/4.5 (Sr0�/0.70433) and
�/0.4, respectively. These results are interpreted to
reflect derivation from a depleted mantle source
which may have assimilated small amounts of
crustal components, as supported by the petrolo-
gical and geochemical characteristics of the low-Ti
tholeiites (see Iacumin et al., 2001, for details). In
contrast, (B2) dykes (A38 and MT70) have oNd(1.6
Ga) values of �/1.2 and �/7.2 (Sr0�/0.70863),
respectively Tables 6 and 7. The latter sample is
affected by late-magmatic alteration (see above),
whereas the Nd signature of A38 dyke can be
related to an enriched mantle source, in agreement
with the distinctive geochemistry of the high-Ti
tholeiites of Tandilia (Iacumin et al., 2001). In
addition, dyke MT70 yields TDM of 2.51 Ga that isotherwise comparable with TDM of the calc-alka-
line dykes (Table 7). Therefore, these two distinct
dyke suites may have originated by variable
enrichment of a late Archean�/early Paleoproter-
ozoic mantle source.
6. Summary and tectonic implications
Two distinct generations of Proterozoic dykes
crosscut the crystalline crust of the Tandilia
system. The 40Ar�/39Ar mineral plateau ages
indicate that the calc-alkaline dykes (I and A)
were emplaced between 2020 and 2007 Ma. The
tholeiitic (B1 and B2) dykes intruded at �/1590
Ma. Therefore, the previous published K�/Ar ageson the Tandilia dykes (1750�/1540 and 1070�/800
Ma) reflect variable Ar loss from the minerals of
these dykes.
The oldest calc-alkaline dykes have E�/W trends
and post-date Trans-Amazonian deformation and
metamorphism. These dykes were intruded essen-
tially subcoevally with the Tandilia tonalitic�/
granitic plutonism (Dalla Salda et al., 1988). Thisplutonic suite was formed during the Trans-
Amazonian orogeny, as supported by U�/Pb and
Rb�/Sr age determinations, and have major and
trace elements and Sr0 (0.7020�/0.7060) that re-
semble those of rocks generated in modern arc
environments (Dalla Salda et al., 1988). The calc-
alkaline dykes are therefore interpreted as trans-
tensional representatives of the Tandilia plutonicarc. This interpretation is also consistent with
geochemical characteristics of the calc-alkaline
dykes (I and A types), given the enriched mantle
source signature influenced by subduction-related
metasomatism (Iacumin et al., 2001). The geologic
scenario of Tandilia system fits with tectonic
interpretations of the Trans-Amazonian orogeny
in the Central Brazil Shield, in which this eventplayed an important role in mantle-differentiation
and crustal shortening processes, surrounding late
Archean domains (Cordani and Sato, 1999; Teix-
eira et al., 1999). In western Gondwanaland, these
late Paleoproterozoic stable remnants, including
the RLCP (Fig. 1) are consistent with the existence
of the Atlantica supercontinent at �/2.0 Ga
(Rogers, 1996).The youngest (B1) and (B2) tholeiitic dykes of
Tandilia have dominantly NW-SE trend and
crosscut both the E�/W mylonitic zones and the
1770 Ma leuco-monzogranites. This situation in-
dicates a significant change of the regional stress
field, post-dating the Trans-Amazonian orogeny.
The emplacement of these dykes at �/1.59 Ga
implies that extensional tectonics accompanied byanorogenic igneous activity predominated after
stabilization of the Trans-Amazonian orogeny,
within the RLPC. This assessment is also sup-
ported by the occurrence of the 1.73 Ga Florida
tholeiitic dyke swarm (western Uruguayan Shield)
and the coeval lllescas rapakivi granite (17489/4
Ma) in the Nico Perez terrane (Teixeira et al.,
W. Teixeira et al. / Precambrian Research 119 (2002) 329�/353 347
1999). The crustally-derived leuco-monzogranites(17709/88 Ma) in Tandilia may also be related to a
continental rift scenario. It is worth noting that
such an intraplate setting characterizes the Stater-
ian period (1.8�/1.6 Ga) in South America, during
which diachronous mafic dykes, anorogenic
AMCG rapakivi suites (anorthosites, mangerites,
charnockites, acid volcanic rocks) and fault block-
basins developed across many Paleoproterozoiccrustal provinces (Brito Neves et al., 1995; Teixeira
et al., 1999).
The 1.59 Ga tholeiitic (B1 and B2) dykes of
Tandilia have geochemical and Nd signatures,
which are consistent with the presence of two
compositionally different magmas (Iacumin et al.,
2001). Also we speculate that such a situation may
be explained by rift dynamics during late Paleo-proterozoic times, since this regime could favour
interaction of the ascending asthenosphere with
variable amounts of the thinned subcontinental
lithosphere.
6.1. Correlations with the southern African
subcontinent
Geologic correlation between South Americaand southern Africa (Porada, 1979; Brito Neves
and Cordani, 1991), considering the Brasiliano/
Pan-African orogenies, allows prior tectonic link
with implications for the Paleoproterozoic evolu-
tion of the RLPC. In this regard, the geologic
framework of the Tandilia system shows many
similarities with the contemporary Eburnean crust
of the Richtersveld and Bushmanland subpro-vinces, within the 1.2�/1.0 Ga Namaqualand
(Hartnady et al., 1985; Colliston and Schoch,
1998), facing the RLPC in the West Gondwana
reconstruction (Figs. 1 and 10). In a global
context, the intercontinental scenario is consistent
with that of many late Mesoproterozoic orogenies
worldwide, representing the amalgamation of the
Rodinia supercontinent (Rogers, 1996), in re-sponse to diachronic rifting and dispersal of
descendants from ‘Atlantica’.
The Richtersveld subprovince, like the Tandilia
system, consists mainly of metamorphic equiva-
lents of igneous rocks (Barton and Burger, 1983).
A calc-alkaline volcanic pile (Orange River
Group) overlies the co-magmatic Vioolsdrif I-type suite that comprises separate intrusive phases
of gabbro, tonalite and granodiorite, dated at
19009/30 Ma (Reid, 1979, 1982). These granitoid
and volcanic rocks display TDM between 2.29 and
2.12 Ga (see Reid, 1997 for review). In addition,
late-tectonic granitoids (quartz monzonite, ada-
mellite, leucogranite) of the Vioolsdrif suite were
emplaced at 17309/20 Ma (Rb�/Sr isochron age;Reid, 1982) yielding Sr and Pb initial isotopic
signatures consistent with derivation from young,
unradiogenic crust similar in bulk composition to
the relatively older (Eburnean) tonalites and
granodiorites (Reid, 1997). It should be noted
that Orange River rhyodacites (see above) have
chondrite normalized REE abundance patterns
(ratios (La/Yb)N�/14.0; (La/Sm)N�/5.0; (Gd/Yb)N�/1.5; (Eu/Eu�)N�/0.6; Reid, 1997) that are
broadly comparable with those of the contempor-
ary calc-alkaline (A) dykes of Tandilia (ratios (La/
Yb)N�/22.0; (La/Sm)N�/5.4; (Gd/Yb)N�/2.2;
(Eu/Eu�)N�/0.7; Table 3).
The current preferred model for the Richters-
veld association involves the evolution of an
island-arc complex of Eburnean age and its latemobilization at depth along an active continental
margin (Hartnady et al., 1985). The available Nd,
Sr and Pb features of the rock suites are consistent
with the subduction process to produce metaso-
matism of a mantle wedge with an undifferentiated
bulk Earth signature, as well as with rapid
recycling of young crust to produce the granitic
components within the arc complex (Reid andBarton, 1983; Reid, 1979, 1997). Thus, the above
scenario resembles that envisaged for subcoeval
rocks of the Tandilia system.
Much of the Bushmanland subprovince (Fig. 10)
to the south of the Richtersveld Subprovince was
similarly formed and metamorphosed during the
late Paleoproterozoic, though severely obscured by
the Namaqua deformation and metamorphism at1.2�/1.0 Ga. In the Okiep terrane (Central Bush-
manland), the Koeris tholeiitic metabasalts (am-
phibolites) form a major volcanic horizon,
penecontemporaneous with the upper part of the
Bushmanland Group composed of quartzite, mar-
ble, schists, and gneiss with minor volcanic inter-
calations. These amphibolites are similar in age to
W. Teixeira et al. / Precambrian Research 119 (2002) 329�/353348
the Tandilia tholeiites, as supported by an Sm�/Nd
whole-rock isochron age of 16499/90 Ma (oNd(t)�/
�/0.48), interpreted as the time of eruption of the
basalt precursors (Reid et al., 1987). Additional
Rb�/Sr and U�/Th�/Pb work on the Koeris amphi-
bolites (Reid, 1997) has confirmed the important
role of the late Mesoproterozoic metamorphism
(Kibaran orogeny; Fig. 10).
Fig. 10. Crustal architecture of southern African subcontinent (a), showing the Paleoproterozoic Richtersveld and Bushmanland
subprovinces of Namaqualand (b) (adapted from Hartnady et al. (1985), Reid et al. (1987), Goodwin (1991)). Keys: intracratonic
sequences of Bushmanland (BS), Waterberg (WA) and Soutpansberg (SB). See text for details.
W. Teixeira et al. / Precambrian Research 119 (2002) 329�/353 349
The Koeris amphibolites have trace element
geochemistry, including REE, consistent with the
existence of mantle heterogeneity, subduction
related metasomatism and crustal contamination
(Reid, 1997). The geochemical inference suggests a
back arc continental extension environment for
these mafic rocks, but it is worth noting that the
geochemical and isotopic signatures may also be
related to rift dynamics, as already proposed for
the origin of the Tandilia tholeiites. It should also
be noted that the Koeris amphibolites show near
flat REE patterns with low (La/Lu)N and high Ti/
Zr ratios (Reid et al., 1987), which compare closely
with those patterns shown by (B1) tholeiitic dykes
of Tandilia (Table 8). In a similar matter, the
Aggeneys/Witberg metabasalt types exhibit low Ti/
Zr ratios, more fractionated REE patterns with
LREE enrichment, negative Eu anomalies and
high (La/Lu)N ratio (Reid, 1997) which may be
compared with the characteristics of the (B2)
tholeiitic dykes, except for the Eu anomaly.
Salient geologic features of the Bushmanland
Subprovince include charnockitic granites, meta-
mafic rocks (gabbro, diorite, norite, anorthosite),
as well as characteristic metavolcanic-sedimentary
assemblages (e.g. Bushmanland Group) filling
intracratonic basins, probably accumulated be-
tween 1.7 and 1.6 Ga (Hartnady et al., 1985).
These intracratonic packages host several giant
stratiform CU�/Pb�/Zn�/Ag ore deposits (Reid et
al., 1987; Colliston and Schoch, 1998). Such a
tectonic framework again has similarities with
typical rock associations of the Statherian period
(Goodwin, 1991). In consequence, a major sig-
nificance for unrecognized intraplate 1.7�/1.6
events within Bushmanland subprovince can be
proposed, suggested also by occurrence of the
Koeris tholeiitic volcanism and the Vioolsdrif late-
tectonic granites (see above). Moreover, such a
scenario opens the possibility of a tectonic rela-
tionship with subcoeval leucogranitoid rocks of
the RLPC (see previous section). Also, we suspect
that a family of tectonically controlled �/1.75�/
1.70 Ga block-faulting basins (e.g. Waterberg�/
Soutpansberg groups) roughly distributed in a
NE-SW zone located within the Kaapvaal craton
(Fig. 10), as well as occurrences of poorly-studied
mafic dykes at the vicinities (Hartnady et al.,
1985), may similarly be relicts of Statherian
extensional tectonics in the southern African
subcontinent.
To conclude, correlation between the RLPC and
the southwest corner of Africa by comparing the
stratigraphy of pre-tectonic platform sedimentary
marine deposits of the La Tinta and the Nama
Group was established long ago (Porada, 1979;
Dalla Salda, 1982). From the geochronologic and
geochemical inferences now available for the
Tandilia system and the Richtersveld arc complex
there is also evidence for a Late Paleoproterozoic
(Trans-Amazonian/Eburnean) link, as already
proposed by Dalla Salda et al. (1988), and further
by some peculiar Paleo-Mesoproterozoic geologic
features of the Bushmanland subprovince.
Finally, the establishment of such an integrated
scenario may contribute to the debate on the
reconstruction of the Rodinia supercontinent and
its descendants (e.g. Atlantica supercontinent; see
Table 8
Average of La/Lu, La/Yb, La/Sm and Eu/Eu� ratios normalized by chondrite (Boynton, 1984) for amphibolites (Koeris tholeiitic
metabasalts) from the Bushmanland Subprovince, South Africa (Reid et al., 1987) and B1 and B2 tholeiitic dykes of the Tandilia
System (RLPC)
Ratios Central Bushmanland Subprovince (Southern Africa) Rio de la Plata Craton/Tandilia System (South America)
Gamsberg (N�/7) Aggeneys/Witberg (N�/4) B1 tholeiitic (N�/7) B2 tholeiitic (N�/1)
(La/Lu)N 1.649/0.27 4.899/0.15 1.619/0.54 6.83
(La/Yb)N 1.639/0.28 4.959/0.26 1.559/0.48 6.72
(La/Sm)N 1.279/0.19 2.539/0.05 1.109/0.35 2.78
(Eu/Eu�)N 0.999/0.06 0.769/0.04 0.989/0.06 1.06
Data from Reid et al. (1987), Iacumin et al. (2001). N , number of samples, standard deviations, 1s. Symbols and legend as in Fig. 3.
See text for explanation.
W. Teixeira et al. / Precambrian Research 119 (2002) 329�/353350
Rogers, 1996). Moreover, because the Bushman-land subprovince is unusually rich in base metal
sulphide deposits, metallogenetic intercontinental
correlations among comparable Paleoproterozoic
rock units are also relevant, as it opens new
possibilities of mineral exploration models and
potentials in the South American counterpart.
Acknowledgements
The authors thank the financial support of the
Brazilian Agencies FAPESP (grant no. 97/0640-5)
and CNPq (grant no. 522975/96-8), and CNR and
MURST (Italian Agencies). We also acknowledge
the technical staffs of the CPGeo (USP) and
Berkeley Geochronology Center (USA) for pro-vinding the Rb�/Sr and Sm�/Nd, and 40Ar�/
39Ar
dates. We are also greatfull to A. Marzoli, A. De
Min and L. Furlan (Dipartimento di Scienze della
Terra, Trieste, Italy) for their valuable collabora-
tion in this research. Special thanks are due to R.
Ernst (Geological Survey of Canada), C. Cingola-
ni (University of la Plata, Argentina) and U.
Cordani (USP, Brazil) for their fruitful suggestionsrelated to the manuscript, and to the constructive
reviewers’ comments and criticism.
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