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Earth and Planetary Science Le
Terrane transfer during the Grenville orogeny: tracing the
Amazonian ancestry of southern Appalachian
basement through Pb and Nd isotopes
E. Tohvera,*, J.S. Bettencourta, R. Tosdalb, K. Mezgerc, W.B. Leited, B.L. Payollae
aInstituto de Geociencias, Universidade de Sao Paulo, Rua do Lago, 562, Cidade Universitaria, CEP 05508-900, Sao Paulo, SP BrazilbMineral Deposit Research Unit, University of British Columbia, 6339 Stores Road, Vancouver, BC V6T 1Z4, Canada
cInstitut fur Mineralogie, Universitat Munster, Corrensstrasse. 24 48149, Munster GermanydInstituto de Geociencias e Ciencias Exatas, Universidade Estadual Paulista, Av. 24 A, no. 1515, CEP 13506-900, Rio Claro, Brazil
eCentrais Eletricas do Norte do Brasil S/A, SQN 408, Bloco L, Apto 202, CEP 70856-120, Brasilia, Brazil
Received 14 April 2004; received in revised form 7 September 2004; accepted 20 September 2004
Editor: K. Farley
Abstract
Whole rock Pb isotope data can be used to determine the provenance of different blocks within the Rodinia
supercontinent, providing a test for paleogeographic reconstructions. Calculated isotopic values for the source region of the
Grenville-deformed SW Amazon craton (Rondonia, Brazil), anchored by published U–Pb zircon ages, are compared to those
from the Grenville belt of North America and bGrenvillianQ basement inliers in the southern Appalachians. Both the SW
Amazon craton and the allochthonous Blue Ridge/Mars Hill terrane are defined by a similar Pb isotopic signature, indicating
derivation from an ancient source region with an elevated U/Pb ratio. In contrast, the Grenville Province of Laurentia
(extending from Labrador to the Llano Uplift of Texas) is characterized by a source region with a distinctly lower, time-
integrated U/Pb ratio. Published U–Pb zircon ages (ca. 1.8 Ga) and Nd model ages (1.4–2.2 Ga) for the Blue Ridge/Mars
Hill terrane also suggest an ancient provenance very different from the rest of the adjacent Grenville belt, which is dominated
by juvenile 1.3–1.5 Ga rocks. The presence of mature continental material in rocks older than 1.15 Ga in the Blue Ridge/
Mars Hill terrane is consistent with characteristics of basement rocks from the SW Amazon craton. High-grade
metamorphism of the Blue Ridge/Mars Hill basement resulted in purging of U, consistent with observations of the rest
of the North American Grenville province. In contrast, the bGrenvillianQ metamorphic history of the Amazon appears to have
been much more heterogeneous, with both U enrichment and U depletion recorded locally. We propose that the Blue Ridge/
Mars Hill portion of the Appalachian basement is of Amazonian provenance and was transferred to Laurentia during
Grenvillian orogenesis after ~1.15 Ga. The presence of these Amazonian rocks in southeastern Laurentia records the
0012-821X/$ - s
doi:10.1016/j.ep
* Correspon
E-mail addr
tters 228 (2004) 161–176
ee front matter D 2004 Elsevier B.V. All rights reserved.
sl.2004.09.029
ding author.
ess: [email protected] (E. Tohver).
E. Tohver et al. / Earth and Planetary Science Letters 228 (2004) 161–176162
northward passage of the Amazon craton along the Laurentian margin, following the original collision with southernmost
Laurentia at ca. 1.2 Ga.
D 2004 Elsevier B.V. All rights reserved.
Keywords: Rodinia; Grenville orogeny; Amazon craton; Blue Ridge; exotic terrane; Pb isotopes; Mesoproterozoic paleogeography
1. Introduction
Paleogeographic reconstructions rely on a variety
of techniques and criteria that, taken individually,
might be considered nonunique in determining the
paleogeographic position of a given continent or
block relative to another. The well-studied example of
the Paleozoic transfer of the Argentine Precordillera
terrane from Laurentia to the shores of western
Gondwana is illustrative [1]. The overlapping views
of the Preocordillera’s origin and final resting place
reconstructed from faunal [2], geochemical [3],
paleomagnetic [4], and stratigraphic (e.g., [5,6]) data
present a more complete picture of Paleozoic paleo-
geography. Likewise, the transfer of an Amazonian
terrane to SE Laurentia proposed in this contribution
serves as a marker for the evolving paleogeography of
Rodinia in late Mesoproterozoic times.
The usefulness of radioisotope geochemistry lies in
its ability to delineate coherent large-scale isotopic
patterns, which suggests the potential of bfingerprintsQfor paleogeographic reconstructions. Such techniques
have been used to recognize crustal boundaries [7–10],
distinct terranes [11–13], and tectonic and sedimentary
provenance [14,15] as well as for accretionary models
of continental growth [16–18]. The contribution of
Fig. 1. (top inset) Outline of North America emphasizing the location o
Laurentian craton. (bottom inset) Position of the Amazon craton (AC) with
white. The dark grey area is the outline of the state of Rondonia with the A
craton (PC), accreted at ~1.1 Ga [37]. (main) Schematic illustration of pale
late Mesoproterozoic times are shown in light silhouette, from top to bottom
constrained position of the Amazon at 1.2 Ga, interpreted as indicating co
configuration at the time of the transfer of the Blue Ridge/Mars Hills terrane
sinistral displacement of ~2.5 cm/yr offset between Laurentia and the Ama
Laurentia (Labrador [83]; Quebec [17]; reworked portions of Superior crat
Green Mountains [16]; the midcontinental region east of the Grenville Fro
[8]), Grenvillian basement inliers in the Appalachian [78,79,81,84], and t
Appalachians (from Bartholomew [66]) separates Paleozoic accreted terran
the time of Rodinia breakup. Dashed line separating southeastern midcon
Abbreviations for Grenvillian basement occurrences, shown in black out
Adirondack Mountains; GMM—Green Mountian Massif; BR–MH—Blue
LU—Llano Uplift; Van Horn Mountains; FM—Franklin Mountains; HBU
geochronology to the recognition of the amalgamation
of Rodinia has been fundamental; geochronological
studies led the way to deciphering the effects of the
Grenville orogeny in eastern Laurentia and identifying
its worldwide equivalents. Geochronology of closed
systems (e.g., minerals or whole rocks) is based on
calculating the time necessary for a measured amount
of a daughter isotope to accumulate from a known
amount of parent isotope after a differentiation event
such as crystallization. However, of potentially greater
interest for paleogeography and provenance studies are
the original isotopic characteristics of a given craton or
terrane imparted by the source region at the time of
crustal formation. These initial ratios are distinctive,
being the product of coupled evolution between long-
lived isotopic heterogeneities in the mantle and its
associated crust [19,20]. The advantage of the U–Pb
system for such studies is that the paired U-decay
schemes, 238U–206Pb and 235U–207Pb, with their
significantly different decay constants, allow con-
straints to be placed on the timing of processes that
modified the U/Pb ratio.
The many proposed versions of the Amazonia–
Laurentia connection in Rodinia provide a good
starting point for isotopic-based reconstructions of
Rodinia. Evidence for the Amazonia–Laurentia con-
f the Grenville province (dark grey) on the eastern margin of the
in South America with major geochronological provinces outlined in
mazon river basin shown in white; dashed black line shows Paragua
ogeographic positions previously proposed for the Amazon craton in
: [21,23,24,26]. The southernmost position is the paleomagnetically
llision with the southern Laurentia. Dark silhouette is the proposed
to the North American craton (ca. 1.15 Ga). This model requires net
zon craton after the initial collision. Numbers are Nd model ages for
on [18,56]; Central Metasedimentary Belt [58,59]; Adirondacks and
nt (toothed line) [60]; the Llano region and occurrences in W. Texas
he Amazon craton [30,32,35,64,65]. The bold grey line through the
es from ancestral North America at the end of the Proterozoic, i.e., at
tinental region with TDMb1.55 Ga is from Van Schmus et al. [60].
line, are as follows: CMB—Central Metasedimentary Belt; AM—
Ridge/Mars Hill terrane; EGR—Eastern Granite–Rhyolite province;
—Honeybrook Uplands.
E. Tohver et al. / Earth and Planetary Science Letters 228 (2004) 161–176 163
nection has been found in the form of matching
metamorphic belts of ca. 1.0 Ga, Grenvillian age [21],
similar postrift thermal histories [22,23], linking the
igneous ages of basement provinces [24,25], and
paleomagnetic evidence [26–28]. Conflicting inter-
pretations have led to the Amazon craton being
correlated to almost every portion of the 3000-km
expanse of the Grenville belt of North America (Fig.
1). Although differences in the stated age of these
reconstructions may explain many discrepancies,
more data from the Amazon craton itself are essential
for resolving the issue. Recently, 1.2-Ga paleomag-
netic data from the Amazon craton [26] have been
used to support a collision between the Amazon
craton and southernmost Laurentia (Llano region,
Texas), with a younger pole suggesting a mid-
E. Tohver et al. / Earth and Planetary Science Letters 228 (2004) 161–176164
Laurentian position for Amazonia by ca. 1.1 Ga
[27,28]. Geochronological and structural data from
the Grenville-aged belts of the SW Amazon provide
support for long-lived, sinistral strike-slip motion
required by this paleomagnetic-based model [29].
In this paper, we use new whole rock Pb and
published Sm–Nd data from the SW Amazon craton
to decipher an isotopic fingerprint of Amazon source
region characteristics. Comparison of this source
region with the signature from the Grenville Prov-
ince of eastern Laurentia demonstrates the distinc-
tiveness of the two cratons by the end of the
assembly of Rodinia at 1.0 Ga. A paleogeographic
marker for the Amazon craton’s position with respect
to Laurentia is provided by the presence of
Amazonian crust in basement rocks of the south-
eastern Appalachians. We propose that the transfer of
the Blue Ridge/Mars Hills terrane to the margin of
southeastern Laurentia took place at ca. 1.15 Ga
during accumulated strike-slip motion of the Amazon
craton along the Grenville margin of Laurentia,
following the initial collision of the Amazon craton
with southern Laurentia at ca. 1.2 Ga [26].
2. Regional geology—SW Amazon Craton
The Amazon craton is composed of NW–SE
trending domains of chiefly Paleoproterozoic age
(Fig. 1), recognized on the basis of Sm–Nd and U–
Pb ages. Although the boundaries between these
basement domains are diffuse, a general trend of
younging to the SW is observed [30–32]. The SW
margin of the Amazon craton, best exposed in the
western Brazilian state of Rondonia [33], is marked
by multiple intrusive episodes during the Mesoproter-
ozoic, with especially voluminous magmas emplaced
at ca. 1.57–1.53 and 1.41–1.31 Ga [34]. The
metamorphic effects of the latter episode are partic-
ularly widespread, as revealed by both U–Pb and40Ar–39Ar dating of metamorphic monazite, titanite,
and hornblende [29,35]. Magmatic products of the
Grenville interval (1.2–1.0 Ga) are less common, but
the postorogenic period is marked by the shallow
level intrusion of the tin-bearing Younger Granites of
Rondonia at ca. 950 Ma [34].
It is the Grenville-deformed SW margin of the
Amazon craton that is most commonly correlated with
Laurentia via a Grenville collision [21,24,26]. In fact,
the effects of this collision are complex, with at least
two late Mesoproterozoic deformation events
observed: an older 1.20–1.12 Ga event recorded in
the basement rocks of the Paleo- to Mesoproterozoic
basement rocks interpreted as recording the Amazo-
nia–Laurentia collision [29], followed by a younger
1.10–0.95 Ga event exclusively recorded in two
metasedimentary belts, the Nova Brasilandia [36,37]
and Aguapeı–Sunsas belts [38–41]. The former
records sinistral transpressive deformation during the
accretion of the Paragua craton, a Paleoproterozoic
block of subcontinental dimensions, to the Amazon
craton in late Mesoproterozoic times, an event
accompanied by amphibolite to granulite facies meta-
morphism and the emplacement of a synkinematic
granite suite at 1.11 Ga [36,37,42]. The Sunsas belt
marks the western boundary of the Paragua block and
is marked by synkinematic granite emplacement at ca.
1.05 Ga along major strike-slip mylonitic shear zones
with sinistral offsets [38]. The Aguapeı belt appears to
record a minor episode of low-grade intracratonic
deformation towards the end of the Grenville interval
at ca. 950 Ma [40,41].
3. Pb isotope data
Fifty-six whole rock samples were collected from a
region covering ~70,000 km2 of the Amazon craton
basement in Rondonia, Brazil. The rocks were
collected from the cratonic region north of the Nova
Brasilandia metasedimentary belt, with samples taken
from both the metaigneous host rock lithologies (see
[35] for sample locations) and from all the intrusive
suites of the six known episodes of Meso-Neoproter-
ozoic magmatism (see [34] for sample localities). U–
Pb zircon ages from the former range of 1.75–1.43 Ga
[35,43]. The intrusive suites range in age from ca.
1.65 to 0.97 Ga [34].
Whole rock U, Th, and Pb data are included in the
electronic Appendix A [46]. Whole rock dissolution
in closed Savillex vials, column chromatography, and
mass spectrometer analysis were carried out in the
laboratories of the U.S. Geological Survey in Menlo
Park, California, as described by Bouse et al. [44]. A
wide range of 206Pb/204Pb values (16.8–33.4) and207Pb/204Pb values (15.5–16.9) characterize the Ama-
E. Tohver et al. / Earth and Planetary Science Letters 228 (2004) 161–176 165
zon craton samples [45]. The 208Pb/204Pb ratios vary
from 36.3 to 54.5, demonstrating time-integrated Th/
U ratios of 3.8 to 6 (Fig. 2a), similar to that observed
by Sinha et al. for the Blue Ridge of the southern
Appalachians [47]. Both the SW Amazon craton and
the Blue Ridge/Mars Hill terrane are marked by
higher thorogenic Pb values than present-day values
of ~3.6 measured from the nearby Honeybrook
Uplands [48] as well as average values for the rest
of the Grenville belt. We will concentrate on the
uranogenic Pb component, simply noting that both
our techniques and conclusions are valid for and
consistent with observations of thorogenic Pb.
The 207Pb/204Pb values for the SWAmazon craton
rocks are clearly elevated for a given range of206Pb/204Pb values, relative to both the Pb evolution
model of average crust and to Laurentian samples
(Fig. 2b). Inasmuch as 207Pb is generated by the decay
of the short-lived 235U, pronounced differences in
present day 207Pb/204Pb must reflect ancient differ-
entiation events; the more recent the differentiation,
the smaller the eventual difference in 207Pb/204Pb
values, given the increasing scarcity of parent 235U.
The coherence of high 207Pb/204Pb values in all
samples, regardless of age, suggests a common
high-l (238U/204Pb) source region (l2 in the two-
stage model of Stacey and Kramers for a differentiated
mantle [49]). In uranogenic Pb space, samples plot
along an apparent secondary isochron with a slope of
0.0875, corresponding to an apparent age of 1372F59
Ma, depicted as a reference line in Fig. 2b. The
present-day whole rock values and their projection
along this reference line indicate an initial Pb initial
ratio well above the Stacey and Kramers [49] second
stage Pb evolution curve for average crust (l2=9.735).
However, in order to be geologically significant as a
secondary isochron, this line must reflect the time
elapsed since the last major U/Pb fractionation. Two
observations suggest that this is not the case: first,
many of the rocks have magmatic ages that are
younger than the age indicated by the slope of the
reference line; and second, 207Pb/206Pb whole rock
isochrons calculated for contemporaneous rock suites
are similar to the U–Pb zircon ages from those rocks.
Hence, we attach no age significance to the line itself,
which is interpreted as the average of an array of
secondary isochrons formed by individual samples,
useful only as a regional indicator of high l2 values.
3.1. Determination of l2 for SW Amazon source
region and l3 for samples
Modern day Pb compositions are tricky to use as
isotopic discriminants, given the many processes
that redistribute Pb within a bulk sample. More
useful would be some measure of the initial Pb
within a sample, which is characteristic of the
source region at the time of the rock’s extraction
from the reservoir and is unaffected by later events
(e.g., metamorphism) that can profoundly alter the
evolution of whole rock Pb isotope compositions to
their modern values. Determinations of the isotopic
composition of initial Pb have been attempted by
two methods: analysis of U- and Th-free minerals
with a supposedly immutable Pb composition (e.g.,
K-feldspar [7,10]) or by correcting for radiogenic Pb
accumulation from the measured amount of U and
Th present in a whole rocks sample over a known
span of time [50]. Unfortunately, for the first
technique, feldspars are not closed to Pb diffusion
during metamorphism, meaning that initial Pb
values at the time of crystallization are not
preserved [10]. The success of the second technique
is foiled by remobilization of soluble U during
weathering [50]. For example, our own attempts to
determine the initial Pb by correcting for radiogenic
Pb using the observed U content and the known
zircon age proved problematic; several samples plot
below the Canyon El Diablo composition for
primordial Pb [51]. This clear overcorrection for in
situ accumulation of radiogenic Pb is probably the
result of recently acquired U, a subject we will
return to later.
We explore a third technique for determining the
initial Pb of a whole rock sample that considers
each sample as a closed system following extraction
from a source reservoir. The projection from a
whole rock–zircon isochron intersects an array of Pb
evolution curves, each of which represents the time-
dependent Pb composition of source region of a
given l2 value (Fig. 3). The best fit l2 value,
solved for iteratively, yields an intercept of the
isochron with the Pb evolution curve at an age
(Tintercept) that is ideally equal to the crystallization
age of the rock (Fig. 3 inset). This calculation is
done by simultaneously solving the three equations
below, first by setting the slope of the secondary
Fig. 2. (a) Present-day thorogenic 208Pb/204Pb (vertical axis) composition vs. 206Pb/204Pb composition, with inset area showing magnified view
of data cluster. Data are from the SWAmazon craton whole rocks (this study): whole rocks of Blue Ridge of North Carolina and Virginia [47],
whole rocks of the Adirondacks [48]; leached feldspar from the Gneiss belt of Ontario [10]; Llano Uplift of Texas (whole rock and feldspars
[62]; Grenville xenoliths [63]); New Mexico and west Texas (whole rock and feldspars [8]); and Grenville belt of Labrador [12]. (b) Uranogenic207Pb/204Pb vs. 206Pb/204Pb compositions; references, inset, and symbols as in panel (a). Note the clear separation in values from the expanse of
the Laurentian Grenville belt vs. data from the Blue Ridge Province, which overlap with Amazon data.
E. Tohver et al. / Earth and Planetary Science Letters 228 (2004) 161–176166
Fig. 3. Graphic demonstrating the calculation of l2 using a two-point isochron consisting of the whole rock composition and the zircon Pb
composition. Crystallization occurs at 2400 Ma, with an increase in U content (i.e., l3Nl2) followed by evolution of the whole rock
compositions to the modern value that plots above and to the right of the average crustal composition. A decrease in U content at the time of
crystallization (i.e., l3bl2) would have resulted in modern whole rock composition that plotted below and to the left of the endpoint of the l2
curve (inset). In determining the initial Pb imparted by the source region, the whole rock–zircon isochron is projected back to a l2 curve so that
the crystallization age and the Pb evolution model age agree. (Inset) Various dotted curve lines represent l2 values 10.2–9.8. Dashed line curve
at the bottom is the Stacey and Kramers value for average crust, 9.735 [49]. The curved, solid line with the arrow is the evolution curve for the
whole rock system with l3. The whole rock–zircon isochron is seen to intersect the l2=10.2 curve at 2400 Ma and the l2=9.8 curve at 2100 Ma
but does not intersect the Stacey and Kramers curve. Solid lines with arrows are paleogeochrons for 100 Ma intervals that project back to the Pb
composition at 3.7 Ga, the beginning of the second stage of the Stacey and Kramers crustal Pb evolution model [49].
E. Tohver et al. / Earth and Planetary Science Letters 228 (2004) 161–176 167
whole rock–zircon isochron (206Pb/204Pbxtl,207Pb/204Pbxtl) equal to the 207Pb/206Pb zircon age
according to the right side of Eq. (1) below.
207Pb=204Pbobs � 207Pb=204Pbxtl206Pb=204Pbobs � 206Pb=204Pbxtl
¼ 1
137:88
ðek235Txtl � 1Þðek238Txtl � 1Þ ð1Þ
where
207Pb=204Pbxtl ¼ 207Pb=204Pb3:7 Ga þ1
137:88
� l2ðek235T3:7 Ga � ek235TxtlÞ ð2Þ
206Pb=204Pbxtl ¼ 206Pb=204Pb3:7 Ga
þ l2ðek238T3:7 Ga � ek238TxtlÞ ð3Þ
The values for 207Pb/204Pb3.7 Ga and206Pb/204Pb3.7 Ga
given by Stacey and Kramers [49] are 12.998 and
11.152, respectively. For the SW Amazon craton
rocks, average l2 values of 9.89F0.17 are required
for all the samples, in keeping with the high207Pb/204Pb values observed for all samples (Fig.
4a). Although in practice the intercept of the isochron
with a l2 evolution curve may yield a Pb model age
(Tintercept) different from the U–Pb crystallization age,
filtering the data by excluding data where this age
difference is N50 Ma does not change the underlying
result; the filtered average is 9.94 F0.19.
This model l2 approach has drawbacks in that it
assumes a single stage evolution following differ-
entiation from the Pb source region, thus ignoring the
obvious concern with felsic intrusive rocks of the
effects of crustal differentiation and contamination.
However, TDM for the rocks in question are rarely
Fig. 4. (a) Frequency diagram for calculated l2 values from data above in data bins of 0.25 units. Geochronological data (U–Pb zircon ages) used to
determine l2 values are as follows: SW Amazon craton [34,35]; Blue Ridge [77,79,85]; Adirondacks ([16,48] and references therein); Llano
[86,87]; Labrador ([12] and references therein). (b) Calculated values for l3 following extraction from Pb reservoir. Excluding, for the moment, the
Adirondacks curve, the Blue Ridge/MarsHill basement and the rest of the LaurentianGrenville belt appear to have been depleted in U at some point
in their respective histories, possibly as a result of high-grade (amphibolite to granulite) Grenvillian metamorphism reported for all of these rocks.
The small, secondary peak from the Adirondacks samples centered around l3=25 units are samples taken from a metasedimentary lithology (one
sample) and pegmatitic facies (three samples) of the Mt. Lyon Granite. The latter unit is reportedly the product of extensive Na-rich
hydrothermalism [48], suggesting a rare, localized occurrence of U enrichment. The greater variation in U contents in the SWAmazonmay reflect a
less homogeneous metamorphic history, with the U-enriched massifs generally in the 1.31–1.41-Ga age range. The bin size is 5 A3 units.
E. Tohver et al. / Earth and Planetary Science Letters 228 (2004) 161–176168
more than 200–300 Ma older than the U–Pb
crystallization age (J.S. Bettencourt, unpublished data;
35), an interval that is too short to have much effect on
Pb–Pb systematics [52]. Secondly, the effects of
metamorphism are ignored, although this is probably
a reasonable assumption for whole rock samples [50].
In support of this, we note that model l2 values from
all rock samples yield a coherent range, regardless of
crystallization age and subsequent metamorphic his-
tory. In addition, the calculated l2 values are in
excellent agreement with the range of values (Fig. 4a)
determined from post-Grenvillian, ca. 950 Ma galena
samples (l2=9.78–10.25) reported by Geraldes [53].
This simplified approach to Pb evolution in a
whole rock sample can be extended to calculate values
for l3 required for an individual whole rock sample to
reach the present-day values after crystallization. We
solve for l3 by setting the observed present day Pb
E. Tohver et al. / Earth and Planetary Science Letters 228 (2004) 161–176 169
composition equal to the Pb composition calculated
for the rock beginning at Txtl according to the
following equations:
l3 ¼ 207Pb=204Pbobs
��1
137:88ðek235Txtl � 1Þ
þ 207Pb=204Pbxtl
�ð4Þ
l3 ¼ 206Pb=204Pbobs=½ðek238Txtl � 1Þ
þ 206Pb=204Pbxtl� ð5Þ
where 207Pb/204Pbxtl and206Pb/204Pbxtl are determined
from Eqs. (2) and (3), respectively. The calculated
values for the time integrated U/Pb ratio (i.e., l3) for
individual samples following crystallization are gen-
erally lower than the modern measured U/Pb values, a
fact attributed to recent U gain for most samples (Fig.
5). The calculated l3 values for the Amazon rocks
range from 0.8 to 75, with an average value of 15.3,
which signifies that most samples did experience a net
gain in U at the time of crystallization. Most of the
high l3 samples, i.e., those with the most radiogenic
Pb, seem to be restricted to the ca. 1.4–1.3 Ga suites
Fig. 5. Calculated (solid line) and measured values (dashed line) of U (l3)
sets depicting pseudochrons with no geochronological significance, as discu
The calculated values of l3 give a U–Pb pseudochron with the same
(1372F59 Ma) for all samples. The plot of U data measured in sample
demonstrative of recently acquired excess U.
(average l3 of 28F16), in contrast with average l3
values of 8F6 for older rocks (Fig. 4b). This
observation supports widespread U scavenging from
older country rocks (>1.4 Ga) during this period of
extensive magma emplacement and regional meta-
morphism, in keeping with widely preserved ca. 1.3-
Ga metamorphic cooling ages [29,35,54].
4. Discussion
4.1. Isotopic differences between Amazon craton and
Laurentian Grenville
Reconstructions of Rodinia rely on the recognition
and identification of the distinct cratonic elements that
were incorporated via tectonic collisions into the
growing supercontinent. The suturing of Amazonia
and Laurentia along the greater Grenville mountains
provides a tectonic framework for identifying the
origin of individual terranes in the roots of the now
dismembered and deeply exhumed mobile belt. To
this end, Pb isotopic data from the Grenville province
vs. 206Pb/204Pb, with two regressed lines through the respective data
ssed in the text for the 207Pb/206Pb reference line depicted in Fig. 2b.
age (1326F25 Ma), within error, as the 207Pb/206Pb pseudochron
s is much more diffuse and yields a much younger apparent age,
E. Tohver et al. / Earth and Planetary Science Letters 228 (2004) 161–176170
of Laurentia, selected Appalachian basement inliers
with Grenvillian overprints, and Grenville-deformed
basement samples of Amazon are compared in Fig. 2.
Laurentian Grenville samples comprise both whole
rock and feldspar analyses and form a coherent pattern
that plots below the Pb evolution curve for the
average crust in the Stacey and Kramers model [49].
The coherence of Pb isotopic composition for rocks
from the entire extent of the Grenville Province (from
Labrador to Texas) is remarkable and is uniformly
lower than the crustal average [48]. The implication of
such uniformly low 207Pb/204Pb values in Grenville
rocks is that there was a homogeneous long-lived
mantle source characterized by early U depletion, as
has been suggested to be typical of the Superior craton
[55]. The l2 values calculated for the Labrador,
Adirondacks, and Llano portions of the Laurentian
Grenville Province form a tight cluster at ~9.5,
uniformly lower than Amazon values (Fig. 4a).
The episode(s) of Grenville deformation in Lau-
rentia affected crust of widely differing age, although
a coherent mass of juvenile crust forms the outboard
eastern portions of the belt (Fig. 1). In the exposed
Grenville belt of Canada, the Nd and Pb isotopic
systems reveal a pattern of older Paleoproterozoic to
Archean crust immediately adjacent to the Superior
province [10,17,18,56] that was reworked during the
late Mesoproterozoic orogeny, corresponding roughly
to the bpolycyclic parautochthonous beltQ of Rivers
[57]. Both Nd model ages and U–Pb crystallization
ages decrease away from the Superior province, with
increasingly juvenile materials, as defined by both Pb
and Nd isotopes, encountered across a southeast-
trending transect [10], with large expanses of Quebec
[17] and the Metasedimentary belt of Ontario [58,59]
defined by juvenile crust (+eND values) with Nd
model ages of 1.4–1.5 Ga. The Adirondacks and
Green Mountains of the NE United States are marked
by predominantly juvenile material with TDM in the
1.3–1.4-Ga range [16]. The expanse of this juvenile
crust is continuous to the south; in the subsurface of
the midcontinental United States, the Eastern Granite–
Rhyolite province is marked by TDM of 1.3–1.4 Ga
[60,61]. Juvenile crust also predominates in the
southernmost Laurentian basement exposures of the
Llano Uplift (TDM ~1.3–1.4 Ga) and the region to the
west [9,62,63]. The predominantly juvenile character
of the outboard easternmost portions of the Grenville
Province is summarized in Fig. 6, where a unimodal
distribution of eNd values for 1.0 Ga cluster about
positive values, indicating a juvenile mantle source.
Comparing the Nd isotopic data for the Amazon
craton with the Laurentian Grenville belt reveals the
different histories of these two cratons prior to the
Grenville episode. The majority of TDM ages from the
SW Amazon craton are generally in the 1.5–2.3 Ga
range [31,64,65]. Much of this material has been
reworked, as evidenced by eNd values that are
negative or close to CHUR values at the time of
crystallization (Fig. 6). Unlike the Laurentian rocks
deformed during the Grenville orogeny, juvenile
material is rare, as indicated by the overwhelmingly
negative eNd values calculated for Amazon samples at
1000 Ma, the approximate end of all collision-related
deformation in the Grenville Province. These values
cluster loosely around �3 e units, with a wider
variance in model ages than that observed in the
Grenville belt of North America. The similarity
between the SW Amazonian and Blue Ridge/Mars
Hill terrane Nd data will be discussed below.
4.2. Origin of Grenvillian basement inliers of the SE
Appalachians
The Paleozoic orogenies that gave rise to the
Appalachian Mountains complicate efforts to locate
the pre-Iapetan cratonic margin of Laurentia. In spite
of this difficulty, the Blue Ridge/Mars Hill terrane is
widely considered to be part of Laurentia by the end
of Proterozoic times [66–68], given its location west
of the Paleozoic suture zone (Fig. 1) that marks the
western limit of accreted terranes [66,67,69]. In
addition, Neoproterozoic plutons and dikes are wide-
spread throughout these massifs (Robertson River,
Crosnore, Bakersville dikes), having been emplaced
prior to the opening of Iapetus [70–72] and are
overlain by extrusive mafic rocks of the Catoction Fm
[73]. The Blue Ridge/Mars Hill terrane itself lies
above a shallowly dipping seismic reflector, demon-
strating that it is allochthonous to Laurentia [74,75],
although this boundary may have been reactivated
during Taconic and Alleghenian deformation. Resto-
ration of Paleozoic deformation in the Appalachians
of Virginia demonstrates a metamorphic gradient that
decreases to the east, with amphibolite–granulite
facies rocks (Lovingston massif) emplaced on top of
Fig. 6. (a) Sm–Nd data compiled from the outboard juvenile portions of the Laurentian Grenville Province including the Adirondacks; buried
Grenville province of the midcontinental region; the Llano Uplift and W. Texas region. Note the presence of eNdb0 for rocks older than 1.15 Ga
in the Blue Ridge/Mars Hill data set and overlap with data from the SW Amazon craton data. References as in Fig. 1. Samples where147Sm/144NdN0.14 are not considered in this distribution so as to represent only rocks of average crustal composition. Two low eNd samples
from both the Adirondacks and the Llano regions are marked with asterisks, indicating metasedimentary samples of suspect provenance. (b)
Frequency diagram of eNd values from the same data as above, calculated for 1000 Ma, showing the overlap in juvenile values for the Grenville
belt. A secondary peak around �6 e in the Blue Ridge/Mars Hill samples with zircon ages greater than 1.15 Ga shows the presence of older
material, demonstrating clear overlap with Amazonian crust. Bin size is 3 e units.
E. Tohver et al. / Earth and Planetary Science Letters 228 (2004) 161–176 171
deeper granulite facies Pedlar River massif to the west
[67,69]. Further south, the Mars Hills block shows
evidence of having been emplaced structurally above
the adjacent Blue Ridge province rocks of North
Carolina and Tennessee [76].
Geochronological constraints on the timing of this
deformation suggest that the early phase of NE–SW
compression took place between 1145 and 1075 Ma
[77], with younger deformation and metamorphism
associated with emplacement of granites, charnockites,
E. Tohver et al. / Earth and Planetary Science Letters 228 (2004) 161–176172
and anorthosites ranging in age from 1077 to ca. 1020
Ma [77–79]. In spite of the similarity of these ages to
typical Grenville Province ages, the Blue Ridge/Mars
Hills domains form an exception to the general isotopic
architecture of Laurentia. Lead compositions from
these rocks display a trend that is clearly separate from
the rest of the Laurentian Grenville belt, as observed by
Sinha et al. [47] and Sinha and McLelland [48].
However, the coherence of the Amazon trend with
the Blue Ridge/Mars Hill Pb data is striking, with both
data sets easily distinguishable from the Laurentian
Grenville data set (Fig. 2b). Indeed, the calculated l2
values for the SW Amazon and the Blue Ridge/Mars
Hill basement are observed to follow the same
distribution about average l2 values of 10, with a
smaller cluster of values at ~10.5 (Fig. 3a).
The high l2 values calculated for the Blue Ridge/
Mars Hills source region strongly suggest extraction
from a source region other than that which gave rise to
the outboard, juvenile regions of the Laurentian Gren-
ville belt for which the present day Pb compositions are
so distinctively and homogeneously nonradiogenic
(Fig. 3a). The uniqueness of the Blue Ridge/Mars Hill
terrane with respect to Laurentia is supported by Nd
isotopic data from metaigneous rocks [79–81], which
reveal a pattern very different from the nearest adjacent
portions of the Grenville belt (Fig. 1). The presence of
mature, continental material with TDM ranging from 1.5
to 2.2 Ga distinguishes the Blue Ridge/Mars Hill
terrane from the rest of the Laurentian Grenville belt.
The bimodal variation in eNd values calculated at 1000
Ma indicates the presence of both reworked continental
material with negative values (�2 to �9) preserved in
rocks older than 1.15 Ga and a more juvenile
contribution (with eNd of �2 to +4) in rocks younger
than 1.15 Ga (Fig. 6). The presence of this anomalous
Paleoproterozoic crust was first recognized on the basis
of 1.8 Ga Rb–Sr mineral isochrons [82] and has been
confirmed by SHRIMP dating of zircons with igneous
cores that yielded ages of ca. 1.8 Ga [79]. There is clear
overlap of the eNd (1000) values from the Amazon and
the older rocks of the Blue Ridge/Mars Hill terrane,
supportive of derivation from the same source region.
The similarity in both Nd and Pb isotopic
signatures from the Amazon and the Blue Ridge/Mars
Hill terrane points to a common ancestry. If the Pb
isotope patterns were solely the product of Grenvillian
metamorphic history, the Blue Ridge/Mars Hill data
would match the pattern observed in the rest of the
Laurentian Grenville belt, inasmuch as the metamor-
phic geochronology of both is practically indistin-
guishable [77,79]. In fact, a high-grade U-depleting
metamorphic history in the late Mesoproterozoic may
be reflected in the low l3, i.e., values calculated for
both (Fig. 4b). Given the distinctiveness of the
modern day Pb compositions for the Blue Ridge/
Mars Hill rocks from the rest of the Laurentian
Grenville Province, later metamorphism and intrusion
did not obliterate the Pb isotopic characteristics
inherited from the source region. In contrast, the
metamorphic effects of Grenvillian orogenesis on the
Amazon craton appear to have been much more
heterogeneous, as observed through both high and
low l3 values, meaning that both localized U enrich-
ment and U depletion occurred.
Our ability to see through the metamorphic veil
to Blue Ridge/Mars Hill source region characteristics
is aided by Nd isotopes. The relative immobility of
Sm and Nd with respect to whole rock samples
means that the effects of high-grade metamorphism
did not prevent the preservation of Paleoproterozoic
Nd model ages in the Blue Ridge/Mars Hill base-
ment. However, unlike Pb, Nd isotopes do demon-
strate the effects of a different source region for
Grenvillian rocks in the Blue Ridge/Mars Hill
basement after ca. 1.15 Ga. This may be explained
through mass balance considerations; Nd concen-
trations do not vary greatly between felsic and mafic
rocks, whereas Pb-poor mafic rocks (anorthosites,
gabbros, basalts) in the post-Grenville interval are
unlikely to have greatly altered the Pb signature
inherited from older Pb-rich felsic rocks. Juvenile
material observed in rocks younger than 1.15 Ga
suggests a transition of source regions for the Blue
Ridge/Mars Hill basement; before this time, Ama-
zonian signatures dominate. Following the tectonic
transfer to Laurentia at ca.1.15 Ga, Nd isotopes
reveal an influx of intrusive rocks with a Laurentian
source (Fig. 6).
5. Conclusions
The ancient, highly radiogenic source region of the
SW Amazon craton provides us with an isotopic
fingerprint for paleogeographic reconstructions. We
E. Tohver et al. / Earth and Planetary Science Letters 228 (2004) 161–176 173
interpret the similarity of Amazon craton Pb and Nd
isotopic signatures with the Blue Ridge/Mars Hills
domain of the southern Appalachian to indicate a
common origin. Both are distinct from Laurentian
isotopic signatures for the rest of the Grenville belt. In
our reconstruction, the transfer of the Blue Ridge/
Mars Hill terrane to Laurentia took place during the
assembly of Rodinia, following the collision of the
Amazon with southernmost Laurentia at ca. 1.2 Ga.
Extensive deformation recorded in the southeast
Appalachian region after ca.1.15 Ga gives a geo-
chronological basis for the timing of this terrane
transfer. The ~50 My that elapsed after the original
collision and the suturing of the Blue Ridge/Mars
Hills terrane to Laurentia is evidence of continued
relative motion between the Amazon craton and
Laurentia. This interpretation of a mobile Rodinia
configuration is supported by the diminishing evi-
dence for Amazon source region characteristics in the
Blue Ridge/Mars Hill basement rocks after 1.15 Ga.
This SWAmazonian crust, later stranded in Laurentia
following the breakup of Rodinia, serves as paleogeo-
graphic marker of the northward passage of the
Amazon craton along the Grenville margin of
Laurentia. The net sinistral displacement between
Amazon and Laurentia suggests that Rodinia paleo-
geography evolved throughout the assembly phase of
the supercontinent’s history.
Acknowledgments
E. Tohver thanks Ben van der Pluijm and Jamie
Gleason for stimulating conversations that preceded
this contribution, which was written with support from
NSF grant #INT-0301807. Fieldwork and analytical
costs were underwritten with support from research
grants to J.S. Bettencourt (FINEP/FUNDUNESP
no. 65.94.0249.00, PADCT/FINEP 64.99.027.00.,
FAPESP-Proc. no. 2000/08033-5) and a scholarship
awarded to B.L.Payolla (FAPESP-Proc. no. 95/0290-
9). The authors acknowledge the cooperation of the
U.S. Geological Survey at Menlo Park where R. Tosdal
analyzed 44 samples. The authors would like to
sincerely thank Dr. Kotov from the Institute of
Precambrian Geology and Geochronology, Russian
Academy of Sciences (IPGG-RAS) in St. Petersburg
where analysis of 12 samples was undertaken.
Thoughtful reviews by Peter Gromet and Randy Van
Schmus are acknowledged and appreciated.
Appendix A. Supplementary data
Supplementary data associated with this article can
be found, in the online version, at doi:10.1016/
j.epsl.2004.09.029.
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