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1 Institut National de la Recherche Scientifique, Eau, Terre et Environnement, 490 de la Couronne, Québec, Québec G1K 9A9, Canada
2 Geological Survey of Canada–Québec, Earth Science Sector, 490 de la Couronne, Québec, Québec G1K 9A9, Canada
3 Geological Survey of Canada–Ottawa, Earth Science Sector, 601 Booth Street, Ottawa, Ontario K1A 0E8, Canada
Correspondence:
E-mail: celine.dupuis.1{at}ulaval.ca.
Correspondence: *E-mail: michel.malo{at}ete.inrs.ca.
Correspondence:
E-mail: Jean.Bedard{at}rncan.gc.ca.
| FOOTNOTES |
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| ABSTRACT |
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Key Words: igneous clasts calc-alkaline tholeiite volcanism back-arc basin Dunnage zone Gaspé Appalachians
| INTRODUCTION |
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Volcano-sedimentary rocks of the extensive Middle Paleozoic Gaspé belt unconformably overlie (or are in faulted contact with) Upper Neoproterozoic to Upper Ordovician rocks of the Humber and Dunnage zones (Figs. 1 and 2). The basal unit of the Gaspé belt is the Upper Ordovician Garin Formation (Fig. 2; Malo, 1988; Malo and Bourque, 1993), a turbiditic siliciclastic unit including conglomerates derived from a source region composed mainly of sedimentary and volcanic rocks (Ducharme, 1979; Vennat, 1979; Malo, 1988). Igneous clasts in the Garin conglomerates include extrusive and intrusive, mafic to felsic varieties. In the southern Gaspé Peninsula, the Garin Formation para-conformably overlies Llanvirnian sandstones of the Arsenault Formation and the McCrea mélange (Malo and Bourque, 1993) and marks a hiatus corresponding to five graptolite zones (~10 m.y.). In the Popelogan inlier of northwestern New Brunswick, the Balmoral Group of the Dunnage zone is overlain by the Grog Brook Group or the White Head Formation (Wilson et al., 2004), a hiatus of 2 to nearly 15 m.y., respectively (Fig. 3, column A). Thus, throughout this part of the Appalachians, there is an age gap separating accretion of terranes during the Taconian from the first deposition of strata in the Gaspé belt successor basin. Since rocks of the McCrea and Popelogan inliers are considered part of the oceanic Dunnage zone (see Williams, 1995), then clasts in the Garin Formation could include fragments of the Ordovician Iapetus oceanic domain, and so provide information about the events in adjoining terranes that are now buried beneath younger units. In this paper, we document the petrography and geochemistry of the igneous clasts from the Garin Formation and provide new geochronological data on some of them. These data allow us to correlate these rocks with putative source terranes. When combined with new age data from the underlying Dunnage zone rocks in the Gaspé Peninsula, we obtain improved constraints for tectonic models of the Dunnage oceanic tract during Ordovician (syn- to post-Taconian) time.
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| GEOLOGICAL SETTING |
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Rocks of the Humber zone consist of rift-related basalts, slope-and-rise deposits of the Laurentian passive margin (Lavoie et al., 2003), and synorogenic foreland basin turbidites (Prave et al., 2000). Regional deformation of the Humber zone is dominated by the Taconian orogeny, which records ophiolite obduction, collision of arc terranes, crustal thickening of the Laurentian margin, and the emplacement of northwest-verging thrust sheets (St-Julien and Hubert, 1975; De Broucker, 1987; Slivitzky et al., 1991; Pincivy et al., 2003). In Gaspé, the contact between the Humber and Dunnage zones is commonly marked by a series of partly dismembered ophiolites and associated mélanges (Malo et al., 1992a) called the Baie Verte–Brompton Line (Williams and St-Julien, 1982).
The Dunnage zone is composed of rocks derived from the Ordovician Iapetus Ocean. It is subdivided into the Notre Dame and Exploits subzones, which correspond to Iapetan terranes formed outboard of Laurentia and Gondwana, respectively. The Red Indian Line (Fig. 1), the tectonic contact between both subzones, was developed during Late Ordovician closure of the main tract of the Iapetus Ocean (van Staal et al., 1998), and it is regarded as the orogen's main suture zone. Near the Baie Verte–Brompton Line, the Dunnage zone in Gaspé is represented by inliers that contain tectonic and/or olistostromal mélanges and serpentinite bodies, which include (from the northwest to the southeast, Fig. 2): the Ruisseau Isabelle mélange, the Lady Step Complex, the Rivière Port-Daniel mélange, the Nadeau ophiolitic mélange, and the McCrea mélange. Some deformational features of the Dunnage zone are attributed to Taconian accretionary processes (De Broucker, 1987; Tremblay et al., 1995), but the major regional deformation event is the Acadian orogeny.
The Gaspé belt post-Taconian successor basin is divided into four broad temporal and lithological assemblages (Fig. 2; Bourque et al., 2000). From the base to the top, these are: (1) the uppermost Ordovician–lowermost Silurian deep-water, fine-grained carbonate-siliciclastic facies of the Matapédia Basin belonging to the Honorat Group (which has only one formation, the Garin Formation) and the Matapédia Group; (2) the Silurian–lowermost Devonian shallow- to deep-shelf facies of the Chaleurs Group; (3) the Lower Devonian mixed siliciclastic and carbonate fine-grained deep-shelf to basin facies of the Upper Gaspé Limestones and Fortin Groups; and (4) the Lower to Middle Devonian near-shore to terrestrial coarse-grained facies of the Gaspé Sandstones Group. The Gaspé belt was deformed mainly by the Acadian orogeny during the Middle Devonian, but it also shows structures related to the Salinic disturbance (Malo, 2001). Rocks have been affected by regional anchimetamorphism to low-grade burial metamorphism (Nowlan and Barnes, 1987; Chagnon, 1988; Hesse and Dalton, 1991).
The Matapédia Basin and Its Dunnage Zone Basement in Southern Gaspé Peninsula and Northern New Brunswick
The lowermost rocks of the Gaspé belt define the Matapédia Basin and outcrop mainly in the southern Gaspé Peninsula, northwestern New Brunswick, and northeastern Maine (Malo, 2004). In Gaspé and New Brunswick, the Matapédia Basin consists of the Garin Formation and the Grog Brook and Matapédia Groups, all of which unconformably overlie rocks of the Dunnage zone (Fig. 2). The Upper Ordovician Garin Formation is made up of terrigenous rocks, including black claystone, noncalcareous gray mudstone, greenish-gray siltstone, calcareous siltstone, calcareous quartz-wacke, lithic wacke, conglomerate, and silty dolomitic limestone (Malo, 1988; Malo and Bourque, 1993). Conglomerates contain volcanic, sedimentary, plutonic, ultramafic, and rare metamorphic clasts derived from a source region located to the south (Ducharme, 1979; Vennat, 1979; Malo, 1989). The Matapédia Group consists of a lower laminated calcareous mudstone unit (Pabos Formation), followed by a succession of calcareous rocks (White Head Formation) (Malo, 2004).
The Upper Ordovician Grog Brook Group in New Brunswick is the lithostratigraphic equivalent of the Garin Formation (Figs. 2 and 3). The Grog Brook Group consists of a thick series of mainly siliciclastic turbidites, sedimentary structures, and bed forms typical of deep-water facies (Wilson et al., 2004). Polymictic conglomerates of the Grog Brook Group contain rounded to angular clasts of unfoliated felsic and mafic volcanic rocks, fine-grained sedimentary rocks, chert, quartz, and feldspar in a mudstone or siltstone matrix (Wilson et al., 2004).
Upper Ordovician rocks of the Matapédia Basin in the Gaspé Peninsula unconformably overlie Dunnage zone rocks of peri-Laurentian affinity of the McCrea inlier (column 2, Fig. 3), whereas in two other inliers, the Maquereau-Mictaw inlier and the Nadeau ophiolitic mélange, the Dunnage zone basement is unconformably overlain by Silurian rocks of the Chaleurs Group (column 3, Fig. 3). The McCrea inlier (Fig. 2) consists of two lithostratigraphic units (column 2, Fig. 3): the McCrea mélange, and the forearc turbidites of the Arsenault Formation. The Maquereau-Mictaw inlier is a tectonic collage made up of Cambrian rift-related basalt, arkose, and slate of the Maquereau Group (Humber zone; Bédard and Wilson, 1997) juxtaposed against Dunnage zone rocks of the Rivière Port-Daniel mélange and the Mictaw Group (De Broucker, 1987). The Lower Ordovician McCrea and Rivière Port-Daniel mélanges are made up of tectonic slices and mappable blocks of serpentinite, listwaenite, granitic rocks, and basalt, and clasts of granitic gneiss, serpentinite, red slate, and calcareous siltstone embedded in a matrix of black shale and pebbly mudstone (De Broucker, 1987; Malo et al., 1992b). The Llanvirnian Arsenault Formation and the basal unit of the Mictaw Group (Neckwick Formation) (Malo and Bourque, 1993) are correlative and consist of turbiditic sandstones, shales, and minor tuffs. Detailed mapping of the McCrea inlier south of the Grand Pabos fault (Fig. 4) shows that the 15-km-long gabbronoritic sill of the MORB-like Pabos Suite is intruded into the pebbly mudstone of the McCrea mélange. In the Maquereau-Mictaw inlier, ferrogabbroic rocks that are potentially correlative with the Pabos Suite (Bédard, 1986) cut sedimentary rocks that might be part of the Rivière Port-Daniel mélange, although they are mapped as Neckwick Formation (De Broucker, 1987). The Nadeau ophiolitic mélange contains blocks of serpentinized peridotite, amphibolite, tuffaceous graywacke, quartzite, and granitic rocks embedded in a serpentinite matrix, as well as very large blocks of metagraywacke and amphibolite correlated with the Chain Lakes Massif (De Broucker, 1987; cf. Gerbi et al., 2006).
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| LOCALIZATION OF SAMPLES AND FIELD DESCRIPTIONS |
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The McCrea mélange contains slivers of dark-gray to green and red, fine- to medium-grained and usually massive basaltic volcanic rocks associated with a fault breccia containing fragments of granitoids and granitic gneiss. The basalts contain phenocrysts of prismatic feldspar and secondary epidote, calcite, and hematite.
Conglomerates of the Garin Formation in the Gaspesian Chaleurs Bay area occur as massive beds (Fig. 2), 1–7 m thick (Simard, 1986; Gosselin, 1988), containing more than 85% igneous and sedimentary pebbles and cobbles, which range from 2 mm to 40 cm in diameter (average 6 cm). Igneous clasts range from gabbro, diabase, and basalt to monzonite, rhyolite, and quartz-feldspar porphyry. Sedimentary clasts are fine to pebbly sandstone, siltstone, mudstone, and chert.
We analyzed three volcanic rocks collected from the deepest geological formation encountered in the Miguasha-Est no. 1 well (Fig. 2). The surface geology consists of sedimentary rocks of the Carboniferous Bonaventure Group, but Paleozoic volcanic rocks were sampled between 1260 and 1430 m depth, below a major unconformity between sedimentary rocks assigned to basal units of the Chaleurs Groups and a sequence of dark-gray to reddish volcanic rocks assigned to the Balmoral Group (C. Morin, Hydro-Québec, 2006, personal commun.). If these volcanic rocks are indeed equivalents of the Balmoral Group, then they would represent samples of the buried Popelogan arc.
| PETROGRAPHY OF GARIN CONGLOMERATE CLASTS |
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All volcanic rocks are porphyritic, with prismatic plagioclase phenocrysts up to 1 cm long. Rhyolites also contain phenocrysts of prismatic alkali-feldspar, subrounded quartz, and euhedral to subhedral hornblende, whereas basalts have additional clinopyroxene phenocrysts. Monzonite and porphyritic latite have prismatic plagioclase, granophyric intergrowths of alkali-feldspar and quartz, subhedral to euhedral clinopyroxene, hornblende, biotite, and ilmenite. Fresh plagioclase, K-feldspar, clinopyroxene, and ilmenite occur in gabbro and diabase. Prismatic plagioclase and euhedral to subhedral clinopyroxene occur as phenocrysts in diabase, or form an ophitic texture.
| WHOLE-ROCK CHEMISTRY |
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Andesitic rocks, monzonites, and rhyolites all have clear calc-alkaline geochemical signatures characterized by strong light rare earth element (LREE) and U-Th enrichment and prominent negative Nb-Ta anomalies (Figs. 8A and 8C). However, variations in REE abundances, especially heavy (H) REEs, define two subgroups among these calc-alkaline rocks. Subgroup 1 is composed of the andesitic rocks GLEN-78 and GLEN-80A and rhyolite GLEN-52 and is enriched in HREE (Fig. 8A). Note that two andesites of the Miguasha-Est no. 1 well have multi-element patterns similar to those of the HREE-rich andesites of subgroup 1, while the rhyolite from this same well somewhat resembles HREE-rich rhyolite GLEN-52, but it has weaker negative Nb-Ta anomalies and slight positive Zr-Hf anomalies (Fig. 8B). Subgroup 2, composed of the monzonites and HREE-poor rhyolites, is more depleted in HREE than subgroup 1 and is more variable in LREE content (Fig. 8C). A trachyandesite (RLH-49A) has a broadly similar pattern to the subgroup 2 samples, except for prominent negative Zr-Hf anomalies, which are not observed in any other sample from the calc-alkaline intermediat-felsic suite (Fig. 8D). Three porphyritic rhyodacites/dacites are also broadly similar, but they have the lowest La/Yb ratios and show slight positive Zr-Hf anomalies (Fig. 8E). One HREE-poor monzonite (RJ-27) and one porphyritic rhyodacite/dacite (RLH-87) were dated by the U-Pb zircon method (see following).
On a tectonic discrimination diagram for silicic rocks, the HREE-poor rocks clearly plot in the field of volcanic arc–related felsic rocks, whereas the HREE-rich rocks, including the Miguasha volcanic rocks, overlap the fields of volcanic arc and within-plate felsic rocks (Fig. 6A). Note that we have also plotted intermediate rocks of the suite on this diagram for comparison purposes. The strong negative Nb-Ta anomalies, enrichment in LILE and LREE, and generally evolved nature of these rocks are typical of calc-alkaline continental magmas (Fig. 8).
Transitional-Alkaline Suite
The tholeiitic-to-alkaline rock suite (two samples) is composed of one diabase and one basaltic andesite, each of which has a slightly different geochemical signature (Fig. 5). On tectonic discrimination diagrams for basalts, rocks of the transitional-alkaline suite plot in the field for continental basalts, and the transitional-alkaline diabase RLH-34 plots close to the rift field (Fig. 7). Diabase RLH-34 has a LRE-enriched pattern and shows very slight positive Nb-Ta and Ti anomalies (Fig. 8F) characteristic of within-plate alkaline basalts (Pearce, 1996), and we infer derivation from an enriched mantle source. The lesser LREE enrichment and slight negative Nb-Ta anomalies of basaltic andesite RJ-24 suggest either a small contribution from a subduction component or minor crustal contamination (Fig. 8F). This rock can therefore be interpreted to represent either a transition between a within-plate source and a developing subduction zone, or contamination by continental crust.
Mafic-Intermediate Suite
Rocks of the mafic-intermediate suite (12 samples) range in composition from tholeiitic basalts and gabbros to andesitic rocks (Fig. 5). All rocks of the suite have oceanic signatures characterized by low REE and U-Th abundances (Figs. 8G–8H). However, variations on the slope of the multi-element patterns define two subgroups. Subgroup 1 is composed of the tholeiitic basalts that have flat to slightly HREE-depleted REE patterns (Fig. 8G). The slight negative Nb-Ta anomalies and slight enrichment in U-Th suggest the influence of an arc component or crustal contamination. Such geochemical signatures are characteristic of marginal basins (Pearce, 1996). On tectonic discrimination diagrams, these samples plot in or close to the field for back-arc basin basalts (Fig. 7).
Subgroup 2 is composed of tholeiitic gabbros and andesites. The tholeiitic gabbros have fairly flat REE patterns, but they are more depleted than the basalts of subgroup 1 (Fig. 8H). They have more pronounced negative Nb-Ta anomalies, slight negative Ti anomalies, and enrichment in U-Th, which together probably imply an important influence from an arc component. The andesites and calc-alkaline andesitic rocks have more enriched compositions and show progressive enrichment in the most incompatible LREE and U-Th (Fig. 8H), pronounced negative Nb-Ta anomalies, and distinct negative Ti anomalies. Subgroup 2 rocks plot in the adjacent and partially overlapping island-arc tholeiite and calc-alkaline basalt fields (Fig. 7). Such geochemical signatures and associations, ranging from tholeiitic to calc-alkaline, are characteristic of oceanic arcs (Pearce, 1996). The importance of the subduction component does not seem to be related to the degree of LREE enrichment.
Granitic and Mafic Rocks of the McCrea Mélange
Granitic rocks of the McCrea mélange overlap the fields of volcanic arc and within-plate felsic rocks on the tectonic discrimination diagram for silicic rocks, similar to subgroup 1 of the calc-alkaline intermediat-felsicsuite (Fig. 8A). Mafic lavas of the McCrea mélange range from tholeiitic to calc-alkaline and have been interpreted as containing an oceanic subduction component (Malo et al., 1992b). On the tectonic discrimination diagram, McCrea basalts plot in the field for back-arc basin basalts, overlapping the fields for transitional MORB (T-MORB) and continental basalts (Fig. 7A). On this diagram, they are mostly similar to tholeiitic basalts of subgroup 1 of the mafic-intermediate suite. However, due to the analytical procedure available at that time, Nb values are not precise and may have been overestimated during analysis. Overall, basalts of the McCrea mélange show close resemblance to the mafic-intermediate suite clasts in the Garin Formation (see discussion on the comparison of Garin clasts with potential source terranes below) and may represent samples of the Garin Formation's source terrane.
| AGE DATA |
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| DISCUSSION |
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Notre Dame Subzone
In contrast to the abundance of geochemical data on volcanic and intrusive rocks of the Exploits subzone in New Brunswick and Maine (van Staal, 1987; Dostal, 1989; van Staal et al., 1991, 2003; Winchester et al., 1992; Winchester and van Staal, 1994; Fyffe, 2001; Rogers et al., 2003b; Schulz and Ayuso, 2003; Wilson, 2003), there are few complete geochemical data sets on volcanic and intrusive rocks of the Notre Dame subzone in the Gaspé Peninsula. The latter mainly come from the McCrea inlier (Malo et al., 1992b) and the Pabos Suite (Bédard, 1986). For the purpose of comparison with volcanic terranes of the Notre Dame subzone, we use the geochemical data on volcanic and intrusive rocks of the Annieopsquotch accretionary tract, a recently recognized and well-studied tectonic collage of volcanic terranes in Newfoundland's Notre Dame subzone (Lissenberg et al., 2005b; Zagorevski et al., 2006). The Annieopsquotch accretionary tract is the most outboard tectonic unit of the peri-Laurentian Notre Dame subzone, and it is closest to the Red Indian Line and the peri-Gondwanan Exploits subzone (van Staal, 2007). It is composed of remnants of ophiolitic and arc–back-arc complexes that were generated over ~20 m.y. above a single west-dipping subduction zone outboard of the Laurentian margin, and it records the final Late Ordovician closure of the main tract of the Iapetus Ocean along the Red Indian Line (Zagorevski et al., 2006; van Staal, 2007). The Annieopsquotch ophiolite belt, the oldest and most inboard unit of the Annieopsquotch accretionary tract, marks the initiation of westward subduction beneath the Laurentian margin at ca. 480 Ma. The Lloyds River ophiolite complex (ca. 473 Ma) preserves a fragment of younger, more MORB-like back-arc oceanic crust, which originated as a back-arc to the Buchans Group (ca. 473 Ma) continental bimodal calc-alkaline arc. These units were stitched and overlain by continental magmatic rocks of the Otter Pond Complex (ca. 468 Ma) immediately after their accretion to composite Laurentia. Following the ca. 468 Ma accretion event, the accreted Buchans arc rifted due to continuing subduction, leaving most of the exposed Buchans Group in a remnant arc position (Fig. 11C). The younger Red Indian Lake Group (465–460 Ma) records the opening of this new back-arc basin and the subsequent establishment of a bimodal continental calc-alkaline arc sequence (Fig. 11C). The main tract of the Iapetus Ocean closed at ca. 450 Ma, resulting in a collision between peri-Laurentian Red Indian Lake arc and peri-Gondwanan Victoria Lake arc (the Newfoundland equivalent of the Popelogan arc; van Staal et al., 1998) and incorporation of the Red Indian Lake Group into the Annieopsquotch accretionary tract.
Origin of the Pabos Suite
Gabbros of the Pabos Suite in the Gaspé Peninsula have a primitive oceanic signature (Fig. 6A) and are interpreted to represent a tensional event and/or an episode of rifting in a marginal basin (Bédard, 1986; De Broucker, 1987). Geochemical comparisons are consistent with the possibility that gabbroic intrusions in the Mictaw Group (Neckwick Formation) (Bédard, 1986) and diabasic intrusions in the Arsenault Formation (Malo et al., 1992b) are cogenetic with the Pabos Suite. Our preferred Early Ordovician age for the Pabos Suite (471.2 ± 11.2 Ma) is therefore consistent with paleontological constraints, since the Arsenault and Neckwick Formations are of Llanvirnian age (Fig. 3; ca. 464 Ma), based on the presence of diagnostic graptolites (Riva and Malo, 1988) from the murchisoni zone of Great Britain or the upper part of the callotheca zone of North America. The paleontological age is within the error limits of our age determination for the Pabos Suite (482.4–460 Ma). Moreover, the geochemical signatures of the Pabos Suite rocks are fairly similar to the older Annieopsquotch accretionary tract ophiolitic rocks (480–473 Ma), which represent peri-Laurentian supra-subduction zone and continental arc–oceanic back-arc complexes (Lissenberg et al., 2005a; Zagorevski et al., 2006).
Should the older age of 489.4 ± 5.0 Ma be retained instead, then the Pabos Suite would be coeval with the development of pericontinental ophiolites all along the Laurentian margin (from southern Québec to Newfoundland). This would imply that the MORB-like intrusions that cut the Llanvirnian Arsenault and Neckwick Formations (Mictaw Group) would represent a second, much younger unrelated phase of back-arc(?) rifting that must postdate accretion of the McCrea mélange to Laurentia. We cannot discriminate unambiguously between these two possibilities, but we tentatively retain the younger age (471.2 Ma) because it is more consistent with the geological relationships, ages, and lithostratigraphic correlations between the different host rocks, and it provides a simpler geological history.
Comparison of Garin Clasts with Potential Source Terranes
Calc-Alkaline Intermediat-felsic Suite
Most of the HREE-poor rocks of the Garin calc-alkaline intermediat-felsic suite show a fair resemblance to the intermediate volcanic to felsic rocks of the Meductic Group (480– 473 Ma) in the Exploits subzone of southern New Brunswick (Figs. 6C, 12A, and 12B). However, they show a much closer resemblance to intermediate and felsic rocks of the Red Indian Lake Group (465–460 Ma) in the peri-Laurentian Annieopsquotch accretionary tract of Newfoundland (Figs. 8E and 12C–12G). Our U-Pb dating on zircons of the HREE-poor rocks of the calc-alkaline intermediat-felsic suite (465–466 Ma, Fig. 10) precludes a correlation with the Meductic Group and favors a correlation with the Red Indian Lake Group of Newfoundland. We conclude that clasts of HREE-poor rocks of the calc-alkaline intermediat-felsic suite in the Garin Formation probably record Late Ordovician erosion of calc-alkaline magmatic rocks formed in a Llanvirn peri-Laurentian continental arc (Fig. 11C).
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Volcanic rocks of the Miguasha-Est no. 1 well represent HREE-rich magmas with signatures typical of calc-alkaline continental arcs, and they are geochemically similar to Popelogan arc volcanic rocks and Tetagouche and California Lake dacite-rhyolites (Figs. 6B–6E and 14B–14E). Furthermore, these rocks are located on the extension of the Popelogan anticlinorium (Fig. 2), and, hence, we infer that they should either be correlated with calc-alkaline rocks of the Popelogan arc (Fig. 11A), or they represent remelting of Popelogan arc crust during Gander margin continental extension and rifting (Fig. 11B).
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Nd values indicate derivation from a long-term depleted mantle, and they have been related to a late period of extension in the Popelogan arc–Tetagouche–Exploits back-arc system (Schulz and Ayuso, 2003). Basaltic andesite RJ-24 correlates better with Llanvirnian tholeiites of the Tetagouche Group (Fig. 15B), which are inferred to have experienced crustal contamination during rift volcanism through thinned continental crust (van Staal et al., 1991). Note that neither alkaline nor transitional-alkaline mafic lavas have been recognized in the Annieopsquotch accretionary tract of Newfoundland. Hence, clasts of the tholeiitic-to-alkaline suite in the Garin Formation may be samples of the magmatism associated with the inferred of late rifting phase of the Popelogan arc (Fig. 11B). Alternatively, they may originate from a geodynamically similar peri-Laurentian back-arc basin (Fig. 11C) that has not yet been identified.
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| TECTONIC EVOLUTION OF THE DUNNAGE ZONE |
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Their geochemical characteristics indicate that the igneous clasts in the Garin conglomerates record the evolution of a continental arc–back-arc complex during Late Ordovician time. Since both peri-Laurentian and peri-Gondwanan terranes have experienced coeval but unrelated arc-building events on opposite sides of the Iapetus Ocean, neither provenance can be entirely ruled out. However, the very good age and geochemical correlation that is observed with units of the Red Indian Lake Group clearly favors a peri-Laurentian origin for rocks of the calc-alkaline intermediat-felsic and mafic-intermediate suites. The transitional to alkaline signatures of the tholeiitic-to-alkaline suite are also consistent with the rifting of a continental arc and opening of a back-arc basin. However, magmas similar to the tholeiitic-to-alkaline suite have not been sampled in Newfoundland's Red Indian Lake Group. We do not see this as a strong argument against a peri-Laurentian origin of the tholeiitic-to-alkaline suite rocks, however, since alkaline magmas are inherently sparse in occurrence, and the Red Indian Lake Group is not widely exposed. We suggest that tholeiitic-to-alkaline-like rocks may have existed in the Red Indian Lake Group or correlatives elsewhere, but they have not yet been sampled.
The Red Indian Lake Group of Newfoundland records arc rifting and the opening of a new back-arc basin, followed by establishment of a new continental calc-alkaline arc sequence (Fig. 11C; van Staal et al., 1998). While these rocks were probably much too distant to act as the direct source for the Garin clasts, we propose that the west-directed subduction responsible for the Red Indian Lake Group also affected the Laurentian margin at the latitude of Gaspé. If this interpretation is correct, then the igneous clasts within the Upper Ordovician Garin Formation sampled a largely unexposed terrane of the Notre Dame subzone that had not previously been recognized in this part of the Québec Appalachians. Considering the good correlations of the HREE-rich rocks of the calc-alkaline intermediat-felsic suite with granitic clasts in the McCrea mélange, and of rocks of the mafic-intermediate suite with mafic lavas of the McCrea mélange, as well as the good correlations between the McCrea mélange lavas and rocks of the Red Indian Lake Group in general, we infer that the tectonic slices of mafic lavas and granitic rocks of the McCrea mélange that are caught up in the Grand Pabos fault zone are the only expression of this poorly exposed arc terrane in Gaspé.
The discovery of this "new" terrane has paleogeographic and chronological implications for the evolution of Appalachians in Québec, New Brunswick, and northern Maine. The Garin Formation, the basal unit of the Gaspé belt basin, was deposited beginning in the late Caradocian (spiniferus zone) (Fig. 3), and it was later deformed during the Early Silurian Salinic and Middle Devonian Acadian orogenesis, together with younger Silurian-Devonian rocks of the basin (Malo and Bourque, 1993). The pre-Acadian palinspastic position of the Garin Formation indicates that it was deposited within the Iapetus oceanic domain to the south of the Taconian-modified Laurentian margin (Malo, 2004). The absence of any clasts in the Garin Formation that could have been derived from continental lavas typical of the Humber zone (e.g., Maquereau Group) supports the inferred oceanic tectonic setting. In addition, the Garin Formation igneous clasts were only affected by low-grade, hydrous metamorphism, and they lack any evidence of accompanying penetrative deformation that could be Taconian-related. On the other hand, volcanic rocks of the Miguasha-Est no. 1 well are not exotic blocks and are located along the inferred extension of the arc volcanic rocks of the Popelogan inlier (anticlinorium) (Fig. 2), which is consistent with their geochemical signatures. The proposed Notre Dame subzone provenance for the bulk of the igneous clasts in the Garin Formation and Exploits subzone volcanic rocks of the Miguasha-Est no. 1 well implies that the Red Indian Line must pass through the southern Gaspé Peninsula, beneath the thick sedimentary cover sequences (Fig. 1). The inferred location and setting of the new terrane, bound to the north by the Grand Pabos fault and to the south by the Red Indian Line, are similar to that of the Annieopsquotch accretionary tract in Newfoundland.
| CONCLUSIONS |
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Igneous clasts in conglomerates of the Upper Ordovician Garin Formation, the basal unit of the middle Paleozoic Gaspé belt in the Gaspé Appalachians of Québec, are undeformed and were affected solely by low-grade hydrous metamorphism, which confirms that the source area was not the Laurentian margin affected by Taconian deformation, but the Iapetus oceanic domain. Igneous clasts define three populations, all of which can be related to the post-Taconian tectonic evolution of the Dunnage oceanic tract during Ordovician time.
(1) The calc-alkaline intermediat-felsic suite has signatures typical of continental arc magmas. Variations in HREE abundances allow two subgroups to be defined. (1a) HREE-poor monzonite and rhyolite are geochemically most similar either to volcanic rocks of the Meductic Group (Exploits subzone, New Brunswick, 480–473 Ma), or to igneous rocks of the Red Indian Lake Group (Notre Dame subzone, Newfoundland, 465–460 Ma). U-Pb zircon ages of 465–466 Ma for HREE-poor Garin pebbles preclude correlation with the Meductic Group and suggest derivation from igneous rocks similar to the Red Indian Lake Group or from equivalent rocks at the latitude of Gaspé. Hence, based on geochemical similarities and geochronological ages, clasts of the calc-alkaline intermediat-felsic suite in the Garin Formation are interpreted to record the calc-alkaline magmatism of a Llanvirn peri-Laurentian continental arc. (1b) HREE-rich andesites and rhyolites can be correlated with volcanic rocks of the Andean-type Popelogan arc (Exploits subzone), or with rocks derived from magmas formed by melting of this crust during Gander margin continental extension. However, they also correlate well with granitic rocks of the McCrea mélange from the Notre Dame subzone of the Gaspé Peninsula. Given the spatial association with HREE-poor clasts, we favor a Notre Dame subzone provenance.
(2) Mafic rocks of the tholeiitic-to-alkaline suite have enriched geochemical signatures typical of within-plate settings, a minor continental crustal contamination component, and they resemble tholeiites and alkaline basalts of the Tetagouche and California Lake Groups (New Brunswick) and alkaline basalts of the Winterville Formation and Stacyville volcanics (Maine). They are interpreted to record magmatism associated with the rifting and initiation of an embryonic back-arc basin, but we cannot be certain of their provenance.
(3) Rocks of the mafic-intermediate suite have geochemical signatures that are common in oceanic arcs and back-arcs. Rocks of this suite are similar to mafic rocks of the Exploits subzone in northern New Brunswick and Maine, but they correlate best with mafic to intermediate rocks of the Notre Dame subzone in the Gaspé Peninsula and in Newfoundland. They are interpreted to represent the products of spreading and off-axis magmatism in a peri-Laurentian back-arc basin.
Igneous clasts within the Upper Ordovician Garin Formation are therefore interpreted to have been eroded from a predominantly weakly or unmetamorphosed arc coeval with development of the Red Indian Lake Group of Newfoundland (Notre Dame subzone) that is only exposed at the latitude of the Gaspé Peninsula in the McCrea mélange.
The correlation between volcanic rocks of the Miguasha-Est no. 1 well in Gaspé with arc volcanic rocks of the Popelogan inlier (New Brunswick) along strike suggests that rocks of the Exploits subzone extend across Chaleurs Bay to the Gaspé Peninsula, but they are now buried beneath the Middle to Upper Paleozoic sedimentary cover sequence. This implies that the Red Indian Line passes through the southern Gaspé Peninsula. The inferred position of the Red Indian Line in the Gaspé Peninsula is similar to what is observed in Newfoundland, where volcanic rocks of the McCrea mélange occur on the Laurentian side and those of the Balmoral Group occur in the Popelogan inlier on the Gondwanan side. The data presented in this paper provide evidence that Newfoundland's geological template may continue into the Québec Appalachians and beyond (New England).
| APPENDIX 1. GEOCHEMICAL ANALYTICAL METHODS |
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| APPENDIX 2. AR-AR GEOCHRONOLOGY |
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Laser 40Ar/39Ar step-heating analysis was carried out at the Geological Survey of Canada (GSC) laboratories in Ottawa, Ontario. Upon return from the reactor, samples were split into two aliquots and loaded into individual 1.5-mm-diameter holes in a copper planchet, where each was run as a separate step-heating experiment. Heating of individual sample aliquots in steps of increasing temperature was achieved using a Merchantek MIR10 10W CO2 laser equipped with a 2 mm x 2 mm flat-field lens. The released Ar gas was cleaned over getters for 10 min and then analyzed isotopically using the secondary electron multiplier system of a VG3600 gas source mass spectrometer; details of data collection protocols can be found in Villeneuve and MacIntyre (1997) and Villeneuve et al. (2000). Error analysis on individual steps follows numerical error analysis routines outlined in Scaillet (2000); error analysis on grouped data follows algebraic methods of Roddick (1988).
Corrected argon isotopic data are available in the GSA Data Repository (see footnote 1) and are presented (Fig. 9) as spectra of gas release and on inverse-isochron plots (Roddick et al., 1980). Each gas-release spectrum plotted contains step-heating data from up to two aliquots, alternately shaded and normalized to the total volume of 39Ar released for each aliquot. Such plots provide a visual image of replicated heating profiles, evidence for Ar-loss in the low-temperature steps, and the error and apparent age of each step.
Neutron flux gradients throughout the sample canister were evaluated by analyzing the sanidine flux monitors included with each sample packet and interpolating a linear fit against calculated J-factor and sample position. The error on individual J-factor values is conservatively estimated at ±0.6% (2
). Because the error associated with the J-factor is systematic and not related to individual analyses, correction for this uncertainty is not applied until calculation of dates from isotopic correlation diagrams (Roddick, 1988). Blanks were measured prior and after each aliquot and levels vary between 40Ar = 2.5–3.6 x 10–7 nm, 39Ar = 4.2–13.3 x 10–9 nm, 38Ar = 0.4–1.7 x 10–9 nm, 37Ar = 0.41.7 x 10–9 nm, 36Ar = 0.7–1.3 x 10–9 nm, all at ±10% uncertainty. Nucleogenic interference corrections are (40Ar/39Ar)K = 0.025 ± 0.005, (38Ar/39Ar)K = 0.011 ± 0.010, (40Ar/37Ar)Ca = 0.002 ± 0.002, (39Ar/37Ar) Ca = 0.00068 ± 0.00004, (38Ar/37Ar)Ca = 0.00003 ± 0.00003, and (36Ar/37Ar)Ca = 0.00028 ± 0.00016. All errors are quoted at the 2
level of uncertainty.
| APPENDIX 3. U-PB GEOCHRONOLOGY |
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external errors of 206Pb/238U ratios reported in Table DR4 incorporate a ±1.7% error in calibrating the standard zircon (see Stern and Amelin, 2003). An age of 416.4 ± 4.1 Ma was determined for the Temora standard, during this analytical session, within error of its accepted age. Isoplot v. 3.01 (Ludwig, 2001) was used to generate concordia plots and calculate ages. All data points plotted in the figures have errors reported at the 2
uncertainty level. Complete data are available in the GSA Data Repository (see footnote 1)
Results
Sample RJ-27: Monzonite
Zircon in this sample dominantly consists of prismatic euhedral grains with moderate oscillatory zoning typical of igneous growth, and no evidence of inherited core material. The U concentrations vary from ~300 to 1000 ppm, with relatively high Th/U ratios ranging from 0.6 to 2.0. The compositions are consistent with the interpretation of a simple zircon population, and the relatively high Th/U ratios are consistent with the rock composition. Seventeen grains were analyzed. All of the analyses cluster and define a concordia age of 466 ± 4.7 Ma (2
, decay-constant errors included; mean square of weighted deviates [MSWD] of concordance = 3.3; probability of concordance = 0.07). This is interpreted as the crystallization age of the monzonite.
Sample RLH-87: Porphyritic Rhyodacite/Dacite
Zircon in this sample is dominated by euhedral prismatic morphologies, with prominent oscillatory zoning. Eighteen zircon grains were analyzed, 15 of which define a concordia age of 465.2 ± 4.9 Ma (2
, decay-constant errors included; MSWD of concordance = 0.23; probability of concordance = 0.63). This is interpreted as the crystallization age of the porphyritic rhyodacite/dacite. Uranium content of these zircons ranges from 108 to 360 ppm (Table DR4). Two grains have significantly higher uranium content (1100–2100 ppm) and older 206Pb/238U ages of 482 and 492 Ma. These grains are interpreted to be inherited and were excluded from the age calculation. One analysis (9015–28.1) has a slightly younger 206Pb/238U age, possibly due to Pb loss, and it was also excluded from the age calculation.
| ACKNOWLEDGMENTS |
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RECEIVED FOR PUBLICATION April 19, 2007
REVISED MANUSCRIPT RECEIVED April 4, 2008
MANUSCRIPT ACCEPTED April 15, 2008
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