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Revista geológica de Chile

versión impresa ISSN 0716-0208

Rev. geol. Chile v.28 n.1 Santiago jul. 2001

http://dx.doi.org/10.4067/S0716-02082001000100005 

Late Triassic detrital zircons in meta-turbidites of the Chonos
Metamorphic Complex, southern Chile

Francisco Hervé
Departamento de Geología, Universidad de Chile, Casilla 13518,
Correo 21, Santiago, Chile
fherve@cec.uchile.cl

C. Mark Fanning
Research School of Earth Sciences, The Australian National University,
Canberra, ACT 0200, Australia.

ABSTRACT

Sensitive High Resolution Ion MicroProbe (SHRIMP) U-Pb age determinations of detrital zircons from metasandstones of the Chonos Metamorphic Complex reveal a significant population of Late Triassic ages. One of the samples is immediately underlying the coquinaceous bed containing fossils which were initially identified as Late Silurian-Early Devonian, and more recently as Late Triassic faunas. The zircon data confirm the latter age as the depositional age of the fossil bearing rocks, excluding completely the possibility of a Paleozoic depositional age. Similar U-Pb detrital zircon ages are recorded in two other samples, one of which was collected in the vicinity of strata containing Lima sp., confirming that a Late Triassic depositional age is widespread in the Eastern belt of the Chonos Metamorphic Complex. However, in a fourth sample, the youngest detrital zircons are Carboniferous in age. Construction of the accretionary prism was thus active in the Late Triassic, and its metamorphism probably took place during the Jurassic, in contrast with a previously accepted Late Paleozoic age.

Key words: Late Triassic, U-Pb ages, Chonos Metamorphic Complex, Southern Chile.

RESUMEN

Circones detríticos del Triásico tardío en metaturbiditas del Complejo Metamórfico Chonos, sur de Chile. Las edades U-Pb de circones detríticos, obtenidas con el SHRIMP en metareniscas del Complejo Metamórfico de Chonos, revelan una abundante población de circones con edades correspondientes al Triásico Superior. Una de las muestras proviene del estrato que se ubica inmediatamente bajo la capa coquinácea con fósiles que inicialmente otros autores asignaron al Silúrico Superior-Devónico Inferior, y recientemente al Triásico Superior. Las edades de circones detríticos concuerdan totalmente con esta última, y eliminan la posibilidad de una edad paleozoica de deposición de las rocas fosilíferas. Otras dos muestras, una de las cuales proviene de las vecindades de un estrato que contiene Lima sp., dan resultados similares, lo que indica que esta edad de deposición tiene amplia distribución en la franja oriental del Complejo Metamórfico de los Chonos. En cambio, en una cuarta muestra la edad más joven de circones detríticos es carbonífera. La construcción del prisma de acreción estaba activa en el Triásico Superior, y su metamorfismo tuvo lugar, probablemente, durante el Jurásico, contrariamente a la edad paleozoica superior que se le asignaba hasta ahora.

Palabras claves: Triásico tardío, Edades U-Pb, Complejo Metamórfico Chonos, Sur de Chile.

INTRODUCTION

The Chonos Metamorphic Complex (CMC) is part of an accretionary complex which crops out as a continuous belt in the coastal area of Chile from Pichilemu (34°S) to the Taitao Peninsula (47°S), and discontinuously from there to the southernmost tip of South America.

The time frame proposed for the evolution of the low grade Chonos Metamorphic Complex (Davidson et al., 1987), and for all the accretionary complex (e.g., Hervé, 1988), has been strongly influenced by the identification by Miller and Sprechmann (1978) of a Late Silurian-Early Devonian fossil fauna in a coquinaceous metaturbidite bed in the southern end of Isla Patranca and in a small unnamed islet 5 km to the north. These fossiliferous localities, unique within the whole complex, were re-examined by Fang et al. (1998) who identified more recently collected fossil specimens as a Late Triassic Monotis species in Isla Patranca (named Potranca in Miller and Sprechmann, 1978) and Lima sp., of a Permian to Triassic age range.

The Chonos Metamorphic Complex has been studied previously by Miller (1979) and Hervé et al. (1981). Detailed field and structural studies led Miller (1979) to recognize three stratigraphic units, the Canal King, Potranca and Canal Pérez Sur informal formations, interpreted to be progressively younger successions, separated by unconformities. However, the three units share a common structural grain, characterized by northwest trending fold axes and stretching lineations. The fossil assemblages noted above occur in the middle Potranca formation, which was assigned to the Late Silurian-Early Devonian. It follows that the underlying Canal King formation is older and that the overlying Canal Pérez Sur formation is younger.

In an alternative view, Hervé et al. (1981) distinguishes an Eastern belt* where primary sedimentary structures are preserved, which grades into a Western belt where all primary structures have been lost due to increasing deformation and metamorphism. This interpretation is based on both structural continuity and a progressive increase in metamorphic grade from one belt to the other. The Eastern belt is considered to have a Devonian protholith, and be composed of the Patranca facies and the Teresa facies, roughly equivalent to the Potranca and Canal Pérez Sur formations of Miller (1979), respectively. Davidson et al. (1987) presented Rb-Sr whole rock ages of ca. 220 Ma on slates from the Eastern belt which were interpreted as the age of the D2 metamorphic episode in the complex. They presented Rb-Sr errorchron data on the schists from the Western belt of ca. 140 Ma and ca. 168 Ma which they interpreted as indicating a Jurassic 'reactivation' of the subduction complex.

Willner et al. (2000) have shown that the metamorphism within the Eastern belt of the Chonos Metamorphic Complex took place under peak P-T conditions of 5.5 Kbar and 250-280°C and 8-10 Kbar and 380-500°C in the Western belt. These rather high P-T gradients are in accordance with a subduction zone environment of metamorphism.

The purpose of this paper is to present the results of SHRIMP U-Pb age determinations for detrital zircons from rocks of the fossiliferous unit. These results elucidate the contradiction between the two previously published paleontological age interpretations and they establish constraints on the age of deposition and metamorphism of the Potranca formation in the Chonos Metamorphic Complex.

SAMPLES AND METHODOLOGY

Three metasedimentary rock samples of the turbiditic unit (Potranca formation or Patranca facies of the Eastern belt) which contain the fossiliferous strata in the Chonos Metamorphic Complex were collected for U-Th-Pb dating of zircon by SHRIMP (Sensitive High Resolution Ion MicroProbe) at The Australian National University. An additional metasedimentary rock from the Teresa facies (Canal Pérez Sur formation ) was also analysed. Zircons were separated using standard crushing, heavy liquid and Frantz isodynamic methods. Grains from the total zircon population were sprinkled onto double sided tape and cast in an epoxy disk together with the Duluth Gabbro reference zircon, AS3 (see Paces and Miller, 1993). The ion microprobe procedures used essentially follow those given in Compston et al. (1992) and Williams (1998). The U/Pb ratios have been calibrated relative to the AS3 zircons, which have an age of 1099 Ma (Paces and Miller, 1993).One spot was analyzed in each crystal, unless specified in the tables by a number of the form n.2, usually in the outer rim.

The age spectra of individual rock units can be used to obtain an inferred maximum depositional age of the original sediments; the depositional age can be no older than the youngest concordant U-Pb zircon age. Where a number of analyses (from different grains) have the same radiogenic 206Pb/238U ratios to within analytical uncertainty, weighted mean ages have been calculated and those are reported, with uncertainties given at the 95% confidence level.

All samples analysed belong to the Eastern Belt of the Chonos Metamorphic Complex. Their location is indicated in figure 1.

CE9603 is a metasandstone with L-tectonite fabric reflecting the intersection of two cleavages in northwest direction. It was collected from a turbidite succesion devoid of fossils.

FO9606 is a medium grained metasandstone with convolute bedding. It was collected near the southern end of Isla Patranca, from an horizon immediately underlying the coarse grained fossil bearing coquinaceous bed from which Miller and Sprechman (1978) and Fang et al. (1998) have identified Late Silurian-Early Devonian and Late Triassic fossils respectively. The coquinaceous bed from this location shows clear indications of having previously been sampled. The authors, therefore, believe that this coquinaceous bed was sampled to produce the Miller and Sprechman (1978) fossils, and the authors know with absolute certainty that this is the location described in Fang et al. (1998) since the material was collected by the senior author. The contact between the metasandstone sampled for this U-Pb zircon study and the coquinaceous bed used for the fossil age determinations is of normal conformable sedimentary nature.

CE9625 is a low grade fine grained metaconglomerate collected in the islet where Lima sp. was identified by Fang et al. (1998). Continuous slate beds form only 5% of the succesion, which is mainly composed here by turbidites with sole marks, dewatering structures, convolute bedding and rip clasts of shale. The rocks are cleaved and have a northwest lineation.

FO9640 is a fine grained metasandstone from the southeastern corner of Isla Yechica, where an inverted succession of turbidites with interbedded banded cherts crops out. Beds are typically 0.5 m thick, bioturbated, and with a subhorizontal tectonic lamination, axial planar to ENE folds of the stratification.

GEOCHRONOLOGICAL RESULTS

The SHRIMP U-Pb detrital zircon results for the samples CE9603, FO9606 and CE9625 (Patranca facies or Potranca formation) are presented in tables 1-4, p. 101-104 . The results for sample FO9640 (Teresa facies or Canal Pérez Sur formation) are presented in table 4. The data are shown on the Tera-Wasserburg diagrams in figure 2, and on relative probability plots in figure 3, respectively.

The three samples of the Potranca facies record similar results, with a wide range of ages. The age spectra are complex revealing multiple source provenance for the detrital zircon grains.

However, some common aspects between the samples can be highlighted:

• Most of the zircons are igneous in origin, they have euhedral to subhedral outlines and cathodoluminescence (CL) images of the sectioned grains show well developed, simple magmatic zoning.

• The youngest zircon analysis in each sample, with isotopic ratios plotting within uncertainty of the Tera-Wasserbug concordia, are ca. 210 Ma (212, 216 and 208 Ma, respectively). There are few analyses which are younger, however these are discordant and so the ages are not considered to necessarily represent the time of crystallisation of the zircons. The youngest concordant ages form a grouping at ca. 220 Ma in all three samples.

• Most (>80%) of the zircons analysed are Paleozoic in age, and they show a complex distribution with age peaks (Figs. 1b, 2b, 3b) at ca. 280 Ma, at 330-350 Ma, at 400 Ma, with very few zircons between 400 and 530 Ma, and a further peak at ca. 550 Ma.

• Proterozoic zircons are scarce, they are mainly concentrated in the 1300-1600 Ma age range, and are absent at 800±50 Ma.

• Only two Late Archean and/or Paleoproterozoic zircons are present in one of the samples.

The results for sample F09640 (from the Teresa facies or Canal Pérez Sur formation) differ quite substantialy from the above. The younger datefor detrital zircons in this sample is 336±5 Ma (Early Carboniferous), and the proportion of Proterozoic grains is larger than in the three previous samples. Two Archean grains are present.


FIG. 1. Geologic sketch map of the Chonos Archipelago region, with indication of geologic units as in Davidson et al. (1987) and location of the analysed samples.


FIG. 2. Tera and Wasserburg (1972) concordia diagrams for a- sample CE9603; b- sample FO9606; c- sample CE9625, and d- sample CE9640. The calibrated 238U/206Pb ratios versus the total 207Pb/206Pb ratios have been plotted as one sigma error ellipses. Note that an analysis that is not within uncertainty of the concordia curve may not necessarily signify a discordant analysis. It may simply reflect that a significant amount of common Pb has been detected in that analysis. The U/Pb isotopic data are given in the tables as both uncorrected and 207Pb corrected radiogenic ratios (see Compston et al., 1992).


 

FIG. 3. Age versus probability diagrams for a- sample CE9603; b- sample FO9606; c- sample CE9625, and d- sample F09640. The relative probability curve takes into account the age and age uncertainty for each analysis. The stacked histogram indicates the number of analyses that contribute to the various peaks in the relative probability curve.

DISCUSSION AND CONCLUSIONS

The U-Pb SHRIMP zircon age data obtained in this study strongly support the Late Triassic (Late Norian) depositional age determination made by Fang et al. (1998) based on the study of fossils in the Chonos Metamorphic Complex, and is in contradiction with the previously proposed Late Silurian-Early Devonian age by Miller and Sprechmann (1978). The fact that three samples from the same unit (the Potranca ormation or Patranca facies) of the Chonos Metamorphic Complex show similar minimum ages indicates that the Late Triassic rocks are extensive and not simply restricted to the fossiliferous localities.

The coincidence between the radioisotopic zircon ages and the biostratigraphic depositional ages (Gradstein and Ogg, 1996) is remarkable, and probably indicates that active magmatism was ocurring in the provenance area of the turbidite sequence during their deposition.

This provenance area is almost instinctively looked for in Patagonia, to the east of the analysed samples. However, in the Chilean slope of the Andes, igneous rocks of Late Triassic age are not known. A few granitic bodies of Late Triassic age do exist in the North Patagonian Massif (Cingolani et al., 1992), hundreds of kilometers inland from the location of the Chonos Archipelago. A Carboniferous magmatic arc in the Lake District of Chile, was exhumated and eroded previously to the Late Triassic (Martin, 1999). Also, the Mesoproterozoic and Late Proterozoic zircons, might have come from the presently covered basement of Patagonia, or they may be far travelled grains coming from the Namaquan belts of southern Africa, which was side by side to Patagonia in the Late Triassic.

Another possible source area for the detrital material is the Antarctic Peninsula (Fig. 4), whose exact position in the Early Mesozoic is not well known, but that in recent paleogeographic reconstructions, is located with its northern tip near the present latitude of the Golfo de Penas (47°S) (Lawver et al., 1998). Turbidites of Norian age in the Trinity Peninsula Group occur near the northern tip of the Antarctic peninsula interbedded with acid volcanic rocks in the Legoupil Formation (Thomson, 1975). Early Triassic turbidites occur in the Myers Bluff Formation of Livingston Island (Willan et al., 1994). Various detrital zircon age population diagrams have been published by Löske et al. (1985) which give strong evidence for Carboniferous and Late Proterozoic source regions.

The confirmation of the Late Triassic depositional age for at least a significant part of the Chonos Metamorphic Complex, implies that its metamorphism took place during the Mesozoic or Cenozoic. However, this metamorphism was probably Jurassic, as the Chonos Metamorphic Complex was intruded by the Early Cretaceous components of the North Patagonian Batholith (Pankhurst et al., 1999), when it had already acquired its main structural charateristics. Also, Thomson et al. (2000) combining some of the SHRIMP data presented here and Fission Track age determinations conclude that the metamorphism in the CMC took place in the Early Jurassic. This allows a more confident interpretation of the Late Triassic to Jurassic Rb-Sr age data on rocks of the same unit (in Hervé, 1988) as related to the metamorphism or Early diagenesis of the complex.


FIG. 4. Part of the tight fit paleogeographic reconstruction of Gondwana at 200 Ma (after Lawver et al., 1998), showing that the present location of the Chonos Metamorphic Complex is just north of the tip of the Antarctic Penisula in the Triassic-Jurassic boundary times.

However, the structurally homogeneous rock units within this metamorphic complex are not necessarily time-restricted depositional units. For example, the metaturbidite from the Teresa facies (Davidson et al., 1987) of the Eastern Belt has given a detrital zircon age spectra which differs from those of the Patranca facies, in that the younger concordant zircon is 336 Ma, and the age versus probability pattern is different. They may represent older deposits.

The geographic and lithologic continuity of the Chonos Metamorphic Complex with the Paleozoic Metamorphic Complex of the Coastal Range of southcentral Chile and of the Chiloé island must now be considered carefully. The consequences of the data presented herein lead to significant changes in the interpreted age of deposition and metamorphism of the so-called Paleozoic basement rocks that previously had been considered on the basis of lithological (structural and metamorphic) criteria to form a simple single 'basement' package. Recent work by Duhart et al. (1997, 1999); and by Martin et al. (1999) in the Lake district of southern Chile, have documented that the Western Series of the paleozoic metamorphic basement includes sedimentary components younger than Early Permian. These same authors indicated that a regional cooling between 220 and 250 Ma is registered in the metamorphic complex, and that it took place after the main deformation and metamorphic event. Söllner et al. (2000) reported the presence of Late Carboniferous-Early Permian acid volcanic rocks in the 'basement' near Puerto Montt.

The Late Triassic turbidites of the Chonos Metamorphic complex dated here, are time equivalent to the Panguipulli Formation of the lake district, but the latter, which sits uncomformably over the metamorphic basement, has not experienced the high P/T metamorphism recorded in the CMC. So, the studied rocks were involved in deep subduction during the Late Triassic-Early Jurassic, which took place beneath the western continental margin of Gondwana while the Panguipulli rocks remained on the upper plate near the surface. In the Lake Region. Martin et al. (1999) suggested that the Western Series and the Late Carboniferous magmatic arc were exposed after the middle Permian to Middle Triassic exhumation and that initial transpressional deformation of the subduction-arc complex associated with an event of dextral oblique convergence along the margin took place during the Late Triassic-Early Jurassic. This scenario is based on structural observations on the rocks of the Western Series, and on previous paleomagnetic studies (Forsythe et al., 1987) indicating northward translation of portions of the Coast Range, now situated near 30°S during Late Triassic to Late Jurassic. It is interesting to note here that starting in the Early Jurassic, the Antarctic Peninsula migrated southward, with a sinistral movement along the margin of Gondwana after the paleogeographic reconstructions (Scotese, 1997). The Chonos area is thus a portion of the margin where continental margin parallell strike slip movements during the Late Triassic to Early Jurassic seem to diverge, in a way similar to what would be expected when the subduction of a rise or indenter, beneath the continental margin occurs.

The oblique subduction which occurred in the area (Martin et al., 1999) during the Late Triassic-Early Jurassic, together with a low subduction angle, could have resulted in the paucity of the production of magmatic rocks observed during this interval. The most conspicuous contemporaneous arc-like igneous complex is the Sub-cordilleran batholith (Haller et al., 1999) in the eastern slope of the present Andes, which might be genetically related to the subduction event giving rise to the Chonos Metamorphic Complex.

It seems clear that the metamorphic basement of southern Chile certainly includes rocks varying widely in ages of deposition and metamorphism, which otherwise are very similar in structure and metamorphic mineralogy. Precise dating of deposition and metamorphism is a needed basis for understanding its evolution.

ACKNOWLEDGEMENTS

Professor H. Miller (University of München) generously indicated the precise location of the fossil bearing localities he discovered in the 70's, which would have been impossible to relocate otherwise in the maze of islands which compose the Chonos Archipelago. R.J. Pankhurst (British Antarctic Survey), A. Demant (Université d'Aix-Marseille III), A. Willner (Ruhr Universität), H. Massone (Stuttgart Universität), C. Pimpirev (Bulgarian

Antarctic Institute) and V. Muñoz (Universidad de Chile) collaborated in the field work. Thorough reviews by H. Miller (München University), M. Martin (Massachussets Institute of Technology) and U. Cordani (Universidad de Sao Paulo) helped to improve the manuscript. This study was funded by Fondecyt Projects 1980741/1010412 and Cátedra Presidencial de Ciencias to FH. It is a contribution to IGCP Project 436 'Pacific Gondwana Margin'.

_______________

Notas:

* The terms Eastern and Western belts as used here should not be confused with the terms Western and Eastern Series, terminology that has been the formal nomenclature since Aguirre et al. (1972), used with the accretionary complex north of Chiloé and more recently by Martin et al. (1999), for rocks found between 38 and 41°S.

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Manuscript received: September 8, 2000; accepted: June 1, 2001.

 

 

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