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ARTICLE in PRESS + MODEL GR-00181; No of Pages 15 ARTICLE IN PRESS + MODEL GR-00181; No of Pages 15 Gondwana Research xx (2007) xxx–xxx 1 www.elsevier.com/locate/gr 2 Foreland basin deposits associated with Cuyania accretion in 3 La Pampa Province, Argentina ⁎ F 4 Carlos J. Chernicoff a,b, , Eduardo O. Zappettini b, João O.S. Santos c,d, 5 Eloise Beyer e, Neal J. McNaughton c 6 a Council for Scientific and Technical Research (CONICET), Julio A. Roca 651, 1322 Buenos Aires, Argentina 7 b Argentine Geological-Mining Survey (SEGEMAR), Julio A. Roca 651, 1322, Buenos Aires, Argentina 8 c University of Western Australia, 35 Stirling Highway, 6009 Perth, Australia 9 d Redstone Resources, 110–116 East Parade, 6004 Perth, Australia 10 e GEMOC, Department of Earth and Planetary Sciences, Macquarie University, Herring Road, North Ryde, Sydney, NSW 2109, Australia 11 Received 13 March 2007; received in revised form 10 April 2007; acceptedPROO 16 April 2007 12 Abstract 13 In the province of La Pampa, south-central Argentina, adjacent to the Cuyania–Pampia terrane boundary, a Late Ordovician–Devonian marine 14 foreland basin generated after the Middle Ordovician (Darriwilian) collision of Cuyania has been recognised, and is herein referred to as the 15 Curacó basin. This basin was formed on crust of the Cuyania terrane, immediately to the west of the Pampia terrane. Its fill primarily comprises 16 sandstones and shales of the La Horqueta Formation, unconformably overlain by Permian continental sediments (Carapacha Formation). The 17 extent of the Curacó basin is investigated using aeromagnetic data; its depocentre is conspicuously delineated by a narrow NNW-orientated 18 magnetic low. In addition, scarce outcrops assigned to the same sequenceCTED are found on the Pampian continental crust, about 50 km to the east, in 19 the proximity of the Valle Daza estate (Valle Daza sub-basin). The studied marine sequence of La Pampa is equivalent to other Lower to Middle 20 Paleozoic units of the eastern margin of the Cuyania terrane and is clearly distinguished from the overlying Permian continental sedimentary 21 sequence. U–Pb SHRIMP dating of detrital zircons from Valle Daza indicates a maximum deposition age of ca. 466 Ma; the minimum age is 22 given by the intrusion of granites at ca. 405 Ma (i.e. Early Devonian). Geochemical data indicate that the Curacó basin was primarily sourced by 23 an active continental margin, possibly the Ordovician Famatinian arc. 24 © 2007 International Association for Gondwana Research. Published by Elsevier B.V. All rights reserved. 25 26 Keywords: Paleozoic marine foreland basin; Curacó basin; La Horqueta Formation; La Pampa province; U–Pb SHRIMP; Hf isotopes 27 ORRE 28 1. Introduction boundaries were defined by Chernicoff and Zappettini (2003, 34 2004a). The origin of the Cuyania terrane from Laurentia (e.g. 35 29 The basement of central La Pampa province, south-central Ramos, 2004; Vujovich et al., 2004a, Porcher et al., 2004, and 36 30 Argentina (Fig. 1), comprises the southern portion of the references therein) or as a para-autochthonous part of Gond- 37 31 Cuyania and PampiaUNC terranes, amalgamated to the western wana (e.g. Aceñolaza et al., 2002; Finney et al., 2003) remains a 38 32 margin of Gondwana during the Middle Ordovician and Cam- matter of debate in the geological community. 39 33 brian times, respectively (Astini et al., 1996); their precise Adjacent to the Cuyania–Pampia terrane boundary, the 40 depocentre of a Late Ordovician–Devonian foreland basin gen- 41 ⁎ Corresponding author. Council for Scientific and Technical Research erated after the Middle Ordovician collision of Cuyania was 42 (CONICET), Julio A. Roca 651, 1322 Buenos Aires, Argentina. Tel.: +54 11 recently identified (Chernicoff and Zappettini, 2003, 2004a,b, 43 4349 3148; fax: +54 11 4349 3171. 2005a,b). This basin, herein referred to as the Curacó basin, was 44 E-mail addresses: [email protected] (C.J. Chernicoff), 45 [email protected] (E.O. Zappettini), [email protected] deposited on Cuyanian crust (Cuyania terrane) immediately to (J.O.S. Santos), [email protected] (E. Beyer), the west of the Pampia terrane. Its fill primarily comprises 46 [email protected] (N.J. McNaughton). sandstones and shales of the La Horqueta Formation, which is 47 1342-937X/$ - see front matter © 2007 International Association for Gondwana Research. Published by Elsevier B.V. All rights reserved. doi:10.1016/j.gr.2007.04.006 Please cite this article as: Chernicoff, C.J. et al. Foreland basin deposits associated with Cuyania accretion in La Pampa Province, Argentina. Gondwana Research (2007), doi:10.1016/j.gr.2007.04.006 ARTICLE IN PRESS 2 C.J. Chernicoff et al. / Gondwana Research xx (2007) xxx–xxx PROOF ED Fig. 1. Locality map of study region (rectangle in Curacó basin depocentre and greater study area, La Pampa province) and surrounding provinces of south-central Argentina. Sample MG40 collected at Valle Daza. 48 unconformably overlain by Permian continental sediments 2. Geological evidence 75 49 (Carapacha Formation). In addition, scarce outcrops assigned 50 to the same sequence are found on the Pampian continental The major discrepancy concerning the age and setting of the 76 51 crust, about 50 km to the east, in the proximity of the ValleRECT Daza Paleozoic sediments of central La Pampa referred to above has 77 52 estate (Valle Daza sub-basin). Drill-hole information also indi- now been resolved as a result of new field observations, com- 78 53 cates the occurrence of buried Siluro-Devonian sandstones in bined with geochronological, petrographical, geophysical and 79 54 the eastern part of La Pampa province (unpublished data of the geochemical studies. The new data has indicated the presence of 80 55 Geological and Mining Survey of Argentina). two unrelated sedimentary units separated by an unconformity. 81 56 In the past, the bulk of the Paleozoic sediments of central La These units are: 82 57 Pampa (i.e. Upper Ordovician–Devonian plus Permian) were 58 undifferentiated and attributed to a single-age and single-origin 1) A lower sequence, of Late Ordovician–Devonian age, 83 59 unit, then regarded as a single formation. This was first defined composed of grayish green mudstones and sandstones 84 60 as a Siluro-Devonian marine sequence named the Carapacha (Fig. 3a), is herein referred to the La Horqueta Formation 85 61 Formation (Vilela and Riggi, 1956), bearing Late Silurian bra- (in the sense of Baldis and Peralta, 1999). This unit was 86 62 chiopods (Sgrosso, in Tapia, 1939). Criado Roqué (1972) cor- affected by low-grade regional metamorphism. The eastern 87 63 related this unit with theUNCOR La Horqueta Formation (exposed outcrops at Valle Daza estate and surroundings show the 88 64 further north, in the San Rafael block of the Cuyania terrane); effect of thermal metamorphism related to the intrusions of 89 65 Linares et al. (1980) followed this assignment. Devonian granitoids (e.g. Chacharramendi granite). Other- 90 66 However, the discovery of a Permian flora of Glossopteris in wise, the La Horqueta Formation is a unit mostly exposed 91 67 a number of exposures in the Puelches area of La Pampa further north, in the San Rafael Block of the Cuyania 92 68 (Terraza, 1981; Terraza et al., 1982; Schultz, 1986; Melchor and Terrane. 93 69 Césari, 1991) led to the redefinition of the whole, undifferen- 2) An upper sequence, composed of reddish gray conglomer- 94 70 tiated Paleozoic sedimentary sequence as constituting a con- ates and sandstones (Fig. 3b), with minor limestones and 95 71 tinental Lower Permian unit (Melchor, 1995, 1999). Fig. 2 pelites bearing a flora of Glossopteris. The term Carapacha 96 72 shows the key outcrop sites of the La Horqueta Formation at the Formation (Vilela and Riggi, 1956) is herein restricted to this 97 73 Curacó basin depocentre, near Puelches, also showing the key upper sequence, of Permian age. Notably, the conglomerates 98 74 outcrop sites of the overlying Carapacha Formation. of the upper sequence (Carapacha Formation) bear sandstone 99 Please cite this article as: Chernicoff, C.J. et al. Foreland basin deposits associated with Cuyania accretion in La Pampa Province, Argentina. Gondwana Research (2007), doi:10.1016/j.gr.2007.04.006 ARTICLE IN PRESS C.J. Chernicoff et al. / Gondwana Research xx (2007) xxx–xxx 3 biotite–albite–titanite, indicating greenschist facies metamor- 116 phism. The alignment of biotite points to an incipient schis- 117 tosity. The pelites contain very scarce angular lithic grains of 118 volcanic rocks (partly replaced by calcite) and monomineralic 119 grains of quartz, ranging 0.053–0.25 mm in size; they also, 120 though rarely, contain grains of microcline, zircon and de- 121 formed muscovite. The matrix is argillaceous, largely recrys- 122 tallized to illite. 123 SWIR reflectance spectrometry studies were applied to the 124 sandstones, resulting in the identification of ammonium-illite, 125 as well as chamosite and sheridanite, the latter two minerals 126 being iron and magnesium chlorites, respectively. Ammonium- 127 illite is indicative of the presence of organic matter (Williams 128 and Ferrell, 1991). The occurrence of chamosite points to a 129 shallow marine environment (e.g. Hallam and Bradshaw, 1979; 130 Van Houten and Purucker, 1984; Schieber and Riciputi, 2004). 131 Chamosite is known to be typical of marine deposits in 132 Argentina of the same age range as the La Horqueta Formation, 133 e.g. the Lipeón Formation (Boso and Monaldi, 1999), the Sierra 134 Grande FormationPROOF (Zanettini, 1999), the Don Braulio Forma- 135 tion (Baldis and Peralta, 1999), as well as elsewhere in the 136 world, e.g. the Clinton Formation (Cotter and Link, 1993) and 137 the Red Mountain Formation (Chowns, 2002) in the USA, and 138 the Djebilet Formation in Algeria (Guerrak, 1988).
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