The Role of Inversion Tectonics in the Structure of the Cordillera Oriental (NW Argentinean Andes)
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Late Mesozoic to Paleogene Stratigraphy of the Salar De Atacama Basin, Antofagasta, Northern Chile: Implications for the Tectonic Evolution of the Central Andes
Late Mesozoic to Paleogene stratigraphy of the Salar de Atacama Basin, Antofagasta, Northern Chile: Implications for the tectonic evolution of the Central Andes Constantino Mpodozisa,T,Ce´sar Arriagadab, Matilde Bassoc, Pierrick Roperchd, Peter Cobbolde, Martin Reichf aServicio Nacional de Geologı´a y Minerı´a, now at Sipetrol. SA, Santiago, Chile bDepartamento de Geologı´a, Universidad de Chile, Santiago, Chile cServicio Nacional de Geologı´a y Minerı´a, Santiago, Chile dIRD/Dep. de Geologı´a, Universidad de Chile, Santiago, Chile eGe´osciences-Rennes (UMR6118 du CNRS), France fDepartment of Geological Sciences University of Michigan, United States Abstract The Salar de Atacama basin, the largest bpre-AndeanQ basin in Northern Chile, was formed in the early Late Cretaceous as a consequence of the tectonic closure and inversion of the Jurassic–Early Cretaceous Tarapaca´ back arc basin. Inversion led to uplift of the Cordillera de Domeyko (CD), a thick-skinned basement range bounded by a system of reverse faults and blind thrusts with alternating vergence along strike. The almost 6000-m-thick, upper Cretaceous to lower Paleocene sequences (Purilactis Group) infilling the Salar de Atacama basin reflects rapid local subsidence to the east of the CD. Its oldest outcropping unit (Tonel Formation) comprises more than 1000 m of continental red sandstones and evaporites, which began to accumulate as syntectonic growth strata during the initial stages of CD uplift. Tonel strata are capped by almost 3000 m of sandstones and conglomerates of western provenance, representing the sedimentary response to renewed pulses of tectonic shortening, which were deposited in alluvial fan, fluvial and eolian settings together with minor lacustrine mudstone (Purilactis Formation). -
The Cambrian System in Northwestern Argentina: Stratigraphical and Palaeontological Framework Discussion Geologica Acta: an International Earth Science Journal, Vol
Geologica Acta: an international earth science journal ISSN: 1695-6133 [email protected] Universitat de Barcelona España Buatois, L.A.; Mángano, M.G. Discussion and reply: The Cambrian System in Northwestern Argentina: stratigraphical and palaeontological framework Discussion Geologica Acta: an international earth science journal, vol. 3, núm. 1, 2005, pp. 65-72 Universitat de Barcelona Barcelona, España Available in: http://www.redalyc.org/articulo.oa?id=50530107 How to cite Complete issue Scientific Information System More information about this article Network of Scientific Journals from Latin America, the Caribbean, Spain and Portugal Journal's homepage in redalyc.org Non-profit academic project, developed under the open access initiative Geologica Acta, Vol.3, Nº1, 2005, 65-72 Available online at www.geologica-acta.com Discussion and reply: The Cambrian System in Northwestern Argentina: stratigraphical and palaeontological framework Discussion L.A. BUATOIS and M.G. MÁNGANO CONICET- INSUGEO Casilla de correo 1 (correo central), 4000 San Miguel de Tucumán, Argentina. Present address: Department of Geological Sciences, University of Saskatchewan, 114 Science Place, Saskatoon, SK S7N 5E2, Canada. Buatois E-mail: [email protected] INTRODUCTION this rift corresponds to the early above-mentioned Punco- viscana basin”. This gives the wrong impression that there As part of the Special Issue on “Advances in the is some sort of consensus on this topic, which is incorrect. knowledge of the Cambrian System” edited by himself, Interestingly enough, this southern rift branch is perpendi- Aceñolaza (2003) attempted to summarize present know- cular to the Gondwana Pacific trench (see his figure 3), an ledge on the Cambrian of northwest Argentina. -
Appendix A. Supplementary Material
Appendix A. Supplementary material Comprehensive taxon sampling and vetted fossils help clarify the time tree of shorebirds (Aves, Charadriiformes) David Cernˇ y´ 1,* & Rossy Natale2 1Department of the Geophysical Sciences, University of Chicago, Chicago 60637, USA 2Department of Organismal Biology & Anatomy, University of Chicago, Chicago 60637, USA *Corresponding Author. Email: [email protected] Contents 1 Fossil Calibrations 2 1.1 Calibrations used . .2 1.2 Rejected calibrations . 22 2 Outgroup sequences 30 2.1 Neornithine outgroups . 33 2.2 Non-neornithine outgroups . 39 3 Supplementary Methods 72 4 Supplementary Figures and Tables 74 5 Image Credits 91 References 99 1 1 Fossil Calibrations 1.1 Calibrations used Calibration 1 Node calibrated. MRCA of Uria aalge and Uria lomvia. Fossil taxon. Uria lomvia (Linnaeus, 1758). Specimen. CASG 71892 (referred specimen; Olson, 2013), California Academy of Sciences, San Francisco, CA, USA. Lower bound. 2.58 Ma. Phylogenetic justification. As in Smith (2015). Age justification. The status of CASG 71892 as the oldest known record of either of the two spp. of Uria was recently confirmed by the review of Watanabe et al. (2016). The younger of the two marine transgressions at the Tolstoi Point corresponds to the Bigbendian transgression (Olson, 2013), which contains the Gauss-Matuyama magnetostratigraphic boundary (Kaufman and Brigham-Grette, 1993). Attempts to date this reversal have been recently reviewed by Ohno et al. (2012); Singer (2014), and Head (2019). In particular, Deino et al. (2006) were able to tightly bracket the age of the reversal using high-precision 40Ar/39Ar dating of two tuffs in normally and reversely magnetized lacustrine sediments from Kenya, obtaining a value of 2.589 ± 0.003 Ma. -
A History of Proterozoic Terranes in Southern South America: from Rodinia to Gondwana
+ MODEL GEOSCIENCE FRONTIERS -(-) (2011) 1e9 available at www.sciencedirect.com China University of Geosciences (Beijing) GEOSCIENCE FRONTIERS journal homepage: www.elsevier.com/locate/gsf REVIEW A history of Proterozoic terranes in southern South America: From Rodinia to Gondwana C. Casquet a,*, C.W. Rapela b, R.J. Pankhurst c, E.G. Baldo d, C. Galindo a, C.M. Fanning e, J.A. Dahlquist d, J. Saavedra f a Departamento de Petrologıa y Geoquımica, IGEO (Universidad Complutense, CSIC), 28040 Madrid, Spain b Centro de Investigaciones Geologicas (CONICET-UNLP), 1900 La Plata, Argentina c Visiting Research Associate, British Geological Survey, Keyworth, Nottingham NG12 5GG, United Kingdom d CICTERRA (CONICET-UNC), 5000 Cordoba, Argentina e Research School of Earth Sciences, The Australian National University, Canberra, Australia f Instituto de Agrobiologıa y Recursos Naturales CSIC, 37071 Salamanca, Spain Received 3 August 2011; accepted 8 November 2011 KEYWORDS Abstract The role played by Paleoproterozoic cratons in southern South America from the Mesopro- Paleoproterozoic; terozoic to the Early Cambrian is reconsidered here. This period involved protracted continental amal- Cratons; gamation that led to formation of the supercontinent Rodinia, followed by Neoproterozoic continental Grenvillian; break-up, with the consequent opening of Clymene and Iapetus oceans, and finally continental Neoproterozoic rifting; re-assembly as Gondwana through complex oblique collisions in the Late Neoproterozoic to Early SW Gondwana assembly Cambrian. The evidence for this is based mainly on a combination of precise U-Pb SHRMP dating and radiogenic isotope data for igneous and metamorphic rocks from a large area extending from the Rio de la Plata craton in the east to the Argentine Precordillera in the west and as far north as Arequipa in Peru. -
Mesozoic to Tertiary Evolution of the Southwestern Proto-Pacific Gondwana Margin
University of Sydney, PhD Thesis, Kayla T. Maloney, 2012. The University of Sydney School of Geosciences Mesozoic to Tertiary evolution of the southwestern proto-Pacific Gondwana margin Kayla T. Maloney 2012 Submitted in fulfilment of the requirements for the degree of Doctor of Philosophy The University of Sydney School of Geosciences Division of Geology and Geophysics Madsen Building (F09) Sydney, NSW, 2006 Australia University of Sydney, PhD Thesis, Kayla T. Maloney, 2012. i DECLARATION I declare that this thesis is less than 100,000 words in length, and that the work contained in this thesis has not been submitted for a higher degree at any other university or institution. Kayla T. Maloney August, 2012 PREFACE This PhD thesis consists of a collection of papers that are published or prepared for submission with international peer-reviewed journals appropriate to the discipline of geology. The publications form part of an integrated project and are presented in an order that represents the related elements of a connected thesis. The thesis contains an introductory section that provides an outline of the thesis, a summary of the contribution of the work to the field of geology, and a critical evaluation of the role of the thesis in informing further research in the field. Common themes in the papers are tied together and a discussion and conclusion of the whole thesis is presented at the end. No animal or ethical approvals were needed during the completion of this study. Data and interpretations in the thesis are the work of the author except where stated in the text. -
Provenance and Tectonic Implications of Orán Group Foreland Basin
Basin Research (2015) 1–17, doi: 10.1111/bre.12139 Provenance and tectonic implications of Oran Group foreland basin sediments,RıoIruyacanyon,NW Argentina (23° S) William H. Amidon,* Lisa V. Luna,* George B. Fisher,† Douglas W. Burbank,† Andrew R. C. Kylander-Clark† and Ricardo Alonso‡ *Middlebury College Geology Department, Middlebury, VT, USA †Earth Research Institute, University of California, Santa Barbara, CA, USA ‡Departamento de Geologıa, Universidad Nacional de Salta, Salta, Argentina ABSTRACT Foreland basins are important recorders of tectonic and climatic processes in evolving mountain ranges. The Rıo Iruya canyon of NW Argentina (23° S) exposes ca. 7500 m of Oran Group foreland basin sediments, spanning over 8 Myr of near continuous deposition in the Central Andes. This study presents a record of sedimentary provenance for the Iruya Section in the context of a revised stratigraphic chronology. We use U-Pb zircon ages from six interbedded ash layers and new magnet- ostratigraphy to constrain depositional ages in the section between 1.94 and 6.49 Ma, giving an aver- 1 age sedimentation rate of 0.93 0.02 (2r) km MyrÀ . We then pair U-Pb detrital zircon dating Æ with quartz trace-element analysis to track changes in sedimentary provenance from ca. 7.6 to 1.8 Ma. Results suggest that from ca. 7.6 to ca. 6.3 Ma, the Iruya watershed did not tap the Salta Group or Neogene volcanics that are currently exposed in the eastern Cordillera and Puna margin. One explanation is that a long-lived topographic barrier separated the eastern Puna from the foreland for much of the mid-late Miocene, and that the arrival of Jurassic-Neogene zircons records regional tectonic reactivation at ca. -
Titanosaur Trackways from the Late Cretaceous El Molino Formation of Bolivia (Cal Orck’O, Sucre)
Annales Societatis Geologorum Poloniae (2018), vol. 88: 223 – 241. doi: https://doi.org/10.14241/asgp.2018.014 TITANOSAUR TRACKWAYS FROM THE LATE CRETACEOUS EL MOLINO FORMATION OF BOLIVIA (CAL ORCK’O, SUCRE) Christian A. MEYER1, Daniel MARTY2 & Matteo BELVEDERE3 1 Department of Environmental Sciences, University of Basel, Bernoullistrasse 32, CH-4056 Basel, Switzerland; e-mail: [email protected] 2 Museum of Natural History Basel, Augustinergasse 2, CH- 4000 Basel, Switzerland; e-mail: [email protected] 3 Office de la culture, Paléontologie A16, Hôtel des Halles, P.O. Box 64, CH-2900 Porrentruy 2, Switzerland; e-mail: [email protected] Meyer, C. A., Marty, D. & Belvedere, M., 2018. Titanosaur trackways from the Late Cretaceous El Mo- lino Formation of Bolivia (Cal Orck’o, Sucre). Annales Societatis Geologorum Poloniae, 88: 223 – 241. Abstract: The Cal Orck’o tracksite is exposed in a quarry wall, approximately 4.4 km NW of Sucre (Department Chuquisaca, Bolivia) in the Altiplano/Cordillera Oriental, in the El Molino Formation (Middle Maastrichtian). Fossiliferous oolitic limestones, associated with large, freshwater stromatolites and nine levels of dinosaur tracks in the El Molino Formation document an open lacustrine environment. The main track-bearing level is almost vertical with a surface area of ~ 65,000 m2. The high-resolution mapping of the site from 1998 to 2015 revealed a total of 12,092 individual dinosaur tracks in 465 trackways. Nine different morphotypes of dinosaur tracks have been documented. Amongst them are several trackways of theropods, orni- thopods, ankylosaurs and sauropods, with the latter group accounting for 26% of the trackways. -
From Rodinia to Gondwana
A history of Proterozoic terranes in southern South America: From Rodinia to Gondwana C. Casquet a,*, c.w. Rapela b, R.J. Pankhurst c, E.G. Baldo d, C. Galindo a, C.M. Fanning e, J.A. Dahlquist d, J. Saavedra f a Departamento de Petrologia y Geoquimica, ICEO (Universidad Complutense, CSIC), 28040 Madrid, Spain b Centra de Investigaciones Geologicas (CONICET-UNLP), 1900 La Plata, Argentina C 'Visiting Research Associate, British Geological SUlVey, Keyworth, Nottingham NG12 SCC, United Kingdom d CICTERRA (CONICET-UNC), 5000 Cordoba, Argentina e Research School of Earth Sciences, The Australian National University, Canberra, Australia f Instituto de Agrobiologia y Recursos Naturales CSIC, 37071 Salamanca, Spain KEYWORDS Abstract The role played by Paleoproterozoic cratons in southern South America from the Mesopro Paleoproterozoic; terozoic to the Early Cambrian is reconsidered here. This period involved protracted continental amal Cratons; gamation that led to formation of the supercontinent Rodinia, followed by N eoproterozoic continental Grenvillian; break-up, with the consequent opening of Clymene and Iapetus oceans, and finally continental Neoproterozoic rifting; re-assembly as Gondwana through complex oblique collisions in the Late Neoproterozoic to Early SW Gondwana assembly Cambrian. The evidence for this is based mainly on a combination of precise U-Pb SHRMP dating and radiogenic isotope data for igneous and metamorphic rocks from a large area extending from the Rio de la Plata craton in the east to the Argentine Precordillera in the west and as far north as Arequipa in Peru. Our interpretation of the paleogeograpbical and geodynamic evolution invokes a hypothetical Paleoproterozoic block (MARA) embracing basement ultimately older than 1.7 Ga in the Western Sierras 1. -
Provenance Study on Neoproterozoic Rocks of Nw Argentina: Puncoviscana Formation – First Results
U N I V E R S I D A D D E C O N C E P C I Ó N DEPARTAMENTO DE CIENCIAS DE LA TIERRA 10° CONGRESO GEOLÓGICO CHILENO 2003 PROVENANCE STUDY ON NEOPROTEROZOIC ROCKS OF NW ARGENTINA: PUNCOVISCANA FORMATION – FIRST RESULTS ZIMMERMANN, U.1 1Dep.of Geol., RAU University, Auckland Park 2092, South Africa [email protected] INTRODUCTION Since more than 20 years the western border of Gondwana is object of controversies related to the basic question if crustal growth is related to terrane accretion or to “recycling” of the same crustal rocks during the Vendian and Lower Paleozoic. Different hypotheses were developed regarding the evolution of that margin. One of the key element to understand the crustal evolution, is the Vendian to Lower Cambrian so-called PVF. Turner (1960) described rock successions in northwestern Argentina (Fig. 1) of Pre-Ordovician age comprising greywackes and sand- and siltstones, but dominated by pelites as the PVF. Afterwards, it was established that mostly all Vendian to Lower Cambrian very-low to low grade metasedimentary rocks in the region are classified, such as Suncho, Negro Peinado or La Cébila Formation (e.g. comp. in Aceñolaza et al., 1988), are equivalents of the PVF. Widely distributed medium- to high-grade metasedimentary rocks (Fig. 1), those rocks were interpreted as exhumed deeper crustal levels of the PVF (Willner, 1990). Other authors deny this opinion and interpret the different metamorphic rocks related to different events, consequently of different ages (Mon and Hongn, 1990). Based on only punctual petrographic work, the depositional area was defined as a passive margin based on petrography and mainly major element geochemistry (Jezek, 1990, Willner et al., 1985, Rossi Toselli et al., 1997), or on preliminary trace element data (Do Campo and Ribeiro Guevara, 2002). -
Analysis of Titanopodus Tracks from the Late Cretaceous of Mendoza, Argentina
“main” — 2011/1/12 — 13:08 — page 1 — #1 Anais da Academia Brasileira de Ciências (Annals of the Brazilian Academy of Sciences) Printed version ISSN 0001-3765 / Online version ISSN 1678-2690 www.scielo.br/aabc Speeds and stance of titanosaur sauropods: analysis of Titanopodus tracks from the Late Cretaceous of Mendoza, Argentina BERNARDO J. GONZÁLEZ RIGA Departamento de Paleontología, IANIGLA, CCT-CONICET-Mendoza, Avda. Ruiz Leal s/n, Parque Gral. San Martín (5500) Mendoza, Argentina/Instituto de Ciencias Básicas, Universidad Nacional de Cuyo Manuscript received on November 13, 2009; accepted for publication on June 21, 2010 ABSTRACT Speed estimations from trackways of Titanopodus mendozensis González Riga and Calvo provide information about the locomotion of titanosaurian sauropods that lived in South America during the Late Cretaceous. Titanopodus ichnites were found at Agua del Choique, a newly discovered track site in the Loncoche Formation, Late Campanian-Early Maastrichtian of Mendoza, Argentina. This speed study follows the hypothesis of dynamic similarity proposed by Alexander. As a refinement of this method, a complementary equation is presented here based on an articulated titanosaurian specimen collected in strata that are regarded as correlative to those that have yielded Titanopodus tracks (Allen Formation, Neuquén Basin). This analysis indicates that hip height can be estimated as 4.586 times the length of the pes track in derived titanosaurs. With an estimation of the hip height and the stride measurements, the speed is calculated. The study of two wide-gauge trackways indicates that Titanopodus ichnites were produced by medium- sized titanosaurs (hip height of 211-229 cm) that walked at 4.7-4.9 km/h towards the south and southwest, following, in part, a sinuous pathway. -
Along-Strike Variation in Structural Styles and Hydrocarbon Occurrences, Subandean Fold-And-Thrust Belt and Inner Foreland, Colombia to Argentina
The Geological Society of America Memoir 212 2015 Along-strike variation in structural styles and hydrocarbon occurrences, Subandean fold-and-thrust belt and inner foreland, Colombia to Argentina Michael F. McGroder Richard O. Lease* David M. Pearson† ExxonMobil Upstream Research Company, Houston, Texas 77252, USA ABSTRACT The approximately N-S–trending Andean retroarc fold-and-thrust belt is the locus of up to 300 km of Cenozoic shortening at the convergent plate boundary where the Nazca plate subducts beneath South America. Inherited pre-Cenozoic differences in the overriding plate are largely responsible for the highly segmented distribution of hydrocarbon resources in the fold-and-thrust belt. We use an ~7500-km-long, orogen- parallel (“strike”) structural cross section drawn near the eastern terminus of the fold belt between the Colombia-Venezuela border and the south end of the Neuquén Basin, Argentina, to illustrate the control these inherited crustal elements have on structural styles and the distribution of petroleum resources. Three pre-Andean tectonic events are chiefl y responsible for segmentation of sub- basins along the trend. First, the Late Ordovician “Ocloyic” tectonic event, recording terrane accretion from the southwest onto the margin of South America (present-day northern Argentina and Chile), resulted in the formation of a NNW-trending crustal welt oriented obliquely to the modern-day Andes. This paleohigh infl uenced the dis- tribution of multiple petroleum system elements in post-Ordovician time. Second, the mid-Carboniferous “Chañic” event was a less profound event that created mod- est structural relief. Basin segmentation and localized structural collapse during this period set the stage for deposition of important Carboniferous and Permian source rocks in the Madre de Dios and Ucayali Basins in Peru. -
From Rodinia to Gondwana
GEOSCIENCE FRONTIERS 3(2) (2012) 137e145 available at www.sciencedirect.com China University of Geosciences (Beijing) GEOSCIENCE FRONTIERS journal homepage: www.elsevier.com/locate/gsf GSF REVIEW A history of Proterozoic terranes in southern South America: From Rodinia to Gondwana C. Casquet a,*, C.W. Rapela b, R.J. Pankhurst c, E.G. Baldo d, C. Galindo a, C.M. Fanning e, J.A. Dahlquist d, J. Saavedra f a Departamento de Petrologıa y Geoquımica, IGEO (Universidad Complutense, CSIC), 28040 Madrid, Spain b Centro de Investigaciones Geologicas (CONICET-UNLP), 1900 La Plata, Argentina c Visiting Research Associate, British Geological Survey, Keyworth, Nottingham NG12 5GG, United Kingdom d CICTERRA (CONICET-UNC), 5000 Cordoba, Argentina e Research School of Earth Sciences, The Australian National University, Canberra, Australia f Instituto de Agrobiologıa y Recursos Naturales CSIC, 37071 Salamanca, Spain Received 3 August 2011; accepted 8 November 2011 Available online 3 December 2011 KEYWORDS Abstract The role played by Paleoproterozoic cratons in southern South America from the Mesopro- Paleoproterozoic; terozoic to the Early Cambrian is reconsidered here. This period involved protracted continental amal- Cratons; gamation that led to formation of the supercontinent Rodinia, followed by Neoproterozoic continental Grenvillian; break-up, with the consequent opening of Clymene and Iapetus oceans, and finally continental Neoproterozoic rifting; re-assembly as Gondwana through complex oblique collisions in the Late Neoproterozoic to Early SW Gondwana assembly Cambrian. The evidence for this is based mainly on a combination of precise U-Pb SHRMP dating and radiogenic isotope data for igneous and metamorphic rocks from a large area extending from the Rio de la Plata craton in the east to the Argentine Precordillera in the west and as far north as Arequipa in Peru.