Sedimentary, Structural, and Provenance Record of the Cianzo Basin, Puna Plateau-Eastern Cordillera Boundary, NW Argentina

Total Page:16

File Type:pdf, Size:1020Kb

Sedimentary, Structural, and Provenance Record of the Cianzo Basin, Puna Plateau-Eastern Cordillera Boundary, NW Argentina Copyright by Benjamin Charles Siks 2011 The Thesis Committee for Benjamin Charles Siks Certifies that this is the approved version of the following thesis: Sedimentary, structural, and provenance record of the Cianzo basin, Puna plateau-Eastern Cordillera boundary, NW Argentina APPROVED BY SUPERVISING COMMITTEE: Supervisor: Brian K. Horton Ronald J. Steel Kitty Milliken Sedimentary, structural, and provenance record of the Cianzo basin, Puna plateau-Eastern Cordillera boundary, NW Argentina by Benjamin Charles Siks, B.S. Geo. Thesis Presented to the Faculty of the Graduate School of The University of Texas at Austin in Partial Fulfillment of the Requirements for the Degree of Master of Science in Geological Sciences The University of Texas at Austin May 2011 Acknowledgements This work could not have been completed without the support of my future wife, Ashley Bens, my mother Debbie Stann, my father Jan Siks, my siblings, my supervisor Dr. Brian Horton, my committee members Dr. Ron Steel and Dr. Kitty Milliken, as well as the members of my research group, and finally the loyal support of my border collie Pippin. iv Abstract Sedimentary, structural, and provenance record of the Cianzo basin, Puna plateau-Eastern Cordillera boundary, NW Argentina Benjamin Charles Siks, MS GeoSci The University of Texas at Austin, 2011 Supervisor: Brian K. Horton The fault-bounded Cianzo basin represents a Cenozoic intermontane depocenter between the Puna plateau and Eastern Cordillera of the central Andean fold-thrust belt in northern Argentina. New characterizations of fold-thrust structure, nonmarine sedimentation, and sediment provenance for the shortening-induced Cianzo basin at 23°S help constrain the origin, interconnectedness, and subsequent uplift and exhumation of the basin, which may serve as an analogue for other intermontane hinterland basins in the Andes. Structural mapping of the Cianzo basin reveals SW and NE-plunging synclines within the >6000 m-thick, upsection coarsening Cenozoic clastic succession in the shared footwall of the N-striking, E-directed Cianzo thrust fault and transverse, NE-striking Hornocal fault. Growth stratal relationships within upper Miocene levels of the succession indicate syncontractional sedimentation directly adjacent to the Hornocal fault. Measured stratigraphic sections and clastic sedimentary lithofacies of Cenozoic basin-fill deposits show upsection changes from (1) a distal fluvial system recorded by v fine-grained, paleosol-rich, heavily bioturbated sandstones and mudstones (Paleocene‒Eocene Santa Bárbara Subgroup, ~400 m), to (2) a braided fluvial system represented by cross-stratified sandstones and interbedded mudstones with 0.3 to 8 m upsection-fining sequences (Upper Eocene–Oligocene Casa Grande Formation, ~1400 m), to (3) a distributary fluvial system in the distal sectors of a distributary fluvial megafan represented by structureless sheetflood sandstones, stratified pebble conglomerates and sandstones, and interbedded overbank mudstones (Miocene Río Grande Formation, ~3300 m), to (4) a proximal alluvial fan system with thick conglomerates interbedded with thin discontinuous sandstone lenses (upper Miocene Pisungo Formation, ~1600 m). New 40Ar/39Ar geochronological results for five interbedded volcanic tuffs indicate distributary fluvial deposition of the uppermost Río Grande Formation from 16.31 ± 0.6 Ma to 9.69 ± 0.05 Ma. Sandstone petrographic results show distinct upsection trends in lithic and feldspar content in the Casa Grande, Río Grande, and Pisungo formations, potentially distinguishing western magmatic arc (Western Cordillera) sediment sources from evolving eastern thrust-belt sources (Puna‒Eastern Cordillera). In addition to growth stratal relationships and 40Ar/39Ar constraints, conglomerate clast compositions reflect distinct lithologic differences, constraining the activation of the Cianzo thrust and coeval movement on the reactivated Hornocal fault. Finally, U-Pb geochronological analyses of sandstone detrital zircon populations in conjunction with paleocurrent data and depositional facies patterns help distinguish localized sources from more distal sources west of the basin, revealing a systematic eastward advance of Eocene to Miocene fold-thrust deformation in the central Andes of northern Argentina. vi Table of Contents List of tables ........................................................................................................... ix List of figures ...........................................................................................................x Chapter 1. Introduction and geologic context .........................................................1 Introduction .....................................................................................................1 Geologic setting ..............................................................................................3 Chapter 2. Tectonic, stratigraphic, and structural framework ................................7 Tectonic history ..............................................................................................7 Regional stratigraphy ....................................................................................10 Structural framework ....................................................................................13 Growth strata .................................................................................................16 Chapter 3. Sedimentology and stratigraphy ..........................................................19 Facies associations ........................................................................................19 40Ar/39Ar age geochronology ........................................................................34 Chapter 4. Depositional systems ............................................................................36 Chapter 5. Provenance ...........................................................................................40 Sandstone compositons .................................................................................40 Conglomerate clast compositions .................................................................46 Detrital zircon U-Pb geochronology .............................................................48 Chapter 6. Basin reconstruction and discussion ....................................................55 Santa Bárbara Group .....................................................................................55 Casa Grande Formation ................................................................................56 Río Grande Formation ..................................................................................57 Pisungo Formation ........................................................................................58 Chapter 7. Conclusions ..........................................................................................61 Appendix 1. Point count tables .............................................................................65 Appendix 2. Clast count tables .............................................................................67 Appendix 3. U-Pb geochronological results .........................................................69 vii Appendix 4. McBride, 2008 U-Pb results .............................................................85 References ..............................................................................................................89 viii List of Tables Table 1. Description and interpretation of lithofacies . ...................................20 Table 2. Summary of facies associations and interpretations .........................21 Table 3. 40Ar/39Ar data for interbedded tuffs ..................................................35 Table 4. Parameters for sandstone mineraloglical point counting. .................41 ix List of Figures Figure 1. Overview map of South America .......................................................4 Figure 2. Regional structures and provenace terranes in northern Argentina. ...6 Figure 3. Location of Cianzo basin and regional structures. ..............................9 Figure 4. Regional stratigraphy of the Cianzo basin ........................................11 Figure 5. Geologic map of Cianzo basin and surronding structures ................14 Figure 6. Growth strata within the Pisungo Formation ....................................18 Figure 7. Simplified stratigraphic section of Cenozoic fill ..............................22 Figure 8. Measured stratigraphic sections in the Cianzo basin ........................23 Figure 9. Lower Río Grande facies photographs .............................................26 Figure 10. Upper Río Grande facies photographs ..............................................29 Figure 11. Pisungo facies photographs...............................................................33 Figure 12. Depostional systems evolution diagram ...........................................39 Figure 13. Sandstone petrographic ternary diagrams .........................................44 Figure 14. Lithologic conglomerate clast count diagrams .................................47 Figure 15. Detrital zircon U-Pb relative probability plots ..................................51 Figure 16. 2D regional basin reconstruction diagrams .......................................60 x Chapter 1. Introduction and geologic context INTRODUCTION Many studies attribute crustal thickening and surface uplift in the central Andean fold-thrust belt and Puna‒Altiplano
Recommended publications
  • 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).
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • O Regist Regi Tro Fós Esta Istro De Sil De C Ado Da a E
    UNIVERSIDADE FEDERAL DO RIO GRANDE DOO SUL INSTITUTO DE GEOCIÊNCIAS PROGRAMA DE PÓS-GRADUAÇÃO EM GEOCIÊNCIAS O REGISTRO FÓSSIL DE CROCODILIANOS NA AMÉRICA DO SUL: ESTADO DA ARTE, ANÁLISE CRÍTICAA E REGISTRO DE NOVOS MATERIAIS PARA O CENOZOICO DANIEL COSTA FORTIER Porto Alegre – 2011 UNIVERSIDADE FEDERAL DO RIO GRANDE DO SUL INSTITUTO DE GEOCIÊNCIAS PROGRAMA DE PÓS-GRADUAÇÃO EM GEOCIÊNCIAS O REGISTRO FÓSSIL DE CROCODILIANOS NA AMÉRICA DO SUL: ESTADO DA ARTE, ANÁLISE CRÍTICA E REGISTRO DE NOVOS MATERIAIS PARA O CENOZOICO DANIEL COSTA FORTIER Orientador: Dr. Cesar Leandro Schultz BANCA EXAMINADORA Profa. Dra. Annie Schmalz Hsiou – Departamento de Biologia, FFCLRP, USP Prof. Dr. Douglas Riff Gonçalves – Instituto de Biologia, UFU Profa. Dra. Marina Benton Soares – Depto. de Paleontologia e Estratigrafia, UFRGS Tese de Doutorado apresentada ao Programa de Pós-Graduação em Geociências como requisito parcial para a obtenção do Título de Doutor em Ciências. Porto Alegre – 2011 Fortier, Daniel Costa O Registro Fóssil de Crocodilianos na América Do Sul: Estado da Arte, Análise Crítica e Registro de Novos Materiais para o Cenozoico. / Daniel Costa Fortier. - Porto Alegre: IGEO/UFRGS, 2011. [360 f.] il. Tese (doutorado). - Universidade Federal do Rio Grande do Sul. Instituto de Geociências. Programa de Pós-Graduação em Geociências. Porto Alegre, RS - BR, 2011. 1. Crocodilianos. 2. Fósseis. 3. Cenozoico. 4. América do Sul. 5. Brasil. 6. Venezuela. I. Título. _____________________________ Catalogação na Publicação Biblioteca Geociências - UFRGS Luciane Scoto da Silva CRB 10/1833 ii Dedico este trabalho aos meus pais, André e Susana, aos meus irmãos, Cláudio, Diana e Sérgio, aos meus sobrinhos, Caio, Júlia, Letícia e e Luíza, à minha esposa Ana Emília, e aos crocodilianos, fósseis ou viventes, que tanto me fascinam.
    [Show full text]
  • Speeds and Stance of Titanosaur Sauropods: Analysis of Titanopodus Tracks from the Late Cretaceous of Mendoza, Argentina
    “main” — 2011/2/10 — 16:13 — page 279 — #1 Anais da Academia Brasileira de Ciências (2011) 83(1): 279-290 (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.
    [Show full text]
  • The Growth of the Central Andes, 22°S–26°S
    Downloaded from memoirs.gsapubs.org on January 15, 2015 The Geological Society of America Memoir 212 2015 The growth of the central Andes, 22°S–26°S J. Quade* M.P. Dettinger B. Carrapa P. DeCelles K.E. Murray Department of Geosciences, University of Arizona, Tucson, Arizona 85721, USA K.W. Huntington Department of Earth and Space Sciences, University of Washington, Seattle, Washington 98195-1310, USA A. Cartwright Mintec, Inc., 3544 East Fort Lowell Road, Tucson, Arizona 85716, USA R.R. Canavan Department of Geology, University of Wyoming, Laramie, Wyoming 82071, USA G. Gehrels Department of Geosciences, University of Arizona, Tucson, Arizona 85721, USA M. Clementz Department of Geology, University of Wyoming, Laramie, Wyoming 82071, USA ABSTRACT We synthesize geologic observations with new isotopic evidence for the timing and magnitude of uplift for the central Andes between 22°S and 26°S since the Paleocene. To estimate paleoelevations, we used the stable isotopic composition of carbonates and volcanic glass, combined with another paleoelevation indicator for the central Andes: the distribution of evaporites. Paleoelevation reconstruction using clumped isotope paleothermometry failed due to resetting during burial. The Andes at this latitude rose and broadened eastward in three stages during the Cenozoic. The fi rst, in what is broadly termed the “Incaic” orogeny, ended by the late Eocene, when magmatism and deformation had elevated to ≥4 km the bulk (~50%) of what is now the western and central Andes. The second stage witnessed the gradual building of the easternmost Puna and Eastern Cordillera, starting with deforma- tion as early as 38 Ma, to >3 km by no later than 15 Ma.
    [Show full text]
  • ABSTRACT BOOK a Cura Della Società Geologica Italiana
    https://doi.org/10.3301/ABSGI.2019.04 Milano, 2-5 July 2019 ABSTRACT BOOK a cura della Società Geologica Italiana 3rd International Congress on Stratigraphy GENERAL CHAIRS Marco Balini, Università di Milano, Italy Elisabetta Erba, Università di Milano, Italy - past President Società Geologica Italiana 2015-2017 SCIENTIFIC COMMITTEE Adele Bertini, Peter Brack, William Cavazza, Mauro Coltorti, Piero Di Stefano, Annalisa Ferretti, Stanley C. Finney, Fabio Florindo, Fabrizio Galluzzo, Piero Gianolla, David A.T. Harper, Martin J. Head, Thijs van Kolfschoten, Maria Marino, Simonetta Monechi, Giovanni Monegato, Maria Rose Petrizzo, Claudia Principe, Isabella Raffi, Lorenzo Rook ORGANIZING COMMITTEE The Organizing Committee is composed by members of the Department of Earth Sciences “Ardito Desio” and of the Società Geologica Italiana Lucia Angiolini, Cinzia Bottini, Bernardo Carmina, Domenico Cosentino, Fabrizio Felletti, Daniela Germani, Fabio M. Petti, Alessandro Zuccari FIELD TRIP COMMITTEE Fabrizio Berra, Mattia Marini, Maria Letizia Pampaloni, Marcello Tropeano ABSTRACT BOOK EDITORS Fabio M. Petti, Giulia Innamorati, Bernardo Carmina, Daniela Germani Papers, data, figures, maps and any other material published are covered by the copyright own by the Società Geologica Italiana. DISCLAIMER: The Società Geologica Italiana, the Editors are not responsible for the ideas, opinions, and contents of the papers published; the authors of each paper are responsible for the ideas opinions and con- tents published. La Società Geologica Italiana, i curatori scientifici non sono responsabili delle opinioni espresse e delle affermazioni pubblicate negli articoli: l’autore/i è/sono il/i solo/i responsabile/i. © Società Geologica Italiana, Roma 2019 STRATI 2019 ABSTRACT INDEX ST1.1 History of Stratigraphy in Italian environments (17th – 20th centuries) ........................................
    [Show full text]
  • Large Theropod Dinosaur Footprint Associations in Western Gondwana: Behavioural and Palaeogeographic Implications
    Large theropod dinosaur footprint associations in western Gondwana: Behavioural and palaeogeographic implications KAREN MORENO, SILVINA DE VALAIS, NICOLÁS BLANCO, ANDREW J. TOMLINSON, JAVIER JACAY, and JORGE O. CALVO Moreno, K., De Valais, S., Blanco, N., Tomlinson, A.J., Jacay, J., and Calvo, J.O. 2012. Large theropod dinosaur footprint associations in western Gondwana: Behavioural and palaeogeographic implications. Acta Palaeontologica Polonica 57 (1): 73–83. In modern terrestrial ecosystems, the population size of large predators is low, and a similar pattern has usually been as− sumed for dinosaurs. However, fossil finds of monospecific, large theropod accumulations suggest that population dynam− ics were more complex. Here, we report two Early Cretaceous tracksites dominated by large theropod footprints, in Querulpa Chico (Peru) and Chacarilla (Chile). The two sites correspond to distinct depositional environments—tidal ba− sin/delta (Querulpa Chico) and meandering river (Chacarilla)—with both subject to extensive arid or semiarid palaeo− climatic conditions. Although most trackways show no preferred orientation, a clear relationship between two trackmakers is observed in one instance. This observation, coupled with the high abundance of trackways belonging to distinct large theropods, and the exclusion of tracks of other animals, suggests some degree of grouping behaviour. The presence of fresh− water sources in a dry climate and perhaps social behaviour such as pair bonding may have promoted interactions between large carnivores. Further, the occurrence of these two tracksites confirms that large theropod dinosaurs, possibly spino− saurids and/or carcharodontosaurids, existed on the western margin of Gondwana as early as the earliest Cretaceous. Key words: Theropoda, footprints, behaviour, palaeogeography, Early Cretaceous, Gondwana, Chile, Peru.
    [Show full text]
  • Carbon and Oxygen Isotopes of Maastrichtian–Danian Shallow Marine Carbonates: Yacoraite Formation, Northwestern Argentina
    Journal of South American Earth Sciences 23 (2007) 304–320 www.elsevier.com/locate/jsames Carbon and oxygen isotopes of Maastrichtian–Danian shallow marine carbonates: Yacoraite Formation, northwestern Argentina Rosa Marquillas a,*, Ignacio Sabino b, Alcides Nobrega Sial c, Cecilia del Papa a, Valderez Ferreira c, Stephen Matthews d a CONICET-Universidad Nacional de Salta, Buenos Aires 177, 4400 Salta, Argentina b Universidad Nacional de Salta-CIUNSa, Buenos Aires 177, 4400 Salta, Argentina c NEG–LABISE, Department of Geology, UFPE, C.P. 7852, Recife 50670-000, Brazil d SERNAGEOMIN, CC 10465, Santiago, Chile Abstract The Maastrichtian–Danian limestones of the Yacoraite Formation (northwestern Argentina) show carbon and oxygen isotopic values consistent with shallow marine conditions. The members of the formation respond to different sedimentary environments and are char- acterised by distinctive stable isotopes and geochemistry. The basal Amblayo Member is composed of high-energy dolomitic limestones and limestones with positive isotopic values (+2& d13C, +2& d18O). The top of the member reveals an isotopic shift of d13C(À5&) and d18O(À10&), probably related to a descent in the sea level. The sandy Gu¨emes Member has isotopically negative (À2& d13C, À1& d18O) limestones, principally controlled by water mixing, decreased organic productivity, and compositional changes in the car- bonates. The isotopically lighter limestones are calcitic, with a greater terrigenous contribution and different geochemical composition (high Si–Mn–Fe–Na, low Ca–Mg–Sr). These isotopic and lithological changes relate to the Cretaceous–Palaeogene transition. The Ale- manı´a Member, composed of dolomitic limestones and pelites, represents a return to marine conditions and shows a gradual increase in isotopic values, reaching values similar to those of the Amblayo Member.
    [Show full text]
  • EGU2018-8280-2, 2018 EGU General Assembly 2018 © Author(S) 2018
    Geophysical Research Abstracts Vol. 20, EGU2018-8280-2, 2018 EGU General Assembly 2018 © Author(s) 2018. CC Attribution 4.0 license. Depositional Environment Interpretation from Organofacies Characterization for Yacoraite Fm. outcrop samples, Cretaceous Salta Basin - Argentina Ricardo Ruiz (1,2), Robert Ondrak (2), Brian Horsfield (2), and Eduardo Rossello (3) (1) Institut für Erd- und Umweltwissenschaften, Universität Potdam, Potsdam, Germany, (2) Helmholtz Centre Potsdam - GFZ German Research Centre for Geosciences, Potsdam; Section 3.2: Organic Geochemistry, Potsdam, Germany, (3) CONICET-FCEN, University of Buenos Aires, Buenos Aire,s Argentina The Yacoraite Formation (Maastrichtian-Danian) is one of the main source rocks in North-West Argentina in the sedimentary basins in Salta and Jujuy provinces. It was deposited following Lower Cretaceous rifting, represent- ing the last Cretaceous marine ingression although locally evidence has been found for lacustrine depositional conditions. Here we show preliminary results for depositional environment characterization of Tres Cruces and Metan-Alemania subbasins, based on the organic geochemistry of rock samples and their extracts. Depending on its depositional environment, the Yacoraite Formation exhibits a wide range of organic content varying from poor up to rich (up to 7% TOC). It contains kerogen Types II and II/III with low sulphur content, consistent with marine organic matter. The presence of Type III kerogen observed in several samples indicates an input of terrestrial organic matter probably related to periods of sea level fall. Biomarker distributions, like the relative abundance of C27-C29 steranes, have been widely used to differentiate between marine, lacustrine or terrestrial depositional environments. The sterane distribution of our samples indi- cates an open marine depositional environment for the Yacoraite Fm.
    [Show full text]
  • Cretaceous-Paleogene Transition at the Paraiba Basin
    Journal of South American Earth Sciences 32 (2011) 379e392 Contents lists available at ScienceDirect Journal of South American Earth Sciences journal homepage: www.elsevier.com/locate/jsames Cretaceous-Paleogene transition at the Paraíba Basin, Northeastern, Brazil: Carbon-isotope and mercury subsurface stratigraphies Maria V. Nascimento-Silva a,*, Alcides N. Sial a, Valderez P. Ferreira a, Virgínio H. Neumann b, José A. Barbosa b, Marcio M. Pimentel c, Luiz D. de Lacerda d a NEG-LABISE, Department of Geology, Federal Univ. of Pernambuco, Recife, PE, 50670-000, Brazil b LAGESE, Department of Geology, Federal Univ. of Pernambuco, Recife, PE, 50670-000, Brazil c Institute of Geosciences, Federal Univ. of Rio Grande do Sul, Porto Alegre, RS, 91509-900, Brazil d LABOMAR, Institute of Marine Sciences, Federal Univ. of Ceará, Fortaleza, CE, 60165-081, Brazil article info abstract Article history: The Paraíba Basin in northeastern Brazil contains a complete carbonate sequence that recorded the Received 27 August 2010 CretaceousePaleogene transition, and is composed of the Itamaracá, Gramame and Maria Farinha Accepted 21 February 2011 formations. In this study, the behavior of C and O isotopes, major and trace element chemistry have been examined in core drill carbonate samples from three drill holes (Poty Quarry, Olinda and Itamaracá). Keywords: The deposition of carbonates in this basin was initiated during a marine transgression with temper- e Cretaceous Paleogene transition ature and bioproductivity increase in the Early Maastrichtian. d18O values for this interval vary from À3& C isotopes to À5& VPDB, and d13C, from À1.2& to 0.1&, reaching a maximum in the Late Maastrichtian, with values O isotopes þ & d13 þ & Northeastern Brazil around 2 .
    [Show full text]