Age Constraints on the Paleozoic Yaguarí-Buena Vista
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Optimal Swimming Speed Estimates in the Early Permian Mesosaurid
This article was downloaded by: [Joaquín Villamil] On: 24 August 2015, At: 10:09 Publisher: Taylor & Francis Informa Ltd Registered in England and Wales Registered Number: 1072954 Registered office: 5 Howick Place, London, SW1P 1WG Historical Biology: An International Journal of Paleobiology Publication details, including instructions for authors and subscription information: http://www.tandfonline.com/loi/ghbi20 Optimal swimming speed estimates in the Early Permian mesosaurid Mesosaurus tenuidens (Gervais 1865) from Uruguay Joaquín Villamilab, Pablo Núñez Demarcoc, Melitta Meneghela, R. Ernesto Blancobd, Washington Jonesbe, Andrés Rinderknechtbe, Michel Laurinf & Graciela Piñeirog a Laboratorio de Sistemática e Historia Natural de Vertebrados, IECA, Facultad de Ciencias, Universidad de la República, Montevideo, Uruguay b Núcleo de Biomecánica, Espacio Interdisciplinario, Montevideo, Uruguay c Click for updates Facultad de Ciencias, Departamento de Geología, Montevideo, Uruguay d Facultad de Ciencias, Instituto de Física, Montevideo, Uruguay e Museo Nacional de Historia Natural, Montevideo, Uruguay f CR2P, Sorbonne Universités, CNRS/MNHN/UPMC, Muséum National d’Histoire Naturelle, Paris, France g Facultad de Ciencias, Departamento de Evolución de Cuencas, Montevideo, Uruguay Published online: 14 Aug 2015. To cite this article: Joaquín Villamil, Pablo Núñez Demarco, Melitta Meneghel, R. Ernesto Blanco, Washington Jones, Andrés Rinderknecht, Michel Laurin & Graciela Piñeiro (2015): Optimal swimming speed estimates in the Early Permian mesosaurid Mesosaurus tenuidens (Gervais 1865) from Uruguay, Historical Biology: An International Journal of Paleobiology, DOI: 10.1080/08912963.2015.1075018 To link to this article: http://dx.doi.org/10.1080/08912963.2015.1075018 PLEASE SCROLL DOWN FOR ARTICLE Taylor & Francis makes every effort to ensure the accuracy of all the information (the “Content”) contained in the publications on our platform. -
Impact Structures and Events – a Nordic Perspective
107 by Henning Dypvik1, Jüri Plado2, Claus Heinberg3, Eckart Håkansson4, Lauri J. Pesonen5, Birger Schmitz6, and Selen Raiskila5 Impact structures and events – a Nordic perspective 1 Department of Geosciences, University of Oslo, P.O. Box 1047, Blindern, NO 0316 Oslo, Norway. E-mail: [email protected] 2 Department of Geology, University of Tartu, Vanemuise 46, 51014 Tartu, Estonia. 3 Department of Environmental, Social and Spatial Change, Roskilde University, P.O. Box 260, DK-4000 Roskilde, Denmark. 4 Department of Geography and Geology, University of Copenhagen, Øster Voldgade 10, DK-1350 Copenhagen, Denmark. 5 Division of Geophysics, University of Helsinki, P.O. Box 64, FIN-00014 Helsinki, Finland. 6 Department of Geology, University of Lund, Sölvegatan 12, SE-22362 Lund, Sweden. Impact cratering is one of the fundamental processes in are the main reason that the Nordic countries are generally well- the formation of the Earth and our planetary system, as mapped. reflected, for example in the surfaces of Mars and the Impact craters came into the focus about 20 years ago and the interest among the Nordic communities has increased during recent Moon. The Earth has been covered by a comparable years. The small Kaalijärv structure of Estonia was the first impact number of impact scars, but due to active geological structure to be confirmed in northern Europe (Table 1; Figures 1 and processes, weathering, sea floor spreading etc, the num- 7). First described in 1794 (Rauch), the meteorite origin of the crater ber of preserved and recognized impact craters on the field (presently 9 craters) was proposed much later in 1919 (Kalju- Earth are limited. -
Impact Melt Rocks in the "Cretaceous
Large Meteorite Impacts (2003) alpha_t-z.pdf Contents — T through Z Locations and Compositions of Mare Ponds in South Pole-Aitken Basin on the Moon and Its Implication to the Impact Tectonics T. Takata and S. Hori ............................................................................................................................. 4058 New Laboratory Results on Field Sections at the Impact Crater of Araguainha (MT, GO, Brazil). Area of Proximal and Distal Impact Ejecta, Including Microspherules Dated from the End of Permian J. M. Théry, A. Crosta, E. Veto Akos, E. Bilal, K. Gal-Solymos, and E. Dransart................................. 4096 Techniques of Shock Wave Experiments and Determination of Hugoniot Data of Solids K. Thoma................................................................................................................................................ 4134 Differential Stress-controlled Deformation of Quartz During and After Hypervelocity Impact — Microstructural Evidence from the Charlevoix Impact Structure, Quebéc, Canada C. A. Trepmann and J. G. Spray............................................................................................................. 4026 Mjølnir Marine Crater Resulting from Oblique Impact: Compelling Evidence F. Tsikalas and J. I. Faleide................................................................................................................... 4005 A New Mid- to Late-Maastrichtian Impact in the Raton Basin 100m Below the K/T Boundary P. Turner, S. C. Sherlock, P. Clarke, and -
A Reassessment of the Taxonomic Position of Mesosaurs, and a Surprising Phylogeny of Early Amniotes
ORIGINAL RESEARCH published: 02 November 2017 doi: 10.3389/feart.2017.00088 A Reassessment of the Taxonomic Position of Mesosaurs, and a Surprising Phylogeny of Early Amniotes Michel Laurin 1* and Graciela H. Piñeiro 2 1 CR2P (UMR 7207) Centre de Recherche sur la Paléobiodiversité et les Paléoenvironnements (Centre National de la Recherche Scientifique/MNHN/UPMC, Sorbonne Universités), Paris, France, 2 Departamento de Paleontología, Facultad de Ciencias, University of the Republic, Montevideo, Uruguay We reassess the phylogenetic position of mesosaurs by using a data matrix that is updated and slightly expanded from a matrix that the first author published in 1995 with his former thesis advisor. The revised matrix, which incorporates anatomical information published in the last 20 years and observations on several mesosaur specimens (mostly from Uruguay) includes 17 terminal taxa and 129 characters (four more taxa and five more characters than the original matrix from 1995). The new matrix also differs by incorporating more ordered characters (all morphoclines were ordered). Parsimony Edited by: analyses in PAUP 4 using the branch and bound algorithm show that the new matrix Holly Woodward, Oklahoma State University, supports a position of mesosaurs at the very base of Sauropsida, as suggested by the United States first author in 1995. The exclusion of mesosaurs from a less inclusive clade of sauropsids Reviewed by: is supported by a Bremer (Decay) index of 4 and a bootstrap frequency of 66%, both of Michael S. Lee, which suggest that this result is moderately robust. The most parsimonious trees include South Australian Museum, Australia Juliana Sterli, some unexpected results, such as placing the anapsid reptile Paleothyris near the base of Consejo Nacional de Investigaciones diapsids, and all of parareptiles as the sister-group of younginiforms (the most crownward Científicas y Técnicas (CONICET), Argentina diapsids included in the analyses). -
GEOLOGY of URUGUAY: a REVIEW. Gómez Rifas,C.G
v 1 GEOLOGY OF URUGUAY: A REVIEW. Gómez Rifas,C.G. Montevideo,Uruguay. 1.Introduction. Uruguay has been a country devoted to breeding cattle and agriculture.Mining has no tradition.The evolution of geological knowledge begun with Dr. Karl Walther who published 53 papers between 1909 and 1948. 2.Preclevonian in Uruguay. 2.1.The Río de la Plata Craton. This unít refers to rocks dated between 1700 to 2300 MY in southern UruguaY,situated on the western side of the Sarandí del Yí-Las Ánimas Suture Zone.This is a my10nitic belt 13000 meters wide. 2.1.1.The Base Complexo 1t i8 integrated by gneiss and migmatites of varied textures,as we11 as deformed granites. Some typical outcrops are:Piedra A1ta,F1orida Department,and near the 1itt1e dam in Costa Azu1,Canelones Department. 2.1.2.Montevideo Formation. ,/~ 2 It is formed by oligoclase gneiss, amp11.ibolites, mieaschist and micaceous quartzites.T11.e gneiss can be visited in Pajas Blancas,Parque Rod6,Carrasco beaches and so on.They are rocks of medium grain size and poor defined sc11.istosity,made by quartz,oligoclase,biotite and muscovite and zoisite as accesory mineraIs. T11.e amphibolites has been classified as ortho and para-amphibolites according to their genesis.The ort11.o- amphibolites have cristalized andesine.The para-amphibolites are generally foliated with medium grain size,integrated by hornblende and andesine with an evident nematoblastic texture.The main accesory mineral is sphene. 2.1.3.San José Formation. lt outcrops at north of San José de Mayo and it is the field rock of Compañia San José Gold Mine,s?uth of Mahoma Granite. -
Polygonal Impact Craters in Argyre Region, Mars: Implications for Geology and Cratering Mechanics
Meteoritics & Planetary Science 43, Nr 10, 1605–1628 (2008) Abstract available online at http://meteoritics.org Polygonal impact craters in Argyre region, Mars: Implications for geology and cratering mechanics T. ÖHMAN1, 2*, M. AITTOLA2, V.-P. KOSTAMA2, J. RAITALA2, and J. KORTENIEMI2, 3 1Department of Geosciences, Division of Geology, University of Oulu, P.O. Box 3000, FI-90014, Finland 2Department of Physical Sciences, Division of Astronomy, University of Oulu, P.O. Box 3000, FI-90014, Finland 3Institut für Planetologie, Westfälische Wilhelms-Universität, Wilhelm-Klemm-Strasse 10, D-48149 Münster, Germany *Corresponding author. E-mail: [email protected] (Received 20 November 2007; revision accepted 15 April 2008) Abstract–Impact craters are not always circular; sometimes their rims are composed of several straight segments. Such polygonal impact craters (PICs) are controlled by pre-existing target structures, mainly faults or other similar planes of weakness. In the Argyre region, Mars, PICs comprise ∼17% of the total impact crater population (>7 km in diameter), and PICs are relatively more common in older geologic units. Their formation is mainly controlled by radial fractures induced by the Argyre and Ladon impact basins, and to a lesser extent by the basin-concentric fractures. Also basin-induced conjugate shear fractures may play a role. Unlike the PICs, ridges and graben in the Argyre region are mostly controlled by Tharsis-induced tectonism, with the ridges being concentric and graben radial to Tharsis. Therefore, the PICs primarily reflect an old impact basin-centered tectonic pattern, whereas Tharsis-centered tectonism responsible for the graben and the ridges has only minor influence on the PIC rim orientations. -
Chapter 6 ______Chapter 6
Chapter 6 _____________________________________________________________________ Chapter 6 Discussion 6.1 Introduction Previous structural studies of the collar rocks of the Vredefort Dome focused predominantly on specific areas of the collar (e.g., Lilly 1978, 1981) or specific features, such as pseudotachylitic breccias (e.g., Martini 1991; Gibson et al. 1997) and shatter cones (e.g., Manton 1962; Albat and Mayer 1989; Nicolaysen and Reimold 1999). Many of the studies were carried out in the era leading up to the confirmation of the dome as part of an impact structure and, hence, they did not necessarily examine these structures within the context of an impact-induced evolutionary history. This study aimed to document all structural features over the entire exposed extent of the collar of the dome in an attempt to establish geometric and/or temporal relationships between individual structures and their relation to the impact process (impact-induced versus non-impact-induced deformation). Furthermore, the temporal relationships between impact-related deformation features were investigated in order to obtain a better understanding of the processes involved in the evolution of the deep central parts of a complex impact structure during the cratering process. More specifically, this study aimed at improving the understanding of the processes that take place during the formation and subsequent collapse of the central uplift in such a crater. A brief summary of the main observations will be provided at the beginning of each section in order to point out the salient facts, which are necessary for a comprehensive discussion of the results with regard to the formation and collapse of the Vredefort Dome, as well as other impact structures in general. -
Giant Comets and Mass Extinctions of Life
Mon. Not. R. Astron. Soc. 000, ?? – ?? (2015) Printed 17 March 2015 (MN LATEX style file v2.2) Giant comets and mass extinctions of life W.M. Napier1⋆ 1Buckingham Centre for Astrobiology, University of Buckingham, Buckingham MK18 1EG, UK Accepted 2014 December 16. Received 2014 December 12; in original form 2014 March 31 ABSTRACT I find evidence for clustering in age of well-dated impact craters over the last 500 Myr. At least nine impact episodes are identified, with durations whose upper limits are set by the dating accuracy of the craters. Their amplitudes and frequency are inconsis- tent with an origin in asteroid breakups or Oort cloud disturbances, but are consistent with the arrival and disintegration in near-Earth orbits of rare, giant comets, mainly in transit from the Centaur population into the Jupiter family and Encke regions. About 1 in 10 Centaurs in Chiron-like orbits enter Earth-crossing epochs, usually repeatedly, each such epoch being generally of a few thousand years duration. On time-scales of geological interest, debris from their breakup may increase the mass of the near-Earth interplanetary environment by two or three orders of magnitude, yielding repeated episodes of bombardment and stratospheric dusting. I find a strong correlation between these bombardment episodes and major biostratigraphic and geo- logical boundaries, and propose that episodes of extinction are most effectively driven by prolonged encounters with meteoroid streams during bombardment episodes. Pos- sible mechanisms are discussed. Key words: comets: general - interplanetary medium - meteorites, meteors, mete- oroids - zodiacal dust 1 INTRODUCTION tention has been paid to the issue of episodes of bombard- ment, although several such have been noted and claims The discovery of an excess of iridium at the Cretaceous- have been made of correlation with mass extinction (Keller Tertiary boundary of 65 Myr BP, and its interpretation as et al 2012; McGhee 1996). -
Implications of a New Paleomagnetic Pole From
Latinmag Letters, Volume 3, Special Issue (2013), PB16, 1-6. Proceedings Montevideo, Uruguay THE PANGEA CONUNDRUM: IMPLICATIONS OF A NEW PALEOMAGNETIC POLE FROM THE PERMO-TRIASSIC ARAGUAINHA IMPACT STRUCTURE (CENTRAL BRAZIL) Elder Yokoyama1*, Daniele Brandt1, Eric Tohver2, Ricardo Trindade1 1 Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, Rua do Matão, 1226, 05508-090, Brazil. 2 School of Earth and Environment, University of Western Australia, 35 Stirling Highway, Crawley, WA 6009, Australia ABSTRACT The configuration of the Pangea supercontinent has been a topic of intense debate for almost half a century, a controversy that stems from discrepancies between the geology-based Pangea A and the paleomagnetically- based Pangea B. Recent paleomagnetic compilations aimed at resolving this controversy have identified the poor quality of paleomagnetic data from Gondwana for late Permian times as a major obstacle. Specifically, the vast majority of Gondwanan poles come from sedimentary rocks that are prone to biases from compaction or are poorly dated. Here we present a new paleomagnetic pole for cratonic South America based on impact- melts from the 254.7 ± 2.5 Ma Araguainha impact structure, an unusual target for paleomagnetic studies. The impact-generated melt sheet and veins were sampled at 22 sites (137 samples) and provide a reliable paleomagnetic record, similar to that of volcanic rocks. Alternating field and thermal demagnetization indicate stable, usually univectorial magnetizations carried by both magnetite and hematite. All sites but one show a single paleomagnetic direction of normal polarity with a mean direction of Dec = 356.4°; Inc = -38.7°; N = 21; k = 91.1; α95 = 3.3°, yielding a paleomagnetic pole (AIS) at Lat = -83.7; Lon = 340.1; K = 83.5; A95 =3.5°; SB =8.3°. -
Pygocephalomorph Crustaceans from the Early Permian of Uruguay: Constraints on Taxonomy
Rev. bras. paleontol. 15(1):33-48, Janeiro/Abril 2012 © 2012 by the Sociedade Brasileira de Paleontologia doi:10.4072/rbp.2012.1.03 PYGOCEPHALOMORPH CRUSTACEANS FROM THE EARLY PERMIAN OF URUGUAY: CONSTRAINTS ON TAXONOMY GRACIELA PIÑEIRO, ELIZABETH MOROSI, ALEJANDRO RAMOS Departamento de Evolución de Cuencas, Facultad de Ciencias, Iguá, 4225, 11400, Montevideo, Uruguay. [email protected], [email protected], [email protected] FABRIZIO SCARABINO Museo Nacional de Historia Natural, 25 de Mayo, 582, 11000, Montevideo, Uruguay. [email protected] ABSTRACT – Hoplita ginsburgi comb. nov. (Fabre & Huard) is described from the Early Permian Mangrullo Formation of Uruguay. It is a large to very large pygocephalomorph characterized by a combination of characters that includes the presence of a round carapace bearing short, anterolateral, spine-like processes and a posteriorly extended, V-shaped cervical groove. Other traits include well-developed angular or round pleomeral pleurae bearing terminal spine-like processes, a tail fan with large and rounded uropod exopod, lacking diaresis, a roughly trapezoidal telson that gives support to small lateral spines and a relatively large triangular caudal spine. This species is also distinguished by the presence of a putative, simplified endophragmal skeleton, a structure not previously described in pygocephalomorphs, but present in fossil and extant higher crustaceans, where its function, although not so well understood, has been related to support for the limb musculature. Sexual dimorphism appears in Hoplita with the recognition of gonopods in males and seminal receptacles in the females. The studied specimens include moulting exuvia distinct from live individuals. The status of Notocarididae, the only currently recognized Gondwanan family, was examined, as well as the strength of the characters previously recognized as diagnostic. -
The Geological Record of Meteorite Impacts
THE GEOLOGICAL RECORD OF METEORITE IMPACTS Gordon R. Osinski Canadian Space Agency, 6767 Route de l'Aeroport, St-Hubert, QC J3Y 8Y9 Canada, Email: [email protected] ABSTRACT 2. FORMATION OF METEORITE IMPACT STRUCTURES Meteorite impact structures are found on all planetary bodies in the Solar System with a solid The formation of hypervelocity impact craters has surface. On the Moon, Mercury, and much of Mars, been divided, somewhat arbitrarily, into three main impact craters are the dominant landform. On Earth, stages [3] (Fig. 2): (1) contact and compression, (2) 174 impact sites have been recognized, with several excavation, and (3) modification. A further stage of more new craters being discovered each year. The “hydrothermal and chemical alteration” is also terrestrial impact cratering record is critical for our considered as a separate, final stage in the cratering understanding of impacts as it currently provides the process (e.g., [4]), and is also described below. only ground-truth data on which to base interpretations of the cratering record of other planets and moons. In this contribution, I summarize the processes and products of impact cratering and provide and an up-to-date assessment of the geological record of meteorite impacts. 1. INTRODUCTION It is now widely recognized that impact cratering is a ubiquitous geological process that affects all planetary objects with a solid surface (e.g., [1]). One only has to look up on a clear night to see that impact structures are the dominant landform on the Moon. The same can be said of all the rocky and icy bodies in the solar system that have retained portions of their earliest crust. -
New Sarcopterygians from the Carboniferous Poti Formation and from the Permian Rio Do Rasto Formation, Brazil
Rev. bras. paleontol. 19(3):401-406, Setembro/Dezembro 2016 © 2016 by the Sociedade Brasileira de Paleontologia doi: 10.4072/rbp.2016.3.05 NEW SARCOPTERYGIANS FROM THE CARBONIFEROUS POTI FORMATION AND FROM THE PERMIAN RIO DO RASTO FORMATION, BRAZIL RODRIGO TINOCO FIGUEROA, RAPHAEL MIGUEL & VALÉRIA GALLO Laboratório de Sistemática e Biogeografia, Departamento de Zoologia, Instituto de Biologia, UERJ, Rua São Francisco Xavier, 524, Maracanã, 20550-013, Rio de Janeiro, RJ, Brazil. [email protected], [email protected], [email protected] ABSTRACT – A new material of sarcopterygian fishes from the Mississippian of the Poti Formation and the Lopingian of the Rio do Rasto Formation are described here. The specimens consist of isolated scales, which show numerous thin and parallel growth lines, a pattern of ornamentation usually found in actinistians, differing from the Westoll-lines present in dipnoans. A precise identification of this new material was not possible, because the scales lack more accurate diagnostic features. The Mississippian occurrence spreads the distribution of coelacanthiforms in the Brazilian Paleozoic, which was restricted to the Permian. This material represents the oldest actinistian record in Brazil and the first Mississippian report of this group from South America. The occurrences from the Rio do Rasto Formation seems to have freshwater affinities, which was inferred by the depositional environment and associated biota. All these new data are important to the comprehension of coelacanths paleogeographical distribution during the Paleozoic in South America. Key words: coelacanths, scales, Poti Formation, Rio do Rasto Formation. RESUMO – Novos espécimes de sarcopterígios do Mississipiano da Formação Poti e do Lopingiano da Formação Rio do Rasto são aqui descritos.