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Durham E-Theses
Durham E-Theses Shock metamorphism of potassic feldspars Robertson, P. B. How to cite: Robertson, P. B. (1973) Shock metamorphism of potassic feldspars, Durham theses, Durham University. Available at Durham E-Theses Online: http://etheses.dur.ac.uk/8594/ Use policy The full-text may be used and/or reproduced, and given to third parties in any format or medium, without prior permission or charge, for personal research or study, educational, or not-for-prot purposes provided that: • a full bibliographic reference is made to the original source • a link is made to the metadata record in Durham E-Theses • the full-text is not changed in any way The full-text must not be sold in any format or medium without the formal permission of the copyright holders. Please consult the full Durham E-Theses policy for further details. Academic Support Oce, Durham University, University Oce, Old Elvet, Durham DH1 3HP e-mail: [email protected] Tel: +44 0191 334 6107 http://etheses.dur.ac.uk SHOCK METAMORPHISM OF POTASSIC FELDSPARS A thesis submitted for the degree of Doctor of Philosophy in the University of Durham P.B. Robertson Graduate Society October, 1973 ABSTRACT Hypervelocity meteorite impact produces transient pressures as high as several megabars and temperatures in excess of 1500°C. Shock metamorphism describes the effects upon the target rocks, effects most distinctive in the range approximately 100-600kb. Shock deformation produced in potassic feldspars at three terrestrial craters and in experimentally shocked K-spar have been examined. Pressures in natural material were estimated from deformation of coexisting quartz and plagioclase, and in experiments pressures were calculated using impedance matching. -
Terrestrial Impact Structures Provide the Only Ground Truth Against Which Computational and Experimental Results Can Be Com Pared
Ann. Rev. Earth Planet. Sci. 1987. 15:245-70 Copyright([;; /987 by Annual Reviews Inc. All rights reserved TERRESTRIAL IMI!ACT STRUCTURES ··- Richard A. F. Grieve Geophysics Division, Geological Survey of Canada, Ottawa, Ontario KIA OY3, Canada INTRODUCTION Impact structures are the dominant landform on planets that have retained portions of their earliest crust. The present surface of the Earth, however, has comparatively few recognized impact structures. This is due to its relative youthfulness and the dynamic nature of the terrestrial geosphere, both of which serve to obscure and remove the impact record. Although not generally viewed as an important terrestrial (as opposed to planetary) geologic process, the role of impact in Earth evolution is now receiving mounting consideration. For example, large-scale impact events may hav~~ been responsible for such phenomena as the formation of the Earth's moon and certain mass extinctions in the biologic record. The importance of the terrestrial impact record is greater than the relatively small number of known structures would indicate. Impact is a highly transient, high-energy event. It is inherently difficult to study through experimentation because of the problem of scale. In addition, sophisticated finite-element code calculations of impact cratering are gen erally limited to relatively early-time phenomena as a result of high com putational costs. Terrestrial impact structures provide the only ground truth against which computational and experimental results can be com pared. These structures provide information on aspects of the third dimen sion, the pre- and postimpact distribution of target lithologies, and the nature of the lithologic and mineralogic changes produced by the passage of a shock wave. -
The Sudbury Basin, the Southern Province, the Grenville Front, and the Penokean Orogeny
The Sudbury Basin, the Southern Province, the Grenville Front, and the Penokean Orogeny STEPHAN J. BROCOUM* IAN W. D. DALZIEL** Lamont-Doherty Geological Observatory of Columbia University, Palisades, New York 10964 ABSTRACT The Sudbury Basin in the Canadian Shield has been proposed as a meteorite impact site subsequently deformed by en- dogenic tectonism. Detailed study of the structural geology strengthens this hypothesis and strongly suggests that the deformation of the basin was coeval with major folding and flattening (2.0 to 1.6 b.y. ago) of the rocks of the eastern Southern province and the northwesternmost Gren- ville province. The structural geometry indicates that most of these rocks have a similar strain history. Finite-strain analysis of deformed concretions within the Sudbury Basin sug- gests that originally it was almost circular in outline. Key words: structural geology, deformation, finite-strain indicators, folds, impact features, meteor crater, orogeny, Precambrian, structural analysis, tectonic Figure 1. Geological setting of the Sudbury Basin. fabric. sublayer (Souch and Podolsky, 1969), 1972) or suevite breccia (Peredery, 1972) INTRODUCTION which apparently also intrudes the country has increased the number of workers who The Sudbury Basin, Ontario, is situated rock as radial and concentric dikes called believe that the Sudbury Basin was formed just north of Lake Huron near the intersec- offsets (Fig. 2; Naldrett and others, 1971). at least in part by the impact of a hyper- tion of the Superior, Southern, and Gren- The sublayer and offsets of the irruptive velocity bolide. ville provinces of the Canadian Shield (Fig. are, at present, the world's largest single Geologists who argue against the meteor- 1). -
Chapter 6 Lawn Hill Megabreccia
Chapter 6 Lawn Hill Megabreccia Chapter 6 Catastrophic mass failure of a Middle Cambrian platform margin, the Lawn Hill Megabreccia, Queensland, Australia Leonardo Feltrin 6-1 Chapter 6 Lawn Hill Megabreccia Acknowledgement of Contributions N.H.S. Oliver – normal supervisory contributions Leonardo Feltrin 6-2 Chapter 6 Lawn Hill Megabreccia Abstract Megabreccia and related folds are two of the most spectacular features of the Lawn Hill Outlier, a small carbonate platform of Middle Cambrian age, situated in the northeastern part of the Georgina Basin, Australia. The megabreccia is a thick unit (over 200 m) composed of chaotic structures and containing matrix-supported clasts up to 260 m across. The breccia also influenced a Mesoproterozoic basement, which hosts the world class Zn-Pb-Ag Century Deposit. Field-studies (undertaken in the mine area), structural 3D modelling and stable isotopic data were used to assess the origin and timing of the megabreccia, and its relationship to the tectonic framework. Previous workers proposed the possible linkage of the structural disruption to an asteroid impact, to justify the extremely large clasts and the conspicuous basement interaction. However, the megabreccia has comparable clast size to some of the largest examples of sedimentary breccias and synsedimentary dyke intrusions in the world. Together with our field and isotope data, the reconstruction of the sequence of events that led to the cratonization of the Centralian Superbasin supports a synsedimentary origin for the Lawn Hill Megabreccia. However, later brittle faulting and veining accompanying strain localisation within the Thorntonia Limestones may represent post-sedimentary, syntectonic deformation, possibly linked to the late Devonian Alice Springs Orogeny. -
Hydrothermal Alteration at the Lonar Lake Impact Structure, India: Implications for Impact Cratering on Mars
Meteoritics & Planetary Science 38, Nr 3, 365–381 (2003) Abstract available online at http://meteoritics.org Hydrothermal alteration at the Lonar Lake impact structure, India: Implications for impact cratering on Mars Justin J. HAGERTY* and Horton E. NEWSOM Institute of Meteoritics, Department of Earth & Planetary Sciences, University of New Mexico, Albuquerque, New Mexico 87131, USA *Corresponding author. E-mail: [email protected] (Received 12 June 2002; revision accepted 20 February 2003) Abstract–The 50,000 year old, 1.8 km diameter Lonar crater is one of only two known terrestrial craters to be emplaced in basaltic target rock (the 65 million year old Deccan Traps). The composition of the Lonar basalts is similar to martian basaltic meteorites, which establishes Lonar as an excellent analogue for similarly sized craters on the surface of Mars. Samples from cores drilled into the Lonar crater floor show that there are basaltic impact breccias that have been altered by post-impact hydrothermal processes to produce an assemblage of secondary alteration minerals. Microprobe data and X-ray diffraction analyses show that the alteration mineral assemblage consists primarily of saponite, with minor celadonite, and carbonate. Thermodynamic modeling and terrestrial volcanic analogues were used to demonstrate that these clay minerals formed at temperatures between 130°C and 200°C. By comparing the Lonar alteration assemblage with alteration at other terrestrial craters, we conclude that the Lonar crater represents a lower size limit for impact-induced hydrothermal activity. Based on these results, we suggest that similarly sized craters on Mars have the potential to form hydrothermal systems, as long as liquid water was present on or near the martian surface. -
Impact Cratering
6 Impact cratering The dominant surface features of the Moon are approximately circular depressions, which may be designated by the general term craters … Solution of the origin of the lunar craters is fundamental to the unravel- ing of the history of the Moon and may shed much light on the history of the terrestrial planets as well. E. M. Shoemaker (1962) Impact craters are the dominant landform on the surface of the Moon, Mercury, and many satellites of the giant planets in the outer Solar System. The southern hemisphere of Mars is heavily affected by impact cratering. From a planetary perspective, the rarity or absence of impact craters on a planet’s surface is the exceptional state, one that needs further explanation, such as on the Earth, Io, or Europa. The process of impact cratering has touched every aspect of planetary evolution, from planetary accretion out of dust or planetesimals, to the course of biological evolution. The importance of impact cratering has been recognized only recently. E. M. Shoemaker (1928–1997), a geologist, was one of the irst to recognize the importance of this process and a major contributor to its elucidation. A few older geologists still resist the notion that important changes in the Earth’s structure and history are the consequences of extraterres- trial impact events. The decades of lunar and planetary exploration since 1970 have, how- ever, brought a new perspective into view, one in which it is clear that high-velocity impacts have, at one time or another, affected nearly every atom that is part of our planetary system. -
Geochemical Characterization of Moldavites from a New Locality, the Cheb Basin, Czech Republic
Geochemical characterization of moldavites from a new locality, the Cheb Basin, Czech Republic Item Type Article; text Authors Řanda, Zdeněk; Mizera, Jiři; Frána, Jaroslav; Kučera, Jan Citation Řanda, Z., Mizera, J., Frána, J. and Kučera, J. (2008), Geochemical characterization of moldavites from a new locality, the Cheb Basin, Czech Republic. Meteoritics & Planetary Science, 43(3), 461-477. DOI 10.1111/j.1945-5100.2008.tb00666.x Publisher The Meteoritical Society Journal Meteoritics & Planetary Science Rights Copyright © The Meteoritical Society Download date 30/09/2021 11:07:40 Item License http://rightsstatements.org/vocab/InC/1.0/ Version Final published version Link to Item http://hdl.handle.net/10150/656405 Meteoritics & Planetary Science 43, Nr 3, 461–477 (2008) AUTHOR’S PROOF Abstract available online at http://meteoritics.org Geochemical characterization of moldavites from a new locality, the Cheb Basin, Czech Republic ZdenÏk ÿANDA1, Ji¯í MIZERA1, 2*, Jaroslav FRÁNA1, and Jan KU»ERA1 1Nuclear Physics Institute, Academy of Sciences of the Czech Republic, 250 68 ÿež, Czech Republic 2Institute of Rock Structure and Mechanics, Academy of Sciences of the Czech Republic, V HolešoviËkách 41, 182 09 Praha 8, Czech Republic *Corresponding author. E-mail: [email protected] (Received 02 June 2006; revision accepted 15 July 2007) Abstract–Twenty-three moldavites from a new locality, the Cheb Basin in Western Bohemia, were analyzed by instrumental neutron activation analysis for 45 major and trace elements. Detailed comparison of the Cheb Basin moldavites with moldavites from other substrewn fields in both major and trace element composition shows that the Cheb Basin is a separate substrewn field. -
Multiple Fluvial Reworking of Impact Ejecta—A Case Study from the Ries Crater, Southern Germany
Multiple fluvial reworking of impact ejecta--A case study from the Ries crater, southern Germany Item Type Article; text Authors Buchner, E.; Schmieder, M. Citation Buchner, E., & Schmieder, M. (2009). Multiple fluvial reworking of impact ejecta—A case study from the Ries crater, southern Germany. Meteoritics & Planetary Science, 44(7), 1051-1060. DOI 10.1111/j.1945-5100.2009.tb00787.x Publisher The Meteoritical Society Journal Meteoritics & Planetary Science Rights Copyright © The Meteoritical Society Download date 06/10/2021 20:56:07 Item License http://rightsstatements.org/vocab/InC/1.0/ Version Final published version Link to Item http://hdl.handle.net/10150/656594 Meteoritics & Planetary Science 44, Nr 7, 1051–1060 (2009) Abstract available online at http://meteoritics.org Multiple fluvial reworking of impact ejecta—A case study from the Ries crater, southern Germany Elmar BUCHNER* and Martin SCHMIEDER Institut für Planetologie, Universität Stuttgart, 70174 Stuttgart, Germany *Corresponding author. E-mail: [email protected] (Received 21 July 2008; revision accepted 12 May 2009) Abstract–Impact ejecta eroded and transported by gravity flows, tsunamis, or glaciers have been reported from a number of impact structures on Earth. Impact ejecta reworked by fluvial processes, however, are sparsely mentioned in the literature. This suggests that shocked mineral grains and impact glasses are unstable when eroded and transported in a fluvial system. As a case study, we here present a report of impact ejecta affected by multiple fluvial reworking including rounded quartz grains with planar deformation features and diaplectic quartz and feldspar glass in pebbles of fluvial sandstones from the “Monheimer Höhensande” ~10 km east of the Ries crater in southern Germany. -
The 3D.Y Knom Example Is /1"<
t Sixth International Congress on Glass - Washington, D. C., 1962. Fossil Glasses Produced by Inpact of Meteorites, Asteroids 2nd Possibly Comets with the Planet Xarth* A. J. Zzhen :&uon Insticute, Pittsburgh, ?ennsylvania (U. S. A. ) Sunnary / (to be trmslzted izto Frerzh and German) - i in recent thes one of the nost intriging aysteries of geGlogy has ceen the occurrence of aerodgnasicdly-shaped glasses on five continents of the earth. Tnese glasses mder discussion are obviously not of f-d- guritic origin. 3ecent research indicates that these glasses laom as tektites are the result of meteorite, esteroid, or sossibly comet hpact. Lqact glass?s, io generzl, differ Tram volcanic glasses in that they are lo;;.tr in ?,iater zontent, have laver gallium and germiun ccntents, and are rot necessarily ia mgnaticalljr unstable continental areas. These hpac- tites may be divided as follovs: (1)Glasses found in or near terrestrial neteorite craters. These glasses usually contain numerous s-,'nerules 02 nickel-iron, coesite, chunlks of partially melted meteoritic inatter and even stishovite. Shattered or fractured melted mi-nerals such as quarts are comxonly gresent. Aerodpaaic-shaping nay or nay not be present in this t-ne. &m?les are Canyon Diablo and Wabar Crster glasses. (2) Impzct- glasses zssociated with craters uitn no evidence of meteoritic mterial i? the @.ass or surrounding the explosisn site. The 3d.y knom example is /1"< Tnis vork vas supported by Xatiocal A-eroEautizs and Space P.dministretioq,$ 3esezrch Grant NsG-37-6O Supplement 1-62. Page 2 glass associated with AoueUoul Crater in the Western Sahara Desert. -
The High-Pressure Mineral Inventory of Shock Veins from the Steen River Impact Structure
46th Lunar and Planetary Science Conference (2015) 2512.pdf The high-pressure mineral inventory of shock veins from the Steen River impact structure. Walton E.L., Sharp T. G. and Hu J. 1MacEwan University, Department of Physical Sciences, 10700 104 Ave, Edmonton, AB, T5J 2S2, Canada ([email protected] / [email protected] ), 2University of Alberta, Department of Earth & Atmospheric Sciences, Edmonton, AB, T6G 2E3, Canada. 3Arizona State University, School of Earth & Space Ex- ploration,Tempe, AZ 85287-1404, USA. Introduction: The Steen River impact struc- equipped with five WDS spectrometers. Raw data ture (SRIS; 59o31'N, 117o39’W) is a buried complex were corrected using the ZAF procedure. The excel crater with an apparent diameter of ~25 km [1]. The spreadsheets of [6,7] where used to recast chemical SRIS is the largest known impact structure in the analyses of amphiboles and garnets following the IMA Western Canada Sedimentary Basin and is a producer reccomentations. Micro-Raman spectra of various and host of oil and gas reservoirs [1]. The target rocks phases were obtained with point measurements, using comprise a 70 m layer of Missippian calcareous shale a Bruker SENTERRA instrument. The 100X objective underlain by a thick (1530 m) sequence of Devonian of a petrographic microscope was used to focus the marine sedimentary rocks including carbonates and excitation laser beam (532 nm line of Ar+ laser) to a evaporates. This ~1.6 km thick sedimentary cover focal spot size of ~1 µm. TEM sections will be pre- overlies Precambrian basement rocks (primarily gran- pared using an FEI Nova200 NanoFab dual-beam FIB, ite / gneiss / granodiorite). -
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. -
The Recognition of Terrestrial Impact Structures
Bulletin of the Czech Geological Survey, Vol. 77, No. 4, 253–263, 2002 © Czech Geological Survey, ISSN 1210-3527 The recognition of terrestrial impact structures ANN M. THERRIAULT – RICHARD A. F. GRIEVE – MARK PILKINGTON Natural Resources Canada, Booth Street, Ottawa, Ontario, KIA 0ES Canada; e-mail: [email protected] Abstract. The Earth is the most endogenically active of the terrestrial planets and, thus, has retained the poorest sample of impacts that have occurred throughout geological time. The current known sample consists of approximately 160 impact structures or crater fields. Approximately 30% of known impact structures are buried and were initially detected as geophysical anomalies and subsequently drilled to provide geologic samples. The recognition of terrestrial impact structures may, or may not, come from the discovery of an anomalous quasi-circular topographic, geologic or geo- physical feature. In the geologically active terrestrial environment, anomalous quasi-circular features, however, do not automatically equate with an impact origin. Specific samples must be acquired and the occurrence of shock metamorphism, or, in the case of small craters, meteoritic fragments, must be demonstrated before an impact origin can be confirmed. Shock metamorphism is defined by a progressive destruction of the original rock and mineral structure with increasing shock pressure. Peak shock pressures and temperatures produced by an impact event may reach several hundreds of gigaPascals and several thousand degrees Kelvin, which are far outside the range of endogenic metamorphism. In addition, the application of shock- wave pressures is both sudden and brief. Shock metamorphic effects result from high strain rates, well above the rates of norma l tectonic processes.