Siljan Ring Findings Remain Unchanged Since 1984
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Laser Argon Dating of Melt Breccias from the Siljan Impact Structure, Sweden: Implications for a Possible Relationship to Late Devonian Extinction Events
Meteoritics & Planetary Science 40, Nr 4, 591–607 (2005) Abstract available online at http://meteoritics.org Laser argon dating of melt breccias from the Siljan impact structure, Sweden: Implications for a possible relationship to Late Devonian extinction events Wolf U. REIMOLD1*, Simon P. KELLEY2, Sarah C. SHERLOCK2, Herbert HENKEL3, and Christian KOEBERL4 1Impact Cratering Research Group, School of Geosciences, University of the Witwatersrand, Private Bag 3, P. O. Wits 2050, Johannesburg, South Africa 2Department of Earth Sciences, Open University, Walton Hall, Milton Keynes MK7 6AA, UK 3Department of Land and Water Resources Engineering, Division of Engineering Geology and Geophysics, Royal Institute of Technology, Teknikringen 72, SE 100-44 Stockholm, Sweden 4Department of Geological Sciences, University of Vienna, Althanstrasse 14, A-1090 Vienna, Austria *Corresponding author. E-mail: [email protected] (Received 12 July 2004; revision accepted 08 February 2005) Abstract–In earlier studies, the 65–75 km diameter Siljan impact structure in Sweden has been linked to the Late Devonian mass extinction event. The Siljan impact event has previously been dated by K- Ar and Ar-Ar chronology at 342–368 Ma, with the commonly quoted age being 362.7 ± 2.2 Ma (2 σ, recalculated using currently accepted decay constants). Until recently, the accepted age for the Frasnian/Famennian boundary and associated extinction event was 364 Ma, which is within error limits of this earlier Siljan age. Here we report new Ar-Ar ages extracted by laser spot and laser step heating techniques for several melt breccia samples from Siljan (interpreted to be impact melt breccia). The analytical results show some scatter, which is greater in samples with more extensive alteration; these samples generally yield younger ages. -
A Detrital Zircon and Apatite Provenance Study of the Stac Fada Member and Wider St
On the track of a Scottish impact structure: a detrital zircon and apatite provenance study of the Stac Fada Member and wider Stoer Group, northwest Scotland Gavin G. Kenny1,2*, Gary J. O’Sullivan1, Stephen Alexander1, Michael J. Simms3, David M. Chew1 and Balz S. Kamber1,4 1Department of Geology, School of Natural Sciences, Trinity College Dublin, Dublin 2, Ireland 2Department of Geosciences, Swedish Museum of Natural History, SE-104 05 Stockholm, Sweden 3Department of Natural Sciences, National Museums Northern Ireland, Cultra, BT18 0EU Northern Ireland, UK 4School of Earth, Environmental and Biological Sciences, Queensland University of Technology, GPO Box 2434, Brisbane, QLD 4001, Australia *[email protected] Abstract The Stac Fada Member of the Stoer Group, within the Torridonian succession of northwest Scotland, is a melt-rich, impact-related deposit that has not been conclusively correlated with any known impact structure. However, a gravity low approximately 50 km east of the preserved Stac Fada Member outcrops has recently been proposed as the associated impact site. Here we aimed to shed light on the location of the impact structure through a provenance study of detrital zircon and apatite in five samples from the Stoer Group. Our zircon U-Pb data is dominated by Archaean grains (>2.5 Ga), consistent with earlier interpretations that the detritus was derived largely from local Lewisian Gneiss Complex, whereas the apatite data (the first for the Stoer Group) display a single major peak at ca. 1.7 Ga, consistent with regional Laxfordian metamorphism. The almost complete absence of Archaean-aged apatite is best explained by later heating of the >2.5 Ga Lewisian basement (the likely source region) above the closure temperature of the apatite U-Pb system (~375-450°C). -
EMD Shale Gas and Liquids Committee Annual Report, FY 2014
EMD Shale Gas and Liquids Committee Annual Report, FY 2014 Neil S. Fishman, Chair March 30, 2014 Vice Chairs: Brian Cardott, (Vice Chair, Government), Oklahoma Geological Survey, Norman, OK Harris Cander (Vice Chair, Industry), BP, Houston, TX Sven Egenhoff, (Vice Chair, University), Colorado State University, Fort Collins, CO Advisory Committee (in alphabetical order): Kent Bowker, Bowker Petroleum, The Woodlands, TX Ken Chew, IHS (retired), Perthsire, Scotland Thomas Chidsey, Utah Geological Survey, Salt Lake City, UT Russell Dubiel, U.S. Geological Survey, Denver, CO Catherine Enomoto, U.S. Geological Survey, Reston, VA William Harrison, Western Michigan University, Kalamazoo, MI Ursula Hammes, Bureau of Economic Geology, Austin, TX Shu Jiang, University of Utah, Salt Lake City, UT Margaret Keller, U.S. Geological Survey, Menlo Park, CA Julie LeFever, North Dakota Geological Survey, Grand Forks, ND Peng Li, Arkansas Geological Survey, Little Rock, AR Jock McCracken, Egret Consulting, Calgary, AB Stephen Nordeng, North Dakota Geological Survey, Grand Forks, ND Rich Nyahay, New York Museum, Albany, NY Stephen Sonnenberg, Colorado School of Mines, Golden, CO Michael D. Vanden Berg, Utah Geological Survey, Salt Lake City, UT Rachel Walker, Countrymark Energy Resources, LLC, Indianapolis, IN INTRODUCTION It is a pleasure to present this Annual Report from the EMD Shale Gas and Liquids Committee. This report contains information about specific shales across the U.S., Canada, Europe, China, as well as SE Asia from which hydrocarbons are currently being produced or shales that are of interest for hydrocarbon exploitation. The inclusion in this report of shales from which any hydrocarbon is produced reflects the expanded mission of the EMD Shale Gas and Liquids Committee to serve as a single point of access to technical information on shales regardless of the hydrocarbons produced from them (e.g., gas, oil, condensate). -
6Th Annual Jackson School of Geosciences Student Research Symposium February 4, 2017
6th Annual Jackson School of Geosciences Student Research Symposium February 4, 2017 Jackson School of Geosciences GSEC Graduate Student Executive Committee Welcome to the 6th Annual Jackson School Research Symposium It is with great pleasure we welcome you all to the 6th Annual Jackson School Research Symposium at UT-Austin! This symposium would not have been possible without the hard work of student volunteers, the support of faculty/research scientists, and generous support from ConocoPhillips. Thank you for taking part in supporting our students and growing research program within the Jackson School. Enjoy the posters! Schedule of Presentations and Events Breakfast, A.M. session poster set-up...............................................8:30 a.m. Early Career Graduate (ECG) posters......................................9:00-11:30 a.m. Late Career Masters (LCM) posters.........................................9:00-11:30 a.m. Lunch, A.M. session poster take-down.............................................11:30 a.m. P.M. session poster set-up................................................................12:30 p.m. Undergraduate (U) posters….....................................................1:00-3:30 p.m. Late Career PhD (LCPhD) posters.............................................1:00-3:30 p.m. Happy hour/judging............................................................................3:30 p.m. Awards/closing....................................................................................4:00 p.m. ii Table of Contents Program -
Pirstekartioista Keurusselällä Ja Maailmalla TEEMU ÖHMAN
Pirstekartioista Keurusselällä ja maailmalla TEEMU ÖHMAN li erittäin ilahduttavaa huomata, että kittävä vaikutus jatkotutkimusten ohjaamisessa lu- jo Marmon (1963, s. 16) mitä ilmei- paavimpiin kohteisiin. Geofysiikalla ei kuitenkaan simmin kuvaamia, joskaan ei tör- koskaan todisteta mahdollisen kraatterin synnystä mäyssyntyisiksi tulkitsemia Keurus- tai pirstekartioista sitä eikä tätä. Se, että törmäys- Oselän pirstekartioita on intouduttu tutkimaan mi- malli selittää muutoin käsittämättömiksi jäävät neralogisesta näkökulmasta (Kinnunen ja Hietala havainnot, joita “perinteisin” teorioin on turhaan 2009, jatkossa KH09). Myös mielipiteiden nopea yritetty ymmärtää, usein vuosikymmenien ajan, on vaihtuminen (KH09 vs. esimerkiksi Hietala ja Moi- varsin vahva viite mallin oikeellisuuden puolesta, lanen 2004, 2007, Pesonen et al . 2005, Ruotsalai- eikä suinkaan kerro siitä, etteikö muita selitysmal- nen et al . 2006 ja vielä Schmieder et al . 2009) on leja olisi yritetty näihin kohteisiin soveltaa. virkistävä poikkeus usein hyvin jääräpäisessä geo- KH09:n väite, että kiistattomia todisteita tör- tieteellisessä tutkimuksessa. Kuten KH09 toteavat- mäyksistä löydettäisiin vain “geologisesti melko kin, ei pirstekartioiden mineralogiaan ole maail- nuorista” kraattereista, on yksinkertaisesti väärä, mallakaan järin paljon huomiota kiinnitetty, ja pirs- ellei sitten lähdetä tieteenfilosofiseen hetteikköön tekartioiden synty on useammastakin teoriasta pohtimaan sitä, mikä on kiistaton todiste. Pääsään- huolimatta edelleen hämärän peitossa. KH09 esit- -
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. -
Lunar and Planetary Science XXIX 1379.Pdf
Lunar and Planetary Science XXIX 1379.pdf TEAGUE RING IMPACT STRUCTURE, WESTERN AUSTRALIA: GRAVITY SURVEY. J. B. Plescia, California Institute of Technology, Jet Propulsion Laboratory, Pasadena, CA 91109 ([email protected]) As part of an effort to better define the nature and the A reconnaissance gravity survey conducted in crustal structure of Teague Ring, a GPS controlled grav- 1986 (2) defined a significant negative anomaly over ity survey was undertaken in the austral winter of 1996. Teague Ring. To better define the structure a more de- The objective was to define the gravity field, identify any tailed survey was conducted in August 1996.. Gravity anomalies, and interpret that anomaly in terms of crustal station positions were established by a GPS survey; structure. positional information was collected for 10 minutes (600 Teague Ring is an impact structure in Western readings) and differentially corrected. The typical stan- Australia (25° 50’ S; 120° 55’ E). It has a diameter of 31 dard deviation of the station locations were 0.2 m hori- km and an age of ~1630 Ma. Teague Ring was first rec- zontal N, 0.2 m horizontal E, 0.6 m vertical with a vertical ognized by Butler (1) and various models of origin have PDOP mean of 3.3. The datum for reduction of the GPS been proposed. The most recent detailed work was un- data was AGD 1966. Gravity values were measured using dertaken by Eugene and Carolyn Shoemaker, but it has a Lacoste Romberg gravity meter (#G-1035). Approxi- been published only in limited form (2). -
Appendix a Recovery of Ejecta Material from Confirmed, Probable
Appendix A Recovery of Ejecta Material from Confirmed, Probable, or Possible Distal Ejecta Layers A.1 Introduction In this appendix we discuss the methods that we have used to recover and study ejecta found in various types of sediment and rock. The processes used to recover ejecta material vary with the degree of lithification. We thus discuss sample processing for unconsolidated, semiconsolidated, and consolidated material separately. The type of sediment or rock is also important as, for example, carbonate sediment or rock is processed differently from siliciclastic sediment or rock. The methods used to take and process samples will also vary according to the objectives of the study and the background of the investigator. We summarize below the methods that we have found useful in our studies of distal impact ejecta layers for those who are just beginning such studies. One of the authors (BPG) was trained as a marine geologist and the other (BMS) as a hard rock geologist. Our approaches to processing and studying impact ejecta differ accordingly. The methods used to recover ejecta from unconsolidated sediments have been successfully employed by BPG for more than 40 years. A.2 Taking and Handling Samples A.2.1 Introduction The size, number, and type of samples will depend on the objective of the study and nature of the sediment/rock, but there a few guidelines that should be followed regardless of the objective or rock type. All outcrops, especially those near industrialized areas or transportation routes (e.g., highways, train tracks) need to be cleaned off (i.e., the surface layer removed) prior to sampling. -
ANIC IMPACTS: MS and IRONMENTAL P ONS Abstracts Edited by Rainer Gersonde and Alexander Deutsch
ANIC IMPACTS: MS AND IRONMENTAL P ONS APRIL 15 - APRIL 17, 1999 Alfred Wegener Institute for Polar and Marine Research Bremerhaven, Germany Abstracts Edited by Rainer Gersonde and Alexander Deutsch Ber. Polarforsch. 343 (1999) ISSN 01 76 - 5027 Preface .......3 Acknowledgements .......6 Program ....... 7 Abstracts P. Agrinier, A. Deutsch, U. Schäre and I. Martinez: On the kinetics of reaction of CO, with hot Ca0 during impact events: An experimental study. .11 L. Ainsaar and M. Semidor: Long-term effect of the Kärdl impact crater (Hiiumaa, Estonia) On the middle Ordovician carbonate sedimentation. ......13 N. Artemieva and V.Shuvalov: Shock zones on the ocean floor - Numerical simulations. ......16 H. Bahlburg and P. Claeys: Tsunami deposit or not: The problem of interpreting the siliciclastic K/T sections in northeastern Mexico. ......19 R. Coccioni, D. Basso, H. Brinkhuis, S. Galeotti, S. Gardin, S. Monechi, E. Morettini, M. Renard, S. Spezzaferri, and M. van der Hoeven: Environmental perturbation following a late Eocene impact event: Evidence from the Massignano Section, Italy. ......21 I von Dalwigk and J. Ormö Formation of resurge gullies at impacts at sea: the Lockne crater, Sweden. ......24 J. Ebbing, P. Janle, J, Koulouris and B. Milkereit: Palaeotopography of the Chicxulub impact crater and implications for oceanic craters. .25 V. Feldman and S.Kotelnikov: The methods of shock pressure estimation in impacted rocks. ......28 J.-A. Flores, F. J. Sierro and R. Gersonde: Calcareous plankton stratigraphies from the "Eltanin" asteroid impact area: Strategies for geological and paleoceanographic reconstruction. ......29 M.V.Gerasimov, Y. P. Dikov, 0 . I. Yakovlev and F.Wlotzka: Experimental investigation of the role of water in the impact vaporization chemistry. -
Fynd Av Bergarter Bildade Vid Meteoritnedslaget I Siljansområdet
Fynd av bergarter bildade vid meteoritnedslaget i Siljansområdet Jan-Olov Svedlund & Thomas Lundqvist december 2010 SGU-rapport 2010:21 Sveriges geologiska undersökning Box 670, 751 28 Uppsala tel: 018-17 90 00 fax: 018-17 92 10 e-post: [email protected] www.sgu.se 1(26) INNEHÅLL Inledning 2 Berggrunden i Siljanstrakten 2 Jordarterna i Siljanstrakten 5 Block av smältbergart nära Ingärdningsbodarna 5 Tuffartad bergart från bergtäkt i Bergkarlås 12 Sammanfattning 14 Litteratur 14 Appendix 17 Omslagsbilden visar en sten från Ingärdningsbodarna med partier av impaktsmälta eller pseudotakylit (mörkbrun till grå) i röd Siljansgranit. 2(26) INLEDNING Vid Sveriges geologiska undersöknings (SGUs) fältarbeten med dokumentation av jordarterna i norra Dalarna påträffade en av oss (JOS) ett flertal block av en smältbergart (s.k. pseudotakylit) som bildats vid det stora meteoritnedslag som skedde i Siljanstrakten under devonperioden. Blocken finns på ett hygge nära Ingärdningsbodarna ca 17 km öster om Mora. Ett par av dem finns numera uppställda i ett vägskäl invid hygget, på en plats med koordinaterna 6764740/1448080 i Rikets Nät (RT 90), samt latitud och longitud 60°59’46’’ resp. 14°50’55’’. Intill blocken finns sedan hösten 2009 en informationstavla uppställd. Ett annat fynd av en bergart som sannolikt också är bildad vid meteoritnedslaget gjordes vid SGUs dokumentationsarbeten i en större bergtäkt vid Bergkarlås. Här rör det sig om en tuffliknande bergart i traktens Järnagranit. Stort tack till Prof. Kord Ernstson, Fakultät für Geowissenschaften, Universität Würzburg, som i appendix gjort en bedömning av slipprover från Siljansområdet och jämförelser med några kända meteoritkratrar. Han har generöst ställt sitt utlåtande till vårt förfogande. -
Discovery of a Meteoritic Ejecta Layer Containing Unmelted Impactor Fragments at the Base of Paleocene Lavas, Isle of Skye, Scotland
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by NERC Open Research Archive Discovery of a meteoritic ejecta layer containing unmelted impactor fragments at the base of Paleocene lavas, Isle of Skye, Scotland 1 1 2 3 4 5 Simon M. Drake *, Andrew D. Beard , Adrian P. Jones , David J. Brown , A. Dominic Fortes , Ian L. Millar , Andrew Carter1, Jergus Baca1, and Hilary Downes1 1School of Earth and Planetary Sciences, Birkbeck College, University of London, Malet Street, Bloomsbury, London WC1E 7HX, UK 2Department of Earth Sciences, University College London, Gower Street, London WC1E 6BT, UK 3School of Geographical and Earth Sciences, University of Glasgow, Lilybank Gardens, Glasgow G12 8QQ, UK 4ISIS Neutron Facility, Rutherford Appleton Laboratory, Harwell Science and Innovation Campus, Chilton, Didcot, Oxfordshire OX11 OQX, UK 5British Geological Survey, Natural Environment Research Council, Keyworth, Nottingham NG12 5GC, UK ABSTRACT extensive comparative geochemistry (see the Evidence for meteorite impacts in the geological record may include the presence of GSA Data Repository1). shocked minerals, spherule layers, and geochemical anomalies. However, it is highly unusual to find unmelted crystals from the actual impactor within an ejecta layer. Here we detail the FIELD RELATIONS AND CHEMISTRY first recorded occurrence of vanadium-rich osbornite (TiVN) on Earth, from two sites on Skye, OF METEORITIC EJECTA LAYER northwest Scotland, which are interpreted as part of a meteoritic ejecta layer. TiVN has only DEPOSITS AT SITES 1 AND 2 previously been reported as dust from comet Wild 2, but on Skye it has been identified as an The Isle of Skye forms part of the British unmelted phase. -
Curriculum Vitae
Dustin E. Sweet Curriculum Vitae (updated 9/1/2020) Department of Geosciences, Science Building, Room 318, Texas Tech University, Lubbock, TX 79409-1053 Contact information: Name: Dustin Edman Sweet E-mail: [email protected] Home Phone: (405) 659-5007 Office Phone: (806) 834-8390 Education 2003-2009 University of Oklahoma, School of Geology and Geophysics, PhD. in Geology Dissertation title: Glaciation in Equatorial Pangaea: Testing the hypothesis in the Pennsylvanian- Permian Fountain Formation (Colorado). Advisor: Dr. Gerilyn S. Soreghan 2000-2003 Boise State University, Department of Geology, M.S. in Geology Thesis title: Tectonostratigraphy of the Central Pequop Mountains, Elko County, Nevada. Advisor: Dr. Walter S. Snyder 1996-2000 Boise State University, Department of Geology, B.S. in Geology Thesis title: Jurassic Sedimentary Sequence in the Izee Terrane of West-Central, Idaho. Advisor: Dr. C.J. Northrup Employment & Appointments 2020-Present: Undergraduate Advisor, Department of Geosciences, Texas Tech University 2017-Present: Journal of Sedimentary Research, Associate Editor 2017-Present: Texas Tech University, Associate Professor 2017-2019: Geology Theme Leader, GSCO2, DOE Energy Frontier Research Center 2011-2017: Texas Tech University, Assistant Professor 2009-2011: Chevron Energy Technology Company, New Ventures Courses Taught Texas Tech University Sedimentology & Stratigraphy, Sequence Stratigraphy, Sedimentary Geology of Carbonates, Sedimentary Processes, Field Geology of Carbonates, Field Methods in Sedimentary Geology, Hydrocarbon Exploration Methods, Application of Hydrocarbon Exploration Methods University of Oklahoma Stratigraphy and Structure for Petroleum Engineers Boise State University Sedimentary Petrology & Petrography, Sedimentation & Stratigraphy Research Funding (Awards: $425,718) Sweet, D.E. (Principal 100% effort), Supplement from Capture and Storage of CO2, Energy Frontier Research Center, Sponsored by the Department of Energy, Awarded, $13,960 (August 1, 2018-July 31, 2019).