Evaluating the Influence of Meteorite Impact Events on Global Potassium Feldspar Availability to the Atmosphere Since 600 Ma
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Cross-References ASTEROID IMPACT Definition and Introduction History of Impact Cratering Studies
18 ASTEROID IMPACT Tedesco, E. F., Noah, P. V., Noah, M., and Price, S. D., 2002. The identification and confirmation of impact structures on supplemental IRAS minor planet survey. The Astronomical Earth were developed: (a) crater morphology, (b) geo- 123 – Journal, , 1056 1085. physical anomalies, (c) evidence for shock metamor- Tholen, D. J., and Barucci, M. A., 1989. Asteroid taxonomy. In Binzel, R. P., Gehrels, T., and Matthews, M. S. (eds.), phism, and (d) the presence of meteorites or geochemical Asteroids II. Tucson: University of Arizona Press, pp. 298–315. evidence for traces of the meteoritic projectile – of which Yeomans, D., and Baalke, R., 2009. Near Earth Object Program. only (c) and (d) can provide confirming evidence. Remote Available from World Wide Web: http://neo.jpl.nasa.gov/ sensing, including morphological observations, as well programs. as geophysical studies, cannot provide confirming evi- dence – which requires the study of actual rock samples. Cross-references Impacts influenced the geological and biological evolu- tion of our own planet; the best known example is the link Albedo between the 200-km-diameter Chicxulub impact structure Asteroid Impact Asteroid Impact Mitigation in Mexico and the Cretaceous-Tertiary boundary. Under- Asteroid Impact Prediction standing impact structures, their formation processes, Torino Scale and their consequences should be of interest not only to Earth and planetary scientists, but also to society in general. ASTEROID IMPACT History of impact cratering studies In the geological sciences, it has only recently been recog- Christian Koeberl nized how important the process of impact cratering is on Natural History Museum, Vienna, Austria a planetary scale. -
Detecting and Avoiding Killer Asteroids
Target Earth! Detecting and Avoiding Killer Asteroids by Trudy E. Bell (Copyright 2013 Trudy E. Bell) ARTH HAD NO warning. When a mountain- above 2000°C and triggering earthquakes and volcanoes sized asteroid struck at tens of kilometers (miles) around the globe. per second, supersonic shock waves radiated Ocean water suctioned from the shoreline and geysered outward through the planet, shock-heating rocks kilometers up into the air; relentless tsunamis surged e inland. At ground zero, nearly half the asteroid’s kinetic energy instantly turned to heat, vaporizing the projectile and forming a mammoth impact crater within minutes. It also vaporized vast volumes of Earth’s sedimentary rocks, releasing huge amounts of carbon dioxide and sulfur di- oxide into the atmosphere, along with heavy dust from both celestial and terrestrial rock. High-altitude At least 300,000 asteroids larger than 30 meters revolve around the sun in orbits that cross Earth’s. Most are not yet discovered. One may have Earth’s name written on it. What are engineers doing to guard our planet from destruction? winds swiftly spread dust and gases worldwide, blackening skies from equator to poles. For months, profound darkness blanketed the planet and global temperatures dropped, followed by intense warming and torrents of acid rain. From single-celled ocean plank- ton to the land’s grandest trees, pho- tosynthesizing plants died. Herbivores starved to death, as did the carnivores that fed upon them. Within about three years—the time it took for the mingled rock dust from asteroid and Earth to fall out of the atmosphere onto the ground—70 percent of species and entire genera on Earth perished forever in a worldwide mass extinction. -
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. -
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. -
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). -
Using the Manicouagan Impact Crater to Calibrate the Cyclostratigraphy Of
Using the Manicouagan Impact Ejecta to Calibrate the Cyclostratigraphy of the Newark Basin Francis D. Winslow III1, E.Troy Rasbury1, Sidney R. Hemming2 1Department of Geosciences, Stony Brook University, Stony Brook, NY 11794-2100, 2Lamont-DohertyEarth Observatory of Columbia University, Palisades, NY 10964 Introduction The Newark Basin, which contains the Triassic-Early Jurassic Newark Supergroup, is one of the best-studied early Mesozoic stratigraphic successions. A high-resolution cyclostratigraphic and magnetostratigraphic framework has been developed for the Newark Basin that encompasses approximately 30 my. When combined with biostratigraphy, this high- resolution record allows for global correlation of the Newark Basin succession with other Mesozoic basins, as well as the marine record. However, the high-resolution framework and the resulting correlations are based upon the assumption that the cyclostratigraphy is periodic and that the periods are known. There are only a few radiometric ages to constrain this cyclostratigraphy, most of which are from sills and basalt flows of the Central Atlantic Magmatic Province (CAMP) that on the basis of biostratigraphy are near the very base of the Jurassic. All other ages are based on extrapolation using the well-developed McLaughlin cycles that are considered to be 404 ky in duration. Our unpublished U-Pb results from stromatolite calcite and phosphate coprolites yield precise ages that support the assumed periodicity of the cycles. However, the occurrence of radiometrically datable syndepositional material in the Newark Basin is barely exploited. The Manicouagan Impact event would have produced a syndepositional horizon that potentially provides an additional test of the age and thus the cycle periods. -
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). -
Cráteres E Impactos
Cráteres e Impactos Historia del conocimiento sobre cráteres e impactos Energía y presión de los impactos Mecánica de Cráteres Estructura y tipos de cráteres Leyes de Craterización Meteoritos e impactitas Criterios para la Identificación de Cráteres Consecuencias ambientales de los impactos Conteo de cráteres El evento de Carancas: ejemplo de Geología Planetaria Practicas: Google Earth - cráteres Conteo de cráteres y ajuste de curvas de edad Virtual Lab: Visualización de secciones finas de meteoritos Cut & Paste Impact Cratering Seminar – H. Jay Melosh Geology and Geophysics of the Solar System – Shane Byrne Impact Cratering – Virginia Pasek Explorer's Guide to Impact Craters! http://www.psi.edu/explorecraters/ Terrestrial Impact Structures: Observation and Modeling - Gordon Osinski Environmental Effects of Impact Events - Elisabetta Pierazzo Traces of Catastrophe: A Handbook of Shock-Metamorphic Effects in Terrestrial Meteorite Impact Structures – Bevan French – Smithsonian Institution Effects of Material Properties on Cratering - Kevin Housen - The Boeing Co. Sedimentary rocks in Finnish impact structures -pre-impact or post- impact? - J.Kohonen and M. Vaarma - Geological Survey of Finland History about impact craters The study of impact craters has a well-defined beginning: 1610 Galileo’s small telescope and limited field of view did not permit him to view the entire moon at once, so his global maps were distorted Nevertheless, he recognized a pervasive landform that he termed “spots” He described them as circular, rimmed depressions But declined to speculate on their origin Robert Hooke had a better telescope in 1665 Hooke make good drawings of Hipparchus and speculated on the origin of the lunar “pits”. Hooke considered impact, but dismissed it because he could not imagine a source for the impactors. -
ABSTRACT 1 Terrestrial Impact Craters
MAPPING TERRESTRIAL IMPACT CRATERS WITH THE TANDEM-X DIGITAL ELEVATION MODEL Manfred Gottwald1, Thomas Fritz1, Helko Breit1, Birgit Schättler1, Alan Harris2 1German Aerospace Center, Remote Sensing Technology Institute, Oberpfaffenhofen, D-82234 Wessling, Germany 2German Aerospace Center, Institute of Planetary Research, Rutherfordstr. 2, D-12489 Berlin, Germany ABSTRACT We use the global digital elevation model (DEM) generated in the TanDEM-X mission for map- ping the confirmed terrestrial impact structures in the Earth Impact Database of the Planetary and Space Science Center (PASSC) at the University of New Brunswick, Canada. The TanDEM- X mission generates a global DEM with unprecedented properties. The achieved global coverage together with the improved accuracy (in the sub-10 m range) and spatial resolution (12 m at the equator) opens new opportunities in impact crater research based on terrestrial space-borne remote sensing data. It permits both for simple and complex craters investigations of the mor- phology of the particular structure (rim height, central uplift, ring-like patterns, elevation pro- files) and of the surrounding terrain (local deformation, drainage patterns) of outstanding quali- ty. 1 Terrestrial Impact Craters Earth, in contrast, the crust underwent continuous modification due to various processes such as plate 1.1 Impact Crater Record tectonics, erosion, sedimentation and glaciation. This prevented the development of an unbiased impact Terrestrial impact craters are the relics of collisions of record. Only the ancient continental shields provide the Earth with Solar System objects of different sizes. opportunities for detecting very old impact structures. Such collisions were frequent in the distant past when In other areas, craters of a certain size have remained the Solar System was young but even today solid bod- sufficiently intact only if they were formed rather re- ies from interplanetary space occasionally hit the ter- cently or if their large size has prevented them from restrial surface. -
Evaluating the Influence of Meteorite Impact Events on Global Potassium Feldspar Availability to the Atmosphere Since 600 Ma
Research article Journal of the Geological Society Published online November 27, 2018 https://doi.org/10.1144/jgs2018-084 | Vol. 176 | 2019 | pp. 209–224 Evaluating the influence of meteorite impact events on global potassium feldspar availability to the atmosphere since 600 Ma B. C. Coldwell1,2 & M. J. Pankhurst1,2,3,4,5* 1 Instituto Tecnológico y de Energías Renovables (ITER), 38600 Granadilla de Abona, Santa Cruz de Tenerife, Spain 2 Instituto Volcanológico de Canarias (INVOLCAN), Calle Álvaro Martín Díaz 1, 38320 San Cristóbal de La Laguna, Santa Cruz de Tenerife, Spain 3 School of Materials, University of Manchester, Manchester M13 9PJ, UK 4 Research Complex at Harwell, Harwell Campus, Didcot OX11 0FA, UK 5 School of Earth and Environment, University of Leeds, Leeds LS2 9JT, UK B.C.C., 0000-0001-9240-6240; M.J.P., 0000-0001-6844-9822 * Correspondence: [email protected] Abstract: Potassium feldspar present in global mineral aerosol (<5%) plays a disproportionate role in modulating the microphysics of mixed-phase cloud. Via exceptional ice nucleation properties, it is capable of changing cloud properties and behaviour. Here we identify times of substantial and abrupt change in the global availability of potassium feldspar since 600 Ma. Normally, weathering and vegetation cover contribute to low availability, with clay dominating mineral aerosol. Periods of maximum availability are reasoned to follow the emplacement and remobilization of ejecta blankets from major meteorite impact events, before returning to background after some hundreds to thousands of years. We review the 44 largest confirmed craters and evaluate the potassium feldspar content of their target rocks, which range from c. -
The Siljan Ring in Central Sweden - a Window Into the Palaeozoic History of Baltoscandia
Geophysical Research Abstracts Vol. 14, EGU2012-11247-1, 2012 EGU General Assembly 2012 © Author(s) 2012 The Siljan Ring in central Sweden - a window into the Palaeozoic history of Baltoscandia O. Lehnert (1), G. Meinhold (2), S.M. Bergström (3), M. Calner (4), J.O.R. Ebbestad (5), S. Egenhoff (6), Å.M. Frisk (7), A.E.S. Högström (8), and J. Maletz (9) (1) GeoZentrum Nordbayern, Lithosphere Dynamics, University of Erlangen-Nürnberg, Schloßgarten 5, D-91054, Erlangen, Germany ([email protected]), (2) Sedimentology & Environmental Geology, Geoscience Centre, University of Göttingen, Goldschmidtstrasse 3, D-37077 Göttingen, Germany ([email protected]), (3) School of Earth Sciences, Division of Earth History, The Ohio State University, 125 S. Oval Mall, Columbus, Ohio 443210, USA ([email protected]), (4) Department of Geology, Lund University, Sölvegatan 12, SE-223 62 Lund, Sweden ([email protected]), (5) Museum of Evolution, Uppsala University, Norbyvägen 16, SE - 752 36 Uppsala, Sweden ([email protected]), (6) Department of Geosciences, Colorado State University, 322 Natural Resources Building, Fort Collins, CO 80523-1482, USA ([email protected]), (7) Paläontologisches Institut und Museum, Karl Schmid-Strasse 4, 8006 Zürich, Switzerland ([email protected]), (8) Tromsö University Museum, Natural Sciences, N-9037 Tromsö, Norway ([email protected]), (9) Institut für Geologische Wissenschaften, Freie Universität Berlin, Malteser Str. 74-100, Haus B, Raum 322, D-12249 Berlin, Germany ([email protected]) The Siljan meteorite crater, the largest known impact crater in Europe, is a main target of the research project ‘Concentric Impact Structures in the Palaeozoic (CISP)’, an integral of the Swedish Deep Drilling Program (SDDP). -
SILJAN AIR PARK PPL/IR EUROPE Siljan Air Park by Russell Myles N the Forests of Central Sweden Next to Lake Siljan Is the Small Airfield of Siljansnäs (ESVS)
PPL/IR EUROPE SILJAN AIR PARK PPL/IR EUROPE Siljan Air Park by Russell Myles n the forests of central Sweden next to Lake Siljan is the small airfield of Siljansnäs (ESVS). It is not very big, with just 850m of hard runway and a parallel 850m of grass, is daylight only and just has an air-to-ground frequency; no radar, approaches or ATC. It is however a great place to visit and if the weather means you need to exercise the privileges of your IR to get there then the nearby airfields at Mora and Borlänge both have ILS. ISiljansnäs is a lovely place to visit and has become a preferred jet all over the world lives about 30 miles north of Charlotte in North destination for pilots touring central Sweden. It has one distinctive Carolina. Danny’s airpark house is his home and his chipmunk is feature which sets it apart from almost all the other Swedish for fun. Here in Europe it seems that airpark homes are more likely airfields. It is not the flying club, although that offers gliding and to be second homes, used for holidays and the weekends. The Pilot powered flying, a regular social calendar and a fantastic fly in article’s author found the Vendée Air Park to be very quiet, with and airshow in early August. It is not the flying club sauna (every only a few people in residence at the time of visiting. We found the flying club should have a sauna!), the guest cabins or same when we took time to visit Siljansnäs in late May.