Keurusselkä - a New Impact Structure in Central Finland
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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. -
Extraordinary Rocks from the Peak Ring of the Chicxulub Impact Crater: P-Wave Velocity, Density, and Porosity Measurements from IODP/ICDP Expedition 364 ∗ G.L
Earth and Planetary Science Letters 495 (2018) 1–11 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl Extraordinary rocks from the peak ring of the Chicxulub impact crater: P-wave velocity, density, and porosity measurements from IODP/ICDP Expedition 364 ∗ G.L. Christeson a, , S.P.S. Gulick a,b, J.V. Morgan c, C. Gebhardt d, D.A. Kring e, E. Le Ber f, J. Lofi g, C. Nixon h, M. Poelchau i, A.S.P. Rae c, M. Rebolledo-Vieyra j, U. Riller k, D.R. Schmitt h,1, A. Wittmann l, T.J. Bralower m, E. Chenot n, P. Claeys o, C.S. Cockell p, M.J.L. Coolen q, L. Ferrière r, S. Green s, K. Goto t, H. Jones m, C.M. Lowery a, C. Mellett u, R. Ocampo-Torres v, L. Perez-Cruz w, A.E. Pickersgill x,y, C. Rasmussen z,2, H. Sato aa,3, J. Smit ab, S.M. Tikoo ac, N. Tomioka ad, J. Urrutia-Fucugauchi w, M.T. Whalen ae, L. Xiao af, K.E. Yamaguchi ag,ah a University of Texas Institute for Geophysics, Jackson School of Geosciences, Austin, USA b Department of Geological Sciences, Jackson School of Geosciences, Austin, USA c Department of Earth Science and Engineering, Imperial College, London, UK d Alfred Wegener Institute Helmholtz Centre of Polar and Marine Research, Bremerhaven, Germany e Lunar and Planetary Institute, Houston, USA f Department of Geology, University of Leicester, UK g Géosciences Montpellier, Université de Montpellier, France h Department of Physics, University of Alberta, Canada i Department of Geology, University of Freiburg, Germany j SM 312, Mza 7, Chipre 5, Resid. -
Shatter Cone and Its Surface Mesh-Structure Formed by Impact
SHATTER CONE AND ITS SURFACE MESHED- STRUCTURE FORMED BY IMPACT MELT-GASIFICATION IN XISHAN TAIHU LAKE CHINA H.N. Wang1, Y. Chen1, X.F. Shen1 L.Y. Zhou1 and Y.W. Wang2 11Department of Earth & Planetary Sciences, Nanjing University, Nanjing, China 210093 ([email protected]) 2 Department of Natural Resources and Environmental Sciences, University of Illinois at Urbana-Champaign, Champaign Introduction: Meshed--structure shatter cone: Discuss ion: Shatter cones are represented by a range of curved to The height of these cones is generally 50 to 70 cm. The 1. Meshed-structure are related to the melt- curvilinear fractures decorated with divergent striations. striation radiates from the original point at the top of cone, gasification of carbonates target rock: Striations radiate from an apex of a conical feature or from a similar to the longitude meridian. Meanwhile, cone surface Carbonates are brittle, fusible and volatile. Under the narrow apical area. Shatter cones are the only distinct meso shock wave, it is easy to be granulated. Its melting point presents hoopline around the cone. (Fig.D) The grid on is as low as 500-600°C. When the shock wave pass to macroscopic recognition criterion for impact structures. cone surface is generally in centimeter scale (2-4cm x Despite being known for 110 yrs, the formation mechanism through, it melts instantly and forms the atherosclerotic 2-3cm), latitude and longitude lines form a grid meshed- fluid, leaving a meshed structure and imprints after of shatter cone remains unclear. Different hypotheses for structure. This is an important and unique phenomenon cooling. -
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. -
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 Tennessee Meteorite Impact Sites and Changing Perspectives on Impact Cratering
UNIVERSITY OF SOUTHERN QUEENSLAND THE TENNESSEE METEORITE IMPACT SITES AND CHANGING PERSPECTIVES ON IMPACT CRATERING A dissertation submitted by Janaruth Harling Ford B.A. Cum Laude (Vanderbilt University), M. Astron. (University of Western Sydney) For the award of Doctor of Philosophy 2015 ABSTRACT Terrestrial impact structures offer astronomers and geologists opportunities to study the impact cratering process. Tennessee has four structures of interest. Information gained over the last century and a half concerning these sites is scattered throughout astronomical, geological and other specialized scientific journals, books, and literature, some of which are elusive. Gathering and compiling this widely- spread information into one historical document benefits the scientific community in general. The Wells Creek Structure is a proven impact site, and has been referred to as the ‘syntype’ cryptoexplosion structure for the United State. It was the first impact structure in the United States in which shatter cones were identified and was probably the subject of the first detailed geological report on a cryptoexplosive structure in the United States. The Wells Creek Structure displays bilateral symmetry, and three smaller ‘craters’ lie to the north of the main Wells Creek structure along its axis of symmetry. The question remains as to whether or not these structures have a common origin with the Wells Creek structure. The Flynn Creek Structure, another proven impact site, was first mentioned as a site of disturbance in Safford’s 1869 report on the geology of Tennessee. It has been noted as the terrestrial feature that bears the closest resemblance to a typical lunar crater, even though it is the probable result of a shallow marine impact. -
New Clues from Earth's Most Elusive Impact Crater: Evidence of Reidite in Australasian Tektites from Thailand
See discussions, stats, and author profiles for this publication at: https://www.researchgate.net/publication/321956231 New clues from Earth's most elusive impact crater: Evidence of reidite in Australasian tektites from Thailand Article in Geology · December 2017 DOI: 10.1130/G39711.1 CITATIONS READS 0 64 4 authors, including: Aaron J. Cavosie Timmons Erickson Curtin University Curtin University 100 PUBLICATIONS 2,285 CITATIONS 27 PUBLICATIONS 159 CITATIONS SEE PROFILE SEE PROFILE All content following this page was uploaded by Aaron J. Cavosie on 16 March 2018. The user has requested enhancement of the downloaded file. New clues from Earth’s most elusive impact crater: Evidence of reidite in Australasian tektites from Thailand Aaron J. Cavosie1, Nicholas E. Timms1, Timmons M. Erickson2, and Christian Koeberl3,4 1The Institute for Geoscience Research (TIGeR), Department of Applied Geology, Curtin University, Perth, WA 6102, Australia 2Lunar and Planetary Institute, Universities Space Research Association, Houston, Texas 77058, USA 3Natural History Museum, 1010 Vienna, Austria 4Department of Lithospheric Research, University of Vienna, 1090 Vienna, Austria ABSTRACT in Australasian tektites from Thailand supports a Australasian tektites are enigmatic drops of siliceous impact melt found in an ~8000 × location for the source crater in Southeast Asia. ~13,000 km strewn field over Southeast Asia and Australia, including sites in both the Indian and Pacific oceans. These tektites formed only 790,000 yr ago from an impact crater estimated MUONG NONG–TYPE TEKTITES to be 40–100 km in diameter; yet remarkably, the young and presumably large structure Muong Nong–type tektites (MN-type, or lay- remains undiscovered. -
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The Ohio Journal of Volume 116 No. 1 April Program ANSCIENCE INTERNATIONAL MULTIDISCIPLINARY JOURNAL Abstracts The Ohio Journal of SCIENCE Listing Services ISSN 0030-0950 The Ohio Journal of Sciencearticles are listed or abstracted in several sources including: EDITORIAL POLICY AcadSci Abstracts Bibliography of Agriculture General Biological Abstracts The Ohio Journal of Scienceconsiders original contributions from members and non-members of the Academy in all fields of science, Chemical Abstracts technology, engineering, mathematics and education. Submission Current Advances in Ecological Sciences of a manuscript is understood to mean that the work is original and Current Contents (Agriculture, Biology & unpublished, and is not being considered for publication elsewhere. Environmental Sciences) All manuscripts considered for publication will be peer-reviewed. Deep Sea Research and Oceanography Abstracts Any opinions expressed by reviewers are their own, and do not Environment Abstracts represent the views of The Ohio Academy of Science or The Ohio Journal of Science. Environmental Information Center Forest Products Abstracts Forestry Abstracts Page Charges Geo Abstracts Publication in The Ohio Journal of Science requires authors to assist GEOBASE in meeting publication expenses. These costs will be assessed at $50 per page for nonmembers. Members of the Academy do not Geology Abstracts pay page charges to publish in The Ohio Journal of Science. In GeoRef multi-authored papers, the first author must be a member of the Google Scholar Academy at the time of publication to be eligible for the reduced Helminthological Abstracts member rate. Papers that exceed 12 printed pages may be charged Horticulture Abstracts full production costs. Knowledge Bank (The Ohio State University Libraries) Nuclear Science Abstracts Submission Review of Plant Pathology Electronic submission only. -
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. -
Lechatelierite in Moldavite Tektites: New Analyses of Composition
52nd Lunar and Planetary Science Conference 2021 (LPI Contrib. No. 2548) 1580.pdf LECHATELIERITE IN MOLDAVITE TEKTITES: NEW ANALYSES OF COMPOSITION. Martin Molnár1, Stanislav Šlang2, Karel Ventura3. Kord Ernstson4.1Resselovo nám. 76, Chrudim 537 01, Czech Republic ([email protected]) 2Center of Materials and Nanotechnologies, University of Pardubice, 532 10 Pardubice, Czech Republic, [email protected] 3Faculty of Chemical Technology, University of Pardubice, 530 02 Pardubice, Czech Republic, [email protected]. 4University of Würzburg, D-97074 Würzburg, Deutschland ([email protected]) Introduction: Moldavites are tektites with a Experiments and Results: Experiments 1 and 2 - beautiful, mostly green discoloration and a very the boron question. The question of lowering the pronounced sculpture (Fig.1), which have been studied melting point and acid resistance led to the possibility many times e.g. [1-3]). of adding boron. The experiment 1 on a moldavite plate etched in 15%-HF to expose the lechatelierite was performed by laser ablation spectrometry and showed B2O3 concentration of >1%. In experiment 2, 38 g of lechatelierite fragments were then separated from 482 g of pure moldavite, and after the boron Fig. 1. Moldavites from Besednice analyzed in this content remained high (Tab. 2), the remaining carbon study. Scale bar 1 cm. was washed away. The analysis in Tab. 3 shows According to the most probable theory, they were remaining low boron content, which is obviously formed 14.5 million years ago together with the Ries bound to the carbon of the moldavites [8]. crater meteorite impact in Germany. They belong to the mid-European tektite strewn field and fell mostly in Bohemia. -
Chicxulub and the Exploration of Large Peak- Ring Impact Craters Through Scientific Drilling
Chicxulub and the Exploration of Large Peak- Ring Impact Craters through Scientific Drilling David A. Kring, Lunar and Planetary Institute, Houston, Texas 77058, USA; Philippe Claeys, Analytical, Environmental and Geo-Chemistry, Vrije Universiteit Brussel, Pleinlaan 2, Brussels 1050, Belgium; Sean P.S. Gulick, Institute for Geophysics and Dept. of Geological Sciences, Jackson School of Geosciences, University of Texas at Austin, Austin, Texas 78758, USA; Joanna V. Morgan and Gareth S. Collins, Dept. of Earth Science and Engineering, Imperial College London SW7 2AZ, UK; and the IODP-ICDP Expedition 364 Science Party. ABSTRACT proving the structure had an impact origin. to assess the depth of origin of the peak- The Chicxulub crater is the only well- The buried structure was confirmed by ring rock types and determine how they preserved peak-ring crater on Earth and seismic surveys conducted in 1996 and were deformed during the crater-forming linked, famously, to the K-T or K-Pg mass 2005 to be a large ~180–200-km–diameter event. That information is needed to effec- impact crater with an intact peak ring tively test how peak-ring craters form on extinction event. For the first time, geolo- (Morgan et al., 1997; Gulick et al., 2008). planetary bodies. gists have drilled into the peak ring of that The discovery of the Chicxulub impact The expedition was also designed to crater in the International Ocean structure initially prompted two scientific measure any hydrothermal alteration in Discovery Program and International drilling campaigns. In the mid-1990s, a the peak ring and physical properties of the Continental Scientific Drilling Program series of shallow onshore wells up to 700 m rocks, such as porosity and permeability, (IODP-ICDP) Expedition 364. -
Geophysical Methods in Impact Crater Hunting – Case Summanen
Geophysical methods in impact crater hunting – Case Summanen L.J. Pesonen1, S. Hietala2*, J. Plado3, T. Kreitsmann3, J. Lerssi2, and J. Nenonen2 1 Solid Earth Geophysics Laboratory, Physics Department, University of Helsinki, Finland 2 Geological Survey of Finland, Kuopio, Finland 3 Department of Geology, University of Tartu, Estonia, *correspondence: [email protected] Abstract Impact cratering is a ubiquitous process in our solar system affecting all planetary surfaces throughout geologic time. On Earth, there are currently 190 confirmed impact structures, which are distributed unevenly. The Fennoscandian Shield houses 17 % of them. The large amount of impact structures makes Fennoscandia one of the most densely cratered terrains on Earth. A dozen (12) impact structures have been discovered in Finland. The latest discovery, Lake Summanen is located in Central Finland, about 9 km southeast of city Saarijärvi. An impact generated structure was first hinted by airborne geophysical mapping by the Geological Survey of Finland in the early 2000`s (Lerssi et al., 2007) that revealed a circular ~2.6 km wide striking aeroelectromagnetic resistivity anomaly. Recent studies in 2017-2018 confirmed its impact origin based on the findings of shatter cone-bearing rocks and the identification of planar deformation features in quartz. 1. INTRODUCTION Summanen impact crater (62°39’00’’N, 25°22’30’’E) is located within the Paleoproterozoic Central Finland Granite Belt and is covered with the Lake Summanen. The lake is somewhat elliptical (8 km x 9 km x 4 km) in shape, whereby the longest axis extends in NW–SE direction due to the erosional influence of the latest (Weichselian) glaciation.