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STEINHEIM CRATER Steinheim Am Albuch, Steinheim Crater Is Located in the Swabain Alb
STEINHEIM CRATER Steinheim am Albuch, Steinheim crater is located in the Swabain Alb. Since the impact a small town has been built on site. However the crater still remains popular due to it being the best preserved crater with a central uplift. Formation: The Steinheim crater is the smaller partner to the Ries crater. It is located in Alb, Steinheim. It is thought that the two craters were formed 15million years ago. However, there are two theories to how the Steinheim crater formed; either a double meteorite or a 150m fragmentation of one larger impactor as it collided with the earth to form the 24km Reis crater. In either theory, the impactor travelled at around 7.2x104 km/hour impacted the Earth. This meteorite collided with the earth with a similar amount of energy as 100,000 Hiroshima bombs. It is thought that the meteorite hit the earth’s crust at an angle between 30 and 50 degrees which, on impact, caused the pressure to increase by a million bar. As the pressure rises, the temperature also increases to 30,000 degrees causing rocks to disintegrate. Formation of a complex crater Morphology The Steinheim crater is a typical complex crater. This means it has a central uplift in the centre of the crater. The central uplift has been measured to be around 1000m in diameter and be 50m above the basin floor, and the crater itself being 3.8 km in diameter and the sides measuring to ~100m deep. However according to gravity re- searchers, the crater could in fact be double the size! Because the impact crater is exposed, it is subject to erosion and weathering and therefore the morphology of the crater has changed little each year that passes. -
Relict Zircon Inclusions in Muong Nong-Type Australasain Tektites: Implications Regarding the Location of the Source Crater
Lunar and Planetary Science XXXI 1196.pdf RELICT ZIRCON INCLUSIONS IN MUONG NONG-TYPE AUSTRALASAIN TEKTITES: IMPLICATIONS REGARDING THE LOCATION OF THE SOURCE CRATER. B. P. Glass, Geology Department, University of Delaware, Newark, DE 19716, USA ([email protected]) Introduction: Over the last thirty years we Australasian tektite samples from which we have have recovered crystalline inclusions from ap- identified inclusions; however, not all of the recov- proximately forty Muong Nong-type tektites from ered inclusions have been identified by XRD. the Australasian tektite strewn field in order to Based on appearance, the percent of inclusion- learn more about the nature of the parent material bearing specimens containing zircon is probably and the formation process [e.g., 1, 2]. More re- 100% or very close to it. Nearly all the zircons cently we have used geographic variations in con- are opaque white and their X-ray patterns show centration (number/gm) of crystalline inclusions to extreme X-ray asterism. However, of the 28 zir- indicate the possible location of the source crater cons identified by X-ray diffraction, only two [3]. The purpose of this abstract is to summarize (both from the same specimen whose place of ori- all the presently available data regarding relict gin is unknown) produced X-ray diffraction pat- zircon inclusions recovered from Australasian terns indicating that baddeleyite may be present. Muong Nong-type tektites and to discuss implica- The X-ray patterns from these two grains con- tions regarding the possible location of the source tained the two strongest lines for baddeleyite and crater which has still not been found. -
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. -
Nördlingen 2010: the Ries Crater, the Moon, and the Future of Human Space Exploration, P
Program and Abstract Volume LPI Contribution No. 1559 The Ries Crater, the Moon, and the Future of Human Space Exploration June 25–27, 2010 Nördlingen, Germany Sponsors Museum für Naturkunde – Leibniz-Institute for Research on Evolution and Biodiversity at the Humboldt University Berlin, Germany Institut für Planetologie, University of Münster, Germany Deutsches Zentrum für Luft- und Raumfahrt DLR (German Aerospace Center) at Berlin, Germany Institute of Geoscience, University of Freiburg, Germany Lunar and Planetary Institute (LPI), Houston, USA Deutsche Forschungsgemeinschaft (German Science Foundation), Bonn, Germany Barringer Crater Company, Decatur, USA Meteoritical Society, USA City of Nördlingen, Germany Ries Crater Museum, Nördlingen, Germany Community of Otting, Ries, Germany Märker Cement Factory, Harburg, Germany Local Organization City of Nördlingen Museum für Naturkunde – Leibniz- Institute for Research on Evolution and Biodiversity at the Humboldt University Berlin Ries Crater Museum, Nördlingen Center of Ries Crater and Impact Research (ZERIN), Nördlingen Society Friends of the Ries Crater Museum, Nördlingen Community of Otting, Ries Märker Cement Factory, Harburg Organizing and Program Committee Prof. Dieter Stöffler, Museum für Naturkunde, Berlin Prof. Wolf Uwe Reimold, Museum für Naturkunde, Berlin Dr. Kai Wünnemann, Museum für Naturkunde, Berlin Hermann Faul, First Major of Nördlingen Prof. Thomas Kenkmann, Freiburg Prof. Harald Hiesinger, Münster Prof. Tilman Spohn, DLR, Berlin Dr. Ulrich Köhler, DLR, Berlin Dr. David Kring, LPI, Houston Dr. Axel Wittmann, LPI, Houston Gisela Pösges, Ries Crater Museum, Nördlingen Ralf Barfeld, Chair, Society Friends of the Ries Crater Museum Lunar and Planetary Institute LPI Contribution No. 1559 Compiled in 2010 by LUNAR AND PLANETARY INSTITUTE The Lunar and Planetary Institute is operated by the Universities Space Research Association under a cooperative agreement with the Science Mission Directorate of the National Aeronautics and Space Administration. -
Determination of the Origin of Unusual Glass with Metallic Spherule
Per. Mineral. (2006), 75, 2-3, 11-24 http://go.to/permin An International Journal of O PERIODICO di MINERALOGIA MINERALOGY, CRYSTALLOGRAPHY, GEOCHEMISTRY, established in 1930 ORE DEPOSITS, PETROLOGY, VOLCANOLOGY and applied topics on Environment, Archaeometry and Cultural Heritage Determination of the origin of unusual glass with metallic spherule inclusions found in the area between Inzingkofen and Sigmaringen (Bavaria, Germany), South-West of the Steinheim-Ries craters Matteo Ardit,1 Anna Maria Fioretti,2* Gianmario Molin,3 Emilio Ramous4 and Ulf-Christian Bauer5 1 Centro di Ateneo per i Musei, via Orto Botanico, 15 – 35122 Padova (Italy) 2 Istituto Geoscienze e Georisorse - CNR, c.so Garibaldi, 37 – 35137 Padova (Italy) 3 Dipartimento di Mineralogia e Petrologia, Università di Padova, c.so Garibaldi, 37 – 35137 Padova (Italy) 4 Dipartimento di Innovazione Meccanica e Gestionale, Università di Padova, via Venezia, 1 – 35139 Padova (Italy) 5 Seestrasse, 46a – 83727 Schliarsee (Germany) Abstract. — This paper reports the characteristics Riassunto. — In questo lavoro vengono studiati of a suite of pale green glass fragments and their diversi frammenti di vetro verde chiaro aventi metallic spherule inclusions (5 to 400 μm) found la particolarità di contenere inclusioni di sferule over a relatively wide area between Inzigkofen and metalliche (di dimensioni variabili tra 5 e 400 Sigmaringen (Bavaria, Germany), about 150 km SW μm), ritrovati in un’area relativamente vasta tra of the Steinheim-Ries impact craters. The distribution Inzigkofen e Sigmaringen (Baviera, Germania), a area of these glasses and their close macroscopic ~150 km SW dai crateri di impatto di Steinheim- similarity (apart from the spherules) with moldavite Ries. -
Shock Wave Distribution at Ries Impact Crater, Germany?:A Micro-Raman Spectroscopical Study of Shocked Zircon
Workshop on Impact Cratering II (2007) 8050.pdf “ANTISYMMETRIC” SHOCK WAVE DISTRIBUTION AT RIES IMPACT CRATER, GERMANY?:A MICRO-RAMAN SPECTROSCOPICAL STUDY OF SHOCKED ZIRCON. A. Gucsik, Max Planck Institute for Chemistry, Department of Geochemistry,. Joh.-J.-Becherweg 27, D-55128 Mainz, Germany (gucsik@mpch- mainz.mpg.de). Introduction: Zircon is a highly refractory and weather- parallel and perpendicular to the c-axis, for the pur- ing-resistant mineral that has proven useful as an indi- pose of Raman spectrometric analysis. cator of shock metamorphism in the study of impact Raman spectra were obtained with a Renishaw structures and formations that are old, deeply eroded, RM1000 confocal micro-Raman spectrometer with a and metamorphically overprinted (e.g., [1-3]. Zircon 20 mW, 632 nm He-Ne laser excitation system and a has advantages compared to quartz or other shock- thermo-electrically cooled CCD detector. The power metamorphosed rock-forming minerals that have been of the laser beam on the sample was approximately 3 widely used as impact indicators, but are far less re- mW. Spectra were obtained in the range 100-1200 cm- fractory. Furthermore, U-Pb dating of zircon can pro- 1, with approximately thirty seconds total exposure vide constraints on the ages of impact events or depo- time. The spectral resolution (apparatus function) was sition of impact formations (e.g., [4] and references 4 cm-1. Raman spectra were taken from 3 µm3 sample therein). volume and CL spectra were obtained from approxi- Effects of high degrees of shock deformation (>10 mately 35 x 45 µm areas. GPa) in quartz and other rock-forming minerals (e.g., Further details on the samples and methodology feldspars), such as planar deformation features (PDFs), can be found in [7]. -
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. -
19980227350.Pdf
NASA TN D-490 =o C_ Z I.- <: .< Z TECHNICAL NOTE D-490 THE ORIGIN OF TEKTITES J. A. O'Keefe Goddard Space Flight Center NATIONAL AERONAUTICS AND SPACE ADMINISTRATION I WASHINGTON November 1960 CONTENTS Summary .................................. i INTRODUCTION ............................. 1 DESCRIPTION AND COMPOSITION OF TEKTITES ..... 1 DISTRIBUTION OF TEKTITES ................... 5 TERRESTRIAL VS. EXTRATERRESTRIAL ORIGIN ...... 6 MODE OF ARRIVAL .......................... 10 Dissimilarity to Ordinary Meteorites ............. 10 Great Meteor Procession of 1913 ............... 11 ORIGIN OF THE METEOR PROCESSION ............ 13 Physical Aspects of the Sputnik II Descent ......... 13 Physical Aspects of the Meteor Procession ......... 18 Inferences from the Analyses .................. 21 LUNAR ORIGIN OF TEKTITES ................... 22 ACKNOWLEDGMENTS ......................... 23 References ................................. 24 111 THE ORIGIN OF TEKTITES by J. A. O'Keefe SUMMARY Tektites are probably extraterrestrial, rather than the result of heating some terrestrial materials, because they are a chemi- cally homogeneous group with definite peculiarities (high silica, excess of alkaline earths over alkalis, excess of potash over soda, absence of water), and because some of them (the australites) appear to have undergone ablation in flight through the atmosphere. Since comparatively slow heating is required to explain the liquefaction of the tektite material, it is suggested that the tektites arrived along orbits which were nearly parallel to the surface of the earth, and which resulted from the decay of the orbit of a natural satellite. The great meteor procession of February 9, 1913, is an example of such an object. Comparison with the re- entry phenomena of the artificial satellite 1957 Beta suggests that the 1913 shower consisted of a single large stone weighing about 400 kilograms, and a few dozen smaller bodies weighing about 40 grams each, formed by ablation from the larger body. -
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,- - 7 I 1 a/ i' # SUBJECT CATEGORfES FOR GODDARD JOURNAL i (To be used for classifying all NASA publications, journal articles, and other pap& for inclusion in the Goddard Journal.) 1 Part A - Space :I. .-JA A 1. A::i,c-4cr.y crr.3 , id .-ophyslos h A 2. Cz 1 e; i ia 1 Mz cnc.; . cs c :.A u;lzodesy A 3. SoiGi ?hyjiCS A 4. io*iosp>.c:.-zcnd dio?bysics r- . A 5. r:~13scnJ ?c.-tiC:Ls A 6: Pi meto, cgy A 7. Picnetcry ;\tnos,:,sres A 8. Generai (subjec.-r not clearly belonging in any of categories 1-7) Part B - Space Technology B 1. Projects and Programs €3 2. Space Dynamics and Control Systems B 3. Spacecraft and Subsystems B 4. Vehicle Technology B 5. Sounding Rockets B 6. Sensors B 7. General Electronics B 8. Environmental Testing - B 9. Tracking Systems B 10. General (subiects not clearly belonging in any of categories 1-9) GPO PRICE CFSTl PRICE ff 653 July 65 a 7 The Chemical Composition and Origin of Moldavites f * J. A. Philpotts and W. H. Pinson, Jr. Department of Geology and Geophysics Massachusetts Iilstizute of Technology Cimbricgc :" asachuse:ts Abstract : Twenty three new ma,cr-eienm: ,nalyads or' moldavites are report&. I 1 The samples include seve-nzean Bohe.Ai<-..i ar.d six Moravian tektites. The 1 ranges in the contents 05 the various oxicies are as follows: Si02, 75.5 - 80.6; A1203, 9.62 - 12.64; TLG 2' 0.253 - 0.460; Fe203, 0.12 - 0.31; FeO, 1.42 - 2.36; MgO, 1.13 - 2.50; CaO, 1.46 - 3.71; Na20, 0.31 - i 1 f 0.67; K20, 3.26 - 3.81.' The Rb and Sr contents and the Rb/Sr ratios are 1 t also reported for the 23 specimens; the ranges are as follows: 1 Rb, I 120 - 160 ppm; Sr, 130 - 156 ppm; Rb/Sr, 0.82 - 1.20. -
Distal Ejecta from the Ries Crater – Moldavites and Projectile
Large Meteorite Impacts (2003) 4050.pdf DISTAL EJECTA FROM THE RIES CRATER – MOLDAVITES AND PROJECTILE. N. A. Artemieva. Institute for Dynamics of Geospheres, Russian Academy of Science, Leninsky pr., 38, bldg.1, 119334, Moscow, Russia, [email protected] Introduction: Using detailed geological, continuous unit, but, probably, some chaotic spots with petrographic, geochemical, and geographical various thickness. In this upper layer shock pressure constraints we have performed numerical modeling drops quickly with a distance and at 5 km from the studies that relate the Steinheim crater (Da = 3.8 km), impact point is below melting pressure for a porous the Ries crater (Da = 24 km) in Southern Germany, and quartz (45 GPa). Figure 1 shows surface material, the moldavite (tektite) strewn field. The known molten after an impact - possible tektites. It is totally moldavite strewn field extends from about 200 to 450 within the growing crater (the Ries final diameter is 26 km from the center of the Ries to the ENE forming a km). Ejection velocity varies from 1-2 km/s behind the fan with an angle of about 57°. An oblique impact of a projectile to 8-11 km/s in a downrange direction. binary asteroid from a WSW direction appears to The model with more thick sandy layer reveals that explain the locations of the craters and the formation 70% of all tektites originate from the upper 20 m, 90% and distribution of the moldavites [1]. In a presented - from the upper 40 m, and only 10% of the material is study we attempt to answer more questions concerning initially below this depth. -
Local Structure of Iron in Tektites and Natural Glass: an Insight Through X-Ray Absorption Fine Structure Spectroscopy
288 JournalL. Wang, of Mineralogical A. Yoshiasa, andM. Okube, Petrological T. Hiratoko, Sciences, Y. Hu, Volume H. Arima 108, andpage K. 288 Sugiyama─ 294, 2013 Local structure of iron in tektites and natural glass: An insight through X-ray absorption fine structure spectroscopy * * ** * *** Ling WANG , Akira YOSHIASA , Maki OKUBE , Tatsuya HIRATOKO , Yuan HU , § § Hiroshi ARIMA and Kazumasa SUGIYAMA * Graduate School of Science and Technology, Kumamoto University, Kumamoto, Kumamoto 860-8555, Japan ** Materials and Structure Laboratory, Tokyo Institute of Technology, Yokomama, Kanagawa 226-8503, Japan ***Testing center for Gold and Jewelry of Jiangsu Province, Nanjing, Jiangsu 210016, China § Institute for materials research, Tohoku University, Sendai, Miyagi 980-8577, Japan The local structure of iron in tektites from six strewn fields, and impact- and non-impact-related glass were studied using the Fe K-edge X-ray absorption near edge structure (XANES) and extended X-ray absorption fine structure (EXAFS) techniques, in order to obtain quantitative data on Fe-O bond length and Fe coordina- tion number. X-ray absorption fine structure (XAFS) spectra and Fe-O bonds in standard minerals such as he- matite, fayalite, and magnetite were compared. The degree of oxidation was measured based on the valencies 3+ of iron in the samples. Tektites contain a greater proportion of ferrous than ferric iron [0.04(1)-0.13(1) Fe / 3+ ƩFe]. The ferric ratios of impact-related glass [0.18(1)-0.52(1) Fe /ƩFe], and volcanic glass [0.26(1)-0.30(1) 3+ Fe /ƩFe] are higher than that in tektites. Based on the measured Fe-O distance, it was inferred that 4- and 5-coordinated Fe exist in tektites, whereas volcanic glass contains 5- and 6-coordinated Fe. -
The Ries-Steinheim Crater Pair and Two Major Earthquakes – New Discoveries Challenging the Double-Impact Theory
The Ries-Steinheim crater pair and two major earthquakes – New discoveries challenging the double-impact theory Elmar Buchner ( [email protected] ) University of Applied Sciences Neu-Ulm Volker Sach Meteorkratermuseum Steinheim Martin Schmieder USRA, Houston, Texas Article Keywords: impact-earthquakes, Nördlinger Ries, Steinheim Basin Posted Date: July 27th, 2020 DOI: https://doi.org/10.21203/rs.3.rs-43745/v1 License: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License Page 1/24 Abstract The Nördlinger Ries and the Steinheim Basin are widely perceived as a Middle Miocene impact crater doublet. We discovered two independent earthquake-produced seismite horizons in North Alpine Foreland Basin deposits. The older seismite horizon,associated with the Ries impact is overlain by in situ-preserved distal impact ejecta, forming a unique continental seismite-ejecta couplet within a distance up to 180 km from the crater. The younger seismite unit, also triggered by a major palaeo-earthquake, comprises clastic dikes that cut through the Ries seismite-ejecta couplet. The clastic dikes were likely formed in response to the Steinheim impact, some kyr after the Ries impact, in line with paleontologic results. With the Ries and Steinheim impacts as two separate events, Southern Germany witnessed a double disaster in the Middle Miocene. The magnitude–distance relationship of seismite formation during large earthquakes suggests the seismic and destructive potential of impact-earthquakes may be signicantly underestimated. Introduction The ~24 km-diameter Nördlinger Ries1,2,3,4 and the ~4 km-diameter Steinheim Basin1,5,6,7,8 impact structures in southern Germany (Fig.