Amelia Creek: a Proterozoic Impact Structure in the Davenport Ranges, Northern Territory
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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. -
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. -
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. -
The Subsurface Structure of Oblique Impact Craters
The subsurface structure of oblique impact craters Dissertation vorgelegt von Dipl.-Geol. Michael H. Poelchau vom Fachbereich Geowissenschaften der Freien Universität Berlin zur Erlangung des akademischen Grades doctor rerum naturalium (Dr. rer. nat.) Berlin, 2010 The subsurface structure of oblique impact craters Dissertation vorgelegt von Dipl.-Geol. Michael H. Poelchau vom Fachbereich Geowissenschaften der Freien Universität Berlin zur Erlangung des akademischen Grades doctor rerum naturalium (Dr. rer. nat.) Berlin, 2010 Gutachter: 1. PD Dr. Thomas Kenkmann 2. Prof. Wolf-Uwe Reimold Tag der Disputation: 23.02.2010 Statement regarding the contributions of the author and others to this thesis This thesis is comprised of three published, peer-reviewed articles and one submitted manuscript, which each form separate chapters within this thesis. The chapters “Introduction” and “General Conclusions” were written especially for this thesis. The PhD candidate is the first author of two of these articles, and the second author of the third article. The PhD candidate is also the first author of a manuscript currently submitted to Earth and Planetary Science Letters. Therefore, these four chapters have their own introduction, methodology, discussion, conclusions and references. The articles and manuscripts used in this thesis are the following: Poelchau, M. H., and T. Kenkmann, 2008. Asymmetric signatures in simple craters as an indicator for an oblique impact direction, Meteoritcal and Planetary Science, 43, 2059-2072. Poelchau M. H., Kenkmann T. and Kring D. A., 2009. Rim uplift and crater shape in Meteor Crater: the effects of target heterogeneities and trajectory obliquity. Journal of Geophysical Research, 114, E01006, doi:10.1029/2008JE003235. Kenkmann, T. -
Twinning, Reidite, and Zro in Shocked Zircon from Meteor Crater
Transformations to granular zircon revealed: Twinning, reidite, and ZrO2 in shocked zircon from Meteor Crater (Arizona, USA) Aaron J. Cavosie1,2,3, Nicholas E. Timms1, Timmons M. Erickson1, Justin J. Hagerty4, and Friedrich Hörz5 1TIGeR (The Institute for Geoscience Research), Department of Applied Geology, Curtin University, Perth, WA 6102, Australia 2NASA Astrobiology Institute, Department of Geoscience, University of Wisconsin–Madison, Madison, Wisconsin 53706, USA 3Department of Geology, University of Puerto Rico–Mayagüez, Mayagüez, Puerto Rico 00681, USA 4U.S. Geological Survey (USGS) Astrogeology Science Center, Flagstaff, Arizona 86001, USA 5NASA Johnson Space Center, Science Department/Jets/HX5/ARES, Houston, Texas 77058, USA ABSTRACT Granular zircon in impact environments has long been recognized but remains poorly A N35° 2.0’ W111° 0.9’ understood due to lack of experimental data to identify mechanisms involved in its genesis. Meteor Crater in Arizona (USA) contains abundant evidence of shock metamorphism, includ- N ing shocked quartz, the high-pressure polymorphs coesite and stishovite, diaplectic SiO2 glass, and lechatelierite (fused SiO2). Here we report the presence of granular zircon, a new shocked-mineral discovery at Meteor Crater, that preserve critical orientation evidence of specific transformations that occurred during formation at extreme impact conditions. The zircon grains occur as aggregates of sub-micrometer neoblasts in highly shocked Coconino Sandstone (CS) comprised of lechatelierite. Electron backscatter diffraction shows that each MCC2 site grain consists of multiple domains, some with boundaries disoriented by 65° around <110>, (main shaft) a known {112} shock-twin orientation. Other domains have {001} in alignment with {110} of neighboring domains, consistent with the former presence of the high-pressure ZrSiO4 polymorph reidite. -
A New Chronology for the Moon and Mercury
A new chronology for the Moon and Mercury Simone Marchi German Aerospace Center (DLR), Institute of Planetary Research, Rutherfordstr. 2, D-12489 Berlin Dipartimento di Astronomia, Universit`adi Padova, Vicolo dell’Osservatorio 2, I-35122 Padova [email protected] Stefano Mottola German Aerospace Center (DLR), Institute of Planetary Research, Rutherfordstr. 2, D-12489 Berlin Gabriele Cremonese INAF, Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 3, I-35122 Padova Matteo Massironi Dipartimento di Geoscienze, Universit`adi Padova, via Giotto 1, I-35137, Padova and Elena Martellato INAF, Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 3, I-35122 Padova ABSTRACT In this paper we present a new method for dating the surface of the Moon, obtained by modeling the incoming flux of impactors and converting it into a size distribution of resulting craters. We compare the results from this model with the standard chronology for the Moon showing their similarities and discrepancies. In particular, we find indications of a non-constant impactor flux in the last 500 Myr and also discuss the implications of our findings for the Late Heavy Bombardment hypothesis. We also show the potential of our model for accurate dating of other inner Solar System bodies, by applying it to Mercury. arXiv:0903.5137v1 [astro-ph.EP] 30 Mar 2009 Subject headings: solar system: general — planets and satellites: Earth, Mercury, Moon 1. Introduction the evolution of the Solar System and in particu- lar of our own planet, the Earth. Recently, thanks Craters are among the most spectacular surface to a fleet of new space missions (Mars Express features of the solid bodies of the Solar System. -
Keurusselkä - Distribution of Shatter Cones
Lunar and Planetary Science XXXVIII (2007) 1762.pdf KEURUSSELKÄ - DISTRIBUTION OF SHATTER CONES. S. Hietala 1 and J. Moilanen 2, 1Kiveläntie 2 B 13, FI-42700 Keuruu, Finland, [email protected], 2Vuolijoentie 2086, FI-91760 Säräisniemi, Finland, [email protected]. Introduction: Keurusselkä impact structure was from the impact point increases. We have come to con- discovered by authors in 2003 [1], [2]. Well-formed clusion that most distant shatter cone like features we shatter cones in situ and boulders confirmed impact have found so far are still related to the impact struc- origin. A breccia with multiple sets of planar deforma- ture but this must be studied more carefully in future. tion features (PDFs) in quartz grains support this con- We have also measured directions of shatter cones. clusion. Structure is located in Central Finland (cen- This is not a simple task since only measurements that tered at 62°08´N, 24°37´E). seem to make any sense are made along the topside Exposed bedrocks of the region are Paleoprotero- striation of a shatter cone. What is the true topside of zoic granites and mica schists with volcanic inliers of the cone is not always so obvious. Central Finland Granitoid Complex. The age of the A breccia dike: In Autumn 2006 we discovered an granite basement is 1880 Ma. in situ breccia dike almost at the center of the structure. Precise age of the structure is unknown. It probably This is the first in situ breccia we have found and it is between 1880 - 600 Ma. 1880 Ma is the youngest may be impact related. -
The Cratered Earth
Lunar and Planetary Science XXXIII (2002) sess33.pdf Tuesday, March 12, 2002 POSTER SESSION I 7:00–9:30 p.m. Gymnasium The Cratered Earth Ormö J. Rossi A. P. Komatsu G. Marchetti M. De Santis A. The Discovery of a Probable Well-preserved Impact Crater Field in Central Italy [#1075] We propose the first impact craters found in Italy. They form a crater field with about 17 craters in the range 2- 20 m, and a main crater 140x115 m. It represents a rare example of well-preserved explosion craters formed in unconsolidated targets. Rossi A. P. Seven Possible New Impact Structures in Western Africa Detected on ASTER Imagery [#1309] Seven possible impact structures have been found in W Africa on ASTER images. Their diameters vary from few hundreds of meters up to few kilometers. They are located in Mauritania, Mali and Niger, on a sedimentary or metamorphic bedrock. Miura Y. Hirota A. Gorton M. Kedves M. Impact-related Events on Active Tectonic Regions Defined by Its Age, Shocked Minerals and Compositions [#1231] New type of impact-related event is defined at active tectonic region by using semi-circular structure, bulk XRF compositions with mixed data, shocked quartz grains with the PDFs texture, and Fe-Ni content. Example is discussed in Takamatsu MKT crater in Japan. Krochuk R. V. Sharpton V. L. Overview of Terny Astrobleme (Ukrainian Shield) Studies [#1832] A brief summary of Terny astrobleme observations, including history, petrographic and mineralogical evidences of impact, structure of the crater at current erosion level. Pesonen L. J. Reimold W. U. -
The Geological Record of Meteorite Impacts
THE GEOLOGICAL RECORD OF METEORITE IMPACTS Gordon R. Osinski Canadian Space Agency, 6767 Route de l'Aeroport, St-Hubert, QC J3Y 8Y9 Canada, Email: [email protected] ABSTRACT 2. FORMATION OF METEORITE IMPACT STRUCTURES Meteorite impact structures are found on all planetary bodies in the Solar System with a solid The formation of hypervelocity impact craters has surface. On the Moon, Mercury, and much of Mars, been divided, somewhat arbitrarily, into three main impact craters are the dominant landform. On Earth, stages [3] (Fig. 2): (1) contact and compression, (2) 174 impact sites have been recognized, with several excavation, and (3) modification. A further stage of more new craters being discovered each year. The “hydrothermal and chemical alteration” is also terrestrial impact cratering record is critical for our considered as a separate, final stage in the cratering understanding of impacts as it currently provides the process (e.g., [4]), and is also described below. only ground-truth data on which to base interpretations of the cratering record of other planets and moons. In this contribution, I summarize the processes and products of impact cratering and provide and an up-to-date assessment of the geological record of meteorite impacts. 1. INTRODUCTION It is now widely recognized that impact cratering is a ubiquitous geological process that affects all planetary objects with a solid surface (e.g., [1]). One only has to look up on a clear night to see that impact structures are the dominant landform on the Moon. The same can be said of all the rocky and icy bodies in the solar system that have retained portions of their earliest crust. -
Rock Magnetism and Palaeomagnetism of Meteorite Impact Craters in India
ROCK MAGNETISM AND PALAEOMAGNETISM OF METEORITE IMPACT CRATERS IN INDIA A THESIS SUBMITTED TO THE UNIVERSITY OF MUMBAI FOR THE PH. D. (SCIENCE) DEGREE IN PHYSICS Submitted By M. D. ARIF UNDER THE GUIDANCE OF PROF. NATHANI BASAVAIAH INDIAN INSTITUTE OF GEOMAGNETISM PLOT NO. 5, SECTOR 18, NEW PANVEL (W), NAVI MUMBAI-410 218 MAHARASHTRA, INDIA APRIL 2013 STATEMENT BY THE CANDIDATE As required by the University Ordinances 770, I wish to state that the work embodied in this thesis titled “Rock Magnetism and Palaeomagnetism of Meteorite Impact Craters in India" forms my own contribution to the research work carried out under the guidance of Prof. Nathani Basavaiah at the Indian Institute of Geomagnetism, New Panvel, Navi Mumbai. This work has not been submitted for any other degree of this or any other University. Wherever references have been made to previous works of others, it has been clearly indicated as such and included in the Bibliography. Signature of Candidate Full Name: Md. Arif Certified by Signature of Guide Name: Prof. Nathani Basavaiah ii Statement required under 0.770 Statement No. 1 I hereby declare that the work described in the thesis has not been submitted previously to this or any other University for Ph. D. or any other degree. Statement required under 0.771 Statement No.2 “Whether the work is based on the discovery of new facts by the candidate or of new relations of facts observed by others, and how the work tends to the general advancement of knowledge.” This thesis introduces a new method for the observation, evaluation and interpretation of the obliquity impact at Lonar based on structural and anisotropy of magnetic susceptibility (AMS) evidence. -
Observations at Terrestrial Impact Structures: Their Utility in Constraining Crater Formation
Meteoritics & Planetary Science 39, Nr 2, 199–216 (2004) Abstract available online at http://meteoritics.org Observations at terrestrial impact structures: Their utility in constraining crater formation Richard A. F. GRIEVE* and Ann M. THERRIAULT Earth Sciences Sector, Natural Resources Canada, 588 Booth Street, Ottawa, Ontario K1A 0Y7, Canada *Corresponding author. E-mail: [email protected] (Received 22 July 2003; revision accepted 15 December 2003) Abstract–Hypervelocity impact involves the near instantaneous transfer of considerable energy from the impactor to a spatially limited near-surface volume of the target body. Local geology of the target area tends to be of secondary importance, and the net result is that impacts of similar size on a given planetary body produce similar results. This is the essence of the utility of observations at impact craters, particularly terrestrial craters, in constraining impact processes. Unfortunately, there are few well-documented results from systematic contemporaneous campaigns to characterize specific terrestrial impact structures with the full spectrum of geoscientific tools available at the time. Nevertheless, observations of the terrestrial impact record have contributed substantially to fundamental properties of impact. There is a beginning of convergence and mutual testing of observations at terrestrial impact structures and the results of modeling, in particular from recent hydrocode models. The terrestrial impact record provides few constraints on models of ejecta processes beyond a confirmation of the involvement of the local substrate in ejecta lithologies and shows that Z-models are, at best, first order approximations. Observational evidence to date suggests that the formation of interior rings is an extension of the structural uplift process that occurs at smaller complex impact structures. -
Impact Melt Rocks from the Paasselkä Impact Structure (SE Finland): Petrography and Geochemistry
Impact melt rocks from the Paasselkä impact structure (SE Finland): Petrography and geochemistry Item Type Article; text Authors Schmieder, M.; Moilanen, J.; Buchner, E. Citation Schmieder, M., Moilanen, J., & Buchner, E. (2008). Impact melt rocks from the Paasselkä impact structure (SE Finland): Petrography and geochemistry. Meteoritics & Planetary Science, 43(7), 1189-1200. DOI 10.1111/j.1945-5100.2008.tb01122.x Publisher The Meteoritical Society Journal Meteoritics & Planetary Science Rights Copyright © The Meteoritical Society Download date 23/09/2021 21:32:30 Item License http://rightsstatements.org/vocab/InC/1.0/ Version Final published version Link to Item http://hdl.handle.net/10150/656454 Meteoritics & Planetary Science 43, Nr 7, 1189–1200 (2008) Abstract available online at http://meteoritics.org Impact melt rocks from the Paasselkä impact structure (SE Finland): Petrography and geochemistry Martin SCHMIEDER1*, Jarmo MOILANEN2, and Elmar BUCHNER1 1Institut für Planetologie, Universität Stuttgart, Herdweg 51, D-70174 Stuttgart, Germany 2Vuolijoentie 2086, FIN-91760 Säräisniemi, Finland *Corresponding author. E-mail: [email protected] (Received 06 March 2007; revision accepted 09 January 2008) Abstract–Recently, samples of allochthonous melt rocks from the ∼10 km and ≤1.9 Ga Paasselkä impact structure, SE Finland, were obtained. In this study, we present a first detailed petrographic and geochemical description of clast-rich Paasselkä impact melt rocks. Shock metamorphic features comprise shocked feldspar grains, intensely shocked and toasted quartz, marginally molten and recrystallized clasts thought to have been diaplectic quartz glass, largely fresh and recrystallized feldspar glasses, decomposed biotite flakes, recrystallized fluidal silica glass (originally probably lechatelierite) in partially molten sandstone clasts, all set into a glassy to cryptocrystalline melt matrix.