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Flynn Creek Crater, Tennessee: Final Report, by David J
1967010060 ASTROGEOLOGIC STUDIES / ANNUAL PROGRESS REPORT " July 1, 1965 to July 1, 1966 ° 'i t PART B - h . CRATERINVESTIGATIONS N 67_1_389 N 57-" .]9400 (ACCEC_ION [4U _" EiER! (THRU} .2_ / PP (PAGLS) (CO_ w ) _5 (NASA GR OR I"MX OR AD NUMBER) (_ATEGORY) DEPARTMENT OF THE INTERIOR UNITED STATES GEOLOQICAL SURVEY • iri i i i i iiii i i 1967010060-002 ASTROGEOLOGIC STUDIES ANNUAL PROGRESS REPORT July i, 1965 to July I, 1966 PART B: CRATER INVESTIGATIONS November 1966 This preliminary report is distributed without editorial and technical review for conformity with official standards and nomenclature. It should not be quoted without permission. This report concerns work done on behalf of the National Aeronautics and Space Administration. DEPARTMENT OF THE INTERIOR UNITED STATES GEOLOGICAL SURVEY 1967010060-003 • #' C OING PAGE ,BLANK NO/" FILMED. CONTENTS PART B--CRATER INVESTIGATIONS Page Introduction ........................ vii History and origin of the Flynn Creek crater, Tennessee: final report, by David J. Roddy .............. 1 Introductien ..................... 1 Geologic history of the Flynn Creek crater ....... 5 Origin of the Flynn Creek crater ............ ii Conc lusions ...................... 32 References cited .................... 35 Geology of the Sierra Madera structure, Texas: progress report, by H. G. Wilshire ............ 41_ Introduction ...................... 41 Stratigraphy ...................... 41 Petrography and chemical composition .......... 49 S truc ture ....................... 62 References cited ............. ...... 69 Some aspects of the Manicouagan Lake structure in Quebec, Canada, by Stephen H. Wolfe ................ 71 f Craters produced by missile impacts, by H. J. Moore ..... 79 Introduction ...................... 79 Experimental procedure ................. 80 Experimental results .................. 81 Summary ........................ 103 References cited .................... 103 Hypervelocity impact craters in pumice, by H. J. Moore and / F. -
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. -
Carlyle Smith Beals Fonds (R15735) Finding Aid No MSS2580 MIKAN
Date: 15/06/2017 Carlyle Smith Beals fonds (R15735) Page 1 Finding aid no MSS2580 Y:\App\Impromptu\Mikan\Reports\Description_reports\finding_aids_&_subcontainers_simplelist.imr MIKAN Container File/Item Cr. file/item Hierarchy Title, etc Date of/de Extent/Media/Dim/Access cde # Contenant Dos./pièce Dos./item cr. Hiérarchie Titre, etc création Support ou Média / Dim. / Accès 4938572 Series Personnal papers [textual record, graphic material] 1922-1978 4941473 1 1 File Personal papers 1947-1972 Textual records / 90 S&C : Biographical information, genealogical information on the Beals family. Contains also a passeport and a manual with french expressions and vocabulary. 4941474 1 2 File Personal correspondence 1965-1978 Textual records / 90 S&C : Correspondence not related to the professional activities of C.S. Beals. Contains also several postal cards. 4941475 1 3 File Scholarship records, Degrees, Honors and letters of 1922-1977 Textual records / 90 recommendation S&C : Contains a scholarship record of Yale University for 1922, letters from the University of London that certify the reception of two Ph.D. by C.S. Beals in 1926 and 1934. Contains the certification of the registrar's Office of the University of Toronto for the M.A. of 1923. Contains also letters of recommendation from the different schools attented by C.S. Beals. Contains also a letter from the Royal Society of Canada informing C..S. Beals.that he'll be recommended as fellow of the RSC, a letter from The Profesionnal Institute of the Public Service of Canada for the reception of the Institute's Gold Medal (1977), correspondence and documentation concerning the reception of a Honorary Degree from Queen's University in Kingston in 1960 and a certificate of the Royal Society of Canada certifying 45 years of membership. -
Four Hundred Years of Hits and Misses in Scientific Impact Crater Research
NIR Workshop, Gardnos − Gol, June 9th 2009 Four Hundred Years of Hits and Misses in Scientific Impact Crater Research Teemu Öhman Division of Geology, Department of Geosciences and Division of Astronomy, Department of Physical Sciences University of Oulu Finland Galileo Galilei Galileo Galilei (1564−1642) • First observer of lunar craters, late November 1609, Padua, Italy • Surface previously supposed smooth can be divided to dark lowlands (“large spots”) and bright highlands, which are covered with pits that have uplifted rims • A clear description of a central uplift Galilaei, D=15.5 km (LO) Johannes Kepler (1571−1630) • Supposed, like e.g. Plutarch in 1st century A.D., that the lunar lowlands are filled with water • Coined the terms “mare” and “terra” • Believed meteor(ite)s to have a cosmic origin(?) Kepler, D=32 km (LO) Robert Hooke (1635−1703) • Crater observer: Hipparchus, D=150 km Halley Micrographia, 1665 Lunar Orbiter Robert Hooke • First crater experimentalist: 1. Dropping bullets to a mixture of tobacco pipe clay and water: Æcraters “not unlike these of the Moon; but considering the state and condition of the Moon, there seems not any probability to imagine, that it should proceed from any cause analogus to this; for it would be difficult to imagine whence those bodies should come; and next, how the substance of the Moon should be so soft;” Robert Hooke 2. A pot of boiling alabaster: • When the boiling ceased, the surface was covered with craters • Compared these to terrestrial volcanoes Æ “…these pits in the Moon seem to -
Astroblemes, Scientific America~?-, Vol
Waste Isolation Pilot Plant Compliance Certification Application Reference 176 Dietz, R.S., August 1961. Astroblemes, Scientific America~?-, Vol. 205, #2, p 50-58. Submitted in accordance with 40 CFR § 194.13, Submission of Reference Materials. .. ~H ..\TTER COXE rour inrhes hi~h is one or many in igneous rork XEST OF COXES in dolomite. a tn~ or lime~tone. is rrom Wrlls or the \·rederort Ring in South ..\rrira. a strurture that i& prob Creek Ba~in ~trurture in Tenllt"'-"ft'. Thi& ~roup i~ II iMhet hi~h. ably the remains or tl1e large>l meteorite crater known on earth. Shork pre~~ur~ generated by meteorite imparl rreate ourh ron~. (;J..\.XT SH.-\TTER COXF., over rour reea long. i& !ihown in 1•lare amons jumbled rorks in a Rat. geolor:iralJy underormrd terrain at the Kentland Jime~tone quarry in Indiana. These c·ones round indirate that the quarry i~ an anrienl meteorite-im:-t ,ite. UMI Article Clearinghouse has reproduced this material with SO perLmLi'~-s~on of the copyright owner. Further reproduction IS Thi~ newly. ('Oined w·ord refers to anctent scars left in the earth·~ cru~t by huge tneteoriteH. The evidence for such itnpacts is largely the h igh-pre~~ure tnineral coesite and ~~shatter cones~' in the rocks b,· Hobert S. Dietz t is ;m awesome experience to stand authorih· was such that it took more than fall every 10,000 years, some 50,000 on the rim of B;minger Crater in :30 years' to re\·erse his judgment. But the giant meteorites must have struck the I Arizona and reflect on the cosmic scienc.-es progress not so much by the dis earth during the past 500 million ~·ears. -
Provincial Plaques Across Ontario
An inventory of provincial plaques across Ontario Last updated: May 25, 2021 An inventory of provincial plaques across Ontario Title Plaque text Location County/District/ Latitude Longitude Municipality "Canada First" Movement, Canada First was the name and slogan of a patriotic movement that At the entrance to the Greater Toronto Area, City of 43.6493473 -79.3802768 The originated in Ottawa in 1868. By 1874, the group was based in Toronto and National Club, 303 Bay Toronto (District), City of had founded the National Club as its headquarters. Street, Toronto Toronto "Cariboo" Cameron 1820- Born in this township, John Angus "Cariboo" Cameron married Margaret On the grounds of his former Eastern Ontario, United 45.05601541 -74.56770762 1888 Sophia Groves in 1860. Accompanied by his wife and daughter, he went to home, Fairfield, which now Counties of Stormont, British Columbia in 1862 to prospect in the Cariboo gold fields. That year at houses Legionaries of Christ, Dundas and Glengarry, Williams Creek he struck a rich gold deposit. While there his wife died of County Road 2 and County Township of South Glengarry typhoid fever and, in order to fulfil her dying wish to be buried at home, he Road 27, west of transported her body in an alcohol-filled coffin some 8,600 miles by sea via Summerstown the Isthmus of Panama to Cornwall. She is buried in the nearby Salem Church cemetery. Cameron built this house, "Fairfield", in 1865, and in 1886 returned to the B.C. gold fields. He is buried near Barkerville, B.C. "Colored Corps" 1812-1815, Anxious to preserve their freedom and prove their loyalty to Britain, people of On Queenston Heights, near Niagara Falls and Region, 43.160132 -79.053059 The African descent living in Niagara offered to raise their own militia unit in 1812. -
Meteorite Impacts, Earth, and the Solar System
Traces of Catastrophe A Handbook of Shock-Metamorphic Effects in Terrestrial Meteorite Impact Structures Bevan M. French Research Collaborator Department of Mineral Sciences, MRC-119 Smithsonian Institution Washington DC 20560 LPI Contribution No. 954 i Copyright © 1998 by LUNAR AND PLANETARY INSTITUTE The Institute is operated by the Universities Space Research Association under Contract No. NASW-4574 with the National Aeronautics and Space Administration. Material in this volume may be copied without restraint for library, abstract service, education, or personal research purposes; however, republication of any portion thereof requires the written permission of the Insti- tute as well as the appropriate acknowledgment of this publication. Figures 3.1, 3.2, and 3.5 used by permission of the publisher, Oxford University Press, Inc. Figures 3.13, 4.16, 4.28, 4.32, and 4.33 used by permission of the publisher, Springer-Verlag. Figure 4.25 used by permission of the publisher, Yale University. Figure 5.1 used by permission of the publisher, Geological Society of America. See individual captions for reference citations. This volume may be cited as French B. M. (1998) Traces of Catastrophe:A Handbook of Shock-Metamorphic Effects in Terrestrial Meteorite Impact Structures. LPI Contribution No. 954, Lunar and Planetary Institute, Houston. 120 pp. This volume is distributed by ORDER DEPARTMENT Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113, USA Phone:281-486-2172 Fax:281-486-2186 E-mail:[email protected] Mail order requestors will be invoiced for the cost of shipping and handling. Cover Art.“One Minute After the End of the Cretaceous.” This artist’s view shows the ancestral Gulf of Mexico near the present Yucatán peninsula as it was 65 m.y. -
Shatter Cones in Hypervelocity Impact Experiments: Structure, Formation and Comparison to Natural Impact Craters
Shatter cones in hypervelocity impact experiments: Structure, formation and comparison to natural impact craters DISSERTATION Zur Erlangung des akademischen Grades “doctor rerum naturalium“ (Dr. rer. nat.) Der Fakultät für Umwelt und natürliche Ressourcen Der Albert-Ludwigs-Universität Freiburg i. Brsg. vorgelegt von Jakob Wilk Geb. in Berlin, Pankow Freiburg im Breisgau 2017 Dekan: Prof. Dr. Tim Freytag Erstbetreuer/Referent: Prof. Dr. Thomas Kenkmann Korreferent: Prof. Dr. Alex Deutsch Zweitbetreuer: Prof. Dr. Stefan Hergarten Tag der Disputation: ABSTRACT Impact processes have dominated the formation and development of planetary bodies in our solar system. The study of impact crater formation provides deeper knowledge of early Earth’s history and enables us to understand a surface process profoundly shaping the surface of most rocky planetary bodies. The highly dynamic process of impact cratering causes a series of characteristic effects in the targeted rocks, which are referred to as shock metamorphic effects. These shock effects provide a valuable tool to analyze impact craters and their formation. Shatter cones are diagnostic for shock metamorphism. They are the only macroscopic effect caused by shock, thus, being unambiguously identifiable in the field, provide a valuable tool to find and verify impact structures. Over the last decades, hypervelocity impact experiments and shock recovery experiments fundamentally enhanced our understanding of impact cratering, by controlled laboratory conditions. With this technique, e.g., microscopic effects were calibrated to corresponding shock pressures, or the effect of target properties on the cratering process was extensively studied. However, in only few experiments shatter cones were found and analyzed. Thus, the conditions of shatter cone formation remained unclear. -
Scientific Contradictions to the Book of Genesis
Scientific Contradictions To The Book Of Genesis www.CreationismOnline.com How Old Are Moon Rocks? According to Genesis 1:14-19 the Moon was made on day 4 of the creation week. According to radiometric dating methods the Moon is: Thorium - Lead Dating = 4.87 to 28.14 Billion Years Old. Uranium-Lead Dating = 5.06 to 10.28 Billion Years Old. Lead - Lead Dating = 5 Billion Years Old. Potassium-Argon Dating = 2.1 to 17 Billion Years Old. Earth And Planetary Science Letters, Volume 14, 1972, Page 281 – 304 The Moon was made on day 4 of the creation week. According to current consensus the Moon is about 5 Thousand Million years old. Science, Volume 167, January 30th, 1970, Page 461-483. Earth And Planetary Science Letters, Volume 14, 1972, Page 169-175, 281 - 304. Clyde Webster states that the Solar System is 4,500 million years old: “Is it possible that the beginning for the consolidation of our Solar System within the universe could have been 4,500 million years ago? Does that impact on scripture? If I understand scripture properly, I have to come back and say NO.”. Record, “A Scientist Talks About Creation”, March 11, 1995, Page 6-9. In an earlier book he states that the Solar System is only 6,000 years old: “These objections can be overcome if we interpret the fourth day of the creation week as addressing only our Solar System and not the entire Universe.” The Earth: Origins And Early History, Dr. Clyde Webster, North American Division Press, 1981, Chapter 3. -
An Unusual Occurrence of Coesite at the Lonar Crater, India
Meteoritics & Planetary Science 52, Nr 1, 147–163 (2017) doi: 10.1111/maps.12745 An unusual occurrence of coesite at the Lonar crater, India 1* 1 2 1 3 Steven J. JARET , Brian L. PHILLIPS , David T. KING JR , Tim D. GLOTCH , Zia RAHMAN , and Shawn P. WRIGHT4 1Department of Geosciences, Stony Brook University, Stony Brook, New York 11794–2100, USA 2Department of Geosciences, Auburn University, Auburn, Alabama 36849, USA 3Jacobs—NASA Johnson Space Center, Houston, Texas 77058, USA 4Planetary Science Institute, Tucson, Arizona 85719, USA *Corresponding author. E-mail: [email protected] (Received 18 March 2016; revision accepted 06 September 2016) Abstract–Coesite has been identified within ejected blocks of shocked basalt at Lonar crater, India. This is the first report of coesite from the Lonar crater. Coesite occurs within SiO2 glass as distinct ~30 lm spherical aggregates of “granular coesite” identifiable both with optical petrography and with micro-Raman spectroscopy. The coesite+glass occurs only within former silica amygdules, which is also the first report of high-pressure polymorphs forming from a shocked secondary mineral. Detailed petrography and NMR spectroscopy suggest that the coesite crystallized directly from a localized SiO2 melt, as the result of complex interactions between the shock wave and these vesicle fillings. INTRODUCTION Although there is no direct observation of nonshock stishovite in nature, a possible post-stishovite phase may High-Pressure SiO2 Phases be a large component of subducting slabs and the core- mantle boundary (Lakshtanov et al. 2007), and Silica (SiO2) polymorphs are some of the simplest stishovite likely occurs in the deep mantle if basaltic minerals in terms of elemental chemistry, yet they are slabs survive to depth. -
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. -
The Ancient Meteorite Crater at Holleford Ontario by Leo Enright
Firefox https://starlightcascade.ca/tourism/holleford/HollefordCrater.php The Ancient Meteorite Crater at Holleford Ontario by Leo Enright Aerial photo of Holleford Meteorite Crater. Holleford Crater, an interesting and very ancient meteorite impace feature, is named after the tiny village located partly within its boundaries. It is a circular depression about 30 meters deep and 2.35 km in diameter, located at latitude 44 deg 47 minutes north, longitude 76 deg 38 minutes west, about 27 km north-north-west of Kingston, Ontario. Although several farms had been maintained at the site for over 100 years, its discovery and confirmation as a meteorite impace site dates only to the mid-1950's. The 1950's research was led by Canadian scientists from the Dominion Observatory in Ottawa, and the project that led to its discovery was the result of the discovery of two other meteorite impace sites, the New Quebec Crater amd the crater at Brent, Ontario. First identification of the feature was a result of a 1955 study of 200,000 aerial photographs of areas of the Canadian Shield conducted by the Dominion Observatory under the direction of Dr. Carlyle S. Beals, the Dominion Astronomer at the time. Subsequently, the research program included a study of the surface geology by the Geologic Survey of Canada, and a series of four geophysical studies, namely (1) magnetic observations of the area, (2) seismic studies which proved consistent with the theory that it was an impact site, (3) gravity studies which also proved consistent with the impact theory, and (4) a diamond drilling program in which 3 holes were drilled.