[Italic Page Numbers Indicate Major References] Abathomphalus
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A Summary of Petroleum Plays and Characteristics of the Michigan Basin
DEPARTMENT OF INTERIOR U.S. GEOLOGICAL SURVEY A summary of petroleum plays and characteristics of the Michigan basin by Ronald R. Charpentier Open-File Report 87-450R This report is preliminary and has not been reviewed for conformity with U.S. Geological Survey editorial standards and stratigraphic nomenclature. Denver, Colorado 80225 TABLE OF CONTENTS Page ABSTRACT.................................................. 3 INTRODUCTION.............................................. 3 REGIONAL GEOLOGY.......................................... 3 SOURCE ROCKS.............................................. 6 THERMAL MATURITY.......................................... 11 PETROLEUM PRODUCTION...................................... 11 PLAY DESCRIPTIONS......................................... 18 Mississippian-Pennsylvanian gas play................. 18 Antrim Shale play.................................... 18 Devonian anticlinal play............................. 21 Niagaran reef play................................... 21 Trenton-Black River play............................. 23 Prairie du Chien play................................ 25 Cambrian play........................................ 29 Precambrian rift play................................ 29 REFERENCES................................................ 32 LIST OF FIGURES Figure Page 1. Index map of Michigan basin province (modified from Ells, 1971, reprinted by permission of American Association of Petroleum Geologists)................. 4 2. Structure contour map on top of Precambrian basement, Lower Peninsula -
COUNTY TWP RNG SEC OPERATOR WELL NAME FORMATIONS from to BOXE S COMMENTS TYPE Alger 44N 21W 19 DNR--ERD Village of Trenary MW 24
COUNTY TWP RNG SEC OPERATOR WELL NAME FORMATIONS FROM TO BOXE COMMENTS TYPE S Alger 44N 21W 19 DNR--ERD Village of MW 24 Limestone with vugs and 10 112 13 Lithologic log available. Core Trenary shale layers Alger 44N 21W 19 DNR--ERD Village of MW 25 (TWQ) Limestone w\lenses of 4 52 8 Lithologic log available. Core Trenary shale and siltstone Alger 44N 21W 19 DNR--ERD Village of MW 26 (TWW) Ls. & vugs w\lenses of 5 92 10 Lithologic log available. Core Trenary shale and siltstone Alger 44N 21W 19 DNR--ERD Village of MW 29 Ls. & vugs w\lenses of 47 81 4 Lithologic log available. Core Trenary shale and siltstone Alger 44N 21W 20 DNR--ERD Village of RL-4 Dolomite 13 29 2 Lithologic log available Core Trenary Alger 44N 21W 20 DNR--ERD Village of RL-6 Dolomite 17 34 2 Lithologic log available. Core Trenary Alger 44N 21W 20 DNR--ERD Village of RL-8 Dolomite 21 37 2 Lithologic log available. Core Trenary Alger 44N 22W 9 Cleveland-Cliffs Kiva Core #1 Black River to 18 567 4 Lithologic log available. Core Precambrian Samples of core chips only Alger 45N 22W 31 Cleveland-Cliffs #1 Dolomite & sandstone 26 132 13 Lithologic log available. Core Alger 46N 18W 29 Amoco Production Per.# St. Amour 1-29 Autrain Fm. 90 361 45 Lithologic log available. Core 021-871-202 Declared a "lost hole" & moved short distance to start 1-29R. Alger 46N 18W 29 Amoco Production Per.# St. Amour 1-29R Autrain, Munising, Oronto 160 7179 929 Lithologic and several electric Core 021-871-202 (Jacobsville) and Portage logs are available. -
A Field and Petrographic Study of the Freda
A FIELD AND PETROGRAPHIC STUDY OF THE FREDA FORMATION ALONG THE MONTREAL RIVER, GOGEBIC COUNTY, MICHIGAN fey GORDON R. SMALE A THESIS Submitted in partial fulfillment of the requirements for the degree of Master of Science in Michigan State University East Lansing, Michigan 1958 ProQuest Number: 10008738 All rights reserved INFORMATION TO ALL USERS The quality of this reproduction is dependent upon the quality of the copy submitted. In the unlikely event that the author did not send a complete manuscript and there are missing pages, these will be noted. Also, if material had to be removed, a note will indicate the deletion. uest. ProQuest 10008738 Published by ProQuest LLC (2016). Copyright of the Dissertation is held by the Author. All rights reserved. This work is protected against unauthorized copying under Title 17, United States Code Microform Edition © ProQuest LLC. ProQuest LLC. 789 East Eisenhower Parkway P.O. Box 1346 Ann Arbor, Ml 48106- 1346 A FIELD AND PETROGRAPHIC STUDY OF THE FREDA FORMATION ALONG THE MONTREAL RIVER, GOGEBIC COUNTY, MICHIGAN •"by Gordon R „ Smal'e ABSTRACT The Montreal River provides a geographic boundary between Wisconsin and Michigan on the south shore of Lake Superior. A geologic study, both field and laboratory, was made of the 12,000 foot thickness of steeply dipping Freda for mation exposed along this river. The field study Includes mapping of sedimentary structures In an effort to determine the dominant current directions during deposition of the formation. Pebble and quartz grain orientation as well as heavy mineral and rock composition analyses were made In the laboratory to supplement the field work. -
Imagining Outer Space Also by Alexander C
Imagining Outer Space Also by Alexander C. T. Geppert FLEETING CITIES Imperial Expositions in Fin-de-Siècle Europe Co-Edited EUROPEAN EGO-HISTORIES Historiography and the Self, 1970–2000 ORTE DES OKKULTEN ESPOSIZIONI IN EUROPA TRA OTTO E NOVECENTO Spazi, organizzazione, rappresentazioni ORTSGESPRÄCHE Raum und Kommunikation im 19. und 20. Jahrhundert NEW DANGEROUS LIAISONS Discourses on Europe and Love in the Twentieth Century WUNDER Poetik und Politik des Staunens im 20. Jahrhundert Imagining Outer Space European Astroculture in the Twentieth Century Edited by Alexander C. T. Geppert Emmy Noether Research Group Director Freie Universität Berlin Editorial matter, selection and introduction © Alexander C. T. Geppert 2012 Chapter 6 (by Michael J. Neufeld) © the Smithsonian Institution 2012 All remaining chapters © their respective authors 2012 All rights reserved. No reproduction, copy or transmission of this publication may be made without written permission. No portion of this publication may be reproduced, copied or transmitted save with written permission or in accordance with the provisions of the Copyright, Designs and Patents Act 1988, or under the terms of any licence permitting limited copying issued by the Copyright Licensing Agency, Saffron House, 6–10 Kirby Street, London EC1N 8TS. Any person who does any unauthorized act in relation to this publication may be liable to criminal prosecution and civil claims for damages. The authors have asserted their rights to be identified as the authors of this work in accordance with the Copyright, Designs and Patents Act 1988. First published 2012 by PALGRAVE MACMILLAN Palgrave Macmillan in the UK is an imprint of Macmillan Publishers Limited, registered in England, company number 785998, of Houndmills, Basingstoke, Hampshire RG21 6XS. -
ALBIAN AMMONITES of POLAND (Plates 1—25)
PALAEONTOLOGIA POLQNICA mm ■'Ъ-Ь POL T S H ACADEMY OF SCIENCES INSTITUTE OF PALEOBIOLOGY PALAEONTOLOGIA POLONICA—No. 50, 1990 t h e a l b ia w AMMONITES OF POLAND (AMQNITY ALBU POLS К I) BY RYSZARD MARCINOWSKI AND JOST WIEDMANN (WITH 27 TEXT-FIGURES, 7 TABLES AND 25 PLATES) WARSZAWA —KRAKÔW 1990 PANSTWOWE WYDAWNICTWO NAUKOWE KEDAKTOR — EDITOR JOZEP KA2MIERCZAK 2ASTEPCA HEDAKTOHA _ ASSISTANT EDITOR m AôDAlenA BÛRSUK-BIALYNICKA Adres Redakcjl — Address of the Editorial Office Zaklad Paleobiologij Polska Akademia Nauk 02-089 Warszawa, AI. 2w irki i Wigury 93 KOREKTA Zespol © Copyright by Panstwowe Wydawnictwo Naukowe Warszawa — Krakôw 1990 ISBN 83-01-09176-2 ISSN 0078-8562 Panstwowe Wydawnielwo Naukowe — Oddzial w Krakowie Wydanie 1, Naklad 670 + 65 cgz. Ark. wyd. 15. Ark. druk. 6 + 25 wkladek + 5 wklejek. Papier offset, sat. Ill kl. 120 g. Oddano do skiadania w sierpniu 1988 r. Podpisano do druku w pazdzierniku 1990 r. Druk ukoriczono w listopadzie 1990 r. Zara. 475/87 Drukarnia Uniwersytetu Jagielloriskiego w Krakowie In Memory of Professor Edward Passendorfer (1894— 1984) RYSZARD MARCINOWSKI and JOST WIEDMANN THE ALBIAN AMMONITES OF POLAND (Plates 1—25) MARCINOWSKI, R. and WIEDMANN, J.: The Albian ammonites of Poland. Palaeonlologia Polonica, 50, 3—94, 1990. Taxonomic and ecological analysis of the ammonite assemblages, as well as their general paleogeographical setting, indicate that the Albian deposits in the Polish part of the Central European Basin accumulated under shallow or extremely shallow marine conditions, while those of the High-Tatra Swell were deposited in an open sea environment. The Boreal character of the ammonite faunas in the epicontinental area of Poland and the Tethyan character of those in the Tatra Mountains are evident in the composition of the analyzed assemblages. -
12. Lower Cretaceous Ammonites from the South Atlantic Leg 40 (Dsdp), Their Stratigraphic Value and Sedimentologic Properties
12. LOWER CRETACEOUS AMMONITES FROM THE SOUTH ATLANTIC LEG 40 (DSDP), THEIR STRATIGRAPHIC VALUE AND SEDIMENTOLOGIC PROPERTIES Jost Wiedmann and Joachim Neugebauer, Geol.-palaont. Institut der Universitat Tubingen, BRD ABSTRACT Eleven ammonites have been cored during Leg 40. They were found concentrated in the lower parts of the drilled section at Sites 363 (Walvis Ridge) and 364 (Angola Basin), and permit recognition of upper Albian, middle Albian, and upper Aptian. So far, no lower Albian could be recognized. A high ammonite density can be assumed for the South Atlantic Mid-Cretaceous. In contrast to data available so far, the Walvis Ridge associations consisting of phylloceratids and desmoceratids show more open- basin relationships than those of the Angola Basin, which are composed of mortoniceratids, desmoceratids, and heteromorphs. Paleobiogeographically, the South Atlantic fauna can be related to the well-known onshore faunas of Angola, South Africa, and Madagascar as well as to the European Mid-Cretaceous. This means that the opening of the South Atlantic and its connection with the North Atlantic occurred earlier as was generally presumed, i.e., in the middle Albian. Records of lower Aptian ammonite faunas from Gabon and Brazil remain doubtful. High rates of sedimentation prevailed especially in the Aptian and Albian, in connection with the early deepening of the South Atlantic basins. The mode of preservation of the ammonites suggests that they were deposited on the outer shelf or on the upper continental slope and were predominantly buried under sediments of slightly reducing conditions. In spite of a certain variability of the depositional environment, the ammonites show a uniform and particular mode of preservation. -
Impact Cratering in the Solar System
Impact Cratering in the Solar System Michelle Kirchoff Lunar and Planetary Institute University of Houston - Clear Lake Physics Seminar March 24, 2008 Outline What is an impact crater? Why should we care about impact craters? Inner Solar System Outer Solar System Conclusions Open Questions What is an impact crater? Basically a hole in the ground… Barringer Meteor Crater (Earth) Bessel Crater (Moon) Diameter = 1.2 km Diameter = 16 km Depth = 200 m Depth = 2 km www.lpi.usra.edu What creates an “impact” crater? •Galileo sees circular features on Moon & realizes they are depressions (1610) •In 1600-1800’s many think they are volcanic features: look similar to extinct volcanoes on Earth; some even claim to see volcanic eruptions; space is empty (meteorites not verified until 1819 by Chladni) •G.K. Gilbert (1893) first serious support for lunar craters from impacts (geology and experiments) •On Earth Barringer (Meteor) crater recognized as created by impact by Barringer (1906) •Opik (1916) - impacts are high velocity, thus create circular craters at most impact angles Melosh, 1989 …High-Velocity Impacts! www.lpl.arizona.edu/SIC/impact_cratering/Chicxulub/Animation.gif Physics of Impact Cratering Understand how stress (or shock) waves propagate through material in 3 stages: 1. Contact and Compression 2. Excavation 3. Modification www.psi.edu/explorecraters/background.htm Hugoniot Equations Derived by P.H. Hugoniot (1887) to describe shock fronts using conservation of mass, momentum and energy across the discontinuity. equation (U-up) = oU of state P-Po = oupU E-Eo = (P+Po)(Vo-V)/2 P - pressure U - shock velocity up - particle velocity E - specific internal energy V = 1/specific volume) Understanding Crater Formation laboratory large simulations explosives (1950’s) (1940’s) www.nasa.gov/centers/ames/ numerical simulations (1960’s) www.lanl.gov/ Crater Morphology • Simple • Complex • Central peak/pit • Peak ring www3.imperial.ac. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
Summary of Hydrogelogic Conditions by County for the State of Michigan. Apple, B.A., and H.W. Reeves 2007. U.S. Geological Surve
In cooperation with the State of Michigan, Department of Environmental Quality Summary of Hydrogeologic Conditions by County for the State of Michigan Open-File Report 2007-1236 U.S. Department of the Interior U.S. Geological Survey Summary of Hydrogeologic Conditions by County for the State of Michigan By Beth A. Apple and Howard W. Reeves In cooperation with the State of Michigan, Department of Environmental Quality Open-File Report 2007-1236 U.S. Department of the Interior U.S. Geological Survey U.S. Department of the Interior DIRK KEMPTHORNE, Secretary U.S. Geological Survey Mark D. Myers, Director U.S. Geological Survey, Reston, Virginia: 2007 For more information about the USGS and its products: Telephone: 1-888-ASK-USGS World Wide Web: http://www.usgs.gov/ Any use of trade, product, or firm names in this publication is for descriptive purposes only and does not imply endorsement by the U.S. Government. Although this report is in the public domain, permission must be secured from the individual copyright owners to reproduce any copyrighted materials contained within this report. Suggested citation Beth, A. Apple and Howard W. Reeves, 2007, Summary of Hydrogeologic Conditions by County for the State of Michi- gan. U.S. Geological Survey Open-File Report 2007-1236, 78 p. Cover photographs Clockwise from upper left: Photograph of Pretty Lake by Gary Huffman. Photograph of a river in winter by Dan Wydra. Photographs of Lake Michigan and the Looking Glass River by Sharon Baltusis. iii Contents Abstract ...........................................................................................................................................................1 -
(Owen Willans) Richardson
O. W. (Owen Willans) Richardson: An Inventory of His Papers at the Harry Ransom Center Descriptive Summary Creator: Richardson, O. W. (Owen Willans), 1879-1959 Title: O. W. (Owen Willans) Richardson Papers Dates: 1898-1958 (bulk 1920-1940) Extent: 112 document boxes, 2 oversize boxes (49.04 linear feet), 1 oversize folder (osf), 5 galley folders (gf) Abstract: The papers of Sir O. W. (Owen Willans) Richardson, the Nobel Prize-winning British physicist who pioneered the field of thermionics, contain research materials and drafts of his writings, correspondence, as well as letters and writings from numerous distinguished fellow scientists. Call Number: MS-3522 Language: Primarily English; some works and correspondence written in French, German, or Italian . Note: The Ransom Center gratefully acknowledges the assistance of the Center for History of Physics, American Institute of Physics, which provided funds to support the processing and cataloging of this collection. Access: Open for research Administrative Information Additional The Richardson Papers were microfilmed and are available on 76 Physical Format reels. Each item has a unique identifying number (W-xxxx, L-xxxx, Available: R-xxxx, or M-xxxx) that corresponds to the microfilm. This number was recorded on the file folders housing the papers and can also be found on catalog slips present with each item. Acquisition: Purchase, 1961 (R43, R44) and Gift, 2005 Processed by: Tessa Klink and Joan Sibley, 2014 Repository: The University of Texas at Austin, Harry Ransom Center Richardson, O. W. (Owen Willans), 1879-1959 MS-3522 2 Richardson, O. W. (Owen Willans), 1879-1959 MS-3522 Biographical Sketch The English physicist Owen Willans Richardson, who pioneered the field of thermionics, was also known for his work on photoelectricity, spectroscopy, ultraviolet and X-ray radiation, the electron theory, and quantum theory. -
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. -
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.