Crustal Structure of Active Deformation Zones in Africa: Implications for Global Crustal Processes C
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Martian Crater Morphology
ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter. -
Depositional Environment of the Gombe Formation in the Gongola Sub-Basin of the Northern Benue Trough: Using Grain Size Parameters
DOI: http://dx.doi.org/10.4314/gjgs.v15i1.3 GLOBAL JOURNAL OF GEOLOGICAL SCIENCES VOL. 15, 2017: 25-39 COPYRIGHT© BACHUDO SCIENCE CO. LTD PRINTED IN NIGERIA ISSN 1596-6798 25 www.globaljournalseries.com, Email: [email protected] DEPOSITIONAL ENVIRONMENT OF THE GOMBE FORMATION IN THE GONGOLA SUB-BASIN OF THE NORTHERN BENUE TROUGH: USING GRAIN SIZE PARAMETERS M. B. USMAN, Y. D. MAMMAN, U. ABUBAKAR, A. SULAIMAN AND H. HAMIDU (Received 16 June 2016; Revision Accepted 25 July 2016) ABSTRACT The depositional environment of the Gombe Formation was determined using grain size parameters in which sixteen sandstone samples and ninety nine pebbles were subjected to granulometric and pebbles morphometric analysis respectively. The granulometric analysis for the sixteen (16) samples of the Gombe Formation show an average graphic mean of 2.51ϕ (fine grained sandstone), mean standard deviation of 0.58ϕ (moderately well sorted sandstone), mean skewness value of 0.09ϕ (nearly symmetrical) and mean kurtosis value of 0.89ϕ (platykurtic). The Bivariate plot of standard deviation vs. skewness indicated dominance of fluvial environment. While the probability curves plots showed a dominance of three sand populations indicating influence of marine processes. Environmental discrimination formulae for Y1, Y2 and Y3 indicated dominance of Aeolian, shallow agitated marine environment and shallow marine environment respectively. The plots of Y2 vs.Y1 and Y3 vs. Y2 showed a dominance shallow marine environment. The morphometric analysis indicates both fluvial and beach environment with dominance of fluvial environment. KEYWORDS: Gombe Formation, Gongola Sub-Basin, Pebbles Morphology, Granulometric analysis, grain size INTRODUCTION Tukur et al. (2015). -
Relative Ages
CONTENTS Page Introduction ...................................................... 123 Stratigraphic nomenclature ........................................ 123 Superpositions ................................................... 125 Mare-crater relations .......................................... 125 Crater-crater relations .......................................... 127 Basin-crater relations .......................................... 127 Mapping conventions .......................................... 127 Crater dating .................................................... 129 General principles ............................................. 129 Size-frequency relations ........................................ 129 Morphology of large craters .................................... 129 Morphology of small craters, by Newell J. Fask .................. 131 D, method .................................................... 133 Summary ........................................................ 133 table 7.1). The first three of these sequences, which are older than INTRODUCTION the visible mare materials, are also dominated internally by the The goals of both terrestrial and lunar stratigraphy are to inte- deposits of basins. The fourth (youngest) sequence consists of mare grate geologic units into a stratigraphic column applicable over the and crater materials. This chapter explains the general methods of whole planet and to calibrate this column with absolute ages. The stratigraphic analysis that are employed in the next six chapters first step in reconstructing -
DMAAC – February 1973
LUNAR TOPOGRAPHIC ORTHOPHOTOMAP (LTO) AND LUNAR ORTHOPHOTMAP (LO) SERIES (Published by DMATC) Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Scale: 1:250,000 Projection: Transverse Mercator Sheet Size: 25.5”x 26.5” The Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Series are the first comprehensive and continuous mapping to be accomplished from Apollo Mission 15-17 mapping photographs. This series is also the first major effort to apply recent advances in orthophotography to lunar mapping. Presently developed maps of this series were designed to support initial lunar scientific investigations primarily employing results of Apollo Mission 15-17 data. Individual maps of this series cover 4 degrees of lunar latitude and 5 degrees of lunar longitude consisting of 1/16 of the area of a 1:1,000,000 scale Lunar Astronautical Chart (LAC) (Section 4.2.1). Their apha-numeric identification (example – LTO38B1) consists of the designator LTO for topographic orthophoto editions or LO for orthophoto editions followed by the LAC number in which they fall, followed by an A, B, C or D designator defining the pertinent LAC quadrant and a 1, 2, 3, or 4 designator defining the specific sub-quadrant actually covered. The following designation (250) identifies the sheets as being at 1:250,000 scale. The LTO editions display 100-meter contours, 50-meter supplemental contours and spot elevations in a red overprint to the base, which is lithographed in black and white. LO editions are identical except that all relief information is omitted and selenographic graticule is restricted to border ticks, presenting an umencumbered view of lunar features imaged by the photographic base. -
Geologic Map of the Victoria Quadrangle (H02), Mercury
H01 - Borealis Geologic Map of the Victoria Quadrangle (H02), Mercury 60° Geologic Units Borea 65° Smooth plains material 1 1 2 3 4 1,5 sp H05 - Hokusai H04 - Raditladi H03 - Shakespeare H02 - Victoria Smooth and sparsely cratered planar surfaces confined to pools found within crater materials. Galluzzi V. , Guzzetta L. , Ferranti L. , Di Achille G. , Rothery D. A. , Palumbo P. 30° Apollonia Liguria Caduceata Aurora Smooth plains material–northern spn Smooth and sparsely cratered planar surfaces confined to the high-northern latitudes. 1 INAF, Istituto di Astrofisica e Planetologia Spaziali, Rome, Italy; 22.5° Intermediate plains material 2 H10 - Derain H09 - Eminescu H08 - Tolstoj H07 - Beethoven H06 - Kuiper imp DiSTAR, Università degli Studi di Napoli "Federico II", Naples, Italy; 0° Pieria Solitudo Criophori Phoethontas Solitudo Lycaonis Tricrena Smooth undulating to planar surfaces, more densely cratered than the smooth plains. 3 INAF, Osservatorio Astronomico di Teramo, Teramo, Italy; -22.5° Intercrater plains material 4 72° 144° 216° 288° icp 2 Department of Physical Sciences, The Open University, Milton Keynes, UK; ° Rough or gently rolling, densely cratered surfaces, encompassing also distal crater materials. 70 60 H14 - Debussy H13 - Neruda H12 - Michelangelo H11 - Discovery ° 5 3 270° 300° 330° 0° 30° spn Dipartimento di Scienze e Tecnologie, Università degli Studi di Napoli "Parthenope", Naples, Italy. Cyllene Solitudo Persephones Solitudo Promethei Solitudo Hermae -30° Trismegisti -65° 90° 270° Crater Materials icp H15 - Bach Australia Crater material–well preserved cfs -60° c3 180° Fresh craters with a sharp rim, textured ejecta blanket and pristine or sparsely cratered floor. 2 1:3,000,000 ° c2 80° 350 Crater material–degraded c2 spn M c3 Degraded craters with a subdued rim and a moderately cratered smooth to hummocky floor. -
Program Schedule
Program Schedule AIAA Science and Technology Forum and Exposition 2015 January 05 - 09, 2015 The Program Report was last updated December 18, 2014 at 04:16 PM EST. To view the most recent meeting schedule online, visit https://aiaa-mst15.abstractcentral.com/planner.jsp Monday, January 05, 2015 Time Session or Event Info 8:00 AM-9:00 AM, Osceola Ballroom CD, PLNRY-01. Opening Keynote , Plenary, Forum 9:00 AM-12:30 PM, St. George 112, ISC-01. International Student Conference (Undergraduate Category), Technical Paper, 53rd AIAA Aerospace Sciences Meeting, Chair: Chris Tavares, The Boeing Company Martian RHOVER Feasibility Study J. Fuentes; R. Pankaja 9:00-9:30 AM Kaluarachchi Satellite Formation Control using Differential Drag S.R. Omar; J.M. 9:30-10:00 AM Wersinger Manufacturing of Triaxial Quasi-three-dimensional Composite 10:00-10:30 AM Materials G. Peterson; D. Liu The Design, Fabrication, and Evaluation of Millimeter Wave Lenses 10:30-11:00 AM for Beamed Energy Applications S.E. Sloan Colorimetric hydrogel-based microfluidic assay system to monitor 11:00-11:30 AM malnutrition in a microgravity environment J.K. Tsosie Significance of Constituent Chemical age on Solid Rocket Propellant 11:30-12:00 PM Regression Rates D.J. Dulin; G.S. Gibson 12:00-12:30 PM Aerodynamic Testing and Development of Sunswift eVe S. Ambrose 9:30 AM-12:30 PM, Miami 2, AA-01. Computational Aeroacoustics I, Technical Paper, 53rd AIAA Aerospace Sciences Meeting, Chair: Walter Eversman, Missouri University of Science and Technology A Computational Study of Flow Within Cavities with Complex 9:30-10:00 AM Geometric Features M.F. -
Scientific Instrument Society
Scientific Instrument Society Bulletin of the Scientific Instrument Society No. 46 September 1995 Bulletin of the Scientific Instrument Society LSSN0956-8271 For Table of Contents, see inside back cover President Gerard Turner Honorary Committee Howard Dawes, Chairman Stuart Talbot, Secretary John Didcock, Treasurer Willem Hackmann, Editor Michael Cowham, Ad~wtising Manager Trevor Waterman, Meetings Secretary Gloria Clifton Jane [nsley Arthur Middleton Alan Morton Membership and Administrative Matters The Executive Officer (Wing Cmdr. Geoffnm] Bennett) 31 High Street Stanford in the Vale Faringdon Tel: 01367 710223 Oxon SN7 8LH Fax: 01367 718963 See inside back cover for information on membership Editorial Matters Dr. Willem D. Hackmann Museum of the History of Science Old Ashmolean Building Tel: 01865 277282 (office) Broad Street Fax: 01865 277288 Oxford OXI 3AZ Tel: 01865 54058 (home) Advertising Mr Michael Cowham The Mount "loft Tel: 01223 263532/262684 Cambridge CB3 7RL Fax: 01223 263948 Organization of Meetings Mr Trevor Waterman 75a Jermyn Street Tel: 0171-930 2954 London SWIY 6NP Fax: 0171-321 0212 Typesetting and Printing Lithoflow Lid 26-36 Wharfdale Road Kings Cross Tel: 0171-833 2344 London NI 9RY Fax: 0171-833 8150 Price: £6 per issue, including back numbers where available. (Please enquire 04 Exec. Officer if sets are required.) The Scientific Instrument Society is Registered Charity No. 326733 © The Scientific lnsVument Society 19')5 Editorial X-ray image of a metal grid taken in THE EM)iF.'.; G.A,ZETTL Crookes' laboratory, but not by him as he -. + .__ was in South Africa when Rontgen's discovery was announced. There is also the metal grid and the X-ray tube used in producing this image. -
PROJECT STREET from to MORATORIUM START FY09-Slurry
PROJECT STREET FROM TO MORATORIUM START FY09-Slurry 01ST AV W WALNUT AV UPAS ST 5/7/2010 FY09-Slurry 01ST AV UPAS ST THORN ST 5/7/2010 FY09-Slurry 01ST AV THORN ST SPRUCE ST 5/7/2010 FY10-Overlay 01ST AV PENNSYLVANIA AV BROOKES AV 7/12/2010 FY10-Slurry 01ST AV LEWIS ST W WASHINGTON ST 1/9/2012 FY10-Slurry 01ST AV ARBOR DR MONTECITO WY 1/11/2012 FY10-Slurry 01ST AV MONTECITO WY LEWIS ST 1/11/2012 FY10-Slurry 01ST AV W WASHINGTON ST UNIVERSITY AV 1/11/2012 FY10-Slurry 01ST AV UNIVERSITY AV ROBINSON AV 1/11/2012 FY11-Slurry 01ST AV BEECH ST ASH ST 9/9/2012 FY11-Slurry 01ST AV ASH ST A ST 9/9/2012 FY11-Slurry 01ST AV A ST W B ST 9/9/2012 FY11-Slurry 01ST AV W B ST C ST 9/9/2012 FY11-Slurry 01ST AV ELM ST CEDAR ST 9/9/2012 FY11-Slurry 01ST AV CEDAR ST BEECH ST 9/9/2012 FY11-Overlay 01ST AV ROBINSON AV PENNSYLVANIA AV 10/10/2012 FY08-Overlay 02ND AV ASH ST A ST 4/10/2009 FY09-Overlay 02ND AV C ST BROADWAY 11/3/2009 FY09-Slurry 02ND AV WALNUT AV UPAS ST 5/26/2010 FY09-Slurry 02ND AV UPAS ST THORN ST 5/26/2010 FY09-Slurry 02ND AV THORN ST SPRUCE ST 5/26/2010 FY11-Overlay 02ND AV MARKET ST ISLAND AV 10/16/2012 FY11-Overlay 02ND AV ISLAND AV J ST 10/16/2012 FY09-Slurry 03RD AV LEWIS ST WASHINGTON ST 5/7/2010 FY09-Slurry 03RD AV END ARBOR DR 5/27/2010 FY09-Slurry 03RD AV ARBOR DR MONTECITO WY 5/28/2010 FY09-Slurry 03RD AV MONTECITO WY LEWIS ST 5/28/2010 FY10-Slurry 03RD AV WALNUT AV UPAS ST 1/11/2012 FY11-Slurry 03RD AV UNIVERSITY AV ROBINSON AV 6/5/2012 FY11-Slurry 03RD AV ROBINSON AV PENNSYLVANIA AV 6/5/2012 FY11-Slurry 03RD AV PENNSYLVANIA AV -
Apollo 17 Index: 70 Mm, 35 Mm, and 16 Mm Photographs
General Disclaimer One or more of the Following Statements may affect this Document This document has been reproduced from the best copy furnished by the organizational source. It is being released in the interest of making available as much information as possible. This document may contain data, which exceeds the sheet parameters. It was furnished in this condition by the organizational source and is the best copy available. This document may contain tone-on-tone or color graphs, charts and/or pictures, which have been reproduced in black and white. This document is paginated as submitted by the original source. Portions of this document are not fully legible due to the historical nature of some of the material. However, it is the best reproduction available from the original submission. Produced by the NASA Center for Aerospace Information (CASI) Preparation, Scanning, Editing, and Conversion to Adobe Portable Document Format (PDF) by: Ronald A. Wells University of California Berkeley, CA 94720 May 2000 A P O L L O 1 7 I N D E X 7 0 m m, 3 5 m m, A N D 1 6 m m P H O T O G R A P H S M a p p i n g S c i e n c e s B r a n c h N a t i o n a l A e r o n a u t i c s a n d S p a c e A d m i n i s t r a t i o n J o h n s o n S p a c e C e n t e r H o u s t o n, T e x a s APPROVED: Michael C . -
Abstract Volume
T I I II I II I I I rl I Abstract Volume LPI LPI Contribution No. 1097 II I II III I • • WORKSHOP ON MERCURY: SPACE ENVIRONMENT, SURFACE, AND INTERIOR The Field Museum Chicago, Illinois October 4-5, 2001 Conveners Mark Robinbson, Northwestern University G. Jeffrey Taylor, University of Hawai'i Sponsored by Lunar and Planetary Institute The Field Museum National Aeronautics and Space Administration Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPI Contribution No. 1097 Compiled in 2001 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 paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication .... This volume may be cited as Author A. B. (2001)Title of abstract. In Workshop on Mercury: Space Environment, Surface, and Interior, p. xx. LPI Contribution No. 1097, Lunar and Planetary Institute, Houston. This report 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: order@lpi:usra.edu Please contact the Order Department for ordering information, i,-J_,.,,,-_r ,_,,,,.r pA<.><--.,// ,: Mercury Workshop 2001 iii / jaO/ Preface This volume contains abstracts that have been accepted for presentation at the Workshop on Mercury: Space Environment, Surface, and Interior, October 4-5, 2001. -
2D Mercury Crater Wordsearch V2
3/24/2019 Word Search Generator :: Create your own printable word find worksheets @ A to Z Teacher Stuff MAKE YOUR OWN WORKSHEETS ONLINE @ WWW.ATOZTEACHERSTUFF.COM NAME:_______________________________ DATE:_____________ Craters on Mercury SICINIMODFIQPVMRQSLJ BEETHOVEN MICHELANGELO BLTVPTSDUOMRCIPDRAEN BYRON RAPHAEL YAPVWYPXSEHAUEHSEVDI CUNNINGHAM SAVAGE RRZAYRKFJROGNIGSNAIA DAMER SHAKESPEARE ORTNPIVOCDTJNRRSKGSW DOMINICI SVEINSDOTTIR NOMGETIKLKEUIAAGLEYT DRISCOLL TOLSTOI PCLOLTVLOEPSNDPNUMQK ELLINGTON VANGOGH YHEGLOAAEIGEGAHQAPRR FAULKNER VIEIRADASILVA NANHIDLNTNNNHSAOFVLA HEMINGWAY VIVALDI VDGYNSDGGMNGAIEDMRAM HOLST GALQGNIEBIMOMLLCNEZG HOMER VMESTIWWKWCANVEKLVRU IMHOTEP ZELTOEPSBOAWMAUHKCIS IZQUIERDO JRQGNVMODREIUQZICDTH JOPLIN SHAKESPEARETOLSTOIOX KIPLING BBCZWAQSZRSLPKOJHLMA LANGE SFRLLOCSIRDIYGSSSTQT LARROCHA FKUIDTISIYYFAIITRODE LENGLE NILPOJHEMINGWAYEGXLM LENNON BEETHOVENRYSKIPLINGV MARKTWAIN 1/2 Mercury Craters: Famous Writers, Artists, and Composers: Location and Sizes Beethoven: Ludwig van Beethoven (1770−1827). German composer and pianist. 20.9°S, 124.2°W; Diameter = 630 km. Byron: Lord Byron (George Byron) (1788−1824). British poet and politician. 8.4°S, 33°W; Diameter = 106.6 km. Cunningham: Imogen Cunningham (1883−1976). American photographer. 30.4°N, 157.1°E; Diameter = 37 km. Damer: Anne Seymour Damer (1748−1828). English sculptor. 36.4°N, 115.8°W; Diameter = 60 km. Dominici: Maria de Dominici (1645−1703). Maltese painter, sculptor, and Carmelite nun. 1.3°N, 36.5°W; Diameter = 20 km. Driscoll: Clara Driscoll (1861−1944). American glass designer. 30.6°N, 33.6°W; Diameter = 30 km. Ellington: Edward Kennedy “Duke” Ellington (1899−1974). American composer, pianist, and jazz orchestra leader. 12.9°S, 26.1°E; Diameter = 216 km. Faulkner: William Faulkner (1897−1962). American writer and Nobel Prize laureate. 8.1°N, 77.0°E; Diameter = 168 km. Hemingway: Ernest Hemingway (1899−1961). American journalist, novelist, and short-story writer. 17.4°N, 3.1°W; Diameter = 126 km. -
Adams Adkinson Aeschlimann Aisslinger Akkermann
BUSCAPRONTA www.buscapronta.com ARQUIVO 27 DE PESQUISAS GENEALÓGICAS 189 PÁGINAS – MÉDIA DE 60.800 SOBRENOMES/OCORRÊNCIA Para pesquisar, utilize a ferramenta EDITAR/LOCALIZAR do WORD. A cada vez que você clicar ENTER e aparecer o sobrenome pesquisado GRIFADO (FUNDO PRETO) corresponderá um endereço Internet correspondente que foi pesquisado por nossa equipe. Ao solicitar seus endereços de acesso Internet, informe o SOBRENOME PESQUISADO, o número do ARQUIVO BUSCAPRONTA DIV ou BUSCAPRONTA GEN correspondente e o número de vezes em que encontrou o SOBRENOME PESQUISADO. Número eventualmente existente à direita do sobrenome (e na mesma linha) indica número de pessoas com aquele sobrenome cujas informações genealógicas são apresentadas. O valor de cada endereço Internet solicitado está em nosso site www.buscapronta.com . Para dados especificamente de registros gerais pesquise nos arquivos BUSCAPRONTA DIV. ATENÇÃO: Quando pesquisar em nossos arquivos, ao digitar o sobrenome procurado, faça- o, sempre que julgar necessário, COM E SEM os acentos agudo, grave, circunflexo, crase, til e trema. Sobrenomes com (ç) cedilha, digite também somente com (c) ou com dois esses (ss). Sobrenomes com dois esses (ss), digite com somente um esse (s) e com (ç). (ZZ) digite, também (Z) e vice-versa. (LL) digite, também (L) e vice-versa. Van Wolfgang – pesquise Wolfgang (faça o mesmo com outros complementos: Van der, De la etc) Sobrenomes compostos ( Mendes Caldeira) pesquise separadamente: MENDES e depois CALDEIRA. Tendo dificuldade com caracter Ø HAMMERSHØY – pesquise HAMMERSH HØJBJERG – pesquise JBJERG BUSCAPRONTA não reproduz dados genealógicos das pessoas, sendo necessário acessar os documentos Internet correspondentes para obter tais dados e informações. DESEJAMOS PLENO SUCESSO EM SUA PESQUISA.