Tunguska Event (1908)
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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. -
Source of Knowledge, Techniques and Skills That Go Into the Development of Technology, and Prac- Tical Applications
DOCUMENT RESUME ED 027 216 SE 006 288 By-Newell, Homer E. NASA's Space Science and Applications Program. National Aeronautics and Space Administration, Washington, D.C. Repor t No- EP -47. Pub Date 67 Note-206p.; A statement presented to the Committee on Aeronautical and Space Sciences, United States Senate, April 20, 1967. EDRS Price MF-$1.00 HC-$10.40 Descriptors-*Aerospace Technology, Astronomy, Biological Sciences, Earth Science, Engineering, Meteorology, Physical Sciences, Physics, *Scientific Enterprise, *Scientific Research Identifiers-National Aeronautics and Space Administration This booklet contains material .prepared by the National Aeronautic and Space AdMinistration (NASA) office of Space Science and Applications for presentation.to the United States Congress. It contains discussion of basic research, its valueas a source of knowledge, techniques and skillsthat go intothe development of technology, and ioractical applications. A series of appendixes permitsa deeper delving into specific aspects of. Space science. (GR) U.S. DEPARTMENT OF HEALTH, EDUCATION & WELFARE OFFICE OF EDUCATION THIS DOCUMENT HAS BEEN REPRODUCED EXACTLY AS RECEIVEDFROM THE PERSON OR ORGANIZATION ORIGINATING IT.POINTS OF VIEW OR OPINIONS STATED DO NOT NECESSARILY REPRESENT OFFICIAL OMCE OFEDUCATION POSITION OR POLICY. r.,; ' NATiONAL, AERONAUTICS AND SPACEADi4N7ISTRATION' , - NASNS SPACE SCIENCE AND APPLICATIONS PROGRAM .14 A Statement Presented to the Committee on Aeronautical and Space Sciences United States Senate April 20, 1967 BY HOMER E. NEWELL Associate Administrator for Space Science and Applications National Aeronautics and Space Administration Washington, D.C. 20546 +77.,M777,177,,, THE MATERIAL in this booklet is a re- print of a portion of that which was prepared by NASA's Office of Space Science and Ap- -olications for presentation to the Congress of the United States in the course of the fiscal year 1968 authorization process. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
P Hot0 M Etric I Nv Est I6 Ations
25 April 1968 RSIC-796 P HOT0M ETRIC INV EST I6 ATIONS OF THE LUNAR SURFACE bY V. G. Fesenkov Astronomicheskii Zhurnal 5, pp. 219-234 (1929) Translated from the Russian THIS DOCUMENT HAS BEEN APPROVED FOR PUBLIC RELEASE AND SALE; ITS DISTRIBUTION IS UNLIMITED Translation Branch Redstone Scientific Information Center Research and Development Directorate U. S. Army Missile Command Redstone Arsenal, Alabama 35809 PHOTOMETRIC INVESTIGATIONS OF THE LUNAR SURFACE V. G. Fesenkov The aim of this paper is the determination of the law according to which , the light is reflected from the different parts of the lunar surface under various angles of incidence, reflection and phase. The photograms of the Moon obtained by Surovtseff in the focus of the normal astrograph of the Tashkent Astronomical Observatory were measured at the Astrophysical Institute of Moscow with the Harmann microphotometer. The photographic densities obtained with this instrument were transformed into brightness of the corresponding points by means of the scale of tubular photo- meter printed on each plate exactly with the same exposure. The extrafocal images of the Polar star photographed on the same plates with many different exposures were utilized for the determination of the same unit of brightness. The brightness of the different points of the Moon were corrected for effect of halation. It is found that our photometrical determinations for all phases from 0" up to 140" may be represented in a very satisfactory way by the simple expression which is a modification of the very well known Lommel-Seeliger's formula. This paper investigates the law of reflection of the light from lunar surface at different angles of incidence, reflection, and phase. -
Meteorites and the Smithsonian Institution Russian)
M.A. IVANOV A & M.A. NAZAROV 236 V M 1811. A report on air stones Of ai~o- 55 Principles of Meteoritics. SEVERGIN, .' . the Museum of the lmpenal KRINov, E.L. 19 . ( d) State publishers ?f lithes preserved l~ 'Technological journal, Fesenkov, V.G. e... Moscow (lll Academy of s clences., Technical/Theoretical LIterature, VIII 129-132 (in Russian). N rth Meteorites and the Smithsonian Institution Russian). R ' Moscow Nauka, ' 1809 On a New Map of the 0 em KRINOV , E.L. 1981. Iro.n am. STEHLIN; jA. d ecimen of native iron. Philoso- 2 Archipelago, an .sp .J' the Royal Society of ROY S. CLARKE, JR!, HOWARD PLOTKIN & TIMOTHY J. McCOY! Moscow, 192 (in Ru~:a~'F Chladny _ a founder phical TransactIOns OJ MASSALSKAYA, K.P. 19 . ' 'M' 'tika 11 33-46 1 Department of Mineral Sciences, National Museum of Natural History, of scientific meteontlcS. eteon , , London LXIY, l774, 46l. Th 'r • A 1807 On Aerial Stones and el STOlKQVICH,.. .' f Kharkov Kharkov, 271 Smithsonian Institution, Washington, DC 20560-0119, USA (in Russian). M' I us Showers 01" Stones Origin. Umverslty 0 , 1M 1819 On tracu 0 'J 2Department of Philosophy, University of Western Ontario, London, Canada N6A 3K7 MUKHI~,.. h~ Air (Aeroli!hes). Imperial Foun~- (in Russian). h in ~alling F~°alm 'Publisher St Petersburg, 207 (m o 1915. AstronomIc P enomena (e-mail: [email protected]) hng-HospJt ' SVI~TSK.Y, ~;st~rical Chronicles Considered from a Russian). A 2000 The meteorite collection of the usswn . "V' Bulletin of the Department NAZAROV, M.. f Sciences In: ALEKSEEVA, Scientific. -
User Guide To
USER GUIDE TO 1 2 5 0 , 000 S CA L E L U NA R MA P S DANNY C. KINSLER Lunar Science Institute 3303 NASA Road #1 Houston, TX 77058 Telephone: 713/488-5200 Cable Address: LUNSI The Lunar Science Institute is operated by the Universities Space Research Association under Contract No. NSR 09-051-001 with the National Aeronautics and Space Administration. This document constitutes LSI Contribution No. 206 March 1975 USER GUIDE TO 1 : 250 , 000 SCALE LUNAR MAPS GENERAL In 1 972 the NASA Lunar Programs Office initiated the Apoll o Photographic Data Analysis Program. The principal point of this program was a detail ed scientific analysis of the orbital and surface experiments data derived from Apollo missions 15, 16, and 17 . One of the requirements of this program was the production of detailed photo base maps at a useabl e scale . NASA in conjunction with the Defense Mapping Agency (DMA) commenced a mapping program in early 1973 that would lead to the production of the necessary maps based on the need for certain areas . This paper is desi gned to present in outline form the neces- sary background information for users to become familiar with the program. MAP FORMAT The scale chosen for the project was 1:250,000* . The re- search being done required a scale that Principal Investigators (PI's) using orbital photography could use, but would also serve PI's doing surface photographic investigations. Each map sheet covers an area four degrees north/south by five degrees east/west. The base is compiled from vertical Metric photography from Apollo missions 15, 16, and 17. -
Terrestrial Impact Structures- a Bibliography 1965-68
Terrestrial Impact Structures- A Bibliography 1965-68 By JACQUELYN H. FREEBERG GEOLOGICAL SURVEY BULLETIN 1320 UNITED STATES GOVERNMENT PRINTING OFFICE, WASHINGTON : 1969 UNITED STATES DEPARTMENT OF THE INTERIOR WALTER J. HICKEL, Secretary GEOLOGICAL SURVEY William T. Pecora, Director Library of Congress catalog-card No. 74-650225 For sale by the Superintendent of Documents, U.S. Government Printing Office Washington, D.C. 20402 - Price 30 cents paper cover CONTENTS Page Abstract--------------------------------------------------------- 1 Introduction______________________________________________________ 1 Seria~----------------------------------------------------------- 2 Bibliography______________________________________________________ 3· Distribution and general characteristics of impact structures_________ 3: Impact sites___________________________________________________ 12: Agnak Island Oraters _ _ __ _ __ _ __ __ _ __ __ _ _ _ __ __ _ _ __ _ _ _ __ _ _ _ __ 1Z Aouelloul Crater___________________________________________ 12 Arn Valley Craters________________________________________ 12 Barringer Crater__________________________________________ 12 Bass Strait_______________________________________________ 13 Boxhole Crater____________________________________________ 14 Brent Crater______________________________________________ 14 Butare Crater_______________________________________ ------ 14 Campo del Cielo Craters----------------------------------- 14 Carswell Lake structure _________________________ . _ _ _ __ _ _ __ _ 15 Chassenon -
Astronautical and Aeronautical Events of 1962
[COMMITTEE PRINT] ASTRONAUTICAL AND AERONAUTICAL EVENTS OF 1962 REPORT OF THE 1 NATIONAL AERONAUTICS AND SPACE ADMINISTRATION TO THE COMMITTEE ON SCIENCE AND ASTRONAUTICS U.S. HOUSE OF REPRESENTATIVES EIGHTY-EIGHTH CONGRESS FIRST SESSION JUNE 12, 1963 I Printed for the use of the Committee on Science and Astronautics I [COMMmEE PRINT] ASTRONAUTICAL AND AERONAUTICAL EVENTS OF 1962 REPORT OF THE NATIONAL AERONAUTICS AND SPACE ADMINISTRATION TO THE COMMITTEE ON SCIENCE AND ASTRONAUTICS U.S. HOUSE OF REPRESENTATIVES EIGHTY-EIGHTH CONGRESS FIRST SESSION JUNE 12, 1963 Printed for the use of the Committee on Science and Astronautics U.S. GOVERNMENT PRINTING OFFICE 97317 WASHINGTON : 1963 For sale by the Superintendent of Documents, U.S. Government Printing OfEw Washington 25, D.C. - Price $1.00 COMMITTEE ON SCIENCE AND ASTRONAUTICS GEORGE P. MILLER, California, Chairman OLIN E. TEAGUE, Texas JOSEPH W. MARTIN, JR., Massachusetts JOSEPH E. RARTH, Minnesota JAMES G. FULTON, Pennsylvania KEN HECHLER, West Virginia J. EDGAR CHENOWETH, Colorado EMILIO Q. DADDARIO, Connecticut WILLIAM I(. VAN PELT, Wisconsin J. EDWARD ROUSH, Indiana R. WALTER RIEHLMAN, New York THOMAS 0. MORRIS, New Mexico CHARLES A. MOSHER, Ohio BOB CASEY, Texas RICHARD L. ROUDEBUSH, Indiana WILLIAM J. RANDALL, Missouri ALPHONZO BELL, California JOHN W. DAVIS, Georgia THOMAS M. PELLY, Washington WILLIAM F. RYAN, New York DONALD RUMSFELD, Jllinois THOMAS N. DOWNING, Virginia JAMES D. WEAVER, Pennsylvania JOE D. WAGGONNER, JR., Louisiana EDWARD J. GURNEY, Florida EDWARD J. PATTEN, New Jersey JOHN W, WYDLER, New York RICHARD H. FULTON, Tennessee DON FUQUA, Florida NEIL STAEBLER, Michigan CARL ALBERT, Oklahoma CHARLESF. DUCANDER,Ezecutive Diretor and Chief Counsel JOHNA. -
Thedatabook.Pdf
THE DATA BOOK OF ASTRONOMY Also available from Institute of Physics Publishing The Wandering Astronomer Patrick Moore The Photographic Atlas of the Stars H. J. P. Arnold, Paul Doherty and Patrick Moore THE DATA BOOK OF ASTRONOMY P ATRICK M OORE I NSTITUTE O F P HYSICS P UBLISHING B RISTOL A ND P HILADELPHIA c IOP Publishing Ltd 2000 All rights reserved. No part of this publication may be reproduced, stored in a retrieval system or transmitted in any form or by any means, electronic, mechanical, photocopying, recording or otherwise, without the prior permission of the publisher. Multiple copying is permitted in accordance with the terms of licences issued by the Copyright Licensing Agency under the terms of its agreement with the Committee of Vice-Chancellors and Principals. British Library Cataloguing-in-Publication Data A catalogue record for this book is available from the British Library. ISBN 0 7503 0620 3 Library of Congress Cataloging-in-Publication Data are available Publisher: Nicki Dennis Production Editor: Simon Laurenson Production Control: Sarah Plenty Cover Design: Kevin Lowry Marketing Executive: Colin Fenton Published by Institute of Physics Publishing, wholly owned by The Institute of Physics, London Institute of Physics Publishing, Dirac House, Temple Back, Bristol BS1 6BE, UK US Office: Institute of Physics Publishing, The Public Ledger Building, Suite 1035, 150 South Independence Mall West, Philadelphia, PA 19106, USA Printed in the UK by Bookcraft, Midsomer Norton, Somerset CONTENTS FOREWORD vii 1 THE SOLAR SYSTEM 1 -
National Aeronautics and Space Administration) 111 P HC AO,6/MF A01 Unclas CSCL 03B G3/91 49797
https://ntrs.nasa.gov/search.jsp?R=19780004017 2020-03-22T06:42:54+00:00Z NASA TECHNICAL MEMORANDUM NASA TM-75035 THE LUNAR NOMENCLATURE: THE REVERSE SIDE OF THE MOON (1961-1973) (NASA-TM-75035) THE LUNAR NOMENCLATURE: N78-11960 THE REVERSE SIDE OF TEE MOON (1961-1973) (National Aeronautics and Space Administration) 111 p HC AO,6/MF A01 Unclas CSCL 03B G3/91 49797 K. Shingareva, G. Burba Translation of "Lunnaya Nomenklatura; Obratnaya storona luny 1961-1973", Academy of Sciences USSR, Institute of Space Research, Moscow, "Nauka" Press, 1977, pp. 1-56 NATIONAL AERONAUTICS AND SPACE ADMINISTRATION M19-rz" WASHINGTON, D. C. 20546 AUGUST 1977 A % STANDARD TITLE PAGE -A R.,ott No0... r 2. Government Accession No. 31 Recipient's Caafog No. NASA TIM-75O35 4.-"irl. and Subtitie 5. Repo;t Dote THE LUNAR NOMENCLATURE: THE REVERSE SIDE OF THE August 1977 MOON (1961-1973) 6. Performing Organization Code 7. Author(s) 8. Performing Organizotion Report No. K,.Shingareva, G'. .Burba o 10. Coit Un t No. 9. Perlform:ng Organization Nome and Address ]I. Contract or Grant .SCITRAN NASw-92791 No. Box 5456 13. T yp of Report end Period Coered Santa Barbara, CA 93108 Translation 12. Sponsoring Agiicy Noms ond Address' Natidnal Aeronautics and Space Administration 34. Sponsoring Agency Code Washington,'.D.C. 20546 15. Supplamortary No9 Translation of "Lunnaya Nomenklatura; Obratnaya storona luny 1961-1973"; Academy of Sciences USSR, Institute of Space Research, Moscow, "Nauka" Press, 1977, pp. Pp- 1-56 16. Abstroct The history of naming the details' of the relief on.the near and reverse sides 6f . -
Ernst Julius Piks (1916) Note on the Theory of Explosion Cratering on The
Meteoritics & Planetary Science 49, Nr 10, 1851–1874 (2014) doi: 10.1111/maps.12367 Ernst Julius Opik’s€ (1916) note on the theory of explosion cratering on the Moon’s surface—The complex case of a long-overlooked benchmark paper Grzegorz RACKI1*, Christian KOEBERL2,3,Tonu~ VIIK4, Elena A. JAGT-YAZYKOVA5,6, and John W. M. JAGT7 1Faculty of Earth Sciences, University of Silesia, ul. Bezdzinska 60, 41-200 Sosnowiec, Poland 2Department of Lithospheric Research, University of Vienna, 1090 Vienna, Austria 3Natural History Museum, Burgring 7, 1010 Vienna, Austria 4Tartu Observatory, Toravere,~ Tartumaa 61602, Estonia 5Laboratory of Paleobiology, Faculty of Natural and Technical Sciences, University of Opole, ul. Oleska 22, 45-052 Opole, Poland 6Saint Petersburg State University, Universitetskaya nab. 7-9, Saint Petersburg 199034, Russia 7Natuurhistorisch Museum Maastricht, de Bosquetplein 6-7, 6211 KJ Maastricht, the Netherlands *Corresponding author. E-mail: [email protected] (Received 09 March 2014; revision accepted 02 August 2014) Abstract–High-velocity impact as a common phenomenon in planetary evolution was ignored until well into the twentieth century, mostly because of inadequate understanding of cratering processes. An eight-page note, published in Russian by the young Ernst Julius Opik,€ a great Estonian astronomer, was among the key selenological papers, but due to the language barrier, it was barely known and mostly incorrectly cited. This particular paper is here intended to serve as an explanatory supplement to an English translation of Opik’s€ article, but also to document an early stage in our understanding of cratering. First, we outline the historical–biographical background of this benchmark paper, and second, a comprehensive discussion of its merits is presented, from past and present perspectives alike. -
Lunar Eclipses and Allais Effect 1
1 LUNAR ECLIPSES AND ALLAIS EFFECT Russell Bagdoo [email protected] ABSTRACT Two anomalies observed during lunar eclipses, the enlargement of the Earth`s shadow and the excessive clarity of the penumbra, possibly attributed to insufficient causes if not doubtful, would refute the assertion of certain experimenters according to which the lunar Allais eclipse effect would be almost impossible to detect. The Earth`s umbra seems to be 2% larger than what is expected from geometrical considerations and it is believed that the Earth`s atmosphere is responsible for the extent of the enlargement, but it is realized that the atmospheric absorption cannot explain light absorption at a height as high as 90 km above the Earth, as required by this hypothesis. It was also argued that the irradiation of the Moon in the Earth`s shadow during the eclipse is caused by the refraction of sunlight in the upper regions of the Earth`s atmosphere. However, the shade toward the center is too bright to be accounted for by refraction of visible sunlight. Although these assumptions are not trifling, we attribute the majority of these abnormalities to the Allais eclipse effect. This effect would cause a slight decrease of gravity during the eclipse: the geodesics would be displaced a small amount outwards, the ray of light coming from the Sun, passing close by the Moon would be less attracted, which would expand the shadow cone of the Moon. On the other hand, the rays emanating from the Moon would have a shorter wavelength and therefore the luminescence would increase by anti-Stoke Raman effect: the scattered photon has more energy than the absorbed photon.