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Lunar Orbiter Photographic Atlas of the Near Side of the Moon Charles J
Lunar Orbiter Photographic Atlas of the Near Side of the Moon Charles J. Byrne Lunar Orbiter Photographic Atlas of the Near Side of the Moon Charles J. Byrne Image Again Middletown, NJ USA Cover illustration: Earth-based photograph of the full Moon from the “Consolidated Lunar Atlas” on the Website of the Lunar and Planetary Institute. British Library Cataloging-in-Publication Data Byrne, Charles J., 1935– Lunar Orbiter photographic atlas of the near side of the Moon 1. Lunar Orbiter (Artificial satellite) 2. Moon–Maps 3. Moon–Photographs from space I. Title 523.3 0223 ISBN 1852338865 Library of Congress Cataloging-in-Publication Data Byrne, Charles J., 1935– Lunar Orbiter photographic atlas of the near side of the Moon : with 619 figures / Charles J. Byrne. p. cm. Includes bibliographical references and index. ISBN 1-85233-886-5 (acid-free paper) 1. Moon–Maps. 2. Moon–Photographs from space. 3. Moon–Remote-sensing images. 4. Lunar Orbiter (Artificial satellite) I. Title. G1000.3.B9 2005 523.3 022 3–dc22 2004045006 Additional material to this book can be downloaded from http://extras.springer.com. ISBN 1-85233-886-5 Printed on acid-free paper. © 2005 Springer-Verlag London Limited Apart from any fair dealing for the purposes of research or private study, or criticism, or review, as permitted under the Copyright, Designs and Patents Act 1988, this publication may only be repro- duced, stored or transmitted, in any form or by any means, with the prior permission in writing of the publishers, or in the case of reprographic reproduction in accordance with the terms of licenses issued by the Copyright Licensing Agency. -
Glossary Glossary
Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts. -
Special Catalogue Milestones of Lunar Mapping and Photography Four Centuries of Selenography on the Occasion of the 50Th Anniversary of Apollo 11 Moon Landing
Special Catalogue Milestones of Lunar Mapping and Photography Four Centuries of Selenography On the occasion of the 50th anniversary of Apollo 11 moon landing Please note: A specific item in this catalogue may be sold or is on hold if the provided link to our online inventory (by clicking on the blue-highlighted author name) doesn't work! Milestones of Science Books phone +49 (0) 177 – 2 41 0006 www.milestone-books.de [email protected] Member of ILAB and VDA Catalogue 07-2019 Copyright © 2019 Milestones of Science Books. All rights reserved Page 2 of 71 Authors in Chronological Order Author Year No. Author Year No. BIRT, William 1869 7 SCHEINER, Christoph 1614 72 PROCTOR, Richard 1873 66 WILKINS, John 1640 87 NASMYTH, James 1874 58, 59, 60, 61 SCHYRLEUS DE RHEITA, Anton 1645 77 NEISON, Edmund 1876 62, 63 HEVELIUS, Johannes 1647 29 LOHRMANN, Wilhelm 1878 42, 43, 44 RICCIOLI, Giambattista 1651 67 SCHMIDT, Johann 1878 75 GALILEI, Galileo 1653 22 WEINEK, Ladislaus 1885 84 KIRCHER, Athanasius 1660 31 PRINZ, Wilhelm 1894 65 CHERUBIN D'ORLEANS, Capuchin 1671 8 ELGER, Thomas Gwyn 1895 15 EIMMART, Georg Christoph 1696 14 FAUTH, Philipp 1895 17 KEILL, John 1718 30 KRIEGER, Johann 1898 33 BIANCHINI, Francesco 1728 6 LOEWY, Maurice 1899 39, 40 DOPPELMAYR, Johann Gabriel 1730 11 FRANZ, Julius Heinrich 1901 21 MAUPERTUIS, Pierre Louis 1741 50 PICKERING, William 1904 64 WOLFF, Christian von 1747 88 FAUTH, Philipp 1907 18 CLAIRAUT, Alexis-Claude 1765 9 GOODACRE, Walter 1910 23 MAYER, Johann Tobias 1770 51 KRIEGER, Johann 1912 34 SAVOY, Gaspare 1770 71 LE MORVAN, Charles 1914 37 EULER, Leonhard 1772 16 WEGENER, Alfred 1921 83 MAYER, Johann Tobias 1775 52 GOODACRE, Walter 1931 24 SCHRÖTER, Johann Hieronymus 1791 76 FAUTH, Philipp 1932 19 GRUITHUISEN, Franz von Paula 1825 25 WILKINS, Hugh Percy 1937 86 LOHRMANN, Wilhelm Gotthelf 1824 41 USSR ACADEMY 1959 1 BEER, Wilhelm 1834 4 ARTHUR, David 1960 3 BEER, Wilhelm 1837 5 HACKMAN, Robert 1960 27 MÄDLER, Johann Heinrich 1837 49 KUIPER Gerard P. -
University Microfilms International T U T T L E , V Ir G in Ia G R a C E
INFORMATION TO USERS This was produced from a copy of a document sent to us for microfilming. While the most advanced technological means to photograph and reproduce this document have been used, the quality is heavily dependent upon the quality of the material subm itted. The following explanation of techniques is provided to help you understand markings or notations which may appear on this reproduction. 1. The sign or “target” for pages apparently lacking from the document photographed is “Missing Page(s)”. If it was possible to obtain the missing page(s) or section, they are spliced into the film along with adjacent pages. This may have necessitated cutting through an image and duplicating adjacent pages to assure you of complete continuity. 2. When an image on the film is obliterated with a round black mark it is an indication that the film inspector noticed either blurred copy because of movement during exposure, or duplicate copy. Unless we meant to delete copyrighted materials that should not have been filmed, you will find a good image of the page in the adjacent frame. 3. When a map, drawing or chart, etc., is part of the material being photo graphed the photographer has followed a definite method in “sectioning” the material. It is customary to begin filming at the upper left hand corner of a large sheet and to continue from left to right in equal sections with small overlaps. If necessary, sectioning is continued again-beginning below the first row and continuing on until complete. 4. For any illustrations that cannot be reproduced satisfactorily by xerography, photographic prints can be purchased at additional cost and tipped into your xerographic copy. -
Oral Histories in Meteoritics and Planetary Science – XX: Dale P
Oral Histories in Meteoritics and Planetary Science – XX: Dale P. Cruikshank by Derek W. G. Sears Planetary Science and Astrobiology Division NASA Ames Research Center, Mountain View California. SUPPLEMENTAL INFORMATION Recollections of Gerard Kuiper DS: Okay, so we have recorded your oral history, let’s spend some time recollecting your interactions with Gerard Kuiper. You described how you met him at Yerkes Observatory as an undergraduate and how you went to graduate school after he moved to the University of Arizona DC: Alan Binder and I applied to graduate school in Arizona and did our graduate training there. At about the same time, Bill Hartmann came to Tucson as a graduate student from Penn State, Elliott Moore and Tobias Owen also came as students from the University of Chicago. Several astronomers and atmospheric physicists also came to Tucson in those first years; Joseph Chamberlain, Donald Hunten, and Lloyd Wallace came to Arizona and joined the staff at the Kitt Peak National Observatory. The National Observatory had decided to locate in Tucson and build its observatory at Kitt Peak some 40 miles outside of town. By the time Kuiper got there Kitt Peak National Observatory was becoming quite a significant national establishment, and that provided a strong draw to the area. The Kitt Peak offices were located on the edge of the University of Arizona campus, just across the street from the University's Steward Observatory. When Kuiper left Yerkes several people involved in his lunar studies enterprise went with him, including David Arthur and Ewen Whitaker. Eventually Tom Gehrels, formerly associated with Kuiper at the University of Chicago, joined the group in Tucson. -
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. -
Its Founding and Early Years Ewen A. Whitaker
The University of Arizona's LUNAR AND PLANETARY LABORATORY Its Founding and Early Years Ewen A. Whitaker Set in Varityper Times Roman and printed at the University of Arizona Printing-Reproductions Department Equal Employment Opportunity· Affirmative Action Employer CONTENTS THE PRE-TUCSON ERA Historical background ........................................ I Enter Gerard P. Kuiper ....................................... 2 The Moon enters the picture ................................... 3 A call for suggestions ......................................... 5 The Harold Urey affair ....................................... 6 Preliminaries for the Lunar Atlas ............................... 7 1957 - a dream begins to take shape ............................. 7 The shot that was seen (and heard) around the world ............... 8 Other irons in the fire ......................................... 9 Kuiper seeks full-time help for the Lunar Project .................. 9 1959 - the Lunar Project gathers momentum ..................... 11 A new factor in the Lunar Project LPL story ................... 12 The Air Force enters the lunar cartography business ............... 13 The Lunar Atlas published at last .............................. 14 Big problems with the Yerkes set-up ............................ : 6 The southwestern U.S. begins to beckon ........................ 17 "There is a tide in the affairs of men ..." ....................... 18 Preparing for the move ...................................... 23 THE TUCSON ERA The Lunar Project makes the transfer -
Water on the Moon, III. Volatiles & Activity
Water on The Moon, III. Volatiles & Activity Arlin Crotts (Columbia University) For centuries some scientists have argued that there is activity on the Moon (or water, as recounted in Parts I & II), while others have thought the Moon is simply a dead, inactive world. [1] The question comes in several forms: is there a detectable atmosphere? Does the surface of the Moon change? What causes interior seismic activity? From a more modern viewpoint, we now know that as much carbon monoxide as water was excavated during the LCROSS impact, as detailed in Part I, and a comparable amount of other volatiles were found. At one time the Moon outgassed prodigious amounts of water and hydrogen in volcanic fire fountains, but released similar amounts of volatile sulfur (or SO2), and presumably large amounts of carbon dioxide or monoxide, if theory is to be believed. So water on the Moon is associated with other gases. Astronomers have agreed for centuries that there is no firm evidence for “weather” on the Moon visible from Earth, and little evidence of thick atmosphere. [2] How would one detect the Moon’s atmosphere from Earth? An obvious means is atmospheric refraction. As you watch the Sun set, its image is displaced by Earth’s atmospheric refraction at the horizon from the position it would have if there were no atmosphere, by roughly 0.6 degree (a bit more than the Sun’s angular diameter). On the Moon, any atmosphere would cause an analogous effect for a star passing behind the Moon during an occultation (multiplied by two since the light travels both into and out of the lunar atmosphere). -
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 -
The Hatfield SCT Lunar Atlas
Jeremy Cook The Hatfield SCT Lunar Atlas Photographic Atlas for Meade, Celestron and Other SCT Telescopes With 216 Figures Jeremy Cook, BSc (Eng) British Library Cataloguing in Publication Data The Hatfield SCT lunar atlas:photographic atlas for Meade, Celestron and other SCT telescopes 1. Moon–Maps I. Cook, Jeremy, 1933–2003 523.3′0223 ISBN 1852337494 Library of Congress Cataloging-in-Publication Data Cook, Jeremy, 1933– The Hatfield SCT lunar atlas:photographic atlas for Meade, Celestron and other SCT telescopes / Jeremy Cook. p. cm. Rev. ed. of: Amateur astronomer’s photographic lunar atlas / Henry Hatfield. 1968. Includes bibliographical references. ISBN 1-85233-749-4 (hc:alk. paper) 1. Moon—Maps. 2. Moon—Remote-sensing images. 3. Moon—Photographs from space. I. Hatfield, Henry. Amateur astronomer’s photographic lunar atlas. II. Title. G1000.3.C6 2004 523.3′022′3—dc22 Apart from any fair dealing for the purposes of research or private study, or criticism or review, as permitted under the Copyright, Designs and Patents Act 1988, this publication may only be reproduced, stored or transmitted, in any form or by any means, with the prior permission in writing of the publishers, or in the case of reprographic reproduction in accordance with the terms of licences issued by the Copyright Licensing Agency. Enquiries concerning reproduction outside those terms should be sent to the publishers. ISBN 1-85233-749-4 Springer-Verlag London Berlin Heidelberg Springer Science+Business Media springeronline.com © British Astronomical Association 2005 Printed in China The use of registered names, trademarks, etc. in this publication does not imply, even in the absence of a specific statement, that such names are exempt from the relevant laws and regulations and therefore free for general use. -
User Guide to 1:250,000 Scale Lunar Maps
CORE https://ntrs.nasa.gov/search.jsp?R=19750010068Metadata, citation 2020-03-22T22:26:24+00:00Z and similar papers at core.ac.uk Provided by NASA Technical Reports Server USER GUIDE TO 1:250,000 SCALE LUNAR MAPS (NASA-CF-136753) USE? GJIDE TO l:i>,, :LC h75- lu1+3 SCALE LUNAR YAPS (Lumoalcs Feseclrch Ltu., Ottewa (Ontario) .) 24 p KC 53.25 CSCL ,33 'JIACA~S G3/31 11111 DANNY C, KINSLER Lunar Science Instltute 3303 NASA Road $1 Houston, TX 77058 Telephone: 7131488-5200 Cable Address: LUtiSI USER GUIDE TO 1: 250,000 SCALE LUNAR MAPS GENERAL In 1972 the NASA Lunar Programs Office initiated the Apollo Photographic Data Analysis Program. The principal point of this program was a detailed 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 useable 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 designed to present in outline form the neces- sary background informatiox or 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. -
Nabs 2004 Final
CURRENT AND SELECTED BIBLIOGRAPHIES ON BENTHIC BIOLOGY 2004 Published August, 2005 North American Benthological Society 2 FOREWORD “Current and Selected Bibliographies on Benthic Biology” is published annu- ally for the members of the North American Benthological Society, and summarizes titles of articles published during the previous year. Pertinent titles prior to that year are also included if they have not been cited in previous reviews. I wish to thank each of the members of the NABS Literature Review Committee for providing bibliographic information for the 2004 NABS BIBLIOGRAPHY. I would also like to thank Elizabeth Wohlgemuth, INHS Librarian, and library assis- tants Anna FitzSimmons, Jessica Beverly, and Elizabeth Day, for their assistance in putting the 2004 bibliography together. Membership in the North American Benthological Society may be obtained by contacting Ms. Lucinda B. Johnson, Natural Resources Research Institute, Uni- versity of Minnesota, 5013 Miller Trunk Highway, Duluth, MN 55811. Phone: 218/720-4251. email:[email protected]. Dr. Donald W. Webb, Editor NABS Bibliography Illinois Natural History Survey Center for Biodiversity 607 East Peabody Drive Champaign, IL 61820 217/333-6846 e-mail: [email protected] 3 CONTENTS PERIPHYTON: Christine L. Weilhoefer, Environmental Science and Resources, Portland State University, Portland, O97207.................................5 ANNELIDA (Oligochaeta, etc.): Mark J. Wetzel, Center for Biodiversity, Illinois Natural History Survey, 607 East Peabody Drive, Champaign, IL 61820.................................................................................................................6 ANNELIDA (Hirudinea): Donald J. Klemm, Ecosystems Research Branch (MS-642), Ecological Exposure Research Division, National Exposure Re- search Laboratory, Office of Research & Development, U.S. Environmental Protection Agency, 26 W. Martin Luther King Dr., Cincinnati, OH 45268- 0001 and William E.