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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. -
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 -
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. -
The Disintegration of the Wolf Creek Meteorite and the Formation of Pecoraite, the Nickel Analog of Clinochrysotile
The Disintegration of the Wolf Creek Meteorite and the Formation of Pecoraite, the Nickel Analog of Clinochrysotile GEOLOGICAL SURVEY PROFESSIONAL PAPER 384-C 1 mm ^^ 5 -fc;- Jj. -f->^ -J^' ' _." ^P^-Arvx^B^ »""*- 'S y^'ir'*'*'/?' trK* ^-7 A5*^v;'VvVr*'^**s! ^^^^V'^"^"''"X^^i^^?l^"%^ - ! ^ Pecoraite, Wolf Creek meteorite of Australia. Upper, Pecoraite grains separated by hand picking from crack fillings in the meteorite (X 25). Lower, Pecoraite grains lining the walls of some cracks in the meteorite. The extent of disintegration of the original metal lic phases into new phases, chiefly goethite and maghemite, is apparent (X 2.3). THE DISINTEGRATION OF THE WOLF CREEK METEORITE AND THE FORMATION OF PECORAITE, THE NICKEL ANALOG OF CLINOCHRYSOTILE The Disintegration of the Wolf Creek Meteorite and the Formation of Pecoraite, the Nickel Analog of Clinochrysotile By GEORGE T. FAUST, JOSEPH J. FAHEY, BRIAN H. MASON and EDWARD J. DWORNIK STUDIES OF THE NATURAL PHASES IN THE SYSTEM MgO-SiO2 -H2O AND THE SYSTEMS CONTAINING THE CONGENERS OF MAGNESIUM GEOLOGICAL SURVEY PROFESSIONAL PAPER 384-C Origin of pecoraite elucidated through its properties and in terms of the geochemical balance in its desert environment UNITED STATES GOVERNMENT PRINTING OFFICE, WASHINGTON : 1973 UNITED STATES DEPARTMENT OF THE INTERIOR ROGERS C. B. MORTON, Secretary GEOLOGICAL SURVEY V. E. McKelvey, Director Library of Congress catalog-card No. 73-600160 For sale by the Superintendent of Documents, U.S. Government Printing Office Washington, D.C. 20402 - Price $1.30 Stock -
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John D. Dingell, Jr. Conservation, Management, and Recreation Act’’
S. 47 One Hundred Sixteenth Congress of the United States of America AT THE FIRST SESSION Begun and held at the City of Washington on Thursday, the third day of January, two thousand and nineteen An Act To provide for the management of the natural resources of the United States, and for other purposes. Be it enacted by the Senate and House of Representatives of the United States of America in Congress assembled, SECTION 1. SHORT TITLE; TABLE OF CONTENTS. (a) SHORT TITLE.—This Act may be cited as the ‘‘John D. Dingell, Jr. Conservation, Management, and Recreation Act’’. (b) TABLE OF CONTENTS.—The table of contents for this Act is as follows: Sec. 1. Short title; table of contents. Sec. 2. Definition of Secretary. TITLE I—PUBLIC LAND AND FORESTS Subtitle A—Land Exchanges and Conveyances Sec. 1001. Crags land exchange, Colorado. Sec. 1002. Arapaho National Forest boundary adjustment. Sec. 1003. Santa Ana River Wash Plan land exchange. Sec. 1004. Udall Park land exchange. Sec. 1005. Confirmation of State land grants. Sec. 1006. Custer County Airport conveyance. Sec. 1007. Pascua Yaqui Tribe land conveyance. Sec. 1008. La Paz County land conveyance. Sec. 1009. Lake Bistineau land title stability. Sec. 1010. Lake Fannin land conveyance. Sec. 1011. Land conveyance and utility right-of-way, Henry’s Lake Wilderness Study Area, Idaho. Sec. 1012. Conveyance to Ukpeagvik Inupiat Corporation. Sec. 1013. Public purpose conveyance to City of Hyde Park, Utah. Sec. 1014. Juab County conveyance. Sec. 1015. Black Mountain Range and Bullhead City land exchange. Sec. 1016. Cottonwood land exchange. Sec. -
01 Edmunson Simulant
SECTION 1: LUNAR HISTORY Dr. Jennifer Edmunson 1.1 Introduction Why understanding events in lunar history is important for engineers and simulant users: • It explains the motivation for exploration of the Moon. o To understand the evolution of our own planet. • It explains the origin of the operating environment for spacecraft, and ultimately influences the spacecraft design. • It describes human and spacecraft hazards. o Morphology of the landing site. o Micrometeorite bombardment. o Lunar regolith (boulders, dust). • It influences landing site locations. o Areas in permanent sunlight and shadow. o Regions of interest to scientists. • It provides the basis for predicting the chemical composition and physical properties of the lunar surface at specific sites. • It explains the impact history of the moon, which has changed the surface into its present form (creating the regolith). • It describes the processes that created the size distribution of regolith components, as well as their chemistry. 1.2 Initial Impact The Earth and Moon have similar chemistries and share the same oxygen isotope signature. This oxygen isotope signature is different from other planets and asteroids. Because of this, the Earth and Moon must have formed at the same distance from the Sun, or from a single chemical reservoir. The “Giant Impact” theory of lunar origin involves the proto-Earth being struck by a Mars-sized impactor (called Theia). Scientists favor this theory because it explains not only the similarities in composition (and the identical oxygen isotope signature) and the known mass of both the Earth and Moon, but the angular momentum of the Earth-Moon system. -
Zootaxa, Revision of the Australo-Papuan Genus
Zootaxa 2486: 1–60 (2010) ISSN 1175-5326 (print edition) www.mapress.com/zootaxa/ Monograph ZOOTAXA Copyright © 2010 · Magnolia Press ISSN 1175-5334 (online edition) ZOOTAXA 2486 Revision of the Australo-Papuan genus Macrolema Baly (Coleoptera: Chrysomelidae: Spilopyrinae), with description of a new genus C. A. M. REID & M. BEATSON Department of Entomology, Australian Museum, 6 College Street, Sydney, NSW 2010, Australia. Email: [email protected]; [email protected] Magnolia Press Auckland, New Zealand Accepted by G. Morse: 16 Apr. 2010; published: 27 May 2010 C. A. M. REID & M. BEATSON Revision of the Australo-Papuan genus Macrolema Baly (Coleoptera: Chrysomelidae: Spilopyrinae), with description of a new genus (Zootaxa 2486) 60 pp.; 30 cm. 27 May 2010 ISBN 978-1-86977-543-8 (paperback) ISBN 978-1-86977-544-5 (Online edition) FIRST PUBLISHED IN 2010 BY Magnolia Press P.O. Box 41-383 Auckland 1346 New Zealand e-mail: [email protected] http://www.mapress.com/zootaxa/ © 2010 Magnolia Press All rights reserved. No part of this publication may be reproduced, stored, transmitted or disseminated, in any form, or by any means, without prior written permission from the publisher, to whom all requests to reproduce copyright material should be directed in writing. This authorization does not extend to any other kind of copying, by any means, in any form, and for any purpose other than private research use. ISSN 1175-5326 (Print edition) ISSN 1175-5334 (Online edition) 2 · Zootaxa 2486 © 2010 Magnolia Press REID & BEATSON Table of contents Introduction . 3 Methods. 4 Allsortsia gen. -
Vol. 23, No. the ORE.-BIN January 1961 STATE of OREGON Portland
THE ORE BIN Volume 23, 1961 Vol. 23, No. THE ORE.-BIN January 1961 STATE OF OREGON Portland, Oregon DEPARTMENT OF GEOLOGY AND MINERAL INDUSTRIES Head Office: 1069 State Office Bldg., Portland 1, Oregon Telephone: CApitol 6-2161, Ext. 488 State Governing Board Hollis M. Dole, Director William Kennedy, Chairman, Portland Harold Banta Baker Stoff Earl S. Mollard Riddle R. G. Bowen Geologist Field Offices R. E. Corcoran Geologist 2033 First Street, Boker L. L. Hoogland Assayer and Chemist N. S. Wagner, Field Geologist Rolph S. Mason Mining Engineer H. C. Brooks, Field Geologist T. C. Matthews Spectroscopist 239 S. E. "H" Street, Grants Pass V. C. Newton, Jr. Petroleum Engineer Len Ramp, Field Geologist H. G. Schlicker Geologist Norman Peterson, Field Geologist M. L. Steere Geologist * * * * * * * * * * * * * * * * * * OREGON MINERAL PRODUCTION IN 1960 By Ralph S. Mason* Oregon's mineral industry produced its second highest value of row minerals in 1960. Following a nation-wide economic trend during the year, the industry was off approximately $3 million from lost year's record-breaking high of $49.8 million, according to preliminary estimates mode by the U. S. Bureau of Mines. The heavy construction commodities, crushed stone and sand and grovel, reflected construction log and were responsible for most of the change from lost year. Metal mining, aside from nickel, was quiet. The state's only uronium mine and one of the two mercury producers shut down. Industrial mineral products showed both gains and losses as compared to the previous year. Cement production was up 12 percent while clays declined 15 percent and diatomite 3 percent. -
DNA1.94Og27.Ool G
DNA1.94Og27.Ool g No. Pub. Year Citations File Name File Size (bytes) 5 1967-1968 857 RADBIB05.TXT 791,604 The search criteria was for radiation or radiological for publication year greater than 1966 and less than 1969. The document database four character field names and a descriptor for each. field are as follows: ABS Abstract ACCD Accession Date ADNO DTIC Number ---*->*h I AUTH Author (s) CCDE Computer Code ( s ) CLSS Classification CONN Contract Number CORP Corporation DATE Report Date DESC Descriptor (s) EFFT Damage Mechanism EMPF Electro Magnetic Pulse File number(s) HESO High Explosive Shot(s) INUM Item Number LA Country or Language PROJ Project Number REPN Report Number SHOT Nuclear Test (s) SUCE Device Designation SUJO DASIAC Subject number(s) SYMJ Published in SYST System Affected TEMP Document Control number(s) TITL Report Title TNFF Tactical Nuclear Warfare TREE Transient Radiation Effects on Electronics number(s) TSHO Shot. Type Statement A Approved for public release;* Distribution unlirnited.ZMi-d=- .folddata Report Log for Bibliography Report 'bibliography' scheduled as 'radbib' Bibliography using full text searching with selection qualification. STILAS text selection v6.2 started on Monday, June 13, 1994, 10:45 AM Search will use the KUNI database Search strings will be read from standard input The catalog key will be written to standard output 19940613104505 BRS/Search-Engine v.5 started for seltextl 11379 records found for #1: RADIATION OR RADIOLOGICAL 1 searches considered 1 searches selected. STILAS text selection finished on Monday, June 13, 1994, 10:49 AM STILAS catalog selection v6.2 started on Monday, June 13, 1994, 10:45 Ah4 Catalog key will be read from standard input The catalog key will be written to standard output The author key will be written to standard output The title key will be written to standard output Catalog will be selected if year-ofjub is more than 1968 and less than 1971 11379 catalog record(s) considered 893 catalog record(s) selected. -
Air-Sea Interactions on Titan: Lake Evaporation, Atmospheric Circulation, and Cloud Formation
Air-Sea Interactions on Titan: Lake Evaporation, Atmospheric Circulation, and Cloud Formation Scot C. R. Rafkin* and Alejandro Soto Department of Space Studies, Southwest Research Institute, 1050 Walnut Street, Suite 300, Boulder, CO, USA, [email protected]. *Corresponding Author Keywords: Titan, Titan Seas, Titan Lakes, Titan Atmosphere, Air-Sea Interaction, Sea breeze, Titan Clouds Abstract Titan’s abundant lakes and seas exchange methane vapor and energy with the atmosphere via a process generally known as air-sea interaction. This turbulent exchange process is investigated with an atmospheric mesoscale model coupled to a slab model representation of an underlying lake. The impact of lake size, effective lake mixed layer depth, background wind speed, air-lake temperature differential, and atmospheric humidity on air-sea interaction processes is studied through dozens of two-dimensional simulations. The general, quasi-steady solution is a non-linear superposition of a very weak background plume circulation driven by the buoyancy of evaporated methane with a stronger opposing thermally direct (sea breeze) circulation driven by the thermal contrast between the cold marine layer over the lake and the warmer inland air. The specific solution depends on the value of selected atmosphere and lake property parameters, but the general solution of the superposition of these two circulations is persistent. Consistent with previous analytical work of others, the sensible heat flux and the latent heat flux trend toward opposite and equal values such that their ratio, the Bowen ratio, approaches -1.0 in most, but not all, of the quasi-steady state solutions. Importantly, in nearly all scenarios, the absolute magnitude of the 1 fluxes trends toward very small values such that the equilibrium solution is also nearly a trivial solution where air-sea energy exchange is ~3 W m-2 or less. -
The Scientific Context for Exploration of the Moon
Committee on the Scientific Context for Exploration of the Moon Space Studies Board Division on Engineering and Physical Sciences THE NATIONAL ACADEMIES PRESS 500 Fifth Street, N.W. Washington, DC 20001 NOTICE: The project that is the subject of this report was approved by the Governing Board of the National Research Council, whose members are drawn from the councils of the National Academy of Sciences, the National Academy of Engineering, and the Institute of Medicine. The members of the committee responsible for the report were chosen for their special competences and with regard for appropriate balance. This study is based on work supported by the Contract NASW-010001 between the National Academy of Sciences and the National Aeronautics and Space Administration. Any opinions, findings, conclusions, or recommendations expressed in this publication are those of the author(s) and do not necessarily reflect the views of the agency that provided support for the project. International Standard Book Number-13: 978-0-309-10919-2 International Standard Book Number-10: 0-309-10919-1 Cover: Design by Penny E. Margolskee. All images courtesy of the National Aeronautics and Space Administration. Copies of this report are available free of charge from: Space Studies Board National Research Council 500 Fifth Street, N.W. Washington, DC 20001 Additional copies of this report are available from the National Academies Press, 500 Fifth Street, N.W., Lockbox 285, Washington, DC 20055; (800) 624-6242 or (202) 334-3313 (in the Washington metropolitan area); Internet, http://www.nap. edu. Copyright 2007 by the National Academy of Sciences. All rights reserved.