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Geologic Structure of Shallow Maria
NASA CR. Photo Data Analysis S-221 NASA Contract NAS 9-13196 GEOLOGIC STRUCTURE OF SHALLOW MARIA Rene' A. De Hon, Principal Investigator John A. Waskom, Co-Investigator (NASA-CR-lq7qoo GEOLOGIC STahJCTUnF OF N76-17001 ISBALOW M1BIA-'(Arkansas Uni.v., mHiticelio.) 96 p BC $5.00' CSCL O3B Unclas G3/91, 09970- University of Arkansas at Monticello Monticello, Arkansas December 1975 Photo Data Analysis S-221 NASA Contract NAS 9-13196 GEOLOGIC STRUCTURE OF SHALLOW MARIA Rene' A. De Hon, Principal Investigator I John A. Waskom, Co-Investigator Un-iversity-of Arkansas-:at-.Monticl o Monticello, Arkansas December 1975 ABSTRACT Isopach maps and structural contour maps of the 0 0 eastern mare basins (30 N to 30 OS; 00 to 100 E) are constructed from measurements of partially buried craters. The data, which are sufficiently scattered to yield gross thickness variations, are restricted to shallow maria with less than 1500-2000 m of mare basalts. The average thickness of b-asalt in the irregular maria is between 200 and 400 m. Multiringed mascon basins are filled to various levels. The Serenitatis and Crisium basins have deeply flooded interiors and extensively flooded shelves. Mare basalts in the Nectaris basin fill only the innermost basin, and mare basalts in the Smythii basin occupy a small portion of the basin floor. Sinus Amoris, Mare Spumans, and Mare Undarum are partially filled troughs concentric to large circular basins. The Tranquillitatis and Fecunditatis are composite depressions containing basalts which flood degraded circular basins and adjacent terrain modified by the formation of nearby cir cular basins. -
Mare Domes in Mare Tranquillitatis: Identification, Distribution, Characteristics, and Implications for Their Origin and the Oldest Lunar Volcanism
51st Lunar and Planetary Science Conference (2020) 1798.pdf MARE DOMES IN MARE TRANQUILLITATIS: IDENTIFICATION, DISTRIBUTION, CHARACTERISTICS, AND IMPLICATIONS FOR THEIR ORIGIN AND THE OLDEST LUNAR VOLCANISM. L. Qiao1, J. W. Head2, L. Wilson3 and Z. Ling1, 1Inst. Space Sci., Shandong Univ., Weihai, Shan- dong, 264209, China ([email protected]), 2Dep. Earth, Env. & Planet. Sci., Brown Univ., Providence, RI, 02912, USA, 3Lancaster Env. Centre, Lancaster Univ., Lancaster LA1 4YQ, UK. Introduction: Volcanism is one of the major geo- General Characteristics and Identification Crite- logical process on the Moon, directly reflecting the ria of Mare Domes. A preliminary survey of previous- composition and thermal state of lunar interior and its ly-catalogued mare domes [1-4] reveals some of their evolution, and serves as an important window into the fundamental characteristics. A typical well-developed geological and thermal evolution of the Moon. Mare mare dome is characterized by a domical raised struc- domes, small (<~30 km diameter) and generally circu- ture with a generally convex-shape and low-slope (<5°) lar structures with convex-upward shapes [1], are profile and a (quasi-)circular or elliptical outline. Some among the most common volcanic landforms on the domes have summit pit craters, while many lack them, Moon. Over 300 mare domes have been previously possibly being filled up by the last eruptions. The de- identified, using mainly telescope and orbital photo- velopment of the circular mound shape of mare domes graphs [e.g., 1-4]. -
The Moon After Apollo
ICARUS 25, 495-537 (1975) The Moon after Apollo PAROUK EL-BAZ National Air and Space Museum, Smithsonian Institution, Washington, D.G- 20560 Received September 17, 1974 The Apollo missions have gradually increased our knowledge of the Moon's chemistry, age, and mode of formation of its surface features and materials. Apollo 11 and 12 landings proved that mare materials are volcanic rocks that were derived from deep-seated basaltic melts about 3.7 and 3.2 billion years ago, respec- tively. Later missions provided additional information on lunar mare basalts as well as the older, anorthositic, highland rocks. Data on the chemical make-up of returned samples were extended to larger areas of the Moon by orbiting geo- chemical experiments. These have also mapped inhomogeneities in lunar surface chemistry, including radioactive anomalies on both the near and far sides. Lunar samples and photographs indicate that the moon is a well-preserved museum of ancient impact scars. The crust of the Moon, which was formed about 4.6 billion years ago, was subjected to intensive metamorphism by large impacts. Although bombardment continues to the present day, the rate and size of impact- ing bodies were much greater in the first 0.7 billion years of the Moon's history. The last of the large, circular, multiringed basins occurred about 3.9 billion years ago. These basins, many of which show positive gravity anomalies (mascons), were flooded by volcanic basalts during a period of at least 600 million years. In addition to filling the circular basins, more so on the near side than on the far side, the basalts also covered lowlands and circum-basin troughs. -
The Soviet Space Program
C05500088 TOP eEGRET iuf 3EEA~ NIE 11-1-71 THE SOVIET SPACE PROGRAM Declassified Under Authority of the lnteragency Security Classification Appeals Panel, E.O. 13526, sec. 5.3(b)(3) ISCAP Appeal No. 2011 -003, document 2 Declassification date: November 23, 2020 ifOP GEEAE:r C05500088 1'9P SloGRET CONTENTS Page THE PROBLEM ... 1 SUMMARY OF KEY JUDGMENTS l DISCUSSION 5 I. SOV.IET SPACE ACTIVITY DURING TfIE PAST TWO YEARS . 5 II. POLITICAL AND ECONOMIC FACTORS AFFECTING FUTURE PROSPECTS . 6 A. General ............................................. 6 B. Organization and Management . ............... 6 C. Economics .. .. .. .. .. .. .. .. .. .. .. ...... .. 8 III. SCIENTIFIC AND TECHNICAL FACTORS ... 9 A. General .. .. .. .. .. 9 B. Launch Vehicles . 9 C. High-Energy Propellants .. .. .. .. .. .. .. .. .. 11 D. Manned Spacecraft . 12 E. Life Support Systems . .. .. .. .. .. .. .. .. 15 F. Non-Nuclear Power Sources for Spacecraft . 16 G. Nuclear Power and Propulsion ..... 16 Te>P M:EW TCS 2032-71 IOP SECl<ET" C05500088 TOP SECRGJ:. IOP SECREI Page H. Communications Systems for Space Operations . 16 I. Command and Control for Space Operations . 17 IV. FUTURE PROSPECTS ....................................... 18 A. General ............... ... ···•· ................. ····· ... 18 B. Manned Space Station . 19 C. Planetary Exploration . ........ 19 D. Unmanned Lunar Exploration ..... 21 E. Manned Lunar Landfog ... 21 F. Applied Satellites ......... 22 G. Scientific Satellites ........................................ 24 V. INTERNATIONAL SPACE COOPERATION ............. 24 A. USSR-European Nations .................................... 24 B. USSR-United States 25 ANNEX A. SOVIET SPACE ACTIVITY ANNEX B. SOVIET SPACE LAUNCH VEHICLES ANNEX C. SOVIET CHRONOLOGICAL SPACE LOG FOR THE PERIOD 24 June 1969 Through 27 June 1971 TCS 2032-71 IOP SLClt~ 70P SECRE1- C05500088 TOP SEGR:R THE SOVIET SPACE PROGRAM THE PROBLEM To estimate Soviet capabilities and probable accomplishments in space over the next 5 to 10 years.' SUMMARY OF KEY JUDGMENTS A. -
Analysis of Lava Tubes and Skylights in the Lunar Exploration Context
EPSC Abstracts Vol. 7 EPSC2012-632-1 2012 European Planetary Science Congress 2012 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2012 Analysis of Lava Tubes and Skylights in the Lunar Exploration Context E. Martellato, B. Foing, J. Benkhoff ESA/ESTEC, Keplerlaan 1, 2201 Noordwijk ZH, The Netherlands (corresponding author: [email protected], [email protected]) collapsed sections of roofs ([6]). Skylights could Abstract originate as enlargement of pre-existing fractures, for instance following a moonquake ([8]), or as The past and current scientific activities related to the incompleting crusting over the melted lava flow (e.g., future robotic and human exploration of the Moon [4]), or as collapse of the lava tubes ceiling caused by have stressed the importance of lava tubes as random meteoroids impacts (e.g., [6]). convenient settlements in an inhospitable planet, providing a natural shielding to a variety of natural 2. Observations hazards with minimizing costs of the construction of manned bases. The detection of lava tubes could be In our analysis, we consider two skylights candidates favoured by the presence of skylights, which also detected by the Terrain Camera onboard the Japanese represent a way to access to these underground orbiter SELenological and Engineering Explorer structures. In this context, we analyze one of the (SELENE) ([9], [10]), and then observed at higher proposed mechanism of skylights formation, that is resolution by Lunar Reconnaissance Orbiter Camera random impacts craters, by comparing crater- (LROC) onboard the NASA spacecraft Lunar geometry argumentations ([11]) with numerical Reconnaissance Orbiter (LRO) ([2]). modelling outcomes. A first pit is located on the Marius Hills region 1. -
Geological Evolution of the Largest Shield Volcano Bearing Mare of The
52nd Lunar and Planetary Science Conference 2021 (LPI Contrib. No. 2548) 1827.pdf GEOLOGICAL EVOLUTION OF THE LARGEST SHIELD VOLCANO BEARING MARE OF THE MOON, MARE TRANQUILLITATIS: BASED ON DETAILED MORPHOLOGICAL, MINERALOGICAL, TOPOGRAPHIC STUDIES USING MULTIPLE DATA SETS. Henal Bhatt1, P. Chauhan2, Paras Solanki1, 1M. G. Science Institute, Ahmedabad 380009, India, 2Indian Institute of Remote Sensing, (ISRO), Dehradun, Uttarakhand, India. ([email protected] ) Introduction: In this work, we have analysed the Results and Discussions: Mare Tranquillitatis is irregular shaped Mare Tranquillitatis based on its delineated in to 22 spectral units based on IBD parameter morphology, mineralogy and topography to understand its analysis (Fig. 1). The band parameters analysis was geological evolution in the Lunar formation history. This conducted as per [8], [9], [10] suggest the abundance of area is very unique as it resides the largest shield volcano mafic silicate mixture, particular, mixture of olivine and of the Moon, compared to all the other circular mare basins medium to high calcium pyroxene bearing basaltic material at the near side of the Moon. It is located towards eastern in the area (Fig. 1). Details of this analysis is reported in the near side at 7°N, 30°E and is a Pre-Nectarian age basin [1]. [11]. Graphical trends suggests that basalts of eastern shield It is well known for Apollo 11 landing site and it shows mare would have been comparatively more pyroxene characteristic two basin ring structure [2], with diameter of bearing compared to the basalts from western deepest part, 800 km from east to west. which would have been more olivine bearing compared to the eastern shield mare basalt (Fig. -
To the Moon and Back - Weighing for NASA
To the Moon and Back - Weighing for NASA A small step carrying a lot of weight: The 1969 lunar landing. It sent TV viewer ratings rocketing into the stratosphere and drove innumerable companies and universities to extraordinary accomplishments. The objective: To ensure the success of the Apollo II mission. Mettler Instrument Corporation was one of the companies that supported NASA. This collaboration is still alive and well. "The eagle has landed!" Those are the words Neil Alden Armstrong transmitted back to the space administration on July 20, 1969. Shortly before, he planted the Eagle lunar module in the Mare Tranquillitatis, the "Sea of Tranquility". A long journey for the astronauts of the Apollo II mission - the average distance from the Earth to the moon is about sixty-times around the world, or about 384,401 kilometers. Mission commander Armstrong and Edwin "Buzz" Aldrin move about like feather weights on the powdery surface of earth's orbiter. Instead of the 360 pounds on Earth, their suits weigh only 60 pounds because of Moon's gravity, which is only one-sixth that of the Earth. Space exploration and Apollo mission Meanwhile, Michael Collins, the third Apollo II astronaut, orbits the moon in the space ship and shoots the pictures that on the next day are circulating around the world: They show the Eagle lunar module on its return voyage from the lunar surface to the mother ship. Around 400,000 people and 20,000 companies and universities worldwide supported the Apollo program at its height. Among them was Mettler Instrument Corporation of Greifensee near Zurich. -
Apollo Over the Moon: a View from Orbit (Nasa Sp-362)
chl APOLLO OVER THE MOON: A VIEW FROM ORBIT (NASA SP-362) Chapter 1 - Introduction Harold Masursky, Farouk El-Baz, Frederick J. Doyle, and Leon J. Kosofsky [For a high resolution picture- click here] Objectives [1] Photography of the lunar surface was considered an important goal of the Apollo program by the National Aeronautics and Space Administration. The important objectives of Apollo photography were (1) to gather data pertaining to the topography and specific landmarks along the approach paths to the early Apollo landing sites; (2) to obtain high-resolution photographs of the landing sites and surrounding areas to plan lunar surface exploration, and to provide a basis for extrapolating the concentrated observations at the landing sites to nearby areas; and (3) to obtain photographs suitable for regional studies of the lunar geologic environment and the processes that act upon it. Through study of the photographs and all other arrays of information gathered by the Apollo and earlier lunar programs, we may develop an understanding of the evolution of the lunar crust. In this introductory chapter we describe how the Apollo photographic systems were selected and used; how the photographic mission plans were formulated and conducted; how part of the great mass of data is being analyzed and published; and, finally, we describe some of the scientific results. Historically most lunar atlases have used photointerpretive techniques to discuss the possible origins of the Moon's crust and its surface features. The ideas presented in this volume also rely on photointerpretation. However, many ideas are substantiated or expanded by information obtained from the huge arrays of supporting data gathered by Earth-based and orbital sensors, from experiments deployed on the lunar surface, and from studies made of the returned samples. -
Glossary of Lunar Terminology
Glossary of Lunar Terminology albedo A measure of the reflectivity of the Moon's gabbro A coarse crystalline rock, often found in the visible surface. The Moon's albedo averages 0.07, which lunar highlands, containing plagioclase and pyroxene. means that its surface reflects, on average, 7% of the Anorthositic gabbros contain 65-78% calcium feldspar. light falling on it. gardening The process by which the Moon's surface is anorthosite A coarse-grained rock, largely composed of mixed with deeper layers, mainly as a result of meteor calcium feldspar, common on the Moon. itic bombardment. basalt A type of fine-grained volcanic rock containing ghost crater (ruined crater) The faint outline that remains the minerals pyroxene and plagioclase (calcium of a lunar crater that has been largely erased by some feldspar). Mare basalts are rich in iron and titanium, later action, usually lava flooding. while highland basalts are high in aluminum. glacis A gently sloping bank; an old term for the outer breccia A rock composed of a matrix oflarger, angular slope of a crater's walls. stony fragments and a finer, binding component. graben A sunken area between faults. caldera A type of volcanic crater formed primarily by a highlands The Moon's lighter-colored regions, which sinking of its floor rather than by the ejection of lava. are higher than their surroundings and thus not central peak A mountainous landform at or near the covered by dark lavas. Most highland features are the center of certain lunar craters, possibly formed by an rims or central peaks of impact sites. -
The Soviet Moon Program
The Moon Race [July 1969] – down to the wire! JAMES OBERG JULY 17, 2019 SPACE CENTER HOUSTON APOLLO-11 FIFTIETH ANNIVERSARY WWW.JAMESOBERG.COM [email protected] OVERVIEW– JULY 1969 Unexpected last-minute drama was added to Apollo-11 by the appearance of a robot Soviet moon probe that might have returned lunar samples to Earth just before the astronauts got back. We now know that even more dramatic Soviet moon race efforts were ALSO aimed at upstaging Apollo, hoping it would fail. But it was the Soviet program that failed -- and they did their best to keep it secret. These Soviet efforts underscored their desperation to nullify the worldwide significance of Apollo-11 and its profound positive impact, as JFK had anticipated, on international assessments of the relative US/USSR balance of power across the board -- military, commercial, cultural, technological, economic, ideological, and scientific. These were the biggest stakes in the entire Cold War, whose final outcome hung in the balance depending on the outcome of the July 1969 events in space. On July 13, 1969, three days before Apollo-11, the USSR launched a robot probe to upstage it DAY BEFORE APOLLO-11 LANDING – BOTH SPACECRAFT ORBITING MOON IN CRISS-CROSS ORBITS THE SOVIET PROBE GOT TO THE MOON FIRST & WENT INTO ORBIT AROUND IT AS APOLLO BEGAN ITS MISSION https://i.ebayimg.com/images/g/T6UAAOSwDJ9crVLo/s-l1600.jpg https://youtu.be/o16I8S3MMo4 A FEW YEARS LATER, ONCE A NEW MISSION HAD SUCCEEDED, MOSCOW RELEASED DRAWINGS OF THE VEHICLE AND HOW IT OPERATED TO LAND, RETRIEVE SAMPLES, AND RETURN TO EARTH Jodrell Bank radio telescope in Britain told the world about the final phase of the Luna 15 drama, in a news release: "Signals ceased at 4.50 p.m. -
Deep Space Chronicle Deep Space Chronicle: a Chronology of Deep Space and Planetary Probes, 1958–2000 | Asifa
dsc_cover (Converted)-1 8/6/02 10:33 AM Page 1 Deep Space Chronicle Deep Space Chronicle: A Chronology ofDeep Space and Planetary Probes, 1958–2000 |Asif A.Siddiqi National Aeronautics and Space Administration NASA SP-2002-4524 A Chronology of Deep Space and Planetary Probes 1958–2000 Asif A. Siddiqi NASA SP-2002-4524 Monographs in Aerospace History Number 24 dsc_cover (Converted)-1 8/6/02 10:33 AM Page 2 Cover photo: A montage of planetary images taken by Mariner 10, the Mars Global Surveyor Orbiter, Voyager 1, and Voyager 2, all managed by the Jet Propulsion Laboratory in Pasadena, California. Included (from top to bottom) are images of Mercury, Venus, Earth (and Moon), Mars, Jupiter, Saturn, Uranus, and Neptune. The inner planets (Mercury, Venus, Earth and its Moon, and Mars) and the outer planets (Jupiter, Saturn, Uranus, and Neptune) are roughly to scale to each other. NASA SP-2002-4524 Deep Space Chronicle A Chronology of Deep Space and Planetary Probes 1958–2000 ASIF A. SIDDIQI Monographs in Aerospace History Number 24 June 2002 National Aeronautics and Space Administration Office of External Relations NASA History Office Washington, DC 20546-0001 Library of Congress Cataloging-in-Publication Data Siddiqi, Asif A., 1966 Deep space chronicle: a chronology of deep space and planetary probes, 1958-2000 / by Asif A. Siddiqi. p.cm. – (Monographs in aerospace history; no. 24) (NASA SP; 2002-4524) Includes bibliographical references and index. 1. Space flight—History—20th century. I. Title. II. Series. III. NASA SP; 4524 TL 790.S53 2002 629.4’1’0904—dc21 2001044012 Table of Contents Foreword by Roger D. -
NASA Symbols and Flags in the US Manned Space Program
SEPTEMBER-DECEMBER 2007 #230 THE FLAG BULLETIN THE INTERNATIONAL JOURNAL OF VEXILLOLOGY www.flagresearchcenter.com 225 [email protected] THE FLAG BULLETIN THE INTERNATIONAL JOURNAL OF VEXILLOLOGY September-December 2007 No. 230 Volume XLVI, Nos. 5-6 FLAGS IN SPACE: NASA SYMBOLS AND FLAGS IN THE U.S. MANNED SPACE PROGRAM Anne M. Platoff 143-221 COVER PICTURES 222 INDEX 223-224 The Flag Bulletin is officially recognized by the International Federation of Vexillological Associations for the publication of scholarly articles relating to vexillology Art layout for this issue by Terri Malgieri Funding for addition of color pages and binding of this combined issue was provided by the University of California, Santa Barbara Library and by the University of California Research Grants for Librarians Program. The Flag Bulletin at the time of publication was behind schedule and therefore the references in the article to dates after December 2007 reflect events that occurred after that date but before the publication of this issue in 2010. © Copyright 2007 by the Flag Research Center; all rights reserved. Postmaster: Send address changes to THE FLAG BULLETIN, 3 Edgehill Rd., Winchester, Mass. 01890 U.S.A. THE FLAG BULLETIN (ISSN 0015-3370) is published bimonthly; the annual subscription rate is $68.00. Periodicals postage paid at Winchester. www.flagresearchcenter.com www.flagresearchcenter.com 141 [email protected] ANNE M. PLATOFF (Annie) is a librarian at the University of Cali- fornia, Santa Barbara Library. From 1989-1996 she was a contrac- tor employee at NASA’s Johnson Space Center. During this time she worked as an Information Specialist for the New Initiatives Of- fice and the Exploration Programs Office, and later as a Policy Ana- lyst for the Public Affairs Office.