Chapter 11: Afterword
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THE AVALANCHE DEPOSITS in LUNAR CRATER REINER. V.V.Shevchenko1,2, P.C.Pinet1, S.Chevrel1, Y.Daydou1, T.P.Skobeleva2, O.I.Kvaratskhelia3, C.Rosemberg1
Lunar and Planetary Science XXXVIII (2007) 1066.pdf THE AVALANCHE DEPOSITS IN LUNAR CRATER REINER. V.V.Shevchenko1,2, P.C.Pinet1, S.Chevrel1, Y.Daydou1, T.P.Skobeleva2, O.I.Kvaratskhelia3, C.Rosemberg1. 1UMR 5562 “Dynamique Terrestre et Planet- aire”/CNRS/UPS, Observatoire Midi-Pyrenees, Toulouse, 31400 France; 2Sternberg Astronomical Institute, Mos- cow University, Moscow, 119992, Russia, 3Abastumany Astrophysical Observatory, Georgian Academy of Sci- ences, Georgia. [email protected] Introduction: Space weathering processes on the Fig. 3 represents the Clementine image of the cra- Moon affect the optical properties of an exposed lunar ter Reiner. soil. The main spectral/optical effects of space weath- ering are a reduction of reflectance, attenuation of the 1-μm ferrous absorption band, and a red-sloped con- tinuum creation [1]. Lucey et al. [2 - 4] proposed to estimate the maturity of lunar soils from Clementine UVVIS data using a method which decorrelates the effects of variations in Fe2+ concentration from the effects of soil maturity. The method calculates optical maturity defined as parameter OMAT [5]. Pinet et al. [6] used the method to analyse the ‘Reiner-γ – Reiner’ region on the basis of Clementine spectral image data. Crater Reiner: Crater Reiner is located in western Oceanus Procellarum. Diameter of the crater is 30 km, its depth is 2.4 km and its central peak height is about 700 m (Fig. 1). Fig.3 Evidence of avalanching and of other downslope movement of material is clearly visible on the inner walls of the crater. In general, freshly exposed lunar material is brighter than undisturbed materials nearby. -
No. 40. the System of Lunar Craters, Quadrant Ii Alice P
NO. 40. THE SYSTEM OF LUNAR CRATERS, QUADRANT II by D. W. G. ARTHUR, ALICE P. AGNIERAY, RUTH A. HORVATH ,tl l C.A. WOOD AND C. R. CHAPMAN \_9 (_ /_) March 14, 1964 ABSTRACT The designation, diameter, position, central-peak information, and state of completeness arc listed for each discernible crater in the second lunar quadrant with a diameter exceeding 3.5 km. The catalog contains more than 2,000 items and is illustrated by a map in 11 sections. his Communication is the second part of The However, since we also have suppressed many Greek System of Lunar Craters, which is a catalog in letters used by these authorities, there was need for four parts of all craters recognizable with reasonable some care in the incorporation of new letters to certainty on photographs and having diameters avoid confusion. Accordingly, the Greek letters greater than 3.5 kilometers. Thus it is a continua- added by us are always different from those that tion of Comm. LPL No. 30 of September 1963. The have been suppressed. Observers who wish may use format is the same except for some minor changes the omitted symbols of Blagg and Miiller without to improve clarity and legibility. The information in fear of ambiguity. the text of Comm. LPL No. 30 therefore applies to The photographic coverage of the second quad- this Communication also. rant is by no means uniform in quality, and certain Some of the minor changes mentioned above phases are not well represented. Thus for small cra- have been introduced because of the particular ters in certain longitudes there are no good determi- nature of the second lunar quadrant, most of which nations of the diameters, and our values are little is covered by the dark areas Mare Imbrium and better than rough estimates. -
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. -
EXPLORING the MOON in the 21St CENTURY
CosmoELEMENTS EXPLORING THE MOON IN THE 21st CENTURY Samuel J. Lawrence1 and Clive R. Neal2 DOI: 10.2138/gselements.15.5.360 INTRODUCTION In 2019, we are celebrating the 50th anniversary of NASA’s momentous Apollo expedi- tions to the Moon. The samples brought back by the astronauts, and the fieldwork those astro- The South Pole of the Moon, pictured here in an oblique view from FIGURE 1 NASA’s Lunar Reconnaissance Orbiter, is the landing site for the nauts performed on the lunar surface, cemented the Moon’s status as seventh human lunar landing. IMAGE COURTESY OF NAC M1195011983LR (NASA/ the cornerstone of the solar system. It is not an exaggeration to say GSFC/ARIZONA STATE UniVERSITY). that the Apollo expeditions transformed our understanding of our solar system, and, in fact, most of the discoveries made in planetary science since the 1960s can trace directly, or indirectly, from the scientific of the Sun’s evolution and history. Finally, this is another area where results of those Apollo expeditions. the Apollo expeditions represent a strength: there are five decades worth of planetary science hypotheses that lunar geological fieldwork Although some erroneously proclaim that the Moon is “Been there, will address. The lunar surface could also provide a unique and stable done that”, nothing could be further from the truth. After a long long-term platform for astronomy. In particular, manned radio obser- st hiatus, beginning in the first years of the 21 century, there has vatories or optical interferometers on the far side of the Moon could been a resurgence of interest in the Moon, including the Kaguya produce dramatic advances in astrophysics. -
Datos De Coyuntura Del 9 Al 15 De Julio De 2019 9 De Julio
Datos de coyuntura del 9 al 15 de julio de 2019 9 de julio de 2019 1. ¿Por qué contratar un seguro contra robos para tu casa? Fuente, El Financiero, encuesta Inegi. https://www.elfinanciero.com.mx/inmobiliario/por-que-contratar-un-seguro- contra-robos-para-tu-casa 2. Se desploma AMLO en encuesta. Fuente, El Financiero, encuesta México Elige. https://www.elfinanciero.com.mx/opinion/alejo-sanchez-cano/se-desploma-amlo-en- encuesta 3. Sube 5.4% la visita a México por turistas internacionales. Fuente, Excélsior, encuesta Inegi. https://www.excelsior.com.mx/nacional/sube-54-la-visita-a-mexico-por-turistas- internacionales/1323401 10 de julio de 2019 4. Trump Seen Marginally as Decisive Leader, but Not Honest. Fuente, Gallup, encuesta Gallup. https://news.gallup.com/poll/260495/trump-seen-marginally-decisive-leader-not- honest.aspx?g_source=link_NEWSV9&g_medium=NEWSFEED&g_campaign=item_&g_con tent=Trump%2520Seen%2520Marginally%2520as%2520Decisive%2520Leader%2c%2520b ut%2520Not%2520Honest 11 de julio de 2019 5. Aumenta esperanza de vida en San Luis Potosí. Fuente, El Financiero, encuesta Coespo. https://www.elfinanciero.com.mx/bajio/aumenta-esperanza-de-vida-en-san-luis-potosi 6. Megan Rapinoe está arriba de Trump en encuesta electora. Fuente, Excélsior, encuesta Public Policy Polling. https://www.excelsior.com.mx/global/megan-rapinoe-esta-arriba- de-trump-en-encuesta-electora/1324075 7. ¿Cuántos y cómo somos los mexicanos? Fuente, Excélsior, encuesta Inegi. https://www.dineroenimagen.com/economia/cuantos-y-como-somos-los- mexicanos/111930 8. Cuánto dinero deben darles los padres a sus hijos. Fuente, El Universal, encuesta T. -
Apollo 12 Photography Index
%uem%xed_ uo!:q.oe_ s1:s._l"e,d_e_em'I flxos'p_zedns O_q _/ " uo,re_ "O X_ pea-eden{ Z 0 (D I I 696L R_K_D._(I _ m,_ -4 0", _z 0', l',,o ._ rT1 0 X mm9t _ m_o& ]G[GNI XHdV_OOZOHd Z L 0T'I0_V 0 0 11_IdVdONI_OM T_OINHDZZ L6L_-6 GYM J_OV}KJ_IO0VSVN 0 C O_i_lOd-VJD_IfO1_d 0 _ •'_ i wO _U -4 -_" _ 0 _4 _O-69-gM& "oN GSVH/O_q / .-, Z9946T-_D-VSVN FOREWORD This working paper presents the screening results of Apollo 12, 70mmand 16mmphotography. Photographic frame descriptions, along with ground coverage footprints of the Apollo 12 Mission are inaluded within, by Appendix. This report was prepared by Lockheed Electronics Company,Houston Aerospace Systems Division, under Contract NAS9-5191 in response to Job Order 62-094 Action Document094.24-10, "Apollo 12 Screening IndeX', issued by the Mapping Sciences Laboratory, MannedSpacecraft Center, Houston, Texas. Acknowledgement is made to those membersof the Mapping Sciences Department, Image Analysis Section, who contributed to the results of this documentation. Messrs. H. Almond, G. Baron, F. Beatty, W. Daley, J. Disler, C. Dole, I. Duggan, D. Hixon, T. Johnson, A. Kryszewski, R. Pinter, F. Solomon, and S. Topiwalla. Acknowledgementis also made to R. Kassey and E. Mager of Raytheon Antometric Company ! I ii TABLE OF CONTENTS Section Forward ii I. Introduction I II. Procedures 1 III. Discussion 2 IV. Conclusions 3 V. Recommendations 3 VI. Appendix - Magazine Summary and Index 70mm Magazine Q II II R ii It S II II T II I! U II t! V tl It .X ,, ,, y II tl Z I! If EE S0-158 Experiment AA, BB, CC, & DD 16mm Magazines A through P VII. -
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 Choice of the Location of the Lunar Base N93-17431
155 PRECEDING PhGE ,,=,_,,c,;_''_'" t¢OT F|Lf_D THE CHOICE OF THE LOCATION OF THE LUNAR BASE N93-17431 V. V. Y__hevchenko P.. K _ AsO_nomtca/In./lute Moscow U_ Moscow 119899 USSR The development of modern methods of remote sensing of the lunar suuface and data from lunar studies by space vehicles make it possgale to assess scientifically the e:qOediowy of the locationof the lunar base in a definite region on the Moon. The prefimlnary choice of the site is important for tackling a range of problems assocfated with ensuring the activity of a manned lunar base and with fulfilh'ng the research program. Based on astronomical dat_ we suggest the Moon's western _, specifically the western part of Oceanus Proceliarurtg where natural scientifically interesting objects have been identifle_ as have surface rocks with enlaanced contents of ilmenite, a poss_le source of oxygen. A comprehensive et_tluation of the region shows timt, as far as natural features are concernetg it is a key one for solving the main problems of the Moon's orlgln and evolution. INTRODUCTION final period of shaping the lunar crust's upper horizons (this period coincided with the final equalization of the Moon's periods The main criteria for choosing a site for the first section of a of orbital revolution and axial rotation), the impact of terrestrial manned lunar base are (1)the most favorable conditions for gravitation on the internal structure of the Moon increased. transport operations, (2)the presence of natural objects of Between 4 and 3 b.y. -
Issue #1 – 2012 October
TTSIQ #1 page 1 OCTOBER 2012 Introducing a new free quarterly newsletter for space-interested and space-enthused people around the globe This free publication is especially dedicated to students and teachers interested in space NEWS SECTION pp. 3-22 p. 3 Earth Orbit and Mission to Planet Earth - 13 reports p. 8 Cislunar Space and the Moon - 5 reports p. 11 Mars and the Asteroids - 5 reports p. 15 Other Planets and Moons - 2 reports p. 17 Starbound - 4 reports, 1 article ---------------------------------------------------------------------------------------------------- ARTICLES, ESSAYS & MORE pp. 23-45 - 10 articles & essays (full list on last page) ---------------------------------------------------------------------------------------------------- STUDENTS & TEACHERS pp. 46-56 - 9 articles & essays (full list on last page) L: Remote sensing of Aerosol Optical Depth over India R: Curiosity finds rocks shaped by running water on Mars! L: China hopes to put lander on the Moon in 2013 R: First Square Kilometer Array telescopes online in Australia! 1 TTSIQ #1 page 2 OCTOBER 2012 TTSIQ Sponsor Organizations 1. About The National Space Society - http://www.nss.org/ The National Space Society was formed in March, 1987 by the merger of the former L5 Society and National Space institute. NSS has an extensive chapter network in the United States and a number of international chapters in Europe, Asia, and Australia. NSS hosts the annual International Space Development Conference in May each year at varying locations. NSS publishes Ad Astra magazine quarterly. NSS actively tries to influence US Space Policy. About The Moon Society - http://www.moonsociety.org The Moon Society was formed in 2000 and seeks to inspire and involve people everywhere in exploration of the Moon with the establishment of civilian settlements, using local resources through private enterprise both to support themselves and to help alleviate Earth's stubborn energy and environmental problems. -
VV D C-A- R 78-03 National Space Science Data Center/ World Data Center a for Rockets and Satellites
VV D C-A- R 78-03 National Space Science Data Center/ World Data Center A For Rockets and Satellites {NASA-TM-79399) LHNAS TRANSI]_INT PHENOMENA N78-301 _7 CATAI_CG (NASA) 109 p HC AO6/MF A01 CSCl 22_ Unc.las G3 5 29842 NSSDC/WDC-A-R&S 78-03 Lunar Transient Phenomena Catalog Winifred Sawtell Cameron July 1978 National Space Science Data Center (NSSDC)/ World Data Center A for Rockets and Satellites (WDC-A-R&S) National Aeronautics and Space Administration Goddard Space Flight Center Greenbelt) Maryland 20771 CONTENTS Page INTRODUCTION ................................................... 1 SOURCES AND REFERENCES ......................................... 7 APPENDIX REFERENCES ............................................ 9 LUNAR TRANSIENT PHENOMENA .. .................................... 21 iii INTRODUCTION This catalog, which has been in preparation for publishing for many years is being offered as a preliminary one. It was intended to be automated and printed out but this form was going to be delayed for a year or more so the catalog part has been typed instead. Lunar transient phenomena have been observed for almost 1 1/2 millenia, both by the naked eye and telescopic aid. The author has been collecting these reports from the literature and personal communications for the past 17 years. It has resulted in a listing of 1468 reports representing only slight searching of the literature and probably only a fraction of the number of anomalies actually seen. The phenomena are unusual instances of temporary changes seen by observers that they reported in journals, books, and other literature. Therefore, although it seems we may be able to suggest possible aberrations as the causes of some or many of the phenomena it is presumptuous of us to think that these observers, long time students of the moon, were not aware of most of them. -
ILWS Report 137 Moon
Returning to the Moon Heritage issues raised by the Google Lunar X Prize Dirk HR Spennemann Guy Murphy Returning to the Moon Heritage issues raised by the Google Lunar X Prize Dirk HR Spennemann Guy Murphy Albury February 2020 © 2011, revised 2020. All rights reserved by the authors. The contents of this publication are copyright in all countries subscribing to the Berne Convention. No parts of this report may be reproduced in any form or by any means, electronic or mechanical, in existence or to be invented, including photocopying, recording or by any information storage and retrieval system, without the written permission of the authors, except where permitted by law. Preferred citation of this Report Spennemann, Dirk HR & Murphy, Guy (2020). Returning to the Moon. Heritage issues raised by the Google Lunar X Prize. Institute for Land, Water and Society Report nº 137. Albury, NSW: Institute for Land, Water and Society, Charles Sturt University. iv, 35 pp ISBN 978-1-86-467370-8 Disclaimer The views expressed in this report are solely the authors’ and do not necessarily reflect the views of Charles Sturt University. Contact Associate Professor Dirk HR Spennemann, MA, PhD, MICOMOS, APF Institute for Land, Water and Society, Charles Sturt University, PO Box 789, Albury NSW 2640, Australia. email: [email protected] Spennemann & Murphy (2020) Returning to the Moon: Heritage Issues Raised by the Google Lunar X Prize Page ii CONTENTS EXECUTIVE SUMMARY 1 1. INTRODUCTION 2 2. HUMAN ARTEFACTS ON THE MOON 3 What Have These Missions Left BehinD? 4 Impactor Missions 10 Lander Missions 11 Rover Missions 11 Sample Return Missions 11 Human Missions 11 The Lunar Environment & ImpLications for Artefact Preservation 13 Decay caused by ascent module 15 Decay by solar radiation 15 Human Interference 16 3. -
Mapping the Moon Arizona Scientists Played Major Role in Locating Lunar Landing Sites
Arizona Daily Star - 12/16/2018 Copy Reduced to 46% from original to fit letter page Page : 18 18 | MOONSHOT AT 50: APOLLO ANNIVERSARY Premium supplement to the Arizona Daily Star Sunday, December 16, 2018 Mapping the moon Arizona scientists played major role in locating lunar landing sites BY MIKAYLA MACE Arizona Daily Star n 1961, when President John F. Kennedy announced the United States would land a man on the moon by the end of the decade, modern lunar and planetary science was still in its infancy. Its birthplace? The University of Arizona in Tucson. IThe story of the Apollo 11 moon land- ing, which occurred nearly 50 years ago, wouldn’t be complete without the endeavors of a team led by Gerard Kui- per, who became the director of the UA Lunar and Planetary Laboratory. Lunar atlases Even before the Space Race began with the launch of Soviet satellite Sput- nik in 1957, Holland-born Kuiper, direc- tor of the University of Chicago’s Yerkes Observatory in southern Wisconsin, was working on compiling the best im- ages of the moon at the time to create a photographic lunar atlas. Until that time, maps of the moon were drawn by hand and the names of the moon’s features were not agreed upon, said Timothy Swindle, the UA lab’s current director. At an astronomical conference in Dublin, Ireland, in 1955, Kuiper asked anyone interested in assisting him in his endeavor to create a moon atlas to reach out to him. Ewen Whitaker, then the director of the lunar section of the British Astro- nomical Association, was the only one to respond.