September 2020 the Lunar Observer by the Numbers
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Petrography, Geochemistry, and Provenance
Lunar and Planetary Science XXXIV (2003) 1454.pdf THE APOLLO 16 MARE COMPONENT: PETROGRAPHY, GEOCHEMISTRY, AND PROVENANCE. R. A. Zeigler, L. A. Haskin, R. L. Korotev, B. L. Jolliff, and J. J. Gillis, Dept. of Earth and Planetary Sciences, Washington University in St. Louis, Campus Box 1169, 1 Brookings Dr., St. Louis, MO 63116 ([email protected]). Introduction: The A16 (Apollo16) site in the lunar ported may be similar to our VLT samples 65703,9-13 nearside highlands is 220 km from the nearest mare. and 62243,10-22. High-Al basalt 60053,2-9 and the Thus it is no surprise that mare basalt samples are un- high-Al basalts previously reported from A16 samples common at the site. Here, we present the petrography are similar only in being aluminous and low in TiO2. and geochemistry of 5 new mare basalt samples found at The VHT picritic glass 60603,10-16 is unlike anything the A16 site. We also discuss possible provenances of previously reported from the A16 collection. all A16 mare basalt samples using high-resolution global Transport mechanisms: We propose that the mare data for the distribution of Fe and Ti on the lunar surface basalts found at the A16 site were transported there derived from Clementine UV-VIS data [1-2]. through post-basin lateral mixing. Other potential meth- Background: The maria nearest to the A16 site are ods do not seem feasible: Pyroclastic eruption: Sinus Asperitatis (220 km) and Mare Nectaris (~400 According to theoretical models, pyroclastic eruptions km). The A16 regolith consists of basin ejecta from Nec- have an effective eruption limit of <300 km [17], less taris and Imbrium, and possibly Serenitatis, mixed with than half the distance to the nearest known pyroclastic pre-Nectarian regolith [3-4]. -
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. -
8.5 X 13.5 Doublelines.P65
Cambridge University Press 978-0-521-74128-6 - Exploring the Solar System with Binoculars: A Beginner’s Guide to the Sun, Moon, and Planets Stephen James O’Meara’s Index More information Index Adams, John Couch, 96 Carrington, Richard C., 15 degree of condensation (DC) of, Agesinax, 24 Carroll, Lewis, 60 111–112 Aionwantha (Hiawatha), 45 Ceres, 70, 99–101 estimating the brightness of, Airy, George Biddell, 50, 51, 55 discovery and history as a planet, 111–112 Alcock, George, 116 99–100 In–Out method, 111 Allen, Richard Hinckley, 136 general description of, 99, Modified–Out method, 111–112 Alphonsus VI (King of Portugal), 104 100–101 experience helps in observing, 112 Andersen, Hans Christian, 92 how to find, 101 flaring in brightness, 111 Arago, Francois, 59 Chaikin, Andrew, 54 how to locate and identify, 110 Araki, Genichi, 116 Challis, James, 50 in history, relating to, 103–108 Arend, Silvio, 115 Chambers, George F., 8, 19 King David, 103 Aristotle, 65 Cheshire Cat, 60 Melville’s Moby-Dick, 107–108 Arlt, Rainer, 132 Children of God (cult), 108 Napoleon, 106 Arrehenius, Svente, 78, 79 Chinese Catalogue (Biot’s), 131–132 Shakespeare’s Julius Caesar, 103–104 Arter, T. R., 131 Cicero (Roman emperor), 77 the broadside of the comets of Asteroid Belt, 101 City of God, The, 90 1680 and 1682, 104 brightest objects in, 101–102 Collins, Peter, 116 the death of Julius Caesar, 104 asteroids Cometographia, 103 the Middle Ages, 104 2003 EH1, 131 comets, 103–117 the Old Testament?, 103 3200 Phaeton, 142 1P (Halley), 103, 109, 114–115, the whaling ship -
G Qjf-- 910 7 3
,. 1. I , Har,.-apy (HC) icrofichs (MF) ff 063 July 06 i I BIBLIOGRAPHY OF CHE&CAL PRODUCTS OF VOLCANISM prepared by Paul Pushkar and Paul E. Damon - Prepared for the National Aeronautics and Space Administration (SC - NGR - 03 - 002 - 076) Laboratory of Geochronometry and Geochemistry Geochronology Department University of Arizona IE ie (PAGES) ,g1: Qjf-- 910 73 , (NASX~ROR TMX OR AD NUMBER) i BIBLIOGRAPHY OF CHEMICAL PRODUCTS OF VOLCANISM prepared by Paul Pushkar and Paul E. Damon Prepared for the National Aeronautics and Space Administration (SC - NGR - 03- 002 - 076) Laboratory of Geochronometry and Geochemistry Geochronology Department University of Arizona +. s i i Lunar Orbiter IV, Frame No. 157 THE EjARIUS HILLS: A LUNAR VOLCANIC FIELD? '- sa 3 TABLE OF CONTENTS Page Preface. 8 . i Acknowledgments . * a e . e i I Volcanic Gases and Sublimates, Gases Contained in Rocks, and Related Matters . e . 1 II Nongaseous Chemical Products of Terrestrial Volcanism . III Gas Content of Meteorites, Lunar Volcanfsm, and Related Subjects . 46 IV General References Dealing with Terrestrial Volcanism . 53 PREFACE This bibliography was compiled during a one-year literature search on possible volcanic products on the Moon. The bibliography is divided into four sections: I. Volcanic Gases and Sublimates, Gases Contained in Rocks, and Related Matters The literature in these fields, as emphasized recently by White and Waring (1963) is scanty, and for the most part by fiussian and Japanese scientists arid hence often presents difficulties in access and language to English-specking scientists. This section is believed to be fairly com- prehensive from the present to at least 1935. -
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. -
INDEX to 1915-1919 Obituaries in the Canton Repository
INDEX To 1915-1919 Obituaries in the Canton Repository Published by the Stark County District Library of Canton, Ohio 2005 Index to 1915-1919 Obituaries in the Canton Repository The following is an alphabetical listing, by the deceased’s surname, of obituaries that appeared in the Canton, Ohio newspaper, The Repository. It was compiled by the library staff during the course of the year in the hope that it would be a useful tool to genealogy, as well as other researchers. To use this index, simply locate the name of the person whose obituary you wish to find. The entries will appear as follows: Miller William A. (Estella M.) Mrs. 1924 Jan. 13 30 The first column is the name of the deceased. The second gives the date on which the item appeared. And the third tells the page number containing the obituary. You may find one name with multiple listings showing different dates and locations in the paper. This indicates consecutive listings for that individual. I encourage you to view each for additional information. Index to 1915-1919 Obituaries in the Canton Repository Surname Given Name Maiden Title Year Mth Day Pg ? Mary 1918 Apr. 18 15 Aaron Benjamin 1918 Nov. 27 2 Abbott Lawrence C. 1919 Mar. 14 24 Abels infant 1919 July 16 6 Abherve Minnie Jacobs Mrs. 1918 Dec. 13 33 Abrams Leo 1917 Apr. 24 2 Abt Leo 1918 Apr. 27 1 Abvrezis Macone 1917 Sept. 17 2 Acker L. E. 1918 Jan. 13 26 Acker Leonard E. 1918 Jan. 12 5 Acker Sarah Mrs. -
NATURE [Dec. 7, 1871
100 NATURE [Dec. 7, 1871 men is usually of the highest quality, both for carefulness evidence to prove that markings of various forms exist on the of investigation and clearness of statement ; and the great surface of the planet. I am the more particularly induced to say this by having before me upwards of sixty sketches of their appear similarity which exists b etwe~n t~e fau~as and floras ?f ance, made by experiencei ob,erven, wh J in the making of ob and of the Scandmav1an reg10n, enables th~,r our islands servations employ telescop~s of great power and excellent defioi work to be used to a certain extent as h andbooks by ti,ln. No doubt the faint cJ.rnrll 0 ke m1rkings can only be made British Naturalists. May their study lead the latter to out after attentive gazing, and then are scarcely visible, though imitate the Scandinavian mode of work! We are led to they have been distinctly ,een by many observers. It i, difficult these remarks by the receipt of the tenth and concluding to account for the fact that Mr. Dawe; could not di;fnguish volume of Prof. Thomson'::; descriptive work on the Scan them, but perhaps the reas m m1y be app.vent, if we co,isider that dinavian Coleoptera, alt~ough this cons_i~ts a lmost entirely an obJt·rver who is the mo;t succ~s;ful in the o:iservatioa of faint of corrections, emendatwns, and add,twns to the con companion; to dou':ile stars, cann') t satisfactorily observe the tents of the nine previous volumes, in which the syste faint markings with which th, plane:'s disc is diversified. -
July 2020 in This Issue Online Readers, ALPO Conference November 6-7, 2020 2 Lunar Calendar July 2020 3 Click on Images an Invitation to Join ALPO 3 for Hyperlinks
A publication of the Lunar Section of ALPO Edited by David Teske: [email protected] 2162 Enon Road, Louisville, Mississippi, USA Recent back issues: http://moon.scopesandscapes.com/tlo_back.html July 2020 In This Issue Online readers, ALPO Conference November 6-7, 2020 2 Lunar Calendar July 2020 3 click on images An Invitation to Join ALPO 3 for hyperlinks. Observations Received 4 By the Numbers 7 Submission Through the ALPO Image Achieve 4 When Submitting Observations to the ALPO Lunar Section 9 Call For Observations Focus-On 9 Focus-On Announcement 10 2020 ALPO The Walter H. Haas Observer’s Award 11 Sirsalis T, R. Hays, Jr. 12 Long Crack, R. Hill 13 Musings on Theophilus, H. Eskildsen 14 Almost Full, R. Hill 16 Northern Moon, H. Eskildsen 17 Northwest Moon and Horrebow, H. Eskildsen 18 A Bit of Thebit, R. Hill 19 Euclides D in the Landscape of the Mare Cognitum (and Two Kipukas?), A. Anunziato 20 On the South Shore, R. Hill 22 Focus On: The Lunar 100, Features 11-20, J. Hubbell 23 Recent Topographic Studies 43 Lunar Geologic Change Detection Program T. Cook 120 Key to Images in this Issue 134 These are the modern Golden Days of lunar studies in a way, with so many new resources available to lu- nar observers. Recently, we have mentioned Robert Garfinkle’s opus Luna Cognita and the new lunar map by the USGS. This month brings us the updated, 7th edition of the Virtual Moon Atlas. These are all wonderful resources for your lunar studies. -
Sterne Und Weltraum 1999
ie Erforschung der Oberfläche des DMondes blieb lange Zeit Astronomen Von den Apollo-Landungen mit lichtstarken Teleskopen vorbehalten (Abb. 1). Die Apollo-Missionen haben den bis heute Begleiter der Erde den Geowissenschaften erschlossen und damit ganz entscheidend Was wir über die Mondoberfläche gelernt haben dazu beigetragen, Morphologie, physikali- sche Eigenschaften, chemisch-mineralogi- Von Jürgen Oberst, Ralf Jaumann und Harald Hoffmann sche Zusammensetzung und Alter der Oberfläche des Mondes zu bestimmen und seine Geschichte besser zu verstehen. Erstmal nach der Landung der Apollo-Astronauten auf dem Mond konnten die Dieser Artikel gibt einen Überblick dar- vielfältigen Methoden der Geowissenschaften auf einen anderen Himmelskörper über, was wir dank Apollo über die Mond- angewandt werden. Hier und in weiteren Beiträgen werden die Ergebnisse dieser oberfläche gelernt haben und welche wich- stillen Revolution beschrieben. tigen Fragen der Mondforschung nach Apollo noch offen geblieben sind. Viele die- ser Fragen sind noch heute ungeklärt – andere konnten mittlerweile mit Hilfe neuer Auswertetechniken und neuer Daten beantwortet werden. Tatsächlich haben die Raumsonden Galileo, Clementine und Lu- nar Prospector viele neue Fragen aufgewor- fen, die zukünftige Mondmissionen und Mondforscher lösen müssen. Morphologie und Kartographie Schon vor dem Zeitalter der Mondflüge waren Größe des Mondes und Details sei- ner Oberflächenmorphologie grob be- kannt. Sternbedeckungen durch den Mond während seines Umlaufs um die Erde kann man nutzen, um die Größe des Erdtraban- ten und die Topographie entlang des Ran- des der Mondscheibe zu ermitteln. Schat- tenwurfmessungen ermöglichten es, die Höhen von Kraterrändern und Zentralber- gen recht genau zu bestimmen. Während der Apollo-Missionen konnten erstmalig direkte und genaue Messungen der Topo- graphie vor Ort durchgeführt werden. -
Effusive Lunar Domes in Mare Tranquillitatis: Morphometry and Mode of Emplacement
Lunar and Planetary Science XXXIX (2008) 1107.pdf EFFUSIVE LUNAR DOMES IN MARE TRANQUILLITATIS: MORPHOMETRY AND MODE OF EMPLACEMENT. K. C. Pau1, R. Lena2, C. Wöhler3, M. T. Bregante4, G. Sbarufatti5 – Geologic Lunar Research (GLR) Group. 1Flat 20A, Fook Chak House, Tung Fai Gardens, 17 Po Yan Street, Sheung Wan, Hong Kong; [email protected]; 2Via Cartesio 144, sc. D, 00137 Rome, Italy; [email protected]; 3Daimler Group Research, P. O. Box 2360, D-89013 Ulm, Germany; [email protected]; 4Via Antica Romana Occ. 13, 16039 Sestri Levante Genova, Italy; [email protected]; 5Via Cabrini 10, 26842 Caselle Landi, Lodi, Italy; [email protected] Introduction: Lunar mare domes are smooth low by a low Titanium content, while the youngest lavas features with gentle convex upward profiles. They are erupted in this region are spectrally blue (high circular to elliptical in shape. Isolated domes may be Titanium content) [4,5]. The Carrel complex largely found in almost all maria, but significant concentra- represents the eastern rim of a ruined crater nearly tions occur in the Hortensius region, Oceanus Procel- completely buried by mare lava. In the Clementine larum, and Mare Tranquillitatis [1]. These domes are colour ratio image, the crater ruin and ejecta from commonly interpreted as shield volcanoes or laccoliths Carrel have the same reddish color as the mare surface [2]. Recent studies about lunar domes are based on the around Jansen. The soil around Ca1 and also C13 is evaluation of their spectrophotometric and morpho- spectrally bluish, indicating a moderate TiO2 content, metric properties, rheologic parameters, and their clas- while the dome A7 appears strongly blue, indicating sification based on the spectral properties and three- basalts of high TiO2 content (Figs. -
THE UNUSUAL ATLAS/HERCULES REGION of the MOON. J. T. S. Cahill1, P
51st Lunar and Planetary Science Conference (2020) 2936.pdf THE UNUSUAL ATLAS/HERCULES REGION OF THE MOON. J. T. S. Cahill1, P. O. Hayne2, G. W. Patter- son1, B. T. Greenhagen1, and M. A. Wieczorek3. Johns Hopkins University Applied Physics Laboratory, Laurel, MD ([email protected]), (2) University of Colorado, Boulder, CO, and (3) Observatoire de la Côte d’Azur, Nice, France. Introduction: A new class of enigmatic deposits known studies have inferred any additional and more on the Moon has emerged since the Lunar Reconnais- expansive volcanic activity that would be coincident sance Orbiter (LRO) entered orbit that contrasts with with the thermophysical boundaries reported here. the lunar regolith at large. Unlike optical anomalies, Making the region even more scientifically intri- such as swirls, these deposits are unusual for their guing, the craters Atlas, Hercules, and Burg have each thermophysical characteristics. One ubiquitous class previously been identified as radar dark halo craters consists of lunar cold-spot craters, so-named because [5]. Ghent et al. [6]’s most recent analysis of the they are characterized by extensive regions, relative physical properties of radar dark halo craters reported to their cavity diameter and depth, of anomalously that the halo material is depleted in surface rocks, but cold regolith temperatures in nighttime Diviner data are otherwise thermophysically indistinct from back- [2]. These cold regions are not easily explained by ground regolith. This directly contrasts with what we conventional impact mechanics. Hayne et al. [1] fur- observe in H-parameter maps of the Atlas region. ther characterized these features with high Diviner- Here, with additional radar, thermal infrared and derived H-parameter values which provides a conven- gravity data sets for further perspective we re- tion for describing thermophysical depth profiles. -
Remote Sensing and Geologic Studies of the Northeastern Portion of the Lunar Nearside: Final Results
40th Lunar and Planetary Science Conference (2009) 1483.pdf REMOTE SENSING AND GEOLOGIC STUDIES OF THE NORTHEASTERN PORTION OF THE LUNAR NEARSIDE: FINAL RESULTS. B.R. Hawke1, T.A. Giguere2, D.T. Blewett3, J.M. Boyce1, J. Cahill1, J.J. Gillis-Davis1, J.J. Hagerty4, P.G. Lucey1, C.A. Peterson1, G.A. Smith1, P.D. Spu- dis5, and G.J. Taylor1, 1Hawaii Institute of Geophysics and Planetology, University of Hawaii, Honolulu, HI 96822, 2Intergraph Corporation, P.O. Box 75330, Kapolei, HI 96707, 3Johns Hopkins University Ap- plied Physics Laboratory, Laurel, MD 20723, 4U.S. Geological Survey, Astrogeology Program, 2255 N. Gemini Drive, Flagstaff, AZ 86001, 5Lunar and Planetary Institute, Houston, TX 77058. Introduction: Parts of the northeastern near- high latitudes. Hence, we have used IRECs to side (NEN) north and east of Mare Frigoris dis- identify possible cryptomare units in the NEN play light plains deposits with a variety of ages region. Numerous IRECs were identified on and possible cryptomare deposits [1, 2, 3]. We highland units in the NEN region and 42 were have selected a portion of this area for an inten- selected for detailed analysis. Earth-based near- sive remote sensing and geologic investigation. IR spectra exist for two of these IRECs. Gartner This NEN region is centered just east of Mare D is a small dark-haloed crater (diameter = 8 km) Frigoris at 52º N, 40º E and includes the craters which excavated material from beneath the sur- Atlas, Hercules, Thales, Gartner, Democritus, Ce- face of a light plains unit in the floor of Gartner pheus, and Kane.