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A Zircon U-Pb Study of the Evolution of Lunar KREEP
A zircon U-Pb study of the evolution of lunar KREEP By A.A. Nemchin, R.T. Pidgeon, M.J. Whitehouse, J.P. Vaughan and C. Meyer Abstract SIMS U-Pb analyses show that zircons from breccias from Apollo 14 and Apollo 17 have essentially identical age distributions in the range 4350 to 4200 Ma but, whereas Apollo 14 zircons additionally show ages from 4200 to 3900 Ma, the Apollo 17 samples have no zircons with ages <4200 Ma. The zircon results also show an uneven distribution with distinct peaks of magmatic activity. In explaining these observations we propose that periodic episodes of KREEP magmatism were generated from a primary reservoir of KREEP magma, which contracted over time towards the centre of Procellarum KREEP terrane. Introduction One of the most enigmatic features of the geology of the Moon is the presence of high concentrations of large ion lithophile elements in clasts from breccias from non mare regions. This material, referred to as KREEP (1) from its high levels of K, REE and P, also contains relatively high concentrations of other incompatible elements including Th, U and Zr. Fragments of rocks with KREEP trace element signatures have been identified in samples from all Apollo landing sites (2). The presence of phosphate minerals, such as apatite and merrillite (3); zirconium minerals, such as zircon (4), zirconolite (5) and badelleyite (6), and rare earth minerals such as yttrobetafite (7), are direct expressions of the presence of KREEP. Dickinson and Hess (8) concluded that about 9000 ppm of Zr in basaltic melt is required to saturate it with zircon at about 1100oC (the saturation concentration increases exponentially with increasing temperature). -
Apollo 14 Press
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION WO 2-4155 WASHINGT0N.D.C. 20546 lELS.wo 36925 RELEASE NO: 71-3K FOR RELEASE: THURSDAY A. M . January 21, 1971 P R E S S K I T -more - 1/11/71 2 -0- NATIONAL AERONAUTICS AND SPACE ADMINISTRATION (m2) 962-4155 N E w s WASHINGTON,D.C. 20546 mu: (202) 963-6925 FOR RELEASE: THURSDAY A..M. January 21:, 1971 RELEASE NO: 71-3 APOLLO 14 LAUNCH JAN. 31 Apollo 14, the sixth United States manned flight to the Moon and fourth Apollo mission with an objective of landing men on the Moon, is scheduled for launch Jan. 31 at 3:23 p.m. EST from Kennedy Space Center, Fla. The Apollo 14 lunar module is to land in the hilly upland region north of the Fra Mauro crater for a stay of about 33 hours, during whick, the landing crew will leave the spacecraft twice to set up scientific experiments on the lunar surface and to continue geological explorations. The two earlier Apollo lunar landings were Apollo 11 at Tranquillity Base and Apollo 12 at Surveyor 3 crater in the Ocean of Storms. Apollo 14 prime crewmen are Spacecraft Commander Alan B. Shepard, Jr., Command Module Pilot Stuart A. Roosa, and Lunar Module Pilot Edgar I). Mitchell. Shepard is a Navy car-sain Roosa an Air Force major and Mitchell a Navy commander. -more- 1/8/71 -2- Lunar materials brought- back from the Fra Mauro formation are expected to yield information on the early history of the Moon, the Earth and the solar system--perhaps as long ago as five billion years. -
Sky and Telescope
SkyandTelescope.com The Lunar 100 By Charles A. Wood Just about every telescope user is familiar with French comet hunter Charles Messier's catalog of fuzzy objects. Messier's 18th-century listing of 109 galaxies, clusters, and nebulae contains some of the largest, brightest, and most visually interesting deep-sky treasures visible from the Northern Hemisphere. Little wonder that observing all the M objects is regarded as a virtual rite of passage for amateur astronomers. But the night sky offers an object that is larger, brighter, and more visually captivating than anything on Messier's list: the Moon. Yet many backyard astronomers never go beyond the astro-tourist stage to acquire the knowledge and understanding necessary to really appreciate what they're looking at, and how magnificent and amazing it truly is. Perhaps this is because after they identify a few of the Moon's most conspicuous features, many amateurs don't know where Many Lunar 100 selections are plainly visible in this image of the full Moon, while others require to look next. a more detailed view, different illumination, or favorable libration. North is up. S&T: Gary The Lunar 100 list is an attempt to provide Moon lovers with Seronik something akin to what deep-sky observers enjoy with the Messier catalog: a selection of telescopic sights to ignite interest and enhance understanding. Presented here is a selection of the Moon's 100 most interesting regions, craters, basins, mountains, rilles, and domes. I challenge observers to find and observe them all and, more important, to consider what each feature tells us about lunar and Earth history. -
Moon Minerals a Visual Guide
Moon Minerals a visual guide A.G. Tindle and M. Anand Preliminaries Section 1 Preface Virtual microscope work at the Open University began in 1993 meteorites, Martian meteorites and most recently over 500 virtual and has culminated in the on-line collection of over 1000 microscopes of Apollo samples. samples available via the virtual microscope website (here). Early days were spent using LEGO robots to automate a rotating microscope stage thanks to the efforts of our colleague Peter Whalley (now deceased). This automation speeded up image capture and allowed us to take the thousands of photographs needed to make sizeable (Earth-based) virtual microscope collections. Virtual microscope methods are ideal for bringing rare and often unique samples to a wide audience so we were not surprised when 10 years ago we were approached by the UK Science and Technology Facilities Council who asked us to prepare a virtual collection of the 12 Moon rocks they loaned out to schools and universities. This would turn out to be one of many collections built using extra-terrestrial material. The major part of our extra-terrestrial work is web-based and we The authors - Mahesh Anand (left) and Andy Tindle (middle) with colleague have build collections of Europlanet meteorites, UK and Irish Peter Whalley (right). Thank you Peter for your pioneering contribution to the Virtual Microscope project. We could not have produced this book without your earlier efforts. 2 Moon Minerals is our latest output. We see it as a companion volume to Moon Rocks. Members of staff -
Apollo 14 Press
/ 17,° " 4 c 0 /r- NATIONAL AERONAUTICS AND SPACE ADMINISTRATION WO 2-4155 FELS . WASHINGTON, D .0 . 20546 WO 3-6925 RELEASE NO: 71-3K FOR RELEASE:THURSDAY A.M. January 21, 1971 PROJECT: APOLLO 14 P (To be launched no earlier than Jan. 31) Eli?:4S7D7 5T- amuouAfX Ce4lift R FEB 1 ign contents E FPFITZcItt‘ GENERAL RELEASE 1-5 S COUNTDOWN 6 7 LAUNCH AND MISSION PROFILE 8 9 Launch Opportunities 9 Ground Elapsed Time Update 10 Launch Events 11 Mission Events 12-22 S Entry Events 23-24 RECOVERY OPERATIONS 25 Crew and Sample Return Schedule 26 MISSION OBJECTIVES 27 Lunar Surface Science 27-39 Lunar Orbital Science 39-46 Engineering/Operational Objectives 46-47 APOLLO LUNAR HAND TOOLS 48-51 FRA MAURO LANDING SITE 52-53 1‹: PHOTOGRAPHIC EQUIPMENT 54-55 TELEVISION 56 Apollo 14 TV Schedule 57-58 ZERO-GRAVITY INFLIGHT DEMONSTRATIONS 59 Electrophoretic Separation 59-61 Heat Flow and Convection 61 Liquid Transfer 62 Composite Casting 62-63 ASTRONAUTS AND CREW EQUIPMENT 64 Space Suits 64-69 Personal Hygiene 70 Medical Kit 70 Survival Kit 71 Crew Food 71 Prime Crew Biographies 72-78 Backup Crew Biographies 79-84 Flight Crew Health Stabilization Program 85 -more- 2 APOLLO 14 FLAGS, LUNAR MODULE PLAQUE 86 LUNAR RECEIVING LABORATORY (LRL) 87- 88 Sterilization and Release of Spacecraft 88-89 SATURN V LAUNCH VEHICLE 90 First Stage 90 Second Stage 90 Third Stage 90-91 Instrument Unit 92 Propulsion 92 Major Vehicle Changes 93 APOLLO SPACECRAFT 94-96 Command-Service Module Modifications 96-97 Lunar Module (LM) 98-100 MANNED -
Workshop on Moon in Transition: Apollo 14, Kreep, and Evolved Lunar Rocks
WORKSHOP ON MOON IN TRANSITION: APOLLO 14, KREEP, AND EVOLVED LUNAR ROCKS (NASA-CR-I"'-- N90-I_02o rRAN31TION: APJLLN l_p KRFEP, ANu _VOLVFD LUNAR ROCKS (Lunar and Pl_net3ry !nst.) I_7 p C_CL O3B Unclas G3/91 0253133 LPI Technical Report Number 89-03 UNAR AND PLANETARY INSTITUTE 3303 NASA ROAD 1 HOUSTON, TEXAS 77058-4399 7 WORKSHOP ON MOON IN TRANSITION: APOLLO 14, KREEP, AND EVOLVED LUNAR ROCKS Edited by G. J. Taylor and P. H. Warren Sponsored by Lunar and Planetary Institute NASA Johnson Space Center November 14-16, 1988 Houston, Texas Lunar and Planetary Institute 330 ?_NASA Road 1 Houston, Texas 77058-4399 LPI Technical Report Number 89-03 Compiled in 1989 by the LUNAR AND PLANETARY INSTITUTE The Institute is operated by Universities Space Research Association under Contract NASW-4066 with the National Aeronautics and Space Administration. Material in this document may be copied without restraint for Library, abstract service, educational, or personal research purposes; however, republication of any portion requires the written permission of the authors as well as appropriate acknowledgment of this publication. This report may be cited as: Taylor G. J. and Warren PI H., eds. (1989) Workshop on Moon in Transition: Apo{l_ 14 KREEP, and Evolved Lunar Rocks. [PI Tech. Rpt. 89-03. Lunar and Planetary Institute, Houston. 156 pp. Papers in this report may be cited as: Author A. A. (1989) Title of paper. In W_nkshop on Moon in Transition: Ap_llo 14, KREEP, and Evolved Lunar Rocks (G. J. Taylor and P. H. Warren, eds.), pp. xx-yy. LPI Tech. Rpt. -
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. -
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. -
12, 1970 30 Pages 10 Cents Apollo Heads for Landing on Moon
3 ft 200 :;.v z AYS 33432 r Vol. 15, No. 90 BOCA RATON NEWS Sunday, April 12, 1970 30 Pages 10 Cents Apollo heads for landing on moon CAPE KENNEDY (UPI)— Apollo with a lunar sample bonanza that Space agency administrator Thomas 13's two prime pilots and a stand-in might contain the oldest rocks ever O. Paine made the decision to go with astronaut rocketed toward the moon seen by man—possibly dating back 5 Swigert after Loveil endorsed him on today on a daring expedition to explore billion years to the birth of the solar the basis of a day and a half of a lunar valley lined with ancient ridges system. moonflight rehearsals hi a spacecraft and boulder-strewn craters. The astronauts, wearing spacesuits trainer. They showed that Swigert Moori veteran James A. Lovell, 42, with the Stars and Stripes on shoulder could work smoothly with Lovell and lunar module pilot Fred W. Haise, 36, patches, left their quarters at 11:05 Haise. and substitute command module pilot ajn. and headed toward the launch The mission is the nation's third John L. Swigert, 38, began the nation's pad. They smiled and waved quickly to lunar landing expedition, and the most third and toughest moon landing onlookers as they stepped into then" ambitious. Apollos 11 and 12 landed mission on a Saturn 5 rocket that van. relatively easy-to-reach flatlands last Commander Jim Lovell leads the Apollo 13 crew from Astronauts John Swigert and Fred Haise. Following the spewed a long plume of orange flame. -
NASA - Apollo 13
Press Kit NASA - Apollo 13 Ä - 1970 - National Aeronautics and Space Administration Ä - 2010 - National Aeronautics and Space Administration Restored version by Matteo Negri (Italy) Web: http://www.siamoandatisullaluna.com NATIONAL AERONAUTICS AND SPACE ADMINISTRATION WO 2-4155 I NEWS WASHINGTON,D .C. 20546 TELS4 WO 3-6925 FOR RELEASr? THURSDAY A.M. 2, 1970 RELEASE NO: 70-~OK April P R F. E S S K I T 2 -0- t RELEASE NO: 70-50 APOLLO 13 THIRD LUNAR LANDING MISSION Apollo 13, the third U.S. manned lunar landing mission, will be launchefi April 11 from Kennedy Space Center, Fla., to explore a hilly upland region of the Moon and bring back rocks perhaps five billion years old, The Apollo 13 lunar module will stay on the Moon more than 33 hours and the landing crew will leave the spacecraft twice to emplace scientific experiments on the lunar surface and to continue geological investigations. The Apollo 13 landing site is in the Fra Mauro uplands; the two National Aeronautics and Space Administration ppevious landings were in mare or ''sea" areas, Apollo 11 in the Sea of Tranqullfty and Apollo 12 in the Ocean of Storms. Apollo 13 crewmen are commander James A. Lovell, Jr.; command module pilot momas K. MBttingly 111, and lunar module pilot Fred W. Haise, Jr. Lovell is a U.S. Navy captain, Mattingly a Navy lieutenant commander, and Haise a civllian. -more- 3/26/70 Launch vehicle is a Saturn V. Apollo 13 objectives are: * Perform selenological inspection, survey and sampling of materials in a preselected region of the Fra Mauro formation, c Deploy and activate an Apollo Lunar Surface Experiment Package (ALSEP) , * Develop man's capability to work in the lunar environment. -
Maps and Meanings: Urban Cartography and Urban Design
Maps and Meanings: Urban Cartography and Urban Design Julie Nichols A thesis submitted in fulfilment of the requirements of the degree of Doctor of Philosophy The University of Adelaide School of Architecture, Landscape Architecture and Urban Design Centre for Asian and Middle Eastern Architecture (CAMEA) Adelaide, 20 December 2012 1 CONTENTS CONTENTS.............................................................................................................................. 2 ABSTRACT .............................................................................................................................. 4 ACKNOWLEDGEMENT ....................................................................................................... 6 LIST OF FIGURES ................................................................................................................. 7 INTRODUCTION: AIMS AND METHOD ........................................................................ 11 Aims and Definitions ............................................................................................ 12 Research Parameters: Space and Time ................................................................. 17 Method .................................................................................................................. 21 Limitations and Contributions .............................................................................. 26 Thesis Layout ....................................................................................................... 28 -
UN I TED STATES DEPARTMENT of the INTERIOR Center Of
IN REPLY REFER TO: UN I TED STATES DEPARTMENT OF THE INTERIOR GEOLOGICAL SURVEY Center of Astrogeology 601 East Cedar Avenue Flagsta.ff, Arizona 86001 November 30, 1971 Memorar1dum To Noel Hinr~ers, Chairman, ad hoc Site Selection Group, A,p_ollo 17 From William R. Muehlberger, Principal Investigator, s~059 Apoll~ Field Geology Investigations Subject: Candidate Apollo 17 landing sites The attached memorandum presents a summary of the recommen_ded sites for Apoilo 17'by. the.photogeologic mappers of the U.S. Geol6gical Survey and my group of Co-investigator's. Please consider this as our basic input to.your ad hoc site selection. group. You will note thaf Alphousus is third on our list--actually it is on the list only because it had b~en a candidate site for Apollo 17 }' c during the Apollo 16 deliberations. None of our group voted for it as their first choice in the slate of three sites herein presented. Littrow highlands was a bare majority over Gassendi; we would be pleased with either side for the Apollo 17 landing site. if·there is further information that we can contribute to your deliberations, please let me know and I'll get it to you. c .. "' . November 30, 1971 ·'· o. APOLLO FIELD GEOLOGY INVESTIGATIONS (S-059) EXPERIMENT GROUP RECOMMENDATIONS FOR APOLLO 17 LANDING SITES R<~;tionale a11c1 Recommemdations ·, Rationale The Apollo 17 mi·ssion to the moon will be 'the culmination and must provide the optim~l realization of the first stage of.man's sci"entific exp-loration of the moon. Our knowle·dge of the maori derived from the preceding Apollo mi~sions has grown with sufficient order~iness and comprehensiveness to indicate unambiguously that the m.a'jor unexplored region.