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Apollo 17 Index
Preparation, Scanning, Editing, and Conversion to Adobe Portable Document Format (PDF) by: Ronald A. Wells University of California Berkeley, CA 94720 May 2000 A P O L L O 1 7 I N D E X 7 0 m m, 3 5 m m, A N D 1 6 m m P H O T O G R A P H S M a p p i n g S c i e n c e s B r a n c h N a t i o n a l A e r o n a u t i c s a n d S p a c e A d m i n i s t r a t i o n J o h n s o n S p a c e C e n t e r H o u s t o n, T e x a s APPROVED: Michael C . McEwen Lunar Screening and Indexing Group May 1974 PREFACE Indexing of Apollo 17 photographs was performed at the Defense Mapping Agency Aerospace Center under the direction of Charles Miller, NASA Program Manager, Aerospace Charting Branch. Editing was performed by Lockheed Electronics Company, Houston Aerospace Division, Image Analysis and Cartography Section, under the direction of F. W. Solomon, Chief. iii APOLLO 17 INDEX 70 mm, 35 mm, AND 16 mm PHOTOGRAPHS TABLE OF CONTENTS Page INTRODUCTION ................................................................................................................... 1 SOURCES OF INFORMATION .......................................................................................... 13 INDEX OF 16 mm FILM STRIPS ........................................................................................ 15 INDEX OF 70 mm AND 35 mm PHOTOGRAPHS Listed by NASA Photograph Number Magazine J, AS17–133–20193 to 20375......................................... -
Apollo 13 on Course, Streaks Toward Earth
m ■ r \ . \\ ?v- ■ , V '-V '.-' ■ •;i ■■ , I ■ ''' ' /,■ ' s ux i , 1 PAOB FORTY WBDNiSSDAY, APRIL 16, 1970 I I jRattrbfiitfr lEn^ning U m ld Most Manchester Stares Open Tonight Until 9 ■ h-'’ 1 . - * '’li ?i Vernon Aasociatlon for Chil The board of trustees of Com champion <dtew player flhnan-' • About Town dren with 'L«amlng Dlsabllltlea munity < Baptist Church will Rabbi, Minister uel Tjasker, Dr. Plata has a i ■ . i will meet tonight at 8 at the meet tonight at 7;S0 In the s a l e o n iaM KatM «M M. Ruah, daugh- long tournament record in the PINENURST Vernon Center Middle School. Ohurch youth M ldlng. Will Present eaat. In h4a moat recent com Average Doily Net Pren Ron The Weather ' * tar of-Mr. wd Mr*. Henry J. RcA>ert J. Duffy of the speech Rd., to In petition, Dr. Plata took the Inoreestng oloudlneaa tonight; i.'l [ Riuh of « department of the University of The Senior Hlg^ Baptist a r r e s t s Dialogue Sermon For Th. Wedi Boded tiM gtoe OpUega title for the ISth time In the April u, ino low 86 to 40. Tomorrow oloudy. Connecticut will apeak about Youth Fellowship of Communi Paul Otto Bwig, 17, of 86 VU- Western MaaeaclHi^ts and chance of showeri; high In low in Weetoii; to a grad- "Description of a Speech-Lan The Rev'. Clifford O. Simpeon, unto of ilo High ty Baptist Church will sponsor fago St., RockvlUe, charged on OonneoUcut VaBey C h ^ Cham eoa. Saturday’ s outlook -4 a tr. -
The Size-Frequency Distribution of Elliptical Impact Craters
Earth and Planetary Science Letters 310 (2011) 1–8 Contents lists available at ScienceDirect Earth and Planetary Science Letters journal homepage: www.elsevier.com/locate/epsl The size-frequency distribution of elliptical impact craters G.S. Collins a,⁎, D. Elbeshausen b, T.M. Davison a, S.J. Robbins c, B.M. Hynek c a Department of Earth Science and Engineering, Imperial College, London, UK b Museum für Naturkunde, Leibniz-Institute at the Humboldt-University of Berlin, Germany c Laboratory for Atmospheric and Space Physics, University of Colorado at Boulder, USA article info abstract Article history: Impact craters are elliptical in planform if the impactor's trajectory is below a threshold angle of incidence. Received 5 January 2011 Laboratory experiments and 3D numerical simulations demonstrate that this threshold angle decreases as the Received in revised form 7 June 2011 ratio of crater size to impactor size increases. According to impact cratering scaling laws, this implies that Accepted 22 July 2011 elliptical craters occur at steeper impact angles as crater size or target strength increases. Using a standard Available online 27 August 2011 size-frequency distribution for asteroids impacting the terrestrial planets we estimate the fraction of elliptical Editor: T. Spohn craters as a function of crater size on the Moon, Mars, Earth, Venus and Mercury. In general, the expected fraction of elliptical craters is ~2–4% for craters between 5 and 100-km in diameter, consistent with the Keywords: observed population of elliptical craters on Mars. At larger crater sizes both our model and observations impact craters suggest a dramatic increase in the fraction of elliptical craters with increasing crater diameter. -
Eugene M. Shoemaker 1928-1997
Eugene M. Shoemaker 1928-1997 A Biographical Memoir by Susan W. Kieffer ©2015 National Academy of Sciences. Any opinions expressed in this memoir are those of the author and do not necessarily reflect the views of the National Academy of Sciences. EUGENE M. SHOEMAKER April 28, 1928–July 18, 1997 Elected to the NAS, 1980 Eugene M. Shoemaker, a leading light of the United States Geological Survey, died on July 18, 1997, in a tragic motoring accident near Alice Springs, Australia. Gene was doing what he loved most—studying meteorite impact craters in the field with his wife of 46 years, Carolyn (Spellman) Shoemaker. Carolyn was badly injured in the accident but recovered. Gene is survived by his three chil- dren, Christine Woodard, Linda Salazar, and Patrick Shoe- maker. On July 31, 1999, some of his ashes were taken to the Moon on the Lunar Prospector space probe, and to this date he is the only person whose remains have been Shoemaker. Photograph by Carolyn laid to rest on the Moon. The brass casing of his memorial capsule bears a quotation from Shakespeare’s Romeo and Juliet: By Susan W. Kieffer And, when he shall die Take him and cut him out in little stars And he will make the face of heaven so fine That all the world will be in love with night And pay no worship to the garish sun. Gene’s enquiring mind spanned an unusually large range of scientific disciplines— petrology, astronomy, stratigraphy, field geology, volcanology, impact dynamics, and paleomagnetism, to name a few. From his work, whole new fields of shock metamorphic studies, impact crater modeling, and stratigraphic relations on planetary bodies evolved. -
National Aeronautics and Space Administration) 111 P HC AO,6/MF A01 Unclas CSCL 03B G3/91 49797
https://ntrs.nasa.gov/search.jsp?R=19780004017 2020-03-22T06:42:54+00:00Z NASA TECHNICAL MEMORANDUM NASA TM-75035 THE LUNAR NOMENCLATURE: THE REVERSE SIDE OF THE MOON (1961-1973) (NASA-TM-75035) THE LUNAR NOMENCLATURE: N78-11960 THE REVERSE SIDE OF TEE MOON (1961-1973) (National Aeronautics and Space Administration) 111 p HC AO,6/MF A01 Unclas CSCL 03B G3/91 49797 K. Shingareva, G. Burba Translation of "Lunnaya Nomenklatura; Obratnaya storona luny 1961-1973", Academy of Sciences USSR, Institute of Space Research, Moscow, "Nauka" Press, 1977, pp. 1-56 NATIONAL AERONAUTICS AND SPACE ADMINISTRATION M19-rz" WASHINGTON, D. C. 20546 AUGUST 1977 A % STANDARD TITLE PAGE -A R.,ott No0... r 2. Government Accession No. 31 Recipient's Caafog No. NASA TIM-75O35 4.-"irl. and Subtitie 5. Repo;t Dote THE LUNAR NOMENCLATURE: THE REVERSE SIDE OF THE August 1977 MOON (1961-1973) 6. Performing Organization Code 7. Author(s) 8. Performing Organizotion Report No. K,.Shingareva, G'. .Burba o 10. Coit Un t No. 9. Perlform:ng Organization Nome and Address ]I. Contract or Grant .SCITRAN NASw-92791 No. Box 5456 13. T yp of Report end Period Coered Santa Barbara, CA 93108 Translation 12. Sponsoring Agiicy Noms ond Address' Natidnal Aeronautics and Space Administration 34. Sponsoring Agency Code Washington,'.D.C. 20546 15. Supplamortary No9 Translation of "Lunnaya Nomenklatura; Obratnaya storona luny 1961-1973"; Academy of Sciences USSR, Institute of Space Research, Moscow, "Nauka" Press, 1977, pp. Pp- 1-56 16. Abstroct The history of naming the details' of the relief on.the near and reverse sides 6f . -
A Home for Heroes-Timber Cove
A HOME FOR HEROES By Rebecca Wright hen Timber Cove was established in 1958, its appealing pathway to the spacious lots. Convinced he had developers had no idea that an announcement made found the perfect place, Jack walked into the contractor’s office three years later by the federal government would impact the and left a deposit. That was in September 1961. Less than two heart and soul of the neighborhood. years later, he and his wife Sylvia moved in. They are still there, Just days after NASA named Houston as its home for and they are not alone. the Manned Spacecraft Center, a small group from Virginia Along with the Kinzlers, other NASA employees moved traveled to see the place where they would be a part of sending into the neighborhood, including rocket scientists, engineers, a man to the moon and returning him safely to Earth. Jack spacecraft designers, and four of the original Mercury 7 Kinzler was among those visitors from the space agency and, astronauts. More followed and, collectively, they transformed knowing he would be relocating, Jack scouted for prospective their neighborhood. Sharing a common goal at work, the homesites. neighbors became friends; friends became extended family; He found little housing available in the mostly undeveloped and the subdivision evolved into a close-knit community. land near the proposed Center. In every direction, Jack saw Today, Timber Cove continues to host a number of those devastation left by the recent occurrence of Hurricane Carla. But who purchased original lots and then spent the next forty-plus in his search, he located the single entrance to Timber Cove. -
HARVARD COLLEGE OBSERVATORY Cambridge, Massachusetts 02138
E HARVARD COLLEGE OBSERVATORY Cambridge, Massachusetts 02138 INTERIM REPORT NO. 2 on e NGR 22-007-194 LUNAR NOMENCLATURE Donald H. Menzel, Principal Investigator to c National Aeronautics and Space Administration Office of Scientific and Technical Information (Code US) Washington, D. C. 20546 17 August 1970 e This is the second of three reports to be submitted to NASA under Grant NGR 22-007-194, concerned with the assignment I of names to craters on the far-side of the Moon. As noted in the first report to NASA under the subject grant, the Working Group on Lunar Nomenclature (of Commission 17 of the International Astronomical Union, IAU) originally assigned the selected names to features on the far-side of the Moon in a . semi-alphabetic arrangement. This plan was criticized, however, by lunar cartographers as (1) unesthetic, and as (2) offering a practical danger of confusion between similar nearby names, par- ticularly in oral usage by those using the maps in lunar exploration. At its meeting in Paris on June 20 --et seq., the Working Group accepted the possible validity of the second criticism above and reassigned the names in a more or less random order, as preferred by the cartographers. They also deleted from the original list, submitted in the first report to NASA under the subject grant, several names that too closely resembled others for convenient oral usage. The Introduction to the attached booklet briefly reviews the solutions reached by the Working Group to this and several other remaining problems, including that of naming lunar features for living astronauts. -
Impact Craters in the Northern Hemisphere of Mars: Layered Ejecta and Central Pit Characteristics
Impact craters in the northern hemisphere of Mars: Layered ejecta and central pit characteristics Item Type Proceedings; text Authors Barlow, Nadine G. Citation Barlow, N. G. (2006). Impact craters in the northern hemisphere of Mars: Layered ejecta and central pit characteristics. Meteoritics & Planetary Science, 41(10), 1425-1436. DOI 10.1111/j.1945-5100.2006.tb00427.x Publisher The Meteoritical Society Journal Meteoritics & Planetary Science Rights Copyright © The Meteoritical Society Download date 07/10/2021 01:19:21 Item License http://rightsstatements.org/vocab/InC/1.0/ Version Final published version Link to Item http://hdl.handle.net/10150/656190 Meteoritics & Planetary Science 41, Nr 10, 1425–1436 (2006) Abstract available online at http://meteoritics.org Impact craters in the northern hemisphere of Mars: Layered ejecta and central pit characteristics Nadine G. BARLOW Department of Physics and Astronomy, Northern Arizona University, NAU Box 6010, Flagstaff, Arizona 86011–6010, USA E-mail: [email protected] (Received 20 October 2005; revision accepted 20 May 2006) Abstract–Mars Global Surveyor (MGS) and Mars Odyssey data are being used to revise the Catalog of Large Martian Impact Craters. Analysis of data in the revised catalog provides new details on the distribution and morphologic details of 6795 impact craters in the northern hemisphere of Mars. This report focuses on the ejecta morphologies and central pit characteristics of these craters. The results indicate that single-layer ejecta (SLE) morphology is most consistent with impact into an ice-rich target. Double-layer ejecta (DLE) and multiple-layer ejecta (MLE) craters also likely form in volatile-rich materials, but the interaction of the ejecta curtain and target-produced vapor with the thin Martian atmosphere may be responsible for the large runout distances of these ejecta.