Pottery and Mobility: a Functional Analysis of Intermountain Brownware
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Flynn Creek Crater, Tennessee: Final Report, by David J
1967010060 ASTROGEOLOGIC STUDIES / ANNUAL PROGRESS REPORT " July 1, 1965 to July 1, 1966 ° 'i t PART B - h . CRATERINVESTIGATIONS N 67_1_389 N 57-" .]9400 (ACCEC_ION [4U _" EiER! (THRU} .2_ / PP (PAGLS) (CO_ w ) _5 (NASA GR OR I"MX OR AD NUMBER) (_ATEGORY) DEPARTMENT OF THE INTERIOR UNITED STATES GEOLOQICAL SURVEY • iri i i i i iiii i i 1967010060-002 ASTROGEOLOGIC STUDIES ANNUAL PROGRESS REPORT July i, 1965 to July I, 1966 PART B: CRATER INVESTIGATIONS November 1966 This preliminary report is distributed without editorial and technical review for conformity with official standards and nomenclature. It should not be quoted without permission. This report concerns work done on behalf of the National Aeronautics and Space Administration. DEPARTMENT OF THE INTERIOR UNITED STATES GEOLOGICAL SURVEY 1967010060-003 • #' C OING PAGE ,BLANK NO/" FILMED. CONTENTS PART B--CRATER INVESTIGATIONS Page Introduction ........................ vii History and origin of the Flynn Creek crater, Tennessee: final report, by David J. Roddy .............. 1 Introductien ..................... 1 Geologic history of the Flynn Creek crater ....... 5 Origin of the Flynn Creek crater ............ ii Conc lusions ...................... 32 References cited .................... 35 Geology of the Sierra Madera structure, Texas: progress report, by H. G. Wilshire ............ 41_ Introduction ...................... 41 Stratigraphy ...................... 41 Petrography and chemical composition .......... 49 S truc ture ....................... 62 References cited ............. ...... 69 Some aspects of the Manicouagan Lake structure in Quebec, Canada, by Stephen H. Wolfe ................ 71 f Craters produced by missile impacts, by H. J. Moore ..... 79 Introduction ...................... 79 Experimental procedure ................. 80 Experimental results .................. 81 Summary ........................ 103 References cited .................... 103 Hypervelocity impact craters in pumice, by H. J. Moore and / F. -
Lick Observatory Records: Photographs UA.036.Ser.07
http://oac.cdlib.org/findaid/ark:/13030/c81z4932 Online items available Lick Observatory Records: Photographs UA.036.Ser.07 Kate Dundon, Alix Norton, Maureen Carey, Christine Turk, Alex Moore University of California, Santa Cruz 2016 1156 High Street Santa Cruz 95064 [email protected] URL: http://guides.library.ucsc.edu/speccoll Lick Observatory Records: UA.036.Ser.07 1 Photographs UA.036.Ser.07 Contributing Institution: University of California, Santa Cruz Title: Lick Observatory Records: Photographs Creator: Lick Observatory Identifier/Call Number: UA.036.Ser.07 Physical Description: 101.62 Linear Feet127 boxes Date (inclusive): circa 1870-2002 Language of Material: English . https://n2t.net/ark:/38305/f19c6wg4 Conditions Governing Access Collection is open for research. Conditions Governing Use Property rights for this collection reside with the University of California. Literary rights, including copyright, are retained by the creators and their heirs. The publication or use of any work protected by copyright beyond that allowed by fair use for research or educational purposes requires written permission from the copyright owner. Responsibility for obtaining permissions, and for any use rests exclusively with the user. Preferred Citation Lick Observatory Records: Photographs. UA36 Ser.7. Special Collections and Archives, University Library, University of California, Santa Cruz. Alternative Format Available Images from this collection are available through UCSC Library Digital Collections. Historical note These photographs were produced or collected by Lick observatory staff and faculty, as well as UCSC Library personnel. Many of the early photographs of the major instruments and Observatory buildings were taken by Henry E. Matthews, who served as secretary to the Lick Trust during the planning and construction of the Observatory. -
Florida Atlantic University
FLORIDA ATLANTIC UNIVERSITY Commencement Classes d196S -1969 Sunday, June 8, 1969 Two o'Clock THE CAMPUS Boca Raton, Florida !fJrogram Prelude Prelude and Fugue in C. Major- ]. S. Bach Processional Pomp and Circumstance- Edward Elgar B. Graham Ellerbee, Organist Introductions Dr. Clyde R. Burnett University Marshal Invocation The Rev. Donald Barrus United Campus Ministries National Anthem - Key- Sousa Richard Wright Instructor in Music Presiding Dr. Kenneth R. Williams President Florida Atlantic University Address "The Generation of City Builders" Dr. Robert C. Wood Director Joint Center for Urban Studies Massachusetts Institute of Technology Presentation of Baccalaureate Degrees Dr. S. E. Wimberly Vice President for Academic Affairs For the College of Business and Public Administration Dean Robert L. Froemke For the College of Education Dean Robert R. Wiegman For the College of Humanities Dean Jack Suberman For the Department of Ocean Engineering Professor Charles R. Stephan For the College of Science Dean Kenneth M. Michels For the College of Social Science Dean John M. DeGrove Presentation of the Master of Education, Master of Public Administration, Master of Science and Master of Arts Degrees Deans of the Respective Colleges Benediction The Reverend Barrus Recessional Recessional - Martin Shaw The Audience will please remain in their places until the Faculty and Graduates have left the area. 1 THE ORDER OF THE PROCE SS IO N The Marshal of the Colleges The Marshals and Candidates of the College of Business and Public Administration -
LRO and the ESMD/SMD Partnership Lessons Learned
LRO and the ESMD/SMD Partnership Lessons Learned John Keller LRO Project Scientist LRO and the ESMD/SMD Partnership • LRO is a highly successful mission of both exploration and science • ESMD (Exploration Systems Mission Directorate, now part of HEOMD) and SMD cooperated closely for the mission’s success – Joint selection of the measurement teams through a joint A.O. – SMD added participating scientist – LEAG established for community participation, modeled after MEPAG • LRO Mission benefited from the strong leadership of Mike Wargo, the ESMD Chief Lunar Scientist – Advocate in ESMD for science and exploration as co-enablers – Ambassador to lunar science and exploration communities. • Buy-in at the AA and Division Levels was critical. 2 LRO Mission Objectives Safe Landing Sites Space Environment Locate Potential Resources High resolution imagery Energetic particles Hydrogen/water at the lunar poles Global geodetic grid Neutrons Continuous solar energy Topography Mineralogy Rock abundances LRO was initiated as a high-priority Discovery-class mission to enable astronaut return to the Moon Slide - 3 HISTORY I • Jan. 2004: President’s “Visions for Space Exploraon” Speech (men7ons “LRO” as 1st step) • Late Jan. 2004: ESMD and SMD agree to charter an ORDT to define LRO (D. Cooke was key official at ESMD with C. Scolese, SMD) • March 2004: ORDT face-to-face with consensus on priori7es for LRO measurements – Specified 8 cri+cal measurement sets for LRO to achieve (if possible) • June 2004: AO release for LRO payload (jointly by SMD and ESMD) • Dec. -
The Widespread Distribution of Swirls in Lunar Reconnaissance Orbiter Camera Images
EPSC Abstracts Vol. 10, EPSC2015-854, 2015 European Planetary Science Congress 2015 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2015 The Widespread Distribution of Swirls in Lunar Reconnaissance Orbiter Camera Images Brett W. Denevi (1), Mark S. Robinson (2), Aaron K. Boyd (2), and David T. Blewett (1) (1) The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, USA, (2) School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA. Email: [email protected]. 1. Introduction fresh plagioclase-rich materials from their shocked or glassy equivalent in the highlands. Lunar swirls are Lunar swirls, the sinuous high- and low-reflectance characterized by this steep UV slope [11], such that a features that cannot be mentioned without the WAC color composite (415 nm, 321/415 nm, and associated adjective “enigmatic,” are of interest 321/360 nm in red, green, and blue, respectively) because of their link to crustal magnetic anomalies reveals their locations (e.g., Fig. 1). We used this [1,2]. These localized magnetic anomalies create WAC composite sampled at 400 m/pixel as the basis mini-magnetospheres [3,4] and may alter the typical for our mapping, noting the locations and margins of surface modification processes or result in altogether the high-reflectance portions of swirls based on their distinct processes that form the swirls. One UV ratios and 415 nm reflectance values. hypothesis is that magnetic anomalies may provide some degree of shielding from the solar wind [1,2], 3. Distribution of Swirls which could impede space weathering due to solar The WAC-based map (Fig. -
EVA Planetary Science
National Aeronautics and Space Administration Planetary Science Context for EVA EVA Exploration Workshop Kelsey Young, Exploration Scientist | Trevor Graff, Exploration Scientist February 2020 Scientific Drivers for Planetary Exploration LRO: NASA GSFC Conceptual Images Lab MSL: NASA/JPL-Caltech/MSSS OSIRIS-REX: NASA/Univ. AZ/Lockheed Martin • Massive advancements made since Apollo surface missions, but there are still a number of outstanding science questions across all potential targets of interest for human exploration • Areas of interest include geology, geophysics, geochemistry, atmospheres, life-related chemistry, etc. – Varying levels of human interaction – Astrobiology: Planetary Protection Lunar Reconnaissance Orbiter (LRO) Image 400m across Apollo 17 Landing Site Apollo 16 S-IVB Impact Crater LRO Traverse Planning NASA/GSFC/ASU NASA/GSFC/ASU Speyerer et al., 2016 • Jointly funded by ESMD/SMD • Initially operated to select landing sites for future crewed missions before being transferred for science operations • LRO Instrumentation: – CRaTER (Cosmic Ray Telescope for the Effects of Radiation) – DLRE (Diviner Lunar Radiometer Experiment) – LAMP (Lyman-Alpha Mapping Project) – LEND (Lunar Exploration Neutron Detector) – LROC (Lunar Reconnaissance Orbiter Camera) – LOLA (Lunar Orbiter Laser Altimeter) Launched: 18 JUNE 2009 – Mini-RF (Miniature Radio Frequency) Science Enabling Exploration • LRO entering 4th extended mission and 10th year in lunar orbit • Fuel for 7 more years • Global topography at 60 m/pixel • Global coverage at 100 m/pixel • Localized topography at 2.5m/px for 4% of Moon • Global temperature data • Illumination maps of entire surface Dewar Cryptomaria Lunar Interior, Farside Volcanism New Advances in Lunar Science LRO Tour of the Moon in 4K • 5-minute animation that takes the viewer on a virtual tour of our nearest neighbor in space. -
Lunar Magnetic Field Models from Lunar Prospector and SELENE/Kaguya Along-Track Magnetic Field Gradients
Downloaded from orbit.dtu.dk on: Oct 08, 2021 Lunar magnetic field models from Lunar Prospector and SELENE/Kaguya along-track magnetic field gradients Ravat, D.; Purucker, M.E.; Olsen, N. Published in: Journal of Geophysical Research: Planets Link to article, DOI: 10.1029/2019JE006187 Publication date: 2020 Document Version Publisher's PDF, also known as Version of record Link back to DTU Orbit Citation (APA): Ravat, D., Purucker, M. E., & Olsen, N. (2020). Lunar magnetic field models from Lunar Prospector and SELENE/Kaguya along-track magnetic field gradients. Journal of Geophysical Research: Planets, 125(7), [e2019JE006187]. https://doi.org/10.1029/2019JE006187 General rights Copyright and moral rights for the publications made accessible in the public portal are retained by the authors and/or other copyright owners and it is a condition of accessing publications that users recognise and abide by the legal requirements associated with these rights. Users may download and print one copy of any publication from the public portal for the purpose of private study or research. You may not further distribute the material or use it for any profit-making activity or commercial gain You may freely distribute the URL identifying the publication in the public portal If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. RESEARCH ARTICLE Lunar Magnetic Field Models From Lunar Prospector and 10.1029/2019JE006187 SELENE/Kaguya Along‐Track -
THE GEOCHEMICAL NEWS Newsletter of the Geochemical Society in Cooperation with the European Association of Geochemistry
January 2005 1 THE GEOCHEMICAL NEWS Newsletter of The Geochemical Society in cooperation with The European Association of Geochemistry In This Issue... An Interview with David Des Marais Geochemistry at Oak Ridge National Laboratory January 2005 Number 122 Newsletter of the Geochemical Society ISSN 0016-7010 2 The Geochemical News EAG OFFICERS - 2005 PRESIDENT Terry Seward, ETH, Zurich PRESIDENT ELECT Bruce Yardley, Leeds, UK OUTGOING PRESIDENT Francis Albarede, Lyon, France TREASURER Catherine Chauvel, Grenoble, France SECRETARY Mark Hodson, Reading, UK EAG COMMITTEE THE GEOCHEMICAL SOCIETY MIRA BAR-MATTHEWS, ISREAL Larryn Diamond, Switzerland Jérôme GAILLARDET, FRANCE Alex Halliday, Switzerland SUSAN STIPP, DENMARK Riccardo Vannucci, Italy The Geochemical Society is a nonprofit scientific society founded to en- GERHARD WORNER, GERMANY Bruce Yardley, UK courage the application of chemistry to the solution of geological and cosmologi- cal problems. Membership is international and diverse in background, encom- passing such fields as organic geochemistry, high- and low-temperature geochem- THE GEOCHEMICAL NEWS istry, petrology, meteoritics, fluid-rock interaction, and isotope geochemistry. The Society produces a Special Publications Series, The Geochemical News (this January 2005 quarterly newsletter), the Reviews in Mineralogy and Geochemistry Series (jointly with the Mineralogical Society of America), the journal Geochimica et Editors Cosmochimica Acta (jointly with the Meteoritical Society), and co-publishes the Johnson R. Haas and Carla M. Koretsky electronic journal G3 (jointly with the American Geophysical Union: AGU); grants Department of Geosciences the V.M. Goldschmidt, F.W. Clarke and Clair C. Patterson Awards, and, jointly Western Michigan University with the European Association of Geochemistry (EAG), the Geochemistry Fel- Kalamazoo, MI 49008 lows title; sponsors the V.M. -
The Surface of Mars 1. Cratered Terrains
VOL. 76, NO. 2 JOURNAL OF GEOPHYSICAL RESEARCH JANUARY 10, 1971 The Surface of Mars i. Cratered Terrains • BRUCEC. MURRAY,LAURENCE A. SODERBLOM, ROBERTP. SHARP,AND JAMESA. CUTTS Division of GeologicalSciences California Institute of Technology,Pasadena 91109 Mariner 6 and 7 pictures show that craters are the dominant landform on Mars and that their occurrenceis not correlated uniquely with latitude, elevation, or albedo markings. Two distinct morphological classesare recognized: small bowl-shaped and large flat-bottomed. The former showlittle evidenceof modifications,whereas the latter appear generally more modified than hmar upland cratersof comparablesize. A regionalmaria/uplands dichotomylike the moon has not yet been recognized on Mars. Crater modification on Mars has involved much greater horizontal redistribution of material than in the lunar uplands. It is possiblethat there are erosionalprocesses only infrequently active. Analysisof the natures and fluxesof bodiesthat have probably impacted the moon and Mars leads to the likelihood that most of the large flat-bottomed craters on Mars have survived from the final phasesof planetary accretion. Significant crater modification, how- ever, has taken place more recently on Mars. Inasmuch as the present small bowl-shaped craters evidence little modification, the postaccretion crater-modification processon Mars may have been primarily episodic rather than continuous. The size-frequency distribution of impacting bodiesthat produced the present small Martian bowl-shapedcraters differs from that responsible for post-mare primary impacts on the moon by a marked deficiency of large bodies. Survival of crater topography from the end of planetary accretion would make any hypothetical earthlike phasewith primitive oceansthere unlikely. The traditional view of Mars as an earthlike planetary neighbor in terms of its surface history is not supported by the picture data. -
Quarterly Journal of the ALPO
ISSN-0039-2502 Journal of the Association of Lunar & Planetary Observers The Strolling Astronomer Volume 59, Number 1, Winter 2017 Now in Portable Document Format (PDF) for Macintosh and PC-compatible computers Online and in COLOR at http://www.alpo-astronomy.org The Super Full Moon of November (see page 2 for details) The Strolling Astronomer Journal of the Inside the ALPO Point of View: Your ALPO! ................................ 2 Association of Lunar & News of General Interest .................................. 3 Our Cover ....................................................... 3 Planetary Observers Special Announcement from the The Strolling Astronomer ALPO Venus Section ................................ 4 Digital Journal of the ALPO Now Available to All ALPO Members ..................................... 4 Volume 59, No.1, Winter 2017 This issue published in December 2016 for distribution in both Update: The ALPO Publications Section portable document format (pdf) and hardcopy format. Gallery ........................................................ 4 ALPO Interest Section Reports ........................ 6 This publication is the official journal of the Association of Lunar & ALPO Observing Section Reports .................... 7 Planetary Observers (ALPO). Obituary: Winifred Sawtell Cameron, 1918–2016 ............................................... 20 The purpose of this journal is to share observation reports, opinions, Contributors and Newest Members ................ 21 and other news from ALPO members with other members and the professional astronomical community. Papers & Presentations © 2016, Association of Lunar and Planetary Observers (ALPO). The A Report on Carrington Rotations 2178 and ALPO hereby grants permission to educators, academic libraries and 2179 (2016-06-06 to 2016-07-31) ................ 25 the professional astronomical community to photocopy material for ALPO Observations of Venus During the educational or research purposes as required. There is no charge for 2012-2013 Western (Morning) Apparition ... -
LUNAR SURFACE REMOTE SENSING 7:00 P.M
Lunar and Planetary Science XXXVI (2005) sess73.pdf Thursday, March 17, 2005 POSTER SESSION II: LUNAR SURFACE REMOTE SENSING 7:00 p.m. Fitness Center Okada T. Arai T. Hosono K. Shirai K. Yamamoto Y. Ogawa K. Kato M. First X-Ray Observation of Lunar Farside from Hayabusa X-Ray Spectrometer [#1175] The X-ray fluorescence spectrometer or XRS on-board Hayabusa has observed the first X-ray emission off the surface of lunar farside on May 17 in 2004, just before the Earth swing-by. The data indicates that the overall average composition of lunar farside is consistent with anorthositic crust. Garrick-Bethell I. Zuber M. T. An Indigenous Origin for the South Pole-Aitken Basin Thorium Anomaly [#2372] Based on analysis of a combination of datasets we propose that the thorium anomaly in the northwest corner of the South Pole-Aitken basin most likely reflects an indigenous process. Thompson T. W. Campbell B. A. Unusual Radar Backscatter Properties Along the Northern Rim of Imbrium Basin [#1535] The terra along the northern rim of Imbrium has unusually low radar backscatter, which is 2–4 times lower than other terra. This may be attributed to a mantle of pyroclastics in this area. Campbell B. A. Campbell D. B. Chandler J. New 70-cm Radar Mapping of the Moon [#1385] We are collecting a new high-resolution 70-cm radar map of the lunar nearside. Saito M. Takata T. Matsushita M. Chishima T. Ikeda Y. Hirao N. Iijima Y. Ground-based Observation of Lunar Surface by Lunar VIS/NIR Spectral Imager [#1513] Ground-based Lunar VIS/NIR Spectral Imager is developed in order to obtain 3 dimensional spectral and spatial images of the nearside of the moon. -
I N S I D E T H I S I S S
February / février 2008 Volume/volume 102 Number/numéro 1 [728] This Issue's Winning Astrophoto! FEATURING A FULL COLOUR SECTION! The Journal of the Royal Astronomical Society of Canada Cassiopeia Rising Over the Plaskett by Charles Banville, Victoria Centre. This is a montage of two pictures I took using a Canon 20Da and a Canon EF 17-40mm f/4L lens. The foreground image was acquired at the Dominion Astrophysical Observatory in Victoria on 2007 July 26. That evening the Plaskett Dome was illuminated by a bright 12-day-old Moon. The star trails were created using 87 light frames of 1 minute each taken from Cattle Point on 2007 August 8. Le Journal de la Société royale d’astronomie du Canada [Editor’s Note: The two-member team of Dietmar Kupke and Paul Mortfield of the Toronto Centre selected this late-entry image from among the 30 or so entries to the “Own the Back Cover” con- test. Thanks to all the submitters. We welcome further entries, so don’t delay – send in yours now! INSIDE THIS ISSUE Watch the back cover of the April issue for the next winner.] One Hundred Editions of the Observer's Handbook · Seriously Seeking Ceres! Mont-Mégantic Dark-Sky Reserve Conference, 2007 September 19-21 Duplicity of ZC1042: My First Double-Star Discovery In Memory of Gertrude Jean Southam Building for the International Year of Astronomy (IYA2009) THE ROYAL ASTRONOMICAL SOCIETY OF CANADA February / février 2008 NATIONAL OFFICERS AND COUNCIL FOR 2007-2008/CONSEIL ET ADMINISTRATEURS NATIONAUX Honorary President Robert Garrison, Ph.D., Toronto President Scott Young, B.Sc., Winnipeg Vol.