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Scientific Rationale and Requirements for a Global Seismic Network on Mars
SCIENTIFIC RATIONALE AND REQUIREMENTS FOR A GLOBAL SEISMIC NETWORK ON MARS MARS Model AR 90 EARTH 180 (NASA-CR-188806) SCIENTIFIC RATIONALE AND N92-14949 REQUIREMENTS FOR A GLOBAL SEISMIC NETWORK ON MARS (Lunar and Planetary Inst.) 48 p CSCL 03B Unclas G3/91 0040098 LPI Technical Report Number 91-02 LUNAR AND PLANETARY INSTITUTE 3303 NASA ROAD 1 HOUSTON TX 77058-4399 LPI/TR-91-02 SCIENTIFIC RATIONALE AND REQUIREMENTS FOR A GLOBAL SEISMIC NETWORK ON MARS Sean C. Solomon, Don L. Anderson, W. Bruce Banerdt, Rhett G. Butler, Paul M. Davis, Frederick K. Duennebier, Yosio Nakamura, Emile A. Okal, and Roger J. Phillips Report of a Workshop Held at Morro Bay, California May 7-9, 1990 Lunar and Planetary Institute 3303 NASA Road 1 Houston TX 77058 LPI Technical Report Number 91-02 LPI/TR-91-02 Compiled in 1991 by the LUNAR AND PLANETARY INSTITUTE The Institute is operated by Universities Space Research Association under Contract NASW-4574 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: Solomon S. C. et al. (1991) Scientific Rationale and Requirements far a Global Seismic Network on Mars. LPI Tech. Rpt. 91-02, Lunar and Planetary Institute, Houston. 51 pp. This report is distributed by: ORDER DEPARTMENT Lunar and Planetary Institute 3303 NASA Road 1 Houston TX 77058-4399 Mail order requestors will be invoiced for the cost of shipping and handling. -
Bibliographyof Space Books Andarticlesfrom Non
https://ntrs.nasa.gov/search.jsp?R=19800016707N 2020-03-11T18:02:45+00:00Zi_sB--rM-._lO&-{/£ 3 1176 00167 6031 HHR-51 NASA-TM-81068 ]9800016707 BibliographyOf Space Books And ArticlesFrom Non-AerospaceJournals 1957-1977 _'C>_.Ft_iEFERENC_ I0_,'-i p,,.,,gvi ,:,.2, , t ,£}J L,_:,._._ •..... , , .2 ,IFER History Office ...;_.o.v,. ._,.,- NASA Headquarters Washington, DC 20546 1979 i HHR-51 BIBLIOGRAPHYOF SPACEBOOKS AND ARTICLES FROM NON-AEROSPACE JOURNALS 1957-1977 John J. Looney History Office NASA Headquarters Washlngton 9 DC 20546 . 1979 For sale by the Superintendent of Documents, U.S. Government Printing Office Washington, D.C. 20402 Stock Number 033-000-0078t-1 Kc6o<2_o00 CONTENTS Introduction.................................................... v I. Space Activity A. General ..................................................... i B. Peaceful Uses ............................................... 9 C. Military Uses ............................................... Ii 2. Spaceflight: Earliest Times to Creation of NASA ................ 19 3. Organlzation_ Admlnlstration 9 and Management of NASA ............ 30 4. Aeronautics..................................................... 36 5. BoostersandRockets............................................ 38 6. Technology of Spaceflight....................................... 45 7. Manned Spaceflight.............................................. 77 8. Space Science A. Disciplines Other than Space Medicine ....................... 96 B. Space Medicine ..............................................119 C. -
Massachusetts Inst. of Thch.) 666 P HC A9NATIF A0L AEOA, CSCD 03F Unclas
lo2 to the " NATIONAL AERONAUTICS AND SPACE ADMINISTRATION Contract NAS9-12334 -APOLLOPASSIVE SEISMICEXPERIMENT PARTICIPATION 'I NASA-CR-151882) LUNAR SEISMOLOGY: THE 1479-17782 INTERNAL STRUCTURE ORHE LOt Ph. Thesis (Massachusetts Inst. of Thch.) 666 p HC A9NATIF A0L AEOA, CSCD 03f Unclas 1 Januarya-19-12 -o 3.0 September .1978 G3/91' 1351 0 M. Nafi Toksbz- Principal Investigator Department of Earth and Planetar SciencesO Massachusetts Institute of Technology Cambridge, Massachusetts 02139 LUNAR SEISMOLOGY: THE INTERNAL STRUCTURE OF THE MOON by -Neal Rodney Goins Submitted to the Department of-Earth -and Planetary Sciences on May 24,.1978, in parti&l .flfillment of the requirements for the degree of Doctor of Philosophy.. ABSTRACT, A primary goal of-the Apollo missions was the exploration and scientific study of the moon. The nature of the lunar interior is of particular interest for comparison with the earth and in studying comparative planetology. The principal experiment designed to study the lunar interior was the passive seismic experiment (PSE) included as part of the science package on missions 12, 14, 15, and 16. Thus seis mologists were provided with a uniqueopportunity ta study the seismicity and seismic characteristics of a second planetary 'bdy and ascertain if analysis methods developed on earth could illuminate the structure of the lunar interior. The lunar seismic data differ from terrestrial data in three major respects. First, the seismic sources are much smaller than on earth, so that no significant information has -been yet obtained for the 4v/ry deep lunar interior. Second, a strong, high Q scattering layer exists on the surface of the moon, resulting in very emergent seismic arrivals, long ringing-codas that obscure secondary (later arriving)-phases., and 'the-destruction of coherent dispersed surface wave trains. -
The Moon and Eclipses
Lecture 10 The Moon and Eclipses Jiong Qiu, MSU Physics Department Guiding Questions 1. Why does the Moon keep the same face to us? 2. Is the Moon completely covered with craters? What is the difference between highlands and maria? 3. Does the Moon’s interior have a similar structure to the interior of the Earth? 4. Why does the Moon go through phases? At a given phase, when does the Moon rise or set with respect to the Sun? 5. What is the difference between a lunar eclipse and a solar eclipse? During what phases do they occur? 6. How often do lunar eclipses happen? When one is taking place, where do you have to be to see it? 7. How often do solar eclipses happen? Why are they visible only from certain special locations on Earth? 10.1 Introduction The moon looks 14% bigger at perigee than at apogee. The Moon wobbles. 59% of its surface can be seen from the Earth. The Moon can not hold the atmosphere The Moon does NOT have an atmosphere and the Moon does NOT have liquid water. Q: what factors determine the presence of an atmosphere? The Moon probably formed from debris cast into space when a huge planetesimal struck the proto-Earth. 10.2 Exploration of the Moon Unmanned exploration: 1950, Lunas 1-3 -- 1960s, Ranger -- 1966-67, Lunar Orbiters -- 1966-68, Surveyors (first soft landing) -- 1966-76, Lunas 9-24 (soft landing) -- 1989-93, Galileo -- 1994, Clementine -- 1998, Lunar Prospector Achievement: high-resolution lunar surface images; surface composition; evidence of ice patches around the south pole. -
WILLIAM MAURICE EWING May 12, 1906-May 4, 1974
NATIONAL ACADEMY OF SCIENCES WILLIAM MAURICE Ew ING 1906—1974 A Biographical Memoir by ED W A R D C . B ULLARD Any opinions expressed in this memoir are those of the author(s) and do not necessarily reflect the views of the National Academy of Sciences. Biographical Memoir COPYRIGHT 1980 NATIONAL ACADEMY OF SCIENCES WASHINGTON D.C. WILLIAM MAURICE EWING May 12, 1906-May 4, 1974 BY EDWARD C. BULLARD* CHILDHOOD, 1906-1922 ILLIAM MAURICE EWING was born on May 12, 1906 in W Lockney, a town of about 1,200 inhabitants in the Texas panhandle. He rarely used the name William and was always known as Maurice. His paternal great-grandparents moved from Kentucky to Livingston County, Missouri, at some date before 1850. Their son John Andrew Ewing, Maurice's grandfather, fought for the Confederacy in the Civil War; while in the army he met two brothers whose family had also come from Kentucky to Missouri before 1850 and were living in De Kalb County. Shortly after the war he married their sister Martha Ann Robinson. Their son Floyd Ford Ewing, Maurice's father, was born in Clarkdale, Mis- souri, in 1879. In 1889 the family followed the pattern of the times and moved west to Lockney, Texas. Floyd Ewing was a gentle, handsome man with a liking for literature and music, whom fate had cast in the unsuitable roles of cowhand, dryland farmer, and dealer in hardware and farm implements. Since he kept his farm through the *This memoir is a corrected and slightly amplified version of one published by the Royal Society in their Biographical Memoirs (21:269-311, 1975). -
Apollo 17 Press
7A-/ a NATIONAL AERONAUTICS AND SPACE ADMINISTRATION Washington. D . C . 20546 202-755-8370 FOR RELEASE: Sunday t RELEASE NO: 72-220K November 26. 1972 B PROJECT: APOLLO 17 (To be launched no P earlier than Dec . 6) R E contents 1-5 6-13 U APOLLC 17 MISSION OBJECTIVES .............14 LAUNCH OPERATIONS .................. 15-17 COUNTDOWN ....................... 18-21 Launch Windows .................. 20 3 Ground Elapsed Time Update ............ 20-21 LAUNCH AND MISSION PROFILE .............. 22-32 Launch Events .................. 24-26 Mission Events .................. 26-28 EVA Mission Events ................ 29-32 APOLLO 17 LANDING SITE ................ 33-36 LUNAR SURFACE SCIENCE ................ 37-55 S-IVB Lunar Impact ................ 37 ALSEP ...................... 37 K SNAP-27 ..................... 38-39 Heat Flow Experiment ............... 40 Lunar Ejecta and Meteorites ........... 41 Lunar Seismic Profiling ............. 41-42 I Lunar Atmospheric Composition Experiment ..... 43 Lunar Surface Gravimeter ............. 43-44 Traverse Gravimeter ............... 44-45 Surface Electrical Properties 45 I-) .......... T Lunar Neutron Probe ............... 46 1 Soil Mechanics .................. 46-47 Lunar Geology Investigation ........... 48-51 Lunar Geology Hand Tools ............. 52-54 Long Term Surface Exposure Experiment ...... 54-55 -more- November 14. 1972 i2 LUNAR ORBITAL SCIENCE ............... .5 6.61 Lunar Sounder ................. .5 6.57 Infrared Scanning Radiometer ......... .5 7.58 Far-Ultraviolet Spectrometer ..........5 -
Aerocenecampusreader FINAL
With Contributions by: Pete Adey ……………….............................Aaron Schuster, The Cosmonaut of the Erotic Future Sasha Engelmann……………………………………….The Cosmic Flight of the Aerocene Gemini Harriet Hawkins………………………………………………………………Imagine… Geoaesthetics Sam Hertz……………………………………………………………………………….The Floating Ear Bronislaw Szerszynski………………………………………………………………Planetary Mobilities Derek McCormack……………………..Sounding: Echoes and Thresholds of Atmospheric Media Andreas Philippopoulos-Mihalopoulos……………........................Withdrawing from Atmosphere Nick Shapiro……………………………………………………………Tim Choy, Air’s Substantiations And from the cosmos of the late Steven Vogel………………………………..Life in Moving Fluids Concept, Edit & Design: Sasha Engelmann and Karina Pragnell Cover Design and Drawings by Irin Siriwattanagul Aerocene Campus NOVEMBER 26, 2016 | EXHIBITION ROAD, LONDON Aerocene comes to Exhibition Road for a multidisciplinary artistic project co-produced by the members of the Exhibition Road Cultural Group, gathering together 17 prestigious cultural and scientific institutions in London, among them, the Serpentine Galleries, Imperial College London, the Natural History Museum, the Science Museum, the Royal Geographical Society, the Victoria and Albert Museum, and the Goethe Institute. How can we hack the Anthropocene to create the Aerocene? The first Aerocene Campus is an open invitation to explore, extend and imagine the Aerocene Epoch through the sculpture of the Aerocene Explorer. The Campus asks how community- driven practices with the Aerocene Explorer can inform environmental, social and mental ecologies in post-Anthropocenic worlds. On November 26th, experts from a wide range of disciplines will gather together for a full day of provocation, discussion, collaboration and 'hacking' to experiment with the Aerocene Explorer and to co-create the Aerocene epoch. To hack is to creatively overcome the limitations of a system, to improve or subvert the intentions of its original form in a spirit of playfulness and exploration. -
This Third Edition Bibliography Lists Books and Teaching Aids Related To
60:CUMENT RESUMB ED 027 215 SE 006 287 Aerospace Bibliography, Third Edition. National Aeronautics and Space Administration, Washingtan, D.C. Repor t No- EP -35 Pub Date (651 Note-68p. EDRS Price f1F-$0.50 HC-$3.50 Descriptors-*Aerospace Technok)gy, *Annotated Bibliographies, Astronomy, *Bibliographies, Physical Sciences, *Science Education, Technology Identifiers-National Aeronautics and Space Administration Thisthirdeditionbibliographylistsbooks and teaching aids related to aeronautics and space. Aeronautics titles are limited toaerospace-related research subjects, and books on astronomy to those direCtly related to space exploration. Also listed are pertinent references like pamphlets, films,film strips, booklets, charts, pictures, periodicals, and sources of in.formation on specific space subjects available from aerospace industry companies. Reading levels for each document are indicated according to primary, intermediate, upper elementary, secondary, and adult or college. (GR) 33' $ t 'k 4 ;(' " ; , othisit-erP-ie I l if= WIN IP , ., k a k ' II U.S. DEPARTMENT OF HEALTH, EDUCATION & WELFARE OFFICE OF EDUCATION THIS DOCUMENT HAS BEEN REPRODUCED EXACTLY AS RECEIVED FROM THE PERSON OR ORGANIZATION ORIGINATING IT.POINTS OF VIEW OR OPINIONS STATED DO NOT NECESSARILY REPRESENT OFF!CIAL OFFICE OF EDUCATION POSITION OR POLICY. 0 ,"'". Al 1011011104- 1,," 1. 1,=z;z0z2i Ent AEROSPACE BIBLIOGRAPHY THIRD EDITION Compiled for Educational Programs Division, Office of Public Affairs NATIONAL AERONAUTICS AND SPACE ADMINISTRATION by National Aerospace -
DTIC) Technical Report Bibliography for Reports Responsive to a Search for Keyword/Subject Term: RADIO RELAY, 1943-1971
Description of document: Defense Technical Information Center (DTIC) Technical Report Bibliography for reports responsive to a search for keyword/subject term: RADIO RELAY, 1943-1971 Requested date: 2013 Released date: 21-October-2013 Posted date: 14-April-2014 Source of document: Defense Technical Information Center (DTIC-R) ATTN: FOIA Requester Service Center 8725 John J. Kingman Road, Suite 0944 Ft. Belvoir, VA 22060-6218 The governmentattic.org web site (“the site”) is noncommercial and free to the public. The site and materials made available on the site, such as this file, are for reference only. The governmentattic.org web site and its principals have made every effort to make this information as complete and as accurate as possible, however, there may be mistakes and omissions, both typographical and in content. The governmentattic.org web site and its principals shall have neither liability nor responsibility to any person or entity with respect to any loss or damage caused, or alleged to have been caused, directly or indirectly, by the information provided on the governmentattic.org web site or in this file. The public records published on the site were obtained from government agencies using proper legal channels. Each document is identified as to the source. Any concerns about the contents of the site should be directed to the agency originating the document in question. GovernmentAttic.org is not responsible for the contents of documents published on the website. From: "Hamilton, Mike CIV DTIC R" Date: Oct 21, 2013 8:22:16 AM Subject: DTIC FOIA 2013-162 Good Morning Attached is information on your below FOIA request. -
Sources of Extraterrestrial Rare Earth Elements: to the Moon and Beyond
resources Article Sources of Extraterrestrial Rare Earth Elements: To the Moon and Beyond Claire L. McLeod 1,* and Mark. P. S. Krekeler 2 1 Department of Geology and Environmental Earth Sciences, 203 Shideler Hall, Miami University, Oxford, OH 45056, USA 2 Department of Geology and Environmental Earth Science, Miami University-Hamilton, Hamilton, OH 45011, USA; [email protected] * Correspondence: [email protected]; Tel.: 513-529-9662; Fax: 513-529-1542 Received: 10 June 2017; Accepted: 18 August 2017; Published: 23 August 2017 Abstract: The resource budget of Earth is limited. Rare-earth elements (REEs) are used across the world by society on a daily basis yet several of these elements have <2500 years of reserves left, based on current demand, mining operations, and technologies. With an increasing population, exploration of potential extraterrestrial REE resources is inevitable, with the Earth’s Moon being a logical first target. Following lunar differentiation at ~4.50–4.45 Ga, a late-stage (after ~99% solidification) residual liquid enriched in Potassium (K), Rare-earth elements (REE), and Phosphorus (P), (or “KREEP”) formed. Today, the KREEP-rich region underlies the Oceanus Procellarum and Imbrium Basin region on the lunar near-side (the Procellarum KREEP Terrain, PKT) and has been tentatively estimated at preserving 2.2 × 108 km3 of KREEP-rich lithologies. The majority of lunar samples (Apollo, Luna, or meteoritic samples) contain REE-bearing minerals as trace phases, e.g., apatite and/or merrillite, with merrillite potentially contributing up to 3% of the PKT. Other lunar REE-bearing lunar phases include monazite, yittrobetafite (up to 94,500 ppm yttrium), and tranquillityite (up to 4.6 wt % yttrium, up to 0.25 wt % neodymium), however, lunar sample REE abundances are low compared to terrestrial ores. -
Inflatable Technology: Using Flexible Materials to Make Large Structures Douglas A
Inflatable technology: using flexible materials to make large structures Douglas A. Litteken* NASA Johnson Space Center, 2101 NASA Parkway, Houston, TX, USA 77058 ABSTRACT Space structures are one of the most critical components for any spacecraft, as they must provide the maximum amount of livable volume with the minimum amount of mass. Deployable structures can be used to gain additional space that would not normally fit under a launch vehicle shroud. This expansion capability allows it to be packed in a small launch volume for launch, and deploy into its fully open volume once in space. Inflatable, deployable structures in particular, have been investigated by NASA since the early 1950’s and used in a number of spaceflight applications. Inflatable satellites, booms, and antennas can be used in low-Earth orbit applications. Inflatable heatshields, decelerators, and airbags can be used for entry, descent and landing applications. Inflatable habitats, airlocks, and space stations can be used for in-space living spaces and surface exploration missions. Inflatable blimps and rovers can be used for advanced missions to other worlds. These applications are just a few of the possible uses for inflatable structures that will continued to be studied as we look to expand our presence throughout the solar system. Keywords: Deployable structures, inflatable structures 1. INTRODUCTION The dream of human exploration beyond our home planet has excited and inspired generations across the world. The dreams of taking vacations to the Moon, visiting cities on Mars, or traveling through black holes to discover new life in other galaxies have been described in fiction stories for decades. -
Lunar Seismology: an Update on Interior Structure Models
Space Science Reviews manuscript No. (will be inserted by the editor) Lunar seismology: An update on interior structure models Raphael F. Garcia · Amir Khan · M´elanie Drilleau · Ludovic Margerin · Taichi Kawamura · Daoyuan Sun · Mark A. Wieczorek · Attilio Rivoldini · Ceri Nunn · Renee C. Weber · Angela G. Marusiak · Philippe Lognonn´e · Yosio Nakamura · Peimin Zhu Received: date / Accepted: date R. F. Garcia (corresponding author) Institut Sup´erieurde l'A´eronautiqueet de l'Espace (ISAE-SUPAERO), Universit´ede Toulouse, 10 Ave E. Belin 31400 Toulouse, France Tel.: +33-561338114 E-mail: [email protected] Institut de Recherche en Astrophysique et Plan´etologie,C.N.R.S., Universit´ede Toulouse, 14 Ave E. Belin, 31400 Toulouse, France A. Khan Institute of Geophysics, ETH Z¨urich, Switzerland. M. Drilleau Universit de Paris, Institut de physique du globe de Paris, CNRS, F-75005 Paris, France L. Margerin Institut de Recherche en Astrophysique et Plan´etologie,C.N.R.S., Universit´ede Toulouse, 14 Ave E. Belin, 31400 Toulouse, France T. Kawamura Institut de Physique du Globe de Paris, Paris, France D. Sun Laboratory of Seismology and Physics of Earths Interior, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China CAS Center for Excellence in Comparative Planetology, Hefei, China M. A. Wieczorek Universit´eC^oted'Azur, Observatoire de la C^oted'Azur, CNRS, Laboratoire Lagrange, Nice, France A. Rivoldini Observatoire Royal de Belgique, 3 Avenue Circulaire, 1050 Bruxelles, Belgique C. Nunn Jet Propulsion Laboratory - California Institute of Technology, Pasadena, U.S.A and Ludwig Maximilian University, Munich, Germany R. C.