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Mars Express Orbiter Radio Science
MaRS: Mars Express Orbiter Radio Science M. Pätzold1, F.M. Neubauer1, L. Carone1, A. Hagermann1, C. Stanzel1, B. Häusler2, S. Remus2, J. Selle2, D. Hagl2, D.P. Hinson3, R.A. Simpson3, G.L. Tyler3, S.W. Asmar4, W.I. Axford5, T. Hagfors5, J.-P. Barriot6, J.-C. Cerisier7, T. Imamura8, K.-I. Oyama8, P. Janle9, G. Kirchengast10 & V. Dehant11 1Institut für Geophysik und Meteorologie, Universität zu Köln, D-50923 Köln, Germany Email: [email protected] 2Institut für Raumfahrttechnik, Universität der Bundeswehr München, D-85577 Neubiberg, Germany 3Space, Telecommunication and Radio Science Laboratory, Dept. of Electrical Engineering, Stanford University, Stanford, CA 95305, USA 4Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91009, USA 5Max-Planck-Instuitut für Aeronomie, D-37189 Katlenburg-Lindau, Germany 6Observatoire Midi Pyrenees, F-31401 Toulouse, France 7Centre d’etude des Environnements Terrestre et Planetaires (CETP), F-94107 Saint-Maur, France 8Institute of Space & Astronautical Science (ISAS), Sagamihara, Japan 9Institut für Geowissenschaften, Abteilung Geophysik, Universität zu Kiel, D-24118 Kiel, Germany 10Institut für Meteorologie und Geophysik, Karl-Franzens-Universität Graz, A-8010 Graz, Austria 11Observatoire Royal de Belgique, B-1180 Bruxelles, Belgium The Mars Express Orbiter Radio Science (MaRS) experiment will employ radio occultation to (i) sound the neutral martian atmosphere to derive vertical density, pressure and temperature profiles as functions of height to resolutions better than 100 m, (ii) sound -
Quantitative Planetary Image Analysis Via Machine Learning
Tina Memo No. 2013-008 External, PhD Thesis, University of Manchester Quantitative Planetary Image Analysis via Machine Learning. Paul Tar Last updated 25 / 09 / 2014 Centre for Imaging Sciences, Medical School, University of Manchester, Stopford Building, Oxford Road, Manchester, M13 9PT. Quantitative Planetary Image Analysis via Machine Learning A thesis submitted to the University of Manchester for the degree of PhD in the faculty of Engineering and Physical Sciences 2014 Paul D. Tar School of Earth, Atmospheric and Environmental Sciences 2 Contents 1 Introduction 19 1.1 Theriseofimagingfromspace. ...... 19 1.1.1 Historicalimages ............................... 20 1.1.2 Contemporaryimages . 20 1.1.3 Futureimages.................................. 21 1.2 Sciencecase ..................................... .. 22 1.2.1 Lunarscience .................................. 22 1.2.2 Martianscience ................................ 22 1.3 Imageinterpretation ............................. ..... 23 1.3.1 Manualanalysis................................ 24 1.3.2 Automatedanalysis.............................. 24 1.4 Measurements.................................... .. 25 1.4.1 Quantitative measurements and The Scientific Method . .......... 26 1.4.2 Theroleofstatistics . ... 27 1.4.3 Assumptionsandapproximations . .... 29 1.5 Argumentforquantitativeautomation . ........ 30 1.6 Criteriaforaquantitativesystem . ......... 31 1.7 Thesisoutline ................................... ... 32 2 Literature Review 35 2.1 Representations ................................ -
Analysis of Photography and Visual Observations
CASE c o ANALYSIS OF PHOTOGRAPHY AND VISUAL OBSERVATIONS NATIONAL AERONAUTICS AN_SP.A_E NASA SP-232 ANALYSIS OF PHOTOGRAPHY AND VISUAL OBSERVATIONS COMPILED BY NASA MANNED SPACECRAFT CENTER Scientific and Technical ln[ormation Office 19"I Is, S._. NATIONAL AERONAUTICS AND SPACE ADMINISTRATION Washington, D.C. For sale by the Superintendent of Documents, U.S. Government Printing Office, Washington, D.C. 20402 Price $4.25 Library of Congress Catalog Card Number 72-606239 Foreword The Apollo 10 mission was a vital step toward the national goal of landing men on the Moon and returning them safely to Earth. This mission used the first complete Apollo spacecraft flown in lunar orbit and took men closer to the Moon than ever before. The mission clearly demonstrated that the Nation was ready to embark with the Apollo 11 crew on the voyage that has been the dream of men for thousands of years. Each Apollo lunar mission acquires photographs of areas on the Moon never before seen in such great detail. This report provides only a small sample of the types of analysis that can be performed with this photography. Even more important, however, this report provides scientists throughout the world with a knowledge of what new lunar photography is available and how the photograph can be obtained. It is hoped that more extensive analysis of this photography will continue, and it is certain that the photographs will be used for many decadesl RICHARD J. ALLENBY 01_ice of Manned Space Flight 111 Contents Page INTRODUCTION ........................................ vii Jamcs H. Sasser CHAPTER 1. VISUAL OBSERVATIONS ............. -
Lunar Orbiter Photographic Atlas of the Near Side of the Moon Charles J
Lunar Orbiter Photographic Atlas of the Near Side of the Moon Charles J. Byrne Lunar Orbiter Photographic Atlas of the Near Side of the Moon Charles J. Byrne Image Again Middletown, NJ USA Cover illustration: Earth-based photograph of the full Moon from the “Consolidated Lunar Atlas” on the Website of the Lunar and Planetary Institute. British Library Cataloging-in-Publication Data Byrne, Charles J., 1935– Lunar Orbiter photographic atlas of the near side of the Moon 1. Lunar Orbiter (Artificial satellite) 2. Moon–Maps 3. Moon–Photographs from space I. Title 523.3 0223 ISBN 1852338865 Library of Congress Cataloging-in-Publication Data Byrne, Charles J., 1935– Lunar Orbiter photographic atlas of the near side of the Moon : with 619 figures / Charles J. Byrne. p. cm. Includes bibliographical references and index. ISBN 1-85233-886-5 (acid-free paper) 1. Moon–Maps. 2. Moon–Photographs from space. 3. Moon–Remote-sensing images. 4. Lunar Orbiter (Artificial satellite) I. Title. G1000.3.B9 2005 523.3 022 3–dc22 2004045006 Additional material to this book can be downloaded from http://extras.springer.com. ISBN 1-85233-886-5 Printed on acid-free paper. © 2005 Springer-Verlag London Limited Apart from any fair dealing for the purposes of research or private study, or criticism, or review, as permitted under the Copyright, Designs and Patents Act 1988, this publication may only be repro- duced, stored or transmitted, in any form or by any means, with the prior permission in writing of the publishers, or in the case of reprographic reproduction in accordance with the terms of licenses issued by the Copyright Licensing Agency. -
Jjmonl 1402.Pmd
alactic Observer GJohn J. McCarthy Observatory Volume 7, No. 2 February 2014 Beneath the Clouds: An in-depth look at Jupiter's wacky weather machine. See inside, pages 6 and 20. The John J. McCarthy Observatory Galactic Observer New Milford High School Editorial Committee 388 Danbury Road Managing Editor New Milford, CT 06776 Bill Cloutier Phone/Voice: (860) 210-4117 Production & Design Phone/Fax: (860) 354-1595 www.mccarthyobservatory.org Allan Ostergren Website Development JJMO Staff Marc Polansky It is through their efforts that the McCarthy Observatory Technical Support has established itself as a significant educational and Bob Lambert recreational resource within the western Connecticut Dr. Parker Moreland community. Steve Barone Jim Johnstone Colin Campbell Carly KleinStern Dennis Cartolano Bob Lambert Mike Chiarella Roger Moore Route Jeff Chodak Parker Moreland, PhD Bill Cloutier Allan Ostergren Cecilia Dietrich Marc Polansky Dirk Feather Joe Privitera Randy Fender Monty Robson Randy Finden Don Ross John Gebauer Gene Schilling Elaine Green Katie Shusdock Tina Hartzell Jon Wallace Tom Heydenburg Paul Woodell Amy Ziffer In This Issue OUT THE WINDOW ON YOUR LEFT .................................... 4 JUPITER AND ITS MOONS ................................................ 20 SCHILLER TO HANSTEEN .................................................. 5 TRANSIT OF THE JUPITER'S RED SPOT .............................. 17 LRO IMAGES CHANG'E 3 LANDING SITE ........................... 6 SUNRISE AND SUNSET .................................................... -
A Guideline for a Sustainable Lunar Base Design for Constructed in Lunar Lava Tubes and Their Vertical Skylights
50th International Conference on Environmental Systems ICES-2021-186 12-15 July 2021 A Guideline for a Sustainable Lunar Base Design for Constructed in Lunar Lava Tubes and Their Vertical Skylights Masato Sakurai1, Asuka Shima2, Isao Kawano3, Junichi Haruyama4 Japan Aerospace Exploration Agency (JAXA), Chofu-shi, Tokyo, 182-8522, Japan. and Hiroyuki Miyajima5 International University of Health and Welfare, Narita Campus 1, 4-3, Kōzunomori, Narita, Chiba, 286-8686 Japan The lunar surface is a hostile environment subject to harmful radiation and meteorite impacts. A recently discovered lava tube avoids these risks and, as it undergoes only slight temperature changes, it is a promising location for constructing a lunar base. JAXA engages in research in regenerative ECLSS (Environmental Control Life Support Systems), particularly addressing water and air recycling and treating organic waste. Overcoming these challenges is essential for long-term lunar habitation. This paper presents a guideline for a sustainable lunar base design. Nomenclature ECLSS = Environmental Control Life Support System HTV = H-II Transfer Vehicle ISS = International Space Station JAXA = Japan Aerospace Exploration Agency JSASS = Japan Society for Aeronautical and Space Science MHH = Marius Hills Hole MIH = Mare Ingenii Hole MTH = Mare Tranquillitatis Hole SELENE = Selenological and Engineering Explorer UZUME = Unprecedented Zipangu Underworld of the Moon Exploration (name of the research group for vertical holes) SDGs = Sustainable Development Goals SELENE = Selenological and Engineering Explorer I. Introduction uture space exploration will extend beyond low Earth orbit and dramatically expand in scope. In particular, F industrial activities are planned for the Moon with the development of infrastructure that includes lunar bases. This paper summarizes our study of the construction of a crewed permanent settlement, which will be essential to support long-term habitation, resource utilization, and industrial activities on the Moon. -
Radar Remote Sensing of Pyroclastic Deposits in the Southern Mare Serenitatis and Mare Vaporum Regions of the Moon Lynn M
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 114, E11004, doi:10.1029/2009JE003406, 2009 Click Here for Full Article Radar remote sensing of pyroclastic deposits in the southern Mare Serenitatis and Mare Vaporum regions of the Moon Lynn M. Carter,1 Bruce A. Campbell,1 B. Ray Hawke,2 Donald B. Campbell,3 and Michael C. Nolan4 Received 21 April 2009; revised 12 July 2009; accepted 3 August 2009; published 5 November 2009. [1] We use polarimetric radar observations to study the distribution, depth, and embedded rock abundance of nearside lunar pyroclastic deposits. Radar images were obtained for Mare Vaporum and the southern half of Mare Serenitatis; the imaged areas contain the large Rima Bode, Mare Vaporum, Sulpicius Gallus, and Taurus-Littrow pyroclastic deposits. Potential pyroclastic deposits at Rima Hyginus crater, the Tacquet Formation, and a dome in Mare Vaporum are also included. Data were acquired at S band (12.6 cm wavelength) using Arecibo Observatory and the Green Bank Telescope in a bistatic configuration. The S band images have resolutions between 20 and 100 m/pixel. The pyroclastic deposits appear dark to the radar and have low circular polarization ratios at S band wavelengths because they are smooth, easily penetrable by radar waves, and generally contain few embedded blocks. Changes in circular polarization ratio (CPR) across some of the pyroclastic deposits show areas with increased rock abundance as well as deposits that are shallower. Radar backscatter and CPR maps are used to identify fine-grained mantling deposits in cases where optical and near-infrared data are ambiguous about the presence of pyroclastics. -
Alactic Observer Gjohn J
alactic Observer GJohn J. McCarthy Observatory Volume 5, No. 2 February 2012 Belly of the Beast At the center of the Milky Way galaxy, a gas cloud is on a perilous journey into a supermassive black hole. As the cloud stretches and accelerates, it gives away the location of its silent predator. For more information , see page 9 inside, or go to http://www.nasa.gov/ centers/goddard/news/topstory/2008/ blackhole_slumber.html. Credit: NASA/CXC/MIT/Frederick K. Baganoff et al. The John J. McCarthy Observatory Galactic Observvvererer New Milford High School Editorial Committee 388 Danbury Road Managing Editor New Milford, CT 06776 Bill Cloutier Phone/Voice: (860) 210-4117 Production & Design Phone/Fax: (860) 354-1595 Allan Ostergren www.mccarthyobservatory.org Website Development John Gebauer JJMO Staff Marc Polansky It is through their efforts that the McCarthy Observatory has Josh Reynolds established itself as a significant educational and recreational Technical Support resource within the western Connecticut community. Bob Lambert Steve Barone Allan Ostergren Dr. Parker Moreland Colin Campbell Cecilia Page Dennis Cartolano Joe Privitera Mike Chiarella Bruno Ranchy Jeff Chodak Josh Reynolds Route Bill Cloutier Barbara Richards Charles Copple Monty Robson Randy Fender Don Ross John Gebauer Ned Sheehey Elaine Green Gene Schilling Tina Hartzell Diana Shervinskie Tom Heydenburg Katie Shusdock Phil Imbrogno Jon Wallace Bob Lambert Bob Willaum Dr. Parker Moreland Paul Woodell Amy Ziffer In This Issue THE YEAR OF THE SOLAR SYSTEM ................................ 4 SUNRISE AND SUNSET .................................................. 11 OUT THE WINDOW ON YOUR LEFT ............................... 5 ASTRONOMICAL AND HISTORICAL EVENTS ...................... 11 FRA MAURA ................................................................ 5 REFERENCES ON DISTANCES ....................................... -
EXPLORING SUBSURFACE LUNAR VOIDS USING SURFACE GRAVIMETRY. Kieran A. Carroll, Da- Vid Hatch2, R. Ghent3, S. Stanley3, N. Urbancic3, Marie-Claude Williamson, W.B
46th Lunar and Planetary Science Conference (2015) 1746.pdf EXPLORING SUBSURFACE LUNAR VOIDS USING SURFACE GRAVIMETRY. Kieran A. Carroll, Da- vid Hatch2, R. Ghent3, S. Stanley3, N. Urbancic3, Marie-Claude Williamson, W.B. Garry4, Manik Talwani5 1Gedex Inc., 407 Matheson Blvd. East, Mississauga, Ontario, Canada L4Z 2H2, [email protected], 2Gedex Inc., 3University of Toronto, 4NASA GSFC, 5Rice University. Introduction: Surface gravimetry is a standard been found to be linear but discontinuous…the space terrestrial geophysics exploration technique. As noth- between such features likely represents uncollapsed ing blocks gravity, this approach can detect subsurface tube.” structures with contrasting densities, both shallow and The structure of these voids is currently unknown, deep. Recently-collected high-resolution imagery of being unobservable via imagery from orbit. Lava tube the Moon has identified numerous pits, indicative of voids presumably might be like terrestrial lava tubes -- subsurface voids. Here we analyze the anomalous - long, linear or sinuous tunnels. In [5], Wagner et al. gravity signal expected at the Moon’s surface due to speculate that “a complex plumbing system may form both localized voids and more-extensive lava tubes, in some impact melt deposits,” and that “where multi- and find that the signal can be large enough to be ple pits were found in a single pond, the pits often oc- measured with Lunar-compatible gravimeters. A po- cur in one or more small regions (~2-5 km square) tential near-term Lunar surface survey of a mare pit within the melt deposit…occasionally, several pits crater in Lacus Mortis is discussed. occur within tens of meters of each other, indicating a possible subsurface connection.” Presumably some Lunar Lava Tubes and Other Subsurface other Lunar subsurface voids might instead be much Voids: Lava tubes can form when an exposed magma more compact, resulting from the draining of a single flow cools at its top surface, forming a solid “lid” over small melt pond. -
Mapping the Surveyor III Crater Large-Scale Maps May Be Produced from Lunar Oribiter Photographs
FIG. 1. The Surveyor I II Crater. CHARLES W. SHULL t LYNN A. SCHENK U. S. Army TOPOCOM Washington, D. C.20315 Mapping the Surveyor III Crater large-scale maps may be produced from lunar Oribiter photographs (Abstract on next page) INRODUCTlON Because of the inclination of the camera, lunar features were viewed more clearly than URVEYOR III spacecraft was launched Son April 17, 1967 toward the moon on a would have been possible on flat terrain. mission to explore possible Apollo landing This crater, then, became an object of in sites. On April 19 the Surveyor landed on the tense interest to the scientific community, moon's Ocean of Storms and almost imme especially to astrogeologists who had the diately began transmitting television pictures unique opportunity of observing high quality back to Earth. When the lunar day ended pictures of the interior of a lunar crater for on May 3, over 6,300 photographs had been the first time. Because of this unusual characteristic, the received from Surveyor III by the Jet Pro pulsion Laboratory.* ational Aeronautics and Space Administra vVhen the spacecraft landed, it came to tion (NASA) requested that the Department of Defense prepare two maps of the crater rest on the inside slope of crater giving it a 12.40 tilt from the local vertical (Figure 1). and surrounding areas. The request was for a photo mosaic at 1 :2,000 scale with 10-meter t Presented at the Annual Convention of the contours and a shaded relief map with con American Society of Photogrammetry in Washing tours at the smallest interval possible. -
Astronomy 2008 Index
Astronomy Magazine Article Title Index 10 rising stars of astronomy, 8:60–8:63 1.5 million galaxies revealed, 3:41–3:43 185 million years before the dinosaurs’ demise, did an asteroid nearly end life on Earth?, 4:34–4:39 A Aligned aurorae, 8:27 All about the Veil Nebula, 6:56–6:61 Amateur astronomy’s greatest generation, 8:68–8:71 Amateurs see fireballs from U.S. satellite kill, 7:24 Another Earth, 6:13 Another super-Earth discovered, 9:21 Antares gang, The, 7:18 Antimatter traced, 5:23 Are big-planet systems uncommon?, 10:23 Are super-sized Earths the new frontier?, 11:26–11:31 Are these space rocks from Mercury?, 11:32–11:37 Are we done yet?, 4:14 Are we looking for life in the right places?, 7:28–7:33 Ask the aliens, 3:12 Asteroid sleuths find the dino killer, 1:20 Astro-humiliation, 10:14 Astroimaging over ancient Greece, 12:64–12:69 Astronaut rescue rocket revs up, 11:22 Astronomers spy a giant particle accelerator in the sky, 5:21 Astronomers unearth a star’s death secrets, 10:18 Astronomers witness alien star flip-out, 6:27 Astronomy magazine’s first 35 years, 8:supplement Astronomy’s guide to Go-to telescopes, 10:supplement Auroral storm trigger confirmed, 11:18 B Backstage at Astronomy, 8:76–8:82 Basking in the Sun, 5:16 Biggest planet’s 5 deepest mysteries, The, 1:38–1:43 Binary pulsar test affirms relativity, 10:21 Binocular Telescope snaps first image, 6:21 Black hole sets a record, 2:20 Black holes wind up galaxy arms, 9:19 Brightest starburst galaxy discovered, 12:23 C Calling all space probes, 10:64–10:65 Calling on Cassiopeia, 11:76 Canada to launch new asteroid hunter, 11:19 Canada’s handy robot, 1:24 Cannibal next door, The, 3:38 Capture images of our local star, 4:66–4:67 Cassini confirms Titan lakes, 12:27 Cassini scopes Saturn’s two-toned moon, 1:25 Cassini “tastes” Enceladus’ plumes, 7:26 Cepheus’ fall delights, 10:85 Choose the dome that’s right for you, 5:70–5:71 Clearing the air about seeing vs. -
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.