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Volcanic History of the Imbrium Basin: a Close-Up View from the Lunar Rover Yutu
Volcanic history of the Imbrium basin: A close-up view from the lunar rover Yutu Jinhai Zhanga, Wei Yanga, Sen Hua, Yangting Lina,1, Guangyou Fangb, Chunlai Lic, Wenxi Pengd, Sanyuan Zhue, Zhiping Hef, Bin Zhoub, Hongyu Ling, Jianfeng Yangh, Enhai Liui, Yuchen Xua, Jianyu Wangf, Zhenxing Yaoa, Yongliao Zouc, Jun Yanc, and Ziyuan Ouyangj aKey Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China; bInstitute of Electronics, Chinese Academy of Sciences, Beijing 100190, China; cNational Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China; dInstitute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China; eKey Laboratory of Mineralogy and Metallogeny, Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, Guangzhou 510640, China; fKey Laboratory of Space Active Opto-Electronics Technology, Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, China; gThe Fifth Laboratory, Beijing Institute of Space Mechanics & Electricity, Beijing 100076, China; hXi’an Institute of Optics and Precision Mechanics, Chinese Academy of Sciences, Xi’an 710119, China; iInstitute of Optics and Electronics, Chinese Academy of Sciences, Chengdu 610209, China; and jInstitute of Geochemistry, Chinese Academy of Science, Guiyang 550002, China Edited by Mark H. Thiemens, University of California, San Diego, La Jolla, CA, and approved March 24, 2015 (received for review February 13, 2015) We report the surface exploration by the lunar rover Yutu that flows in Mare Imbrium was obtained only by remote sensing from landed on the young lava flow in the northeastern part of the orbit. On December 14, 2013, Chang’e-3 successfully landed on the Mare Imbrium, which is the largest basin on the nearside of the young and high-Ti lava flow in the northeastern Mare Imbrium, Moon and is filled with several basalt units estimated to date from about 10 km south from the old low-Ti basalt unit (Fig. -
Copyrighted Material
Index Abulfeda crater chain (Moon), 97 Aphrodite Terra (Venus), 142, 143, 144, 145, 146 Acheron Fossae (Mars), 165 Apohele asteroids, 353–354 Achilles asteroids, 351 Apollinaris Patera (Mars), 168 achondrite meteorites, 360 Apollo asteroids, 346, 353, 354, 361, 371 Acidalia Planitia (Mars), 164 Apollo program, 86, 96, 97, 101, 102, 108–109, 110, 361 Adams, John Couch, 298 Apollo 8, 96 Adonis, 371 Apollo 11, 94, 110 Adrastea, 238, 241 Apollo 12, 96, 110 Aegaeon, 263 Apollo 14, 93, 110 Africa, 63, 73, 143 Apollo 15, 100, 103, 104, 110 Akatsuki spacecraft (see Venus Climate Orbiter) Apollo 16, 59, 96, 102, 103, 110 Akna Montes (Venus), 142 Apollo 17, 95, 99, 100, 102, 103, 110 Alabama, 62 Apollodorus crater (Mercury), 127 Alba Patera (Mars), 167 Apollo Lunar Surface Experiments Package (ALSEP), 110 Aldrin, Edwin (Buzz), 94 Apophis, 354, 355 Alexandria, 69 Appalachian mountains (Earth), 74, 270 Alfvén, Hannes, 35 Aqua, 56 Alfvén waves, 35–36, 43, 49 Arabia Terra (Mars), 177, 191, 200 Algeria, 358 arachnoids (see Venus) ALH 84001, 201, 204–205 Archimedes crater (Moon), 93, 106 Allan Hills, 109, 201 Arctic, 62, 67, 84, 186, 229 Allende meteorite, 359, 360 Arden Corona (Miranda), 291 Allen Telescope Array, 409 Arecibo Observatory, 114, 144, 341, 379, 380, 408, 409 Alpha Regio (Venus), 144, 148, 149 Ares Vallis (Mars), 179, 180, 199 Alphonsus crater (Moon), 99, 102 Argentina, 408 Alps (Moon), 93 Argyre Basin (Mars), 161, 162, 163, 166, 186 Amalthea, 236–237, 238, 239, 241 Ariadaeus Rille (Moon), 100, 102 Amazonis Planitia (Mars), 161 COPYRIGHTED -
A Summary of the Unified Lunar Control Network 2005 and Lunar Topographic Model B. A. Archinal, M. R. Rosiek, R. L. Kirk, and B
A Summary of the Unified Lunar Control Network 2005 and Lunar Topographic Model B. A. Archinal, M. R. Rosiek, R. L. Kirk, and B. L. Redding U. S. Geological Survey, 2255 N. Gemini Drive, Flagstaff, AZ 86001, USA, [email protected] Introduction: We have completed a new general unified lunar control network and lunar topographic model based on Clementine images. This photogrammetric network solution is the largest planetary control network ever completed. It includes the determination of the 3-D positions of 272,931 points on the lunar surface and the correction of the camera angles for 43,866 Clementine images, using 546,126 tie point measurements. The solution RMS is 20 µm (= 0.9 pixels) in the image plane, with the largest residual of 6.4 pixels. We are now documenting our solution [1] and plan to release the solution results soon [2]. Previous Networks: In recent years there have been two generally accepted lunar control networks. These are the Unified Lunar Control Network (ULCN) and the Clementine Lunar Control Network (CLCN), both derived by M. Davies and T. Colvin at RAND. The original ULCN was described in the last major publication about a lunar control network [3]. Images for this network are from the Apollo, Mariner 10, and Galileo missions, and Earth-based photographs. The CLCN was derived from Clementine images and measurements on Clementine 750-nm images. The purpose of this network was to determine the geometry for the Clementine Base Map [4]. The geometry of that mosaic was used to produce the Clementine UVVIS digital image model [5] and the Near-Infrared Global Multispectral Map of the Moon from Clementine [6]. -
Modeling and Adjustment of THEMIS IR Line Scanner Camera Image Measurements
Modeling and Adjustment of THEMIS IR Line Scanner Camera Image Measurements by Brent Archinal USGS Astrogeology Team 2255 N. Gemini Drive Flagstaff, AZ 86001 [email protected] As of 2004 December 9 Version 1.0 Table of Contents 1. Introduction 1.1. General 1.2. Conventions 2. Observations Equations and Their Partials 2.1. Line Scanner Camera Specific Modeling 2.2. Partials for New Parameters 2.2.1. Orientation Partials 2.2.2. Spatial Partials 2.2.3. Partials of the observations with respect to the parameters 2.2.4. Parameter Weighting 3. Adjustment Model 4. Implementation 4.1. Input/Output Changes 4.1.1. Image Measurements 4.1.2. SPICE Data 4.1.3. Program Control (Parameters) Information 4.2. Computational Changes 4.2.1. Generation of A priori Information 4.2.2. Partial derivatives 4.2.3. Solution Output 5. Testing and Near Term Work 6. Future Work Acknowledgements References Useful web sites Appendix I - Partial Transcription of Colvin (1992) Documentation Appendix II - HiRISE Sensor Model Information 1. Introduction 1.1 General The overall problem we’re solving is that we want to be able to set up the relationships between the coordinates of arbitrary physical points in space (e.g. ground points) and their coordinates on line scanner (or “pushbroom”) camera images. We then want to do a least squares solution in order to come up with consistent camera orientation and position information that represents these relationships accurately. For now, supported by funding from the NASA Critical Data Products initiative (for 2003 September to 2005 August), we will concentrate on handling the THEMIS IR camera system (Christensen et al., 2003). -
Book of Abstracts: Studying Old Master Paintings
BOOK OF ABSTRACTS STUDYING OLD MASTER PAINTINGS TECHNOLOGY AND PRACTICE THE NATIONAL GALLERY TECHNICAL BULLETIN 30TH ANNIVERSARY CONFERENCE 1618 September 2009, Sainsbury Wing Theatre, National Gallery, London Supported by The Elizabeth Cayzer Charitable Trust STUDYING OLD MASTER PAINTINGS TECHNOLOGY AND PRACTICE THE NATIONAL GALLERY TECHNICAL BULLETIN 30TH ANNIVERSARY CONFERENCE BOOK OF ABSTRACTS 1618 September 2009 Sainsbury Wing Theatre, National Gallery, London The Proceedings of this Conference will be published by Archetype Publications, London in 2010 Contents Presentations Page Presentations (cont’d) Page The Paliotto by Guido da Siena from the Pinacoteca Nazionale of Siena 3 The rediscovery of sublimated arsenic sulphide pigments in painting 25 Marco Ciatti, Roberto Bellucci, Cecilia Frosinini, Linda Lucarelli, Luciano Sostegni, and polychromy: Applications of Raman microspectroscopy Camilla Fracassi, Carlo Lalli Günter Grundmann, Natalia Ivleva, Mark Richter, Heike Stege, Christoph Haisch Painting on parchment and panels: An exploration of Pacino di 5 The use of blue and green verditer in green colours in seventeenthcentury 27 Bonaguida’s technique Netherlandish painting practice Carole Namowicz, Catherine M. Schmidt, Christine Sciacca, Yvonne Szafran, Annelies van Loon, Lidwein Speleers Karen Trentelman, Nancy Turner Alterations in paintings: From noninvasive insitu assessment to 29 Technical similarities between mural painting and panel painting in 7 laboratory research the works of Giovanni da Milano: The Rinuccini -
Film Front Weimar: Representations of the First World War in German Films from the Weimar Period (1919-1933) Kester, Bernadette
www.ssoar.info Film Front Weimar: Representations of the First World War in German Films from the Weimar Period (1919-1933) Kester, Bernadette Veröffentlichungsversion / Published Version Monographie / monograph Zur Verfügung gestellt in Kooperation mit / provided in cooperation with: OAPEN (Open Access Publishing in European Networks) Empfohlene Zitierung / Suggested Citation: Kester, B. (2002). Film Front Weimar: Representations of the First World War in German Films from the Weimar Period (1919-1933). (Film Culture in Transition). Amsterdam: Amsterdam Univ. Press. https://nbn-resolving.org/ urn:nbn:de:0168-ssoar-317059 Nutzungsbedingungen: Terms of use: Dieser Text wird unter einer CC BY-NC-ND Lizenz This document is made available under a CC BY-NC-ND Licence (Namensnennung-Nicht-kommerziell-Keine Bearbeitung) zur (Attribution-Non Comercial-NoDerivatives). For more Information Verfügung gestellt. Nähere Auskünfte zu den CC-Lizenzen finden see: Sie hier: https://creativecommons.org/licenses/by-nc-nd/4.0 https://creativecommons.org/licenses/by-nc-nd/4.0/deed.de * pb ‘Film Front Weimar’ 30-10-2002 14:10 Pagina 1 The Weimar Republic is widely regarded as a pre- cursor to the Nazi era and as a period in which jazz, achitecture and expressionist films all contributed to FILM FRONT WEIMAR BERNADETTE KESTER a cultural flourishing. The so-called Golden Twenties FFILMILM FILM however was also a decade in which Germany had to deal with the aftermath of the First World War. Film CULTURE CULTURE Front Weimar shows how Germany tried to reconcile IN TRANSITION IN TRANSITION the horrendous experiences of the war through the war films made between 1919 and 1933. -
PEANUTS and SPACE FOUNDATION Apollo and Beyond
Reproducible Master PEANUTS and SPACE FOUNDATION Apollo and Beyond GRADE 4 – 5 OBJECTIVES PAGE 1 Students will: ö Read Snoopy, First Beagle on the Moon! and Shoot for the Moon, Snoopy! ö Learn facts about the Apollo Moon missions. ö Use this information to complete a fill-in-the-blank fact worksheet. ö Create mission objectives for a brand new mission to the moon. SUGGESTED GRADE LEVELS 4 – 5 SUBJECT AREAS Space Science, History TIMELINE 30 – 45 minutes NEXT GENERATION SCIENCE STANDARDS ö 5-ESS1 ESS1.B Earth and the Solar System ö 3-5-ETS1 ETS1.B Developing Possible Solutions 21st CENTURY ESSENTIAL SKILLS Collaboration and Teamwork, Communication, Information Literacy, Flexibility, Leadership, Initiative, Organizing Concepts, Obtaining/Evaluating/Communicating Ideas BACKGROUND ö According to NASA.gov, NASA has proudly shared an association with Charles M. Schulz and his American icon Snoopy since Apollo missions began in the 1960s. Schulz created comic strips depicting Snoopy on the Moon, capturing public excitement about America’s achievements in space. In May 1969, Apollo 10 astronauts traveled to the Moon for a final trial run before the lunar landings took place on later missions. Because that mission required the lunar module to skim within 50,000 feet of the Moon’s surface and “snoop around” to determine the landing site for Apollo 11, the crew named the lunar module Snoopy. The command module was named Charlie Brown, after Snoopy’s loyal owner. These books are a united effort between Peanuts Worldwide, NASA and Simon & Schuster to generate interest in space among today’s younger children. -
Shallow Crustal Composition of Mercury As Revealed by Spectral Properties and Geological Units of Two Impact Craters
Planetary and Space Science 119 (2015) 250–263 Contents lists available at ScienceDirect Planetary and Space Science journal homepage: www.elsevier.com/locate/pss Shallow crustal composition of Mercury as revealed by spectral properties and geological units of two impact craters Piero D’Incecco a,n, Jörn Helbert a, Mario D’Amore a, Alessandro Maturilli a, James W. Head b, Rachel L. Klima c, Noam R. Izenberg c, William E. McClintock d, Harald Hiesinger e, Sabrina Ferrari a a Institute of Planetary Research, German Aerospace Center, Rutherfordstrasse 2, D-12489 Berlin, Germany b Department of Geological Sciences, Brown University, Providence, RI 02912, USA c The Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA d Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80303, USA e Westfälische Wilhelms-Universität Münster, Institut für Planetologie, Wilhelm-Klemm Str. 10, D-48149 Münster, Germany article info abstract Article history: We have performed a combined geological and spectral analysis of two impact craters on Mercury: the Received 5 March 2015 15 km diameter Waters crater (106°W; 9°S) and the 62.3 km diameter Kuiper crater (30°W; 11°S). Using Received in revised form the Mercury Dual Imaging System (MDIS) Narrow Angle Camera (NAC) dataset we defined and mapped 9 October 2015 several units for each crater and for an external reference area far from any impact related deposits. For Accepted 12 October 2015 each of these units we extracted all spectra from the MESSENGER Atmosphere and Surface Composition Available online 24 October 2015 Spectrometer (MASCS) Visible-InfraRed Spectrograph (VIRS) applying a first order photometric correc- Keywords: tion. -
A Comparative Analysis of the Geology Tools Used During the Apollo Lunar Program and Their Suitability for Future Missions to the Om on Lindsay Kathleen Anderson
University of North Dakota UND Scholarly Commons Theses and Dissertations Theses, Dissertations, and Senior Projects January 2016 A Comparative Analysis Of The Geology Tools Used During The Apollo Lunar Program And Their Suitability For Future Missions To The oM on Lindsay Kathleen Anderson Follow this and additional works at: https://commons.und.edu/theses Recommended Citation Anderson, Lindsay Kathleen, "A Comparative Analysis Of The Geology Tools Used During The Apollo Lunar Program And Their Suitability For Future Missions To The oonM " (2016). Theses and Dissertations. 1860. https://commons.und.edu/theses/1860 This Thesis is brought to you for free and open access by the Theses, Dissertations, and Senior Projects at UND Scholarly Commons. It has been accepted for inclusion in Theses and Dissertations by an authorized administrator of UND Scholarly Commons. For more information, please contact [email protected]. A COMPARATIVE ANALYSIS OF THE GEOLOGY TOOLS USED DURING THE APOLLO LUNAR PROGRAM AND THEIR SUITABILITY FOR FUTURE MISSIONS TO THE MOON by Lindsay Kathleen Anderson Bachelor of Science, University of North Dakota, 2009 A Thesis Submitted to the Graduate Faculty of the University of North Dakota in partial fulfillment of the requirements for the degree of Master of Science Grand Forks, North Dakota May 2016 Copyright 2016 Lindsay Anderson ii iii PERMISSION Title A Comparative Analysis of the Geology Tools Used During the Apollo Lunar Program and Their Suitability for Future Missions to the Moon Department Space Studies Degree Master of Science In presenting this thesis in partial fulfillment of the requirements for a graduate degree from the University of North Dakota, I agree that the library of this University shall make it freely available for inspection. -
Conceptual Human-System Interface Design for a Lunar Access Vehicle
Conceptual Human-System Interface Design for a Lunar Access Vehicle Mary Cummings Enlie Wang Cristin Smith Jessica Marquez Mark Duppen Stephane Essama Massachusetts Institute of Technology* Prepared For Draper Labs Award #: SC001-018 PI: Dava Newman HAL2005-04 September, 2005 http://halab.mit.edu e-mail: [email protected] *MIT Department of Aeronautics and Astronautics, Cambridge, MA 02139 TABLE OF CONTENTS 1 INTRODUCTION..................................................................................................... 1 1.1 THE GENERAL FRAMEWORK................................................................................ 1 1.2 ORGANIZATION.................................................................................................... 2 2 H-SI BACKGROUND AND MOTIVATION ........................................................ 3 2.1 APOLLO VS. LAV H-SI........................................................................................ 3 2.2 APOLLO VS. LUNAR ACCESS REQUIREMENTS ...................................................... 4 3 THE LAV CONCEPTUAL PROTOTYPE............................................................ 5 3.1 HS-I DESIGN ASSUMPTIONS ................................................................................ 5 3.2 THE CONCEPTUAL PROTOTYPE ............................................................................ 6 3.3 LANDING ZONE (LZ) DISPLAY............................................................................. 8 3.3.1 LZ Display Introduction................................................................................. -
Stereo Reconstruction from Apollo 15 and 16 Metric Camerazachary
42nd Lunar and Planetary Science Conference (2011) 2267.pdf Stereo Reconstruction from Apollo 15 and 16 Metric Camera Zachary Moratto1, Ara Nefian1,2, Taemin Kim1, Michael Broxton1,2, Ross Beyer1,3, and Terry Fong1, 1NASA Ames Research Center, MS 269-3, Moffett Field, CA, USA ([email protected]), 2Carnegie Mellon University, 3Carl Sagan Center SETI Introduction saic, DIM, and precision maps are produced for both This paper presents the production of digital terrain mod- missions separately. els (DTMs) and digital image mosaics (DIMs) of the Lu- The DTM mosaic is formed by a weighted average of nar surface that cover a large portion of the near-side of the stereo pair DTMs. Input DTMs were weighted max- the Moon at 40 m/px and 10 m/px respectively. These imum value at their centers and then feathered to zero at data products, produced under direction of the NASA the edges. The DTM mosaics are shown in Fig. 1 and 2. ESMD Lunar Mapping and Modeling Project (LMMP), The DIM was created by projecting the original res- are based on 2600 stereo image pairs from the Apollo olution images onto the 40 m/px DTMs, creating indi- 15 and 16 missions that were digitized at high resolution vidual orthoimages. Those orthoimages were then mo- from the original mission films [1]. Our reconstruction saicked by a process described in [5] without reflectance. was carried out using the highly automated Ames Stereo Therefore, only the final image mosaic and time expo- Pipeline software [2], which runs on NASA’s Pleiades sures were calculated. -
Picturing France
Picturing France Classroom Guide VISUAL ARTS PHOTOGRAPHY ORIENTATION ART APPRECIATION STUDIO Traveling around France SOCIAL STUDIES Seeing Time and Pl ace Introduction to Color CULTURE / HISTORY PARIS GEOGRAPHY PaintingStyles GOVERNMENT / CIVICS Paris by Night Private Inve stigation LITERATURELANGUAGE / CRITICISM ARTS Casual and Formal Composition Modernizing Paris SPEAKING / WRITING Department Stores FRENCH LANGUAGE Haute Couture FONTAINEBLEAU Focus and Mo vement Painters, Politics, an d Parks MUSIC / DANCENATURAL / DRAMA SCIENCE I y Fontainebleau MATH Into the Forest ATreebyAnyOther Nam e Photograph or Painting, M. Pa scal? ÎLE-DE-FRANCE A Fore st Outing Think L ike a Salon Juror Form Your Own Ava nt-Garde The Flo ating Studio AUVERGNE/ On the River FRANCHE-COMTÉ Stream of Con sciousness Cheese! Mountains of Fra nce Volcanoes in France? NORMANDY “I Cannot Pain tan Angel” Writing en Plein Air Culture Clash Do-It-Yourself Pointillist Painting BRITTANY Comparing Two Studie s Wish You W ere Here Synthétisme Creating a Moo d Celtic Culture PROVENCE Dressing the Part Regional Still Life Color and Emo tion Expressive Marks Color Collectio n Japanese Prin ts Legend o f the Château Noir The Mistral REVIEW Winds Worldwide Poster Puzzle Travelby Clue Picturing France Classroom Guide NATIONAL GALLERY OF ART, WASHINGTON page ii This Classroom Guide is a component of the Picturing France teaching packet. © 2008 Board of Trustees of the National Gallery of Art, Washington Prepared by the Division of Education, with contributions by Robyn Asleson, Elsa Bénard, Carla Brenner, Sarah Diallo, Rachel Goldberg, Leo Kasun, Amy Lewis, Donna Mann, Marjorie McMahon, Lisa Meyerowitz, Barbara Moore, Rachel Richards, Jennifer Riddell, and Paige Simpson.