Some Aspects of Multilingual Planetary Map Producing for Non- Professional Audience: Visualization and Nomenclature
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Planetary Nomenclature: an Overview and Update
3rd Planetary Data Workshop 2017 (LPI Contrib. No. 1986) 7119.pdf PLANETARY NOMENCLATURE: AN OVERVIEW AND UPDATE. T. Gaither1, R. K. Hayward1, J. Blue1, L. Gaddis1, R. Schulz2, K. Aksnes3, G. Burba4, G. Consolmagno5, R. M. C. Lopes6, P. Masson7, W. Sheehan8, B.A. Smith9, G. Williams10, C. Wood11, 1USGS Astrogeology Science Center, Flagstaff, Ar- izona ([email protected]); 2ESA Scientific Support Office, Noordwijk, The Netherlands; 3Institute for Theoretical Astrophysics, Oslo, Norway; 4Vernadsky Institute, Moscow, Russia; 5Specola Vaticana, Vati- can City State; 6Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California; 7Uni- versite de Paris-Sud, Orsay, France; 8Lowell Observatory, Flagstaff, Arizona; 9Santa Fe, New Mexico; 10Minor Planet Center, Cambridge, Massachusetts; 11Planetary Science Institute, Tucson, Arizona. Introduction: The task of naming planetary Asteroids surface features, rings, and natural satellites is Ceres 113 managed by the International Astronomical Un- Dactyl 2 ion’s (IAU) Working Group for Planetary System Eros 41 Nomenclature (WGPSN). The members of the Gaspra 34 WGPSN and its task groups have worked since the Ida 25 early 1970s to provide a clear, unambiguous sys- Itokawa 17 tem of planetary nomenclature that represents cul- Lutetia 37 tures and countries from all regions of Earth. Mathilde 23 WGPSN members include Rita Schulz (chair) and Steins 24 9 other members representing countries around the Vesta 106 globe (see author list). In 2013, Blue et al. [1] pre- Jupiter sented an overview of planetary nomenclature, and Amalthea 4 in 2016 Hayward et al. [2] provided an update to Thebe 1 this overview. Given the extensive planetary ex- Io 224 ploration and research that has taken place since Europa 111 2013, it is time to update the community on the sta- Ganymede 195 tus of planetary nomenclature, the purpose and Callisto 153 rules, the process for submitting name requests, and the IAU approval process. -
THE FOUR ARACHNOID GROUPS of VENUS. Kostama, V-P
Lunar and Planetary Science XXXIII (2002) 1115.pdf THE FOUR ARACHNOID GROUPS OF VENUS. Kostama, V-P. Astronomy, Department of Physical Sciences, Uni- versity of Oulu, P.O. BOX 3000, FIN-90014, Finland (<[email protected]>). Introduction: A population of 96 arachnoids has some parts of the ridge belt cut the arachnoids. This been found on Venus [1]. These surface structures implies that the arachnoids or the group may have had were first discovered on the Venera 15/16 radar images several evolution phases. and later defined in detail by the Magellan mission [2, 3]. The arachnoids have a peculiar distribution, which is generally different to that of the coronae and particu- larly the novae [4]. The global distribution of arach- noids reflects certain noticeable facts: There is a clear concentration of arachnoid features in the northern hemisphere as 65,6 percent (63 feat.) of the features is located there, while only 34,4 percent (33 feat.) of the population is located in the southern hemisphere [5]. In addition, the arachnoids form four large groups which include roughly 25 % of the total population. The arachnoids of Bereghinya and Ganiki Planitia: The arachnoid group of Bereghinya Planitia is by far the largest arachnoid concentration on Venus. The structural composition of the features of the group are generally distinct and the features are connected by a uniform, chain-like pattern of lineaments. Figure 2. Scetch map of the large arachnoid group on Bereghinya Planitia. Brown lines are ridges, red repre- sents the lava channel within the area. Deformation zones are in grey. -
Mapping of Inner and Outer Celestial Bodies Using New Global and Local Topographic Data Derived from Photogrammetric Image Processing
The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Volume XLI-B4, 2016 XXIII ISPRS Congress, 12–19 July 2016, Prague, Czech Republic Mapping of inner and outer celestial bodies using new global and local topographic data derived from photogrammetric image processing I.P. Karachevtsevaa*, A.A. Kokhanova, J.F. Rodionovaa,b, A.Yu. Zharkovaa,, M.S. Lazarevaa aMoscow State University of Geodesy and Cartography (MIIGAiK), MIIGAiK Extraterrestrial laboratory (MExLab), 105064. Gorokhovsky per., Moscow, Russia [email protected] bSternberg State Astronomical Institute, 1198993, Moscow, Russia Commission IV, WG IV/8 KEY WORDS: Planetary cartography, DEM, geomorphology study, Phobos, the Moon, Mercury, Ganymede and Enceladus ABSTRACT: New estimation of fundamental geodetic parameters and global and local topography of planets and satellites provide basic coordinate systems for mapping as well as opportunities for studies of processes on their surfaces. The main targets of our study are Europa, Ganymede, Calisto and Io (satellites of Jupiter), Enceladus (a satellite of Saturn), terrestrial planetary bodies, including Mercury, the Moon and Phobos, one of the Martian satellites. In particular, based on new global shape models derived from three-dimensional control point networks and processing of high-resolution stereo images, we have carried out studies of topography and morphology. As a visual representation of the results, various planetary maps with different scale and thematic direction were created. For example, for Phobos we have produced a new atlas with 43 maps, as well as various wall maps (different from the maps in the atlas by their format and design): basemap, topography and geomorphological maps. In addition, we compiled geomorphologic maps of Ganymede on local level, and a global hypsometric Enceladus map. -
Geologic Map of the Ganiki Planitia Quadrangle (V–14), Venus Eric B
Claremont Colleges Scholarship @ Claremont Pomona Faculty Publications and Research Pomona Faculty Scholarship 1-1-2011 Geologic Map of the Ganiki Planitia Quadrangle (V–14), Venus Eric B. Grosfils Pomona College Sylvan M. Long Elizabeth M. Venechuk Debra M. Hurwitz Joseph W. Richards See next page for additional authors Recommended Citation Grosfils, E.B., Long, S.M., Venechuk, E.M., Hurwitz, D.M., Richards, J.W., Kastl, Brian, Drury, D.E., and Hardin, Johanna, 2011, Geologic map of the Ganiki Planitia quadrangle (V-14), Venus: U.S. Geological Survey Scientific nI vestigations Map 3121. This Report is brought to you for free and open access by the Pomona Faculty Scholarship at Scholarship @ Claremont. It has been accepted for inclusion in Pomona Faculty Publications and Research by an authorized administrator of Scholarship @ Claremont. For more information, please contact [email protected]. Authors Eric B. Grosfils, Sylvan M. Long, Elizabeth M. Venechuk, Debra M. Hurwitz, Joseph W. Richards, Brian Kastl, Dorothy E. Drury, and Johanna S. Hardin This report is available at Scholarship @ Claremont: http://scholarship.claremont.edu/pomona_fac_pub/303 Prepared for the National Aeronautics and Space Administration Geologic Map of the Ganiki Planitia Quadrangle (V–14), Venus By Eric B. Grosfils, Sylvan M. Long, Elizabeth M. Venechuk, Debra M. Hurwitz, Joseph W. Richards, Brian Kastl, Dorothy E. Drury, and Johanna Hardin Pamphlet to accompany Scientific Investigations Map 3121 75° 75° V–1 V–3 V–6 50° 50° V–4 V–5 V–11 V–16 V–12 V–15 V–13 V–14 25° 25° V–23 V–28 V–24 V–27 V–25 V–26 90° 120° 150° 180° 210° 240° 270° 0° 0° V–37 V–38 V–36 V–39 V–35 V–40 –25° –25° V–49 V–50 V–48 V–51 V–47 V–52 V–58 V–59 –50° –50° V–57 V–60 2011 V–62 –75° –75° U.S. -
2013 October
TTSIQ #5 page 1 OCTOBER 2013 Reducing space transportation costs considerably is vital to achievement of mankind’s goals & dreams in space NEWS SECTION pp. 3-70 p. 3 Earth Orbit and Mission to Planet Earth p. 17 Cislunar Space and the Moon p. 26 Mars and the Asteroids p. 45 Other Planets and their moons p. 62 Starbound ARTICLES & ESSAYS pp. 72-95 p. 72 Covering Up Lunar Habitats with Moondust? - Some Precedents Here on Earth - Peter Kokh p. 74 How can we Stimulate Greater Use of the International Space Station? - Peter Kokh p. 75 AS THE WORLD EXPANDS The Epic of Human Expansion Continues - Peter Kokh p. 77 Grytviken, South Georgia Island - Lessons for Moonbase Advocates - Peter Kokh K p. 78 The “Flankscopes” Project: Seeing Around the Edges of the Moon - Peter Kokh p. 81 Integrating Cycling Orbits to Enhance Cislunar Infrastructure - Al Anzaldua p. 83 The Responsibilities of Dual Citizenship for Our economy, Our planet, and the Evolution of a Space Faring Civilization - David Dunlop p. 87 Dueling Space Roadmaps - David Dunlop p. 91 A Campaign for the International Lunar Geophysical Year: Some Beginning Considerations - David Dunlop STUDENTS & TEACHERS pp. 97-100 p. 97 Lithuanian Students Hope for free Launch of 2 Amateur Radio CubeSats p. 98 NASA Selects 7 University Projects For 2014 X-Hab Innovation Challenge Penn State University “Lions” take on the Google Lunar X-Prize Challenge p. 99 Do you experience “Manhattan Henge” in your home town? Advanced Robot with more sophisticated motion capabilities unveiled The Ongoing CubeSat Revolution: what it means for Student Space Science p. -
Nomenclature for Lunar Features at the Chang'e-3 Landing Site
Acta Geochim (2017) 36(2):213–223 DOI 10.1007/s11631-017-0159-1 ORIGINAL ARTICLE Nomenclature for lunar features at the Chang’e-3 landing site Zhoubin Zhang1,2 · Chunlai Li1,2,3 · Wei Zuo1,2,3 · Xingguo Zeng1,2 Received: 22 December 2016 / Revised: 15 February 2017 / Accepted: 9 April 2017 / Published online: 27 April 2017 © Science Press, Institute of Geochemistry, CAS and Springer-Verlag Berlin Heidelberg 2017 Abstract Nomenclatures for lunar features always published after some necessary approval procedures by the accompany the progresses of human lunar exploration, International Astronomical Union. which has an important dual meaning in culture and sci- ence. The naming of lunar features not only can Keywords Moon · Chang’e-3 · Landing site · Lunar commemorate the outstanding contributions of academics, feature nomenclature masters in various fields, and popularize the traditional cultures of ethnic groups all over the world, but also have a critical function of providing accurate indicative informa- 1 Introduction tion on features with special morphology, origin, nature and scientific value. However, nomenclature for features at Planetary nomenclature, like terrestrial nomenclature, is the Chang’e-3 landing site, which has a more arbitrary used to uniquely identify a feature on the surface of a form without many constrains posed by a uniformed sys- planet or satellite so that the feature can be easily located, tem, is unlike the features for other morphological units. described, and discussed. Nomenclature for lunar features This paper originated from the actual needs for the originated in the seventeenth century, as early scientists in description of scientific exploration activities, interpreta- that era used telescopes to observe the lunar surface, named tion of scientific research and dissemination of scientific the remarkable features on the lunar surface according to results. -
Mars Activities
MARS ACTIVITIES Teacher Resources and Classroom Activities Mars Education Program Jet Propulsion Laboratory Arizona State University Mars Missions Information and Updates Mission Information Available at Jet Propulsion Laboratory Mars Exploration Home Page http://mars.jpl.nasa.gov More Educational Activities Available at Jet Propulsion Laboratory Mars Education & Public Outreach Program http://mars.jpl.nasa.gov/classroom or Arizona State University Mars K-12 Education Program http://tes.asu.edu/neweducation.html Table of Contents 1. Earth, Moon, Mars Balloons 1 2. Rover Races 4 3. Areology - The Study of Mars 11 4. Strange New Planet 16 5. Lava Layering 24 6. Searching for Life on Mars 33 7. Mars Critters 42 8. Exploring Crustal Material from a Mystery Planet 46 - Graph Paper 48 9. Edible Mars Rover 49 - Mars Pathfinder Rover 51 10. Edible Mars Spacecraft 52 - Mars Global Surveyor 54 - Mars Pathfinder 55 - Mars Pathfinder Rover 56 11. Mars Meteorites’ Fingerprints 57 12. Introduction to Creating a Mission Plan 65 13. Out of Sight: Remote Vehicle Activity 66 - Mars Rover Websites 69 15. Probing Below the Surface of Mars 74 16. Good Vibrations 85 17. The Mathematics of Mars 90 - “I Have…Who Has?” Cards 93 18. Mars Bingo 100 19. Mud Splat Craters 112 20. Solar System Beads Distance Activity 115 21. Alka-Seltzer Rockets 118 22. Soda Straw Rockets 122 23. Mars Pathfinder: Two-Dimensional Model 126 24. Mars Pathfinder: Egg Drop and Landing 127 25. Cool Internet Sites 128 Earth, Moon, Mars Balloons 1 Introduction: How big is the Moon; how far is it relative to Earth? Earth science and astronomy books depict a moon that is much closer and much larger than in reality. -
The Red Planet
The Red Planet LEARNING RESOURCE GUIDE Grades 3-8 A companion to The Martian 4D Experience MARS FACT SHEET Mars is the fourth planet from the Sun. It is sometimes called the ‘Red Planet’ because of its red soil. The soil on Mars is red because it contains iron oxide (rust). Mars is one of the brightest objects in the night sky. It has been known since ancient times. The planet is named for the Roman god of War. It has two moons, Phobos (fear) and Deimos (panic). The moons get their scary names from the horses that pulled the chariot of the Greek god Ares. SUN JUPITER SATURN EARTH URANUS NEPTUNE MERCURY VENUS MARS! WHAT’S IT LIKE ON MARS? 1. Mars is a little like Earth, only smaller, drier and colder. There are places 3. Mars is a rocky planet. It is dusty and dry. The sky would be hazy and red on Earth that are a little like Mars—Death Valley, California; Antarctica instead of blue. Sometimes giant dust storms cover the whole planet. and volcanoes in Hawaii. Both planets have polar ice caps, volcanoes, 4. Exploring Mars would be hard. But there are lots of things to see and canyons and four seasons. The seasons on Mars are twice as long. learn. Olympus Mons may be the largest volcano in our solar system. It is 2. The thin air on Mars makes it a dangerous place for humans. It is three times taller than Mt. Everest (the tallest mountain on Earth) and as mostly poisonous carbon dioxide. -
The Lachesis Tessera Quadrangle (V-18), Venus
52nd Lunar and Planetary Science Conference 2021 (LPI Contrib. No. 2548) 2557.pdf THE LACHESIS TESSERA QUADRANGLE (V-18), VENUS. L. A. Fattaruso1, D. L. Buczkowski3, E. M. McGowan1,2, and G. E. McGill1. 1University of Massachusetts, Amherst, MA; 2Johns Hopkins Applied Physics La- boratory, Laurel, MD 20723; 3Mount Holyoke College, South Hadley, MA, [email protected]. Introduction: The Lachesis Tessera V-18 quad- to that of tessera. Exposures are widely scattered, and rangle (25o-50oN, 300o-330oE) includes parts of Sedna too small to determine age relations with tessera. and Guinevere Planitiae; regional plains [1] cover Plains materials: Regional plains, the most exten- ~80% of the quadrangle. The region includes 2 defor- sive materials in the quadrangle, are mapped as two mation belts and embayed fragments of 1-2 possible units, based on radar brightness. While the number of additional belts, 3 large central volcanoes, abundant impact craters superposed on the plains is too small to small shield volcanoes and associated flow materials, measure age differences between the emplacement of 13 impact craters, 3 named coronae, many coronae-like the darker (pr1) and brighter (pr2) regional plains features, arachnoid-like features, and dark spots [2]. units [3], stratigraphic markers imply that pr2 is The quadrangle contains a linear grouping of a promi- younger than pr1. However, clear cut examples of nent NW to SE oriented structural belt, coronae, and wrinkle ridges and fractures superposed on pr1 but coronae-like structures [2]. Important individual struc- truncated by pr2 have not been found, indicating that tural features include radar-bright lineaments, graben, the age difference is very small. -
Towards the Development of Supplements to the Gazetteer of Planetary Nomenclature
EPSC Abstracts Vol. 5, EPSC2010-865, 2010 European Planetary Science Congress 2010 c Author(s) 2010 Towards the development of supplements to the Gazetteer of Planetary Nomenclature H. Hargitai1, Á. Kereszturi2 1 Eötvös Loránd University, 1117 Pázmány P st 1/A Budapest, Hungary [email protected], 2Collegium Budapest Institute for Advanced Study; and Eotvos University, Planetary Science Research Group 1117 Pázmány P st 1/A Budapest, Hungary Abstract nomenclature. Since some – and in the future, presumably more and more – names originate from Various international organizations are working on nations that use a non Latin writing system, publishing databases that supplement the official transliteration or transcription of names should be Gazetteer of Planetary Nomenclature. This paper unambiguous and reversable. It is also a major question why would all nations of the Earth accept focuses on the online Planetary Nomenclature Latin or Romanized forms of these names being the Pronunciation Guide created by ICA Commission on only, official forms, once the principle of planetary Planetary Cartography. nomenclature is to be truly international, not placing any nations ahead of any other. It does not seem to 1. Introduction be right for example to have a Chinese name written The present day official Planetary Nomenclature in Latin characters in a planetary map published for Gazetteer is maintained for IAU by personell of the use by Chinese schoolchildren. It would first be USGS on their website [1]. It reflects decisions by necessary to define which transcription / IAU Working Group for Planetary System transliteration system IAU uses in any particular Nomenclature. There are needs from various parts of language when they form the official Romanized the planetary scientist and planetary cartographer version. -
Planetary Geologic Mapping Handbook – 2010
Planetary Geologic Mapping Handbook – 2010 K.L. Tanaka, J.A. Skinner, Jr., and T.M. Hare U.S. Geological Survey, Astrogeology Science Center 2255 N. Gemini Dr., Flagstaff, AZ 86001 Endorsed by: The Geologic Mapping Subcommittee (GEMS) of the NASA Planetary Cartography and Geologic Mapping Working Group (PCGMWG) M.S. Kelley1, L.F. Bleamaster III2, D.A. Crown2, L.R. Gaddis3, T.K.P. Gregg4, J.R. Johnson3, S.C. Mest2, and K.K. Williams5 1NASA Headquarters, Washington, DC 2Planetary Science Institute, Tucson, AZ 3U.S. Geological Survey, Astrogeology Science Center, Flagstaff, AZ 4University at Buffalo, Buffalo, NY 5Buffalo State College, Buffalo, NY TABLE OF CONTENTS What’s New ..........................................................................................................................2 1. Introduction..........................................................................................................................2 2. Purpose of this handbook.....................................................................................................3 3. Map processing ....................................................................................................................3 a. Proposals........................................................................................................................3 b. Map base package..........................................................................................................4 c. Digital mapping .............................................................................................................5 -
Planetary Nomenclature: Overview and Update for 2020
51st Lunar and Planetary Science Conference (2020) 2237.pdf PLANETARY NOMENCLATURE: OVERVIEW AND UPDATE FOR 2020. T. A. Gaither1, K. Aksnes2, G. A. Burba3, G. J. Consolmagno5, R. M. C. Lopes6, P. Masson7, W. Sheehan8, G. V. Williams9, and C. Wood10, 1USGS Astrogeology Science Center, Arizona, USA, [email protected], 2ESA Science Directorate, ESTEC, Noordwijk, The Netherlands, 3Institute for Theoretical Astrophysics, Oslo, Norway, 4Vernadsky Institute, Moscow, Russia, 5Specola Vaticana, Vatican City State, 6Jet Propulsion Laboratory, California Institute of Technology, California, USA, 7Universite de Paris-Sud, Orsay, France, 8Lowell Observatory, Arizona, USA, 9 Minor Planet Center, Massachusetts, USA, 10Planetary Science Institute, Arizona, USA. Introduction: The task of naming planetary surface • Solar system nomenclature should be inter- features, rings, and natural satellites is managed by the national in its choice of names. International Astronomical Union’s (IAU) Working • Names having political, military, or religious Group for Planetary System Nomenclature (WGPSN). significance are not allowed. The volunteer members of the WGPSN and its task • Commemoration is not a goal in itself, but may be groups have worked since the early 1970s to provide a employed in special circumstances and is reserved for clear, unambiguous system of planetary nomenclature persons of high and enduring international standing. that represents cultures and countries from all regions of Persons being so honored must have been deceased for Earth. Since the 1980s, the USGS Astrogeology Science at least three years. Center has managed (for the IAU and with the financial Guidelines for Requesters: An official name may support of NASA) the ever-growing database of be requested for any unnamed morphological or planetary names and the Gazetteer of Planetary topographic feature that will be a primary focus of a Nomenclature website.