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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. -
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. -
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. -
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. -
Planetary Maps for Public and Educational Outreach - Experiences from the Making of the Multilingual Map of Mars and Venus
PLANETARY MAPS FOR PUBLIC AND EDUCATIONAL OUTREACH - EXPERIENCES FROM THE MAKING OF THE MULTILINGUAL MAP OF MARS AND VENUS Hargitai, H.I. Eötvös University, Faculty of Science, Planetology Group, H-1117 Budapest, Pázmány P. sétány. 1/a. Hungary. E-mail: [email protected] 1. INTRODUCTION In recent years we obtained detailed topographic and geologic information on the planetary bodies’ surfaces (namely Venus, the Earth, Mars, the Moon and - though in somewhat less details - the Jovian Moons). The next planetary body to fully mapped will be Titan in 2005. These worlds all have their own characteristics. Maps are powerful tools not only for scientific research but also for education. Children love to browse World Atlases and wander their pages. Geography books or classes targeted for any age group can not miss maps, usually contour or thematic maps. In this paper I propose to use planetary maps for the same purpose, published in the first language of its users. Now, years after the publication of detailed planetary maps, the broad public and students still do not have planetary maps designed specially for them. Maps for amateur “backyard” astronomers (albedo maps for Mars, shade relief maps for the Moon) and maps for scientific research (published by USGS, for example) are not the subjects of this paper. There are planetary maps for download on the internet but this I also list among the scientific maps. In this paper I will (1) review the possible reasons for the making of such planetary maps; (2) give recommendations for various examples where such maps could be published, (3) analyze the making of one such series in detail, which has been made by an international cooperation (the Multilingual Map of Mars and the Multilingual Map of Venus as part of the multilingual map series of the ICA Commission on Planetary Cartography) and (4) discuss the relevance of nomenclature and terminology system used on planetary maps made for the general public. -
Planets Solar System Paper Contents
Planets Solar system paper Contents 1 Jupiter 1 1.1 Structure ............................................... 1 1.1.1 Composition ......................................... 1 1.1.2 Mass and size ......................................... 2 1.1.3 Internal structure ....................................... 2 1.2 Atmosphere .............................................. 3 1.2.1 Cloud layers ......................................... 3 1.2.2 Great Red Spot and other vortices .............................. 4 1.3 Planetary rings ............................................ 4 1.4 Magnetosphere ............................................ 5 1.5 Orbit and rotation ........................................... 5 1.6 Observation .............................................. 6 1.7 Research and exploration ....................................... 6 1.7.1 Pre-telescopic research .................................... 6 1.7.2 Ground-based telescope research ............................... 7 1.7.3 Radiotelescope research ................................... 8 1.7.4 Exploration with space probes ................................ 8 1.8 Moons ................................................. 9 1.8.1 Galilean moons ........................................ 10 1.8.2 Classification of moons .................................... 10 1.9 Interaction with the Solar System ................................... 10 1.9.1 Impacts ............................................ 11 1.10 Possibility of life ........................................... 12 1.11 Mythology ............................................. -
Planetary Nomenclature: Information and Guidelines for Geologic Mappers
Planetary Geologic Mappers 2021 (LPI Contrib. No. 2610) 7018.pdf PLANETARY NOMENCLATURE: INFORMATION AND GUIDELINES FOR GEOLOGIC MAPPERS. Tenielle Gaither1 and Amber Gullikson1, 1USGS Astrogeology Science Center, Flagstaff, Arizona ([email protected]). Introduction: The task of naming planetary is useful to the scientific and cartographic surface features, rings, and natural satellites is communities at large. managed by the International Astronomical Un- • Name duplication on two or more bodies is ion’s (IAU) Working Group for Planetary System discouraged. Nomenclature (WGPSN). The volunteer members • Solar system nomenclature should be interna- of the WGPSN and its task groups have worked tional in its choice of names. since the early 1970s to provide a clear, unambig- • Names with political, military, or religious sig- uous system of planetary nomenclature that repre- nificance are not allowed. sents cultures and countries from all regions of Guidelines for Geologic Mappers: Standard- Earth. WGPSN members include Rita Schulz ized planetary nomenclature is particularly useful (chair) and 8 other members representing countries in planetary geologic maps. These names provide around the globe. Since the 1980s, the USGS As- reliable points of reference for mappers to describe trogeology Science Center has managed (for the features, units, and histories. As such, planetary IAU and with the financial support of NASA) the mappers are some of the heaviest users of planetary ever-growing database of planetary names, the names. To facilitate the correct use of these names, online Gazetteer of Planetary Nomenclature. This mappers should continuously review the official abstract provides a summary of the program status nomenclature in their map area early in the map- as well as guidelines for geologic mappers. -
How Astronomical Objects Are Named
How Astronomical Objects Are Named Jeanne E. Bishop Westlake Schools Planetarium 24525 Hilliard Road Westlake, Ohio 44145 U.S.A. bishop{at}@wlake.org Sept 2004 Introduction “What, I wonder, would the science of astrono- use of the sky by the societies of At the 1988 meeting in Rich- my be like, if we could not properly discrimi- the people that developed them. However, these different systems mond, Virginia, the Inter- nate among the stars themselves. Without the national Planetarium Society are beyond the scope of this arti- (IPS) released a statement ex- use of unique names, all observatories, both cle; the discussion will be limited plaining and opposing the sell- ancient and modern, would be useful to to the system of constellations ing of star names by private nobody, and the books describing these things used currently by astronomers in business groups. In this state- all countries. As we shall see, the ment I reviewed the official would seem to us to be more like enigmas history of the official constella- methods by which stars are rather than descriptions and explanations.” tions includes contributions and named. Later, at the IPS Exec- – Johannes Hevelius, 1611-1687 innovations of people from utive Council Meeting in 2000, many cultures and countries. there was a positive response to The IAU recognizes 88 constel- the suggestion that as continuing Chair of with the name registered in an ‘important’ lations, all originating in ancient times or the Committee for Astronomical Accuracy, I book “… is a scam. Astronomers don’t recog- during the European age of exploration and prepare a reference article that describes not nize those names.