caa a22 4500 445863145 CHVBK 20180317145449.0 cr unu---uuuuu 170323e20110201xx s 000 0 eng 10.1007/s10569-010-9320-4 doi (NATIONALLICENCE)springer-10.1007/s10569-010-9320-4 Report of the IAU Working Group on Cartographic Coordinates and Rotational Elements: 2009 [Elektronische Daten] [B. Archinal, M. A'Hearn, E. Bowell, A. Conrad, G. Consolmagno, R. Courtin, T. Fukushima, D. Hestroffer, J. Hilton, G. Krasinsky, G. Neumann, J. Oberst, P. Seidelmann, P. Stooke, D. Tholen, P. Thomas, I. Williams] Every three years the IAU Working Group on Cartographic Coordinates and Rotational Elements revises tables giving the directions of the poles of rotation and the prime meridians of the planets, satellites, minor planets, and comets. This report takes into account the IAU Working Group for Planetary System Nomenclature (WGPSN) and the IAU Committee on Small Body Nomenclature (CSBN) definition of dwarf planets, introduces improved values for the pole and rotation rate of Mercury, returns the rotation rate of Jupiter to a previous value, introduces improved values for the rotation of five satellites of Saturn, and adds the equatorial radius of the Sun for comparison. It also adds or updates size and shape information for the Earth, Mars' satellites Deimos and Phobos, the four Galilean satellites of Jupiter, and 22 satellites of Saturn. Pole, rotation, and size information has been added for the asteroids (21) Lutetia, (511) Davida, and (2867) Šteins. Pole and rotation information has been added for (2) Pallas and (21) Lutetia. Pole and rotation and mean radius information has been added for (1) Ceres. Pole information has been updated for (4) Vesta. The high precision realization for the pole and rotation rate of the Moon is updated. Alternative orientation models for Mars, Jupiter, and Saturn are noted. The Working Group also reaffirms that once an observable feature at a defined longitude is chosen, a longitude definition origin should not change except under unusual circumstances. It is also noted that alternative coordinate systems may exist for various (e.g. dynamical) purposes, but specific cartographic coordinate system information continues to be recommended for each body. The Working Group elaborates on its purpose, and also announces its plans to occasionally provide limited updates to its recommendations via its website, in order to address community needs for some updates more often than every 3years. Brief recommendations are also made to the general planetary community regarding the need for controlled products, and improved or consensus rotation models for Mars, Jupiter, and Saturn. Springer Science+Business Media B.V.(outside the USA), 2010 Cartographic coordinates nationallicence Longitude nationallicence Latitude nationallicence Rotation axes nationallicence Rotation periods nationallicence Sizes nationallicence Shapes nationallicence Planets nationallicence Satellites nationallicence Dwarf planets nationallicence Minor planets nationallicence Comets nationallicence Archinal B. U.S. Geological Survey, Flagstaff, AZ, USA aut A'Hearn M. University of Maryland, College Park, MD, USA aut Bowell E. Lowell Observatory, Flagstaff, AZ, USA aut Conrad A. W.M. Keck Observatory, Kamuela, HI, USA aut Consolmagno G. Vatican Observatory, Vatican City, Vatican City State aut Courtin R. LESIA, Observatoire de Paris, CNRS, Paris, France aut Fukushima T. National Astronomical Observatory of Japan, Tokyo, Japan aut Hestroffer D. IMCCE, Observatoire de Paris, CNRS, Paris, France aut Hilton J. U.S. Naval Observatory, Washington, DC, USA aut Krasinsky G. Institute for Applied Astronomy, St. Petersburg, Russia aut Neumann G. NASA Goddard Space Flight Center, Greenbelt, MD, USA aut Oberst J. DLR Berlin Adlershof, Berlin, Germany aut Seidelmann P. University of Virginia, Charlottesville, VA, USA aut Stooke P. University of Western Ontario, London, Canada aut Tholen D. University of Hawaii, Honolulu, HI, USA aut Thomas P. Cornell University, Ithaca, NY, USA aut Williams I. Queen Mary University of London, London, UK aut Celestial Mechanics and Dynamical Astronomy Springer Netherlands 109/2(2011-02-01), 101-135 0923-2958 109:2<101 2011 109 10569 https://doi.org/10.1007/s10569-010-9320-4 text/html Onlinezugriff via DOI 1 research-article jats NATIONALLICENCE 856 40 https://doi.org/10.1007/s10569-010-9320-4 text/html Onlinezugriff via DOI NATIONALLICENCE 700 1- Archinal B. U.S. Geological Survey, Flagstaff, AZ, USA aut NATIONALLICENCE 700 1- A'Hearn M. University of Maryland, College Park, MD, USA aut NATIONALLICENCE 700 1- Bowell E. Lowell Observatory, Flagstaff, AZ, USA aut NATIONALLICENCE 700 1- Conrad A. W.M. Keck Observatory, Kamuela, HI, USA aut NATIONALLICENCE 700 1- Consolmagno G. Vatican Observatory, Vatican City, Vatican City State aut NATIONALLICENCE 700 1- Courtin R. LESIA, Observatoire de Paris, CNRS, Paris, France aut NATIONALLICENCE 700 1- Fukushima T. National Astronomical Observatory of Japan, Tokyo, Japan aut NATIONALLICENCE 700 1- Hestroffer D. IMCCE, Observatoire de Paris, CNRS, Paris, France aut NATIONALLICENCE 700 1- Hilton J. U.S. Naval Observatory, Washington, DC, USA aut NATIONALLICENCE 700 1- Krasinsky G. Institute for Applied Astronomy, St. Petersburg, Russia aut NATIONALLICENCE 700 1- Neumann G. NASA Goddard Space Flight Center, Greenbelt, MD, USA aut NATIONALLICENCE 700 1- Oberst J. DLR Berlin Adlershof, Berlin, Germany aut NATIONALLICENCE 700 1- Seidelmann P. University of Virginia, Charlottesville, VA, USA aut NATIONALLICENCE 700 1- Stooke P. University of Western Ontario, London, Canada aut NATIONALLICENCE 700 1- Tholen D. University of Hawaii, Honolulu, HI, USA aut NATIONALLICENCE 700 1- Thomas P. Cornell University, Ithaca, NY, USA aut NATIONALLICENCE 700 1- Williams I. Queen Mary University of London, London, UK aut NATIONALLICENCE 773 0- Celestial Mechanics and Dynamical Astronomy Springer Netherlands 109/2(2011-02-01), 101-135 0923-2958 109:2<101 2011 109 10569 Metadata rights reserved Springer special CC-BY-NC licence nationallicence BK010053 XK010053 XK010000 NATIONALLICENCE NATIONALLICENCE NL-springer