Report of the IAU/IAG Working Group on cartographic coordinates and rotational elements: 2006 |
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Authors: | P Kenneth Seidelmann B A Archinal M F A’hearn A Conrad G J Consolmagno D Hestroffer J L Hilton G A Krasinsky G Neumann J Oberst P Stooke E F Tedesco D J Tholen P C Thomas I P Williams |
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Institution: | (1) University of Virginia, Charlottesville, VA, USA;(2) U.S. Geological Survey, Flagstaff, AZ, USA;(3) University of Maryland, College Park, MD, USA;(4) W. M. Keck Observatory, Kamuela, HI, USA;(5) Vatican Observatory, Vatican City State, Italy;(6) IMCCE, Paris Observatory, CNRS, Paris, France;(7) U.S. Naval Observatory, Washington DC, USA;(8) Institute for Applied Astronomy, St. Petersburg, Russia;(9) NASA Goddard Space Flight Center, Greenbelt, MD, USA;(10) DLR Berlin Adlershof, Berlin, Germany;(11) University of Western Ontario, London, Canada;(12) University of New Hampshire, Durham, NH, USA;(13) University of Hawaii, Honolulu, HI, USA;(14) Cornell University, Ithaca, NY, USA;(15) Queen Mary, University of London, London, UK |
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Abstract: | Every three years the IAU/IAG 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
introduces improved values for the pole and rotation rate of Pluto, Charon, and Phoebe, the pole of Jupiter, the sizes and
shapes of Saturn satellites and Charon, and the poles, rotation rates, and sizes of some minor planets and comets. A high
precision realization for the pole and rotation rate of the Moon is provided. The expression for the Sun’s rotation has been
changed to be consistent with the planets and to account for light travel time |
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Keywords: | Cartographic coordinates Rotation axes Rotation periods Sizes Shapes Planets Satellites Minor planets Comets |
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