VI/88ivo://CDS.VizieR/VI/88CDSChapront J.Francou G.Bureau des Longitudes (France).CDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frephemeridesPluto's motion has been represented with series resulting of an approximation by frequency analysis (see Chapront 1995) of JPL numerical integration DE200. Series represent the heliocentric coordinates of Pluto as functions of time between 1700 and 2100. This catalog completes the VSOP87 theories developed at the Bureau des Longitudes (see Cat. <VI/81>) Authors' Address: J. Chapront, G. Francou Bureau des Longitudes Group : Dynamics of Solar System 77, avenue Denfert-Rochereau F-75014 Paris - France E-mail : jchapron@bdl.fr francou@bdl.fr Phone : (33) 1 40 51 22 71 (33) 1 40 51 22 60 Fax : (33) 1 46 33 28 34 Contents: The presentation of the tables is given in file : pluto.txt. A Fortran subroutine pluto.sub (95.1) is provided for the computation of the heliocentric rectangular positions and velocities of Pluto.Bureau des Longitudes, Group : Dynamics of Solar System (1995)https://cdsarc.cds.unistra.fr/viz-bin/cat/VI/88CatalogResearchIsServedByTAP VizieR generic servicerelated-toVI/81 : Planetary Solutions VSOP87 (Bretagnon+, 1988)VI/87 : Planetary Ephemerides based on DE403 (Chapront+ 1996)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=VI/88https://vizier.iucaa.in/viz-bin/VizieR-2?-source=VI/88http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=VI/88https://vizier.cds.unistra.fr/viz-bin/votable?-source=VI/88https://vizier.iucaa.in/viz-bin/votable?-source=VI/88http://vizieridia.saao.ac.za/viz-bin/votable?-source=VI/88GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefault