Abstract. The PLANETS database contains the data of astrometric optical observations of the Sun and seven major planets from Mercury to Neptune, performed with meridian instruments, astrographs and astrolabes from 1960 to the present. The database structure and some problems that were resolved during the first (1980)(1981)(1982)(1983)(1984)(1985) and second (1988-1995) stages of the 15-year database history are described. The discussion focuses on the present status and future scientific applications of the database.
Key words: databases -astrometry: Sun, planets and satellitesIn the early sixties a worldwide campaign of intensive astrometric observations of the Sun and major planets, especially Mercury, Venus and Mars, was initiated. The principal campaign objectives, formulated by the IAU, were twofold: to refine the old Newcomb theory and to improve the orientation of the fundamental catalogs with respect to the dynamical reference frame. These observations continued until the early eighties when new modern numerical ephemerides were developed and more accurate analytical theories were constructed. Only six classical meridian instruments in Kislovodsk, Tashkent, Belgrade, Washington and Black Birch continue routine daytime visual observations of the Sun, Mercury and Venus. The outer planets are observed at night only with new automatic meridian circles at Bordeaux, La Palma and Tokyo.