Optical CCD astrometry was done at the U.S. Naval Observatory FIagstaf
f Station to obtain positions of solar system bodies to be encountered
by the Galileo spacecraft. The objects observed were the minor planet
s 951 Gaspra and 243 Ida, discussed in this paper, and the Galilean sa
tellites of Jupiter, to be discussed in Paper II. Observations of Gasp
ra were made from April through August 1991, and Ida was observed from
1991 November through 1993 May. Each observing campaign was followed
by a successful encounter. The instrumentation, techniques, analysis m
ethods, and astrometric results are described.