We present observations of the M87 jet made with the Faint Object Camera on
board the Hubble Space Telescope at five epochs between 1994 and 1998. The
se observations reveal 10 superluminal features within the first 6 " of the
jet, with eight of these having apparent speeds in the range 4c-6c. Two ad
ditional features within the first arcsecond of the jet have subluminal spe
eds of 0.63c and 0.84c. The latter of these, named HST-1 East, appears to e
mit new superluminal features moving at 6c, which subsequently fade with a
half-intensity timescale of similar to 2 yr. The fastest speeds we observe
require a Lorentz factor gamma greater than or equal to 6 for the bulk flow
and a jet orientation within 19 degrees of the line of sight, in the conte
xt of the relativistic jet model. Finding such large gamma in an FR I radio
source like M87 strongly supports BL Lac/FR I unification models. These la
rge speeds help to mitigate the particle lifetime problem posed by the opti
cal emission, as well as the jet confinement problem.