  We present the first observations of the circumstellar (CS) disk system 51
Ophiuchi with the Far Ultraviolet Spectroscopic Explorer. We detect several
absorption lines arising from the unusual metastable atomic species NI (2D), NI
(2P), and SII (2D). These levels lie 1.8 - 3.6 eV above the ground level and
have radiative decay lifetimes of 2 days or less, indicating that the lines
arise from warm CS gas. The high S/N FUSE spectra, obtained six days apart,
also show time-variable absorption features arising from NI, NII, OI (1D), and
FeIII, which are redshifted with respect to the stellar velocity. The resolved
redshifted absorption extends over many tens of km/s (40 for NI, 100 for NII,
65 for OI, and 84 for FeIII). We calculate column densities for all the
variable infalling CS gasses, using the apparent optical depth method. The
FeIII and NII infalling gasses must be produced through collisional ionization,
and the ionization fraction of nitrogen suggests a gas temperature between
20000 and 34000 K. The infalling gas shows a peculiar, non-solar composition,
with nitrogen and iron more abundant than carbon. We also set upper limits on
the line-of-sight column densities of molecular hydrogen and carbon monoxide.
These observations strengthen the connection between 51 Oph and the older
debris-disk system Beta Pictoris, and indicate that there may be infalling
planetesimals in the 51 Oph system.
