  We report on millisecond variability from the X-ray transient XTE J1739-285.
We detected six X-ray type I bursts and found evidence for oscillations at 1122
+/- 0.3 Hz in the brightest X-ray burst. Taking into consideration the power in
the oscillations and the number of trials in the search, the detection is
significant at the 99.96% confidence level. If the oscillations are confirmed,
the oscillation frequency would suggest that XTE J1739-285 contains the fastest
rotating neutron star yet found. We also found millisecond quasiperiodic
oscillations in the persistent emission with frequencies ranging from 757 Hz to
862 Hz. Using the brightest burst, we derive an upper limit on the source
distance of about 10.6 kpc.
