A new X-ray transient, designated XTE J1739-302, was discovered with t
he proportional counter array on the Rossi X-Ray Timing Explorer in da
ta from 1997 August 12. Although it was the brightest source in the Ga
lactic center region while active (about 3.0 x 10(-9) ergs cm(-2) s(-1
) from 2 to 25 keV), it was only observed on that one day; it was not
detectable 9 days earlier or 2 days later. There is no known counterpa
rt at other wavelengths, and its proximity to the Galactic center will
make such an identification difficult due to source confusion and ext
inction. The X-ray spectrum and intensity suggest a giant outburst of
a Be/neutron star binary, although no pulsations were observed and the
outburst was shorter than is usual from these systems.