  We report on 5.4 yr of phase-coherent timing, using the Rossi X-ray Timing
Explorer, of the X-ray pulsar 1RXS 1708-4009, a member of the class known as
``anomalous X-ray pulsars.'' This object exhibited a rotational glitch in 1999.
Here we report a second much larger rotational glitch which occured ~1.5 yr
after the first. We show that the recoveries from the two glitches are
different, with the first showing only a possible slow, approximately linear
recovery, while the second showed a nearly complete recovery on a time scale of
\~50 days. The approximately exponential recovery time scale of the second
glitch is similar to that seen recently in 1E 2259+586 at the time of a major
outburst. This suggests 1RXS 1708-4009 undergoes similar bursting behavior,
although with our sparse observations we have detected no other evidence for
bursts from this source.
