  We present an updated measurement of orbital period evolution of LMXB XTE
J1710-281 by using eclipse timing technique. Using data obtained with
XMM-Newton, Suzaku, RXTE, Chandra and AstroSat observatories, we report 21 new
measurements of X-ray mid-eclipse times. We have discovered a third orbital
period glitch in XTE J1710-281 with an F-test false alarm probability of ~0.7%
for occurrence of the third glitch and report detection of four distinct epochs
of orbital period in this system. This work presents a more robust estimation
of occurrence of the second orbital period glitch. However, the epoch of
occurrence of the third glitch is poorly constrained, between MJD 55726 to
56402. We have put lower limits of 1.48 ms, 0.97 ms and 0.45 ms, on sudden
changes in orbital period between the successive epochs. We discuss the
implications of our findings in context of magnetic nature of the companion
star and possible scattering events with circum-binary objects around this
binary system.
