  Results from BVRI photometric observations of the young stellar object V2492
Cyg collected during the period from August 2010 to December 2017 are
presented. The star is located in the field of the Pelican Nebula and it was
discovered in 2010 due to its remarkable increase in the brightness by more
than 5 mag in R-band. According to the first hypothesis of the variability
V2492 Cyg is an FUor candidate. During subsequent observations it was reported
that the star shows the characteristics inherent to EXor- and UXor-type
variables. The optical data show that during the whole time of observations the
star exhibits multiple large amplitude increases and drops in the brightness.
In the beginning of 2017 we registered a significant increase in the optical
brightness of V2492 Cyg, which seriously exceeds the maximal magnitudes
registered after 2010.
