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Results from BVRI photometric observations of the young stellar object V2492Cyg collected during the period from August 2010 to December 2017 arepresented. The star is located in the field of the Pelican Nebula and it wasdiscovered in 2010 due to its remarkable increase in the brightness by morethan 5 mag in R-band. According to the first hypothesis of the variabilityV2492 Cyg is an FUor candidate. During subsequent observations it was reportedthat the star shows the characteristics inherent to EXor- and UXor-typevariables. The optical data show that during the whole time of observations thestar exhibits multiple large amplitude increases and drops in the brightness.In the beginning of 2017 we registered a significant increase in the opticalbrightness of V2492 Cyg, which seriously exceeds the maximal magnitudesregistered after 2010.

V2492 Cygni: Optical BVRI variability during the period 2010-2017