All data in the B band for quasar 3C 345 have been compiled into a lig
ht curve from twenty one publications, dating back to 1896; 1642 value
s are available. The light curve shows that 3C 345 is very active and
exhibits very complicated nonsinusoidal variations. Using this data we
have found a period of 10.1+/-0.8 years (or 21.8+/-1.5 years) for the
outbursts in 3C 345. This value is in good agreement with the period
of 11.4 year between outbursts found previously by Webb et al. (1988).
Based on this period we can predict that the next outburst should be
at its maximum around January 2002.