A photometric period of about 380 days is found in 6810 visual magnitu
de estimates of AG Dra. This is unexpected, since the orbital period o
f the system is about 552 days. The period is confirmed by Hipparcos p
hotometry. The new periodicity provides an additional constraint on ph
ysical models for AG Dra. Detailed observations before the end of the
present outburst phase may help to clarify its nature.