UBV(RI)(c) observations of a G6/G8 IV star HD 17025 suggest a variatio
n period of about 9 days. The light curve has a marginal amplitude of
about 0.015 of a magnitude but is poorly defined and needs an independ
ent confirmation. No prominent chromospheric emission is visible in a
spectrum of this star. The other observed star, a K2 dwarf HD 38392, d
id not show measurable light variations over a two weeks period of obs
ervations.