In 1999 and 2000 we obtained spectroscopic and photometric observations of
the A-type binary star HD 169981. The observations were part of a campaign
to search for short-term photometric and radial-velocity variations among e
arly-type binaries. From the radial velocities of 18 metal lines we derived
more precise orbital elements. Quite unexpectedly, our photometric data sh
ow a dip that could be caused by an eclipse. The same feature is also visib
le in the Hipparcos data. From our analysis of the available observations w
e have estimated the physical parameters of the binary. Neither the spectro
scopic nor the photometric observations hint at any short-term variations.