  $\iota$ Dra (HIP 75458) is a well-known example for a K giant hosting a
substellar companion since its discovery by Frink et al. (2002). We present
radial velocity measurements of this star from observations taken with three
different instruments spanning nearly 8 years. They show more clearly that the
RV period is long-lived and coherent thus supporting the companion hypothesis.
The longer time baseline now allows for a more accurate determination of the
orbit with a revised period of P=511 d and an additional small linear trend,
indicative of another companion in a wide orbit. Moreover we show that the star
exhibits low amplitude, solar like oscillations with frequencies around 3-4
d$^{-1}$ (34.7-46.3 $\mu$Hz).
