Is there a way to estimate or calculate the tidal range induced on a water-bearing planet?
Wikipeida (quoting Icarus ) gives
$$\frac{15}{8}\frac{mA^4}{Mr^3}$$
Where $m$ and $M$ are the masses of the moon and planet, respectively; $r$ is the orbit radius of the moon and $A$ is the radius of the planet. For Earth this is a little less than a metre.
Systems with multiple moons (or moon and sun, like on Earth) will have multiple bulges which can add up.
This tells you very little about the sizes of actual tides, which are strongly magnified by topography. It predicts tides of 0.7 m, whereas real tides have ranges of between 0 and 16 m.