Most of the planets found so far have been discovered with either the radial velocity or transit method. Both these methods have a strong bias toward finding massive (RV) or large (transit) planets close in to their host star. So any trends in the data need to be treated with a big grain of salt. Ideally the statistical effects of the bias should be taken into account.
One trend that does seem to be holding up: stars with more metals (elements higher atomic mass than Helium) tend to have more planets than low metalicity stars. But the strength and exact causes of this trend are debated.
Types of planets:
Jupiters 100+ Earth masses (1/3 Jupiter mass) up to about 20 Jupiter mass (Brown dwarf limit)
Saturns about 20 Earth mass to about 100 Earth Mass
Neptunes (gaseous) about 10 to about 20 Earth mass
Super Earth 3 to about 12 Earth mass (rocky, icy, water)
Earth like 1/2 to 3 Earth mass (rocky, ice/water)
Hot Jupiters etc: Jupiters etc close in to their host with high (eg 1000 K) surface temperatures. Many in Mercury sized orbits. About half are in eccentric (elongated) orbits (e or ecc values 0 to 1 in tables)
Cold Jupiters etc: planets beyond the "snow line". The snow line is the distance at which water will be ice. In our solar system roughly in the asteroid belt.