I'm personally rather partial to the classical definition of a planet, being a point of light that can be seen by the human eye, crossing the heavens against the background of stars at night. Mercury, Venus, Mars, Jupiter, and Saturn. But in the end, I suppose I am inclined to take more of a periodic table approach, and just expand the table when people start creating lots of new elements, like Plutonium.

Geomodder, the rest of the mass is not in planets, but in comets, satellites (moons, etc), meteoroids, and interplanetary medium.
GU Piscium b may be a brown dwarf if it is at the very high end of its mass estimate. Although, funny enough for this discussion, there is also some disagreement over the definition for where a brown dwarf begins and ends.
Regardless, the point is that the formation histories of various extrasolar systems are widely different. Our studies of other stellar proplyds and debris disks has revealed that they come in a wild variety of shapes and sizes. There are proplyd objects detected near Cygnus OB2 that are 50,000 to 100,000 AU across, which is apparently "in agreement with the theoretical scaling of proplyd size with distance from the ionizing source." HD 100546 has a binary disk, .2 to 4 AU, then after a gap, 13 to 100+ AU, with signs of a protoplanet forming at 47 AU. While Lynds 1551 IRS5's disk is apparently 20 AU across.