That is possible, but seems unlikely to me. There are an awful lot of KBOs and other objects in the far reaches of the solar system in inclined orbits -- sometimes much more highly inclined than Pluto's. Perhaps a few are captured objects, but it seems to me that we wouldn't see as many objects inclined to the plane of the ecliptic if this only happened due to gravitational capture. My guess is that there is a trend as you get further out; perhaps early rotation in the protoplanetary nebula puts a bias on a forming object's orbit, and this bias becomes progressively less significant the further out you get. That's my hunch right now, but I don't really have the scientific background to explore it further.<br /><br />Gravitational interactions are also sometimes blamed; after all, there are definite known cases of objects changing orbital inclination due to interactions with more massive planets.<br /><br />Some have speculated that Pluto and Triton may have shared a common past. Triton orbits retrograde (backwards -- against planetary rotation) around Neptune, which is highly unstable and clear evidence that it has not always been in that orbit. Most likely, it was gravitationally captured by Neptune. And Pluto is in an orbital resonance with Neptune (2:3 if memory serves; for every three Neptune "years", Pluto has two "years"). Could a gravitational interaction with Neptune have shoved Pluto away from the ecliptic? Perhaps, but of course that doesn't explain things like Sedna, which is much too far away for that explanation. <div class="Discussion_UserSignature"> <p> </p><p><font color="#666699"><em>"People assume that time is a strict progression of cause to effect, but actually from a non-linear, non-subjective viewpoint it's more like a big ball of wibbly wobbly . . . timey wimey . . . stuff."</em> -- The Tenth Doctor, "Blink"</font></p> </div>