<blockquote><font class="small">In reply to:</font><hr /><p>Neither the original proposal nor the revision would likely be applicable to all Extrasolar planetary systems; there are certainly going to be systems that are just too alien to fit into a simple classification system -- this is "Bodes Law" kind of thinking. <br /><br />I really like that the new proposal keeps the planet designation only for the largest and most significant members of Solar Systems; the original plan was just too revisionist -- not everything under the Sun needs to be called a planet. <p><hr /></p></p></blockquote><br /><br />Aside from the "pluton" junk, I think the first definition is the most applicable one can get for other stellar systems. Large enough to gravitationally become round, too small to fuse, orbits a star. Simple. Once it's determined an object orbits a star, all that has to be confirmed is size (and shape if its between 400-1000km or so).<br /><br />Adding in orbital dominance as a criteria opens the door for many more arbitrary limits and cutoffs. What constitutes orbital dominance? 70% orbital mass? 80%? How spread out can a belt get while still remaining a belt? Realize the Kuiper Belt is wider than the distance between Mercury and Neptune...<br /><br />While I'm on the subject, is Sedna a planet? Right now it's not known to share its orbit with other bodies, so technically it qualifies as a planet. Sure, there may be other objects near it but we don't know that for sure now. So what do we do? <br /><br />Orbital dominance criteria also means more demotions. Let's say we find an object by itself and it's classified a planet. Then some time later, other objects are found and it's considered to be in a "belt" and not a planet. Pluto redux...and I rather not go through this kind of debate again. <br /><br />Yet another issue...with very small systems now being discovered, it is not a stretch to believe there could be an "orbitally dominant" Ceres-sized object out there. If that's the case, then