<p>There are two different competing ways that people distinguish between planets and brown dwarfs/stars. </p><p>As others have mentioned, the simplest is really in terms of mass. A solar composition object that is larger than about 80 jupiter masses will, as it collapses, reach a point where hydrogen fusion ignites in its core preventing further collapse - such an object is called a star. An object that is smaller than this but larger than about 13 jupiter masses will reach a point where deuterium fusion ignites in its core, but the deuterium burns out very quickly and the object will then continue to collapse until the core becomes degenerate and supports it from further collapse - it never achieves hydrogen ignition, however. Such an object is called a brown dwarf. If the object is less than 13 jupiter masses it will be held up by degeneracy pressure (or static coulomb forces in the case of small planets) and never even achieve deuterium fusion. Such an object is deemed a planet. So for this nomenclature Jupiter is a planets (it would be a failed star by a factor of ~80 and a failed brown dwarf by a factor of ~13). Note that the deuterium burning only has a fairly minor effect on the life of a brown dwarf - it keeps it hot and shining for a little while longer than you would naively expect. In simplest terms a brown dwarf is just a bigger, hotter version of jupiter (though the word "just" sweeps under the rug all the neat differences in the atmospheres that come into play as the temperature changes). </p><p> The other way that's been proposed to classify objects is based on how they're formed. This method is quite a bit more speculative at present than the one described above, but it may in time prove to be a very useful way to think about things. In this scheme, stars/brown dwarfs are objects that form from direct gravitational collapse out of the interstellar medium. Planets are objects that coallesce in the debris disks that form around baby stars. Jupiter would definitely be a planet since it presumably was born in the disk that existed around the pre-main sequence sun. You may, however, have free floating Jupiter-sized objects that formed as stars (direct graviational collapse) but never got very big - these would be considered failed stars rather than planets. There may also be objects larger than 13 jupiter masses that formed in stellar disks and would thus be considered planets rather than brown dwarfs or failed stars (despite the fact that they'd be large enough for deuterium fusion). The mass function, though, appears to drop off precipitously toward higher masses for planets orbiting close to their stars (ones that seem likely to have formed in stellar disks), and so we know these brown-dwarf massed planets are quite rare (at least for sun-like stars, for larger stars it's harder to say because we don't have a very good census of planets around A-type and hotter stars). This method is speculative since it's not all that clear how gas planets form - the most popular model is that they form first by accreting a core out of the debris in the disk, and then capturing a massive gas atmosphere - but they may very well form by direct gravitational collapse of the gas in the disk. </p> <div class="Discussion_UserSignature"> </div>