J
jaxtraw
Guest
"There are plenty of other KBO objects of similar mass in the vicinity of Pluto. Even if they aren't right next to it, they are far closer in size, and orbit than for any other planet."<br /><br />I'm not disputing this. I'm simply asking somebody to justify why, from first principles, this should be a criterion for planethood. It has nothing for instance to do with the body itself- why does it make sense to define a planet purely in terms of its neighbours?<br /><br />Back with Jupier and Mercury- they really have nothing whatsoever in common. One is a very small rocky body, the other a vast agglomeration of gases, largely hydrogen. They don't share any traits at all. I wonder if intelligent beings had evolved on a Jovian moon, they'd probably relegate Mercury and the other terrestrials as unimportant "solar satellites" <img src="/images/icons/smile.gif" /><br /><br />There are clearly two very, very distinct classes of planet- gas giants and terrestrials, so vastly different that "planet" can only loosely mean "body that orbits the Sun". I would add a third category- icy planets- the members of which more closely resemble the terrestrials than the terrestrials do the gas giants. It'd probably make more sense to have "gas planets" and "solid planets" with the latter subdivided into "rockies" and "icies". Astronomers are then free to define sub-groupings of them by composition, size, orbital characteristics, or any other useful categorisations.<br /><br />And I still think that the idea of "demotion" is inherently wrong. As Enceladus has shown, we really don't know which worlds are the interesting ones until we get a spacecraft or two there <img src="/images/icons/smile.gif" />