![Laughing :lol:](./images/smilies/icon_lol.gif)
http://news.bbc.co.uk/1/hi/sci/tech/4795755.stm
Neethis wrote:The IAC has finnally agreed, Pluto is a planet. So is Ceres, Charon, and Xena (2003 UB313). Solarsys.ssc needs updating I thinkhehe. They're putting it to a vote next month in Prague, then it becomes official...
http://news.bbc.co.uk/1/hi/sci/tech/4795755.stm
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http://www.iau2006.org/mirror/www.iau.org/iau0601/iau0601_resolution.html
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http://www.shatters.net/forum/viewtopic.php?t=7719&highlight=
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http://www.iau2006.org/mirror/www.iau.org/iau0601/iau0601_Q_A.html
The IAU has finnally agreed, Pluto is a planet. So is Ceres, Charon, and Xena (2003 UB313). Solarsys.ssc needs updating I think Laughing hehe. They're putting it to a vote next month in Prague, then it becomes official...
Malenfant wrote:
Right. So they haven't agreed to it then, have they - because they haven't voted on it yet.
Malenfant wrote:....And after all this, they didn't even bother defining the upper end of the planet scale, so we have no definitions for brown dwarfs or superjovians or gas giants.
selden wrote:The fact that it took so long would seem to give some hint as to how hard it was to come up with something that made everyone equally unhappy.
speedfreek wrote:I don't really see why Ceres shouldn't be a planet. I know its in the asteroid belt, but it orbits the sun, is certainly big enough and more importantly, spherical! It looks like a planet should look.
Could Ceres not just be a planet thats inside an asteroid belt? That seems plausible to me.
1) The object must directly orbit a star. [I guess we can make an exception for "double planets" orbiting a barycentre outside both bodies, but THAT has to be orbiting the star].
2) The upper limit of its mass is 13 Jupiter masses [if it's higher then it's a Brown Dwarf, this is the lowest mass where fusion can be initiated in the interior but not sustained] and the lower mass limit would be where it could pull itself into a sphere [personally I think that's too ambiguous. I'd say call it 1 lunar mass. Yes, it's arbitrary, but this sphere-shape definition is waaaay too fuzzy].
3) It must not have any bodies in nearby orbits (+/- 10% of its semimajor axis from the star) that are of similar mass (+/- 50% of its mass) - if four or more other such bodies are present then it's part of a swarm of bodies in a belt, and is therefore an asteroid (made of rock or ice, it doesn't matter). [the limits here may need tweaking, but you get the idea. Yes, it's arbitrary, but that doesn't matter so long as it's consistent ]
Malenfant wrote:I think that's an incredibly complicated way to classify things. One of the things I hate about the IAU proposal is that you've got "classical planets", "dwarf planets", "plutons", and all sorts of other crud we don't need.