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| | == The dwarf planet controversy == | | == The dwarf planet controversy == |
| | [[Image:Pluto3.gif|left|thumb|Pluto(center) with moon [[Charon]]. NASA image]] | | [[Image:Pluto3.gif|left|thumb|Pluto(center) with moon [[Charon]]. NASA image]] |
| − | The discovery of [[Eris]], a scatter-disk body 27% more massive than Pluto, caused a controversy concerning what does, and what does not, constitute a [[planet]]. If Pluto were to retain its historical designation of "planet," then Eris would also qualify. But Eris was held not to qualify because it was in a neighborhood with multiple other objects, a situation similar to those of similar bodies in the [[asteroid]] belt, namely [[Ceres]] and [[Eros]]. | + | The discovery of [[Eris]], a scatter-disk body 27% more massive than Pluto, caused a controversy concerning what does, and what does not, constitute a [[planet]]. If Pluto were to retain its historical designation of "planet," then Eris would also qualify. But Eris was held not to qualify because it was in a neighborhood with multiple other objects, a situation similar to those of similar bodies in the [[asteroid]] belt, namely [[Ceres]] and [[Eris]]. |
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| | In 2006, the [[International Astronomical Union]] passed the following resolution:{{cquote|'''RESOLUTION 5A''' | | In 2006, the [[International Astronomical Union]] passed the following resolution:{{cquote|'''RESOLUTION 5A''' |
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| | Brown suspects the IAU wanted to demote Pluto, because Pluto violates, by its very existence, every conventional theory of planetary origin. | | Brown suspects the IAU wanted to demote Pluto, because Pluto violates, by its very existence, every conventional theory of planetary origin. |
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| | + | According to Number 1 (c) and 2 (c) of the IAU definition, also [[Earth]] and [[Mars]] wouldn't be planets because they haven't "cleared" their orbits, but have several asteroids in them, also called "quasi-moons" of Earth and Mars. |
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| | == Orbital characteristics == | | == Orbital characteristics == |