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Added possible number of dwarf planets with link to source.
Next follows dwarf planets, followed by Small Solar System Bodies, which are defined as "celestial bodies that are not massive enough to be rounded by their own gravity."
Next follows dwarf planets, followed by Small Solar System Bodies, which are defined as "celestial bodies that are not massive enough to be rounded by their own gravity."
As of March 19, 2013; scientists have identified 394 objects which could possibly be classified as dwarf planets by the IAU. <ref>http://www.gps.caltech.edu/~mbrown/dps.html</ref>
== Eris ==
== Eris ==