Pluto: Pagkakaiba sa mga binago

<!--{{efn| name = wiki-kbo| The dwarf planet [[Eris (dwarf planet)|Eris]] is roughly the same size as Pluto, about 2330&nbsp;km; Eris is, however, 28% more massive than Pluto. [[Eris (dwarf planet)|Eris]] is a [[scattered-disc object]], often considered a distinct population from Kuiper-belt objects like Pluto; Pluto is the largest body in the Kuiper belt proper, which excludes the scattered-disc objects.}}-->

<!--{{efn| name = Perihelion| 1 = The discovery of Charon in 1978 allowed astronomers to accurately calculate the mass of the Plutonian system. But it did not indicate the two bodies' individual masses, which could only be estimated after other moons of Pluto's were discovered in late 2005. As a result, because Pluto came to perihelion in 1989, most Pluto perihelion date estimates are based on the Pluto–Charon [[barycenter]]. Charon came to perihelion [http://ssd.jpl.nasa.gov/horizons.cgi?find_body=1&body_group=mb&sstr=901 4 September 1989.] The Pluto–Charon barycenter came to perihelion [http://ssd.jpl.nasa.gov/horizons.cgi?find_body=1&body_group=mb&sstr=9 5 September 1989.] Pluto came to perihelion [http://ssd.jpl.nasa.gov/horizons.cgi?find_body=1&body_group=mb&sstr=999 8 September 1989.]}}-->