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The major eight planets are Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. The gas-giant planets have some moons as large as Mercury and the dwarf planets. Pluto was once considered a planet, but in 2006, it was re-classified as a dwarf planet, along with the asteroid Ceres and three distant Pluto-like planets : Eris, Makemake, and Haumea. Other candidates for the status are Sedna, Quaoar, Orcus, and Varuna : Sedna - The discovery of Sedna was not entirely unexpected, in that new technology is helping astronomers to look deeper into the void beyond Pluto to search out dark objects, some of them clearly sizable. If Sedna turns out to be as large as Pluto, which is still possible, then it would properly be called a dwarf planet. Pluto itself may be simply a large, spherical asteroid, accompanied by its relatively large 'moon' Charon. At the moment, Sedna is thought to be smaller than Pluto, but bigger than Quaoar, so it is by no means certain what will be decided for it in time. Sedna is currently at its closest approach to the Sun, or 'perihelion'. Its orbit is elliptical, but falls well within the boundary of the inner Oort Cloud at its most distant point. So it behaves somewhat like a planetary comet. This finding might cause astronomers to rethink the position and composition of the comet-cloud. Quaoar , Orcus, and Varuna - "50000 Quaoar" and "90482 Orcus"" also seem to have moons and all three have orbits that bring them closer to the Sun than the farthest points of Pluto's orbit. Orcus is sometimes referred to as the "anti-Pluto" because orbital resonance with Neptune keeps it on the opposite side of the Sun from Pluto. "20000 Varuna" seems to be the smallest of the current dwarf candidates. Ceres is the smallest dwarf planet. Ceres and the other asteroids of the Main Belt are much smaller than the larger planetary moons. When first discovered in 1801 Ceres was classified as a planet, but was later re-categorized as an asteroid until the category of Dwarf Planet was created in 2006.

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