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Dwarf planet candidates

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Prime plutoid candidates[1]
Name Category Estimated diameter (km) Absolute
Magnitude

(H)
Mass
(×1020 kg)
Orbital
radius
(AU)
by [2] by [3] by [4] by [5]
Orcus plutino
(1 moon)
1,100 909 946 1,500 2.3 6.32 ± 0.05 39.2
Huya plutino 480 480 4.7 0.6–1.8? 39.4
Pluto plutoid 2,306 –0.7 130 39.4
Ixion plutino 980 570 650 1,065 3.2 ~3? 39.6
Varuna cubewano 780 874 500 900 3.7 ~3.7? 42.9
Haumea plutoid 1,436 0.17 40 43.3
Quaoar cubewano
(1 moon)
1,290 1,260 844 1,200 2.7 21–29 43.5
Makemake plutoid 1,500 –0.45 30 45.3
(55565) 2002 AW197 cubewano 940 793 735 890 3.2 ~4.1? 47.0
(84522) 2002 TC302 5:2 SDO 710 1,200 1,150 3.8 15? 55.4
(225088) 2007 OR10 10:3? SDO 1200? 1.9 ? 67.3
Eris plutoid 2,600 –1.12 167 68.0
(15874) 1996 TL66 SDO 632 460–690 5.4 2? 83.9
Sedna Detached object 1,800 1,500 < 1,600 < 1,500 1.5 8–70? 509
  1. ^ All bodies with estimated diameters of 900 km or more, with 3 additional prime suspects (Huya, 2007 OR10, 1996 TL66) cited in Tancredi & Favre. "Which are the dwarfs in the Solar system?" (PDF). Asteroids, Comets, Meteors. Retrieved 2008-09-20.
  2. ^ Mike Brown. "The Dwarf Planets". Retrieved 2008-01-20.
  3. ^ Johnston, Robert (2007-11-24). "List of Known Trans-Neptunian Objects". Johnston's Archive.net. Retrieved 2008-01-26.
  4. ^ Barucci, M.A. (2007). "Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope". The Solar System beyond Neptune. University of Arizona Press. arXiv:astro-ph/0702538. Bibcode:2008ssbn.book..161S. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  5. ^ David C. Jewitt. "Kuiper Belt: The 1000 km Scale KBOs". University of Hawaii, Institute for Astronomy. Retrieved 2008-02-10.