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  2. Haumea - Wikipedia

    en.wikipedia.org/wiki/Haumea

    Haumea (minor-planet designation: 136108 Haumea) is a dwarf planet located beyond Neptune's orbit. [25] It was discovered in 2004 by a team headed by Mike Brown of Caltech at the Palomar Observatory, and formally announced in 2005 by a team headed by José Luis Ortiz Moreno at the Sierra Nevada Observatory in Spain, who had discovered it that year in precovery images taken by the team in 2003.

  3. Haumea family - Wikipedia

    en.wikipedia.org/wiki/Haumea_family

    Orbits of Haumea family members, sharing semimajor axes around 43 AU, and inclinations around 27°.. The dwarf planet Haumea is the largest member of the family, and the core of the differentiated progenitor; other identified members are the moons of Haumea and the Kuiper belt objects (55636) 2002 TX 300, (24835) 1995 SM 55, (19308) 1996 TO 66, (120178) 2003 OP 32, (145453) 2005 RR 43, (86047 ...

  4. List of trans-Neptunian objects - Wikipedia

    en.wikipedia.org/wiki/List_of_trans-Neptunian...

    The largest known trans-Neptunian objects are Pluto and Eris, followed by Haumea, Makemake, Gonggong, Quaoar, Sedna, and Orcus, all of them being officially recognized as dwarf planets by the IAU except for Gonggong, Sedna, and Orcus. There are also many possible dwarf planets, such as Salacia, (307261) 2002 MS 4, Varda, Ixion, and Varuna.

  5. File:TheKuiperBelt Orbits Haumea moons.svg - Wikipedia

    en.wikipedia.org/wiki/File:TheKuiperBelt_Orbits...

    The view from the pole of the Hi'iaka's orbit The view from the plane of the Hi'iaka's orbit. Orbits Hi'iaka in blue; Namaka in green; The orbit Namaka is plotted in a brighter colour above the plane of the orbit of Hi'iaka and in a darker colour below.

  6. Category:Haumea family - Wikipedia

    en.wikipedia.org/wiki/Category:Haumea_family

    Haumea (dwarf planet) (1 C, 5 P) Pages in category "Haumea family" The following 16 pages are in this category, out of 16 total. ... This page was last edited on 19 ...

  7. (24835) 1995 SM55 - Wikipedia

    en.wikipedia.org/wiki/(24835)_1995_SM55

    1995 SM 55 is a member of the Haumea family. [3] It has the highest collisional velocity, a δv of 123.3 m/s, of all confirmed members. [19] Based on their common pattern of IR water-ice absorptions, neutral visible spectrum [20] and the clustering of their orbital elements, the other KBOs 1996 TO 66, 2002 TX 300, 2003 OP 32 and 2005 RR 43 all appear to be collisional fragments broken off of ...

  8. Category:Haumea (dwarf planet) - Wikipedia

    en.wikipedia.org/wiki/Category:Haumea_(dwarf_planet)

    Haumea is a dwarf planet in the Kuiper belt, and named after the Hawaiian goddess of childbirth – see Haumea (mythology). Subcategories. This category has only the ...

  9. List of gravitationally rounded objects of the Solar System

    en.wikipedia.org/wiki/List_of_gravitationally...

    The radii of these objects range over three orders of magnitude, from planetary-mass objects like dwarf planets and some moons to the planets and the Sun. This list does not include small Solar System bodies , but it does include a sample of possible planetary-mass objects whose shapes have yet to be determined.

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