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  2. List of the brightest Kuiper belt objects - Wikipedia

    en.wikipedia.org/wiki/List_of_the_brightest...

    Other objects, such as 28978 Ixion (discovered in 2001) and 20000 Varuna (discovered in 2000) measure roughly 500 km across. [1] This has led gradually to the acceptance of Pluto as the largest member of the Kuiper belt. [citation needed] The brightest known dwarf planets and other KBOs (with absolute magnitudes < 4.0) are:

  3. List of trans-Neptunian objects - Wikipedia

    en.wikipedia.org/.../List_of_trans-Neptunian_objects

    This is a list of trans-Neptunian objects (TNOs), which are minor planets in the Solar System that orbit the Sun at a greater distance on average than Neptune, that is, their orbit has a semi-major axis greater than 30.1 astronomical units (AU). The Kuiper belt, scattered disk, and Oort cloud are three conventional divisions of this volume of ...

  4. Kuiper belt - Wikipedia

    en.wikipedia.org/wiki/Kuiper_belt

    While many asteroids are composed primarily of rock and metal, most Kuiper belt objects are composed largely of frozen volatiles (termed "ices"), such as methane, ammonia, and water. The Kuiper belt is home to most of the objects that astronomers generally accept as dwarf planets: Orcus, Pluto, [5] Haumea, [6] Quaoar, and Makemake. [7]

  5. List of Solar System objects - Wikipedia

    en.wikipedia.org/wiki/List_of_Solar_System_objects

    Euler diagram showing the types of bodies orbiting the Sun. The following is a list of Solar System objects by orbit, ordered by increasing distance from the Sun.Most named objects in this list have a diameter of 500 km or more.

  6. Category:Kuiper belt objects - Wikipedia

    en.wikipedia.org/wiki/Category:Kuiper_belt_objects

    All asteroids should be sorted using a 0-padded 6-digit sortkey based on their numerical designation.Otherwise, their provisional designation should be used. For example:

  7. Solar System belts - Wikipedia

    en.wikipedia.org/wiki/Solar_System_belts

    Ceres, 2.8 AU in the asteroid belt; Orcus 39.4 AU, Trans-Neptunian-Kuiper belt object; Pluto 39 AU, Kuiper belt (a planet until 2006) Haumea 43 AU, Kuiper belt; Makemake 45.8 AU, Kuiper belt; Eris 95.6 AU, Kuiper belt; Gonggong Scattered disc object, 34 to 101 AU; Quaoar Kuiper belt object, 41.9 to 45.4 AU; Sedna 76 to 506 AU

  8. File:TheKuiperBelt 75AU All.svg - Wikipedia

    en.wikipedia.org/wiki/File:TheKuiperBelt_75AU...

    (voir plus loin pour la description en français) Distribution of Kuiper belt objects' orbits. Objects in resonance are plotted in red (Neptune trojans 1:1, plutinos 2:3, twotinos 1:2,…). Confirmed plutinos are in dark red. Classical objects are plotted in blue. Scattered disk objects (not members of the Kuiper Belt) are shown in grey for ...

  9. (55636) 2002 TX300 - Wikipedia

    en.wikipedia.org/wiki/(55636)_2002_TX300

    2002 TX 300 is a classical Kuiper belt object with an absolute magnitude between that of 50000 Quaoar and 20000 Varuna. 2002 TX 300 has the most eccentric and inclined orbit of the three. A variability of the visual brightness was also detected which could fit to 7.9 h or 15.8 h rotational period (the distinction between single or double-peaked ...