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  2. Kuiper belt - Wikipedia

    en.wikipedia.org/wiki/Kuiper_belt

    The scattered disc was created when Neptune migrated outward into the proto-Kuiper belt, which at the time was much closer to the Sun, and left in its wake a population of dynamically stable objects that could never be affected by its orbit (the Kuiper belt proper), and a population whose perihelia are close enough that Neptune can still ...

  3. 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:

  4. Classical Kuiper belt object - Wikipedia

    en.wikipedia.org/wiki/Classical_Kuiper_belt_object

    A classical Kuiper belt object, also called a cubewano (/ ˌ k juː b iː ˈ w ʌ n oʊ / "QB1-o"), [a] is a low-eccentricity Kuiper belt object (KBO) that orbits beyond Neptune and is not controlled by an orbital resonance with Neptune. Cubewanos have orbits with semi-major axes in the 40–50 AU range and, unlike Pluto, do not cross Neptune's ...

  5. 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:

  6. 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 ...

  7. Category:Classical Kuiper belt objects - Wikipedia

    en.wikipedia.org/wiki/Category:Classical_Kuiper...

    0–9. 1999 OD4; 1999 OZ3; 19521 Chaos; 20000 Varuna (24835) 1995 SM55 (35671) 1998 SN165 (49673) 1999 RA215; Quaoar (55565) 2002 AW197 (55636) 2002 TX300 (55637) 2002 UX25

  8. 486958 Arrokoth - Wikipedia

    en.wikipedia.org/wiki/486958_Arrokoth

    486958 Arrokoth (provisional designation 2014 MU 69; formerly nicknamed Ultima Thule [a]) is a trans-Neptunian object located in the Kuiper belt.Arrokoth became the farthest and most primitive object in the Solar System visited by a spacecraft when the NASA space probe New Horizons conducted a flyby on 1 January 2019.

  9. (307261) 2002 MS4 - Wikipedia

    en.wikipedia.org/wiki/(307261)_2002_MS4

    (307261) 2002 MS 4 (provisional designation 2002 MS 4) is a large trans-Neptunian object in the Kuiper belt, which is a region of icy planetesimals beyond Neptune.It was discovered on 18 June 2002 by Chad Trujillo and Michael Brown during their search for bright, Pluto-sized Kuiper belt objects at Palomar Observatory.