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  2. Category:Kuiper belt objects - Wikipedia

    en.wikipedia.org/wiki/Category:Kuiper_belt_objects

    Pages in category "Kuiper belt objects" The following 13 pages are in this category, out of 13 total. This list may not reflect recent changes. ...

  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. 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 ...

  5. Category:Classical Kuiper belt objects - Wikipedia

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

    Cold classical Kuiper belt objects (1 C, 107 P) M. Makemake (4 P) Q. 50000 Quaoar (4 P) S. 120347 Salacia (3 P) V. 174567 Varda (2 P) Pages in category "Classical ...

  6. Deep Ecliptic Survey - Wikipedia

    en.wikipedia.org/wiki/Deep_Ecliptic_Survey

    Since 1998 through the end of 2003, the survey covered 550 square degrees with sensitivity of 22.5, which means an estimated 50% of objects of this magnitude have been found. The survey has also established the mean Kuiper Belt plane and introduced new formal definitions of the dynamical classes of Kuiper belt objects.

  7. 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 ...

  8. (55636) 2002 TX300 - Wikipedia

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

    The present positions (as of April 2006) are marked with the spheres, illustrating relative sizes and differences in albedo (both objects appear neutral in the visible spectrum). 2002 TX 300 is classified as a classical Kuiper belt object and follows an orbit very similar to that of Haumea : highly inclined (26°) and moderately eccentric (e ~0 ...

  9. File:Kuiper belt plot objects of outer solar system.png

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

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