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  2. Makemake - Wikipedia

    en.wikipedia.org/wiki/Makemake

    Makemake [e] (minor-planet designation: 136472 Makemake) is a dwarf planet and the largest of what is known as the classical population of Kuiper belt objects, [b] with a diameter approximately that of Saturn's moon Iapetus, or 60% that of Pluto. [24] [25] It has one known satellite. [26]

  3. Category:Makemake - Wikipedia

    en.wikipedia.org/wiki/Category:Makemake

    Download as PDF; Printable version; In other projects Wikimedia Commons; ... Pages in category "Makemake" The following 4 pages are in this category, out of 4 total.

  4. S/2015 (136472) 1 - Wikipedia

    en.wikipedia.org/wiki/S/2015_(136472)_1

    S/2015 (136472) 1, unofficially nicknamed MK2 by the discovery team, [2] is the only known moon of the trans-Neptunian dwarf planet Makemake. [1] [4] It is estimated to be 175 km (110 mi) in diameter and has a semi-major axis of at least 21,000 km (13,000 mi) from Makemake. [1] Its orbital period is at least 12 days if it has a circular orbit.

  5. Wikipedia : Featured article candidates/Makemake (dwarf planet)

    en.wikipedia.org/.../Makemake_(dwarf_planet)

    As far as anyone can tell, Image:Makemake precovery.jpg is the only photograph of makemake on the internet at all. Regardless, any images not taken by NASA would be copyrighted by the observatory from which they were taken, and it doesn't appear that NASA has imaged this planet dwarf planet yet (as strange as that seems). If you can find ...

  6. (230965) 2004 XA192 - Wikipedia

    en.wikipedia.org/wiki/(230965)_2004_XA192

    This article about a centaur (minor planet) or trans-Neptunian object is a stub. You can help Wikipedia by expanding it.

  7. (120132) 2003 FY128 - Wikipedia

    en.wikipedia.org/wiki/(120132)_2003_FY128

    This article about a centaur (minor planet) or trans-Neptunian object is a stub. You can help Wikipedia by expanding it.

  8. Dwarf planet - Wikipedia

    en.wikipedia.org/wiki/Dwarf_planet

    The second resolution, 5B, defined dwarf planets as a subtype of planet, as Stern had originally intended, distinguished from the other eight that were to be called "classical planets". Under this arrangement, the twelve planets of the rejected proposal were to be preserved in a distinction between eight classical planets and four dwarf planets.

  9. (90568) 2004 GV9 - Wikipedia

    en.wikipedia.org/wiki/(90568)_2004_GV9

    M. E. Brown estimates that is very likely a dwarf planet. [9] A diameter of 680 ± 34 km has been determined from combined observations of the Herschel and Spitzer space telescopes. [ 5 ] Tancredi notes that light-curve-amplitude analysis shows only small deviations, suggesting that (90568) 2004 GV 9 could be a spheroid with small albedo spots ...