Cinto de Kuiper: Diferenzas entre revisións
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Liña 8:
* [[90482 Orcus]] (1.500 - 2.600 km)
* [[Makemake (planeta anano)|Makemake]] (1.360 - 1.480 kms.<ref name=Lim2010>{{cita publicación periódica |autor=T.L. Lim, J. Stansberry, T.G. Müller|título=“TNOs are Cool”: A survey of the trans-Neptunian region III. Thermophysical properties of 90482 Orcus and 136472 Makemake|ano=2010| volume=518|páxina=L148|doi=10.1051/0004-6361/201014701|revista=Astronomy and Astrophysics|bibcode=2010A&A...518L.148L}}</ref>), [[Haumea (planeta anano)|Haumea]] (~1.150<ref name="spitzer haumea">
{{Cita
|título=Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope
|autor=John Stansberry, Will Grundy, Mike Brown, Dale Cruikshank, John Spencer, David Trilling, Jean-Luc Margot
Liña 45:
|ano=2008|isbn=0-8165-2755-5
|páxinas=161–179}}
</ref> - < 822 km de diámetro<ref name="johnston ixion">{{Cita
|autor=W. R. Johnston
|data=17-09-2008
Liña 52:
|dataacceso=28-07-2010
}}</ref> )
* [[20000 Varuna|Varuna]] (900 km), [[(55565) 2002 AW197]] (734 (+116 -108) [[quilómetro|km]]<ref name="spitzer AW197">{{Cita
|título=Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope
|autor=John Stansberry, Will Grundy, Mike Brown, Dale Cruikshank, John Spencer, David Trilling, Jean-Luc Margot
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