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(308193) 2005 CB79 : ウィキペディア英語版 | (308193) 2005 CB79
is a trans-Neptunian object that is a member of the Haumea family.〔 As a member of the Haumea family, is suspected of being an icy mantle collisional fragment from dwarf planet Haumea. With an absolute magnitude (H) of 4.7,〔 and a Haumea-family albedo of 0.7, this object would have a diameter of 158 km.〔 Observations by Mike Brown in 2012 using the W. M. Keck Observatory suggest that does not have a companion. ==References==
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