(308193) 2005 CB79
Introduction '''''' is a trans-Neptunian object that is a member of the Haumea family.
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.2005 RR43 (B-V=0.77, V-R=0.41) on this color plot of TNOs. All the other Haumea-family members (2005 CB79: 0.73, 0.37) are located to the lower left of this point.
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