(308193) 2005 CB79
Sidereal rotation period | 13.52 h[8] | |
0.7 (assumed) | ||
(Neutral) B-V=0.73, V-R=0.37[9] | ||
21.1[10] | ||
4.6[4] | ||
(308193) 2005 CB79 is a trans-Neptunian object that is a member of the Haumea family.[9]
Haumea family
As a member of the Haumea family, (308193) 2005 CB79 is suspected of being an icy mantle collisional fragment from
Haumea. With an absolute magnitude (H) of 4.7,[4] and a Haumea-family albedo of 0.7, this object would have a diameter of 158 km.[7]
Observations by
companion.[11]
References
- ^ Marsden, Brian G. (September 1, 2007). "MPEC 2007-R02 : 2003 UY413, 2003 UZ413, 2004 NT33, 2005 CA79, 2005 CB79, 2005 UQ513". IAU Minor Planet Center. Harvard-Smithsonian Center for Astrophysics. Retrieved January 10, 2010.
- ^ "MPEC 2010-A05 :Distant Minor Planets (14 January 2010.0 TT)". IAU Minor Planet Center. January 2, 2010. Archived from the original on 14 January 2010. Retrieved January 10, 2010.
- Marc W. Buie (December 20, 2008). "Orbit Fit and Astrometric record for 308193". SwRI (Space Science Department). Archivedfrom the original on August 18, 2010. Retrieved January 10, 2010.
- ^ a b c "JPL Small-Body Database Browser: (2005 CB79)". December 20, 2008. Retrieved 7 April 2016.
- 3-sigma.)
- Haumea-like albedo of 0.7
- ^ a b Dan Bruton. "Conversion of Absolute Magnitude to Diameter for Minor Planets". Department of Physics & Astronomy (Stephen F. Austin State University). Archived from the original on March 23, 2010. Retrieved December 27, 2009.
- S2CID 119256112. Archived from the original(PDF) on 7 November 2014. Retrieved 8 June 2014.
- ^ S2CID 62880843.
- ^ "AstDys 2005CB79 Ephemerides". Department of Mathematics, University of Pisa, Italy. Retrieved January 10, 2010.
- ^ Plutokiller (February 3, 2012). "2005 CB79 looks solitary". Twitter. Retrieved February 3, 2012.