- Vesta family
The Vesta family of asteroids is a large and prominent grouping of mostly V-type
asteroid s in innermain belt in the vicinity of4 Vesta . Approximately 6% of main belt asteroids belong to this family.Characteristics
It consists of
4 Vesta , the second-largest of all asteroids (mean diameter of 530 km), and many small asteroids below 10 km diameter. The brightest of these:1929 Kollaa and2045 Peking , have anabsolute magnitude of 12.2, which would give them a radius of about 7.5 km given the same high albedo as4 Vesta , or somewhat more if they are darker.The family members originated from an impact on asteroid
4 Vesta , with the giant south pole crater the likely impact site. The family members are thought to be the source of theHED meteorite s.The family also includes a few
J-type asteroid s (related to the V-type), which are thought to have come from the deeper layers of Vesta's crust, and correspond to thediogenite meteoritesA HCM numerical analysis by (Zappala 1995) determined a large group of 'core' family members, whose
proper orbital elements lie in the approximate rangesThis gives the approximate boundaries of the family. At the present epoch, the range of osculatingorbital elements of these core members isThe Zappala 1995 analysis found 235 core members. A search of a recent proper element database ( [http://hamilton.dm.unipi.it/cgi-bin/astdys/astibo?proper_elements:0;main AstDys] )for 96944
minor planet s in 2005 yielded 6051 objects (about 6% of the total) lying within the Vesta family region as per the first table above.Interlopers
Spectroscopic analyses have shown that some of the largest non-Vesta membersare in fact interlopers. They are not of the V or J spectral class, but have similar orbital elements by coincidence. These include
306 Unitas ,442 Eichsfeldia ,1697 Koskenniemi ,1781 Van Biesbroeck ,2024 McLaughlin ,2029 Binomi ,2086 Newell ,2346 Lilio , and others. (Identified by inspection of the [http://www.psi.edu/pds/archive/tax.html PDS asteroid taxonomy data set] ).References
* V. Zappalà, Ph. Bendjoya, A. Cellino, P. Farinella and C. Froeschlé, " [http://www.sciencedirect.com/science?_ob=ArticleURL&_udi=B6WGF-45NJHPF-3C&_coverDate=08%2F31%2F1995&_alid=267428521&_rdoc=1&_fmt=&_orig=search&_qd=1&_cdi=6821&_sort=d&view=c&_acct=C000056973&_version=1&_urlVersion=0&_userid=2337731&md5=6a0ee5be29f8c0489e922cb06868ae45 Asteroid Families: Search of a 12,487-Asteroid Sample Using Two Different Clustering Techniques] ", Icarus, Volume 116, Issue 2 (August 1995), pages 291-314
* S.J. Bus and R.P. Binzel, "Phase II of the Small Main-Belt Asteroid Spectroscopic Survey", Icarus Vo.. 158, p. 106 (2002). [http://smass.mit.edu/Bus.Taxonomy Data set online here] .
* [http://hamilton.dm.unipi.it/cgi-bin/astdys/astibo?proper_elements:0;main AstDys site] . Proper elements for 96944 numbered minor planets.
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