The Vesta family of asteroids is a large and prominent grouping of mostly V-type asteroids in inner main belt in the vicinity of 4 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 and 2045 Peking, have an absolute magnitude of 12.2, which would give them a radius of about 7.5 km given the same high albedo as 4 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 the HED meteorites. The family also includes a few J-type asteroids (related to the V-type), which are thought to have come from the deeper layers of Vesta's crust, and correspond to the diogenite meteorites A HCM numerical analysis by (Zappala 1995) determined a large group of 'core' family members, whose proper orbital elements lie in the approximate ranges
| ap | ep | ip | |
|---|---|---|---|
| min | 2.26 AU | 0.075 | 5.6° |
| max | 2.48 AU | 0.122 | 7.9° |
This gives the approximate boundaries of the family. At the present epoch, the range of osculating orbital elements of these core members is
| a | e | i | |
|---|---|---|---|
| min | 2.26 AU | 0.035 | 5.0° |
| max | 2.48 AU | 0.162 | 8.3° |
The Zappala 1995 analysis found 235 core members. A search of a recent proper element database (AstDys)for 96944 minor planets 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 members are 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 PDS asteroid taxonomy data set).
References
- V. Zappalà, Ph. Bendjoya, A. Cellino, P. Farinella and C. Froeschlé, 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). Data set online here.
- AstDys site. Proper elements for 96944 numbered minor planets.
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| Vulcanoids · Near-Earth asteroids · Main belt · Jupiter Trojans · Centaurs · Damocloids · Neptune Trojans · Comets · Trans-Neptunians (Kuiper belt • Scattered disc objects • Oort cloud) |
| For other objects and regions, see Asteroid groups and families, Binary asteroids, Asteroid moons, meteoroids and the Solar System. For a complete listing, see List of asteroids. See also Pronunciation of asteroid names and Meanings of asteroid names. |
