V-type asteroid

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The spectra of the V-type asteroids or Vestoids are similar to that of 4 Vesta, by far the largest asteroid in this class (hence the name).

A large proportion have orbital elements similar to those of 4 Vesta, either close enough to be part of the Vesta family, or having similar eccentricities and inclinations but with a semi-major axis lying between about 2.18 AU and the 3:1 Kirkwood gap at 2.50 AU. This suggests that most or all of them originated as fragments of Vesta's crust, possibly blasted out by a single very large impact at some point in its history. The enormous southern-hemisphere crater on Vesta is the prime candidate for the impact site ^[1].

The V-type asteroids are moderately bright, and rather similar to the more common S-type, which are also made up of stony irons and ordinary chondrites. This rather rare type of asteroid contains more pyroxene than the S-type.

The electromagnetic spectrum has a very strong absorption feature longward of 0.75 μm, another feature around 1 μm and is very red shortwards of 0.7 µm. The visible wavelength spectrum of the V-type asteroids (including 4 Vesta itself) is similar to the spectra of basaltic achondrite HED meteorites.

A J-type has been suggested for asteroids having a particularly strong 1 μm absorption band similar to diogenite meteorites ^[2], likely being derived from deeper parts of the crust of 4 Vesta.

[edit] Distribution

The vast majority of V-type asteroids are members of the Vesta family along with Vesta itself. There are some Mars-crossers such as 9969 Braille, and some Near-Earth objects like 3908 Nyx.

There is also a scattered group of objects in the general vicinity of the Vesta family but not part of it. These include^[3]:

• 809 Lundia Orbits within the Flora family region
• 956 Elisa
• 1459 Magnya Orbits in the outer main belt, too far from Vesta to be genetically related. May be the remains of a different ancient differentiated body that was shattered long ago.
• 2113 Ehrdni
• 2442 Corbett
• 2566 Kirghizia
• 2579 Spartacus — contains a significant portion of olivine, which may indicate origin deeper within Vesta than other V-types.
• 2640 Hallstrom
• 2653 Principia
• 2704 Julian Loewe
• 2763 Jeans
• 2795 Lepage
• 2851 Harbin
• 2912 Lapalma
• 3849 Incidentia
• 3850 Peltier Orbits within the Flora family region
• 3869 Norton
• 4188 Kitezh
• 4278 Harvey Member of Baptistina family.
• 4434 Nikulin
• 4796 Lewis
• 4977 Rauthgundis
• 5379 Abehiroshi

[edit] References

1. ^ S. J. Bus and R. P. Binzel (2002). "Phase II of the Small Main-belt Asteroid Spectroscopy Survey: A feature-based taxonomy". Icarus 158: 146. 
2. ^ R. P. Binzel and S. Xu (1993). "Chips off of asteroid 4 Vesta: Evidence for the parent body of basaltic achondrite meteorites". Science 260: 186. doi:10.1126/science.260.5105.186. 
3. ^ V. Carruba et al (2005). "On the V-type asteroids outside the Vesta family". Astronomy & Astrophysics 441: 819. 

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