O-type asteroid

The rare O-type asteroids have spectra similar to the unusual asteroid 3628 Boznemcová, which is the best asteroid match to the spectra of L6 and LL6 ordinary chondrite meteorites. Their spectra have a deep absorption feature longward of 0.75 μm.[1]

List

Seven asteroids have been classified as O-type by the second Small Main-Belt Asteroid Spectroscopic Survey (SMASSII) and none by Tholen's Eight-Color Asteroid Survey. With the exception of main-belt asteroid 3628 Božněmcová, all other bodies are near-Earth asteroids from the Apollo, Aten or Amor group:

DesignationClassDiam.Refs
3628 Božněmcovámain-belt6.914 kmMPC · JPL
4034 VishnuApollo0.42 kmMPC · JPL
4341 PoseidonApollo2 kmMPC · JPL
5143 HeraclesApollo4.843 kmMPC · JPL
(8201) 1994 AH2Apollo1.859 kmMPC · JPL
(162385) 2000 BM19Aten0.57 kmMPC · JPL
1997 RTAmor0.3 kmMPC · JPL
Diameter: averaged estimates only; may change over time
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See also

References

  1. S. J. Bus and R. P. Binzel, Phase II of the Small Main-belt Asteroid Spectroscopy Survey: A feature-based taxonomy, Icarus, Vol. 158, pp. 146 (2002).


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