K-type asteroid
K-type asteroids are relatively uncommon asteroids with a moderately reddish spectrum shortwards of 0.75 μm, and a slight bluish trend longwards of this. They have a low albedo. Their spectrum resembles that of CV and CO meteorites.
These asteroids were described as "featureless" S-types in the Tholen classification. The K-type was proposed by J. F. Bell and colleagues in 1988 for bodies having a particularly shallow 1 μm absorption feature, and lacking the 2 μm absorption. These were found during studies of the Eos family of asteroids.
See also
References
- J. F. Bell A probable asteroidal parent body for the CV and CO chondrites, Meteoritics, Vol. 23, pp. 256 (1988).
- J. F. Bell et al. The 52-color asteroid survey: Final results and interpretation, Lunar and Planetary Science, Vol. 19, pp. 57 (1988).
| Main |
| ||||||||
|---|---|---|---|---|---|---|---|---|---|
| Distribution |
| ||||||||
| Classification |
| ||||||||
| Exploration | |||||||||
| Lists |
| ||||||||
| |||||||||
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.