Q-type asteroid
Q-type asteroids are relatively uncommon inner-belt asteroids with a strong, broad 1 micrometre olivine and pyroxene feature, and a spectral slope that indicates the presence of metal. There are absorption features shortwards and longwards of 0.7 μm, and the spectrum is generally intermediate between the V and S-type.
Q-type asteroids are spectrally more similar to ordinary chondrite meteorites (types H, L, LL) than any other asteroid type. This has led scientists to speculate that they are abundant, but only about 20 of this type has been characterized.[1] Examples of Q-type asteroids are: 1862 Apollo, 2102 Tantalus, 3753 Cruithne, 6489 Golevka, and 9969 Braille.
See also
- Asteroid spectral types
References
- ^ "JPL Small-Body Database Search Engine: spec. type = Q (SMASSII)". JPL Solar System Dynamics. Retrieved 2015-06-16.
- v
- t
- e
- Trojans
- Interior to Earth
- Near-Earth
- Between Earth and the main belt
- Asteroid belt
- Outer Solar System, does not include distant minor planets
- Centaurs
- Exoasteroids
Orbital | |||||
---|---|---|---|---|---|
Spectral |
|
Category
![]() | This asteroid-related article is a stub. You can help Wikipedia by expanding it. |
- v
- t
- e