There are at least five taxonomic classification systems used by various camps
(see Tholen & Barucci).
In Tholen's scheme,there are at least 14 asteroid classes, based on albedo and
spectral characteristics. However, most asteroids fall into one of the following
classes:
| Class | albedo | spectrum | surface mineralogy[a] |
| C | low | flat to slightly reddish | hydrated silicates + carbon, organics |
| D | low | featureless, slightly red shortward of 5500 Å, very red longward of 5500 Å | carbon, organic-rich silicates? |
| P | low | featureless, flat, intermediate between C and D | carbon, organic-rich silicates? |
| M | moderate | featureless, flat | metal (possible trace silicates) |
| S | moderate | moderate to strong absorption feature shortward of 7000 Å | metal + olivine + pyroxene |
[a] See Gaffey et al.
Birlan et al. performed
a multivariate statistical analysis to determine asteroid reflection spectra in an
automated manner, as opposed to the usual "by hand" approach of classification. One
of the most interesting findings from this study is that infrared colors are very
important in discriminating between the various asteroid types.