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S-type asteroid

S-type asteroids are asteroids with a spectral type that is indicative of a siliceous mineralogical composition, hence the name. They have relatively high density. Approximately 17% of asteroids are of this type, making it the second-most common after the carbonaceous C-type.

Characteristics
S-type asteroids, with an astronomical albedo of typically 0.20, == S-group asteroids ==
S-group asteroids
SMASS classification In the SMASS classification, several generally "stony" types of asteroids are brought together into a wider S-group which contains the following types: • A-typeK-typeL-typeQ-typeR-type • a "core" S-type for asteroids having the most typical spectra for the S-group • Sa, Sk, Sl, Sq, and Sr-types containing transition objects between the core S-type and the A, K, L, Q, and R-types, respectively. The entire "S"-assemblage of asteroids is spectrally quite distinct from the carbonaceous C-group and the often metallic X-group. Tholen classification In the Tholen classification, the S-type is a very broad grouping which includes all the types in the SMASS S-group except for the A, Q, and R, which have particularly strong "stony" absorption features around 1 μm. Stony asteroid families Prominent stony asteroid families with their typical albedo are the: • Eos family (0.14) • Eunomia family (0.21) • Flora family (0.24) • Koronis family (0.24) • Nysa family (0.20) • Phocaea family (0.23) == See also ==
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