Asteroids - Spectral reflectance and color characteristics

Mathematics – Logic

Scientific paper

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Asteroids, Astronomical Photometry, Colorimetry, Light Curve, Spectral Reflectance, Absorption Spectra, Data Reduction, Graphs (Charts), Mineralogy, Near Infrared Radiation, Orbital Elements, Spectral Bands, Visual Photometry

Scientific paper

We present visible and near-infrared spectral reflectance curves for 35 asteroids, making a total sample of 67 including our previous work. Several previously unknown spectral types have been discovered. Absorption bands and other features, from which information about the surface composition of the asteroids can be derived, continue to appear. Sampling statistics suggest we have observed about half of the significantly different mineralogical assemblages present in the asteroid belt. There is a general, but imperfect, correlation between spectral type and semimajor axis, which is consistent with the hypothesis that meteorites are derived from the asteroid belt. The color-frequency histogram for the 67 objects is bimodal, probably associated with 'stony' objects and 'carbonaceous' objects. Hirayama family pairs usually show disparate spectral types. 19 Fortuna may show strikingly different photometric properties on opposite sides.

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