Olivine of 446 Aeternitas As an Example of Olivines of A-class Asteroids

Details Olivine of 446 Aeternitas As an Example of Olivines of A-class Asteroids Olivine of 446 Aeternitas As an Example of Olivines of A-class Asteroids

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sosyr..35..376g&link_type=abstract

Solar System Research, v. 35, Issue 5, p. 376-382 (2001).

Computer Science

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Scientific paper

A reflectance spectrum of A-asteroid 446 Aeternitas was numerically simulated. Probable mineral composition of the asteroid surface (Px > Ol ~ Met) and probable spectra of these minerals were obtained. Since the grain size of asteroid regolith is unknown, a method for estimating the range of the chemical composition of olivine is proposed. According to the modeled spectra of the asteroid olivine, the probable range for the concentration of the forsterite molecule is from 40 to 56 mol %. No analogues of the material of A-asteroids were found among differentiated meteorites.

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