Asteroid spectroscopy - Progress and perspectives

Details Asteroid spectroscopy - Progress and perspectives Asteroid spectroscopy - Progress and perspectives

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993metic..28..161g&link_type=abstract

Meteoritics (ISSN 0026-1114), vol. 28, no. 2, p. 161-187.

Astronomy and Astrophysics

Astronomy

111

Asteroids, Astronomical Spectroscopy, Meteoritic Composition, Solar System Evolution, Classifying, Meteorites, Meteoroids, Planetary Composition, Protoplanets, Satellite Surfaces, Spectrum Analysis, Asteroids, Spectroscopy, Meteorites, Parent Bodies, Solar System, Origin, Thermal History, Heating, Structure, Interior, Size, Physical Properties, Collisions, Orbit, Planetesimals, Composition, Solar Nebula, Surface, Spectra, Optical Properties, Taxonomy, Classification, Stony Meteorites, Achondrites, Ordinary

Scientific paper

A broad understanding of meteorite and asteroidal studies is needed for the most dynamic progress of both disciplines, in their common goal of understanding the origin and early evolution of the solar system. Asteroid compositional investigations are currently shifting from the survey mode to focused investigations of selected targets, in pursuit of specific problems. Attention is presently given the compositional nature and diversity of asteroid taxonomic classes, as addressed by the Small Main-Belt Asteroid Spectroscopic Survey.

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