Spectroscopic Comparison Between Near-Earth Asteroids and Ordinary Chondrites Meteorites

Details Spectroscopic Comparison Between Near-Earth Asteroids and Ordinary Chondrites Meteorites Spectroscopic Comparison Between Near-Earth Asteroids and Ordinary Chondrites Meteorites

Jul 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997dps....29.0510l&link_type=abstract

American Astronomical Society, DPS meeting #29, #05.10; Bulletin of the American Astronomical Society, Vol. 29, p.966

Astronomy and Astrophysics

Astronomy

Scientific paper

The population of NEA represents one of the most peculiar and heterogeneous classes of objects in the Solar System. In particular, as their dynamical lifetimes are shorter than the age of the Solar System, one of the most interesting aspects in the study of NEA is to understand their origin. To investigate the compositional properties of this population we started a spectroscopic survey in the visible region (0.5

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