S-asteroids of the main belt and meteorite sources

Details S-asteroids of the main belt and meteorite sources S-asteroids of the main belt and meteorite sources

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992avest..26..116g&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 26, no. 6, p. 116-124.

Astronomy and Astrophysics

Astrophysics

Asteroid Belts, Orbital Elements, Spectrum Analysis, Stony Meteorites, Albedo, Meteoritic Composition

Scientific paper

Planets exhibiting spectral characteristics similar to achondrites and ordinary chondrites are identified among the main belt asteroids on the basis of diagrams of the meteorites' spectral parameters. Astrophysical data on S-asteroids support the hypothesis of the 2/5 resonance (2.824 AU) as the probable mechanism of mass transfer from the asteroid belt in the neighborhood of each orbit.

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