Meteorite research

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Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979rvgsp..17..912w&link_type=abstract

Reviews of Geophysics and Space Physics, vol. 17, June 1979, p. 912-925.

Physics

Space Physics

1

Chemical Composition, Meteoritic Composition, Radioactive Isotopes, Solar System, Abundance, Bibliographies, Chondrites, Evolution (Development), Protoplanets, Review, Meteorites, Composition, Isotopic Abundance, Anomalies, Radioisotopes, Carbonaceous Chondrites, Allende Meteorite, Supernova, Irradiation, Cosmic Rays, Solar Nebula, Planetesimals, Petrography, Condensation, Inclusions, Fractionation, Nucleation, Chondrules, Volatile Elements, Agglutinates, Metamorphism, Melting, Regolith, Minerology, Trace E

Scientific paper

Meteorites contain a record of events and processes that occurred in the three earliest stages of solar system history: (1) formation of the raw material that was to become the solar system, (2) processing of the condensable component of this material in a nebular disk that circle the protosun, and (3) processing of condensed material after it accumulated into planetesimals of asteroidal dimension. Progress toward interpreting this record, made during the period 1975-1978, is summarized.

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