Computer Science
Scientific paper
Jul 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988rspta.325..459k&link_type=abstract
(Royal Society, Discussion on the Solar System: Chemistry as a Key to its Origin, London, England, July 15, 16, 1987) Royal Soci
Computer Science
38
Meteoritic Composition, Nebulae, Solar System, Carbonaceous Chondrites, Chondrites, Chondrule, Condensation, Enstatite, Evaporation, Iron Compounds, Olivine, Silicates, Ureilites
Scientific paper
A model for solar nebula processes is developed that recognizes genetic
links between almost all meteorites. This model attempts to explain why
most meteorites are probably primitive, and what processes provide the
links between the different meteorites. The term 'primitive' is
restricted to presolar and solar nebula processes and their products.
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