Computer Science
Scientific paper
Jul 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988rspta.325..391t&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
Chemical Evolution, Nuclear Fusion, Solar System, Interstellar Gas, Star Formation, Stellar Activity, Supernovae
Scientific paper
It was originally believed that the Solar System was formed from a gas cloud that was chemically and isotopically homogeneous, with the variation of composition of objects today being attributed to processes occurring in the solar nebula. This was changed by the discovery of isotopic anomalies in meteorites. It is now clear that there was some departure from fine-scale mixing in the solar nebula. This may have resulted from late irradiation by a supernova or from the survival of interstellar grains with particular nucleosynthetic origins, or both, as well as from incomplete mixing of the interstellar gas.
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