Computer Science
Scientific paper
Jan 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991natur.349...18n&link_type=abstract
Nature (ISSN 0028-0836), vol. 349, Jan. 3, 1991, p. 18, 19.
Computer Science
1
Chondrites, Interstellar Matter, Rotating Disks, Solar Corona, Solar System Evolution, Aluminum Isotopes, Asymptotic Giant Branch Stars, Silicon Carbides, Solar System, Origin, Isotopes, Anomalies, Trace Elements, Graphite, Silicon Carbide, Aluminum 26, Magnesium 26, Concentration, Grains, Samples, Extraterrestrial, Nitrogen, Condensation, Origin, Formation, Condensates, Models, Isotopic Ratios, Aluminum 27, Hypotheses, Samples, Meteorite
Scientific paper
The evidence concerning the formation of the solar nebula from preexisting clouds found in the chemical composition of solar system grains is discussed. Evidence for sequential star formation in the grains is examined. It is argued that there is no model for the origin of the solar system which can account for the increasing complexity of the evidence.
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