Computer Science
Scientific paper
Dec 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981rspta.303..369r&link_type=abstract
(Royal Society, Discussion on Planetary Exploration, London, England, Nov. 4, 5, 1980.) Royal Society (London), Philosophical Tr
Computer Science
1
Big Bang Cosmology, Meteoritic Composition, Molecular Clouds, Solar System, Deuterium, Hydrogen, Isotopes, Mass Ratios, Space Exploration, Supernova Remnants, Xenon Isotopes, Solar System, Origin, Planets, Formation, Isotopes, Anomalies, Nebula, Radioactivity, Thermal Properties, Luminosity, Meteorites, Composition, Hypotheses, Deuterium, Contamination, Chronology
Scientific paper
Relics of the molecular cloud origins of the solar system found in the deuterated molecules of meteorites are discussed. The situation is summarized and discussed in conjunction with the isotopic anomalies of heavier elements in order to obtain an overall view of the whole event. Attention is given to the possibility that the formation of the solar system took place during an extended period of time, during which matter, variously affected by the nearby supernova remnants, could have been introduced, as suggested from the Xe-129/Xe-127-Xe-129/Xe-132 data of the Heidelberg group (Jordan et al., 1977).
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