Computer Science
Scientific paper
Jan 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978natur.271..150b&link_type=abstract
Nature, vol. 271, Jan. 12, 1978, p. 150-153.
Computer Science
Planets, Earth, Mars, Volatiles, Nitrogen, Carbon, Argon, Rare Gases, Venus, Atmospheres, Meteorites, Terrestrial Planets, Origin, Abundance
Scientific paper
Relative concentrations of noble gases and C and N are evaluated for the terrestrial planets. Comparisons between amounts of volatile materials in carbonaceous chondrites and on Earth and Mars are presented as support for the accretion model of planetary formation. However, attention is given to the large differences in the C/noble gas ratios on various bodies in the solar system, e.g. the Sun, Venus, Earth, Mars, stressing that the data are too incomplete to provide a reliable model for the sources of volatile and noble elements on the terrestrial planets.
Bogard Donald D.
Gibson Everett K.
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