Primordial noble gases in chondrites - The abundance pattern was established in the solar nebula

Details Primordial noble gases in chondrites - The abundance pattern was established in the solar nebula Primordial noble gases in chondrites - The abundance pattern was established in the solar nebula

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977sci...198..927a&link_type=abstract

Science, vol. 198, Dec. 2, 1977, p. 927-930.

Computer Science

4

Abundance, Chondrites, Rare Gases, Solar System, Meteoritic Composition, Planetary Composition, Planetary Nebulae

Scientific paper

Ordinary chondrites, like carbonaceous chondrites, contain primordial noble gases mainly in a minor phase comprising not more than 0.05 percent of the meteorite, probably an iron-chromium sulfide. The neon-20/argon-36 ratios decrease with increasing argon-36 concentration, as expected if the gas pattern was established by condensation from the solar nebula, and was negligibly altered by metamorphism in the meteorite parent bodies. Meteoritic and planetary matter apparently condensed over a substantial range of temperatures.

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