Light element stable isotopes in meteorites - From grams to picograms

Details Light element stable isotopes in meteorites - From grams to picograms Light element stable isotopes in meteorites - From grams to picograms

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984gecoa..48.2739p&link_type=abstract

Geochimica et Cosmochimica Acta (ISSN 0016-7037), vol. 48, Dec. 1984, p. 2739-2766. Research supported by the Science and Engine

Computer Science

19

Abundance, Isotopes, Meteoritic Composition, Carbon Isotopes, Nitrogen Isotopes, Oxygen Isotopes, Sulfur Isotopes

Scientific paper

A historical account is given of the development of studies concerned with the stable isotopes of H, C, N, O, and S in meteorites over the last 50 years, from the Manian et al. (1934) paper which inaugurated the field to the 15th Lunar and Planetary Science Conference of March, 1984. Unlike terrestrial problems, meteorite investigations are restricted by sample availability rather than precision of measurement, so that for 30 years meteorite stable isotope studies were confined to bulk samples, rather than being used to establish the distribution of isotopes within different phases as a means of tracing their origin and history.

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