Carbonaceous chondritic xenoliths and planetary-type noble gases in gas-rich meteorites

Details Carbonaceous chondritic xenoliths and planetary-type noble gases in gas-rich meteorites Carbonaceous chondritic xenoliths and planetary-type noble gases in gas-rich meteorites

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976lpsc....7.3549w&link_type=abstract

In: Lunar Science Conference, 7th, Houston, Tex., March 15-19, 1976, Proceedings. Volume 3. (A77-34651 15-91) New York, Pergamon

Computer Science

3

Carbonaceous Chondrites, Meteoritic Composition, Planetary Composition, Rare Gases, Abundance, Trace Elements, Xenon

Scientific paper

The source of the planetary-type noble gases in gas-rich meteorites is identified as finely divided (submillimeter to millimeter-sized), widely dispersed carbonaceous chondritic fragments. Trace-element abundances, noble-gas elemental abundances and isotopic abundances of xenon are compatible with the hypothesis that the carbonaceous chondritic carrier is present in amounts of a few percent in the gas-bearing portions of gas-rich chondrites and achondrites.

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