Alternative hypothesis for the origin of CCF xenon

Details Alternative hypothesis for the origin of CCF xenon Alternative hypothesis for the origin of CCF xenon

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.253..417b&link_type=abstract

Nature, vol. 253, Feb. 6, 1975, p. 417-419.

Astronomy and Astrophysics

Astronomy

14

Abundance, Astronomical Models, Carbonaceous Meteorites, Meteoritic Composition, Nuclear Fusion, Xenon, Cosmic Dust, Fission Products, Solar System

Scientific paper

The relative abundances and origins of the xenon isotopes found in carbonaceous meteorites are discussed. It is proposed that carbonaceous-chondrite-fission (CCF) xenon is not caused by fission, but is the direct result of a modified r-process nucleosynthesis which produces a peak at Z = 54 and N = 82. The xenon produced in this way would have been trapped in dust grains which were subsequently incorporated in the solar system with minimal degassing.

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