Published September 1985 | Version v1
Journal article

The nature of the heterogeneity of the isotopic composition of xenon in meteorites, terrestrial and lunar rocks

Creators

Description

This paper discusses protogenic or solar xenon, the unique component of the primary gas cloud. Changes in the isotopic composition of primitive xenon are caused by the fission process of U-238 and Pu-244, and Cm-248, and by the B-decay of I-129 as well as by the formation of spalogenic xenon during the interaction of cosmic rays with barium and other elements. This model is confirmed by the numerous isotopic data obtained by many researchers, for meteorites, lunar and terrestrial rocks

Additional details

Publishing Information

Journal Title
Sov. Radiochem. (Engl. Transl.)
Journal Volume
27
Journal Issue
1
Series
Sov. Radiochem. (Engl. Transl.).
Journal Page Range
72-79
ISSN
0038-576X
CODEN
SVRDA

Optional Information

Notes
Cover-to-cover translation of Radiokhimiya (USSR).