Isotopic inhomogeneity of the solar system - Causes and consequences

Details Isotopic inhomogeneity of the solar system - Causes and consequences Isotopic inhomogeneity of the solar system - Causes and consequences

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988geokh......200s&link_type=abstract

Geokhimiia (ISSN 0016-7525), Feb. 1988, p. 200-211. In Russian.

Computer Science

Earth Core, Isotopes, Meteoritic Composition, Nuclear Fusion, Solar System, Earth Atmosphere, Earth Mantle, Earth Planetary Structure, Planetary Evolution

Scientific paper

The various nuclear processes that led to the origin of the solar system are discussed. Based on data on the isotopic anomalies in meteorites, in particular on the correlated excesses of Xe-129 and Xe-136 in basaltic glasses of the mid-ocean ridges and of rocks obtained from a deep gas well, speculations are offered concerning the nature of the earth's initial matter and the time of the earth's origin. These data also suggest that the degassing of the mantle matter and the formation of the atmosphere took place very early in the earth's history and were very rapid.

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