Geochemistry of Non-Traditional Stable Isotopes by Clark M. Johnson

By Clark M. Johnson

Technology

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1969; Schramm et al. 1970; Huey and Kohman 1972). The searches for isotopic variations due to irradiation by an early active Sun failed as well (Fowler et al. 1962; Burnett et al. 1966). Hence until the early 1970s, it was generally accepted that the solar system had undergone a high temperature stage volatilizing all, or almost all solids, and homogenizing at least the inner solar system where the samples were coming from (Cameron 1969). Nucleosynthetic theory in the same time was directed toward reproducing the solar system abundances (Burbidge et al.

Nickel has not been investigated in FUN inclusions. 5 H). C1 has only a hint of an excess in 58Fe (30 ± 15 H). In an inclusion similar to C1, but extracted from the Vigarano meteorite, a deficit in 66Zn has been evidenced by Loss et al. (1994). This is in agreement with the deficit in neutron-rich isotopes of the other iron-group elements in the same inclusion. The data of EK141 are in agreement with the model deduced from the other iron group elements Heavy elements (Fig. 4). This is the domain where the FUN inclusions differ the most from normal inclusions.

Nickel has not been investigated in FUN inclusions. 5 H). C1 has only a hint of an excess in 58Fe (30 ± 15 H). In an inclusion similar to C1, but extracted from the Vigarano meteorite, a deficit in 66Zn has been evidenced by Loss et al. (1994). This is in agreement with the deficit in neutron-rich isotopes of the other iron-group elements in the same inclusion. The data of EK141 are in agreement with the model deduced from the other iron group elements Heavy elements (Fig. 4). This is the domain where the FUN inclusions differ the most from normal inclusions.

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