Mary Wilson
Well-known member
15 January 2024
https://doi.org/10.1016/j.epsl.2023.118473
Nathan Asset [SUP]a[/SUP], Marc Chaussidon [SUP]a[/SUP], Johan Villeneuve [SUP]b[/SUP], Sébastien Charnoz [SUP]a[/SUP], Christian Koeberl [SUP]c[/SUP], Mario Wannier [SUP]d[/SUP], François Robert [SUP]e[/SUP]
Highlights
- The Hiroshima glasses are condensates produced by the Hiroshima nuclear explosion.
- The wide silicon kinetic fractionations in the Hiroshima glasses can only be explained by condensation.
- In Hiroshima glasses, oxygen mass-independent fractionations resulted from chemical reactions during condensation.
- A scenario was established to describe the formation of the Hiroshima fallout.
- The Hiroshima glasses can be considered an analog of the first condensates of the solar system.
Abstract
A new kind of Hiroshima nuclear fallout, the Hiroshima glasses, was discovered around the Hiroshima Bay. Here, the chemical compositions and the silicon and oxygen triple isotope compositions were analyzed to understand the formation process of these new fallouts. The chemical analysis shows four different families of glasses: the melilitic glasses, the anorthositic glasses, the soda-lime glasses, and the silica glass. The silicon isotopic compositions show wide variations in the glasses, with δ[SUP]30[/SUP]Si varying between -23.0 ± 1.8 ‰ and -1.5 ± 1.1 ‰. The oxygen isotopic compositions indicate the presence of mass-independent fractionation on ≈38 % of the analyses, reaching a Δ[SUP]17[/SUP]O of -3.1 ± 0.6 ‰. The chemical and silicon isotopic compositions of the Hiroshima glasses show that these glasses were formed by condensation within the nuclear fireball. Our scenario for the Hiroshima glasses formation, tested by modeling (GGchem code), considers a rapid condensation (1.7–5.5 s) in the nuclear fireball (3200–1000 K) at atmospheric pressure with a gas resulting from a mixing between air, and vaporized water and city materials. Chemical reactions during the Hiroshima glasses condensation are the most probable source for the oxygen mass-independent fractionation. The formation of the Hiroshima glasses by condensation implies that they may be an analog to the first condensates in the solar system: Calcium-Aluminum-rich Inclusions (CAIs), which are found in chondrites. The Hiroshima glasses exhibit similarities with CAIs in their chemical and isotopic compositions (Si and O).
https://www.sciencedirect.com/science/article/abs/pii/S0012821X23004867?via=ihub
https://doi.org/10.1016/j.epsl.2023.118473
Nathan Asset [SUP]a[/SUP], Marc Chaussidon [SUP]a[/SUP], Johan Villeneuve [SUP]b[/SUP], Sébastien Charnoz [SUP]a[/SUP], Christian Koeberl [SUP]c[/SUP], Mario Wannier [SUP]d[/SUP], François Robert [SUP]e[/SUP]
Highlights
- The Hiroshima glasses are condensates produced by the Hiroshima nuclear explosion.
- The wide silicon kinetic fractionations in the Hiroshima glasses can only be explained by condensation.
- In Hiroshima glasses, oxygen mass-independent fractionations resulted from chemical reactions during condensation.
- A scenario was established to describe the formation of the Hiroshima fallout.
- The Hiroshima glasses can be considered an analog of the first condensates of the solar system.
Abstract
A new kind of Hiroshima nuclear fallout, the Hiroshima glasses, was discovered around the Hiroshima Bay. Here, the chemical compositions and the silicon and oxygen triple isotope compositions were analyzed to understand the formation process of these new fallouts. The chemical analysis shows four different families of glasses: the melilitic glasses, the anorthositic glasses, the soda-lime glasses, and the silica glass. The silicon isotopic compositions show wide variations in the glasses, with δ[SUP]30[/SUP]Si varying between -23.0 ± 1.8 ‰ and -1.5 ± 1.1 ‰. The oxygen isotopic compositions indicate the presence of mass-independent fractionation on ≈38 % of the analyses, reaching a Δ[SUP]17[/SUP]O of -3.1 ± 0.6 ‰. The chemical and silicon isotopic compositions of the Hiroshima glasses show that these glasses were formed by condensation within the nuclear fireball. Our scenario for the Hiroshima glasses formation, tested by modeling (GGchem code), considers a rapid condensation (1.7–5.5 s) in the nuclear fireball (3200–1000 K) at atmospheric pressure with a gas resulting from a mixing between air, and vaporized water and city materials. Chemical reactions during the Hiroshima glasses condensation are the most probable source for the oxygen mass-independent fractionation. The formation of the Hiroshima glasses by condensation implies that they may be an analog to the first condensates in the solar system: Calcium-Aluminum-rich Inclusions (CAIs), which are found in chondrites. The Hiroshima glasses exhibit similarities with CAIs in their chemical and isotopic compositions (Si and O).
https://www.sciencedirect.com/science/article/abs/pii/S0012821X23004867?via=ihub