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- W2146648503 abstract "To predict the concentration gradients in meteoritic kamacite, the newly determined Fe-Ni phase diagram of Goldstein and Ogilvie was applied and a diffusion analysis was developed. The results of the diffusion analysis show that for cooling rates of about 2×10−6 deg/yr the kamacite phase cannot remain in equilibrium at low cooling temperatures and a Ni depletion in the kamacite near the α-γ interface occurs below 450°C. Certain other features of the kamacite phase are predicted: (1) an increasing Ni concentration from the center of the kamacite phase toward the α-γ interface in coarse and medium octahedrites, (2) a variation in the average Ni content of the average kamacite bandwidths with the over-all Ni content of the meteorite, and (3) a similar average composition of kamacite plates of the same width regardless of the over-all Ni content of the parent meteorite. These predictions have been confirmed by electron probe measurements of several metallic meteorites. This study shows that the composition of the kamacite phase in meteorites can be predicted from cooling rates of parent bodies which form at low pressure." @default.
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- W2146648503 date "1965-12-15" @default.
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- W2146648503 title "The formation of the kamacite phase in metallic meteorites" @default.
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- W2146648503 doi "https://doi.org/10.1029/jz070i024p06223" @default.
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