Data from "The IAB iron-meteorite complex: A group, five subgroups, numerous grouplets, closely related, mainly formed by crystal segregation in rapidly cooling melts" by Wasson and Kallemeyn (2002)
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Description
This dataset contains mean concentrations of Cr, Cu, Ni, Cu, Ga, Ge, As, Sb, W, Re, Ir, Pt, and Au in IAB complex iron meteorites and some ungrouped iron meteorites. Germanium and Sb were analyzed by radiochemical neutron activation analysis (RNAA), while other elements were analyzed by instrumental neutron activation analysis (INAA) at the University of California, Los Angeles.
How To Cite
Wasson, J., Kallemeyn, G., 2021. Data from "The IAB iron-meteorite complex: A group, five subgroups, numerous grouplets, closely related, mainly formed by crystal segregation in rapidly cooling melts" by Wasson and Kallemeyn (2002), Version 1.0. Astromaterials Data Archive. https://doi.org/10.26022/IEDA/112042 Accessed 2026-09-29.
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Wasson, J. T., & Kallemeyn, G. W. (2002). The IAB iron-meteorite complex: A group, five subgroups, numerous grouplets, closely related, mainly formed by crystal segregation in rapidly cooling melts. Geochimica et Cosmochimica Acta, 66(13), 2445-2473.
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