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. Author manuscript; available in PMC: 2020 Dec 2.
Published in final edited form as: Geochim Cosmochim Acta. 2019 Feb 27;251:217–228. doi: 10.1016/j.gca.2019.02.035

Fig. 3.

Fig. 3.

Compilation of μ94Mo vs. μ95Mo data for iron meteorites and pallasites from Burkhardt et al. (2011), Kruijer et al. (2017), Poole et al. (2017), and Worsham et al. (2017). Some data have not been corrected for CRE. Blue squares represent meteorites classified as CC type and red diamonds represent meteorites classified as NC type. Data from this study for the SBT and Milton are also plotted. Black lines were obtained by regressing the NC and CC data using ISOPLOT (Ludwig, 2003); the CC line has a slope of 0.57 ± 0.05 and a y-intercept of 26.3 ± 7.5 (MSWD = 1.15) and the NC line has a slope of 0.50 ± 0.04 and a y-intercept of −8.5 ± 3.2 (MSWD = 0.49). The inset shows an enlarged view of the Mo isotopic compositions of the SBT and Milton without other meteorites.