Figure 22.
(a) CI-chondrite normalized HSE abundances and (b) 187Re/188Os versus 187Os/188Os for eucrite and diogenite meteorites. Data from Day et al. (2012a) and Dale et al. (2012). Shown in (b) is the 4.568 Ga IIIAB iron isochron from Smoliar et al. (1996). The highest HSE contents have been measured in anomalous eucrite, Dho 007.