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. Author manuscript; available in PMC: 2019 Mar 6.
Published in final edited form as: Rev Mineral Geochem. 2016 Jan 1;81(1):161–238. doi: 10.2138/rmg.2016.81.04

Figure 9.

Figure 9.

Plots of average, minimum (lower lines) and maximum (upper lines) HSE abundances for carbonaceous (CC), ordinary (OC) and enstatite (EC) chondrites versus mantle estimates for Earth (× 150; TM), Mars (× 150; MM) and the Moon (× 6000; LM). Data are plotted with a linear Y-axis in (a) and a logarithmic Y-axis in (b). The mantles of Earth, Mars and the Moon have broadly or nearly chondritic relative abundances of the HSE. Chondrite compilation is given in Table 3 and Earth, Mars and Moon mantle HSE abundances are from Becker et al. (2006), Day (2013) and Day et al. (2007) and are provided in Table 2. Orgueil values (CI-chondrite composition) from Horan et al. (2003).