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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 8.

Figure 8.

Comparison of terrestrial mantle (TM) composition established from peridotites versus terrestrial, lunar (LM), martian (MM; I-HSE = dashed gray line), howardite-eucrite-diogenite (HEDM) and angrite parent body (APBM) mantle estimates based on HSE–MgO or interelement–HSE (I-HSE) covariation from volcanic products. Values are presented in Table 2 or for I-HSE in HEDM and APBM in Dale et al. (2012). HSE–MgO regression data for the APBM or HEDM are not presented due to the wide range in HSE contents for the meteorite suites, which indicate that further information is required prior to interpreting possible mantle HSE abundances for these bodies.