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. Author manuscript; available in PMC: 2021 Sep 15.
Published in final edited form as: Geochim Cosmochim Acta. 2015 Feb 14;155:122–153. doi: 10.1016/j.gca.2015.02.004

Fig. 9.

Fig. 9.

Regressed or averaged 187Os/188Os (a), Ru/Ir (b) and Pd/Ir (c) versus formation ages (listed in Table 1) for the lunar impact melt rocks examined here and in literature. Vertical dashed lines denote the period of large-basin formation during the putative late heavy bombardment with Imbrium and Serenitatis events highlighted. Horizontal field represents the range of known chondrite groups. Symbols and data sources are the same as Fig. 6.