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. 2021 Oct 19;600(7887):54–58. doi: 10.1038/s41586-021-04100-2

Fig. 3. Initial 206Pb/204Pb ratios versus crystallization ages of the lunar basalts and meteorites.

Fig. 3

The lines represent the two-stage Pb isotope evolution of lunar mantle sources at given μ values6. The gradient areas are associated with KREEP-poor (yellow) to KREEP-rich (blue) mantle sources according to μ values. The Apollo and meteorite data are from refs. 6,7,10. Error bars are 2σ s.e. A11, Apollo 11 high-Ti basalts; A12, Apollo 12 low-Ti basalts; A15, Apollo low-Ti basalts; A17, Apollo 17 high-Ti basalts; High-Al, Apollo 14 high-Al basalts; KREEP, Apollo 15 KREEP basalts; Lunar basalt meteorite, low-Ti and very-low-Ti basaltic meteorites (NWA 4734 and NWA 773 clan).

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