The origin of geochemical diversity of lunar mantle sources inferred from the combined U–Pb, Rb–Sr, and Sm–Nd isotope systematics of mare basalt 10017

The results of our combined U–Pb, Rb–Sr, and Sm–Nd isotope study of mare basalt 10017 contribute to the understanding of the petrogenetic processes involved in the origin of geochemical diversity in lunar mare basalt sources, as well as the U–Pb isotope systematics of the Moon. The Rb–Sr, Sm–Nd, and U–Pb isotope systems yield concordant crystallization ages of 3.633 ± 0.057 Ga, 3.678 ± 0.069 Ga, and 3.616 ± 0.098 Ga, respectively. The U–Pb isochron yields an older, though still concordant, age of 3.80 ± 0.12 Ga. Neither the Pb–Pb system nor U–Pb concordia system yields an age for 10017 that is concordant with the age determined from the Sm–Nd, Rb–Sr, and U–Pb systems. The initial Sr/Sr of 10017 is 0.69941 ± 7 and the initial eNd is +3.2 ± 0.4. Initial Pb isotopic compositions, determined from the U–Pb isochrons, are Pb/Pbi = 31 ± 11 and Pb/Pbi = 34 ± 15. Together, these initial Pb compositions constrain the l value of the 10017 source to be 70 ± 30, assuming a single-stage Pb growth model. This is considerably lower than l values typically estimated for mare basalt sources ( 100–600). Regardless, the l values calculated for the sources of mare basalts, as well as other lunar samples, show a range that is larger than can be explained by fractionation of U from Pb solely by crystallization of silicate phases and ilmenite during magma ocean solidification and formation of lunar mantle sources. The U–Pb isotope systematics may reflect late-stage formation of a sulfide phase, which strongly fractionates Pb from U but has minimal effect on Rb/Sr or Sm/Nd compositions, during crystallization of the lunar magma ocean. 2007 Elsevier Ltd. All rights reserved.