Isotopic studies of ferroan anorthosite 62236: A young lunar crustal rock from a light rare-earth-element-depleted source

Isotopic analyses of mineral fractions and whole rocks from the ferroan ano rthosite 62236 yield a Sm-Nd isochron with an age of 4.29 +/- 0.06 Ga and a n initial epsilon(Nd)(143) value of +3.1 +/- 0.9. We have also measured eps ilon(Nd)(142) anomalies of +0.25 on two fractions of 62236. These values ar e higher than the value of -0.1 predicted if 62236 was derived from a chond ritic source at 4.29 Ga, but are consistent with the positive initial epsil on(Nd)(143) value. The Sm-Nd isotopic composition of 62236 has been modifie d by the capture of thermal neutrons such that the Sm-147/Nd-144, Nd-143/Nd -144, and Nd-142/Nd-144 ratios measured on the mineral fractions and whole rocks must be corrected. The corrections do not significantly alter the Sm- Nd isotopic results determined on 62236, Despite the fact that the Ar-Ar an d Rb-Sr isotopic systematics of 62236 have been reset by impact metamorphis m at 3.93 +/- 0.04 Ga, the Sm-Nd systematics appear to have been unaffected . The Sm-Nd isotopic systematics of 62236 provide several constrains on mod els of lunar crustal differentiation provided they have not been reset sinc e crystallization. First, the relatively young age of 62236, as well as the old ages determined on several crustal plutonic rocks of the Mg-suite, req uire multiple sources of magmas on the Moon very early in its history. Seco nd, positive epsilon(Nd)(143) values determined on all analyzed ferroan ano rthosites suggest that they were derived from sources depleted in light rar e earth elements. And third, models based on initial epsilon(Nd)(143) and p resent-day epsilon(Nd)(143) values suggest that the source of 62236 was dep leted in light rare earth elements at similar to 4.46 Ga. In order to recon cile these observations with the lunar magma ocean model (1) the magma ocea n must have existed for a very short period of time, and may have had a sub -chondritic Nd/Sm ratio, and (2) the youngest ferroan anorthosites, such as 62236, cannot be cumulates from the magma ocean, but must form by other pr ocesses. Copyright (C) 1999 Elsevier Science Ltd.