U-Th-Pb and Rb-Sr systematics of Apollo 17 boulder 7 from the North Massif of the Taurus-Littrow Valley
Abstract
Portions of highland breccia boulder 7 collected during the Apollo 17 mission were studied using U sbnd Th sbnd Pb and Rb sbnd Sr systematics. A Rb sbnd Sr internal isochron age of 3.89 ± 0.08b.y. with an initial 87Sr/ 86Sr of0.69926 ± 0.00008 was obtained for clast 1 (77135,57) (a troctolitic microbreccia). A troctolitic portion of microbreccia clast 77215,37 yielded a U sbnd Pb internal isochron of 3.8 ± 0.2b.y. and an initial 206Pb/ 207Pb of 0.69. These internal isochron age are interpreted as reflecting metamorphic events, probably related to impacts, which reset Rb sbnd Sr and U sbnd Pb mineral systems of older rocks. Six portions of boulder 7 were analyzed for U, Th, and Pb as whole rocks. Two chemical groups appear to be defined by the U, Th, and Pb concentration data. Chemical group A is characterized by U, Th, and Pb concentrations and 238U/ 204Pb values which are higher than those of group B. Group A rocks have typical 232Th/ 238U ratios of ∼ 3.85, whereas-group B rocks have unusually high Th/U values of ∼ 4.1. Whole-rock U sbnd Pb and Pb sbnd Pb ages are nearly concordant. Two events appear to be reflected in these data — one at ∼ 4.4 b.y. and one at ∼ 4.5 b.y. The chemical groupings show no correlation with documented ages. The old ages of ∼ 4.4 b.y. and ∼ 4.5 b.y. may, like the younger ∼ 4.0 b.y. ages, be related to basin excavation events.
- Publication:
-
Earth and Planetary Science Letters
- Pub Date:
- October 1974
- DOI:
- 10.1016/0012-821X(74)90134-4
- Bibcode:
- 1974E&PSL..23..445N
- Keywords:
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- Apollo 11 Flight;
- Breccia;
- Lunar Evolution;
- Lunar Rocks;
- Radioactive Age Determination;
- Lead Isotopes;
- Lunar Geology;
- Rubidium Isotopes;
- Strontium Isotopes;
- Thorium Isotopes;
- Uranium Isotopes