J.N. Rosholt M. Tatsumoto 1970 <p><span id="_mce_caret" data-mce-bogus="1" data-mce-type="format-caret"><span>Concentrations of U, Th, and Pb in Apollo 11 samples studied are low (U. 0.16 to 0.87; Th, 0.53 to 3.4; Pb, 0.29 to 1.7, in ppm) but the extremely radiogenic lead in samples allows radiometric dating. The fine dust and the breccia have a concordant age of 4.66 billion years on the basis of&nbsp;</span>²⁰⁷<span>Pb/</span>²⁰⁶<span>Pb,&nbsp;</span>²⁰⁶<span>Pb/</span>²³⁸<span>U,&nbsp;</span>²⁰⁷<span>Pb/</span>²³⁵<span>U, and&nbsp;</span>²⁰⁸<span>Pb/</span>²³²<span>Th ratios. This age is comparable with the age of meteorites and with the age generally accepted for the earth. Six crystalline and vesicular samples are distinctly younger than the dust and breccia. The&nbsp;</span>²³⁸<span>U/</span>²³⁵<span>U ratio is the same as that in earth rocks, and&nbsp;</span>²³⁴<span>U is in radioactive equilibrium with parent&nbsp;</span>²³⁸<span>U.</span></span></p> application/pdf 10.1126/science.167.3918.461 en American Association for the Advancement of Science Age of the moon: An isotopic study of uranium-thorium-lead systematics of lunar samples article