Lead-Lead Constraints on the Timescale of Early Planetary Differentiation

Details Lead-Lead Constraints on the Timescale of Early Planetary Differentiation Lead-Lead Constraints on the Timescale of Early Planetary Differentiation

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998lpico.957....6c&link_type=abstract

Origin of the Earth and Moon, Proceedings of the Conference held 1-3 December, 1998 in Monterey, California. LPI Contribution N

Mathematics

Logic

Solar System, Geochronology, Cosmochemistry, Extraterrestrial Matter, Meteoritic Composition, Planetary Evolution, Terrestrial Planets, Lead Compounds, Aluminum Isotopes, Hafnium Isotopes, Manganese Isotopes, Geochemistry

Scientific paper

The U-Pb-isotopic system provides unparalleled chronological resolution in the determination of absolute ages of events occurring in early solar system history. Proper comparison of these absolute ages with the relative chronologies emerging from studies of now-extinct nuclides such as Al-26, Mn-53, and Hf-182 requires identification of fixed time points in the evolution of materials in the early solar system.

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