Affiliation:
1. Institut für Mineralogie, Universität Münster, Corrensstrasse 24, 48149 Münster, Germany.
Abstract
Well-defined constants of radioactive decay are the cornerstone of geochronology and the use of radiogenic isotopes to constrain the time scales and mechanisms of planetary differentiation. Four new determinations of the lutetium-176 decay constant (λ
176
Lu) made by calibration against the uranium-lead decay schemes yield a mean value of 1.865 ± 0.015 × 10
−11
year
−1
, in agreement with the two most recent decay-counting experiments. Lutetium-hafnium ages that are based on the previously used λ
176
Lu of 1.93 × 10
−11
to 1.94 × 10
−11
year
−1
are thus ∼4% too young, and the initial hafnium isotope compositions of some of Earth's oldest minerals and rocks become less radiogenic relative to bulk undifferentiated Earth when calculated using the new decay constant. The existence of strongly unradiogenic hafnium in Early Archean and Hadean zircons implies that enriched crustal reservoirs existed on Earth by 4.3 billion years ago and persisted for 200 million years or more. Hence, current models of early terrestrial differentiation need revision.
Publisher
American Association for the Advancement of Science (AAAS)
Reference51 articles.
1. The value of ε Hf is the deviation of the 176 Hf/ 177 Hf of a sample in parts per 10 4 from that of the CHUR reference: [( 176 Hf/ 177 Hf) sample /( 176 Hf/ 177 Hf) CHUR – 1] × 10 4 . The initial ε Hf or ε Hf ( t ) is the deviation from CHUR when the sample crystallized at time t : {[( 176 Hf/ 177 Hf) sample – ( 176 Lu/ 177 Hf) sample (e λ t – 1)]/[( 176 Hf/ 177 Hf) CHUR – ( 176 Lu/ 177 Hf) CHUR (e λ t – 1)] – 1} × 10 4 .
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