Nebel, OliverScherer, Erik EMezger, Klaus2015-12-100012-821Xhttp://hdl.handle.net/1885/65027The Rb-Sr decay system is one of the most widely used geochronometers for obtaining ages and cooling rates of terrestrial magmatic, metamorphic, and hydrothermal events. It has also been extensively applied to date extraterrestrial, early solar system events. The accuracy of Rb-Sr ages, however, strongly depends on the accuracy of the87Rb decay constant (λ87Rb). We determined λ87Rb relative to the decay constants of235U and238U by comparing Rb-Sr ages of minerals with U-Pb ages obtained from the same intrusion. Comparison of U-Pb emplacement ages with high-precision Rb-Sr mineral ages from three rapidly cooled igneous rocks covering an age range of ca. 2.5Ga yields an unweighted mean λ87Rb of 1.393±0.004×10λ11yr-1 (i.e., ±0.3%), corresponding to a half-life of 49.76×109years. Because this decay constant is 2% lower than the presently recommended one, many previously published ages are 2% too young and the resulting geologic interpretations may need revision.Keywords: Age comparison; Cooling rates; Decay constants; Early solar systems; Geologic interpretation; High-precision; Rb-Sr; U-Pb ages; Decay (organic); Gallium; Igneous rocks; Lead; Minerals; Solar system; Rubidium; age determination; emplacement; rubidium-stron Age comparison; Decay constant; Rb-Sr; Rubidium201110.1016/j.epsl.2010.11.0042016-02-24