[meteorite-list] ASU recalculates age of solar system/ Interesting Allende CAI details
From: power ofunity <energylightandlove_at_meteoritecentral.com>
Date: Fri, 1 Jan 2010 10:55:06 -0800 (PST) Message-ID: <311364.22307.qm_at_web59002.mail.re1.yahoo.com> Interesting read from ASU -?with supporting details and fascinating info regarding Allende's CAIs http://asunews.asu.edu/20091231_brennecka ? ? http://www.sciencemag.org/cgi/content/abstract/science.1180871 ? ? Published Online December 31, 2009 Science DOI: 10.1126/science.1180871 ? Reports 238U/235U Variations in Meteorites: Extant 247Cm and Implications for Pb-Pb DatingG. A. Brennecka,1, S. Weyer,2, M. Wadhwa,1 P. E. Janney,1 J. Zipfel,3 A. D. Anbar1,4 The 238U/235U isotope ratio has long been considered invariantin meteoritic materials (i.e., 137.88). This assumption is acornerstone of the high-precision Pb-Pb dates that define theabsolute age of the Solar System. Calcium-aluminum-rich inclusionsof the Allende meteorite display variable 238U/235U ratios,ranging between 137.409?0.039 and 137.885?0.009.This range implies substantial uncertainties in the ages previouslydetermined by Pb-Pb dating of CAIs, which may be overestimatedby several million years. The correlation of U isotope ratioswith proxies for Cm/U (i.e., Th/U and Nd/U) provides strongevidence that the observed variations of 238U/235U in CAIs wereproduced by the decay of extant 247Cm to 235U in the early SolarSystem, with an initial 247Cm/235U of ~ 1.1 to 2.4 x 10-4. ?1 School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA. 2 Institut fur Geowissenschaften, Goethe-Universit?t, Frankfurt, Germany. 3 Senckenberg Forschungsinstitut und Naturmuseum, Frankfurt, Germany. 4 Department of Chemistry and Biochemistry, Arizona State University, Tempe, AZ 85287, USA. Current address: Institut f?r Geology und Mineralogie,Universit?t zu K?ln, Cologne, Germany. To whom correspondence should be addressed. E-mail: brennecka at asu.edu ________________________________ Received for publication 20 August 2009. Accepted for publication 11 December 2009. Received on Fri 01 Jan 2010 01:55:06 PM PST |
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