title: Barium isotopes in chondritic meteorites: implications for planetary reservoir models.
abstract: High-precision barium isotope measurements yielded differences of up to 25 parts per million in the 137Ba/136Ba ratio and 60 parts per million in the 138Ba/136Ba ratio between chondrites and Earth. These differences probably arose from incomplete mixing of nucleosynthetic material in the solar nebula. Chondritic meteorites have a slight excess of supernova-derived material as compared to Earth, demonstrating that the solar nebula was not perfectly homogenized upon formation.
authors.affiliation: Department of Earth and Planetary Sciences, Harvard University, 20 Oxford Street, Cambridge, MA 02138, USA. ranen@fas.harvard.edu
authors.forename: Michael C
authors.initials: MC
authors.lastname: Ranen
authors.forename: Stein B
authors.initials: SB
authors.lastname: Jacobsen