| Literature DB >> 17525335 |
Richard W Carlson1, Maud Boyet, Mary Horan.
Abstract
Isotopic variability in barium, neodymium, and samarium in carbonaceous chondrites reflects the distinct stellar nucleosynthetic contributions to the early solar system. We used 148Nd/144Nd to correct for the observed s-process deficiency, which produced a chondrite 146Sm-142Nd isochron consistent with previous estimates of the initial solar system abundance of 146Sm and a 142Nd/144Nd at average chondrite Sm/Nd ratio that is lower than that measured in terrestrial rocks by 21 +/- 3 parts per million. This result strengthens the conclusion that the deficiency in 142Nd in chondrites relative to terrestrial rocks reflects 146Sm decayand earlyplanetary differentiation processes.Entities:
Year: 2007 PMID: 17525335 DOI: 10.1126/science.1140189
Source DB: PubMed Journal: Science ISSN: 0036-8075 Impact factor: 47.728