The isotopic composition of our Solar System reflects the blending of materials derived from
numerous past nucleosynthetic events, each characterized by a distinct isotopic signature …

In order to better constrain the Li isotope composition of the bulk solar system and Li isotope
fractionation during accretion and parent body processes, Li isotope compositions and …

We report the Li isotopic compositions of nine large, greater than 5 μm, presolar SiC grains
from the Murchison (CM) meteorite. Most of the SiC grains analyzed are isotopically similar …

We report the Ti isotopic compositions of 8 mainstream, 22 Y, 9 Z, and 26 AB presolar SiC
grains from two SiC-rich residues of the Murchison CM2 meteorite together with Si, C and …

We report the first measurements of lithium and boron isotope ratios and abundances
measured in “gently separated” presolar SiC grains. Almost all analyses of presolar SiC …

Thirteen presolar silicon carbide grains—three of supernova (SN) origin and ten of
asymptotic giant branch (AGB) star origin—were examined with time‐of‐flight‐secondary ion …

We have analyzed eleven presolar SiC grains from the Murchison meteorite using time‐of‐
flight secondary ion mass spectrometry. The Si isotopic compositions of the grains indicate …

Historically, uranium has received intense study of its chemical and isotopic properties for
use in the nuclear industry, but has been largely ignored by geoscientists despite properties …

This review surveys the literature on the chemical analysis of terrestrial and extraterrestrial
solids for the 2-year period October 2004 through September 2006. We continue to include …

Abstract 207 Pb*/206 Pb* chronometry was used to obtain the ages of Ca, Al-rich inclusions
(CAIs) and chondrules found in ancient meteorites. Assuming a 238 U/235 U= 137.88 …