Nucleosynthetic isotope anomalies are powerful tracers to determine the provenance of
meteorites and their components, and to identify genetic links between these materials. Here …

The early evolution of the solar nebula involved substantial transport of mass, resulting in
mixing and homogenization of isotopically diverse materials that were contributed to the …

Mass-dependent Mo isotope fractionation has been investigated for a wide range of
meteorites including chondrites (enstatite, ordinary and carbonaceous chondrites), iron …

Abstract Changes in the chemical and isotopic composition of the solar nebula with time are
reflected in the properties of different constituents that are preserved in chondritic meteorites …

Whole rock Δ 17 O and nucleosynthetic isotopic variations for chromium, titanium, nickel,
and molybdenum in meteorites define two isotopically distinct populations: carbonaceous …

Several stages in the evolution of ordinary chondritic meteorites are recorded in the oxygen
isotopic composition of the meteorites and their separable components (chondrules …

We have investigated nucleosynthetic Mo isotope anomalies in 38 different bulk iron
meteorites from 11 groups, to produce by far the largest and most precise dataset available …

Nucleosynthetic isotope anomalies in bulk chondrites and differentiated meteorites reflect
variable proportions of isotopically diverse presolar components in bulk planetary bodies …

We present an overview of the chondrite groups focusing on the major constraints that can
be derived on thermal history of silicates in the solar nebula from the mineralogical …

Chondritic meteorites are the oldest and most primitive rocks in the solar system. They
formed as conglomerates of particles, many of which record individual, diverse nebular …