Nucleosynthetic isotope variations are powerful tools to investigate genetic relationships
between meteorite groups and planets. They are instrumental to assess the early evolution …

Nucleosynthetic isotope signatures in meteorites provide key insights into the structure and
dynamics of the solar protoplanetary disk and the accretion history of the planets. We …

The isotopic composition of meteorites and terrestrial planets holds important clues about
the earliest history of the Solar System and the processes of planet formation. Recent work …

The fundamentally different isotopic compositions of non-carbonaceous (NC) and
carbonaceous (CC) meteorites reveal the presence of two distinct reservoirs in the solar …

Understanding the formation of our planetary system requires identification of the materials
from which it originated and the accretion processes that produced the planets. The …

Stable-isotope variations exist among inner solar system solids, planets, and asteroids, but
their importance is not understood. We report correlated, mass-independent variations of …

The recent advent of nontraditional isotopic systems has revealed that meteorites display a
fundamental isotopic dichotomy between noncarbonaceous (NC) and carbonaceous (C) …

Nucleosynthetic isotope variability among solar system objects provides insights into the
accretion history of terrestrial planets. We report on the nucleosynthetic Fe isotope …

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

The isotopic composition of meteorites reveals a fundamental dichotomy between non-
carbonaceous (NC) and carbonaceous (CC) meteorites. However, the origin of this …