The great isotopic dichotomy of the early Solar System
TS Kruijer, T Kleine, LE Borg - Nature Astronomy, 2020 - nature.com
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 earliest history of the Solar System and the processes of planet formation. Recent work …
The non-carbonaceous–carbonaceous meteorite dichotomy
The isotopic dichotomy between non-carbonaceous (NC) and carbonaceous (CC)
meteorites indicates that meteorite parent bodies derive from two genetically distinct …
meteorites indicates that meteorite parent bodies derive from two genetically distinct …
Isotopic evolution of the inner solar system inferred from molybdenum isotopes in meteorites
The fundamentally different isotopic compositions of non-carbonaceous (NC) and
carbonaceous (CC) meteorites reveal the presence of two distinct reservoirs in the solar …
carbonaceous (CC) meteorites reveal the presence of two distinct reservoirs in the solar …
The partitioning of the inner and outer Solar System by a structured protoplanetary disk
R Brasser, SJ Mojzsis - Nature Astronomy, 2020 - nature.com
Mass-independent isotopic anomalies define two cosmochemically distinct regions: the
carbonaceous and non-carbonaceous meteorites, implying that the non-carbonaceous …
carbonaceous and non-carbonaceous meteorites, implying that the non-carbonaceous …
The NC-CC isotope dichotomy: Implications for the chemical and isotopic evolution of the early Solar System
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 …
from which it originated and the accretion processes that produced the planets. The …
Origin of the non-carbonaceous–carbonaceous meteorite dichotomy
The isotopic composition of meteorites reveals a fundamental dichotomy between non-
carbonaceous (NC) and carbonaceous (CC) meteorites. However, the origin of this …
carbonaceous (NC) and carbonaceous (CC) meteorites. However, the origin of this …
Iron isotope evidence for very rapid accretion and differentiation of the proto-Earth
Nucleosynthetic isotope variability among solar system objects provides insights into the
accretion history of terrestrial planets. We report on the nucleosynthetic Fe isotope …
accretion history of terrestrial planets. We report on the nucleosynthetic Fe isotope …
Origin of isotopic diversity among carbonaceous chondrites
Carbonaceous chondrites are some of the most primitive meteorites and derive from
planetesimals that formed a few million years after the beginning of the solar system. Here …
planetesimals that formed a few million years after the beginning of the solar system. Here …
Isotopic dichotomy among meteorites and its bearing on the protoplanetary disk
ERD Scott, AN Krot, IS Sanders - The Astrophysical Journal, 2018 - iopscience.iop.org
Whole rock Δ 17 O and nucleosynthetic isotopic variations for chromium, titanium, nickel,
and molybdenum in meteorites define two isotopically distinct populations: carbonaceous …
and molybdenum in meteorites define two isotopically distinct populations: carbonaceous …
Age of Jupiter inferred from the distinct genetics and formation times of meteorites
The age of Jupiter, the largest planet in our Solar System, is still unknown. Gas-giant planet
formation likely involved the growth of large solid cores, followed by the accumulation of gas …
formation likely involved the growth of large solid cores, followed by the accumulation of gas …