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 …
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 …
Bifurcation of planetary building blocks during Solar System formation
T Lichtenberg, J Dra̧żkowska, M Schönbächler… - Science, 2021 - science.org
Geochemical and astronomical evidence demonstrates that planet formation occurred in two
spatially and temporally separated reservoirs. The origin of this dichotomy is unknown. We …
spatially and temporally separated reservoirs. The origin of this dichotomy is unknown. We …
Dust masses of young disks: constraining the initial solid reservoir for planet formation
Ł Tychoniec, CF Manara, GP Rosotti… - Astronomy & …, 2020 - aanda.org
Context. Recent years have seen building evidence that planet formation starts early, in the
first~ 0.5 Myr. Studying the dust masses available in young disks enables us to understand …
first~ 0.5 Myr. Studying the dust masses available in young disks enables us to understand …
The effect of Jupiter's formation on the distribution of refractory elements and inclusions in meteorites
We present a comprehensive evolutionary model of the Sun's protoplanetary disk,
constructed to resolve the" CAI storage problem" of meteoritics. We predict the abundances …
constructed to resolve the" CAI storage problem" of meteoritics. We predict the abundances …
[HTML][HTML] Molybdenum isotopic evidence for the origin of chondrules and a distinct genetic heritage of carbonaceous and non-carbonaceous meteorites
Nucleosynthetic isotope anomalies are powerful tracers to determine the provenance of
meteorites and their components, and to identify genetic links between these materials. Here …
meteorites and their components, and to identify genetic links between these materials. Here …
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 …
Evidence of fast pebble growth near condensation fronts in the HL Tau protoplanetary disk
Water and simple organic molecular ices dominate the mass of solid materials available for
planetesimal and planet formation beyond the water snow line. Here we analyze ALMA long …
planetesimal and planet formation beyond the water snow line. Here we analyze ALMA long …
Mass fractionation laws, mass-independent effects, and isotopic anomalies
N Dauphas, EA Schauble - Annual Review of Earth and …, 2016 - annualreviews.org
Isotopic variations usually follow mass-dependent fractionation, meaning that the relative
variations in isotopic ratios scale with the difference in mass of the isotopes involved (eg …
variations in isotopic ratios scale with the difference in mass of the isotopes involved (eg …