Add to ORKGThe process responsible for the mass independent oxygen isotope variation observed in Solar System materials remains poorly understood. While self-shielding of CO, either in the early solar nebula, or precursor molecular cloud, appears to be a viable mechanism, alternative models have also been proposed
Chondritic meteorites contain a diversity of particle components, i.e., chondrules and calcium-, alu...
The isotopic composition of oxygen as well as ^(26)Al-^(26)Mg and ^(36)Cl-^(36)S systematics were st...
Carbonaceous chondrites contain a mixture of solar system condensates, pre-solar grains, and primiti...
As originally demonstrated by Clayton and co-workers, primitive meteorites and their components comm...
AbstractCalcium–aluminium-rich Inclusions (CAIs) and the thin Wark–Lovering (WL) rims of minerals su...
Water played a critical role in the early evolution of asteroids and planets, as well as being an es...
Calcium–aluminium-rich Inclusions(CAIs) and the thin Wark–Lovering (WL) rims of minerals surrounding...
Dark inclusions (DIs) are lithic fragments that form a volumetrically small, but important, componen...
International audiencePrimitive chondrites have bulk compositions close to that of the solar photosp...
Oxygen isotope analysis has become an indispensable tool in the study of early Solar System processe...
We report the mineralogy, petrology, major, minor and trace element geochemistry, O and Si isotopes ...
AbstractNucleosynthetic isotope anomalies are powerful tracers to determine the provenance of meteor...
Oxygen isotopic compositions of the high-temperatue phases in carbonaceous chondrites define a mixin...
Anhydrous alteration of eleven Allende chondrules with already-known oxygen isotopic compositions we...
Oxygen isotopes were measured in four chondritic hydrated interplanetary dust particles (IDPs) and f...
Chondritic meteorites contain a diversity of particle components, i.e., chondrules and calcium-, alu...
The isotopic composition of oxygen as well as ^(26)Al-^(26)Mg and ^(36)Cl-^(36)S systematics were st...
Carbonaceous chondrites contain a mixture of solar system condensates, pre-solar grains, and primiti...
As originally demonstrated by Clayton and co-workers, primitive meteorites and their components comm...
AbstractCalcium–aluminium-rich Inclusions (CAIs) and the thin Wark–Lovering (WL) rims of minerals su...
Water played a critical role in the early evolution of asteroids and planets, as well as being an es...
Calcium–aluminium-rich Inclusions(CAIs) and the thin Wark–Lovering (WL) rims of minerals surrounding...
Dark inclusions (DIs) are lithic fragments that form a volumetrically small, but important, componen...
International audiencePrimitive chondrites have bulk compositions close to that of the solar photosp...
Oxygen isotope analysis has become an indispensable tool in the study of early Solar System processe...
We report the mineralogy, petrology, major, minor and trace element geochemistry, O and Si isotopes ...
AbstractNucleosynthetic isotope anomalies are powerful tracers to determine the provenance of meteor...
Oxygen isotopic compositions of the high-temperatue phases in carbonaceous chondrites define a mixin...
Anhydrous alteration of eleven Allende chondrules with already-known oxygen isotopic compositions we...
Oxygen isotopes were measured in four chondritic hydrated interplanetary dust particles (IDPs) and f...
Chondritic meteorites contain a diversity of particle components, i.e., chondrules and calcium-, alu...
The isotopic composition of oxygen as well as ^(26)Al-^(26)Mg and ^(36)Cl-^(36)S systematics were st...
Carbonaceous chondrites contain a mixture of solar system condensates, pre-solar grains, and primiti...