53Mn–53Cr systematics of the early Solar System revisited
A Trinquier, JL Birck, CJ Allègre, C Göpel… - … et Cosmochimica Acta, 2008 - Elsevier
We have reinvestigated the Mn–Cr systematics in a number of primitive meteorites,
differentiated planetesimals and terrestrial planets in order to address the chronology of the …
differentiated planetesimals and terrestrial planets in order to address the chronology of the …
Organic thermometry for chondritic parent bodies
A unique spectroscopic feature has been identified in a study of twenty-five different samples
of meteoritic insoluble organic matter (IOM) spanning multiple chemical classes, groups, and …
of meteoritic insoluble organic matter (IOM) spanning multiple chemical classes, groups, and …
Experimental calibration of aluminum partitioning between olivine and spinel as a geothermometer
Z Wan, LA Coogan, D Canil - American Mineralogist, 2008 - pubs.geoscienceworld.org
The temperature dependence of the partitioning of Al2O3 between forsterite-rich olivine and
Cr-rich spinels has been experimentally calibrated at 100 kPa between 1250 and 1450° C …
Cr-rich spinels has been experimentally calibrated at 100 kPa between 1250 and 1450° C …
The origin and evolution of organic matter in carbonaceous chondrites and links to their parent bodies
DP Glavin, CMOD Alexander, JC Aponte… - Primitive meteorites and …, 2018 - Elsevier
The nature of organic matter in meteorites reveals information about early solar system
chemistry and the histories of parent bodies as recorded in the effects of physical and …
chemistry and the histories of parent bodies as recorded in the effects of physical and …
Sulfide-olivine Fe-Ni exchange and the origin of anomalously Ni rich magmatic sulfides
Equilibration between sulfide liquid and olivine is expressed in terms of the exchange
coefficient for Fe and Ni, KD=(XNiS/XFeS) sulfide_liquid/(XNiO/XFeO) olivine. The positive …
coefficient for Fe and Ni, KD=(XNiS/XFeS) sulfide_liquid/(XNiO/XFeO) olivine. The positive …
Thermal history of type 3 chondrites from the Antarctic meteorite collection determined by Raman spectroscopy of their polyaromatic carbonaceous matter
L Bonal, E Quirico, L Flandinet, G Montagnac - … et Cosmochimica Acta, 2016 - Elsevier
This paper is focused on the characterization of the thermal history of 151 CV, CO and
unequilibrated ordinary chondrites (UOCs) from the NASA Antarctic meteorite collection …
unequilibrated ordinary chondrites (UOCs) from the NASA Antarctic meteorite collection …
The Fe/S ratio of pyrrhotite group sulfides in chondrites: An indicator of oxidation and implications for return samples from asteroids Ryugu and Bennu
Determining compositional trends among individual minerals is key to understanding the
thermodynamic conditions under which they formed and altered, and is also essential to …
thermodynamic conditions under which they formed and altered, and is also essential to …
Hf–W mineral isochron for Ca, Al-rich inclusions: age of the solar system and the timing of core formation in planetesimals
Application of 182Hf–182W chronometry to constrain the duration of early solar system
processes requires the precise knowledge of the initial Hf and W isotope compositions of the …
processes requires the precise knowledge of the initial Hf and W isotope compositions of the …
The accretion and impact history of the ordinary chondrite parent bodies
T Blackburn, CMOD Alexander, R Carlson… - … et Cosmochimica Acta, 2017 - Elsevier
A working timeline for the history of ordinary chondrites includes chondrule formation as
early as 0–2 Ma after our Solar System's earliest forming solids (CAIs), followed by rapid …
early as 0–2 Ma after our Solar System's earliest forming solids (CAIs), followed by rapid …
[HTML][HTML] Hf–W thermochronometry: closure temperature and constraints on the accretion and cooling history of the H chondrite parent body
We obtained Hf–W metal-silicate isochrons for several H chondrites of petrologic types 4, 5,
and 6 to constrain the accretion and high-temperature thermal history of the H chondrite …
and 6 to constrain the accretion and high-temperature thermal history of the H chondrite …