A quantitative understanding of the elemental and isotopic fractionations recorded in the
compositions of the chondritic meteorites would provide fundamental constraints for …

Two models that for the first time attempt to quantitatively reproduce the bulk elemental and
isotopic fractionations amongst the non-carbonaceous chondrites (non-CCs) are explored …

Twenty carbonaceous chondrites were analyzed by instrumental and radiochemical neutron
activation analysis for Na, Mg, Al, K, Ca, Sc, V. Cr, Mn. Fe, Co, Ni, Zn, Ga, Ge, As, Se. Br. Ru …

We report the bulk C abundances, and C and O isotopic compositions of carbonates in 64
CM chondrites, 14 CR chondrites, 2 CI chondrites, LEW 85332 (C2), Kaba (CV 3), and …

Abstract Seven carbonaceous chondrites (Allan Hills A77307, Adelaide, Al Rais, Coolidge,
Grosnaja, Karoonda and Renazzo) with uncertain classifications were analyzed by …

Compared to the composition of CI chondrites and the Sun, all other carbonaceous
chondrites are variably depleted in volatile elements. However, the origin of these …

We present new hydrogen isotope data for separated matrix, hydrated chondrules, and other
hydrated coarse silicate fragments from nine carbonaceous chondrites. These data were …

We have undertaken a comprehensive study of carbon and nitrogen elemental abundances
and isotopic compositions of bulk carbonaceous chondrites. A strategy of multiple analyses …

To better understand the environment of chondrule formation and constrain the O-isotope
composition of the ambient gas in the Renazzo-like carbonaceous (CR) chondrite chondrule …

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 …