Chondritic components such as chondrules and matrix are the key time capsules that can
help us understand the evolution and dynamics of the protoplanetary disk from which the …

Chondrules, millimeter-sized igneous spherules comprising the major component of most
chondritic meteorites, formed during the first 4 million to 5 million years of the evolution of the …

We report microscopic, cathodoluminescence, chemical, and O isotopic measurements of
FeO‐poor isolated olivine grains (IOG) in the carbonaceous chondrites Allende (CV3) …

FeO-poor (type I) porphyritic chondrules formed by incomplete melting of solid dust
precursors via a yet-elusive mechanism. Two settings are generally considered for their …

We studied the texture of 256 chondrules in thin sections of 16 different carbonaceous (CV,
CR, CO, CM, CH) and Rumuruti chondrites. In a conservative count∼ 75% of all chondrules …

We investigate the coupling between H, minor, trace, and ultra-trace element incorporations
in 17 olivines from ten different locations covering various petrological origins: magmatic …

Compound chondrules, ie chondrules fused together, make a powerful probe of the density
and compositional diversity in chondrule-forming environments, but their abundance among …

We report trace element concentrations of silicate phases in chondrules from LL3 ordinary
chondrites Bishunpur and Semarkona. Results are similar to previously reported data for …

We report combined oxygen isotope and mineral‐scale trace element analyses of amoeboid
olivine aggregates (AOA) and chondrules in ungrouped carbonaceous chondrite, Northwest …

In order to investigate the influence of very reducing conditions, we report enstatite-melt
trace element partition coefficients (D) obtained on enstatite chondrite material at 5 GPa and …