Chondrules formed by the melting of dust aggregates in the solar protoplanetary disk and as
such provide unique insights into how solid material was transported and mixed within the …

Renazzo-type carbonaceous (CR) chondrites are distinct from most other chondrites in
having younger chondrule 26 Al-26 Mg ages, but the significance of these ages and whether …

Abstract Changes in the chemical and isotopic composition of the solar nebula with time are
reflected in the properties of different constituents that are preserved in chondritic meteorites …

Chondritic meteorites are the oldest and most primitive rocks in the solar system. They
formed as conglomerates of particles, many of which record individual, diverse nebular …

The high-temperature materials in chondritic meteorites, the chondrules (silicate spherules
produced by flash heating) and refractory inclusions (the CAI, or calcium-aluminum–rich …

Dynamic models of the protoplanetary disk indicate there should be large-scale material
transport in and out of the inner Solar System, but direct evidence for such transport is …

We present an overview of the chondrite groups focusing on the major constraints that can
be derived on thermal history of silicates in the solar nebula from the mineralogical …

Chondrite meteorites are samples of primitive asteroidal bodies that have escaped melting
and differentiation. The only record of our Solar System's formative stages comes from the …

The elemental and isotopic compositions of meteorites are expected to reflect several key
processes that occurred in the early solar system, including the migration of gas and dust …

We review the oxygen isotopic compositions of chondrite components (refractory inclusions,
chondrules, and matrix) and their inter-and intra-crystalline oxygen isotopic distributions …