Carbonaceous chondrites are some of the most primitive meteorites and derive from planetesimals that formed a few million years after the beginning of the solar system. Here …
HC Connolly Jr, GR Huss - Geochimica et Cosmochimica Acta, 2010 - Elsevier
Chondrules are the dominant component of chondritic meteorites and attest to high- temperature transient heating events within the protoplanetary disk. They provide valuable …
DL Schrader, K Nagashima, AN Krot, RC Ogliore… - … et Cosmochimica Acta, 2017 - Elsevier
We report on the mineralogy, petrography, and in situ measured oxygen-and magnesium- isotope compositions of eight porphyritic chondrules (seven FeO-poor and one FeO-rich) …
K Zhu, J Liu, F Moynier, L Qin… - The Astrophysical …, 2019 - iopscience.iop.org
Chondrules are the main components of primitive meteorites and possibly the building blocks of planetary embryos and terrestrial planets. However, their ages and modes of …
We report on the petrology, magnesium isotopes and mass-independent 54 Cr/52 Cr compositions (μ 54 Cr) of 42 chondrules from CV (Vigarano and NWA 3118) and CR (NWA …
Chondrules are sub-millimetric spheroids that are ubiquitous in chondrites and whose formation mechanism remains elusive. Textural and oxygen isotopic characteristics of …
CV chondrites are one of the most studied group of carbonaceous chondrites. Based on a number of mineralogical features, they have been divided into three sub-groups: CV OxA …
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 …
Isotopic anomalies in chondrules hold important clues about the dynamics of mixing and transport processes in the solar accretion disk. The meaning of these anomalies is debated …