Chondrules: Precursors and interactions with the nebular gas

RH Hewins, B Zanda - Meteoritics & Planetary Science, 2012 - Wiley Online Library
Chondrule compositions suggest either ferroan precursors and evaporation, or magnesian
precursors and condensation. Type I chondrule precursors include granoblastic olivine …

Evaporation and recondensation of sodium in Semarkona Type II chondrules

RH Hewins, B Zanda, C Bendersky - Geochimica et Cosmochimica Acta, 2012 - Elsevier
We have investigated the Na distributions in Semarkona Type II chondrules by electron
microprobe, analyzing olivine and melt inclusions in it, mesostasis and bulk chondrule, to …

Magnetic fields recorded by chondrules formed in nebular shocks

C Mai, SJ Desch, AC Boley… - The Astrophysical …, 2018 - iopscience.iop.org
Recent laboratory efforts have constrained the remanent magnetizations of chondrules and
the magnetic field strengths to which the chondrules were exposed as they cooled below …

Dynamic evolution of C-type asteroids inferred from carbonaceous CM chondrites

CJ Floyd - 2024 - theses.gla.ac.uk
The Mighei-like (CM) group of carbonaceous chondrites are water and carbon-rich
meteorites which have been identified as the most chemically primitive chondrites available …