Redox conditions in the solar nebula: Observational, experimental, and theoretical constraints

L Grossman, JR Beckett, AV Fedkin… - … in Mineralogy and …, 2008 - pubs.geoscienceworld.org
Crystallization experiments on liquids with compositions similar to those of compact Type A,
Type B1 and Type B2 refractory inclusions were conducted under controlled temperature …

Dynamic mechanical behavior of multilayer graphene via supersonic projectile penetration

JH Lee, PE Loya, J Lou, EL Thomas - Science, 2014 - science.org
Multilayer graphene is an exceptional anisotropic material due to its layered structure
composed of two-dimensional carbon lattices. Although the intrinsic mechanical properties …

Nanophase Iron Particles Derived From Fayalitic Olivine Decomposition in Chang'E‐5 Lunar Soil: Implications for Thermal Effects During Impacts

Z Guo, C Li, Y Li, Y Wen, K Tai, X Li… - Geophysical …, 2022 - Wiley Online Library
Surface‐correlated nanophase iron particles (npFe0) alter the reflectance spectrum
characteristics of airless bodies, thus making it an essential aspect of studying space …

Solar nebula magnetic fields recorded in the Semarkona meteorite

RR Fu, BP Weiss, EA Lima, RJ Harrison, XN Bai… - Science, 2014 - science.org
Magnetic fields are proposed to have played a critical role in some of the most enigmatic
processes of planetary formation by mediating the rapid accretion of disk material onto the …

Experimental constraints on chondrule formation

RH Hewins, HC Connolly… - Chondrites and the …, 2005 - adsabs.harvard.edu
Chondrule textures depend on the extent of melting of the chondrule precursor material
when cooling starts. If viable nuclei remain in the melt, crystallization begins immediately …

[HTML][HTML] The most primitive CM chondrites, Asuka 12085, 12169, and 12236, of subtypes 3.0–2.8: Their characteristic features and classification

M Kimura, N Imae, M Komatsu, JA Barrat… - Polar Science, 2020 - Elsevier
CM chondrites (CMs) are the most abundant group of carbonaceous chondrites. CMs
experienced varying degrees of secondary aqueous alteration and heating that modified or …

Petrographic constraints on the diversity of chondrule reservoirs in the protoplanetary disk

RH Jones - Meteoritics & Planetary Science, 2012 - Wiley Online Library
Chondrules from different chondrite groups show characteristic properties, including
abundances of different chondrule textural types, chondrule sizes, oxygen isotope …

Oxygen isotopic diversity of chondrule precursors and the nebular origin of chondrules

Y Marrocchi, J Villeneuve, V Batanova, L Piani… - Earth and Planetary …, 2018 - Elsevier
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 …

Chemical, mineralogical and isotopic properties of chondrules: Clues to their origin

RH Jones, JN Grossman… - Chondrites and the …, 2005 - adsabs.harvard.edu
We review chemical, mineralogical and isotopic properties of chondrules that can be used to
investigate chondrule origins. Although many interpretations of chondrule properties are …

SIMS matrix effects in oxygen isotope analysis of olivine and pyroxene: Application to Acfer 094 chondrite chondrules and reconsideration of the primitive chondrule …

M Zhang, K Fukuda, MJ Spicuzza, G Siron, A Heimann… - Chemical …, 2022 - Elsevier
The instrumental bias (here expressed as bias*, the difference relative to San Carlos Olivine,
SC-Ol) of oxygen isotopes in secondary ion mass spectrometry (SIMS) analyses of olivine …