Results 131 to 140 of about 74,370 (266)
Hybrid Olivine Phenocryst Populations in the 1959 Kīlauea Eruption and Constraints on their Time of Arrival in the Summit Reservoir [PDF]
Rosalind T. Helz, Timothy M. Rose
openalex +1 more source
The \textit{Spitzer}/Infrared Spectrograph spectra of three spectroscopically anomalous galaxies (IRAS~F10398+1455, IRAS~F21013-0739 and SDSS~J0808+3948) are modeled in terms of a mixture of warm and cold silicate dust, and warm and cold carbon dust ...
Hao, Lei +3 more
core +1 more source
Abstract We conducted a scanning electron microscopy (SEM) and transmission electron microscopy (TEM) study of sulfide–metal assemblages (SMAs) in minimally to moderately altered CR2 chondrites. The assemblages occur on chondrule rims and consist of kamacite cores rimmed by pyrrhotite.
S. A. Singerling, A. J. Brearley
wiley +1 more source
Experimental constraints on the origin of metal and carbon in ureilite meteorites
Abstract Ureilites are carbon‐rich ultramafic achondrites that display unique textures, including strips of metal and carbon phases situated along grain boundaries and in fractures. Shock metamorphism observed in ureilites suggests an episode of brittle deformation caused by impact disruption of their parent body.
Nicolas P. Walte +2 more
wiley +1 more source
Structural Evolution of Olivine during Mechanochemically Assisted Mineral Carbonation under CO2 Flow
The mechanism of the mechanically assisted mineral carbonation of commercial olivine under the flow of a carbon dioxide (CO2)/nitrogen (N2) mixture has been elucidated by ex situ powder X-ray diffraction and Fourier-transform infrared spectroscopy.
Costantino Cau +7 more
doaj +1 more source
Chromite in main group pallasite meteorites: Accessory mineral tracing planetesimal differentiation
Abstract Main group pallasite meteorites (PMG) are samples of an early, highly differentiated magmatic planetesimal dominated by olivine and metal‐sulfide‐phosphide assemblages with accessory chromite among other phases. This mineralogy reflects mantle‐ and core‐related reservoirs, but the relative contributions of each and the overall petrogenesis are
Seann J. McKibbin +6 more
wiley +1 more source
Quantifying the timescales of fluid-rock interaction on Mars using the nakhlite meteorites [PDF]
Etch pits within olivine grains from the nakhlite meteorites reveal the magnitude and timescale of water-mediated alteration of the martian ...
Lee, M.R. +4 more
core
Upper mantle deformation is mainly controlled by the mechanical behavior of olivine. Crystallographic preferred orientations (CPOs) develop in olivine due to crystal‐plastic deformation during mantle flow, where the a‐axes of olivine polycrystalline ...
Y. Yu +7 more
doaj +1 more source
The Mobility of Major and Trace Elements in EOC Minerals on Parent Chondrite Bodies
The combined EPMA and SIMS study of the geochemical features of olivine, low-Ca pyroxene and plagioclase in equilibrated ordinary chondrites (EOCs) has revealed the effect of thermal metamorphism on trace element concentrations in EOC silicate minerals ...
Kristina Sukhanova, Sergey Skublov
doaj +1 more source
Parent body thermal metamorphism of enstatite chondrites: Disentangling the effects of shock melting
Abstract Enstatite chondrites (ECs) formed on at least two parent bodies, EH and EL. After the accretion of the EC parent bodies, EC material was subjected to varying degrees of parent body thermal metamorphism (measured by petrologic types 3–6), due to heat released by radioactive isotope decay.
Peter Mc Ardle +9 more
wiley +1 more source

