0000000000205072

AUTHOR

Dominik C. Hezel

0000-0002-5059-2281

showing 3 related works from this author

Evidence for fractional condensation and reprocessing at high temperatures in CH chondrites

2003

We performed a detailed study of silica-rich components (SRC) in the paired CH chondrites Acfer 182 and 207. These SRCs appear either as chondrules or fragments, and they contribute <0.1 vol% to the bulk meteorite. They usually contain a silica and a silicate portion. Both portions are, in most cases, cryptocrystalline and have bulk SiO2-concentrations between 65 and 85 wt%. The silicate generally has a pyroxene normative composition. The silica often appears as blebs within the silicate matrix or vice versa. If there are no blebs, silica and silicate still form rounded interfaces. The SRCs are depleted in refractory elements like Ca, Al, and Ti relative to CI. A few SRC- like objects are e…

OlivineAnalytical chemistryChondruleMineralogyPyroxeneForsteriteengineering.materialCristobaliteSilicatechemistry.chemical_compoundGeophysicschemistrySpace and Planetary ScienceChondriteEnstatiteengineeringGeologyMeteoritics &amp; Planetary Science
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In situ micro-Raman and X-ray diffraction study of diamonds and petrology of the new ureilite UAE 001 from the United Arab Emirates

2008

International audience; A new olivine-pigeonite ureilite containing abundant diamonds and graphite was found in the United Arab Emirates. This is the first report of a meteorite in this country. The sample is heavily altered, of medium shock level, and has a total weight of 155 g. Bulk rock, olivine (Fo79.8-81.8) and pyroxene (En73.9-75.2, Fs15.5-16.9, Wo8.8-9.5) compositions are typical of ureilites. Olivine rims are reduced with Fo increasing up to Fo96.1-96.8. Metal in these rims is completely altered to Fehydroxide during terrestrial weathering. We studied diamond and graphite using micro-Raman and in situ synchrotron X-ray diffraction. The main diamond Raman band (LO=TO mode at ~1332 c…

in-situ XRD010504 meteorology & atmospheric sciencesMaterial properties of diamondMineralogyDiamondUreiliteChemical vapor depositionengineering.material010502 geochemistry & geophysicsureilite01 natural sciencesDiamond typesymbols.namesakeGeophysicsMeteoritediamondSpace and Planetary Sciencesymbolsengineeringmicro-RamanGraphiteRaman spectroscopyGeology0105 earth and related environmental sciences[SDU.STU.MI]Sciences of the Universe [physics]/Earth Sciences/Mineralogy
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Origin of SiO2-rich components in ordinary chondrites

2006

Abstract Silica-rich objects are common minor components in ordinary chondrites (OC), occurring as fragments and as chondrules. Their typical paragenesis is orthopyroxene + SiO 2 (with bulk SiO 2 >65 wt%) and occasionally with additional olivine and/or spinel. Individual silica-rich components (SRC) have previously been studied in various types of OCs, although there is only one comprehensive study of these objects by Brigham et al. [Brigham, C.A., Murrell, M.T., Yabuki, H., Ouyang, Z., El Goresy, A., 1986. Silica-bearing chondrules and clasts in ordinary chondrites. Geochim. Cosmochim. Acta 50, 1655–1666]. Several different explanations of how SRCs formed have been published. The main ques…

TridymiteOlivineGeochemistry and PetrologyChondriteengineeringMineralogyChondrulePyroxeneengineering.materialFormation and evolution of the Solar SystemCristobaliteGeologyParent bodyGeochimica et Cosmochimica Acta
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