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dc.date.accessioned 2021-10-21T14:13:21Z
dc.date.available 2021-10-21T14:13:21Z
dc.date.issued 2009
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/127036
dc.description.abstract The crystal structure of druse clinopyroxene from the D'Orbigny angrite, (Ca0.944 Fe 2+ 0.042 Mg0.010Mn0.004) (Mg0.469Fe 2+ 0.317Fe 3+ 0.035Al0.125Cr0.010Ti0.044) (Si1.742Al0.258) O6, a = 9.7684(2), b = 8.9124(2), c = 5.2859(1) A, β = 105.903(1)°, V = 442.58 A 3 , space group C2/c, Z = 2, has been refined to an R1 index of 1.92% using single-crystal X-ray diffraction data. The unit formula, calculated from electron microprobe analysis, and the refined site scattering values were used to assign site populations. The distribution of Fe 2+ and Mg over the M1 and M2 sites suggests a closure temperature of 1000 °C. Mossbauer spectroscopy measurements were done at room temperature on a single crystal and a powdered sample. The spectra are adequately fit by a Voigt-based quadrupole-splitting distribution model having two generalized sites, one for Fe 2+ with two Gaussian components and one for Fe 3+ with one Gaussian component. The two ferrous components are assigned to Fe 2+ at the M1 site, and arise from two different next-nearest-neighbor configurations of Ca and Fe cations at the M2 site: (3Ca,0Fe) and (2Ca,1Fe). The Fe 3+ /Fetot ratio determined by Mossbauer spectroscopy is in agreement with that calculated from the electron microprobe analysis. The results are discussed in connection with the redox and thermal history of D'Orbigny. en
dc.format.extent 581-587 es
dc.language en es
dc.subject Crystal structure es
dc.subject Electron microprobe es
dc.subject Chemistry es
dc.subject Diffraction es
dc.subject Druse (geology) es
dc.subject Spectral line es
dc.subject X-ray crystallography es
dc.subject Mössbauer spectroscopy es
dc.subject Single crystal es
dc.subject Crystallography es
dc.title Druse clinopyroxene in D'Orbigny angritic meteorite studied by single-crystal X-ray diffraction, electron microprobe analysis and Mössbauer spectroscopy en
dc.type Articulo es
sedici.identifier.other doi:10.1111/j.1945-5100.2009.tb00753.x es
sedici.identifier.issn 1086-9379 es
sedici.identifier.issn 1945-5100 es
sedici.creator.person Abdu, Yassir A. es
sedici.creator.person Scorzelli, R. B. es
sedici.creator.person Varela, Maria Eugenia es
sedici.creator.person Kurat, Gero es
sedici.creator.person Souza Azevedo, Izabel de es
sedici.creator.person Stewart, Silvana Jacqueline es
sedici.creator.person Hawthorne, Frank C. es
sedici.subject.materias Geofísica es
sedici.description.fulltext true es
mods.originInfo.place Instituto de Física La Plata es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution 4.0 International (CC BY 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Meteoritics & Planetary Science es
sedici.relation.journalVolumeAndIssue vol. 44, no. 4 es


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Creative Commons Attribution 4.0 International (CC BY 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution 4.0 International (CC BY 4.0)