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dc.contributor.authorPaque, J. M.
dc.contributor.authorBurnett, D. S.
dc.contributor.authorBeckett, J. R.
dc.date.accessioned2021-02-12T21:41:42Z
dc.date.available2021-02-12T21:41:42Z
dc.date.issued2007-01-01
dc.identifier.citationPaque, J. M., Burnett, D. S., & Beckett, J. R. (2007). Zoning patterns of Fe and V in spinel from a type B Ca‐Al‐rich inclusion: Constraints on subsolidus thermal history. Meteoritics & Planetary Science, 42(6), 899-912.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2007.tb01140.x
dc.identifier.urihttp://hdl.handle.net/10150/656279
dc.description.abstractWe obtained two-dimensional concentration maps for the minor elements Fe and V in 21 spinel crystals in the Allende type B1 inclusion TS-34 with a 4-5 micrometer resolution. Locally high concentrations of Fe occur along at least one edge of the spinels and decrease toward the center of the grains. Enrichment in V can also occur along edges or at corners. In general, there is no overall correlation of the Fe and V distributions, but in local regions of two grains, the V and Fe distributions are correlated, strongly suggesting a local source for both elements. In these two grains, opaque assemblages are present that appear to locally control the V distributions. This, coupled with previous work, suggests that prior to alteration, TS-34 contained V-rich metal. Oxidation of this metal during alteration can account for the edge/corner V enrichments, but provide only minor FeO contributions, explaining the overall lack of correlation between Fe and V. Most of the FeO appears to have been externally introduced along spinel boundaries during alteration. These alteration phases served as sources for diffusion of FeO into spinel. FeO distributions in spinel lead to a mean attenuation length of ~8 micrometer and, using literature diffusion coefficients in isothermal and exponential cooling approximations for peak temperatures in the range 600-700 degrees C, this leads to a time scale for calciumaluminum- rich inclusion (CAI) alteration in the range of decades to centuries.
dc.language.isoen
dc.publisherThe Meteoritical Society
dc.relation.urlhttps://meteoritical.org/
dc.rightsCopyright © The Meteoritical Society
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjectalteration
dc.subjectElement mapping
dc.subjectspinels
dc.subjectCalcium-aluminum-rich inclusions (CAIs)
dc.titleZoning patterns of Fe and V in spinel from a type B Ca-Al-rich inclusion: Constraints on subsolidus thermal history
dc.typeArticle
dc.typetext
dc.identifier.journalMeteoritics & Planetary Science
dc.description.collectioninformationThe Meteoritics & Planetary Science archives are made available by the Meteoritical Society and the University of Arizona Libraries. Contact lbry-journals@email.arizona.edu for further information.
dc.eprint.versionFinal published version
dc.description.admin-noteMigrated from OJS platform February 2021
dc.source.volume42
dc.source.issue6
dc.source.beginpage899
dc.source.endpage912
refterms.dateFOA2021-02-12T21:41:42Z


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