首页 | 本学科首页   官方微博 | 高级检索  
     检索      


XANES and Mg isotopic analyses of spinels in Ca‐Al‐rich inclusions: Evidence for formation under oxidizing conditions
Authors:J M Paque  S R Sutton  S B Simon  J R Beckett  D S Burnett  L Grossman  H Yurimoto  S Itoh  H C Connolly Jr
Institution:1. Division of Geological and Planetary Sciences, Caltech, , Pasadena, California, 91125 USA;2. Department of Geophysical Sciences, The University of Chicago, , Chicago, Illinois, 60637 USA;3. Enrico Fermi Institute, The University of Chicago, , Chicago, Illinois, 60637 USA;4. Department of Natural History Science, Hokkaido University, , Sapporo, Hokkaido, Japan;5. Department of Physical Sciences, Kingsborough Community College of the City University of New York, , Brooklyn, New York, 11235 USA;6. Department of Earth and Environmental Sciences, The Graduate Center of the City University of New York, , New York, New York, 10016 USA;7. Department of Earth and Planetary Sciences, American Museum of Natural History, , New York, New York, 10024 USA;8. Lunar and Planetary Laboratory, University of Arizona, , Tucson, Arizona, 85721 USA
Abstract:Ti valence measurements in MgAl2O4 spinel from calcium‐aluminum‐rich inclusions (CAIs) by X‐ray absorption near‐edge structure (XANES) spectroscopy show that many spinels have predominantly tetravalent Ti, regardless of host phases. The average spinel in Allende type B1 inclusion TS34 has 87% Ti+4. Most spinels in fluffy type A (FTA) inclusions also have high Ti valence. In contrast, the rims of some spinels in TS34 and spinel grain cores in two Vigarano type B inclusions have larger amounts of trivalent titanium. Spinels from TS34 have approximately equal amounts of divalent and trivalent vanadium. Based on experiments conducted on CAI‐like compositions over a range of redox conditions, both clinopyroxene and spinel should be Ti+3‐rich if they equilibrated with CAI liquids under near‐solar oxygen fugacities. In igneous inclusions, the seeming paradox of high‐valence spinels coexisting with low‐valence clinopyroxene can be explained either by transient oxidizing conditions accompanying low‐pressure evaporation or by equilibration of spinel with relict Ti+4‐rich phases (e.g., perovskite) prior to or during melting. Ion probe analyses of large spinel grains in TS34 show that they are enriched in heavy Mg, with an average Δ25Mg of 4.25 ± 0.028‰, consistent with formation of the spinel from an evaporating liquid. Δ25Mg shows small, but significant, variation, both within individual spinels and between spinel and adjacent melilite hosts. The Δ25Mg data are most simply explained by the low‐pressure evaporation model, but this model has difficulty explaining the high Ti+4 concentrations in spinel.
Keywords:
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号