Experiment title: Experiment Fe local structure in tektites and impactites by XANES number: and EXAFS 08-01-251
Beamline: Date of experiment: Date of report: BM-08 from: 8-11-2000 to: 10-11-2000 30-4-2001
Shifts: Local contact(s): Received at ESRF: 6 Pier Lorenzo Solari
Names and affiliations of applicants (* indicates experimentalists): Gabriele Giuli* Dip. Scienze della Terra and INFM, Universita’ di Camerino (I) Eleonora Paris * Dip. Scienze della Terra and INFM, Universita’ di Camerino (I) Giovanni Pratesi* Museo di Mineralogia e Litologia, , Universita’ di Firenze (I) Curzio Cipriani Museo di Mineralogia e Litologia, , Universita’ di Firenze (I)
Report: This project is focused on the structural study of glasses formed during the impact of asteroids on the earth surface, and in particular on the Fe coordination number and oxidation state. The interest on impact cratering, due to the its importance as a geological process and, partly, to the economic importance of several big impact craters (see Montanary and Koeberl, 2000 for a review), has stimulated a wealth of studies on impact glasses; however, relatively few were devoted to the structural study of these glasses (Korotayeva et al., 1985; Farges et al., 1997; Rossano et al., 1999; Giuli et al., 2000; Giuli et al., 2001). In this study the samples are studied by means of EXAFS and High resolution XANES. To get information on the Fe local environment and oxidation state we collected High-resolution XANES spectra of several Fe compounds with known Fe-coordination number and oxidation state (Fe2+ in 4-, 5-, 6-, and 8-fold coordination and Fe3+ in 6-fold coordination) to be compared with the studied 2 samples. For some of the standards we collected also EXAFS spectra in order to calibrate the S0 factor, which is needed to extract information on the coordination number from EXAFS. In the previous run (08-01-197) we collected EXAFS and High resolution XANES spectra of several tektites (a moldavite, an indochinite and an australite) and impact glasses (a suevite from the Ries crater, germany; an irzighite from the Zamanshin crater, Khazakstan; and an impact glass from the Wabar craters, Saudi Arabia). The data on tektites were analysed to get Fe-O distances and coordination number (
Refences cited:
Farges F., and Brown G.E. (1997). Geochimica et Cosmochimica Acta, 61 (9), 1863-1870. Giuli G., Pratesi G., Corazza M., and Cipriani C. (2000a). American Mineralogist,85,1172-1174. Giuli G., Pratesi G., Paris E., Cipriani C; (2001) submitted to Geochimica et Cosmochimica Acta Korotayeva N.N., Polosin A.V., and Malysheva T.V. (1985). Geokhimiya, 6, 899-903. Montanari A., & Koeberl C. (2000) Impact Stratigraphy, Lecture Notes in Earth Sciences. Springer, Berlin. Rossano S., Balan E., Morin G., Bauer J.P., Calas G., Bronder C. (1999). Physics and Chemistry of Minerals, 26, 530-538.