42nd Lunar and Planetary Science Conference (2011) 1157.pdf CATHODOLUMINESCENCE CHARACTERIZATION OF THE FORSTERITE IN KABA METEORITE: AN ASTROMINERALOGICAL APPLICATION. A. Gucsik1,2, T. Endo3, E. Nakazato3 H. Nishido3, K. Ninagawa4, M. Kayama3, Sz. Bérczi5, Sz. Nagy6, P. Ábrahám2, Y. Kimura7, I. Gyollai8, I. Simonia9, P. Rózsa10, J. Posta10, M. Nagy10, K. Mihályi10, D. Apai11 & P. Futó12 1Abteilung Geochemie, Max-Planck-Institut für Chemie, Joh-J.-Becherweg 27, Universitätcampus, Mainz, D-55128, Germany (E-mail:
[email protected]); 2Konkoly Observatory of the Hungarian Academy of Sciences, H-1121 Budapest, Konkoly Thege Miklós út 15-17., Hungary; 3Research Institute of Natural Sciences, Okayama University of Science, 1-1 Ridai-cho, Okayama, 700-0005, Japan; 4Department of Applied Physics, Okayama University of Science, 1-1 Ridai-cho, Okayama, 700-0005, Japan; 5Institute of Physics, Department of Material Physics, Eötvös University, Pázmány P. s. 1/a, Budapest, H-1117, Hungary; 6Eötvös University, Dept. Petrology and Geochemistry, H-1117 Budapest, Pázmány Péter sétány 1/c, Hungary; 7Department of Earth and Planetary Materials Science, Graduate School of Science, Tohoku University, Sendai 980-8578, Japan; 8Department of Lithospheric Research Center for Earth Sciences, University of Vienna, Althanstrasse 14, A-1090 Vienna, Austria; 9School of Graduate Studies of Ilia Sate University, Tbilisi, Georgia; 10University of Debrecen, Egyetem tér 1., Debrecen, H-4032, Hungary; 11Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA; 12Enese, Radnóti utca 7, H-9143, Hungary. in %: matrix (55.2), chondrule (27.7), CAI (3.4), Introduction: Kaba carbonaceous chondrite is the aggregated olivine (2.5), and isolated coarse grained most primitive unshocked CV fall (in 1857) collected olivine (0.8).