| BOROVIĈKA, J., WEBER, H. W., JOPEK, T., JAKEŜ, P., RANDA, Z., BROWN, P. G., REVELLE, D. O., KALENDA, P., SCHULTZ, L., KUCERA, J., HALODA, J., TÝCOVÁ, P., FRÝDA, J., BRANDSTÄTTER, F. (2003) The Morávka meteorite fall: 3. Meteoroid initial size, history, structure, and composition. Meteoritics & Planetary Science, 38 (7) 1005-1021 doi:10.1111/j.1945-5100.2003.tb00295.x | Journal (article/letter/editorial) | available online at http://meteoritics.org The Morávka meteorite fall: 3. Meteoroid initial size, history,...the Academy of Sciences, 25165 Ondrejov, The Czech Republic für Chemie, Joh. J.-Becher-Weg 27, D–55128...University, Albertov 6, 12843 Prague 2, The Czech Republic 5Nuclear Physics Institute, Academy of Sciences...Sciences, 25068 Rez near Prague, The Czech Republic 6Department of Physics and Astronomy, University of... The Czech Republic 9Czech Geological Survey, Geologická 6, 15200 Prague 5, The Czech Republic 10Department | | | Journal (article/letter/editorial) | been reported in this region. As part of an ongoing project to discover meteorite impact sites, this area...Fe-Ni-metal (33.3–44.6 wt% Ni and 0.15–0.34 Co in taenite and 3.82–5.3 wt% Ni and 0.74–1.15 Co in kamacite...Single spinel grains and copper inclusions in taenite grain were found in the largest HP aggregate from...tend to have the same REE pattern within a given meteorite. REEs are homogeneous in a given grain but vary...fitting was constrained to the 1301 to 233 cm−1 region. Compositions were calculated on a water and CO2-free |
|