TY  - JOUR
AU  - Kovács, János
AU  - Sajó, István
AU  - Márton, Zsuzsanna
AU  - Jáger, Viktor
AU  - Hegedüs, Tibor
AU  - Berecz, Tibor
AU  - Tóth, Tamás Ferenc
AU  - Gyenizse, Péter
AU  - Podobni, András
TI  - Csátalja, the largest H4-5 chondrite from Hungary
JF  - PLANETARY AND SPACE SCIENCE
J2  - PLANET SPACE SCI
VL  - 105
PY  - 2015
SP  - 94
EP  - 100
PG  - 7
SN  - 0032-0633
DO  - 10.1016/j.pss.2014.11.009
UR  - https://m2.mtmt.hu/api/publication/2814679
ID  - 2814679
N1  - Department of Geology and Meteorology, University of Pécs, Ifjúság u. 6, Pécs, H-7624, Hungary            
            Environmental Analytical and Geoanalytical Research Group, Szentágothai Research Center, University of Pécs, Ifjúság u. 20, Pécs, H-7624, Hungary            
            MTA-PTE High-Field Terahertz Research Group, Ifjúság u. 6, Pécs, H-7624, Hungary            
            Institute of Physics, University of Pécs, Ifjúság u. 6, Pécs, H-7624, Hungary            
            Baja Astronomical Observatory, POB 766, Baja, H-6500, Hungary            
            Department of Materials Science and Engineering, Budapest University of Technology and Economics, Bertalan L. u. 7, Budapest, H-1111, Hungary            
            Department of Cartography and Geoinformatics, University of Pécs, Ifjúság u. 6, Pécs, H-7624, Hungary            
            Cited By :7            
            Export Date: 29 September 2023            
            CODEN: PLSSA            
            Correspondence Address: Kovács, J.; Department of Geology and Meteorology, University of Pécs, Ifjúság u. 6, Hungary
AB  - We report here for the first time the composition and 
mineralogical studies on a new meteorite, which was found in 
August 2012 near the village of Csátalja, Hungary (46°0'21-N; 
18°59'27'E). The Csátalja meteorite is classified as a H4-5 
ordinary chondrite with shock stage S2 and a degree of 
weathering W1 and the total mass is 15 kg. The Csátalja 
meteorite is characterized by well-defined chondrules composed 
either of olivine or pyroxene. X-ray diffractogram shows the 
primary phases olivine, pyroxene, kamacite, and albite. Metal 
particles were extracted from the bulk powdered samples exhibit 
only kamacite and small amounts of the intergrowth 
taenite/kamacite. Raman spectra of forsterite indicate that 
Csátalja meteorite suffered from relatively low shock pressure 
regime. The texture of chondrules varies from nonporphyritic 
(e.g., barred olivine, radial pyroxene) to porphyritic ones 
(e.g., granular olivine as well as olivine pyroxene). The 
meteorite name has not yet approved by the Nomenclature 
Committee of the Meteoritical Society.
LA  - English
DB  - MTMT
ER  -