Abstract
The investigation of different samples of SNC (Shergotty-Nakhla-Chassigny) meteorites was chosen to test the ability of micro-Raman spectroscopy to cope with extraterrestrial material. The following SNC meteorites were investigated: Sayh al Uhaymir 060, Dar al Gani 735, Dar al Gani 476, Northwest Africa 856, Los Angeles, Northwest Africa 1068 and Zagami. Pyrite as a hitherto undescribed phase in the picritic (olivine-phyric) shergottite NWA 1068 and reduced carbon (e.g. graphite) and anatase in the shergottite Say al Uhaymir 060 are new findings for this class of meteorites.
Dokumententyp: | Zeitschriftenartikel |
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Fakultät: | Geowissenschaften > Department für Geo- und Umweltwissenschaften > Kristallographie und Materialwissenschaft |
Themengebiete: | 500 Naturwissenschaften und Mathematik > 550 Geowissenschaften, Geologie |
Sprache: | Englisch |
Dokumenten ID: | 18526 |
Datum der Veröffentlichung auf Open Access LMU: | 10. Mrz. 2014, 14:09 |
Letzte Änderungen: | 04. Nov. 2020, 13:00 |