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.
| Item Type: | Journal article |
|---|---|
| Faculties: | Geosciences > Department of Earth and Environmental Sciences > Crystallography and Materials Science |
| Subjects: | 500 Science > 550 Earth sciences and geology |
| Language: | English |
| Item ID: | 18526 |
| Date Deposited: | 10. Mar 2014 14:09 |
| Last Modified: | 04. Nov 2020 13:00 |
