Comparative Raman microscopy of a Martian meteorite and Antarctic lithic analogues

Edwards, H. G. M.; Farwell, D. W.; Grady, M. M.; Wynn-Williams, D. D.; Wright, I. P.. 1999 Comparative Raman microscopy of a Martian meteorite and Antarctic lithic analogues. Planetary and Space Science, 47 (3-4). 353-362. https://doi.org/10.1016/S0032-0633(98)00127-5

Full text not available from this repository. (Request a copy)

Abstract/Summary

The Raman microspectra of the Nakhla SNC meteorite, which probably originates from Mars, are reported here for the first time. The specimen is shown to be heterogeneous, even at a sampling level of 2 μm, but several important mineralogical features have been identified, including clinopyroxene, olivine and plagioclase. In some sampling regions, α-quartz particles are evident and in one sample region the ν(CO2−3) mode of calcite at 1086 cm−1 is found. There is no evidence for organic chemical content detectable in this meteorite specimen, based on an absence of ν(CH) and δ(CH2) modes near 3000 and 1400 cm−1, respectively. Comparative Raman spectroscopic analyses were made on epilithic examples of Xanthoria elegans from Crater Cirque, northern Victoria Land, Antarctica, and cryptoendoliths from East Beacon, McMurdo Dry Valleys, as positive controls for microbial organics in cold, arid habitats analogous to former Martian conditions. Finally, an assessment is made of the potential role of Raman spectroscopy for extra-terrestrial characterisation of geological specimens.

Item Type:	Publication - Article
Digital Object Identifier (DOI):	https://doi.org/10.1016/S0032-0633(98)00127-5
Programmes:	BAS Programmes > Pre 2000 programme
ISSN:	00320633
Additional Keywords:	meteorites, Mars, martian, Nakhla, microscopy, composition
Date made live:	14 Oct 2013 10:25 +0 (UTC)
URI:	https://nora.nerc.ac.uk/id/eprint/503171

Actions (login required)

View Item

Document Downloads

More statistics for this item...