Comparative Raman microscopy of a Martian meteorite and Antarctic lithic analogues

被引:51
作者
Edwards, HGM [1 ]
Farwell, DW
Grady, MM
Wynn-Williams, DD
Wright, IP
机构
[1] Univ Bradford, Bradford BD7 1DP, W Yorkshire, England
[2] Nat Hist Museum, Meteorite Sect, London SWY 5BD, England
[3] British Antarctic Survey, Cambridge CB32 0ET, England
[4] Open Univ, Planetary Sci Res Inst, Milton Keynes MK7 6AA, Bucks, England
关键词
D O I
10.1016/S0032-0633(98)00127-5
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 mu m, but several important mineralogical features have been identified, including clinopyroxene, olivine and plagioclase. In some sampling regions, rs-quartz particles are evident and in one sample region the nu(CO32-) mode of calcite at 1086 cm(-1) is found. There is no evidence lbr organic chemical content detectable In this meteorite specimen, based on an absence of nu(CH) and delta(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. (C) 1999 Elsevier Science Ltd. All rights reserved.
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页码:353 / 362
页数:10
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