Raman spectroscopic study of mellite - A naturally occurring aluminium benzenehexacarboxylate from lignite - Claystone series of the tertiary age

被引:22
作者
Jehlicka, J. [1 ]
Edwards, H. G. M.
Villar, S. E. Jorge
机构
[1] Charles Univ Prague, Inst Geochem Mineral & Mineral Resources, Prague, Czech Republic
[2] Univ Bradford, Bradford BD7 1DP, W Yorkshire, England
[3] Univ Burgos, Fac Human & Educ, Area Geodinam Interna, Burgos 09001, Spain
关键词
mellite; aluminium benzenehexacarboxylate; Raman spectroscopy; lignite; sedimentary rocks; CRYSTAL-STRUCTURE; ACID; OXALATES; PEATS; RATES;
D O I
10.1016/j.saa.2005.10.036
中图分类号
O433 [光谱学];
学科分类号
0703 ; 070302 ;
摘要
Raman spectra have been obtained for crystals of the organic mineral mellite, from three different sites. Mellite occurs in the frame of the Tertiary series including lignite and coaly slates at Artern (Thuringia), Tula (Russia) and Bilina (Northern Bohemia). Mellite, Al2C6(COO)(6)center dot 16H(2)O, can be considered as evidence of previous biological activity in the geological record, similar to other salts of carboxylic acids such as whewellite and weddellite. Assignments of the major Raman features of mellite are proposed on the basis of comparison with the parent, mellitic acid, C-6(COOH)(6) During diagenesis and epigenesis, mellite is formed from the reaction between organic carbon rich solutions with aluminosilicates, hence, with the current interest in the adoption of Raman spectroscopy for incorporation into robotic instrumentation for space mission landers, it is important that organic minerals be included into a spectroscopic database for the recognition of biomolecular signatures for remote life-detection experiments. (c) 2005 Elsevier B.V. All rights reserved.
引用
收藏
页码:229 / 234
页数:6
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