Raman spectroscopic analysis of cyanobacterial gypsum halotrophs and relevance for sulfate deposits on Mars
Abstract
The
* Corresponding authors
a Chemical and Forensic Sciences, School of Pharmacy, University of Bradford, Bradford, UK
b Area Geodinamica Interna, Facultad de Humanidades y Educación, University of Burgos, Calle Villadiego s/n, 09001 Burgos, Spain
c Geofluids Research Group, Department of Geology and Petroleum Geology, University of Aberdeen, Meston Building, King's College, Aberdeen, UK
d Planetary and Space Sciences Research Institute, Open University, Milton Keynes, UK
e
Mars Institute, SETI Institute and NASA Ames Research Center, Moffett Field, CA 94035-1000, California, USA
E-mail:
h.g.m.edwards@bradford.ac.uk
Fax: 00-44-1274-235350
Tel: 00-44-1274-233787
The
H. G. M. Edwards, S. E. J. Villar, J. Parnell, C. S. Cockell and P. Lee, Analyst, 2005, 130, 917 DOI: 10.1039/B503533C
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