Preston, L. J.; Shuster, J.; Fernandez-Remolar, D.; Banerjee, N. R.; Osinski, G. R. and Southam, G.
biomolecules within iron oxide deposits at Rio Tinto, Spain.
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|DOI (Digital Object Identifier) Link:||http://dx.doi.org/doi:10.1111/j.1472-4669.2011.00275.x|
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One of the keys to understanding and identifying life on other planets is to study the preservation of organic compounds and their precursor micro-organisms on Earth. Rio Tinto in southwestern Spain is a well documented site of microbial preservation within iron sulphates and iron oxides over a period of 2.1 Ma. This study has investigated the preservation of filamentous iron oxidising bacteria and organics through optical microscopy, scanning electron microscopy (SEM) and Fourier transform infra-red (FTIR) spectroscopy, from laboratory cultures of natural samples to contemporary natural materials to million-year old river terraces. Up to 40% elemental carbon and >7% nitrogen has been identified within microbial filaments and cell clusters in all samples through SEM EDS analyses. FTIR spectroscopy identified C–Hx absorption bands between 2960 and 2800 cm−1, Amide I and II absorption bands at 1656 and 1535 cm−1, respectively and functional group vibrations from within nucleic acids at 917, 1016 and 1124 cm−1. Absorption bands tracing the diagenetic transformation of jarosite to goethite to hematite through the samples are also identified. This combination of mineralogy, microbial morphology and biomolecular evidence allows us to further understand how organic fossils are created and preserved in iron-rich environments, and ultimately will aid in the search for the earliest life on Earth and potential organics on Mars.
|Item Type:||Journal Article|
|Copyright Holders:||2011 Blackwell Publishing Ltd|
|Funders:||Interdisciplinary Development Initiative award to the Centre for Planetary Science and Exploration (CPSX) at the University of Western Ontario.|
|Academic Unit/Department:||Science > Physical Sciences|
|Depositing User:||Louisa Preston|
|Date Deposited:||17 Jan 2012 12:56|
|Last Modified:||24 Oct 2012 04:40|
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