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Evidence for biological activity in mineralization of secondary sulphate deposits in a basaltic environment: implications for the search for life in the Martian subsurface

Published online by Cambridge University Press:  24 July 2013

C. Doc Richardson
Affiliation:
Geosciences Department, University of Montana, Missoula, 32 Campus Drive #1296, Missoula, MT 59812, USA
Nancy W. Hinman
Affiliation:
Geosciences Department, University of Montana, Missoula, 32 Campus Drive #1296, Missoula, MT 59812, USA
Jill R. Scott
Affiliation:
Chemical and Radiation Measurement, Idaho National Laboratory, 1765 North Yellowstone Hwy, Idaho Falls, ID 83415-2208, USA e-mail: Jill.Scott@inl.gov
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Abstract

Evidence of microbial activity associated with mineralization of secondary Na-sulphate minerals (thenardite, mirabilite) in the basaltic subsurface of Craters of the Moon National Monument (COM), Idaho were examined by scanning electron microscopy, X-ray diffraction, laser desorption Fourier transform ion cyclotron resonance mass spectrometry (LD-FTICR-MS), Fourier transform infrared spectroscopy (FTIR) and isotope ratio mass spectrometry. Peaks suggestive of bio/organic compounds were observed in the secondary Na-sulphate deposits by LD-FTICR-MS. FTIR provided additional evidence for the presence of bio/organic compounds. Sulphur fractionation was explored to assist in determining if microbes may play a role in oxidizing sulphur. The presence of bio/organic compounds associated with Na-sulphate deposits, along with the necessity of oxidizing reduced sulphur to sulphate, suggests that biological activity may be involved in the formation of these secondary minerals. The secondary Na-sulphate minerals probably form from the overlying basalt through leached sodium ions and sulphate ions produced by bio-oxidation of Fe-sulphide minerals. Since the COM basalts are one of the most comparable terrestrial analogues for their Martian counterparts, the occurrence of biological activity in the formation of sulphate minerals at COM has direct implications for the search for life on Mars. In addition, the presence of caves on Mars suggests the importance of these environments as possible locations for growth and preservation of microbial activity. Therefore, understanding the physiochemical pathways of abiotic and biotic mineralization in the COM subsurface and similar basaltic settings has direct implications for the search for extinct or extant life on Mars.

Information

Type
Research Article
Copyright
Copyright © Cambridge University Press 2013 
Figure 0

Fig. 1. (a) Map of COM lava field showing cave locations in Blue Dragon flow. Map modified from Kuntz (1989) with permission of American Geophysical Union. (b) Photograph of the COM surface terrain.

Figure 1

Fig. 2. Photograph of thenardite deposit in a wall cavity inside Arco Tunnel.

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Fig. 3. (a) SEM image of efflorescent secondary mineral deposit. (b) EDX spectrum showing elements associated with deposit. (c) Background corrected XRD pattern of secondary mineral demonstrating that it is primarily thenardite.

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Table 1. Sulphur isotopic values of secondary deposits and host basalts

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Table 2. Literature compilation of biotic and abiotic sulphur fractionation for oxidation of sulphidic minerals

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Fig. 4. (a) LD-FTICR-MS chemical pseudo-image showing heterogeneity of chemical composition within the sample. Colored circles indicate areas with potential organic compounds: green for m/z 183, orange for m/z 339 and black for a mix of m/z 183 and 339. Blank circles are locations with peaks indicative of inorganic only compounds. (b) Negative mode laser desorption ion FTICR-MS spectrum of secondary sulphate deposits. Peaks at (c) m/z 183 and (d) m/z 339 have mass defects and isotopic distributions suggestive of bio/organic cluster ions.

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Table 3. Suggestive chemical formulae for bio/organic peaks associated with the secondary sulphate deposits observed in the LD-FTICR-MS spectra

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Fig. 5. Positive mode LD-FTICR-MS spectrum of a secondary sulphate deposit from a floor deposit within a cave in the Wilderness Caves area.

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Fig. 6. Representative FTIR spectra of secondary deposits. (a) FTIR spectrum dominated by sulphate oxyanion, whereas FTIR spectrum (b) shows additional bands corresponding to carbonate oxyanion. Both spectra show bands suggestive of organic compounds (indicated by *).

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Fig. 7. Schematic illustrating biotic and abiotic weathering of the overlying basalts at COM and subsequent mineralization of secondary Na-sulphate minerals on the cave floors.