Identifying elements in rocks from the Dry Valleys desert (Antarctica) by ion beam proton induced X-ray emission

https://doi.org/10.1016/j.nimb.2006.03.057Get rights and content

Abstract

In some zones of Antarctica’s cold and dry desert, the extinction of cryptoendolithic microorganisms leaves behind inorganic traces of microbial life. The extinction of these microorganisms is considered to be the best terrestrial analogue of the disappearance of possible life on early Mars. In the present study, sandstone rock samples from several sites of the Dry Valleys known to harbour endolithic microorganisms, as well as samples with microbial fossils, were analysed by proton induced X-ray emission (PIXE). Our findings suggest significant differences in major element concentrations among the different zones within the same sample. In some sample fractions, these differences could be considered as traces of the microbial origin. However, other samples reveal contamination produced by allochthonous minerals of abiogenetic origin.

Introduction

The endolithic microbial ecosystems of the Dry Valleys of Antarctica are a good terrestrial model of the last stages of life on early Mars [1]. In this cold desert, microbial life is mostly confined to a narrow layer beneath the rock surface [2]. In several zones of Dry Valleys microbial life expires. The extinction of microorganisms could leave behind indirect signs. The first life trace observed was a whitish iron-leaching layer attributed to the mobilization of iron hydroxides due to activity of cryptoendolithic lichens [3], [4]. Later, it was demonstrated that some minerals in Antarctic rocks are biogenetically transformed to generate inorganic biomarkers [5]. Recently through in situ scanning electron microscopy in backscattered electrons detection mode (SEM-BSE), microbial fossils left behind by endolithic microorganisms in Antarctica were demonstrated for the first time [6]. However, research into detecting inorganic traces of life, past and present, in these rocks requires much further work using unconventional microanalytical techniques. Indeed, according to [7], chemical analysis might be an essential tactic for exploring fossil evidence also on Mars. All robotic missions to Mars have been equipped with microanalytical devices based on detection of X-rays in order to determine chemical composition of the minerals.

The aim of our study was to give response on the question: could the present and/or past microbial life in Antarctic sandstones left chemical traces detectable with microanalytical systems? In the present study, rock samples from several sites of the Dry Valleys known to harbour endolithic microorganisms, as well as samples in which life was not present, were analysed by proton induced X-ray emission (PIXE) in order to detail characterization of rock fragments. For this purpose we have performed a macro PIXE measurement for the determination of the elemental composition in different fractions of the rocks from Dry Valley.

Section snippets

Materials and analytical methods

For the aim of this study eight samples of sandstone rocks were collected from different regions of the Dry Valleys desert, Antarctica (76.5–78.5°S, 160–164°E). Climatological conditions of the sampling area, as well as mineralogical composition of these sandstones are given in [6], [11]. All these samples have been previously examined in order to search for live microorganisms, as well as for biomarkers and microbial fossil presence (references in Table 1). A detailed description of the

Results and discussion

Several major and trace elements were detected in the pellets. However, for the purpose of this study we have reported data only for Si, S, Cl, K, Ca, Ti, Mn and Fe elements. We have considered these elements as the most indicative of the expected traces of cryptoendolithic microorganisms activity and/or past life within studied fraction of rocks. These elements were also considered relevant to characterize the rock fractions in order to simplify the discussion, due to the high amount of data.

Conclusions

Our findings suggest significant differences in major element concentrations among the different zones within the same sample. In some of the samples, these differences could be carefully attributed to a microbial origin. However, variation in concentration of these elements in other sample fractions should be interpreted as a contamination by airborne dust and/or by allochthonous minerals and salts infiltration during some unknown geochemical event occurred after the decay of microbes. These

Acknowledgements

This study was funded by grants REN2003-07366-C02-02 and BOS2003-02418 of the Plan Nacional I + D. Thanks are due to I. Ranz for her technical assistance.

References (13)

  • J. García López et al.

    Nucl. Instr. and Meth. B

    (2000)
  • J.A. Maxwell et al.

    Nucl. Instr. and Meth. B

    (1989)
  • J.E. Martín et al.

    Nucl. Instr. and Meth. B

    (2000)
  • C.P. McKay

    Antarctic Microbiology

    (1993)
  • J. Wierzchos et al.

    Polar Biol.

    (2001)
  • E.I. Friedmann

    Science

    (1982)
There are more references available in the full text version of this article.
View full text