Truncated Hexa-Octahedral Magnetite Crystals in ALH84001: Presumptive Biosignatures

McKay et al. [(1996) Science 273, 924-930] suggested that carbonate globules in the meteorite ALH84001 contained the fossil remains of Martian microbes. We have characterized a subpopulation of magnetite (Fe3O4) crystals present in abundance within the Fe-rich rims of these carbonate globules. We fi...

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Veröffentlicht in:Proceedings of the National Academy of Sciences - PNAS 2001-02, Vol.98 (5), p.2164-2169
Hauptverfasser: Thomas-Keprta, Kathie L., Clemett, Simon J., Bazylinski, Dennis A., Kirschvink, Joseph L., McKay, David S., Wentworth, Susan J., Vali, Hojatollah, Gibson, Everett K., McKay, Mary Fae, Romanek, Christopher S.
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Sprache:eng
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Zusammenfassung:McKay et al. [(1996) Science 273, 924-930] suggested that carbonate globules in the meteorite ALH84001 contained the fossil remains of Martian microbes. We have characterized a subpopulation of magnetite (Fe3O4) crystals present in abundance within the Fe-rich rims of these carbonate globules. We find these Martian magnetites to be both chemically and physically identical to terrestrial, biogenically precipitated, intracellular magnetites produced by magnetotactic bacteria strain MV-1. Specifically, both magnetite populations are single-domain and chemically pure, and exhibit a unique crystal habit we describe as truncated hexa-octahedral. There are no known reports of inorganic processes to explain the observation of truncated hexa-octahedral magnetites in a terrestrial sample. In bacteria strain MV-1 their presence is therefore likely a product of Natural Selection. Unless there is an unknown and unexplained inorganic process on Mars that is conspicuously absent on the Earth and forms truncated hexa-octahedral magnetites, we suggest that these magnetite crystals in the Martian meteorite ALH84001 were likely produced by a biogenic process. As such, these crystals are interpreted as Martian magnetofossils and constitute evidence of the oldest life yet found.
ISSN:0027-8424
1091-6490
DOI:10.1073/pnas.051500898