Planned maintenance
A system upgrade is planned for 24/9-2024, at 12:00-14:00. During this time DiVA will be unavailable.
Change search
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf
Dubiofossils from a Mars‐analogue subsurface palaeoenvironment: The limits of biogenicity criteria
UK Centre for Astrobiology School of Physics and Astronomy University of Edinburgh Edinburgh UK;School of Geosciences Grant Institute University of Edinburgh Edinburgh UK.ORCID iD: 0000-0001-8589-2041
Swedish Museum of Natural History, Department of Paleobiology. Department of Paleobiology Swedish Museum of Natural History Stockholm Sweden.
Centre for Microscopy Characterisation and Analysis The University of Western Australia Perth WA Australia.
Centre for Microscopy Characterisation and Analysis The University of Western Australia Perth WA Australia.ORCID iD: 0000-0001-6873-7816
Show others and affiliations
2021 (English)In: Geobiology, ISSN 1472-4677, E-ISSN 1472-4669, Vol. 19, no 5, p. 473-488Article in journal (Refereed) Published
Abstract [en]

The search for a fossil record of Earth's deep biosphere, partly motivated by potential analogies with subsurface habitats on Mars, has uncovered numerous assemblages of inorganic microfilaments and tubules inside ancient pores and fractures. Although these enigmatic objects are morphologically similar to mineralized microorganisms (and some contain organic carbon), they also resemble some abiotic structures. Palaeobiologists have responded to this ambiguity by evaluating problematic filaments against checklists of “biogenicity criteria”. Here, we describe material that tests the limits of this approach. We sampled Jurassic calcite veins formed through subseafloor serpentinization, a water–rock reaction that can fuel the deep biosphere and is known to have occurred widely on Mars. At two localities ~4 km apart, veins contained curving, branched microfilaments composed of Mg-silicate and Fe-oxide minerals. Using a wide range of analytical techniques including synchrotron X-ray microtomography and scanning transmission electron microscopy, we show that these features meet many published criteria for biogenicity and are comparable to fossilized cryptoendolithic fungi or bacteria. However, we argue that abiotic processes driven by serpentinization could account for the same set of lifelike features, and report a chemical garden experiment that supports this view. These filaments are, therefore, most objectively described as dubiofossils, a designation we here defend from criticism and recommend over alternative approaches, but which nevertheless signifies an impasse. Similar impasses can be anticipated in the future exploration of subsurface palaeo-habitats on Earth and Mars. To avoid them, further studies are required in biomimetic geochemical self-organization, microbial taphonomy and micro-analytical techniques, with a focus on subsurface habitats.

Place, publisher, year, edition, pages
Wiley-Blackwell, 2021. Vol. 19, no 5, p. 473-488
Keywords [en]
General Earth and Planetary Sciences, General Environmental Science, Ecology, Evolution, Behavior and Systematics
National Category
Natural Sciences Other Earth and Related Environmental Sciences
Research subject
Diversity of life; The changing Earth
Identifiers
URN: urn:nbn:se:nrm:diva-4514DOI: 10.1111/gbi.12445OAI: oai:DiVA.org:nrm-4514DiVA, id: diva2:1618772
Funder
Paul Scherrer Institut, PSI, 20130185Swedish Research Council, 2017-04129Australian Research Council, FT140100321EU, Horizon 2020, 747877Paul Scherrer Institut, PSI, 20141047
Note

S. M. acknowledges funding by the European Union's Horizon 2020 Research and Innovation Program under Marie Skłodowska-Curie grant agreement 747877. MI acknowledges funding from Swedish Research Council (Contract 2017-04129) and funding from the Paul Scherrer Institute, Villigen, Switzerland (20130185, 20141047) granted to Stefan Bengtson. DW acknowledges funding from the Australian Research Council via a Future Fellowship (FT140100321). The authors acknowledge the facilities, and the scientific and technical assistance of Microscopy Australia at the Centre for Microscopy, Characterisation & Analysis, The University of Western Australia, a facility funded by the University, State and Commonwealth Governments. The chemical garden experiments were supported by the National Science Foundation under Grant No. 1609495 to O.S. Chemical garden SEM measurements were carried out at the Condensed Matter and Materials Physics User Facility of Florida State University. We thank Dr. Eric Lochner for sharing his technical expertise. We acknowledge the Paul Scherrer Institut, Villigen, Switzerland for provision of synchrotron radiation beamtime at the TOMCAT beamline X02DA of the Swiss Light Source and would like to thank Federica Marone for help at the beamline and SRXTM analyses. 

Available from: 2021-12-10 Created: 2021-12-10 Last updated: 2021-12-10Bibliographically approved

Open Access in DiVA

No full text in DiVA

Other links

Publisher's full texthttps://doi.org/10.1111/gbi.12445

Search in DiVA

By author/editor
McMahon, SeanIvarsson, MagnusSaunders, MartinBelivanova, Veneta
By organisation
Department of Paleobiology
In the same journal
Geobiology
Natural SciencesOther Earth and Related Environmental Sciences

Search outside of DiVA

GoogleGoogle Scholar

doi
urn-nbn

Altmetric score

doi
urn-nbn
Total: 38 hits
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf