Earth as a Tool for Astrobiology: A European Perspective

Z. Martins, H. Cottin, J.M. Kotler, N. Carrasco, C.S. Cockell, R. de la Torre Noetzel, R. Demets, J.P. de Vera, L. d'Hendecourt, P. Ehrenfreund, A. Elsaesser, B. Foing, S. Onofri, R. Quinn, E. Rabbow, P. Rettberg, A.J. Ricco, K. Slenzka, F. Stalport, I.L. ten KateJ.J.W.A. van Loon, Frances Westall

Research output: Contribution to JournalArticleAcademicpeer-review

Abstract

Scientists use the Earth as a tool for astrobiology by analyzing planetary field analogues (i.e. terrestrial samples and field sites that resemble planetary bodies in our Solar System). In addition, they expose the selected planetary field analogues in simulation chambers to conditions that mimic the ones of planets, moons and Low Earth Orbit (LEO) space conditions, as well as the chemistry occurring in interstellar and cometary ices. This paper reviews the ways the Earth is used by astrobiologists: (i) by conducting planetary field analogue studies to investigate extant life from extreme environments, its metabolisms, adaptation strategies and modern biosignatures; (ii) by conducting planetary field analogue studies to investigate extinct life from the oldest rocks on our planet and its biosignatures; (iii) by exposing terrestrial samples to simulated space or planetary environments and producing a sample analogue to investigate changes in minerals, biosignatures and microorganisms. The European Space Agency (ESA) created a topical team in 2011 to investigate recent activities using the Earth as a tool for astrobiology and to formulate recommendations and scientific needs to improve ground-based astrobiological research. Space is an important tool for astrobiology (see Horneck et al. in Astrobiology, 16:201–243, 2016; Cottin et al., 2017), but access to space is limited. Complementing research on Earth provides fast access, more replications and higher sample throughput. The major conclusions of the topical team and suggestions for the future include more scientifically qualified calls for field campaigns with planetary analogy, and a centralized point of contact at ESA or the EU for the organization of a survey of such expeditions. An improvement of the coordinated logistics, infrastructures and funding system supporting the combination of field work with planetary simulation investigations, as well as an optimization of the scientific return and data processing, data storage and data distribution is also needed. Finally, a coordinated EU or ESA education and outreach program would improve the participation of the public in the astrobiological activities.
Original languageEnglish
Pages (from-to)43-81
Number of pages39
JournalSpace Science Reviews
Volume209
Issue number1-4
Early online date20 Jun 2017
DOIs
Publication statusPublished - Jul 2017

Funding

In 2003 the ESF initiated a new research support activity called Investigating Life in Extreme Environments (ILEE). This initiative showed the need for a coordinated, interdisciplinary approach to improve future opportunities for funding research on “Life in extreme environments” (LEXEN). The coordination action for research on study of life in extreme environments (CAREX) was a Seventh Framework Programme (FP7) project funded by the European Commission (EC) and coordinated by the British Antarctic Survey and the Natural Environment Research Council (NERC). The project operated from 1 January 2008 to 30 June 2011 and addressed the enhanced coordination of LEXEN research in Europe by providing networking and exchange of knowledge opportunities to the scientific community. It was an interdisciplinary initiative covering all life forms existing in extreme environments on Earth, as well as addressing the use of extreme environments as planetary field analogues in the search for extra-terrestrial life. The four priority areas identified in the CAREX strategic roadmap included: (1) contributions of life in extreme environments (LEXEN) to biogeochemical cycles and responses to environmental change, (2) stressful environments—responses, adaptation and evolution, (3) biodiversity, bioenergetics and interactions in extreme environments, and (4) life and habitability (final CAREX report summary available at http://cordis.europa.eu/result/rcn/55055_en.html ). The resulting strategic roadmap for European research on LEXEN is a basis for strategic programme planning for science organizations such as the EC, COSPAR, and other institutions outside Europe such as the National Aeronautics and Space Administration (NASA) Astrobiology Institute and the Japan Agency for Marine-Earth Science and Technology (JAMSTEC). One example of a European follow-on research project funded by the EC in the Framework Program 7 is the Mars Analogues for Space Exploration (MASE, 2014–2017, http://mase.esf.org/ ). It has the aim (i) to isolate and characterise anaerobic microorganisms from selected sites that closely match environmental conditions that might have been habitable on early Mars, (ii) to study their responses to realistic combined environmental stresses that might have been experienced in habitable environments on Mars, and (iii) to investigate their potential for fossilization on Mars and their detectability by carrying out a systematic study of the detectability of artificially fossilized organisms exposed to known stresses. This work has been supported by ESA, through a Topical Team grant from 2011 to 2016. We are grateful to Oliver Angerer, Jason Hatton and René Demets from ESA for their help and support. UPEC and LISA provided important administrative help (Mireille Paul, Sabrina Hammache, Valérie Simard, Nicolas Vautrin). Zita Martins is funded by a Royal Society University Research Fellowship (grant UF080820 and grant UF130324). Nathalie Carrasco acknowledges the financial support of the European Research Council (ERC Starting Grant PRIMCHEM, grant agreement no. 636829). Pascale Ehrenfreund acknowledges support from the NASA Astrobiology Institute. Louis d’Hendecourt acknowledges support from the French Space Agency (CNES) Exobiology Group. Silvano Onofri acknowledges the Italian Space Agency (ASI) for financial support. Inge Loes ten Kate acknowledges the Netherlands Space Office (NSO), the Netherlands Organization for Scientific Research (NWO) and Raheleh Motamedi for fruitful discussions. Jean-Pierre de Vera acknowledges the Helmholtz-Gemeinschaft for financial support through the Helmholtz-Alliance Planetary Evolution and Life. Frances Westall acknowledge support from the French Space Agency (CNES), the Agence Nationale de la Recherche (ANR), the Centre national de la recherche scientifique (CNRS-MI-2014), the MASE project (supported by European Community’s Seventh Framework Programme (FP7/2007-2013) under Grant Agreement no. 607297), and the H2020 EUROCARES programme.

FundersFunder number
Horizon 2020 Framework Programme607297, 636829
Seventh Framework Programme
Natural Environment Research Council
European Commission
European Space Agency
Seventh Framework Programme

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