A micro-Raman and X-ray study of erupted submarine pyroclasts from El Hierro (Spain) and its' astrobiological implications.


Journal

Life sciences in space research
ISSN: 2214-5532
Titre abrégé: Life Sci Space Res (Amst)
Pays: Netherlands
ID NLM: 101632373

Informations de publication

Date de publication:
May 2019
Historique:
received: 23 11 2018
revised: 12 04 2019
accepted: 14 04 2019
entrez: 19 5 2019
pubmed: 19 5 2019
medline: 12 9 2019
Statut: ppublish

Résumé

The pumice volcanic samples could have possible connections to the evolution of life and give us insight about their bio-geochemical processes related. In this regard, the samples from the volcanic eruption from La Restinga (El Hierro, Spain) in 2011 have been mainly studied by means of Raman spectroscopy. The research also includes analysis of XRD, Scanning Electron Microscopy and Optical Microscopy to support the Raman analysis. The results show that the Raman methods and mineral analyses are in strong agreement with the results obtained from other authors and techniques. The internal white foamy core (WFC) of the studied pumice samples shows amorphous silica, Fe-oxides, Ti-oxides, quartz, certain sulfates, carbonates, zeolites and organics. On the other hand, the external part (dark crust - DC) of these samples mainly presents primary-sequence mineralogy combined with some secondary alteration minerals such as olivine, feldspar, pyroxene, amorphous silica, and Fe-oxide. Raman spectroscopy detected other minerals not yet reported on these samples like barite, celestine and lepidocrocite. Also, the different chemometric and calibration methods for Raman spectroscopy in elemental composition, mineral classification and structural characterization has been successfully applied. From the astrobiological perspective, the research was also complemented with comparisons to other similar samples from terrestrial analogs. The main consideration was taking into account the proposed hypothesis regarding the potential behavior of the pumice as a substrate for the evolution of life. Furthermore, the detailed analysis from La Restinga eruption is coherent with the mineral phases and processes discussed from previous literature. The white internal part fulfills the conditions to work as an organic reservoir, confirmed by the detection of organic matter and selected minerals that could be used as energy sources for bacterial communities. The external layers of the samples work as a shielding layer to protect the organics from decay in extreme conditions. Finally, here we have demonstrated that the characteristics and advantages of Raman spectroscopy could help to assess and understand the possible biogenicity and alteration processes of any geological sample to be found on Mars.

Identifiants

pubmed: 31101155
pii: S2214-5524(18)30099-3
doi: 10.1016/j.lssr.2019.04.003
pii:
doi:

Substances chimiques

Minerals 0

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

49-64

Informations de copyright

Copyright © 2019 The Committee on Space Research (COSPAR). All rights reserved.

Auteurs

E Lalla (E)

Centre for Research in Earth and Space Science, York University, Petrie Science Building, 4700 Keele St, Toronto, M3J 1P3, ON, Canada; Austrian Space Forum, Sillufer 3a, Innsbruck, 6020, Austria. Electronic address: elalla@yorku.ca.

A Sanz-Arranz (A)

Departamento de Física de la Materia Condensada, Cristalografía y Mineralogía. Universidad de Valladolid, P de Belén 7, 47011, Valladolid, Spain.

G Lopez-Reyes (G)

Departamento de Física de la Materia Condensada, Cristalografía y Mineralogía. Universidad de Valladolid, P de Belén 7, 47011, Valladolid, Spain.

K Cote (K)

Centre for Research in Earth and Space Science, York University, Petrie Science Building, 4700 Keele St, Toronto, M3J 1P3, ON, Canada.

M Daly (M)

Centre for Research in Earth and Space Science, York University, Petrie Science Building, 4700 Keele St, Toronto, M3J 1P3, ON, Canada.

M Konstantinidis (M)

Centre for Research in Earth and Space Science, York University, Petrie Science Building, 4700 Keele St, Toronto, M3J 1P3, ON, Canada.

J A Rodriguez-Losada (JA)

Departamento de Biología Animal, Edafología y Geología, Universidad de La Laguna, Tenerife, C/ Astrofisco Sanchez s/n, 38211, La Laguna, Santa Cruz de Tenerife, Spain.

G Groemer (G)

Austrian Space Forum, Sillufer 3a, Innsbruck, 6020, Austria.

J Medina (J)

Departamento de Física de la Materia Condensada, Cristalografía y Mineralogía. Universidad de Valladolid, P de Belén 7, 47011, Valladolid, Spain.

J Martínez-Frías (J)

Dinámica Terrestre y Observación de la Tierra, Instituto de Geociencias, C/Severo Ochoa 7, Ed Entrepabellones 7 y 8, Ciudad Universitaria, 28040 Madrid, Spain.

F Rull-Pérez (F)

Austrian Space Forum, Sillufer 3a, Innsbruck, 6020, Austria.

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Classifications MeSH