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dc.contributor.authorAmils, Ricardoen_US
dc.contributor.authorGonzález-Toril, Elenaen_US
dc.contributor.authorFernández-Remolar, Daviden_US
dc.contributor.authorGómez-Gómez, Felipeen_US
dc.contributor.authorAguilera, Ángelesen_US
dc.contributor.authorRodríguez, Nuriaen_US
dc.contributor.authorMalki, Moustafáen_US
dc.contributor.authorGarcía-Moyano, Antonioen_US
dc.contributor.authorGonzález-Fairén, Albertoen_US
dc.contributor.authorFuente, Vicenta de laen_US
dc.contributor.authorSanz, José Luisen_US
dc.date.accessioned2009-06-03T05:53:30Z-
dc.date.available2009-06-03T05:53:30Z-
dc.date.issued2007-02en_US
dc.identifier.citationPlanetary and Space Science 55(3): 370-381 (2007)en_US
dc.identifier.issn0032-0633-
dc.identifier.urihttp://hdl.handle.net/10261/13417-
dc.description12 pages, 5 figures, 2 tables.-- ISI Article Identifier: 000244695500010.-- Available online Sep 28, 2006.-- Issue title: "Planet Mars II".en_US
dc.description.abstractThe geomicrobiological characterization of the Río Tinto (Iberian Pyritic Belt) has recently proven the importance of the iron cycle, not only in the generation of the extreme conditions of the habitat (low pH, high concentration of heavy metals), but also in the maintenance of a high level of microbial diversity. The presence of vast deposits of sulfates and iron oxides on Mars, the main products of the bioleaching of iron containing sulfides found in Río Tinto, and the physico-chemical properties of iron as a source of energy, protection from radiation and oxidative stress as well as pH control, make Río Tinto an interesting Mars terrestrial analog.-
dc.description.sponsorshipThis work was supported by Grant BOS2002-02148 from the CICYT and Institutional Grants to the Centro de Astrobiología.-
dc.format.extent2373 bytes-
dc.format.mimetypetext/plain-
dc.publisherElsevier-
dc.rightsclosedAccessen_US
dc.subjectExtremophiles-
dc.subjectAcidophiles-
dc.subjectIberian Pyritic Belt-
dc.subjectChemolithoautotrophy-
dc.subjectIron cycle-
dc.subjectSulfates-
dc.subjectIron oxides-
dc.subjectHematite-
dc.subjectMars-
dc.subjectMeridiani planum-
dc.titleExtreme environments as Mars terrestrial analogs: The Rio Tinto caseen_US
dc.typeartículoen_US
dc.identifier.doi10.1016/j.pss.2006.02.006-
dc.description.peerreviewedPeer revieweden_US
dc.relation.publisherversionhttp://dx.doi.org/10.1016/j.pss.2006.02.006-
dc.contributor.funderComisión Interministerial de Ciencia y Tecnología, CICYT (España)-
dc.identifier.funderhttp://dx.doi.org/10.13039/501100007273es_ES
dc.type.coarhttp://purl.org/coar/resource_type/c_6501es_ES
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.openairetypeartículo-
item.cerifentitytypePublications-
item.grantfulltextnone-
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