Show simple item record

dc.contributor.authorFernandez-Remolar, David C.
dc.contributor.authorMorris, Richard V.
dc.contributor.authorGruener, John E.
dc.contributor.authorAmils, Ricardo
dc.contributor.authorKnoll, Andrew
dc.date.accessioned2009-07-28T13:19:35Z
dc.date.issued2005
dc.identifier.citationFernandez-Remolar, David C., Richard V. Morris, John E. Gruener, Ricardo Amils, and Andrew H. Knoll. 2005. The Rio Tinto basin, Spain: Mineralogy, sedimentary geobiology, and implications for interpretation of outcrop rocks at Meridiani Planum, Mars. Earth and Planetary Science Letters 240, no. 1: 149-167.en
dc.identifier.issn0012-821Xen
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:3200261
dc.description.abstractExploration by the NASA rover <i>Opportunity</i> has revealed sulfate- and hematite-rich sedimentary rocks exposed in craters and other surface features of Meridiani Planum, Mars. Modem, Holocene, and Plio-Pleistocene deposits of the Rio Tinto, southwestern Spain, provide at least a partial environmental analog to Meridiani Planum rocks, facilitating our understanding of Meridiani mineral precipitation and diagenesis, while informing considerations of martian astrobiology. Oxidation, thought to be biologically mediated, of pyritic ore bodies by groundwaters in the source area of the Rio Tinto generates headwaters enriched in sulfuric acid and ferric iron. Seasonal evaporation of river water drives precipitation of hydronium jarosite and schwertmannite, while (Mg,Al,Fe3+)-copiapite, coquimbite, gypsum, and other sulfate minerals precipitate nearby as efflorescences where locally variable source waters are brought to the surface by capillary action. During the wet season, hydrolysis of sulfate salts results in the precipitation of nanophase goethite. Holocene and Plio-Pleistocene terraces show increasing goethite crystallinity and then replacement of goethite with hematite through time. Hematite in Meridiani spherules also formed during diagenesis, although whether these replaced precursor goethite or precipitated directly from groundwaters is not known. The retention of jarosite and other soluble sulfate salts suggests that water limited the diagenesis of Meridiam rocks. Diverse prokaryotic and eukaryotic microorganisms inhabit acidic and seasonally dry Rio Tinto environments. Organic matter does not persist in Rio Tinto sediments, but biosignatures imparted to sedimentary rocks as macroscopic textures of coated microbial streamers, surface blisters formed by biogenic gas, and microfossils preserved as casts and molds in iron oxides help to shape strategies for astrobiological investigation of Meridiani outcrops.en
dc.description.sponsorshipOrganismic and Evolutionary Biologyen
dc.language.isoen_USen
dc.publisherElsevieren
dc.relation.isversionofhttp://dx.doi.org/10.1016/j.epsl.2005.09.043en
dash.licenseMETA_ONLY
dc.subjectgeobiologyen
dc.subjecthematiteen
dc.subjectchemical weatheringen
dc.subjectRio Tinto basinen
dc.subjectMeridiani Planumen
dc.subjectMarsen
dc.titleThe Rio Tinto Basin, Spain: Mineralogy, Sedimentary Geobiology, and Implications for Interpretation of Outcrop Rocks at Meridiani Planum, Marsen
dc.relation.journalEarth and Planetary Science Lettersen
dash.depositing.authorKnoll, Andrew
dash.embargo.until10000-01-01
dc.identifier.doi10.1016/j.epsl.2005.09.043*
dash.contributor.affiliatedKnoll, Andrew


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record