Please use this identifier to cite or link to this item: http://hdl.handle.net/1893/17151
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dc.contributor.authorKlingelhoefer, Goestaren_UK
dc.contributor.authorDeGrave, Eddyen_UK
dc.contributor.authorMorris, Richard Vanen_UK
dc.contributor.authorVan Alboom, A Toonen_UK
dc.contributor.authorde Resende, Valdirene Gen_UK
dc.contributor.authorde Souza Jr, Paulo Aen_UK
dc.contributor.authorRodionov, Daniel Sen_UK
dc.contributor.authorSchröder, Christianen_UK
dc.contributor.authorMing, Douglas Wayneen_UK
dc.contributor.authorYen, Albert Sen_UK
dc.date.accessioned2016-09-28T22:30:34Z-
dc.date.available2016-09-28T22:30:34Zen_UK
dc.date.issued2005-11en_UK
dc.identifier.urihttp://hdl.handle.net/1893/17151-
dc.description.abstractIn January 2004 the USA space agency NASA landed two rovers on the surface of Mars, both carrying the Mainz Mössbauer spectrometer MIMOS II. The instrument on the Mars-Exploration-Rover (MER) Spirit analyzed soils and rocks on the plains and in the Columbia Hills of Gusev crater landing site on Mars. The surface material in the plains have an olivine basaltic signature suggesting physical rather than chemical weathering processes present in the plains. The Mössbauer signature for the Columbia Hills surface material is very different ranging from nearly unaltered material to highly altered material. Some of the rocks, in particular a rock named Clovis, contain a significant amount of the Fe oxyhydroxide goethite, α-FeOOH, which is mineralogical evidence for aqueous processes because it is formed only under aqueous conditions. In this paper we describe the analysis of these data using hyperfine field distributions (HFD) and discuss the results in comparison to terrestrial analogues.en_UK
dc.language.isoenen_UK
dc.publisherSpringeren_UK
dc.relationKlingelhoefer G, DeGrave E, Morris RV, Van Alboom AT, de Resende VG, de Souza Jr PA, Rodionov DS, Schröder C, Ming DW & Yen AS (2005) Mössbauer spectroscopy on Mars: goethite in the Columbia Hills at Gusev crater. Hyperfine Interactions, 166 (1-4), pp. 549-554. https://doi.org/10.1007/s10751-006-9329-yen_UK
dc.rightsThe publisher does not allow this work to be made publicly available in this Repository. Please use the Request a Copy feature at the foot of the Repository record to request a copy directly from the author. You can only request a copy if you wish to use this work for your own research or private study.en_UK
dc.rights.urihttp://www.rioxx.net/licenses/under-embargo-all-rights-reserveden_UK
dc.subjectMIMOS IIen_UK
dc.subjectweatheringen_UK
dc.subjectMarsen_UK
dc.subjectgoethiteen_UK
dc.subjecthematiteen_UK
dc.subjectfield distributionen_UK
dc.subjectGusev crateren_UK
dc.subjectMars-Exploration-Roversen_UK
dc.subjectmineralogyen_UK
dc.titleMössbauer spectroscopy on Mars: goethite in the Columbia Hills at Gusev crateren_UK
dc.typeJournal Articleen_UK
dc.rights.embargodate2999-12-31en_UK
dc.rights.embargoreason[Klingelhoefer2006_moessbauer_spectroscopy_on_mars-goethite_in_the_columbia_hills_at_gusev_crater.pdf] The publisher does not allow this work to be made publicly available in this Repository therefore there is an embargo on the full text of the work.en_UK
dc.identifier.doi10.1007/s10751-006-9329-yen_UK
dc.citation.jtitleHyperfine Interactionsen_UK
dc.citation.issn1572-9540en_UK
dc.citation.issn0304-3843en_UK
dc.citation.volume166en_UK
dc.citation.issue1-4en_UK
dc.citation.spage549en_UK
dc.citation.epage554en_UK
dc.citation.publicationstatusPublisheden_UK
dc.citation.peerreviewedRefereeden_UK
dc.type.statusVoR - Version of Recorden_UK
dc.author.emailchristian.schroeder@stir.ac.uken_UK
dc.contributor.affiliationJohannes Gutenberg University of Mainzen_UK
dc.contributor.affiliationGhent Universityen_UK
dc.contributor.affiliationNational Aeronautics and Space Administration (NASA)en_UK
dc.contributor.affiliationGhent Universityen_UK
dc.contributor.affiliationUniversidade Federal de Ouro Preto, Brazilen_UK
dc.contributor.affiliationUniversity of Tasmaniaen_UK
dc.contributor.affiliationJohannes Gutenberg University of Mainzen_UK
dc.contributor.affiliationBiological and Environmental Sciencesen_UK
dc.contributor.affiliationNational Aeronautics and Space Administration (NASA)en_UK
dc.contributor.affiliationCalifornia Institute of Technologyen_UK
dc.identifier.isiWOS:000242969500034en_UK
dc.identifier.scopusid2-s2.0-33845750584en_UK
dc.identifier.wtid682774en_UK
dc.contributor.orcid0000-0002-7935-6039en_UK
dcterms.dateAccepted2005-11-30en_UK
dc.date.filedepositdate2013-10-28en_UK
rioxxterms.typeJournal Article/Reviewen_UK
rioxxterms.versionVoRen_UK
local.rioxx.authorKlingelhoefer, Goestar|en_UK
local.rioxx.authorDeGrave, Eddy|en_UK
local.rioxx.authorMorris, Richard Van|en_UK
local.rioxx.authorVan Alboom, A Toon|en_UK
local.rioxx.authorde Resende, Valdirene G|en_UK
local.rioxx.authorde Souza Jr, Paulo A|en_UK
local.rioxx.authorRodionov, Daniel S|en_UK
local.rioxx.authorSchröder, Christian|0000-0002-7935-6039en_UK
local.rioxx.authorMing, Douglas Wayne|en_UK
local.rioxx.authorYen, Albert S|en_UK
local.rioxx.projectInternal Project|University of Stirling|https://isni.org/isni/0000000122484331en_UK
local.rioxx.freetoreaddate2999-12-31en_UK
local.rioxx.licencehttp://www.rioxx.net/licenses/under-embargo-all-rights-reserved||en_UK
local.rioxx.filenameKlingelhoefer2006_moessbauer_spectroscopy_on_mars-goethite_in_the_columbia_hills_at_gusev_crater.pdfen_UK
local.rioxx.filecount1en_UK
local.rioxx.source0304-3843en_UK
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